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k 

COURSE 

OF 

MATHEMATICS; 

FOR  THB 

USE  OF  ACADEMIES 

AS  WILL  AS 

PRIVATE  TUITION. 


IN  TWO  VOLUMES* 


CHARLj^g;  IWTTON,.  LUR  JFJtS. 

fcATS  PROFESSOR  OF  ajA&XMATICS  IN  THE WfAL VlMTART  ACADEMY . 

THE  FIFTH  AMENlfeKlV  FROM  THE  NINTH 

WITH  MANY  COR.RjplC£i0r;S4  AND  IMPROVEMENTS. 

RV  OUNTHUS  GREGORY,  LL.D. 

-CorretponSing  Associate  of  the  Academy  of  Dijon.  Honorary  Member  of  the  Literary 
and  Philosophical  Society  of  New- York,  of  the  New- York  Historical  Society, of  the 
Literary  and  Philosophical,  and  the  Antiquarian  Societies  of  Newcastle  opoa  Tyoa, 
of  the  Cambridge  Philosophical  Society,  of  tho  Institution  of  Civil  Engineers,  ate. fce. 
Secretary  to  the  Astronomical  Society  of  London,  and  Professor  of  TTithamatioa  in 
wfaa  Royal  Military  Academy. 


WITH  THE  ADDITIONS 
or 

ROBERT  ADRAIN,  LL.D.  F  A. P  S.  F.A.A.S,  lie. 

And  Professor  of  Mathematics  and  Natural  Philosophy. 

THE  WHOLE 

CORRECTED  AND  IMPROVED. 


VOL.  I. 


NEW-YORK:  . 

W.  JL  DZAJf,  PR  UTTER.' 
r.  AMD  I.  SW0RD8;  T.  A.  RONALDS ;  COLLINS  AND  CO. ;  COLLINS  iNb  RAN* 
NAT  J  H.  AND  C.  AND  H.  CARVILL;  WHITE,  OALLARERj  AND  WHITE  f 
a  A.  ROORBACHf  AND  M'CLRATB  AND  BANGS. 

1831. 


SiutiUr*  JHrtrict  o/  JrVw-Ter*,  to  wit  I 
BE  IT  REMEMBERED,  That  oatb«  224  day  of  February,  Ana©  Domini  ISSt,  W. 
E.  DEAN,  of  the  Mid  district,  bath  jirwiti4  U  «kU  edbce  the  title  of  a  book,  the  title 
ef  which  U  in  the  word*  following,  to  wit: 

•  A  Count  of  Mathematics ;  for  the  nse  of  Academies  as  well  eg  private  toitioo.  la 
Two  Volomes.  By  Charles  Hottoo,  LL.D.  F.R.S„  Uto  Profeieor  of  Mathematics  in 
the  Royal  Military  Academy.  The  Fifth  American  from  the  Ninth  London  Edition, 
with  many  corrections  and  improvements.  By  Olinthus  Gregory,  LL.D.  Correspond* 
Ing  Associate  of  the  Academy  of  Dijon,  Honorary  Member  of  the  Literary  and  Philo- 
sophical Society  of  New- Fork,  of  the  New- York  Historical  Society,  of  the  Literary 
and  Philosophical,  and  the  Antiquarian  Societies  of  Newcastle  upon  Tyno,  of  the 
Cambridge  Philosophical  Society,  of  the  Institution  of  Clril  Engineers,  dec  dec  Secre- 
tary to  the  Astronomical  Society  of  London,  and  Professor  of  Mathematics  in  the  Ro- 
yal Military  Academy.  With  the  Additions  of  Robert  Adrain,  LL.D.  F.A.P.8.  F.A. 
AA,  dec  and  Professor  of  Mathematics  and  Natural  Philosophy.  The  whole  correct* 
od  and  improved." 

Om  right  whereof  ho  claim  as  proprietor.  In  conformity  with  an  Aat  of  Congress,  e*> 
ttttt  «  A*  Act  to  sjmb4  the  atreral  Acts  respecting  eopy-rights." 

FRED.  J.  BETTS, 
Cfcr*  «/  we  fiaHws  Dirtrtrt  e/AWFerfc  . 


PREFACE. 


The  present  American  edition  is  in  part  a  re- 
print  of  the  Ninth  English  edition  by  Dr.  Oun- 
thus  Gregory,  with 'mQst.pf,  the  improvements 
introduced  into  former  Al^ejricaa  editions  by  Dr. 
Adrain,  together  with  mich  modifications  of  the 
English  editions  as  appeared  calculated  to  in- 
crease the  general  usefulness  of  the  work.  At 
the  same  time  two  or  three  Chapters,  devoted 
to  subjects  of  no  great  value  at  present  to  the 
American  student,  have  been  omitted,  to  leave 
room  for  matter  of  more  interest  and  importance. 


CONTENTS 


OF 
VOL.  I. 


Gin iRAt.  Preliminary  Principles  I  ] 

ARITHMETIC, 
ffotaiion  and  Numeration  *j 
Roman  Notation  -  .  7 
Addition  g 
Subtraction  -  .  -  ][ 
Multiplication  -  13 
Division  -         .         -  IS 

Reduction  - 

Compound  Addition  •  32 

Commissioned  Officers'  Regimen 

talPay  . 
Compound  Subtraction  * 

 Multiplication 

Division  - 
1  Rule,  or  Rule  of  Thr**  ■ 


r_  jnd  Proportion 
Vulgar  Fractions 
Reduction  of  Vulgar  Fractions 
Addition  of  Vulgar  Fractions 
Subtra  ct  ion  of  VwTgar  Fractions 
Multiplication  t*f  Vol  fat  Frtfst&ns'.  ib. 
Di v i s ion  of  Vu *r*c«loas  ?  (ft 


Roto  of  Three  ia  Vulgar  Fractions  65 
imnl  Fractions  *  .«HSe 


Involution  by  Logarithms 
Evolution  by  Logvrtthntt 

ALGEBRA,. 

Definitions  and  ] 
Addition 
Subtraction 
Multiplication 
Division  - 
Fractious 
Involution 
Evolution 
Surds  * 
Arithmaticiil 


Pa.  159 
160 


Decimal .  . 

Su1*ra™m  ofDectmftlf.  *- :  "  A  i .  ^ 
Multiplication  of  Decimal*-  -  .  ,.ib* 
Division  of  Decimals*     m -l   *'  ^.55 

Duodecimals  -         -  77 

Involution  -         -         -  70 

Evolution  -  -  60 
To  extract  the  Square  Root  -  ft  I 
To  extract  »he  Cube  Root  -  85 
VTo  extract  any  Root  whatever  •  8ti 
Table  nf  Powers  and  Roots  -  9] 
Ratios,  Proportions,  end  Progres- 
sion* -  -  .  -  Hi 
Ariihmetical  Proportion  -  112 
Geometrical  Proportion  -  -  116 
Harmonical  Proportion  -  181 
Fellowship,  or  Partnership  -  132 
Single  Fellowship  *  -  ib. 
Double  Fellowship  *  -  125 
Simple  Interest  -  -  127 
Compound  Interest  -  -  13Q 
13* 

-  119 
136 

-  las 

141 


-  16* 
166 

-  170 
172 

-  175 
179 

-  189 
192 

-  196 
id  Pro- 

-  203 
207 

Geometrical  Proportion  and  Pro- 
gression      -         -         -  212 
Infinite  Series,  and  their  Summa- 
tion *  214 
Simple.  Equations     *          •  231 
Qrvulca(jc  Equal iona       -         .  249 
Xu&cTiftitl  Higher  Equations-  256 
.  Sixfiih  inlerest    -         -         -  266 
,Coni  pound  Interest  *         -  267 

-  270 


gression 
Piles  of  Shot  and  Shells 


frfinhloas 


- 


Alligation  Alternate 
Single  Position 
Double  Position  * 
Practical  Questions 

LOGARITHM*. 
Definition  and  Properties  of  Loga- 
rithms •         -         -  .146 
To  compute  Logarithms  149 
Description  and  Use  of  Logarithms  15 
Multiplication  by  Logarithms      -  157 
Division  by  Logarithms  15* 


GEOtt£TRT* 

-  275 
281 

-  ib. 
Defi- 

.318 

Theorems  <-  320 
Of  Plane*  and  Sollds^Deftriitions  336 
Theorems  -         ,         .  340 

Problems  *        .  355 

Application  of  Algebra  to  Geome- 

iry  -  ,  .  .371 
Problems     »  -  372 

Plane  Trigonometry  *  -  378 
Trigonometrical  Formula  -  393 
Heights  and  Distances  -  -  396 
Mensuration  otPianes  or  Areas  405 
Mensuration  of  Solids  -  *  420 
Land  Surveying  -  •  430 
ArtifuerV  Worls  -         -  459 

Timber  Measuring  -  .  468 
Conic  SecUoM  -  -  -472 
Of  the  Ellipse  -         -  476 

Of  the  Hyperbole  .  -494 

Of  lhe  Parabola  -  -  518- 
Problems,  &c,  in  Conic  Sections  -  534 
Equations  of  the  Curve  -  536 
Element*  of  Isoperiim try  *  -  539 
Surfaces  -  -  -  541 
Solids  •  -  -  .551 
PracticaT  Qiie^cmiinMantiiratlOB  562 
Logarithms  of  Numbers  *  •  571 
Table  of  Lorarithznic  Sines,  and 

590 


A 


COURSE 


OF 


MATHEMATICS,  &c. 


GENERAL  PRINCIPLES. 

1.  Quantity,  or  Magnitude,  is  any  thing  that  will 
admit  of  increase  or  decrease  ;  or  that  is  capable  of  any  sort 
of  calculation  or  mensuration  ;  such  as  numbers,  lines,  space, 
time,  motion,  weight,  &c. 

-  2.  Mathematics  is  the  science  which  treats  of  all  kinds 
of  quantity  whatever,  that  can  be  numbered  or  measured.— 
That  part  which  treats  of  numbering  is  called  Arithmetic ; 
and  that  which  concerns  measuring,  or  figured  extension, 
is  called  Geometry. — Not  only  these  two,  but  Algebra  and 
Fluxions,  which  are  conversant  about  multitude,  magnitude, 
form,  and  motion,  being  the  foundation  of  all  the  other 
parts,  are  called  Pure  or  Abstract  Mathematics ;  because 
they  investigate  and  demonstrate  the  properties  of  abstract 
numbers  and  magnitudes  of  all  sorts.  And  when  these  two 
parts  are  applied  to  particular  or  practical  subjects,  they 
constitute  the  branches  or  parts  called  Mixed  Mathematics* 
— Mathematics  is  also  distinguished  into  Speculative  and 
Practical:  viz.  Speculative,  when  it  is  concerned  in  dis- 
covering properties  and  relations ;  and  Practical,  when 
applied  to  practice  and  real  use  concerning  physical  objects. 

The  peculiar  topics  of  investigation  in  the  four  prmci^ %1 
departments  of  pure  mathematics  may  be  indicated  Vw  fo\u 

Vol.  L  2 


2 


OEIfEKAL  PRINCIPLES. 


words :  viz.  arithmetic  by  number,  geometry  by  form,  algtbrm 
by  generality,  fluxions  by  motion. 

3.  In  mathematics  are  several  general  terms  or  principles  ? 
such  as,  Definitions,  Axioms,  Propositions,  Theorems,  Pro- 
blems, Lemmas,  Corollaries,  Scholia,  &c. 

4.  A  Definition  is  the  explication  of  any  term  or  word  in  a 
science  ;  showing  the  'sense  and  meaning  in  which  the  term 
is  employed. — Every  Definition  ought  to  be  clear,  and  ex* 
pressed  in  words  that  are  common  and  perfectly  well  under* 
stood. 

5.  A  Proposition  is  something  proposed  to  be  demon- 
strated, or  something  required  to  be  done ;  and  is  accordingly 
either  a  Theorem  or  a  Problem. 

6.  A  Theorem  is  a  demonstrative  Proposition ;  in  which 
some  property  is  asserted,  and  the  truth  of  it  required  to  be 
proved.  Thus,  wpea  R  is  said  that,  The  sum  of  the  three 
angles  of  a  plane  triangle  is  equal  to  two  right  angles,  that  is 
a  Theorem,  the  truth  of  which  is  demonstrated  by  Geometry* 
— A  set  or  collection  of  such  Theorems  constitutes  a  Theory, 

7.  A  Problem  is  a  proposition  or  a  question  requiring 
something  to  be  done  ;  either  to  investigate  some  truth  or 
property,  or  to  perform  some  operation.  As,  to  find  out  the 
quantity  or  sum  of  all  the  three  angles  of  any  triangle,  or  to 
draw  one  line  perpendicular  to  another. — A  Limited  Pro* 
blem  is  that  which  has  but  one  answer  or  solution.  An  Un- 
limited Problem  is  that  which  has  innumerable  answers. 
And  a  Determinate  Problem  is  that  which  has  a  certain  nun*, 
her  of  answer*. 

8.  Solution  of  a  Problem,  is  the  resolution  or  answer 
given  to  it.  A  Numerical  or  Numeral  Solution,  is  the  an. 
89  ex  given  in  numbers.  A  Geometrical  Solution,  is  the  an- 
swer even  by  tl*e  principles  of  Geometry.  And  a  Mechani- 
cal Solution,  is  one  whicji  is  gained  by  trials. 

9.  A  Lemma  is  a  preparatory  proposition,  lajd  down  in 
ojrder  U>  shorten  the  demonstration  of  the  main  proposition 
which  follows  it. 

ip.  A  Corollary,  or  Conseetary,  is  a  consequence  draws 
imq^aWy  from  some  proposition  or  other  premises. 

11.  A  Scholium  is  a  remark  or  observation  nade  upon 
some  foregping  proposition  or  premises. 

12.  MMim,Qr  Masim,  is  a  self-evident  prejwwuon  ; 
requiring  no  formal  deopnsteation  to  prove  its  truth  ;  but 
received  and  assented  to  as  soon  as  mentioned.  Such  as, 
Tb*  wlpole  of  any  thing  is.  greater  than  a  part  of  it ;  or,  The 
wjhoJ*  i*  equal  to  a)|  its  parts  taken  together ;  or,  Two  quan. 
tides  that  are  each  of  them  equal  to  a  third  quantity,  are 
equal  to  eaqh  other, 


OSNK&AL  AINCIPLE8. 


3 


13.  A  Postulate,  or  Petition,  is something  required  to  be 
done,  which  is  so  easy  and  evident  that  no  person  will  hesi- 
tate to  allow  it. 

14.  An  Hypothesis  is  *  stipulation  assumed  to  be  true, 
in  order  to  argue  from,  or  to  found  upon  it  the  reasoning  and 
demonstration  of  some  proposition. 

19k  Demonstration  is  the*  collecting  the  several  torments 
alri  proofs,  4nd  ttryiilg  them  together  in  proper  order  to  shbifr 
the  trtitt  of  the  proposition  under  consideration, 

10»  A  Ihtreet,  TbsUloe,  of  Affirmative  D&ntviishiitiun',  is 
thai  *hr6h  cotidrides  with  the  direct  and  certain  pttibf  df  th* 
prtjpoeitioh  in  hand. 

IT.  4ji  Indira*,  or  irt&trtttxr  Beinortstrdtioh,  is  that  whicti 
shows  a  proposition  to  be  true,  by  proving  that  some  ab- 
aofdlry  would  hecessanly  fblloW  if  the  proposition  advanced 
were  false*  This  is  also  sometitties  called  Redbctio  ad  Afr- 
HftNAdSi ;  because  it  shows  the  absurdity  arid  falsehood  of 
alt  suppositions  cbritrarjr  to  that  contained  in  the  proposi- 
tion. 

18.  Method  is  the  art  of  disposing  a  train  of  arguments  in 
a  proper  order,  to  investigate  either  the  truth  or  falsity  of 
a  proposition,  df  to  demonstrate  it  to  others  when  it  has  been 
(bund  oat.— 'this  is  either  Analytical  or  Synthetical. 

19.  Analysis  or  the  Analytic  Method,  is  the  art  or  mode  of 
finding  out  the  truth  of  a  proposition,  by  first  supposing 
the  thing  to  be  done,  and  then  reasoning  back,  step  by  step, 
till  we  arrive  at  some  known  truth.  This  is  also  called  the 
Method  of  Invention,  or  Resolution ;  and  is  that  which  is  com- 
monly used  in  Algebra. 

20.  Synthesis,  or  the  Synthetic  Method,  is  the  searching 
out  truth,  by  first  laying  down  some  simple  and  easy  prin- 
ciples, and  then  pursuing  the  consequences  flowing  from 
them  till  we  arrive  at  the  conclusion. — This  is  also  called 
the  Method  of  Composition ;  and  is  the  reverse  of  the  Ana* 
lytic  method,  as  this  proceeds  from  known  principles  to  an 
unknown  conclusion  ;  while  the  other  goes  in  a  retrograde 
order,  from  the  thing  sought,  considered  as  if  it  were  true, 
to  some  known  principle  or  fact.  Therefore,  when  any 
troth  has  been  found  out  by  the  Analytic  method,  it  may  be 
demonstrated  by  a  process  in  the  contrary  order,  by  Syn- 
thesis :  and  in  the  solution  of  geometrical  propositions,  it  is 
Vety  instructive  to  carry  through  both  the  analysis  and  the 
synthesis* 


4 


ARITHMETIC. 

Arithmetic  is  the  art  or  science  of  numbering ;  being 
that  branch  of  Mathematics  which  treats  of  the  nature  and 
properties  of  numbers. — When  it  treats  of  whole  numbers, 
it  is  called  Vulgar,  or  Common  Arithmetic  ;  but  when  of 
broken  numbers,  or  parts  of  numbers,  it  is  called  Fractions. 

Unity,  or  an  Unit,  is  that  by  which  every  thing  is  called 
one  ;  being  the  beginning  of  number  ;  as,  one  man,  one 
ball,  one  gun. 

Number  is  either  simply  one,  or  a  compound  of  several 
units ;  as,  one  man,  three  men,  ten  men. 

An  Integer,  or  Whole  Number,  is  some  certain  precise 
quantity  of  units  ;  as,  one,  three,  ten. — These  are  so  called 
as  distinguished  from  Fractions,  which  are  broken  num- 
bers, or  parts  of  numbers  ;  as,  one-half,  two-thirds,  or  three- 
fourths. 

A  Prime  Number  is  one  which  has  no  other  divisor  than 
unity ;  as  2,  3,  5, 7,  17,  19,  &c.  A  Composite  Number  is 
one  which  is  the  product  of  two  or  more  numbers  ;  as,  4*  6, 
8,  9,  28,  &c. 


NOTATION  AND  NUMERATION. 

These  rules  teach  how  to  denote  or  express  any  pro* 
posed  number,  either  by  words  or  characters :  or  to  read 
and  write  down  any  sum  or  number. 

The  Numbers  in  Arithmetic  are  expressed  by  the  follow- 
ing ten  digits,  or  Arabic  numeral  figures,  which  were  intro- 
duced into  Europe  by  the  Moors,  about  eight  or  nine 
hundred  years  since ;  viz.  1  one,  2  two,  3  three,  4  four, 
5  five,  6  six,  7  seven,  8  eight,  9  nine,  0  cipher,  or  nothing. 
These  characters  or  figures  were  formerly  all  called  by  the 
general  name  of  Ciphers ;  whence  it  came  to  pass  that  the 
art  of  Arithmetic  was  then  often  called  Ciphering.  The 
first  nine  are  called  Significant  Figures,  as  distinguished 
from  the  cipher,  which  is  of  itself  quite  insignificant. 

Besides  this  value  of  those  figures,  they  have  also  another, 
which  depends  on  the  place  they  stand  in  when  joined  to- 
gether ;  as  in  the  following  table  :  • 


NOTATION  AND  KUXBBAITON. 


s 


-3 


6c.    '9     8     7     6     5     4     3     2  1 
98  765432 
9     8     7     6     5     4  3 
9     8     7     6     5  4 
9     8     7     6  5 
9     8     7  6 
9     8  7 
9  8 
9 


Here,  any  figure  in  the  first  place,  reckoning  from  right 
to  left,  denotes  only  its  own  simple  value  ;  but  that  in  the 
second  place,  denotes  ten  times  its  simple  value  ;  and  that  in 
the  third  place,  a  hundred  times  its  simple  value  ;  and  so 
on  :  the  value  of  any  figure,  in  each  successive  place,  be- 
ing always  ten  times  its  former  value. 

Thus,  in  the  number  1796,  the  6  in  the  first  place  denotes 
only  six  units,  or  simply  six  ;  9  in  the  second  place  signifies 
nine  tens,  or  ninety  ;  7  in  the  third  place,  seven  hundred  ; 
and  the  1  in  the  fourth  place,  one  thousand :  so  that  the 
whole  number  is  read  thus,  one  thousand  seven  hundred  and 
ninety- six. 

As  to  the  cipher,  0,  though  it  signify  nothing  of  itself,  yet 
being  joined  on  the  right-hand  side  to  other  figures,  it  in- 
creases their  value  in  the  same  ten-fold  proportion  :  thus,  5 
signifies  only  five  ;  but  50  denotes  5  tens,  or  fifty  ;  and  500 
is  five  hundred  ;  and  so  on. 

For  the  more  easily  reading  of  large  numbers,  they  are 
divided  into  periods  and  half-periods,  each  half-period  con. 
sisting  of  three  figures ;  the  name  of  the  first  period  being 
units ;  of  the  secoud,  millions ;  of  the  third,  millions  of 
millions,  or  bi-millions,  contracted  to  billions  ;  of  the  fourth, 
millions  of  millions  of  millions,  or  tri-millions,  contracted  to 
trillions,  and  so  on.  Also  the  first  part  of  any  period  is  so 
many  units  of  it,  and  the  latter  part  so  many  thousands. 


6  AUOTonnno. 

The  following  Table  contains  a  summary  of  the  whole 
doctrine. 


Periods.  Quadril. ;  Trillions ;  Billions ;  Millions ;  Units. 


Half-per. 


th.  un.     th.  un.    th.  un.    th.  un.  th.  un. 


Figures.  (123,456 ;  789,098 ;  765,432  ;  101,234 ;  567,890. 


Numeration  is  the  reading  of  any  number  in  words  that 
is  proposed  or  set  down  in  figures  ;  which  will  be  easily  done 
by  help  of  the  following  rule,  deduced  from  the  foregoing 
tables  and  observations — viz. 

Divide  the  figures  in  the  proposed  number,  as  in  the  sum- 
mary, above,  into  periods  and  half-periods  ;  then  begin  at  the 
left-hand  side,  and  read  the  figures  with  the  names  set  to 
them  in  the  two  foregoing  tables. 


EXAMPLXfi. 


Express  in  words  the  following  numbers ;  viz. 


34 
96 
380 
704 
6134 
9028 


15080 
72003 
109026 
483500 
2500639 
7523000 


13405670 
47050023 
309025600 
4723507689 
274856390000 
6578600307024 


Notation  is  the  setting  down  in  figures  any  number 
proposed  in  words ;  which  is  done  by  setting  down  the  figures 
instead  of  the  words  or  names  belonging  to  them  in  the  sum- 
mary above  ;  supplying  the  vacant  places  with  ciphers 
where  any  words  do  not  occur. 


EXAMPLES. 


Set  down  in  figures  the  following  numbers : 
Fifty-seven. 

Two  hundred  eighty-six. 
Nine  thousand  two  hundred  and  ten. 
Twenty-seven  thousand  five  hundred  and  ninety-four. 
Six  hundred  and  forty  thousand,  four  hundred  and  eighty-one. 
Three  millions,  two  hundred  sixty  thousand,  one  hundred 
and  six. 


NOTATION  AND  NUMXBATION. 


Four  hundred  and  eight  millions,  two  hundred  and  fifty-five 
thousand,  one  hundred  and  ninety-two. 

Twenty-seven  thousand  and  eight  millions,  ninety-six  thou- 
sand two  hundred  and  four. 

Two  hundred  thousand  and  five  hundred  and  fifty  millions, 
one  hundred  and  ten  thousand,  and  sixteen. 

Twenty-one  billions,  eight  hundred  and  ten  millions,  sixty, 
four  thousand,  one  hundred  and  fifty. 

OF  THE  BOKAN  NOTATION. 

The  Romans,  like  several  other  nations,  expressed  their 
numbers  by  certain  letters  of  the  alphabet.  The  Romans 
used  only  seven  numeral  letters,  being  the  seven  following 
capitals  :  viz.  i  for  one ;  v  for  five ;  x  for  ten ;  l  for  fifty ; 
c  for  an  hundred ;  d  for  five  hundred ;  m  for  a  thousand ;  The 
other  numbers  they  expressed  by  various  repetitions  and 
combinations  of  these,  after  the  following  manner : 


1  = 

i 

2  = 

ii 

As  often  as  any  character  is  re- 

3 = 

iii 

peated,  so  many  times  is  its 

value  repeated. 

4  = 

mi  or  iv 

A  less  character  before  a  greater 

5  = 

V 

diminishes  its  value. 

6  = 

VI 

A  less  character  after  a  greater 

7  = 

VII 

increases  its  value. 

8  = 

VIII 

9  = 

IX 

10  = 

X 

60  = 

L 

100  = 

C 

500  = 

d  or  io 

For  every  o  annexed,  this  be- 

comes 10  times  as  many. 

1000  = 

m  or  cu 

For  every  c  and  o,  placed  one 

2000  = 

MM 

at  each  end,  it  becomes  10 

times  as  much. 

6000  = 

v  or  loo 

A  bar  over  any  number  in- 

6000  = 

VI 

creases  it  1000  fold. 

10000  = 

x  or  ccioo 

50000  = 

|  l  or  1003 

00000  = 

f- 

100000  = 

■  <  c  or  ccciooo 

1000000  =  nor  CCCCI0O33 
2000000  =  ra 


9 


ARITHMETIC. 


EXPLANATION  OF  CERTAIN  CHARACTERS* 

There  are  various  characters  or  marks  used  in  Arithmetic, 
and  Algebra,  to  denote  several  of  the  operations  and  propo- 
sitions ;  the  chief  of  which  are  as  follow : 

+  signifies  plus,  or  addition. 
—    -     .   minus,  or  subtraction. 
X  or     -  multiplication. 
H-    -  division, 
t  ::  :    -  proportion. 
«=*    -    T  equality. 
«v/   -     -   square  root. 
%/    -     -   cube  root,  &c. 

*r    .    .   diff.  between  two  numbers  when  it  is  not  known 
which  is  the  greater. 

Thus, 

5  +  3,  denotes  that  3  is  to  be  added  to  5. 

6  —  2,  denotes  that  2  is  to  be  taken  from  6. 

7  X  3,  or  7  •  3,  denotes  that  7  is  to  be  multiplied  by  3. 

8  -r-  4,  denotes  that  8  is  to  be  divided  by  4. 

2  :  3  : :  4  :  6,  shows  that  2  is  to  3  as  4  is  to  6. 

6  +  4  =  10,  shows  that  the  sum  of  6  and  4  is  equal  to  10. 

or  3^,  denotes  the  square  root  of  the  number  3. 

$/5,  or  5^,  denotes  the  cube  root  of  the  number  5. 
7s,  denotes  that  the  number  7  is  to  be  squared. 
S3,  denotes  that  the  number  8  is  to  be  cubed, 
dec. 


OF  ADDITION. 

Addition  is  the  collecting  or  pitting  of  several  numbers 
together,  in  order  to  find  their  sum,  or  the  total  amount  of  the 
whole.   This  is  done  as  follows : 

Set  or  place  the  numbers  under  each  other,  so  that  each 
figure  may  stand  exactly  under  the  figures  of  the  same  value, 


ADDITION* 


9 


that  is,  units  under  units,  tens  under  tens,  hundreds  under 
hundreds,  dec.  and  draw  a  line  under  the  lowest  number,  to 
separate  the  given  numbers  from  their  sum,  when  it  is  found. 
— Then  add  up  the  figures  in  the  column  or  row  of  units, 
and  find  how  many  tens  are  contained  in  that  sum. — Set 
down  exactly  below,  what  remains  more  than  those  tens,  or 
if  nothing  remains,  a  cipher,  and  carry  as  many  ones  to  the 
next  row  as  there  are  tens. — Next  add  up  the  second  row, 
together  with  the  number  carried,  in  the  same  manner  as  the 
first.  And  thus  proceed  till  the  whole  is  finished,  setting 
down  the  total  amount  of  the  last  row. 


TO  PROVE  ADDITION. 


First  Method. — Begin  at  the  top,  and  add  together  all  the 
rows  of  numbers  downwards,  in  the  same  manner  as  they 
were  before  added  upwards  ;  then  if  the  two  sums  agree,  it 
may  be  presumed  the  work  is  right. — This  method  of  proof 
is  only  doing  the  same  work  twice  over,  a  little  varied. 

Second  Method. — Draw  a  line  below  the  uppermost  num. 
ber,  and  suppose  it  cut  off. — Then  add  all  the  rest  of  the 
numbers  together  in  the  usual  way,  and  set  their  sum  under 
the  number  to  be  proved. — Lastly,  add  this  last  found  num- 
ber and  the  uppermost  line  together  ;  then  if  their  sum  be 
the  same  as  that  found  by  the  first  addition,  it  may  be  pre- 
sumed the  work  is  right. — This  method  of  proof  is  founded 
on  the  plain  axiom,  that  "  The  whole  is  equal  to  all  its  parts 
taken  together." 

Third  Method. — Add  the  figures  in 
the  uppermost  line  together,  and  find       example  i. 
how  many  nines   are    contained  in 
their   sum. — Reject  those  nines,  and       3497    g  5 
set  down  the  remainder  towards  the       6512    .g  5 
right   hand  directly  even    with    the       8295   £  6 

figures  in  the  line,  as  in  the  annexed  — —  o  

example. — Do  the  same  with  each  of     18304    8  7 
the  proposed  lines  of  numbers,   set-  — —    g  — 
ting  all  these  excesses  of  nines  in  a  co-  W 
lumn  on  the  right-hand,  as  here  5,  5,  0.  Then,  if  the  excess 
of  9's  in  this  sum,  found  as  before,  be  equal  to  the  excess 
of  9's  in  the  total  sum  18304,  the  work  is  probably  right. — 
Thus,  the  sum  of  the  right-hand  column,  5,  5,  6,  is  16,  the 
excess  of  which  above  9  is  7.    Also  the  sum  of  the  figure*  V& 

Vol.  I.  3 


10 


ABZTHMSTXC. 


the  sum  total  18304,  is  16,  the  excess  of  which  above  9  m 
also  7>  the  same  as  die  former*. 


OTHER  EXAHPLES. 


2. 

3. 

4. 

12345 

12345 

12345 

87890 

67890 

876 

98765 

9876 

9087 

432)0 

543 

56 

12345 

21 

234 

67890 

9 

1012 

302445 

90684 

23610 

290100 

78339 

11265 

302445 

90684 

23610 

Ex.  5.  Add  3426 ;  9024  ;  5106  ;  8890  ;  1204,  together. 

Ans.  27650. 

6.  Add  509267;  235809;  72920  ;  8392;  420  ;  21;  and 
9,  together.  Ans.  82683a. 


*  This  method  of  proof  depends  on  a  property  of  the  number  9, 
which,  except  the  number  3;  belongs  to  no  other  digit  whatever ; 
namely*  that  44  any  number  divided  by  9,  will  leave  the  same  remain- 
der as  the  sum  of  its  figures  are  digits  divided  by  9:"  which  may  be 
demonstrated  in  this  manner. 

Demonstration.  Let  there  be  any  number  proposed,  as  4668.  This, 
separated  into  its  several  parts,  becomes,  4000  +  600+60  4-  8.  Bnt 
4000  =  4  X  1000  =  4  X  (999  +  1)  =  (4  X  999)  +  4.  In  like  man- 
ner 600  =  (6  X  99)  +6 ;  and  50  =  (5  X  9)  4-5.  Therefore  the  gi- 
ven number  4658  =  (4  X  999)  +  4  +  (6  X  99) +6 +(5  X9)  +  6  + 
8  =  (4  X  999)  +  (6  X  99)  +  (5  X  9)  +  4  +  6  +  5  +  8;  and 
4658  + 9  =  (4  X  999+6  X  99  +  5  X  9 +  4+ 6 +  5 +8) +  9.  But 
(4  X  999)  +  (6  X  99;  +  (5  X  9)  is  evidently  divisible  by  9,  without 
a  remainder ;  therefore  if  the  given  number  4658  be  divided  by  9, 
it  will  leave  the  same  remainder  as4+6+6+6  divided  by  9.  And 
the  same,  it  is  evident,  will  hold  for  any  other  number  whatever. 

In  like  manner,  the  same  property  may  be  shown  to  belong  to  the 
number  3 ;  but  the  preference  is  usually  given  to  the  number  9,  on  ac- 
count of  its  being  more  convenient  in  practice. 

Now,  from  the  demonstration  above  given,  the  reason  of  the  rale  it- 
self is  evident :  for  the  eicess  of  9's  in  two  or  more  numbers  being 
taken  separately,  and  the  excess  of  9's  taken  also  out  of  the  sum  of  the 
former  excesses,  it  is  plain  that  this  last  excess  must  be  equal  to  the  ex- 
cess of  9's  contained  in  the  total  sum  of  all  these  numbers ;  all  the  parts 
taken  together  being  equal  to  the  whole.— This  rule  was  first  given  by 
Dr.  Waflis  in  his  Arithmetic,  published  in  the  year  1657. 


•mmuonoN.  11 

7.  Add  2;  19;  817;  4298  ;  50916  ;  730205  ;  91806% 
together.  Ans.  9966891. 

8.  How  many  days  are  in  the  twelve  calendar  months  ? 

Ana.  965. 

9.  How  many  days  are  there  from  the.  15th  day  of  April  to 
die  24th  day  of  November,  both  days  included  f     Ans,  224% 

10.  An  army  consisting  of  52714  infantry*,  or  fbot,  51  HI 
horse,  6250  dragoons,  3927  light-horse,  928  artillery,  of 
pinners,  1410  pioneers,  250  sappers,  and  406  miners  :  what 
is  the  whole  number  of  men  ?  Ans.  70995. 


OF  SUBTRACTION. 

Subtraction  teaches  to  find  how  much  one  number  ex- 
ceeds another,  called  their  difference,  or  the  remainder,  by 
taking  the  less  from  the  greater.  The  method  of  doing  which 
is  as  follows: 

Place  the  less  number  under  the  greater,  in  the  same  man- 
ner as  in  Addition,  that  is,  units  under  units,  tens  under  tens, 
and  so  on  ;  and  draw  a  line  below  them. — Begin  at  the  right 
hand,  and  take  each  figure  in  the  lower  line,  or  number, 
from  the  figure  above  it,  setting  down  the  remainder  below 
it. — But  if  the  figure  in  the  lower  line  be  greater  than  that 
above  it,  first  borrow,  or  add,  10  to  the  upper  one,  and  then 
take  the  lower  figure  from  that  sum,  setting  down  the  remain- 
der,  and  carrying  1,  for  what  was  borrowed,  to  the  next 
lower  figure,  with  which  proceed  as  before ;  and  so  on  till  the 
whole  is  finished. 


*  The  whole  body  of  foot  soldiers  is  denoted  by  the  word  htfanlrg; 
and  all  those  that  charge  on  horseback  by  the  word  Cavalry. — Some 
authors  conjecture  that  the  term  infantry  is  derived  from  a  certain  In- 
fanta of  Spain,  who,  finding  that  the  army  commanded  by  the  king 
her  lather  had  been  defeated  by  the  Moors,  assembled  n  body  of  the 
people  together  on  foot,  with  which  she  engaged  and  totally  rooted  the 
enemy.  In  honour  of  this  event,  and  to  distinguish  the  foot  soldiers, 
who  were  not  before  held  In  much  estimation,  they  received  the  name 
of  Infantry,  from  her  own  title  of  Infanta. 


4 


12 


AxrrBXxnc. 


TO  PSOVE  SUBTRACTION. 

Add  the  remainder  to  the  less  number,  or  that  which  is 
just  above  it ;  and  if  the  sum  be  equal  to  the  greater  or  up- 
permost  number,  the  work  is  right*. 


EXAMPLES. 


From  5386427 
Take  2164315 


From  5386427 
Take  4258792 


From  1234567 
Take  702973 


Rem.  3222112 


Rem.  1127635 


Rem.  531594 


Proof.  5366427 


Proof.  5386427 


Proof.  1234567 


4.  From  5331806  take  5073918.  Ans.  257888. 

5.  From  7020974  take  2766809.  Ans.  4254 165. 

6.  From  8503402  take  574271.  Ans.  7929131. 

7.  Sir  Isaac  Newton  was  born  in  the  year  1642,  and  he 
died  in  1727 :  how  old  was  he  at  the  time  of  his  decease  ? 

Ans.  85  years. 

8.  Homer  was  born  2560  years  ago,  and  Christ  1827  years 
ago :  then  how  long  before  Christ  was  the  birth  of  Homer  ? 

Ans.  733  years. 

9.  Noah's  flood  happened  about  the  year  of  the  world  1656, 
and  the  birth  of  Christ  about  the  year  4000  :  then  how  long 
was  the  flood  before  Christ  ?  Ans.  2344  years. 

10.  The  Arabian  or  Indian  method  of  notation  was  first 
known  in  England  about  the  year  1150:  then  how  long  is 
it  since  to  this  present  year  1827 1  Ans.  677  years. 

11.  Gunpowder  was  invented  in  the  year  1330  :  how  long 
was  that  before  the  invention  of  printing,  which  was  in  1441  ? 

Ans.  Ill  years. 

12.  The  mariner's  compass  was  invented  in  Europe  in  the 
year  1302 :  how  long  was  that  before  the  discovery  of  Ame- 
rica by  Columbus,  which  happened  in  1492  ? 

Ans.  190  years. 


*  The  reason  of  this  method  of  proof  is  evident;  for  if  the  difference 
of  two  jpombers  be  added  to  the  less,  it  most  manifestly  make  up  a  sum 
equal  to  the  greater. 


jcttltolicatioh.  18 


OF  MULTIPLICATION. 

Multiplication  is  a  compendious  method  of  Addition, 
teaching  how  to  find  the  amount  of  any  given  number  when 
repeated  a  certain  number  of  times  ;  as,  4  times  6,  which 
is  24. 

The  number  to  be  multiplied,  or  repeated,  is  called  the 
Multiplicand. — The  number  you  multiply  by,  or  the  number 
of  repetitions,  is  the  Multiplier. — And  the  number  found, 
being  the  total  amount,  is  called  the  Product. — Also,  both 
the  multiplier  and  multiplicand  are,  in  general,  named  the 
Terms  or  Factors. 

Before  proceeding  to  any  operations  in  this  rule,  it  is 
necessary  to  learn  off  very  perfectly  the  following  Table,  of 
all  the  products  of  the  first  12  numbers,  commonly  called 
the  Multiplication  Table,  or  sometimes  Pythagoras's  Table, 
from  its  inventor. 


MULTIPLICATION  TABLE. 


JJ 

2| 

3 

4 

5 

6 

71 

8 

3 

11 

12 

2 

4 

6 

8 

JO 

12 

14 

LO 

18 

20 

S3 

24 

3 

6 

9 

15 

18 

21 

34 

27 

30 

33 

361 

4 

8 

12 

16 

20 

24 

28 

32 

36 

40 

44 

48 

5 

10 

15  1 

20 

25 

30 

35 

40 

45 

50 

55 

60 

6 

12 

18 

24 

30 

36 

42 

48 

54 

60  66 

72 

7 

14 

21 

28 

35 

42 

49 

56 

63 

70 

77 

84 

8 

16 

24 

32 

40 

48 

56 

64 

72 

80 

88 

96 

9 

18 

27 

36 

45 

54 

63 

72 

81 

130 

99 

108 

10 

20 

30 

40 

50 

60 

70 

80 

00 

100 

110 

120 

11 

22 

33 

44 

55 

66 

77 

88 

99 

110 

121 

132 

12 

24 

36 

48 

00 

72 

84 

96 

10s|l20 

132 

144; 

14 


ARITHMETIC* 


To  multiply  any  Given  Number  by  a  Single  Figure,  or  by  any 
Number  not  exceeding  12. 

*  Set  the  multiplier  under  the  unite9  figure  or  right-hand 
place,  of  the  multiplicand,  and  draw  a  line  below  it. — Then, 
beginning  at  the  right-hand,  multiply  every  figure  in  this 
by  the  multiplier. — Count  how  many  tens  there  are  in  the 
product  of  every  single  figure,  and  set  down  the  remainder 
directly  under  the  figure  that  is  multiplied  ;  and  if  nothing 
remains,  set  down  a  cipher. — Carry  as  many  units  or  ones  as 
mere  are  tens '  counted,  to  the  product  of  the  next  figures ; 
and  proceed  in  the  same  manner  till  the  whole  is  finished. 


EXAMPLE* 

Multiply  9876543210  the  Multiplicand. 
By  2  the  Multiplier. 


19753066420 


To  multiply  by  a  Number  consisting  of  Several  Figures. 

f  Set  the  multiplier  below  the  multiplicand,  placing  them 
as  in  Addition,  namely,  units  under  units,  tens  under  tens,  &c. 
drawing  a  line  below  it.  —Multiply  the  whole  of  the  multi- 
plicand by  each  figure  of  the  multiplier,  as  in  the  last  article ; 


6678 

*  The  reason  of  this  rale  is  the  same  as  for  4 
the  process  in  Addition,  in  which  1  is  car-  — — 
ried  for  every  10,  to  the  next  place,  gradu-        32  =  8X4 
ally  as  the  several  products  are  produced      280  =      70  X  4 
one  after  another,  instead  of  setting  them  all     2400  =     600  X  4 
down  below  each  other,  as  in  the  annexed  ex-  20000  =   6000  X  4 

ample.    ■ 

22712  =   5678  X  4 


t  After  having  found  the  product  of  the  multiplicand  by  the  first 
figure  of  the  multiplier,  as  in  the  former  case,  the  multiplier  is  supposed 
to  be  divided  into  parts,  and  the  product  is  found  for  the  second  figure 
in  the  same  manner:  but  as  this  figure  stands  in  the  place  of  tens,  the 
product  must  be  ten  times <jts  simple  value  ;  and  therefore  the  first 
figure  of  this  product  must  be  set  in  the  place  of  tens ;  or,  which  is  the 
same  thing,  directly  under  the  figure  multiplying  by.   And  proceeding 


MULTIPLICATION. 


15 


setting  down  a  line  of  products  for  each  figure  in  the  multi- 
plier, oo  as  that  the  first  figure  of  each  line  may  stand  straight 
under  the  figure  multiplying  by.  Add  all  the  lines  of  pro* 
ducts  together,  in  the  order  in  which  they  stand,  and  their 
sum  will  be  the  answer  or  whole  product  required. 

TO  PROVE  MULTIPLICATION. 

There  are  three  different  ways  of  proving  multiplication, 
which  are  as  below  : 

First  Method.  —  Make  the  multiplicand  and  multiplier 
change  places,  and  multiply  the  latter  by  the  former  in  the 
same  manner  as  before.  Then  if  the  product  found  in  this 
way  be  the  same  as  tho  former,  the  number  is  right. 

Second  Method.—*  Cast  all  the  9's  out  of  the  sum  of  the 
figures  in  each  of  the  two  factors,  as  in  Addition,  and  set 
down  the  remainders.  Multiply  these  two  remainders  to- 
gether, and  cast  the  9's  out  of  the  product,  as  also  out  of  the 
whole  product  or  answer  of  the  question,  reserving  the  re- 
mainders of  these  last  two,  which  remainders  must  be  equal 
when  the  work  is  right. — Note,  It  is  common  to  set  the  four 
remainders  within  the  four  angular  spaces  of  a  cross,  as  in 
the  example  below. 


In  this  manner  separately  with  all  the      1234567  the  multiplicand, 
figures  of  the  multiplier,  it  is  evident  4567 

that  we  shall  multiply  all  the  parts  of  

the  multiplicand  by  all  the  parts  of      8641969—     7  times  the  mult, 
the  multiplier,  or  the  whole  of  the    7407402  =    60  times  ditto, 
multiplicand  by  the  whole  of  the  mul-  6172b35    =  500 times  ditto, 
tiplier:  therefore  these  several  pro- 4938268     =4000  times  ditto. 

ducts  being  added  together,  will  be  

equal  to  the  whole  required  product ;  6638267489— 4667  times  ditto, 
as  in  the  example  annexed.     

*  This  method  of  proof  is  derived  from  the  peculiar  property  of  the 
number  9,  mentioned  in  the  proof  of  Addition,  and  the  reason  for  the 
one  includes  that  of  the  other.  Another  more  ample  demonstration  of 
this  rule  may,  however,  be  as  follows : — Let  p  and  q  denote  the  number 
of  9's  in  the  factors  to  be  multiplied,  and  a  and  6  what  remain  ;  then  9p 
-4-  a  and  9q  +  6  will  be  the  numbers  themselves,  and  their  product  ia 
(9r  X  9q)  +  (9p  X  b)  +  (9q  X  fl)  +  («  v  6  J ;  but  the  first  three  of  these 
products  are  each  a  precise  number  of  9's,  because  their  factors  are  so, 
either  one  or  both :  these  therefore  being  cast  away,  there  remains  only 
II X  6;  and  if  the  9's  also  be  cast  out  of  this,  the  excess  is  the  excess  of 
9's  in  the  total  product :  but  a  and  b  are  the  eicesses  in  the  factors 
themselves,  and  a  X  b  is  their  product ;  therefore  the  rule  is  true.  This 
mode  of  proof,  however,  is  not  an  ample  check  against  the  errors  that 
night  arise  from  a  transposition  of  figures. 


16 


ARITHMETIC. 


Third  Method. — Multiplication  is  also  very  naturally  prov- 
ed by  Division ;  for  the  product  divided  by  either  of  the  fac- 
tors, will  evidently  give  the  other.  But  this  cannot  be  prac- 
tised till  the  rule  of  division  is  learned. 


EXAMPLES* 


Mult  3542  or  Mult.  6190 

by     6196  Proof.  by  3542 


21252  \       /  12392 

31878              \2/  24784 

3542  30980 

21252  X  *\  18588 


21946232  21946232  Proof! 


OTHER  EXAMPLES. 


Multiply  123456789 
Multiply  123456789 
Multiply  123456789 
Multiply  123456789 
Multiply  123456789 
Multiply  123456789 
Multiply  1234567b9 
Multiply  123456789 
Multiply  123456789 
Multiply  302914603 
Multiply  273580961 
Multiply  402097316 
Multiply  82164973 
Multiply  7564900 
Multiply  8496427 
Multiply  2760625 


by  3. 
by  4. 
by  5. 
by  6. 
by  7. 
by  8. 
by  9. 
by  11. 
by  12. 
by  16. 
by  23. 
by  195. 
by  3027. 
by  579. 
by  874359. 
by  37072. 


Ans.  370370367. 
Ans.  493827156. 
Ans.  617288945. 
Ans.  740740734; 
Ans.  864197523. 
Ans.  987654312. 
Ans.  1111111101. 
Ans.  1358024679. 
Ans.  1481481468. 
Ans.  4846633648. 
Ans.  6292362103. 
Ans.  78408976620. 
Ans.  248713373271. 
Ans.  4380077100. 
Ans.  7428927415293. 
Ans.  102330768400. 


CONTRACTIONS  IN  MULTIPLICATION. 

I.  When  there  are  Ciphers  in  the  Factors. 

If  the  ciphers  be  at  the  right-hand  of  the  numbers  ;  mul- 
tiply the  other  figures  only,  and  annex  as  many  ciphers  to 
the  right-hand  of  the  whole  product,  as  are  in  both  the  fac- 
tors.— When  the  ciphers  are  in  the  middle  parts  of  the  mul- 
tiplier ;  neglect  them  as  before,  oniy  taking  care  to  place 


MULTIPLICATION. 


17 


the  first  figure  of  every  line  of  products  exactly  under  the 
figure  you  are  multiplying  with. 


EXAMPLES. 


1. 

Mult.  9001035 
by   -  70100 


9001635 
63011445 


2. 

Mult.  390720400 
by    .  406000 

23443224 
15628816 


631014613500    Products  158632482400000 


3.  Multiply  81503600  by  7030.        Ans.  572970308000. 

4.  Multiply  9030100  by  2100.        Ans.  18963210000. 

5.  Multiply  8057069  by  70050.       Ans.  564397683450. 

II.  When  the  Multiplier  is  the  Product  of  iwo  or  more  Num- 
bers in  the  Table  ;  then 

*  Multiply  by  each  of  those  parts  separately,  instead  of 
the  whole  number  at  once. 


EXAMPLES. 

1.  Multiply  51307298  by  56,  or  7  times  8. 
51307298 
7 


359151086 
8 


2873208088 


2.  Multiply  31704592  by 

3.  Multiply  29753804  by 

4.  Multiply  7128368  by 

5.  Multiply  160430800  by 

6.  Multiply  61835720  by 


36.  Ans.  1141365312. 

72.  Ans.  2142273888. 

96.  Ans.  684323328. 

108.  Ans.  17326526400. 

1320.  Ans.  81623150400. 


*  The  reason  of  this  rule  is  obvious  enough  ;  for  any  number  multi- 
plied by  the  component  parts  of  another,  must  give  the  same  product 
as  if  it  were  multiplied  by  that  number  at  once.  Thus,  in  the  1st  ex- 
ample, 7  times  the  product  of  8  by  the  given  number,  makes  66  time! 
the  same  number,  as  plainly  as  7  times  8  make  5o\ 

Vol.  I.  4 


is 


ARITHMETIC. 


7.  There  was  an  army  composed  of  104 4  battalions,  eacb 
consisting  of  500  men  ;  what  was  the  number  of  men  con- 
tained in  the  whole  ?  Ans.  52000. 

8.  A  convoy  of  ammunition  f  bread,  consisting  of  250 
waggons,  and  each  waggon  containing  320  loaves,  having 
been  intercepted  and  taken  by  the  enemy,  what  is  the  num- 
ber of  loaves  lost  ?  Ans.  80000. 


OF  DIVISION. 

Division  is  a  kind  of  compendious  method  of  Subtrac- 
tion, teaching  to  find  how  often  one  number  is  contained  in 
another,  or  may  be  taken  out  of  it  :  which  is  the  same  thing. 

The  number  to  be  divided  is  called  the  Dividend*— 
The  number  to  divide  by,  is  the  Divisor. — And  the  number 
of  times  the  dividend  contains  the  divisor,  is  called  the 
Quotient. — Sometimes  'there  is  a  Remainder  left,  after  the 
division  is  finished. 

The  usual  manner  of  placing  the  terms,  is,  the  dividend 
in  the  middle,  having  the  divisor  on  the  left  hand,  and  the 
quotient  on  the  right,  each  separated  by  a  curve  line;  as, 
to  divide .  12  by  4,  the  quotient  is  3, 

Dividend  12 
Divisor  4)         12         (3  Quotient;  4subtr. 
showing  that  the  number  4  is  3  times  — 
contained  in  12,  or  may  be  3  times  8 
subtracted  out  of  it,  as  in  the  margin.  4  subtr. 

%  Ride.— Having  placed  the  divisor  — 
before  the  dividend,  as  above  directed,  4 
find  how  often  the  divisor  is  contained  4  subtr. 

in  as  many  figures  of  the  dividend  as  — 
are  just  necessary,  and  place  the  num-  0 
ber  on  the  right  in  the  quotient.    Mul-  — 


*  A  battalion  is  a  body  of  foot,  consisting  of  500,  or  000,  or  700  men, 
more  or  less. 

t  The  ammunition  bread,  is  that  which  is  provided  for,  and  distribut- 
ed to,  the  soldiers ;  the  usual  allowance  being  a  loaf  of  6  pounds  to 
•vary  soldier,  once  in  4  days. 

X  In  this  way  the  dividend  is  resolved  into  parts,  and  by  trial  is  found 
how  often  the  divisor  is  contained  in  each  of  those  parti,  one  after  an- 
other, arranging  the  several  figures  of  the  quotient  one  after  another, 
into  one  number. 


19 


tiply  the  divisor  by  this  number,  and  set  the  product  under 
the  figures  of  the  dividend,  before-mentioned. — Subtract  this 
product  from  that  part  of  the  dividend  under  which  it  stands, 
and  bring  down  the  next  figure  of  the  dividend,  or  more  if 
necessary,  to  join  oh  the  right  of  the  remainder.— Divide  this 
numbef,  so  increased,  in  the  same  manner  as  before  ;  and  so 
on,  till  all  the  figures  are  brought  down  and  used. 

Note*  If  it  be  necessary  to  bring  down  more  figures  than 
one  to  any  remainder,  in  order  to  make  it  as  large  as  the  di- 
visor, or  larger,  a  cipher  must  be  set  in  the  quotient  for  every 
figure  so  brought  down  more  than  one. 

TO  PROVE  DIVISION. 

*  Multiply  the  quotient  by  the  divisor ;  to  this  product 
add  the  remainder,  if  there  bo  any  ;  then  the  sum  will  be 
equal  to  the  dividend,  when  the  work  is  right. 


When  there  is  no  remainder  to  a  division,  the  quotient  is  the  whole 
and  perfect  answer  to  the  question.   But  when  there  is  a  remainder,  it 

res  so  much  towards  another  time,  as  it  approaches  to  the  divisor :  so, 
the  remainder  be  half  the  divisor,  it  will  go  the  half  of  a  time  more  ; 
if  the  4th  part  of  the  divisor,  it  will  go  one-fourth  of  a  time  more  ;  and 
so  on.  Therefore,  to  complete  the  quotient,  set  the  remainder  at  (he 
end  of  it,  above  a  small  line,  and  the  divisor  below  it,  thus  forming  a 
fractional  part  of  the  whole  quotient. 

*  This  method  of  proof  is  plain  enough:  for  since  the  quotient  is  the 
number  of  times  the  dividend  contains  the  divisor,  the  quotient  multi- 
plied by  the  divisor  must  evidently  be  equal  to  the  dividend. 

There  are  several  other  methods  sometimes  used  for  proving  Divi- 
sion, some  of  the  most  useful  of  which  are  as  follow: 

Second  Method  Subtract  the  remainder  from  the  dividend,  and  di- 
vide what  is  left  by  the  quotient ;  so  shall  tbe  new  quotient  from  this 
last  division  be  equal  to  the  former  divisor,  when  the  work  is  right. 

Third  Method. — Add  together  the  remainder  and  all  the  products  of 
the  several  quotient  figures  by  the  divisor,  according  to  the  order  in 
which  they  stand  in  the  work ;  and  the  sum  will  be  equal  to  the  divi- 
dend, when  the  work  is  right 


to 


abithottic. 


examples. 


1  QuoU 
3)  1234567  (  411522 
12  mult.  3 


3 
3 


15 
15 


1234566 
add  1 


4  1234567 
3   


Proof. 


2  Quot, 
37)  12345678  (  333666 
111  37 


124 
111 

135 
111 


2335662 
1000996 
rem.  36 

12345G78 


246  Proof. 
222 


6 
6 


247 
222 


7 
6 


258 
222 


Rem.  1 


Rem.  36 


Divide  73146085  by  4. 
Divide  53179b6027  by  7. 
Divide  570196382  by  12. 
Divide  74638105 
Divide  137896254 
Divide  35821649 
Divide  72091365 


Ana.  18286521J. 
Ans.  759712289$. 
Ans.  47516365/,. 
Ans.  2017246,^. 
Ans.  142I6l6f$. 
Ans.  46886}Jf . 


An*.  13*61  §y±\, 


by  37. 
by  97. 
by  764. 
by  5201. 

10.  Divide  4637064283  by  57606.     Ans.  80496ftf£f 

11.  Suppose  471  men  are  formed  into  ranks  of  3  deep, 
what  is  the  number  in  each  rank?  Ans.  157. 

12.  A  party,  at  the  distance  of  378  miles  .from  the  head 
quarters,  receive  orders  to  join  their  corps  in  18  days :  what 
number  of  miles  must  they  march  each  day  to  obey  their 
orders?  Ans.  21. 

13.  The  annual  revenue  of  a  nobleman  being  37960Z.  ; 
how  much  per  day  is  that  equivalent  to,  there  being  365  days 
in  the  year  ?  Ans.  104Z. 


CONTRACTIONS  IN  DIVISION. 


There  are  certain  contractions  in  Division,  by  which  the 
operation  in  particular  cases  may  be  performed  in  a  shorter 
manner  :  as  follows  : 


DIVISION. 


21 


I.  Division  by  any  Small  Number,  not  greater  than  12,  may- 
be expeditiously  performed,  by  multiplying  and  subtracting 
mentally,  omitting  to  set  down  the  work  except  only  the  quo- 
tient immediately  below  the  dividend. 

BXAMPLXS. 

3)  56103061  4)52610675         5)  1370192 


Quot.  18701320$ 


6)  38672040         7)  81306627  8)  23718020 


9)  43081062        11)  576 14230        12)  27080373 


II.  *  When  Ciphers  are  annexed  to  the  Divisor';  cut  off 
those  ciphers  from  it,  and  cut  off  the  same  number  of  figures 
from  the  right-hand  of  the  dividend  ;  then  divide  with  the  re- 
maining figures,  as  usual.  And  if  there  be  any  thing  remain- 
ing after  this  division,  place  the  figures  cut  off  from  the  di- 
vidend to  the  right  of  it,  and  the  whole  will  be  the  true  re- 
mainder ;  otherwise,  the  figures  cut  off  only  will  be  the  re- 
mainder. 

EXAMPLES. 

1.  Divide  3704196  by  20.       2.  Divide  31086901  by  7100, 
2,0)  3*/04l9,6       .     71,00)  310869,01  (4378$Hft. 

  284 

Quot.  185209$}   

268 
213 

556 
497 

599 

568 

31 


*  This  method  serves  to  avoid  a  needless  repetition  of  ciphers,  wVncb 
would  happen  in  the  common  way.  And  the  truth  of  the  pnivdpYt  ou 


82 


ARITHMETIC 


3.  Divide  7380064  by  23000. 

4.  Divide  2304109  by  5800. 


Ana.  320}f£f 
Ant.  397ifiJ. 


III.  When  the  Divisor  is  the  exact  Product  of  two  or  more 
of  the  small  Numbers  not  greater  than  12  :  *  Divide  by  each 
of  those  numbers  separately,  instead  of  the  whole  divisor  at 
once. 

Note.  There  are  commonly  several  remainders  in  work- 
ing by  this  rule,  one  to  each  division  ;  and  to  find  the  true  or 
whole  remainder,  the  same  as  if  the  division  had  been  per- 
formed all  at  once,  proceed  as  follows  :  Multiply  the  last  re. 
mainder  by  the  preceding  divisor,  or  last  but  one,  and  to  the 
product  add  the  preceding  remainder  ;  multiply  this  sum  by 
the  next  preceding  divisor,  and  to  the  product  add  the  next 
preceding  remainder  ;  and  so  on  till  you  have  gone  backward 
through  all  the  divisors  and  remainders  to  the  first.  As  in 
the  example  following : 


EXAMPLES. 


1.  Divide  31046835  by  56  or  7  times  8. 


7)  31046835 

8)  4435262—1  first  rem. 

554407 — 6  second  rem. 


Ans.  554407}} 


6  the  last  rem. 
mult.  7  preced.  divisor. 

42 

add    1  to  the  1st  rem. 
43  whole  rem. 


2.  Divide  7014596  by  72. 

3.  Divide  5130652  by  132. 

4.  Divide  83016572  by  240. 


Ans.  974244f. 
Ans.  38808TW- 
Ans.  345902,VV- 


which  it  is  founded,  is  evident ;  for,  cutting  off  the  same  number  of 
ciphers,  or  figures,  from  each,  is  (he  same  as  dividing  each  of  them  by 
10,  or  100,  or  1000,  &c.  according  to  the  number  of  ciphers  cut  off; 
and  it  is  evident,  that  as  often  as  the  whole  divisor  is  contained  in  the 
whole  dividend,  so  often  must  any  part  of  the  former  be  contained  in  a 
like  part  of  the  latter. 

*  This  follows  from  the  second  contraction  in  Multiplication,  being 
only  the  converse  of  it ;  for  the  half  of  the  third  part  of  any  thing,  is 
evidently  the  same  as  the  sixth  part  of  the  whole ;  and  so  of  any  other 
numbers. — The  reason  of  the  method  of  finding  the  whole  remainder 
from  the  Several  particular  ones,  will  best  appear  from  the  nature  of 
Vulgar  Fractions.  Thus,  in  the  first  example  above,  the  first  remainder 
being  1,  when  the  divisor  is  7,  makes  ;  this  must  be  added  to  the  se- 
cond remainder,  6,  making  6+  to  the  divisor  8,  or  to  be  divided  by  8. 

Bat  6f =^|±?= y;  and  this  divided  by  8  gives  ^g-^- 


REDUCTION. 


28 


•  IV.  Common  Division  may  be  performed  more  concisely, 
by  omitting  the  several  products,  and  setting  down  only  the 
remainders;  namely,  multiply  the  divisor  by  the  quotient 
figures  as  before,  and,  without  setting  down  the  product, 
subtract  each  figure  of  it  from  the  dividend,  as  it  is  produced ; 
always  remembering  to  carry  as  many  to  the  next  figure  as 
were  borrowed  before. 


EXAMPLES. 

1.  Divide  3104679  by  833. 
833)  3104679  (3727#5. 
6050 
2257 
5919 


2.  Diyide  79165238  by  238. 

3.  Divide  29137062  by  5317. 

4.  Divide  62015735  by  7803. 


Ans.  832627,^. 
Ans.  5479f|{J. 
Ans.  79474f f f. 


OF  REDUCTION. 

Reduction  is  the  changing  of  numbers  from  one  name 
or  denomination  to  another,  without  altering  their  value. — 
This  is  chiefly  concerned  in  reducing  money,  weights,  and 
measures. 

When  the  numbers  are  to  be  reduced  from  a  higher  name 
to  a  lower,  it  is  called  Reduction  descending  ;  but  when, 
contrarywise,  from  a  lower  name  to  a  higher,  it  is  Reduction 
ascending. 

Before  we  proceed  to  the  rules  and  questions  of  Reduction, 
it  will  be  proper  to  set  down  the  usual  tables  of  money, 
weights,  and  measures,  which  are  as  follow  : 


OF  MONEY,  WEIGHTS,  AND  MEASURES. 


TABLES  OF  MONET. 


2  Farthings  =  1  Halfpenny  | 
4  Farthings  =  1  Penny  d 
12  Pence      =  1  Shilling  s 
20  Shillings  =  1  Pound  £ 


qrs  d 

4=1  s 
48  =   12  =   1  £ 
960  =  240  =  20  =  \ 


24 


ASXTHMBTIC. 


PBNCB  TABLE.  SHILLINGS  TABLE* 


d 

8 

d 

t 

d 

20 

is 

1 

8 

1 

is 

12 

30 

2 

6 

2 

24 

40 

3 

4 

3 

36 

50 

4 

2 

4 

48 

60 

5 

0 

5 

60 

70 

5 

10 

6 

72 

80 

6 

8 

7 

84 

90 

7 

6 

8 

96 

100 

8 

4 

9 

108 

110 

9 

2 

10 

120 

120 

10 

0 

11 

132 

/Vote.— £  denotes  pounds,  «  shillings,  and  d  denotes  pence. 

|  denotes  1  farthing,  or  one  quarter  of  any  thing. 

£  denotes  a  halfpenny,  or  the  half  of  any  thing. 

}  denotes  3  farthings  or  three  quarters  of  any  thing. 
The  fall  weight  and  value  of  the  English  gold  and  silver  coin, 
old  and  new,  are  as  here  below. 


both 


Gold. 

Guinea 
Half  do. 
Third  do. 
Double  Sov. 
Sovereign 
Half  do. 


Value 
£   $  d 

1  1 
0  10 

0  7 

2  0 

1  0 
0  10 


Weight, 
dwtgr 

'6  h 

2  16} 

1  l*t 
10  6+t 

5  6A 

2  13-fr 


Silver. 


Value, 
s  d 


A  Crown  5 
Half-crown  2 
Shilling  1 
Sixpence  0 


Old  Wt 
dwt  gr 
19  8* 
9  I6t 
3  21 
1  22A 


New  Wt. 

dwt  gr. 

18  4^ 
9  2^ 
3  15* 
119# 


The  usual  value  of  gold  is  nearly  41  an  ounce,  or  2d  a  grain  ;  and 
that  of  silver  is  nearly  5*  an  ounce.  Also  the  value  of  any  quantity  of 
gold,  was  to  the  value  of  the  same  weight  of  standard  silver,  as  l^rir 
to  1,  in  the  old  coin ;  bdt  in  the  new  coin  they  are  as  14^  to  1. 

Pure  gold,  free  from  mixture  with  other  metals,  usually  called  fine 

Sold,  is  of  so  pure  a  nature,  that  it  will  endure  the  fire  without  wasting, 
lough  it  be  kept  continually  melted.  But  silver,  not  having  the  purity 
of  gold,  will  not  endure  the  fire  like  it :  yet  fine  silver  will  waste  but 
very  little  by  being  in  the  fire  any  moderate  time  ;  whereas  copper, 
tin,  lead,  kc.  will  n#t  only  waste,  but  may  be  calcined,  or  burnt  to  a 
powder. 

Both  gold  and  silver,  in  their  purity,  are  so  soft  and  flexible  (like  new 
lead,  &c.)  that  they  are  not  so  useful,  either  in  coin  or  otherwise  (ex- 
cept to  beat  into  leaf  gold  or  silver),  as  when  they  are  alloyed,  or  mix- 
ed and  hardened  with  copper  or  brass.  And  though  most  nations  differ, 
more  or  less,  in  the  quantity  of  such  alloy,  as  well  as  in  the  same  place 
at  different  times,  yet  in  England  the  standard  for  gold  and  silver  coin 
has  been  for  a  long  time  as  follows— viz.  That  22  parts  of  fine  gold, 
and  2  parts  of  copper,  being  melted  together,  shall  be  esteemed  the 
true  standard  for  sold  coin  :  And  that  11  ounces  and  2  pennyweights 
of  fine  silver,  and  18  pennyweights  of  copper,  being  melted  together, 
be  esteemed  the  true  standard  for  silver  coin,  called  Sterling  silver. 

In  the  old  coin  the  pound  of  sterling  gold  was  coined  into  42|  gui- 
neas, of  21  shillkip  each,  of  which  the  pound  of  sterling  silver  was  di- 
vided into  02.  Tie  new  coin  is  also  of  the  same  quality  or  degree  of 


TABUS  OF  WEIGHTS.  2$ 


TKOY  WEIGHT*. 

Grains  -  -  marked  gr 
24  Grains  make  1  Pennyweight  dwt 
20  Pennyweightsi  Ounce  oz 
12  Ounces         1  Pound  lb 


fr  dwt 
4=    I  oz 
480=  20=  1  lb 
5760=240=12=1 


By  this  weight  are  weighed  Gold,  Silver,  and  Jewels. 

APOTHECARIES'  WEIGHT. 

Grains   -    -   marked  gr  , 
20  Grains  make  1  Scruple  sc  or  3 
3  Scruples       1  Dram   dr  or  3 
8  Drams         1  Ounce  oz  or  J 
12  Ounces        1  Pound   lb  or  ft 


8C 

20  = 

1 

dr 

60  = 

3  = 

1 

02? 

480  = 

24  = 

8  = 

1 

lb 

5760  = 

288  = 

96  = 

12  = 

1 

This  is  the  same  as  Troy  weight,  only  having  some  dif- 
ferent divisions.  Apothecaries  make  use  of  this  weight  in 
compounding  their  medicines  ;  but  they  buy  and  sell  their 
Drugs  by  Avoirdupois  weight. 


AVOIHDUPOIS  WEIGHT. 


Drams 
16  Drams 
16  Ounces 
28  Pounds 
4  Quarters 


make  1  Ounce 
-    1  Pound  - 
1  Quarter  - 
1  Hundred  weight 


marked  dr 
oz 
lb 

cwt 


20  Hundred  Weight  1  Ton 


ton 


fineness  with  that  of  the  old  sterling  gold  and  silver  above  described,  but 
divided  into  pieces  of  other  names  or  values  ;  viz.  the  pound  of  the  sil- 
ver into  66  shillings,  of  course  each  shilling  is  the  66th  part  of  a  pound ; 
and  20  pounds  of  the  gold  into  934£  pieces  called  sovereigns,  or  the 
pound  weight  into  4Gf«  sovereigns,  each  equal  to  20  of  the  new  shil- 
lings. So  that  the  weight  of  the  sovereign  is  46^$Ujs  of  a  pound, 
which  is  equal  to  pennyweights,  or  equal  to  5  dwt.  3^  gr.  very 
nearly,  as  stated  in  the  preceding  table.  And  multiples  and  parts  of  the 
sovereign  and  shilling  in  their  several  proportions. 

*  The  original  of  all  weights  used  in  England,  was  a  grain  or  corn 
of  wheat,  gathered  out  of  the  middle  of  the  ear,  and,  being  well  dried, 
SI  of  them  were  to  make  one  pennyweight,  20  penny  weigjhU  out 

Vol.  I.  5 


26 


ARITHMETIC. 


dr  oz 
16  =        1  lb 

256  =       16  =       1  qr 

7168  =     448  =     28=  1  ewi 

28672  =    1752  =    112  =  4  =    1  Urn 

573440  =  35840  =  2240  =  80  =  20  =  1 

By  this  weight  are  weighed  all  things  of  a  coarse  or  drossy 
nature,  as  Corn,  Bread,  Butter,  Cheese,  Flesh,  Grocery 
Wares,  and  some  Liquids  ;  also  all  metals,  except  Silver 
and  Gold. 

oz  dwt  gr 

Note,  that  lib  Avoirdupois  =  14  11  15J  Troy 
\oz    -      -      =   0  18 
Idr    .       -  =013} 


LONG  MEASURE. 


2  Barley-corns  make 
12  Inches  - 

3  Feet 

6  Feet  - 
5  Yards  and  a  half 
40  Poles 
8  Furlongs 
3  Miles 

69  iV  Miles  nearly 


1  Inch  - 
1  Foot  - 
1  Yard  - 
1  Fathom 
1  Pole  or  Rod 
1  Furlong 
1  Mile 
1  League 
1  Degree  - 


In  Ft 

12=  1 

36=  3  = 

V98  =  16}  = 


In 
Ft 

Yd  ' 

Fth 

PI 

Fur 

Mile 

Lea 

Deg  or 


Yd 

1  PI 
5}  =     1  Far 
7920  =    660"  =    220  =    40=  1  Mile 
63360  =  5280  =  1760  =  320  =  8  =  1 


CLOTH  MEASURE. 


2  Inches  and  a  quarter  make 
4  Nails 

3  Quarters 

4  Quarters 

6  Quarters  - 

4  Quarters  l£  Inch 


1  Nail     -      -  Nl 
1  Quarter  of  a  Yard  Qr 
1  Ell  Flemish     -  EF 
1  Yard      .       -  Yd 
1  Ell  English     -  EE 
1  Ell  Scotch       -     E  S 


ounce,  and  12  ounces  one  pound.  But  in  later  times  it  was  thought 
sufficient  to  divide  the  same  pennyweight  into  24  equal  parts*  still, 
called  grains,  being  the  least  weight  now  in  common  use ;  and  from 
thence  the  rest  are  computed,  as  in  the  Tables  above. 


TABLES  OP  HEASURE8. 


27 


SQUARE  MEA8URB. 

144  Square  Inches  make  1  Sq  Foot  -  Ft 

9  Square  Feet      .      1  Sq  Yard  -  Yd 

30$  Square  Yards    -      1  Sq  Pole  -  Pole 

40  Square  Poles    -      1  Rood  -  Rd 

4  Roods      -      -      1  Acre  -  Act 

Sq  Inc  SqFt 

144  =        1         Sq  Yd 
1296=        9  =       1  SqPl 
39204  =     272±  =     30}=     1  Rd 
1568160  =  10890  =  1210  =   40  =  1  Acr 
6272640  =  43560  =  4840  =  160  =  4  =  1 

By  this  measure,  Land,  and  Husbandmen  and  Gardeners' 
work  are  measured ;  also  Artificers'  work,  such  as  Board, 
Glass,  Pavements,  Plastering,  Wainscoting,  Tiling,  Floor- 
ing,  and  every  dimension  of  length  and  breadth  only. 

When  three  dimensions  are  concerned,  namely,  length, 
breadth,  and  depth  or  thickness,  it  is  called  cubic  or  solid 
measure,  which  is  used  to  measure  Timber,  Stone,  dec. 

The  cubic  or  solid  Foot,  which  is  12  inches  in  length  and 
breadth  and  thickness,  contains  1728  cubic  or  solid  inches, 
and  27  solid  feet  make  one  solid  yard. 


DRY,  OR  CORN  MEASURE* 


2  Pints  make  1  Quart  -      -  Qt 

2  Quarts    -    1  Pottle  -      -  Pot 

2  Pottles    -    1  Gallon  -      -  Gal 

2  Gallons  -    1  Peck  -      -  Pec 

4  Pecks  -  1  Bushel  -  -  Bu 
8  Bushels      1  Quarter  -       -  Qr 

5  Quarters  1  Wey,  Load,  or  Ton  Wey 
2  Weys    -    1  Last  -      -  Last 

Put  Gal 
8=1  Pec 
16=     2=     1  Bu 

64=     8=     4=    1  Qr 
512=    64  =    32  =    8=    1  Wey 

2560  =  320  =  160  =  40=  5=1  Last 

5120  =  640=320  =  80  =  10  =  2=1 


28 


▲uiTMjcmc* 


By  this  are  measured  all  dry  wares,  as,  Corn,  Seeds, 
Roots,  Fruits,  Salt,  Coals,  Sand,  Oysters,  <Scc. 

The  standard  Gallon  dry-measure  contained  268$  cubic  or 
solid  inches,  and  the  corn  or  Winchester  bushel  2150}  cubic 
inches ;  for  the  dimensions  of  the  Winchester  bushel,  by  the 
old  Statute,  -  were  8  inches  deep,  and  18£  inches  wide  or  in 
diameter.  But  the  Coal  bushel  was  to  be  19£  inches  in  dia- 
meter ;  and  36  bushels,  heaped  up,  made  a  London  chaldron 
of  coals,  the  weight  of  which  was  3136  lb  Avoirdupois,  or  1 
ton  8  cwt  nearly.    See,  however,  page  29. 


ALE  AND  BEER  MEASURE. 


2  Pints  make 

1  Quart 

Qt 

4  Quarts 

1  Gallon  . 

Gal 

36  Gallons  - 

1  Barrel 

Bar 

1  Barrel  and  a  half 

1  Hogshead  - 

Hhd 

2  Barrels  - 

1  Puncheon  ~ 

Pun 

2  Hogsheads 

1  Butt 

Butt 

2  Butts 

1  Tun 

Tun 

Pfc  Qt 

2=  1 

Gal 

8  =     4  = 

1 

Bar 

288  =  144  = 

36  = 

1  Hhd 

432  =  216  = 

54  = 

1}=  1  Butt 

864=  432  = 

108  = 

3=2=1 

Nate.  The  Ale  Gallon  contained  282  cubic  or  solid  inches, 
by  which  also  milk  was  measured. 


WISE  MEASURE. 


2  Pints  make 

1  Quart 

Qt 

4  Quarts 

1  Gallon 

Gal 

42  Gallons,  . 

1  Tierce 

Tier 

63  Gallons  or  1£  Tierces 

1  Hogshead  • 

Hhd 

2  Tierces  - 

1  Puncheon  - 

Pun 

2  Hogsheads 

1  Pipe  or  Butt 

Pi 

2  Pipes  or  4  Hhds 

1  Tun 

Tun 

Pts  Qt 

2  =       1  Gal 

8=       4=  1 

Tier 

336  =    168  =    42  = 

1 

Hhd 

504  =    252  =    63  = 

H 

=  1  Pun 

672  =    336  =    84  = 

2 

=  1*=  1 

Pi 

1008  =    504  =  126  = 

3 

-4-3*- 

1  Tun 

2016  =  1008  =  252  = 

6 

2  =  1 

TABLES  OF  MEASURES  AITD  TIME.  29 

Note,  by  this  are  measured  all  Wines,  Spirits,  Strong- 
waters,  Cyder,  Mead,  Perry,  Vinegar,  Oil,  Honey,  &c. 

The  old  Wine  Gallon  contained  231  cubic  or  solid  inches. 
And  it  is  remarkable  that  these  Wine  and  Ale  Gallons  have 
the  same  proportion  to  each  other,  as  the  Troy  and  Avoir- 
dupois Pounds  have ;  that  is,  as  one  Pound  Troy  is  to  one 
Pound  Avoirdupois,  so  is  one  Wine  Gallon  to  one  Ale 
Gallon. 


OF 


60  Seconds  or  60"  make 

-   1  Minute  - 

ilfor' 

60  Minutes 

-    1  Hour  - 

Hr 

24  Hours 

•   1  Day 

Day 

7  Days 

.    lWeek  - 

»* 

4  Weeks 

.    1  Month  - 

Mo 

13  Months  1  Day  6  Hours,  ) 
or  365  Days  6  Hours  $ 

1  Julian  Year 

Yr 

Sec 
60  = 
3600  = 
86400  = 


Min 
1 

60  *= 
1440  = 


Hr 

1  Day 
24  =  1 


Wk 


604800  =    10080  =    168  =     7  =  1  Mo 
2419200  =    40320  =    672  =    28  =  4  =  1 
31557600  ==  525960  =  8766  =  365J        =      1  Year 


Wk  Da  Hr  Mb 
Or  52      1     6  =  13 

Da  Hr  M  Sec 

But  365  5   48  -  45£  =  Solar  Year 


Da  Hr 
1    6=1  Julian  Year 


IMPERIAL  MEASURES. 

By  the  late  Act  of  Parliament  for  Uniformity  of  Weights 
and  Measures,  which  commenced  its  operation  on  the  1st  of 
January,  1826,  the  chief  part  of  the  weightsjand  measures 
are  allowed  to  remain  as  they  were ;  the  Act  simply  pre- 
scribing scientific  modes  of  determining  them,  in  case  they 
should  be  lost. 

The  pound  troy  contains  5760  grains. 
The  pound  avoirdupois  contains  7000  grains. 
The  imperial  gallon  contains  277*274  cubic  inches. 
The  corn  bushel,  eight  times  the  above. 


30 


ARITHMETIC. 


Henco,  with  respect  to  Ale,  Wine,  and  Corn,  it  will  be 
expedient  to  possess  a 

TABLE  OF  FACTORS, 


For  converting  old  measures  into  new,  and  the  contrary. 


By  decimals. 

By  vulgar  frac- 
tions nearly. 

Corn 
Measure. 

Wine 
Measure. 

Ale 
Measure. 

Corn 
Mea- 
sure. 

Wine 
Mea- 
sure. 

Ale 
Mm. 
sure. 

To  convert  old  j 
measures  to  neW.  1 

•96943 

•83311 

1-01704 

H 

H 

To  convert  new  )  f  ,*« . . 
measures  to  old.  \  1H)3IM 

1-20032 

•98324 

!  H 

* 

N.  B.  For  reducing  the  prices,  these  numbers  must  all 
be  reversed. 


RULES  FOR  REDUCTION. 

I.  When  the  Numbers  are  to  be  reduced  from  a  Higher 
Denomination  to  a  Lower  : 

Multiply  the  number  in  the  highest  denomination  by  as 
many  of  the  next  lower  as  make  an  integer,  or  1,  in  that 
higher  ;  to  this  product  add  the  number,  if  any,  which  was 
in  this  lower  denomination  before,  and  set  down  the  amount. 

Reduce  this  amount  in  like  manner,  by  multiplying  it  by 
as  many  of  the  next  lower  as  make  an  integer  of  this,  taking 
in  the  odd  parts  of  this  lower,  as  before.  And  so  proceed 
through  all  the  denominations  to  the  lowest ;  so  shall  the 
number  last  found  be  the  value  of  all  the  numbers  which 
were  in  the  higher  denominations,  taken  together*. 


*  The  reason  of  this  rule  is  very  evident;  for  pounds  are  brought 
into  shillings  by  multiplying  them  by  20 ;  shillings  into  pence,  by  mul- 
tiplying them  by  12  ;  and  pence  into  farthings,  by  multiplying*  by  4; 
and  the  reverse  of  this  rule  by  division.— And  the  same,  it  is  evident, 
will  be  true  in  the  reduction  of  numbers  consisting  of  any  denomina- 
tions whatever. 


HOLES  FOR  SEDUCTION. 


31 


EXAMPLE. 

1.  Ill  12342  15*  7d,  how  many  farthings  ? 
I        8  d 
1234    15  7 


24095  Shillings 
12 


206347  Pence 
4 


Answer    1 1 85388  Farthings. 


II.  When  the  Numbers  are  to  be  reduced  from  a  Lower  De- 
nomination to  a  Higher  : 

Divide  the  given  number  by  as  many  of  that  denomina- 
tion as  make  1  of  the  next  higher,  and  set  down  what  re- 
mains, as  well  as  the  quotient. 

Divide  the  quotient  by  as  many  of  this  denomination  as 
make  1  of  the  next  higher  ;  setting  down  the  now  quotient, 
and  remainder,  as  before. 

Proceed  in  the  same  manner  through  all  the  denomina- 
tions to  the  highest ;  and  the  quotient  last  found,  together 
with  the  several  remainders,  if  any,  will  be  of  the  same  value 
as  the  first  number  proposed. 

EXAMPLES. 

2.  Reduce  1185388  farthings  into  pounds,  shillings,  and 
pence. 

4)  1185388 
12)  2963474 


2,0)    2469,5*— Id 


Answer    1234Z  15*  Id 


3.  Reduce  24Z  to  farthings.  Ans.  23040. 

4.  Reduce  337587  farthings  to  pounds,  &c. 

Ans.  3511  \3s 


83 


.ARITHMETIC* 


5.  How  many  farthings  are  in  36  guineas  ?   Ans.  36288. 

6.  In  36288  farthings  how  many  guineas  ?         Ans.  36. 

7.  In  69  lb  13  dwts  5  gr.  how  many  grains  ?  Ans.  340157. 

8.  In  8012131  grains  how  many  pounds,  d&c. 

Ans.  1390  lb  11  oz  18  dwfc  19  gr. 

9.  In  35  ton  17  cwt  1  qr  23  lb  7  oz  13  dr  how  many  drams  ? 

Ans.  20571005. 

10.  How  many  barley-corns  will  reach  round  the  earth, 
supposing  it,  according  to  the  best  calculations,  to  be  25000 
miles?  Ans.  4752000000. 

11.  How  many  seconds  are  in  a  solar  year,  or  365  days 
5  hrs  48  min.  45}  sec  ?  Ans.  31556925}. 

12.  In  a  lunar  month,  or  29  ds  12  hrs  44  min  3  sec,  how 
many  seconds?  Ans.  2551443. 


COMPOUND  ADDITION. 

Compound  Addition  shows  how  to  add  or  collect  several 
numbers  of  different  denominations  into  one  sum. 

Rule. — Place  the  numbers  so,  that  those  of  the  same  de- 
nomination may  stand  directly  under  each  other,  and  draw  a 
line  below  them.  Add  up  the  figures  in  the  lowest  deno- 
mination, and  find,  by  Reduction,  how  many  units,  or  ones, 
of  the  next  higher  denomination  are  contained  in  their  sum. 
—Set  down  the  remainder  below  its  proper  column,  and 
carry  those  units  or  ones  to  the  next  denomination,  which 
add  up  in  the  same  manner  as  before. — Proceed  thus  through 
all  the  denominations,  to  the  highest,  whose  sum,  together 
with  the  several  remainders,  will  give  the  answer  sought. 

The  method  of  proof  is  the  same  as  in  Simple  Addition. 


COMPOUND  ADDITION. 


SI 


EXAMPLES  OF  MONEY*. 


1. 

2. 

3. 

4. 

I 

s 

d 

/  1 

<* 

/ 

8 

d 

Z 

d 

7 

13 

3 

14  7 

5 

15 

17 

10 

53 

14 

8 

3 

5 

lO-i 

8  19 

2f 

3 

14 

6 

5 

10 

Sf 

6 

18 

7 

7  8 

1} 

23 

6 

*1 

93 

11 

6 

0 

2 

5j 

21  2 

9 

14 

9 

*i 

7 

5 

0 

4 

0 

3 

7  16 

8J- 

15 

6 

4 

13 

2 

5 

17 

15 

*i 

0  4 

3 

6 

12 

0 

18 

7 

99 

15 

9? 

32 

2 

6j 

39 

15 

9J 

5.  6. 

I     s  d  lad 

14    0  7J  37  15  8 

8  15  3  14  12  9; 

62   4  7  17  14  9 

4  17  8  23  10  9J 

23   0  4f  8   6  0 

6   6  7  14   0  5J 

91    0  10{  54   2  l\ 


7. 

8. 

1      8  d 

/  8 

d 

61    3  2£ 

472  15 

3 

7  16  8 

9  2 

29  13  lOf 

27  12 

si 

12  16  2 

370  16 

21 

0    7  5J 

13  7 

4 

24  13  0 

6  10 

5f 

5   0  10? 

30  0 

11* 

Exam.  9.  A  nobleman,  going  out  of  town,  is  informed  by 
his  steward,  that  his  butcher's  bill  comes  to  197/  13*  7\d  ; 
his  baker's  to  592  5*  2Jd  ;  his  brewer's  to  85/ ;  his  wine* 
merchant's  to  103/  13*  ;  to  his  corn  chandler  is  due  75/  3d  ; 
to  his  tallow-chandler  and  cheesemonger,  27/  15*  11{</;  and 
to  his  tailor  55/  3*  5f  d  ;  also  for  rent,  servants'  wages,  and 
other  charges,  127/  3*  :  Now,  supposing  he  would  take  100/ 
with  him,  to  defray  his  charges  on  the  road,  for  what  sum 
must  he  send  to  -bis  bankor  ?  Ans.  8301 14s  $Vd 

Vol.  I.  6 


34 


ARITHMETIC. 


10.  The  strength  of  a  regiment  of  foot,  of  10  companies, 
and  the  amount  of  their  subsistence*,  for  a  month  of  SO 
days,  according  to  the  annexed  Table,  are  required  ? 


Numb. 

Rank. 

Subsistence  for  a  Month. 
• 

1 

Colonel 

£27 

0 

0 

1 

Lieutenant  Colonel 

19 

10 

0 

1 

Major 

17 

5 

0 

7 

Captains 

78 

15 

0 

11 

Lieutenants 

57 

15 

0 

9 

Ensigns 

40 

10 

0 

1 

Chaplain 

7 

10 

0 

1 

Adjutant 

4 

10 

0 

1 

Quarter-Master 

5 

5 

0 

1 

Surgeon 

4 

10 

0 

1 

Surgeon's  Mate 

4 

10 

0 

30 

Serjeants 

45 

0 

0 

30 

Corporals 

30 

0 

0 

20 

Drummers 

20 

0 

0 

2 

Fifers 

2 

0 

0 

390 

Private  Men 

292 

10 

0 

507 

Total. 

£656  10 

0 

*  Subsistence  Money,  is  the  money  paid  to  the  soldiers  weekly ; 
which  is  short  of  their  fall  pay,  because  their  clothes,  accoutrements, 
Ac.  are  to  be  accounted  for.  It  is  likewise  the  money  advanced  to 
officers  till  their  accounts  are  made  up,  which  is  commonly  once  a 
year,  when  they  are  paid  their  arrears.  The  following  table  shows  the 
foil  pay  and  subsistence  of  each  rank  on  the  English  establishment. 


COMPOUND  ADDITION. 


35 


1*4 
a  in 


7  4 «  —  «  _  o  ~  no<  d  _  t  t-  ' 
|         o  as    "  o  '<=       o  *  -  » 


if  3 


i 


£3 


CS=J         CI  Q  w  2  .  ,  O  Q  .  ,  , 

1W         -  Q  3  O  O   .  .QQ  -  .  . 

5*^>  -  -  -  -»  cor-'  +vo  | 

2*  *  n  cc*fl  ,«t^  .  ,  —  l- 


*"-    QQ      '  5    '3000    ,  (QO 

«  o  o  a  v  o  ^  a,  6  -a  »~ — 

^  £  S£  **  *o    *^     » <c  .  .  — *  r* 

O    w  i  fi  ^  g  o  "   

:  "  ii  ■  ^  , 


Ira   Jtuoq  fg 

"TV  r»™  <wj  w»n 


.irfj  Pin  .>i!.|..„[  *a 
Pi  Jiff  4#J  .uinj.ttdE 
-jy  ptrm  liv  j  wajQ 


U  mi  Lii.ifi  r 
ail  ,rjtu)*Min 


3IJ]    Mtl    JUJCM]  STT 

-(V  pin  Vq,[  twijij 


2  *  *S    ■  ■  & «  c  ^  r«S 

*    «   «  7J      .    <£>    .  T    .  O  i  c 


.3.  K 


2  -  "2   •  :  'a  ■ 

r  9    -  O  O    .      O  O 


3* 


1 


f  s  1 1 

■i|f! 

■  c 


2U 

-  c 


-    £  = 


in 

ill 
ill 

if  5 
HI 


■ 

Mi 


*  111 


5  I  : 
1  t5S 

c      -  — 

*^  _  — 

|  • 

I.1? 

ti: 

*  r-  51 


36 


ARITHMETIC. 


EXAMPLES  OF  WEIGHTS.  MEASURES,  <f . 


TROT  WEIGHT.  APOTHEC ARIES'  WEIGHT. 


1. 

2. 

3. 

4. 

lb 

oz 

dwt 

oz 

dwt  gr 

lb 

oz  dr 

sc 

oz 

dr 

sc 

17 

3 

15 

37 

9  3 

3 

5  7 

2 

3 

5 

1 

17 

7 

9 

4 

9 

5  3 

13 

7  3 

0 

7 

3 

2 

5 

0 

10 

7 

8 

12  12 

19 

10  6 

2 

16 

7 

0 

12 

9 

5 

0 

17 

7  8 

0 

9  1 

2 

7 

3 

2 

9 

176 

2 

17 

5 

9  0 

36 

3  5 

0 

4 

1 

2 

18 

23 

11 

12 

3 

0  19 

5 

8  6 

1 

36 

4 

1 

14 

AVOIRDUPOIS  WEIGHT.  LONG  MEASURE. 

5.  6.  7.  8. 

lb  oz  dr  cwt  qr  lb  mis  fur  pis  yds  feet  inc 

17  10  13  15    2  15  29   3  14  127    1  5 

5  14  8  6  3  2  4  19  6  29  12  2  9 
12  9  18  9  1  14  7  0  24  10  0  10 
27    1    6  9    1  17  9    1  37  54    1  11 

040  10   2    6  703  527 

6  14  10  3    0    3  4    5    9  23    0  5 


CTOTH  MEASURE.  LAND  MEASURE. 

9.  10  11.  12. 

yds  qr  nls  el  en  qrs  nls  ac  ro  |>  ac   ro  p 

26    3    1  270    1  0  225  3  37  19    0  16 

13    1    2  57    4  3  16  1  25  270    3  29 

9    1    2  18    1  2  7  2  18  6    3  13 

217    0    3  0    3  2  4  2    9  23    0  34 

9    1    0  10    1  0  42  1  19  7    2  16 

55    3    1  4    4  1  7  0    6  75    0  23 


WINE  .MEASURE.  ALF.  AND  BEER  MEASURE. 

13.  14.  15.  16. 

t  hds  gal  hds  gal  pts  hds  gal  pts  hds  gal  pts 

13  3  15  15  61    5  17  37    3  29  43  5 
8    1  37  17  14  13  9  10  15  12  19  7 

14  1  20  29  23  7  3  6  2  14  16  6 
25    0  12  3  15    1  5  14    0  6    8  1 

3    1    9  16    8    0  12  .9    6  57  13  4 

72    3  21  4  96    (5  8  42    4  5    6  0 


COMPOUND  SUBTRACTION. 


37 


COMPOUND  SUBTRACTION. 


Compound  Subtraction  shows  how  to  find  the  difference 
between  any  two  numbers  of  different  denominations.  To 
perform  which,  observe  the  following  Rule. 

*  Place  the  less  number  below  the  greater,  so  that  the 
parts  of  the  same  denomination  may  stand  directly  under 
each  other ;  and  draw  a  line  below  them. — Begin  at  the 
right-hand,  and  subtract  each  number  or  part  in  the  lower 
line,  from  the  one  just  above  it,  and  set  the  remainder 
straight  below  it. — But  if  any  number  in  the  lower  line.be 
greater  than  that  above  it,  add  as  many  to  the  upper  number 
as  make  1  of  the  next  higher  denomination  ;  then  take  the 
lower  number  from  the  upper  one  thus  increased,  and  set 
down  the  remainder.  Carry  the  unit  borrowed  to  the  next 
number  in  the  lower  line  ;  after  which  subtract  this  number 
from  the  one  above  it,  as  before ;  and  so  proceed  till  the 
whole  is  finished.  Then  the  several  remainders,  taken  to- 
gether, will  be  the  whole  difference  sought. 

The  method  of  proof  is  the  same  as  in  Simple  Subtraction. 


EXAMPLES  OP  MONKF. 


1.  2.               3.  4. 

1    s  d  1      *  d  1     s    d  1     s  d 

From  79  17  8}  103    3  2£  81  10  11  254  12  0 

Take  35  12  4'  71  12  5j  29  13    3|  37    9  4f. 

Rem.  44    5  4£  31  10  83 

Proof  79  17  8J-  103    3  2£ 


5.  What  is  the  difference  between  73/  5irf  and  19/  13s  10J  ? 

Ans.  53Zt>*7irf. 


*  The  reason  of  this  Rule  will  easily  appear  from  what  has  been  said 
in  Simple  Subtraction  ;  for  the  borrowing  depends  on  the  same  princi- 
ple, and  is  only  different  as  the  numbers  to  be  subtracted  are  of  differ- 
ent denominations. 


38  ARITHMETIC 

Ex.  6.  a  lends  to  b  100/,  how  much  is  b  in  debt  after  a 
has  taken  goods  of  him  to  the  amount  of  73/  12*  4|c/  ? 

Ans.  26/  7s  7J<*. 

7.  Suppose  that  my  rent  for  half  a  year  is  20/  12s,  and 
that  I  have  laid  out  for  the  land-tax  14s  6</,  and  for  several 
repairs  1/3*  3*d,  what  have  I  to  pay  of  ray  half- year's  rent? 

Ans.  \81Us2$d. 

8.  A  trader,  failing,  owes  to  a  35/  7s  6d,  to  b  91/  13s  \d, 
to  c  53/  7»  cZ,  to  d  87/  5*,  and  to  e  111/  2s  5$d.  When 
this  happened,  he  had  by  him  in  cash  23/  7s  bd,  in  wares 
53/11*  10{df  in  household  furniture  63/  17*  7£</,  and  in 
recoverable  book-debts  25/  7s  5d.  What  will  his  creditors 
lose  by  him,  supposing  these  things  delivered  to  them  ? 

Ans.  212/  5*  3}<*. 

EXAMPLES  OF  WEIGHTS,  MEASURES,  6fC. 

TROT  WEIGHT.  APOTHECARIES1  WEIGHT. 

1.  2.  3. 

lb  oz  dwt  gr  lb  oz  dwt  gr  lb  oz  dr  scr  gr 

From  9   2  12  10  7  10   4  17  73  4   7   0  14 

Take  5    4    6  17  3    7  16  12  29  5    3    4  19 


Rem. 
Proof 


AVOIRDUPOIS  WEIGHT.  LONG  MEASURE. 

4.                 5.  6.  7. 

c  qrs  lb        lb    oz  dr  m  fu  pi        vd    ft  in 

From  5   0  17       71    5    9  14   3  17       96    0  4 

Take  2    3  10        17    9  18  7    6  11        72    2  9 


Rem. 


Proof 


CLOTH  MEASURE.  LAND  MEASURE. 

8.  ».  10.  11. 

yd  qr  nl      vd  qr  nl       ac  ro  p        ac  ro  p 

From  17   2    1        9   0  2        17    1  14       57    1  16 

Take   9    0    2       7    2  1        16    2    8       22    3  29 

Rem. 


Proof 


COMPOUND  MULTIPLICATION. 


39 


WI5*  MEASURE.  ALE  AND  BEER  MEASURE. 

12.  13.                 14.  15. 

t    hd  gal  hd  gal  pt        hd  gal  pt      hd  gal  pt 

From  17    2  23  5   0   4         14  29  3      71  16  5 

Take   9    1  36  2  12   6          9  35  7      19    7  I 

Rem. 

Proof 


DRY  MEASURE.  TIME.. 

16.  17.  18.  19. 

la  qr  bu  bu  gal  pt  mo  we  da  ds  hrs  min 

From  9   4   7  13    7    1  71  2    5  114  17  26 

Take  6   3    5  9   2   7  17  1    6  72  10  37 

Rem. 

Proof 


20.  The  line  of  defence  in  a  certain  polygon  being  236 
yards,  and  that  part  of  it  which  i9  terminated  by  the  curtain 
and  shoulder  being  146  yards  1  foot  4  inches  ;  what  then  was 
the  length  of  the  face  of  the  bastion  ?     Ans.  89  yds  1  ft  8  in. 


COMPOUND  MULTIPLICATION. 

Compound  Multiplication  shows  how  to  find  the  amount 
of  any  given  number  of  different  denominations  repeated  a 
certain  proposed  number  of  times  ;  which  is  performed  by 
the  following  rule. 

Set  the  multiplier  under  the  lowest  denomination  of  the 
multiplicand,  and  draw  a  line  below  it. — Multiply  the  num- 
ber in  the  lowest  denomination  by  the  multiplier,  and  find 
how  many  units  of  the  next  higher  denomination  arc  con- 
tained in  the  product,  setting  down  what  remains. — In  like 
manner,  multiply  the  number  in  the  next  denomination,  and 
to  the  product  carry  or  add  the  units,  before  found,  and  dud 
how  many  units  of  the  next  higher  denomination  arc  m  VVvvs 


40 


ARITHMETIC 


amount,  which  carry  in  like  manner  to  the  next  product, 
setting  down  the  overplus. — Proceed  thus  to  the  highest  de- 
nomination proposed  :  so  shall  the  last  product,  with  the  se- 
veral remainders,  taken  as  one  compound  number,  be  the 
whole  amount  required. — The  method  of  Proof,  and  the  rea- 
son of  the  Rule,  are  the  same  as  in  Simple  Multiplication. 


EXAMPLES  OF  MONF.Y. 


1.  To  find  the  amount  of  8  lb  of  Tea,  at  5*.  8hd.  per  lb. 
s  d 

5  Si 


£2    5    8  Answer. 

/     -v  d 

2.  4  lb  of  Tea,  at  7s  8d  per  lb.  Ans.   1  10  8 

3.  6  lb  of  Butter,  at  $\d  per  lb.  Ans.   0    4  9 

4.  7  lb  of  Tobacco,  at  1*  8$d  per  lb.  Ans.  0  11  1H 

5.  8  stone  of  Beef,  at  2s  l\d  per  st.  Ans.  110 

6.  10  cwt  cheese,  at  2Z 17*  lOcZ  per  cwt.  Ans.  28  18  4 

7.  12  cwt  of  Sugar,  at  3Z  Is  4d  per  cwt.  Ans.  40    8  0 


CONTRACTIONS. 


I.  If  the  multiplier  exceed  12,  multiply  successively  by  its 
component  parts,  instead  of  the  whole  number  at  once. 


EXAMl'l.KS. 


1.  15  cwt  of  Cheese,  at  17*  tod  per  cwt. 

/   *  d 
0  17  6 
3 


2  12  0 

5 


13   t   6  Answer. 


I  s  d 

2.  20  cwt  of  Hops,  at  41  7*  2d  per  cwt.     Ans.  87  3  4 

3.  24  tons  of  Hay,  at  3J  7*  672  per  ton.     Ans.  81  0  0 

4.  46  eUs  of  Cloth,  at  1*  M  per  ell.         Ans.  3  7  6 


COMPOUND  HULTOUCATION. 


41 


I  sd 

Ex.  5.  63  gallons  of  Oil,  at  2s  3d  per  gall.     Ana.   7  19 

&  70  barrels  of  Ale,  at  11  4*  per  barrel.  Ans.  84  0  0 

7.  84  quarters  of  Oats,  at  1/  12*  Sd  per  qr.  Ans.  137  4  0 

8.  96quartersofBarley,atH3*4<2perqr.  Ans.112  0  0 

9.  120  days'  Wages,  at  5s  9d  per  day.     Ans.  34*  10  0 

10.  144  reams  of  Paper,  at  13s  4d  per  ream.  Ans.  96  0  0 

11.  If  the  multiplier  cannot  be  exactly  produced  by  the 
multiplication  of  simple  numbers,  take  the  nearest  number 
to  it,  either  greater  or  less,  which  can  be  so  produced,  and 
multiply  by  its  parts,  as  before. — Then  multiply  the  given 
multiplicand  by  the  difference  between  this  assumed  number 
and  the  multiplier,  and  add  the  product  to  that  before  found, 
when  the  assumed  number  is  less  than  the  multiplier,  but 
subtract  the  same  when  it  is  greater. 

EXAMPLES. 

1.  26  yards  of  Cloth,  at  3*  Of  cZ  per  yard. 
I    s  d 
0   3  0; 
5 


0  15  3J 

5 


3  16  Of 
3    0|  add 

£3  19   7*  Answer. 


EXAMPLES  OF  WEIGHTS  AND  MEASURES. 

2.  29  quarters  of  Corn,  at  21  5s  3{d  per  qr. 

Ans.  65  12  lOj 

3.  53  loads  of  Hay,  at  3Z 15*  2d  per  Id.  Ans.  199   3  10 

4.  79  bushels  of  Wheat,  at  11*  5fd  per  bush. 

Ans.  45  6  10* 

5.  97  casks  of  Beer,  at  12*  2d  per  cask.  Ans.  59  0  2 
C.  114  stone  of  Meat,  at  15*  3jrf  per  st.  Ans.   87    5  7} 

1.  2.  3. 

lb  oz  dwt  gr  lb  oz  dr  sc  gr  cwt  qr   lb  oz 

28   7    14  10  2   6   3  2    10  29    2    16  14 

5  8  12 


Vol.  L 


7 


48 


rote  fit .  pis  yds 
22   5   20  .6 
4 


5. 

yds  qra  na 
126   3  1 
7 


6. 

EC    10  pO 

28   8  27 
9 


7,     .  8.  9. 

luns  hhd  gal  pts  we  qr  bu  pe  mo  we  da  ho  mm 

20   2   26  2  24  2   5   3  172  3   6  16  49 

3  6  10 


COMPOUND  DIVISION. 

Compound  Division  teaches  how  to  divide  a  number  of 
several  denominations  by  any  given  number,  or  into  any 
number  of  equal  parts ;  as  follows : 

Place  the  divisor  on  the  left  of  the  dividend,  as  in  Simple 
Division. — Begin  at  the  left-hand,  and  divide  the  number  of 
jflfehighest  denomination  by  the  divisor,  setting  down  the 
^Hrent  in  its  proper  place. — If  there  be  any  remainder  after 
this  division,  reduce  it  to  the  next  lower  denomination,  which 
add  to  the  number,  if  any,  belonging  to  that  denomination, 
and*  divide  the  sum  by  the  divisor. — Set  down  again  this  quo- 
tient, reduce  its  remainder  to  the  next  lower  denomination 
again,  and  so  on  through  all  the  denominations  to  the  last. 


EXAMPLE*  OF  MONEY. 

Divide  237Z  8*  6d  by  2. 

I        8  d 

2)  237   8  6 


£118  14  3  the  Quotient. 


conform  Division. 


I      9  d  I       9  d 

2.  Divide   482  12  1}  by  3.  Ans.  144  4  Oj 

3.  Divide   507  3  5  by  4.  Ana.  126  15  10' 

4.  Divide  032  7  0}  by  5.  Ans.  126   9  6 

5.  Divide   090  14  3fby6.  Ana.  115   2  4* 

6.  Divide   705  10  2  by  7.  Ans.  100  15  8} 

7.  Divide  760  5  6  by  a  Ans.   95   0  s\ 

8.  Divide  761    5  7}  by  9.  Ans.    84  11  8} 

9.  Divide   829  17  10  by  10.  Ans.    82  19  9£ 

10.  Divide   937   8  8}  by  11.  Ans.   85   4  5 

11.  Divide  1145  11  4}  by  12.  Ans.   95   9  3J 


COATKACTlOlfS. 

i 

I.  If  the  divisor  eieeed  12,  find  what  simple  numbers, 
multiplied  together,  will  produce  it,  and  divide  by  them 
separately,  as  in  Simple  Division,  as  below. 


EXAXFLES. 


1.  What  is  Cheese  per  cwt,  if  16  cwt  cost  252 14i  Sdl 
I      9  d 

4)  25    14  8 


4)    6     8  8 


£  1    12  2  the  Answer. 


I  $  d 

2.  If  20  cwt  of  Tobacco  come  to  )  k     7  in  ± 

1501 6s  8rf,  what  is  that  per  cwt  ?  \ 

3.  Divide  982  8s  by  36.  Ans.  2  14  8 

4.  Divide  712  13s  \0d  by  56.  Ans.  1    5  1{ 

5.  Divide  442  4s  by  96.  Ans.  0   9  2} 

6.  At  312 10s  per  cwt,  how  much  per  lb  ?  Ans.  0   5  7} 

II.  If  the  divisor  cannot  be  produced  by  the  multiplica- 
tion of  small  numbers,  divide  by  the  whole  divisor  at  once, 
after  the  mariner  oT  Long  division,  as  follows. 


44 


ARITHMETIC* 


EXAMPLES. 


1.  Divide  59Z  6*  3fd  by  19. 
I    s    d  ltd 
19)  59   6   3}  '(3   2   5j  Ana. 
57 


09  (5 
95 

'  ~4 
4 

19  (i 

I   s     d  I   s  d 

2.  Divide  89  14    5}  by   57.  Ans.  0  13  llj 

3.  Divide  125   4   9  by   43.  Ans.  2  18  3 

4.  Divide  542   7  10  by   97.  Ans.  5  11  10 

5.  Divide  123  11    2 J  by  127.  Ans.  0  19  5* 


EXAMPLES  OF  WEIGHTS  AND  XEASUBS8. 

1.  Divide  17  lb  9  oz  0  dwts  2  gr  by  7. 

Ans.  2  lb  6  oz  8  dwts  14  gr. 

2.  Divide  17  lb  5  oz  2  dr  1  scr  4  gr  by  12. 

Ans.  1  lb  5  oz  3  dr  1  scr  12  gr. 

3.  Divide  178  cwt  3  qrs  14  lb  by  53.  Ans.  3  cwt  1  qr  14  lb. 

4.  Divide  144 mi  4  fur  20po  1  yd  2ft  0  in  by  39. 

Ans.  3  mi  5  fur  26  po  0  yds  2  ft  8  in. 

5.  Divide  534  yds  2  qrs  2  na  by  47.  Ans.  11  yds  1  qr  2  na. 

6.  Divide  77  ac  1  ro  33  po  by  51.      Ans.  1  ac  2  ro  3  po. 

7.  Divide  2  tu  0  hhds  47  gal  7  pi  by  65.  Ans.  27  gal  7  pi. 

8.  Divide  387  la  9  qr  by  72.  Ans.  5  la  3  qrs  7  bu. 

9.  Divide  206  mo  4  da  by  26.         Ans.  7  mo  3  we  5  ds. 


BULK  OF  THREE. 


45 


THE  GOLDEN  RULE,  OR  RULE  OF  THREE. 

The  Rule  of  Thus- teaches  how  to*  find  a  fourth  propor- 
tional to  three  numbers  given :  for  which  reason  it  is  some, 
times  called  the  Rule  of  Proportion.  It  is  called  the  Rule 
of  Three,  because  three  terms  or  numbers  are  given,  to  find 
a  fourth.  And  because  of  its  great  and  extensive  usefulness, 
it  is  often  called  the  Golden  Rule.  This  Rule  is  usually  by 
practical  men  considered  as  of  two  kinds,  namely,  Direct 
and  Inverse.  The  distinction,  however,  as  well  as  the  man- 
ner of  stating,  though  retained  here  for  practical  purposes, 
does  not  well  accord  with  the  principles  of  proportion ;  as 
will  be  shown  farther  on. 

The  Rule  of  Three  Direct  is  that  in  which  more  requires 
more,  or  less  requires  less.  As  in  this ;  if  three  men  dig  21 
yards  of  trench  in  a  certain  time,  how  much  will  six  men  dig 
in  the  same  time  ?  Here  more  requires  more,  that  is,  6  men, 
which  are  more  than  three  men,  will  also  perform  more  work, 
in  the  same  time.  Or  when  it  is  thus  :  if  6  men  dig  42  yards, 
how  much  will  3  men  dig  in  the  same  time  ?  Here  then,  less 
requires  less,  or  3  men  will  perform  proportionately  less  work 
than  6  men,  in  the  same  time.  In  both  these  cases  then, 
the  Rule,  or  the  Proportion,  is  Direct ;  and  the  stating  must 
be 

thus,  as  3  :  21  : :  6  :  42,  or  as  3  :  6  : :  21  :  42. 

And,  as  6  :  42  : :  3  :  21,  or  as  6  :  3  : :  42  :  21. 
But  the  Rule  of  Three  Inverse,  is  when  more  requires  less, 
or  less  requires  more.  As  in  this :  if  3  men  dig  a  certain 
quantity  of  trench  in  14  hours,  in  how  many  hours  will  6 
men  dig  the  like  quantity  ?  Here  it  is  evident  that  6  men, 
being  more  than  3,  will  perform  an  equal  quantity  of  work 
in  less  time,  or  fewer  hours.  Or  thus  :  if  6  men  perform  a 
certain  quantity  of  work  in  7  hours,  in  how  many  hours  will 
3  men  perform  the  same  ?  Here  less  requires  more,  for  3 
men  will  take  more  hours  than  6  to  perform  the  same  work. 
In  both  these  cases  then  the  Rule,  or  the  Proportion,  is  In- 
verse ;  and  the  stating  must  be 

thus,  as  6  :  14  : :  3  :   7,  or  as  6  :  3  :  :  14  :  7. 

And,  as  3  :  7  : :  6  :  14,  or  as  3  :  6  : :   7  :  14. 
And  in  all  these  statings,  the  fourth  term  is  found,  by  mul- 
tiplying the  2d  and  3d  terms  together,  and  dividing  the  pro* 
duct  by  the  1st  term. 

Of  the  three  given  numbers  :  two  of  them  contain  the  sup- 
position, and  the  third  a  demand.  And  for  stating  and  work- 
ing questions  of  these  kinds,  observe  the  following  general 
Rule: 


46 


ARITHMETIC. 


State  the  question  by  setting  down  in  a  straight  line  the 
three  given  numbers,  in  the  following  manner,  viz.  so  that 
the  2nd  term  be  that  number  of  supposition  which  is  of  the 
same  kind  that  the  answer  or  4th  term  is  to  be ;  majtiog  the 
other  number  of  supposition  the  1st  term,  and  the  demanding 
number  the  3d  term,  when  the  question  is  in  direct  propor- 
tion ;  but  contrariwise,  the  other  number  of  supposition  the 
3d  term,  and  the  demanding  number  the  1st  term,  when  the 
question  has  inverse  proportion. 

Thon,  in  both  cases,  multiply  the  2d  and  3d  terms  together, 
and  divide  the  product  by  the  1st,  which  will  give  the  answer, 
or  4th  term  sought,  viz.  of  the  same  denomination  as  the 
second  term. 

Note,  If  the  first  and  third  terms  consist  of  different  deno- 
minations, reduce  them  both  to  the  same  :  and  if  the  second 
term  be  a  compound  number,  it  is  mostly  convenient  to  re* 
duce  it  to  the  lowest  denomination  mentioned.  —  If,  after 
division,  there  be  any  remainder,  reduce  it  to  the  next  lower 
denomination,  and  divide  by  the  same  divisor  as  before,  and 
the  quotient  will  be  of  this  last  denomination.  Proceed  in 
the  same  manner  with  all  the  remainders,  till  they  be. reduc- 
ed to  the  lowest  denomination  which  the  second  admits  of, 
and  the  several  quotients  taken  together  will  be  the  answer 
required. 

Note  also,  The  reason  for  the  foregoing  Rules  will  appear, 
when  we  come  to  treat  of  the  nature  of  Proportions. — Some- 
times two  or  more  statings  are  necessary,  which  may  always 
be  known  from  the  nature  of  the  question. 

EXAMPLES. 

1.  If  8  yards  of  Cloth  cost  11  4*,  what  will  96  yards  cost? 
yds  1  s     yds    1  s 
As  8  :  1  4  : :  96  :  14  8  the  Answer. 
20 

24 
96 


144 
216 

8)2304 

2,0)  28,8* 

£14  8  Answer. 


BULB  OF  THREE. 


47 


Ex.  2.  An  engineer  having  raised  100  yards  of  a  certain 
work  in  34  days  with  5  men  ;  how  many  men  must  he  em* 
ploy  to  finish  a  like  quantity  of  work  in  15  days  ? 


ds  men    ds  men 
As  15  :  5  :  :  24  :  8  Ans. 
5 

15)  120  (8  Answer. 
120 


3.  What  will  72  yards  of  cloth  cost,  at  the  rate  of  9  yards 
for  52  12*  ?  Ans.  44/  16*. 

4.  A  person's  annual  income  being  146/ ;  how  much  is 
that  per  day  ?  Ans.  8*. 

5.  If  3  paces  or  common  steps  of  a  certain  person  be  equal 
to  2  yards,  how  many  yards  will  160  of  his  paces  make  ? 

Ans.  106  yds  2  ft. 

6.  What  length  must  be  cut  off  a  board,  that  is  9  inches 
broad,  to  make  a  square  foot,  or  as  much  as  12  inches  in 
length  and  12  in  breadth  contains  ?  Ans.  16  inches. 

7.  If  750  men  require  22500  rations  of  bread  for  a 
month  ;  how  many  rations  will  a  garrison  of  1000  men  re. 
quire  ?  Ans.  36000. 

8.  If  7  cwt  1  qr.  of  sugar  cost  26/  10*  4d  ;  what  will  be 
the  price  of  43  cwt  2  qrs  ?  Ans.  159/  2*. 

9.  The  clothing  of  a  regiment  of  foot  of  750  men  amount- 
ing to  28312  5*  ;  what  will  the  clothing  of  a  body  of  3500 
men  amount  to  ?  Ans.  13212/  10*. 

10.  How  many  yards  of  matting,  that  is  3  ft  broad,  will 
cover  a  floor  that  is  27  feet  long  and  20  feet  broad  ? 

Ans.  60  yards. 

11.  What  is  the  value  of  six  bushels  of  coals,  at  the  rate 
of  1/  14*.  6d  the  chaldron  ?  Ans.  5*  \)d. 

12.  If  6352  stones  of  3  feet  long  complete  a  certain  quan- 
tity of  walling  ;  how  many  stones  of  2  feet  long  will  raise  a 
like  quantity  ?  Ans.  9528. 

13.  What  must  be  given  for  a  piece  of  silver  weighing 
73  lb  5  oz  15  dwts,  at  the  rate  of  5*  9d  per  ounce  ? 

Ans.  253/  10*  0f<Z. 

14.  A  garrison  of  536  men  having  provision  for  12 
months  ;  how  long  will  those  provisions  last,  if  the  garrison 
be  increased  to  1124  men  ?  Ans.  174  days  and  Tf  |T. 

15.  What  will  be  the  tax  upon  763/  15*  at  the  rate  of 
3t  Qd  per  pound  sterling  ?  Ans.  1331  \3s  \\d. 


46 


ARITHMETIC. 


16.  A  certain  work  being  raised  in  12  days,  by  working  4 
hours  each  day  ;  how  long  would  it  nave  been  in  raising  by 
working  6  hours  per  day  ?  Ans.  8  days. 

17.  What  quantity  of  corn  can  I  buy  for  90  guineas,  at 
the  rate  of  6*  the  bushel  ?  Ans.  39  qra  3  bu. 

18.  A  person,  failing  in  trade,  owes  in  all  9772  ;  at  which 
time  he  has,  in  money,  goods,  and  recoverable  debts,  420Z  6* 
3JcZ ;  now  supposing  these  things  delivered  to  his  creditors,  - 
how  much  will  they  get  per  pound?  Ans.  8*  7\d. 

19.  A  plain  of  a  certain  extent  having  supplied  a  body  of 
3000  horse  with  forage  for  18  days  ;  then  how  many  days 
would  the  same  plain  have  supplied  a  body  of  2000  horse  ? 

Ans.  27  days. 

20.  Suppose  a  gentleman's  income  is  600  guineas  a  year, 
and  that  he  spends  25*  6d  per  day,  one  day  with  another  ; 
how  much  will  he  have  saved  at  the  year's  end  ? 

Ans.  164/  12*  6c*. 

21.  What  cost  30  pieces  of  lead,  each  weighing  1  cwt 
121b.  at  the  rate  of  16*  4d  the  cwt  ?  Ans.  27Z  2s  6d, 

22.  The  governor  of  a  besieged  place  having  provision  for 
54  days,  at  the  rate  of  l£lb  of  bread  ;  but  being  desirous  to 
prolong  the  siege  to  80  days,  in  expectation  of  succour,  in 
that  case  what  must  the  ration  of  bread  be  ?       Ans.  1  ^¥lb. 

23.  At  half-a-guinea  per  week,  how  long  can  I  be  boarded 
for  20  pounds  ?  Ans.  38T<&  wks. 

24.  How  much  will  75  chaldrons  7  bushels  of  coals  come 
to,  at  the  rate  of  11  13*  6d  per  chaldron  ? 

Ans.  125Z  19*  0j<*. 

25.  If  the  penny  loaf  weigh  8  ounces  when  the  bushel  of 
wheat  costs  7*  3d,  what  ought  the  penny  loaf  to  weigh  when 
the  wheat  is  at  8*  4d  ?  Ans.  6  oz  15  ffo  dr. 

26.  How  much  a  year  will  173  acres  2  roods  14  poles  of 
land  give,  at  the  rate  of  11  Is  8d  per  acre  ? 

Ans.  240Z  2*  7&d. 

27  To  how  much  amounts  73  pieces  of  lead,  each  weigh- 
ing  1  cwt  3  qrs  7  lb,  at  10Z  4*  per  fother  of  19|  cwt  ? 

Ans.  69Z4*2d  l^fq. 

28.  How  many  yards  of  stuff,  of  3  qrs  wide,  will  line  a 
cloak  that  is  1 J  yards  in  length  and  3J  yards  wide  ? 

Ans.  8  yds  Oqrs  2$  nl. 

29.  If  5  yards  of  cloth  cost  14*  2d,  what  must  be  given  for 
9  pieces,  containing  each  21  yards  1  quarter  ? 

Ans.  27Z 1* 

30.  If  a  gentleman's  estate  be  worth  2107Z  12*  a  year  ; 
what  may  he  spend  per  day,  to  save  500Z  in  the  year  ? 

Ans.  4Z  8s  ljftd. 


RULE  OF  TIIHKE.  49 

31.  Wanting  just  an  acre  of  land  cut  off  from  a  piece 
which  is  131  poles  in  breadth,  what  length  must  the  picco 
be  ?  Ans.  11  po  4  yds  2  ft  Otf  in. 

32.  At  7s  9' d  per  yard,  what  is  the  value  of  a  piece  of 
cloth  containing  53  ells  English  1  qr  ?      Ans.  25/  ISs  1  J<J. 

33.  If  the  carriage  of  5  cwt  11  lb  for  90  miles  he  1/  12s  (yd; 
how  fur  may  I  have  3  cwt  1  qr  carried  for  the  same  money? 

Ans.  151  m  3  fur  3,-^  pol. 
3-1.  Bought  a  silver  tankard,  weighing  1  lb  7  oz  14  dwts  ; 
what  did  it  cost  me  at  Hs  4d  the  ounce  ?        Ans.  (U  4s  9jd. 

35.  What  is  tho  half  3Tear's  rent  jf  547  acres  of  land,  at 
15s  Oct  the  acre  ?  Ans.  211/  19*  3d. 

36.  A  wall  that  is  to  be  built  to  the  height  of  30  feet,  was 
raised  0  feet  high  by  10  men  in  0  days ;  then  how  many  men 
must  be  employed  to  finish  the  wall  in  4  days,  at  the  same 
rate  of  working  /  Ans.  72  men. 

37.  What  will  be  the  charge  of  keeping  20  horses  for  a 
year,  at  the  rate  of  14 id  pur  dav  for  each  horse? 

Ans.  441/  0*  lOd. 

38.  If  18  ells  of  stuff  that  is  J  yard  wide,  cost  39s  M  ; 
what  will  50  oils,  of  the  same  goodness,  cost,  being  yard 
wide?  Ans.  11  i\s  3J{<#. 

39.  How  many  yards  of  paper  that  is  30  inches  wide,  will 
hang  a  room  that  is  20  yards  in  circuit  and  9  feet  high  ? 

Ans.  72  yards. 

40.  If  a  gentleman's  estate  be  worth  384/  1  0*  a  year,  and 
the  Jand-ta.x  be  assessed  at  2s  \)}Ad  per  pound,  what  is  his  net 
annual  income  ?  Ans.  331/  Is  9£<Z. 

41.  The  circumference  of  the  earth  is  about  25000  miles  ; 
at  what  rate  per  hour  is  a  person  at  the  middle  of  its  surface 
carried  round,  one  whole  rotation  being  made  in  23  hours 
56  minutes  ?  Ans.  1044TsAfe  miles. 

42.  If  a  person  drink  20  bottles  of  wine  per  month,  when 
it  costs  8s.  a  gall ;  how  many  bottles  per  month  may  ho 
drink,  without  increasing  the  expense,  when  wine  costs  10s 
he  gallon  ?  Ans.  16  bottles. 

43.  What  cost  43  nrs  5  bushels  of  corn,  at  1/  8s  6*2  the 
quarter  ?  *  Ans.  62/  3s  3J<Z. 

44.  HowT  many  yards  of  canvas  that  is  ell  wide  will  line 
50  yards  of  say  that  is  3  quartern  wide  ?  Ans.  30  yds. 

45.  If  an  ounce  of  gold  cost  4  guineas,  what  is  the  value 
of  a  grain  ?  Ans.  2TVd. 

40.  If  3  cwt  of  tea  cost  10/  12s ;  at  how  much  a  pound 
must  it  L9  rolailH,  to  gain  10/  by  the  whole  \     Ans.  3^$. 


Vol.  I. 


50 


COMPOUND  PROPORTION. 

Compound  Pbofostion  is  a  rule  by  means  of  which  the 
student  may  resolve  such  questions  as  require  two  or  more 
stsiings  in  simple  proportion. 

The  general  rule  for  questions  of  this  kind  may  be  ex. 
hibited  in  the  following  precepts :  viz. 

1.  Set  down  the  terms  that  express  the  conditions  of  the 
question  in  one  line. 

2.  Under  each  conditional  term,  set  its  corresponding  one, 
in  another  line,  putting  the  letter  a  in  the  (otherwise)  blank 
place  of  the  term  required. 

3.  Multiply  the  producing  terms  of  one  line,  and  the  pro* 
duced  terms  of  the  other  line,  continually,  and  take  the  re. 
suit  for  a  dividend. 

4.  Multiply  the  remaining  terms  continually,  and  let  the 
product  be  a  divisor. 

5.  The  quotient  of  this  division  will  be  q,  the  term  re. 
quired.** 

Note.  By  producing  terms  are  here  meant  whatever  ne- 
cessarily and  jointly  produce  any  effect ;  as  the  cause  and 
the  time ;  length,  breadth,  and  depth ;  buyer  and  his  mo- 
ney ;  things  carried,  and  their  distance,  dec.  all  necessarily 
inseparable  in  producing  their  several  effects. 

In  a  question  where  a  term  is  only  understood,  and  not  ex- 
pressed, that  term  may  always  be  expressed  by  unity. 

A  quotient  is  represented  by  the  dividend  put  above  a  line, 
and  the  divisor  put  below  it. 


EXAMPLES. 

1.  How  many  men  can  complete  a  trench  of  135  yards 
long  in  8  days,  when  16  men  can  dig  54  yards  of  the  same 
trench  in  6  days  ? 

M  D  Yds 

16  •  ...  6  ...  •  54 
a    ....   8   ....  135 


*  This  rale,  which  is  as  applicable  to  Simple  as  to  Compmmd  Propor- 
tion, was  given,  in  1706,  by  W.  Jones,  Esq.  F.R.S.,  the  father  of  the 
late  Sir  W.  Jones. 


COMPOUND  PROPORTION. 


51 


Here  16  men  and  6  days,  are  the  producing  terms  of  the 
first  line,  and  185  yards,  the  produced  term  of  the  other. 
Therefore,  by  the  rule, 

16X6X135     2X135  m 

UCa-8X54-  9  * 

the  number  of  men  required. 


ANOTHER  question. 

If  a  garrison  of  3600  men  have  bread  for  35  days,  at 
94  os  each  a  day  :  How  much  a  day  must  be  allowed  to 
4800  men,  each  for  45  days,  that  the  same  quantity  of  bread 
may  serve? 

men  ok  days  bread 

3600  .  .  24  .  .  35  .  .  1 
4800   .   .    a    .    .   45   .    .  1 

3600X24X35 


AN  EXAJfPLE  IN  SIMPLE  PROPORTION. 

If  14  yards  of  cloth  cost  21Z,  how  many  yards  may  be 
bought  for  73/ 10f? 

man  £  yds. 

1  ....  21  ....  14 
1    ....   73*  ....  q 

a  =  =  {  of  73*  =  49  yards,  Answer. 

«1 

2.  If  1002  in  one  year  gain  51  interest,  what  will  be  the 
interest  of  7501  for  seven  years  ?  Ans.  2622  10*. 

3.  If  a  family  of  8  peraons  expend  200/  in  9  months  ; 
how  much  will  serve  a  family  of  18  people  12  months  ? 

Ans.  600/. 

4.  If  27#  be  the  wages  of  4  men  for  7  days  ;  what  will  be 
the  wages  of  14  men  for  10  days  ?  Ans.  6/  15*. 

If  a  footman  travel  130  miles  in  3  days,  when  the  days 
are  12  hours  long  ;  in  how  many  days,  of  10  hours  each, 
may  he  travel  360  miles  7  Ans.  9j j  days. 

G.  If  120  bushels  of  corn  can  serve  14  horses  56  days  ; 
how  many  days  will  94  bushels  serve  6  horses  ? 

Ans.  VXL\\  day*. 


52 


ARITHMETIC. 


7.  If  8000  lbs  of  beef  serve  340  men  15  days ;  how  many 
lbs  will  serve  120  men  for  25  days  ?  Ans.  1764  lb  1 1  ^  oz. 

8.  If  a  barrel  of  beer  be  sufficient  to  last  a  family  of  8 
persons  12  days  ;  how  many  barrels  will  be  drank  by  16 
persons  in  the  space  of  a  year  7  Ans.  60 J  barrels. 

9.  If  180  men,  in  six  days,  of  10  hours  each,  can  dig  a 
trench  200  yards  long,  3  wide,  and  2  deep  ;  in  how  many 
days  of  8  hours  long,  will  100  men  dig  a  trench  of  360  yards 
long,  4  wide,  and  3  deep  ?  Ans.  48}  days. 


OP  VULGAR  FRACTIONS. 

A  Fraction,  or  broken  number,  is  an  expression  of  a 
part,  or  some  parts,  of  something  considered  as  a  whole. 

It  is  denoted  by  two  numbers,  placed  one  below  tho  other, 
with  a  line  between  them  : 

Thus,  JLIjumer*tor    \  which  is  named  3-fourths. 
4  denominator  > 

The  denominator,  or  number  placed  below  the  line,  shows 
how  many  equal  parts  the  whole  quantity  is  divided  into  ; 
and  it  represents  the  Divisor  in  Division. — And  the  Nu- 
merator, or  number  set  above  the  line,  shows  how  many  of 
these  parts  are  expressed  by  the  Fraction  :  being  the  re- 
mainder after  division. — Also,  both  these  numbers  are  in 
general  named  the  Terras  of  the  Fraction. 

Fractions  are  either  Proper,  Improper,  Simple,  Compound, 
Mixed,  or  Complex. 

A  Proper  Fraction,  is  when  the  numerator  is  less  than  the 
denominator  ;  as,  £,  or  |,  or  £,  &c. 

An  Improper  Fraction,  is  when  the  numerator  is  equal  to, 
or  exceeds,  the  denominator  ;  as,  f ,  or  f ,  or  },  &c.  In 
these  cases  the  fraction  is  called  Improper,  because  it  is  equal 
to,  or  exceeds  unity. 

A  Simple  Fraction,  is  a  single  expression,  denoting  any 
number  of  parts  of  the  integer  ;  as,  f ,  or  |. 

A  Compound  Fraction,  is  the  fraction  of  a  fraction,  or 
two  or  more  fractions  connected  with  the  word  of  between 
them  ;  as,  j  of  §,  or  $  of  £  of  3,  dec. 

A  Mixed  Number,  is  composed  of  a  whole  number  and  a 
fraction  together ;  as,  3|,  or  12f ,  dec. 

A  Complex  Fraction,  is  one  that  has  a  fraction  or  a  mixed 
number  for  its  numerator,  or  its  denominator,  or  both  ; 

i       2       I       3*  jt 
**'  "t"'  or7'  01  4  '  or  4  9  &c' 


REDUCTION  OF  VULGAR  FRACTIONS. 


53 


A  whole  or  integer  number  may  be  expressed  like  a  frac- 
tion, by  writing  1  below  it,  as  a  denominator ;  so  3  is  f ,  or  4 
is  f ,  Ac. 

A  fraction  denotes  division ;  and  its  value  is  equal  to  the 
quotient  obtained  by  dividing  the  numerator  by  the  deno- 
minator :  so  y  is  equal  to  3,  and  V  '8  equal  to  4}. 

Hence  then,  if  the  numerator  be  less  than  the  denominator, 
the  value  of  the  fraction  is  less  than  1.  But  if  the  numerator 
be  the  same  as  the  denominator,  the  fraction  is  just  equal  to 
1.  And.  if  the  numerator  be  greater  than  the  denominator, 
the  fraction  is  greater  than  1. 


REDUCTION  OF  VULGAR  FRACTIONS. 

Reduction  of  Vulgar  Fractions,  is  the  bringing  them  out 
of  one  form  or  denomination  into  another  ;  commonly  to  pre- 
pare them  for  the  operations  of  Addition,  Subtraction,  dec. ; 
of  which  there  are  several  cases. 

PROBLEM. 

To  find  the  Greatest  Common  Measure  of  Two  or  more 
Numbers. 

The  Common  Measure  of  two  or  more  numbers,  is  that 
number  which  will  divide  them  all  without  remainder ;  so,  3 
is  a  common  measure  of  18  and  24;  the  quotient  of  the 
former  being  6,  and  of  the  latter  8.  And  the  greatest  num- 
ber that  will  do  this,  is  the  greatest  common  measure  :  so  6 
is  the  greatest  common  measure  of  18  and  24  ;  the  quotient 
of  the  former  being  3,  and  of  the  latter  4,  which  will  not 
both  divide  further. 

RULE. 

If  there  be  two  numbers  only,  divide  the  greater  by  the 
less ;  then  divide  the  divisor  by  the  remainder  ;  and  so  on, 
dividing  always  the  last  divisor  by  the  last  remainder,  till 
nothing  remains  ;  so  shall  the  last  divisor  of  all  be  the  great, 
est  common  measure  sought. 

When  there  are  more  than  two  numbers,  find  the  greatest 
common  measure  of  two  of  them,  as  before ;  then  do  tho 
same  for  that  common  measure  and  another  of  lYifc  uronfofct*% 


54  ARITHMETIC 

and  so  on,  through  all  the  numbers ;  so  will  the  greatest  com- 
mon measure  last  found  be  the  answer. 

If  it  happen  that  the  common  measure  thus  found  is  1 ; 
then  the  numbers  are  said  to  be  incommensurable,  or  not  to 
have  any  common  measure,  or  they  are  said  to  be  prime  to 
each  other. 

examples. 

1.  To  find  the  greatest  common  measure  of  1908,  086, 
and  030. 

036  )  1908  (  2  So  that  36  is  the  greatest  common 

1872  measure  of  1908  and  930. 

36  )  936  (  26.    Hence  36  )  630  (  17 
7©  36 

216  270 
216  252 

18)  36  (2 
36 

m  

Hence  18  is  the  answer  required. 

2.  What  is  the  greatest  common  measure  of  246  and  372  ? 

An?.  6. 

3.  What  is  the  greatest  common  measure  of  324,  612, 
and  1032?  Ans.  12. 

CASE  I. 

To  Abbreviate  or  Reduce  Fractions  to  their  Lowest  Terms. 

*  Divide  the  terms  of  the  given  fraction  by  any  number 
that  will  divide  them  without  a  remainder  ;  then  divide  these 


*  That  dividing  both  the  terms  of  the  fraction  by  the  same  number, 
whatever  it  be,  will  give  another  fraction  equal  to  the  former,  is  evi- 
dent. And  when  these  divisions  are  performed  as  often  as  can  be  done, 
or  when  the  common  divisor  is  the  greatest  possible,  the  terms  of  the 
resulting  fraction  must  be  the  least  possible 

Note.  1.  Any  number  ending  with  an  even  number,  or  a  cipher,  is 
divisible,  or  can  be  divided,  by  2. 

2.  Any  number,  ending  with  6,  or  0,  is  divisible  by  6. 

3.  If  the  right-hand  place  of  any  number  be  0,  the  whole  is  divisible 
by  10 ;  if  there  be  two  ciphers,  it  is  divisible  by  100 ;  if  three  ciphers,  by 
1000 :  and  so  on ;  which  if  only  cutting  off  those  ciphers. 


REDUCTION  OF  WLQAJL  FRACTIONS* 


35 


quotients  again  in  the  same  manner ;  and  so  on,  till  it  appears 
that  there  is  no  number  greater  than  1  which  will  divide 
them  ;  then  the  fraction  will  be  in  its  lowest  terms. 

Or,  divide  both  the  terms  of  the  fraction  by  their  greatest 
common  measure  at  once,  and  the  quotients  will  be  the  terms 
of  the  fraction  required,  of  the  same  value  as  at  first. 

EXAMPLES. 

1.  Reduce  }jf  to  its  least  terms. 

ttt  =  tt  =  »  =  tt  =  f  =  h  the  answer. 
Or  thus : 

216)  288  (1  Therefore  72  is  the  greatest  common 

216  measure  ;  and  72)  |jj  =  J  the 

  Answer,  the  same  as  before. 

72)  216  (3 
216 

2.  Reduce       t0  iis  ^west  terms.  Ans.  J. 

3.  Reduce  J$f  to  its  lowest  terms.  Ans.  §. 

4.  Reduce  £f$  to  its  lowest  terms.  Ans.  |. 


4.  If  the  two  right-hand  figures  of  any  number  be  divisible  by  4,  the 
whole  is  divisible  by  4.  And  if  ihe  three  right-hand  figures  be  divisible 
by  8,  the  whole  is  divisible  by  8.    And  so  on. 

5.  If  the  sum  of  the  digits  in  any  number  be  divisible  by  3,  or  by  9, 
the  whole  is  divisible  by  3,  or  by  9. 

6.  If  the  right-hand  digit  be  even,  and  the  sum  of  all  the  digits  be  di- 
visible by  6,  then  the  whole  is  divisible  by  6. 

7.  A  number  is  divisible  by  11,  when  the  sum  of  the  1st,  3d,  5th,  &c. 
or  all  the  odd  places,  is  equal  to  the  sum  of  the  2d,  4th,  6th,  Ac.  or  of 
all  the  even  places  of  digits. 

8.  If  a  number  cannot  be  divided  by  some  quantity  less  than  the 
square  root  of  the  same,  that  number  is  a  prime,  or  cannot  be  divided 
by  any  number  whatever. 

9.  All  prime  numbers,  except  2  and  5,  have  either  1,  3,  7,  or  9,  in  the 
place  of  units;  and  all  other  numbers  are  composite,  or  can  be  divided. 

10.  When  numbers,  with  the  sign  of  addition  or  subtraction  between 
them,  are  to  be  divided  by  any  number,  then  each  of  those  numbers 

must  be  divided  by  it.   Thus  l^iAlli  =  5-1-4  —  2  =  7. 

11.  But  if  the  numbers  have  the  sign  of  multiplication  between  them, 
only  one  of  them  must  be  divided.  Thus, 

10X8X3  _  10  X  4  X  3  _  10  X  4  X  1  =  10  X  2  X  1  20 

6X2"      6X1  2X1  1X1  1 


56 


AKITHIUETIC. 


CASE  II. 

To  Reduce  a  Mixed  Number  to  its  Equivalent  Improper  Frac- 
tion* 

*  Multiply  the  integer  or  whole  number  by  the  deno- 
minator of  the  fraction,  and  to  the  product  add  the  numera- 
tor ;  then  set  that  sum  above  the  denominator  for  the  fraction 
required. 

EXAMPLES. 

1.  Reduce  23}  to  a  fraction. 
23 
5 


115  Or,  thus, 

2          (23X5)+2     117   t  . 
 _   ~  =        the  Answer. 

117 

5 

2.  Reduce  12 J  to  a  fraction.  Ans.  1  j5. 

3.  Reduce  14T\  to  a  fraction.  Ans.  y77. 

4.  Reduce  183fsr  to  a  fraction.  Ans.  3£-f ». 

CASE  III. 

To  Reduce  an  Improper  Fraction  to  its  Equivalent  Whole  or 
Mixed  Number. 

f  Divide  the  numerator  by  the  denominator,  and  the  quo- 
tient will  be  the  whole  or  mixed  number  sought. 

EXAMPLES. 

1.  Reduce  ^  to  its  equivalent  number. 
Here  y  or  12-7-3=4,  the  Answer. 


*  This  is  no  more  than  first  multiplying  a  Quantity  by  some  number, 
and  then  dividing  the  result  back  again  by  the  same :  which  it  is  evi- 
dent does  not  alter  the  value ;  for  any  fraction  represents  a  division  of 
the  numerator  by  the  denominator. 

t  This  rule  is  evidently  the  reverse  of  the  former ;  aod  the  reason  of 
it  is  manifest  from  the  nature  of  Common  Division. 


.msBUonozr  or  vulgab  fkactiojci.  57 

3.  Reduce  y  to  its  equivalent  number. 

Here  y  or  15-4-7=24,  the  Answer. 

&  Reduce  7Ty  to  its  equivalent  number. 

Thus,  17  )  749  (  4TV4 
68 

69   So  that  \y  =44  jV,  the  Answer. 
68 

1 

4.  Reduce  y  to  its  equivalent  number.  Ans.  8. 

5.  Reduce        to  its  equivalent  number.  Ans.  54}}. 

6.  Reduce  *ff  •  to  its  equivalent  number.  Ans.  171ff. 

CASE  IV. 

To  Reduce  a  Whole  Number  to  an  Equivalent  Fraction,  hav- 
ing a  Given  Denominator. 

*  Multiply  the  whole  number  by  the  given  denominator ; 
then  set  the  product  over  the  said  denominator,  and  it  will 
form  the  fraction  required. 

EXAMPLES. 

1.  Reduce  9  to  a  fraction  whose  denominator  shall  be  7. 

Here  9X7=63:  then  V  is  the  Answer; 
For  y =63-r-7=9,  the  Proof. 

2.  Reduce  12  to  a  fraction  whose  denominator  shall  be  13. 

Ans.  yj. 

3.  Reduce  27  to  a  fraction  whose  denominator  shall  be  11. 

Ans.  yp. 

CASE  V. 

7b  Reduce  a  Compound  Fraction  to  an  Equivalent  Simple 
one. 

f  Multiply  all  the  numerators  together  for  a  numerator, 
.  and  all  the  denominators  together  for  a  denominator,  and 
they  will  form  the  simple  fraction  sought. 


•  Multiplication  and  Division  being  here  equally  osetf,  the  result 
mst  be  the  same  as  the  quantity  first  proposed. 

f  The  troth  of  this  rule  may  be  shown  as  follows :  Let  the  compound 
faction  be  |  of  Now  }  of  ^  is  which  is  ^  \  tonaftqtMutty 
Vol,  I  9 


58  ARITHMETIC, 

When  part  of  the  compound  fraction  is  a  whole  or  mixed 
number,  it  must  first  be  reduced  to  a  fraction  by  one  of  the 
former  cases. 

And,  when  it  can  be  done,  any  two  terms  of  the  fraction 
may  be  divided  by  the  same  number,  and  the  quotients  used 
instead  of  them.  Or,  when  there  are  terms  that  are  com* 
mon,  they  may  be  omitted,  or  cancelled. 

EXAMPLES. 

1.  Reduce  J  of  f  of  f  to  a  simple  fraction. 

_     1X2X3     6      1   ,  . 

Here  2^3X4  =  24  =  4*  *•  An8Wer' 

♦ 

Or,  ^^|  =  1,  by  cancelling  the  2*s  and  3's. 

2.  Reduce  |  of  J  of  H  to  a  simple  fraction. 

2X3X10     60      12     4    .  . 
Here  3  X5X11  =  165  =  33  =  TP  the  Answer' 
2 

_    2X£X20     4    .  .  _  . 

^XjgXll  =  IP     same  as  tofore,  by  cancelling  the 

3's,  and  dividing  by  5's. 

3.  Reduce  ^  of  f  to  a  simple  fraction.  Ana. 

4.  Reduce  $  of  }  of  $  to  a  simple  fraction.        Ans.  }• 

5.  Reduce  f  pf  f  of  3}  to  a  simple  fraction.       Ans.  }. 

6.  Reduce  f  of  \  of  }  of  4  to  a  simple  fraction.  Ans.  f  • 

7.  Reduce  2  and  f  of  £  to  a  fraction.  Ans.  2. 

CASE  vi. 

Tb  Reduce  Fraction*  of  Different  Denominations  to  Equivalent 
Fractions  having  a  Common  Denominator. 

*  Multiply  each  numerator  by  all  the  denominators  ex* 
cept  its  own  for  the  new  numerators :  and  multiply  all  the 
denominators  together  for  a  common  denominator. 


f  of  f  will  be  ^X2  or  ^ ;  that  is,  the  numerators  are  multiplied  to- 
gether, and  also  the  denominators,  as  in  the  Role.  When  the  compound 
fraction  consists  of  more  than  two  single  ones ;  having  first  reduced 
two  of  them  as  above,  then  the  resulting  fraction  and  a  third  will  be  the 
same  as  a  compound  fraction  of  two  parts ;  and  so  on  to  the  last  of  all. 

*  This  is  evidently  no  more  than  multiplying  each  numerator  and  its- 
denominator  by  the  same  quantity r  and  consequently  the  value  of  the* 
fraction  ti  not  altered. 


mttcnoK  or  vttloae  fractions. 


59 


Male,  It  it  evident,  that  in  this  and  several  other  operations, 
'when  any  of  the  proposed  quantities  are  integers,  or  mixed 
tratnbersy  or  oompoond  fractions,  they  must  first  be  reduced, 
by  their  proper  Rules,  to  the  form  of  simple  fractions. 


EXAMPLES. 


1.  Reduce  *,  },  and  },  to  a  common  denominator, 

1  X  3  X  4  =  12  the  new  numerator  for  £. 
2X2X4  =  16  ditto  |. 
3  X  2  X  3  =*  18  ditto  f . 

2  X  3  X  4  =  24  the  common  denominator. 
Therefore  the  equivalent  fractions  are  £},  £f ,  and  J  }. 

Or  the  whole  operation  of  multiplying  may  often  be  per- 
formed mentally,  only  setting  down  the  results  and  given 
^0M««*»^tt|»  =  «,Jf,if  =  ^A.A»by  abbre. 
vianon. 

2.  Reduce  f  and  |  to  fractions  of  a  common  denominator. 

Ans-  Ih  *f • 

3.  Reduce  |,  },  and  f  to  a  common  denominator, 

Ans.      f$,  |f, 

4.  Reduce  |,  2},  and  4  to  a  common  denominator. 

Ans.H,}f,W- 

iVsfe  1,  When  the  denominators  of  two  given  fractions 
have  a  common  measure,  let  them  be  divided  by  it ;  then 
multiply  the  terms  of  each  given  fraction  by  the  quotient 
arising  from  the  other's  denominator. 

Ex.  ft  and  ft  =  {ft  {ft,  by  multiplying  the  former 
5        7  by  7  and  the  latter  by  5. 

2.  When  the  less  denominator  of  two  fractions  exactly 
divides  the  greater,  multiply  the  terms  of  that  which  has  the 
less  denominator  by  the  quotient. 

Ex.  4  and  ft  =  ft  and  ft,  by  mult,  the  former  by  2.* 
2 

3.  When  more  than  two  fractions  are  proposed,  h  is  some- 
times convenient,  first  to  reduce  two  of  them  to  a  common 
denominator ;  then  these  and  a  third ;  and  so  on  till  they  he 
-all  reduced  to  their  least  common  denominator. 

Ex.  |  and  J  and  J  =  J  and  f  and  \  =»  \\  and  \\  and  \\. 


CASK  VII. 

7b  reduce  Complex  Fractions  to  single  ones. 

Reduce  the  two  parts  both  to  simple  fractions ;  then  mul. 
tiply  the  numerator  of  each  by  the  denominator  of  the  other ; 
which  is  in  fact  only  increasing  each  part  by  equal  multi- 


fft  Asrrusnc. 

pUCatjons,  which  makes  no  difference  in  the  value  of  the 
▼hole. 


6' 


And 


=  Also?i  =  V: 
4     12  4J-  f 


17  v  2  _  34 
~5  *  9  ~  45' 


CASE  Tin. 

3b  find  the  valve  of  a  Fraction  in  Parte  of  the  Integer. 

Multiply  the  integer  by  the  numerator,  and  divide  the 
product  by  the  denominator,  by  Compound  Multiplication 
and  Division,  if  the  integer  be  a  compound  quantity. 

Or,  if  it  be  a  single  integer,  multiply  the  numerator  by  the 
parts  in  the  next  inferior  denomination,  and  divide  the  pro- 
duct by  the  denominator.  Then,  if  any  thing  remains,  mul- 
tiply it  by  the  parts  in  the  next  inferior  denomination,  and 
divide  by  the  denominator,  as  before  ;  and  so  on  as  far  as  ne- 
cessary ;  so  shall  the  quotients,  placed  in  order,  be  the  value 
of  the  fraction  required.* 

EXAMPLES. 


1.  What  is  the  \  of  2J6*? 
By  the  former  part  of  the  Rule 
2/6* 
4 


5)  9  4 

11  \QsQd2iq. 


2.  What  is  the  value  of  |of  III 
By  the  2d  part  of  the  Rule, 
2 
20 

3)  40  (13*  4d  Ans. 

1 
12 

3)  12  (4d 


3.  Find  the  value  of  }  of  a  pound  sterling.      Ans.  lit  W. 

4.  What  is  the  value  of  }  of  a  guinea  ?  Ads.  As  8d. 
&  What  is  the  value  of  J  of  a  half  crown  ? 


6.  What  is  the  value  of}  of  4*  \0dl 

7.  What  is  the  value  off  lb  troy  ? 

8.  What  is  the  value  of  ft  of  a  cwt  ? 

9.  What  is  the  value  of  J  of  an  acre  ? 
10.  What  is  the  value  of  ft  of  a  day? 


Ans  1*  lOjrf. 
Ans.  Ullfd. 
Ans.  9  oz  12  dwts. 
Ans.  1  qr  7  lb. 
Ans.  3  ro  20  po. 
Ans.  7  hrs  12  min. 


*  The  numerator  of  a  fraction  being  considered  as  a  remainder,  in 
.  Division,  and  the  denominator  as  the  divisor,  this  rule  is  of  ibe  same 
aature  as  Compound  Division,  or  the  valuation  of  remainders  in  the 
Hole  of  Three,  before  explained. 


mwcTioN  op  tom^r  nuonoics.  tt 


cabs  is.  ft 


7>  JMpMtf  a  JVaefofi  ,/r©ii  one  JDe^onifiafiofi  to  another. 

*  Consider  how  many  of  the  leas  denomination  make 
one  of  the  greater ;  then  multiply  the  numerator  by  that 
number,  if  the  reduction  be  to  a  leas  name,  but  multiply  the 
denominator,  if  to  a  greater. 


1.  Reduce  }  of  a  pound  to  the  fraction  of  a  penny. 

f  X  Y  *  Y  =  T  =  lVt  Ae  Answer. 

2.  Reduce  4  of  a  penny  to  the  fraction  of  a  pound. 

#  x  tV  *  1V  88       ^  Answer. 

$.  Reduce  ftl  to  the  fraction  of  a  penny.         Ana.  *fd. 

4.  Reduce  }g  to  the  fraction  of  a  pound.         Ana.  t*Vt* 

5.  Reduce  f  cwt  to  the  fraction  of  a  lb.  Ana.  y . 

6.  Reduce  ]  dwt  to  the  fraction  of  a  lb  troy.      Ana.  T£r. 

7.  Reduce  f  crown  to  the  fraction  of  a  guinea.    Ana.  fy, 

8.  Reduce  {  half-crown  to  the  fract.  of  a  shilling.  Ana.  . 

9.  Reduce  2*  6d  to  the  fraction  of  a  £.  Ana.  \. 
10.  Reduce  17*  Id  3{?  to  the  fraction  of  a  £.    Ans.  fiff. 


ADDITION  OF  VULGAR  FRACTIONS. 

If  the  fractions  have  a  common  denominator ;  add  all  the 
numerators  together,  then  place  the  sum  over  the  common 
denominator,  and  that  will  be  the  sum  of  the  fractions  re* 
quired. 

f  If  the  proposed  fractions  have  not  a  common  denomina- 
tor, they  must  be  reduced  to  one.    Also  compound  fractions 


*  This  is  the  same  as  the  Rale  of  Reduction  in  whole  numbers  from 
one  denomination  to  another. 

\  Before  fractions  are  reduced  to  a  common  denominator,  they  are 
quite  dissimilar,  as  much  as  shillings  and  pence  are,  and  therefore  can- 
not be  incorporated  with  one  another,  any  more  than  these  can.  But 
when  they  are  reduced  to  a  common  denominator,  and  made  parts  of 
the  same  thing,  their  sum,  or  difference,  may  then  be  as  properly  ex- 
pressed by  the  sum  or  difference  of  the  numerators,  as  the  sum  or  dif- 
ference of  any  two  quantities  whatever,  by  the  sum  or  ditfemw*  <A 


62  AKrr&wftncr 

must  be  reduced  to  simple  ones,  and  fractions  of  different 
denominations  to  -those  |>f  the  same  denomination.  Then 
add  the  numerators,  as  before.  As  to  mixed,  numbers,  they 
may  either  be  reduced  to  improper  fractions,  and  so  added 
with  the  others  ;  or  else  the  fractional  parts  only  added,  and 
the  integers  united  afterwards. 

'  examples. 

1.  To  add  |  and  £  together. 

Here  }+|  =  J  =  If,  the  Answer. 

2.  To  add  }  and  |  together. 

*  +  *  =  it  +  tt  =  it  =  Hi*  Answer. 

3.  To  add  J  and  7\  and  |  of  f  together. 

i+7i+i  off  =  i+.V+i  «  i+V+t  =  V 

4.  To  add  ^  and  4  together.  Ans.  If. 

5.  To  add  $  and  f  together.  Ans. 

6.  Add  \  and  ft  together.  Ans.  ft. 


their  individuals.  Whence  the  reason  of  the  Role  is  manifest,  both  for 
Addition  and  Sob  traction. 

When  several  fractions  are  to  be  collected,  it  is  commonly  best  first 
to  add  two  of  them  together  that  most  easily  reduce  to  a  common  de- 
nominator; then  add  their  sum  and  a  third,  and  so  on. 

Note  2.  Taking  any  two  fractions  whatever,  ft  and  f-j-t  for  example, 
after  reducing  them  to  a  common  denominator,  we  judge  whether  they 
are  equal  or  unequal,  by  observing  whether  the  products  35  X  11,  and 
7  X  65,  which  constitute  the  new  numerators,  are  equal  or  unequal. 
If,  therefore,  we  have  two  equal  products  35x11=7X56,  we  may 
compose  from  them  two  equal  fractions,  as  -g-f-  =  ft,  or      =  ^ . 

If,  then,  we  take  two  equal  fractions,  such  as  ft  and  we  shall 
have  36  X  11  =  7  X  56 ;  taking  from  each  of  these  7  X  11,  there  will 

OK   J 

remain  (35  —  7)  X  11  =  (65  — 11)  X  7,  whence  we  have  ^  = 

55  —  11 

In  like  manner,  if  the  terms  of  ft  were  respectively  added  to 
those  of  ff,  we  should  have  =  tf  =  ft. 

Or,  generally,  if   =  ^,  it  may  in  a  similar  way  be  shown,  that 
_  tf  _  c 

Hence,  when  two  fractions  are  of  equal  valuta  the  fraction  formed  by  ta- 
king the  sum  (or  Ike  diffirence)  of  their  numerators  respctireJy,  and  of  their 
denominators  respecticelij,  it  a  fraction  equal  in  value  to  each  of  the  original 
fractions.  This  proposition  will  be  found  useful  in  the  doctrine  of  pro- 
portions. 


MULTlFJJCATIOlf  OF  VULGAR  FRACTIOUS.  68 

•  7.  What  is  the  sum  of  f  and  f  and  4  !  Ans.  l}ff . 

&  What  is  the  sum  of  f  and  |  and     ?  Ans.  3f|. 

9.  What  is  the  sum  off  and  \  of  |,  and  9ft  ?  Ans.  10^. 

10.  What  is  the  sum  of  }  of  a  pound  and  $  of  a  shilling  ? 

Ans.  l|»t  or  13*  MM  2}?. 
11:  What  is  the  sum  of  }  of  a  shilling  and  ft  of  a  penny  1 

Ans.  y/dor7d  Hftf- 
12.  What  is  the*  sum  of }  of  a  pound,  and  f  of  a  shilling, 
and  ft  of  a  penny  ?  Ans.  fiff*  or  3*  ld  Hffl- 


SUBTRACTION  OF  VULGAR  FRACTIONS. 

Prepare  the  fractions  the  same  as  for  Addition,  when 
necessary  ;  then  subtract  the  one  numerator  from  the  other, 
and  set  the  remainder  over  the  common  denominator,  for  the 
difference  of  the  fractions  sought. 

EXAMPLES. 

1.  To  find  the  difference  between  £  and  £. 

Here  $  —  £  =  $  =  |,  the  Answer. 

2.  To  find  the  difference  between  J  and  f . 

?  —  i  =  H  —  H  =  *V  Answer. 

3.  What  is  the  difference  between  ft  and  ft  1  Ans. 

4.  What  is  the  difference  between  ft  and  ft  ?    Ans.  ft. 

5.  What  is  the  difference  between  ft  and  ft  ?   Ans.  T\fr. 

6.  What  is  the  diff.  between  5}  and  4  of  4$  ?  Ans.  4^- 

7.  What  is  the  difference  between  £  of  a  pound,  and  |  of 
I  of  a  shilling  ?  Ans.  'ft  8  or  10*  Id  \\q. 

8.  What  is  the  difference  between  $  of  5£  of  a  pound,  and 
}  of  a  shilling.  Ans.         or  11  Ss  llftd. 


MULTIPLICATION  OF  VULGAR  FRACTIONS. 
^  *  Reduce  mixed  numbers,  if  there  be  any,  to  equivalent 


♦  Multiplication  of  any  thing  by  a  fraction,  implies  the  taking  some 
put  or  parts  of  the  thing;  it  may  therefore  be  truly  eipresaadb^  * 


▲RlTHttBTft/* 


fractions ;  then  multiply  all  the  numerators  together  for  a 
numerator,  and  all  the  denominators  together  for  a  denomi- 
nator, which  will  give  the  product  required. 


BXAMPLS8. 


1.  Required  the  product  of  }  and  f . 

Here  J  Xf =^=^,  the  Answer. 
Or|X*=iX*=*. 

2.  Required  the  continued  product  of  |,  3£,  5,  and  f  of  j. 

Heiey x  T    T   T  5r"4xf""I"'^ 

3.  Requited  the  product  of  f  and  f .  Ans. 

4.  Required  the  product  of  <fo  and  Ana.  ^ . 

5.  Required  the  product  of     f,  }|.  Ans. 

6.  Required  the  product  of  },  },  and  3.  Ans.  1. 

7.  Required  the  product  of  },  f ,  and  4^.  Ans.  3^. 

8.  Required  the  product  of  f ,  and  }  of  f .  Ans. 

9.  Required  the  product  of  6,  and  }  of  5.  Ans.  20. 

10.  Required  the  product  off  of  j,  and  f  of  3f.   Ans.  |{. 

11.  Required  the  product  of  8}  and  4}}.        Ans.  14|}f  • 

12.  Required  the  product  of  5,  f,  f  of},  and  4}.  Ans.  2^-. 


DIVISION  OP  VULGAR  FRACTIONS. 

*  Prepabb  the  fractions  as  before  in  Multiplication  :  then 
divide  the  numerator  by  the  numerator,  and  the  denominator 
by  the  denominator,  if  they  will  exactly  divide  :  but  if  not, 


compound  fraction ;  which  is  resolved  by  multiplying  together  the 
numerators  and  the  denominators. 

Ad/a.  A  Fraction  b  best  multiplied  by  an  integer,  by  dividing  the 
denominator  by  it ;  bat  if  it  will  not  exactly  divide,  then  multiply  the 
numerator  by  ft. 

•  Division  being  the  reverse  of  Multiplication,  the  reason  of  the  rale 
is  evident. 

Acta,  A  fraction  is  best  divided  by  an  integer,  by  dividing  the  nume- 
rator by  It ;  bat  if  it  will  not  exactly  divide,  then  multiply  the  denorni- 
nstor  by  it. 


ftULE  Or  THXE1  IN  VULGAR  FRACTIONS.  65 

invert  the  terms  of  the  divisor,  and  multiply  the  dividend  by 
K,  as  in  Multiplication.  • 

EXAMPLES. 

1.  Divide  V  by  |. 

Here  y  4.  f  =  a  =  If,  by  the  first  method. 

2.  Divide  f  by  ft. 
Heref^A=*Xy=|Xf  =  V-4}. 


3.  It  is  required  to  divide     by  |.  Ans.  f . 

4.  It  is  required  to  divide  ^  by  }.  Ans.  fa 

5.  It  is  required  to  divide  y  by  J.  Ans.  1  J. 

6.  It  is  required  to  divide  {  by  y .  Ans.  y^. 

7.  It  is  required  to  divide     by  |.  Ans.  4. 

8.  It  is  required  to  divide  ij-  by  }.  Ans.  . 

9.  It  is  required  to  divide  ft  by  3.  Ans.  fa 

10.  It  is  required  to  divide  }  by  2.  Ans.  fa 

11.  It  is  required  to  divide  7±  by  9|.  Ans.  }|. 

12.  It  is  required  to  divide  f  of  }  by  |  of  7|.  Ans.  jJt. 


RULE  OF  THREE  IN  VULGAR  FRACTIONS. 

Make  the  necessary  preparations  as  before  directed  ;  then 
multiply  continually  together,  the  second  and  third  terms, 
and  the  first  with  its  parts  inverted  as  in  Division,  for  the 
answer*. 

EXAMPLES. 

1.  If  }  of  a  yard  of  velvet  cost  f  of  a  pound  sterling ;  what 
will  -f€  of  a  yard  cost  ? 

2.  What  will  3f  oz.  of  silver  cost,  at  6s  4d  an  ounce  ? 

Ans.  I/  I*  4J<*. 


*  This  Is  only  multiplying  the  2d  And  Sd  terms  together,  and  divld- 
bftbe  product  by  the  first,  as  in  the  Rale  of  Three  in  whole  nunbtm 
Vol.  I.  10 


AJtlTHXBTIC. 


a  If  A  of  a  ihip  be  worth  27813*  64;  what  are  A  of 
her  worth?  •  An*  8871 12$  Id. 

4.  What  is  the  purchase  of  12901  bank-stock,  at  108f  per 
cent.?  Ana.  133«1#  W. 

5.  What  is  the  interest  of  2731 15*  for  a  year,  at  3£  per 
cent.?  Ans.  8Z17*  11J<*. 

6.  If  |  of  a  ship  be  worth  731  Is  3d  ;  what  part  of  her  is 
worth  250Z 10*  ?  Ans.  J. 

7.  What  length  must  be  cut  off  a  board  that  is  7|  inches 
broad,  to  contain  a  square  foot,  or  as  touch  as  another  piece 
of  12  inches  long  and  12  broad  ?  Ans.  18jf  inches* 

8.  What  quantity  of  shalloon  that  is  J  of  a  yard  wide,  will 
line  flivards  of  cloth,  that  is  2}  yards  wide?  Ans.  31 J  yds. 

fc'  if  the  penny  loaf  weigh  6^  0z.  when  the  price  of 
wheat  is  5*  the  bushel ;  what  ought  it  to  weigh  when  the 
wheat  is  8a  6d  the  bushel  ?  Ans.  4^  oz. 

10.  How  much  in  length,  of  a  piece  of  land  that  is  11{4 
ptoles  broad,  will  make  an  acre  of  land,  or  as  much  as  40 
pdlei  in  length  and  4  in  breadth  ?  Ans.  13TyT  poles. 

Hi  If  a  courier  perform  a  certain  journey  in  35$  days, 
travelling  13f  hours  a  day  ;  how  long  would  he  be  in  per- 
forming  the  same,  travelling  only  11 -ft  hours  a  day  ? 

Ans.  40f)f  days. 

12.  A  regiment  of  soldiers,  consisting  of  976  men,  are  to 
be  new  clothed ;  each  coat  to  contain  2J  yards  of  cloth  that 
is  If  yard  wide,  and  lined  with  shalloon  J  yard  wide  :  how 
many  yards  of  shalloon  will  line  them  ? 

Ans.  4531  yds  1  qr  2f  nails. 


DECIMAL  FRACTIONS. 

A  Decimal  Fraction  is  that  which  has  for  its  deno- 
minator an  unit  (1),  with  as  many  ciphers  annexed  as  the 
numerator  has  places  ;  and  it  is  usually  expressed  by  setting 
down  thgfiumetator  only,  with  a  point  before  it,  on  the  left, 
hand.  Thus,  &  is  -4,  and  ffr  is  -24,  and  rifo  is  *074,  and 
ttVvVt  i*  '00124 ;  where  ciphers  are  prefixed  to  make  up  as 
many  placet  ma  are  ciphers  in  the  denominator,  when  there 
is  a  deficiency  in  the  figures. 

A  mixpd  numbejr  is  made  up  of  a  whole  number  with  some 
.decimal  fraction,  the  one  being  separated  from  the  other  by 
a  fcoint.   Thus,  3*25  is  the  same  as         or  f| f . 

Ciphers  on  the  right-hand  of  decimals  make  no  alteration 
in  their  value ;  for  -4,  or  '40,  or  *400  are  decimals  having  all 
IbeMne  value,  each  being  =  ^  or  f .  Bur  when  they  are 


ADDlfHMI  W  MCDIAIS. 


placed  m  the  left-hand,  they  decrease  the  value  in  m  ten4bld 
proportion :  That,  -4  is  ^  or  4  tenths ;  but  -04  is  only  t4y> 
or4himfw>dths>  and  -004  is  «nly  y/^,  or  4  thousandths. 

Ia  sWrknalfr  as  well  as  in  whole  numbers,  the  vahief  .of 
tfcefiaee*  increase  towards  Joe  left-hand,  and  4e&*ase  to. 
wards  die  right,  both  in  the  same  tenfold  proportion $  s#  in 
the  following  Scale  or  Table  of  Notation. 


3333338*333939 


ADDITION  OF  DECIMALS. 

Sbt  the  numbers  under  each  other  according  to  the  value 
of  their  places,  as  in  whole  numbers ;  in  which  state  the 
decimal  separating  points  will  stand  all  exactly  under  each 
other.  Then,  beginning  at  the  right  hand,  add  up  all  the 
columns  of  numbers  as  in  integers ;  and  point  off  as  many 
places  for  decimals,  as  are  in  the  greatest  number  of  decimal 
places  in  any  of  the  lines  that  are  added  ;  or  pla<?e  the  point 
directly  below  all  the  other  points. 


1.  To  add  together  29-0146,  and  3146*5,  and  2 J  09,  tod 
03417,  and  14-16. 


29  0146 
8146-5 
2109- 

•62417 

1416 


EXAMPLES. 


5299-29877  the  Sum. 


6S 


ABXTHXSTIC* 


2.  What  is  the  sum  of  276,  39-213,  72014-9,  417,  -and 
50821  Ans.  77770-113. 

3.  What  is  the  sum  of  7530,  16  201,  3-0142,  957*13, 
6*72119  and  -03014  ?  Ans.  8513-09653. 

4.  What  is  the  sum  of  312-09,  3-5711,  7195-6,  71-498, 
9739-215, 179,  and  -0027  ?  Ans.  17500-9718. 


SUBTRACTION  OF  DECIMALS. 

Place,  the  numbers  under  each  other  according  to  the 
value  of  their  places,  as  in  the  last  Rule.  Then,  beginning 
at  the  right-hand,  subtract  as  in  whole  numbers,  and  point  off 
the  decimals  as  in  Addition. 

EXAMPLES. 

1.  To  find  the  difference  between  91*73  and  2*138. 
91*73 
2*138 


Ans.  89.592  the  Difference. 


2.  Find  the  diff.  between  1  -9185  and  2*73.    Ans.  0*81 15. 

3.  To  subtract  4*90142  from  214*81.         Ans.  209*90858. 

4.  Find  the  diff.  between  2714  and  -916.     Ans.  2713*084. 


MULTIPLICATION  OF  DECIMALS. 

*  Place  the  factors,  and  multiply  them  together  the  same 
as  if  they  were  whole  numbers. — Then  point  off  in  the  pro- 
duct just  as  many  places  of  decimals  as  there  are  decimals  in 
both  the  factors.  But  if  there  be  not  so  many  figures  in  the 
product,  then  supply  the  defect  by  prefixing  ciphers. 


*  The  rule  will  be  evident  from  this  example Let  it  be  required  to 
multiply  -12  by  '961 ;  these  numbers  are  equivalent  to  -jfo  and  ftftfc  ; 
the  product  of  which  is  v\  g  g  g  0  =  04432,  by  the  nature  of  Notation, 
which  consists  of  as  many  places  as  there  are  ciphers,  that  isv  of  as 
many  places  as  there  are  in  both  numbers.  And  in  like  manner  for  any 
other  numbers. 


HULTIPLICATfOll  OF  DECIMAL!. 


69 


EXAMPLES* 

1.  Multiply  -321006 
by  -2465 


1605480 
1926576 
1284384 
642192 


Ana.'  •0791501640  the  Product. 


2.  Multiply  79-347  by  23-15.  Ans,  1836-88305. 

3.  Multiply  -63478  by  -8204.  Ana.  -520773512. 

4.  Multiply  -385746  by  -00464.       Ana.  -00178986144. 

CONTRACTION  I. 

To  multiply  Decimals  by  1  with  any  Number  of  Ciphers,  as 
by  10,  or  100,  or  1000,  $c. 

This  is  done  by  only  removing  the  decimal  point  so  many 
places  farther  to  the  right-hand,  as  there  are  ciphers  in  the 
multiplier ;  and  subjoining  ciphers  if  need  be. 

EXAMPLES. 

1.  The  product  of  51-3  and  1000  is  51300. 

2.  The  product  of  2-714  and  100  is 
8.  The  product  of  -916  and  1000  is 
4.  The  product  of  2i»31  and  10000  is 

CONTRACTION  II. 

To  contract  the  Operation  so  as  to  retain  only  as  many  Deci- 
mals in  the  Product  as  may  be  thought  necessary,  when  the 
Product  would  naturally  contain  several  more  Places. 

Set  the  unit's  place  of  the  multiplier  under  the  figure  of 
the  multiplicand  whose  place  is  the  same  as  is  to  be  retained 
for  the  last  in  the  product ;  and  dispose  of  the  rest  of  the 
figures  in  the  inverted  or  contrary  order  to  what  they  are 
usually  placed  in. — Then,  in  multiplying,  reject  all  the 
figures  that  are  more  to  the  right-hand  than  each  multiplying 
figure,  and  set  down  the  products,  so  that  their  njVv\-\i«iA 


70 


figures  may  fall  in  a  column  straight  below  each  other  ;  but 
observe  to  increase  the  first  figure  of  every  line  with  what 
would  arise  from  the  figures  omitted,  in  this  manner  namely 
1  from  5  to  14,  2  from  15  to  24,  3  from  25  to  34,  dec.  ;  and 
the  sum  of  all  the  lines  will  be  the  product  as  required,  com- 
monly to  the  nearest  unit  in  the  last  figure. 

EXAMPLES. 


1.  To  multiply  27-14986  by  92-41035,  so  as  to  retain  only 
four  places  of  decimals  in  the  product 


Contracted  Way. 
27  14986 
53014-29 


Common  Way. 
27-14986 
92-41035 


24434874 

13 

574930 

542997 

81 

44958 

108599 

2714 

986 

2715 

108599 

44 

81 

542997 

2 

14 

24434874 

2508-9280 

2508-9280 

650510 

2.  Multiply  480*14936  by  2-72416,  retaining  only  four 
decimals  in  the  product. 

3.  Multiply  2490-3048  by  -5*73286,  retaining  only  five 
decimals  in  the  product. 

4.  Multiply  325-701428  by  -7218393,  retaining  only  three 
decimals  in  the  product. 


DIVISION  OF  DECIMALS. 


Divide  as  in  whole  numbers  ;  and  point  off  in  the  quo- 
tient as  many  places  for  decimals,  as  the  decimal  places  in 
the  dividend  exceed  those  in  the  divisor*. 


*  The  mason  of  this  Rale  is  evident;  for,  since  the  divisor  multiplied 
by  the  quotient  gives  the  dividend,  therefore  the  Dumber  of  deoimal 
places  iu  the  dividend,  is  equal  to  those  in  the  divisor  and  quotient, 
taken  together,  by  the  nature  of  Multiplication ;  and  consequently 
the  quotient  itself  mast  contain  as  many  as  the  dividend  eieeeds  the 
divisor. 


DIVISION  OF  9MQULLL8. 


71 


Another  way  to  know  the  place  for  the  decimal  point  is 
this  :  The  first  figure  of  the  quotient  must  be  made  to  occupy 
the  same  place,  of  integers  or  decimals,  as  that  figure  of  the 
dividend  which  stands  over  the  unit's  figure  of  the  first  pro- 

When  the  places  of  the  quotient  are  not  so  many  as)  the 
Rule  requires,  the  defect  is  to  be  supplied  by  prefixing 
ciphers. 

When  there  happens  to  be  a  remainder  after  the  division  ; 
or  when  the  decimal  places  in  the  divisor  are  more  than  those 
in  the  dividend  ;  then  ciphers  may  be  annexed  to  the  divi- 
dend, and  the  quotient  carried  on  as  far  as  required. 


EXAMPLES. 


00272589  -2639 


1. 

178)  "48580998  ( 
1392 
460 
1049 
1599 
1758 
156 


3.  Divide  123-70536  by  54  25. 

4.  Divide  12  by  -7854. 

5.  Divide  4195-68  by  100. 

6.  Divide  -8297592  by  -153. 


1. 

n  27-00000  (102-3114 
6100 

8220 
3030 
3910 
12710 
2154 

Ans.  2-2802. 
Ans.  15-278. 
Ans.  41-9568. 
Ans.  5-4232. 


CONTRACTION  I. 


When  the  divisor  is  an  integer,  with  any  number  of  ciphers 
annexed :  cut  off  those  ciphers,  and  remove  the  decimal 
point  in  the  dividend  as  many  places  farther  to  the  left  as 
there  are  ciphers  cut  off,  prefixing  ciphers,  if  need  be  ;  then 
proceed  as  before. 

EXAMPLES. 

1.  Divide  45-5  by  2100. 

21-00)  -455  (  0216,  <&c. 
35 
140 
14 


3.  Divide  41020  by  32000. 
&  Divide    953  by  21600. 

4.  Divide      61  by  79000. 


73 


ARITHMETIC. 


CONTRACTION  II. 


Hence,  if  the  divisor  be  1  with  ciphers,  as  10,  100,  or 
1000,  &c ;  then  the  quotient  will  be  found  by  merely  mov- 
ing the  decimal  point  in  the  dividend  so  many  places  farther 
to  the  left,  as  the  divisor  hath  ciphers ;  prefixing  ciphers  if 
need  be. 


EXAMPLES. 

So,  217-3  -r  100  =  2  173  Ans.  419        10  = 

And   5-16  -f-  100=  Ans.  -21  -f- 1000  = 

CONTRACTION  HI. 

When  there  are  many  figures  in  the  divisor ;  or  when  only 
a  certain  number  of  decimals  are  necessary  to  be  retained 
in  the  quotient ;  then  take  only  as  many  figures  of  the  divi- 
sor as  will  be  equal  to  the  number  of  figures,  both  integers 
and  decimals,  to  be  in  the  quotient,  and  find  how  many  times 
they  may  be  contained  in  the  first  figures  of  the  dividend,  as 
usual. 

Let  each  remainder  be  a  new  dividend ;  and  for  every  such 
dividend,  leave  out  one  figure  more  on  the  right-hand  side 
of  the  divisor ;  remembering  to  carry  for  the  increase  of  the 
figures  cut  off,  as  in  the  2d  contraction  in  Multiplication. 

Note.  When  there  are  not  so  many  figures  in  the  divisor 
as  are  required  to  be  in  the  quotient,  begin  the  operation  with 
all  the  figures,  and  continue  it  as  usual  till  the  number  of 
figures  in  the  divisor  be  equal  to  those  remaining  to  be  found 
in  the  quotient ;  after  which  begin  the  contraction. 

examples. 

1.  Divide  2508-92800  by  92*41035,  so  as  to  have  only 
four  decimals  in  the  quotient,  in  which  case  the  quotient  will 
contain  six  figures. 


Contracted. 
92-4103,5)  2608-928,09(971498 
660721 
13849 
4608 
912 
80 
6  • 


Coitittum. 
92.4103,5)  2608-928,06  (27-1498 
66072106 
18848610 
46075750 
91116100 
79467850 
5639570 


2.  Divide  4109*2351  by  230-409,  so  that  the  quotient  may 
contain  only  four  decimals.  Ans.  17*8345. 


REDUCTION  OP  DECIMALS. 


78 


3.  Divide  37- 10438  by  5713-96,  that  the  quotient  may 
contain  only  five  decimals.  Ans.  '00649. 

4.  Divide  913  08  by  2137-2,  that  the  quotient  may  contain 
only  three  decimals. 


REDUCTION  OF  DECIMALS. 


CASE  I, 

To  reduce  a  Vulgar  Fraction  to  its  equivalent  Decimal. 

Divide  the  numerator  by  the  denominator,  as  in  Division 
ef  Decimals,  annexing  ciphers  to  the  numerator  as  far  as 
necessary ;  so  shall  the  quotient  be  the  decimal  required*. 


*  The  following  method  of  throwing  a  vulgar  fraction,  whose  de- 
nominator is  a  prime  number,  into  a  decimal  consisting  of  a  great  num- 
ber of  figures,  is  given  by  Mr.  Cohan  in  page  162  of  Sir  Isaac  Newton's 
Fluxions. 

[ EXAMPLE. 

Let  ^  be  the  fraction  which  is  to  be  converted  into  an  equivalent 
decimal. 

Then,  by  dividing  in  the  common  way  till  the  remainder  becomes  a 
tingle  figure,  we  shall  have  -fy  —  -03448^  for  the  complete  quotient^ 
and  this  equation  being  multiplied  by  the  numerator  8,  wiJJ  give  -f^  == 
275g4ji4.f  (,r  rather  u%  ~  27586\/ff  :  and  if  this  be  substituted  instead 
of  the  friction  in  the  first  equation,  it  will  make  ^  =  -0344827586^. 
Again,  let  this  eqaation  be  multiplied  by  6,  and  it  will  give  A  = 
'206*8965517^ ;  and  then  by  substituting  as  before 
-if  =  -034482758610689605175^ ; 

and  so  on,  as  far  as  may  he  thought  proper;  each  fresh  multiplication 
doubling  the  number  of  figures  in  the  decimal  value  of  the  fraction. 

In  the  present  instance  the  decimal  circulates  in  a  complete  period  of 
28  figures,  i.  e.  one  less  than  the  denominator  of  the  fraction.  This, 
again,  may  be  divided  into  equal  periods,  each  ot  14  figures,  as  below  : 
•03448275862068 
•96551724137931 

in  which  it  will  be  found  that  each  figure  with  the  figure  vertically  be- 
low it  makes  9;  0  +  9  =  9;  3  -f  6  ^  9 ;  and  so  on.  This  circulate  also 
comprehends  all  the  separate  values  of  &c.  in  correspond- 

ing circulates  of  28  figures,  only  each  beginning  in  a  distinct  place,  easi- 
ly ascertainable.  Thus,  ^  —  06896,  &c.  beginning  at  the  12th  place 
of  the  primitive  circulate.  ^  =  103448,  &c.  beginning  at  the  28th 
plnce.    So  that,  in  fact,  this  circle  includes  28  complete  circles. 

8ee,  on  this  curious  subject,  Mr.  Goodwyn's  Tables  of  Decimal  Cir- 
cles, and  the  Ladies'  Diary  for  1824. 
Vol.  I.  11 


AKTEOtBTICV 


BX  AMPLE** 


I.  Reduce  yV  to  a  decimal. 
24  =  4  X  6.  Then  4)  7- 


6)  1*750000 
•291606  dec. 


2.  Reduce  J,  and  J,  and  J,  to  decimals. 


3»  Reduce  f  to  a  decimal. 
4.  Reduce  ^  to  a  decimal. 
5*  Reduce  TJ¥  to  a  decimal. 


6\  Reduce        to  a  decimah. 


Ans*  *25,  and  #5,  and  *75v 
Ana.  -625. 
Ana.  -12. 
Ana.  -08135. 

Ana.  -14*154  IK- 


CASE  n. 


To  Jmd  the  Yakut  of  a  Decimal  in  terms  of  the  Inferior 
Denominations. 

Multiply  the  decimal  by  the  number  of  parts  in  the 
next  lower  denomination ;  and  cut  off  as  many  places  for  a 
remainder  to  the  right-hand,  as  there  are  places  in  the  given 
decimal. 

Multiply  that  remainder  by  the  parts  in  the  next  lower 
denomination  again,  cutting  off  for  another  remainder  as 
before. 

Proceed  in  the  same  manner  through  all  the  parts  of  the 
integer ;  then  the  several  denominations  separated  on  the 
left-hand  will  make  up  the  answer. 

Note,  This  operation  is  the  same  as  Reduction  Descending 
in  whole  numbers. 


1.  Required  to  find  the  value  of  -775  pounds  sterling. 


EXAMPLE?. 


•775 
20 


s  15-500 
12 


4  6-0Q0 


Ans.  15*  6rf» 


■SDUCTlOlf  OF  BECfMALS.  76 

%  What  is  the  value  of  -625  shil  ?fc  Ans.  74*. 

3.  What  is  the  value  of  -86352  ?  Ans.  17s  3-242. 

4.  What  is  the  value  of  -0125  lb  troy?  Ans.  3  dwts. 
&  What  is  the  value  of  -4694  lb  troy  ? 

Ans.  5  or.  12  dwts  15*744  gr. 
&  What  is  the  value  of  -625  cwt  ?  Ans.  2  qr  14  lb. 

7.  What  is  the  value  of  -009943  miles? 

Ans.  17  yd  1  ft  5-98848  inc. 
&  What  is  the  value  of  -6875  yd  ?         Ans.  2  qr  3  nls. 
9.  What  is  the  value  of  -3375  acr  ?     Ans.  1  rd  14  poles* 
19.  What  is  the  value  of  -2083  hhd of  wine? 

Ans.  13-4229  gaL 

CASS  III. 

lb  reduce  Integer*  or  Decimals  to  Equivalent  Decimal*  of 
Higher  Denominations. 

Divide  by  the  number  of  parts  in  the  next  higher  deno- 
ounation  ;  continuing;  the  operation  to  as  many  higher  de- 
aominations  as  may  be  necessary,  the  same  as  in  Reduction 
Ascending  of  whole  numbers. 

EXAMPLES. 

1.  Reduce  1  dwt  to  the  decimal  of  a  pound  troy* 

20  \  1  dwt 
12   0-05  os 

1  0-004166  dec,  lb.  Ans. 

2.  Reduce  9d  to  the  decimal  of  a  pound.       Ans/ 0*3757. 

3.  Reduce  7  drams  to  the  decimal  of  a  pound  avoird. 

Ans.  -027343751b. 

4.  Reduce  -264  to  the  decimal  of  a  I.  Ans.  0910833  6zc.  /. 

5.  Reduce  2-15  lb  to  the  decimal  of  a  cwt. 

Ans.  -019196  +  cwt. 

6.  Reduce  24  yards  to  the  decimal  of  a  mile. 

Ans.  013636  &c.  mile. 

7.  Reduce  -056  pole  to  the  decimal  of  an  acre. 

Ans.  O0035  ac. 

8.  Reduce  1-2  pint  of  wine  to  the  decimal  of  a  hhd. 

Ans.  -00238  +  hhd. 

3.  Reduce  14  minutes  to  the  decimal  of  a  day. 

Ans.  -009722  <fcc.  da* 

JO.  Reduce  -21  pint  to  the  decimal  of  a  peck. 

Ans.  -031325  pec. 

11.  Reduce  28"  12"  to  the  decimal  of  a  minute. 


79 


AKIfflMlG* 


Hon,  When  (here 
to  Vke  ieemdl  of  the  highest ; 

Set  the  given  numbers  directly  under  each  other,  for  di- 
vidends* proceeding  orderly  from  the  lowest  denomination 
to  the  highest. 

Opposite  to  each  dividend,  on  the  left-hand,  set  such  a 
number  for  a  divisor  as  will  bring  it  to  the  next  higher  name  ; 
drawing  a  perpendicular  line  between  all  the  divisors  and 
dividends  ' 

Begin  at  the  uppermost,  and  perform  all  the  divisions : 
only  observing  to  set  the  quotient  of  each  division,  as  deci- 
mal parts,  on  the  right-hand  of  the  dividend  next  below  it ; 
so  shall  the  last  quotient  be  the  decimal  required. 


EXAMPLES. 

1.  Seduce  17*  9f  J  to  the  decimal  of  a  pound. 
4  1  3- 
12  9-75 
20  J  17-8125 

£0  890625  Aits. 


2.  Beduce  191 17s  3}d  to  a  I.     Ans.  19*86354166  &c.  I. 

3.  Reduce  15*  6d  to  the  decimal  of  a  I.         Ans., -775/. 

4.  Reduce  l\d  to  the  decimal  of  a  shilling.     Ans.  *625*. 

5.  Reduce  5  oz  12  dwts  16  gr  to  lb.    Ans.  -46944  dec.  lb. 


RULE  OP  THREE  IN  DECIMALS. 

•  Pbbpaxe  the  terms,  by  reducing  the  vulgar  fractions  to 
decimals,  and  any  compound  number  either  to  decimals  of 
the  higher  denominations,  or.  to  integers  of  the  lower,  also 
the  first  and  third  terms  to  the  same  name  :  Then  multiply 
and  divide  as  in  whole  numbers. 

Note.  Any  of  the  convenient  Examples  in  the  Rule  of 
Three  or  Rule  of  Five  in  Integers,  or  Vulgar  Fractions,  may 
be  taken  as  proper  examples  to  the  same  rules  in  Decimals. 
—The  following  example,  which  is  the  first  in  Vulgar  Frac- 
tions, is  wrought  out  here,  to  show  the  method. 


DUODKCTJLAXt*  77 

If  I  of  a  yard  of  relvet  cost  fJ,  what  will  ^  yd  cost? 

yd     I        yd       I  9  d 

}  =  -375  -375  :  -4  : :  -3125  :  -333  dec.  or  6  8 

•4 


J  =  -4  -375)  -12500  (-333333  fcc. 

1250  20 
125 


#6-60666  &c. 
^  =  -8125  12 


Ans.  6*  Bd.   d  7-99099  &c.  =  8d. 


DUODECIMALS. 


Duodecimals,  or  Cross  Multiplication,  is  a  rule  used 
by  workmen  and  artificers,  in  computing  the  contents  of 
their  works.  ♦ 

Dimensions  are  usually  taken  in  feet,  inches,  and  quarters ; 
any  parts  smaller  than  these  being  neglected  as  of  no  con- 
sequence. And  the  same  in  multiplying  them  together,  or 
computing  the  contents.    The  method  is  as  follows. 

Set  down  the  two  dimensions  to  be  multiplied  together, 
one  under  the  other,  so  that  feet  may  stand  under  feet,  inches 
under  inches,  &c. 

Multiply  each  term  in  the  multiplicand,  beginning  at  the 
lowest,  by  the  feet  in  the  multiplier,  and  set  the  result  of 
each  straight  under  its  corresponding  term,  observing  to  car- 
ry  1  for  every  12,  from  the  inches  to  the  feet. 

In  like  manner,  multiply  all  the  multiplicand  by  the  inches 
and  parts  of  the  multiplier,  and  set  the  result  of  each  term 
one  place  removed  to  the  right-hand  of  those  in  the  mul- 
tiplicand ;  omitting,  however,  what  is  below  parts  of  inches, 
only  carrying  to  these  the  proper  numbers  of  units  from  the 
lowest  denomination. 

Or,  instead  of  multiplying  by  the  inches,  take  such  parts 
of  the  multiplicand  as  these  are  of  a  foot. 

Then  add  the  two  lines  together,  after  the  manner  of 
Compound  Addition,  carrying  1  to  the  feet  for  every  12 
inches,  when  these  come  to  so  many. 


78 


▲JEtlTHMBTIC. 


EXAMPLES. 

1.  Multiply  4  f  7  inc.  2.  Multiply  14  f  9  inc. 

by  6   4  by  4  6 


27 

6 

59 

0 

1 

<** 

7 

Ans.  29 

°* 

Ans.  66 

4* 

3.  Multiply  5  feet  7  inches  by  9  f  6  inc.  Ans.  43  f  6 J.  inc. 

4.  Multiply  12  f  5  inc  by  6  f  8  inc.        Ans.  82  9} 

5.  Multiply  35  f  4£  inc  by  12  f  3  inc.    Ans.  433  4| 

6.  Multiply  64  f  6  inc  by  8  f  9i  inc.     Ans.  565  8f 

Nate,  The  denomination  which  occupies  the  place  of 
inches  in  these  products,  means  not  square  inches,  but  recf- 
angles  of  an  inch  broad  and  a  foot  long.  Thus,  the  answer 
to  the  first  example  is  29  sq.  feet,  4  sq.  inches ;  to  the  second 
66  sq.  feet,  54  sq.  inches* 


INVOLUTION. 

Involution  is  the  raising  of  Powers  from  any  given  num. 
ber,  as  a  root. 

A  Power  is  a  quantity  produced  by  multiplying  any  given 
number,  called  the  Root,  a  certain  number  of  times  conti- 
nually by  itself.  Thus, 

2  =  2  is  the  root,  or  1st  power  of  2. 
2X2  =  4  is  the  2d  power,  or  square  of  2. 
2X2X2=  8  is  the  3d  power,  or  cube  of  2. 
'  2X2X2X2  =  16  is  the  4th  power  of  2,  &c. 

And  in  this  manner  may  be  calculated  the  following  Table  of 
the  first  nine  powers  of  the  first  9  numbers* 


nrroLtmozr.  79 


TABLE  OT  THE  FIRST  NINE  POWERS  OF  NUMBERS. 


1 

5 

3d 

4th 

5  th 

6th 

7th 

8th 

9ih  " 

1 

2 
3 
4 
5 
8 
7 
8 
9 

I 

1 

1 

1 

1 

1 

1 

1 

1 

8 

16 

32 

64 

128 

256 

512 

0 

27 

81 

243 

729 

2187 

6561 

19683 

16 

64 

256 

1024 

409G 

16384 

65536 

262144 

25 

125 

625 

31^5 

15620 

78125 

390625 

1953125 

m 

216 

1296 

7776 

46656 

279936 

1679616 

10077696 

id 

343 

2401  16807 

117649 

823543 

5764801 

40353607 

H 
si 

512 

721) 

4006(32768 
6561  59049 

262144 

2097152 

16777216 

134217728 

[6814*] 

4782969 

43046721 

387420489 

The  Index  or  Exponent  of  a  Pnwer,  is  the  number  de- 
noting the  height  or  degree  of  that  power  ;  and  it  is  1  more 
than  the  number  of  multiplications  used  in  producing  the 
same.  So  1  is  the  index  or  exponent  of  the  1st  power  or 
root,  2  of  the  2d  power  or  square,  8  of  the  third  power  or 
cube,  4  of  the  4th  power,  and  so  on. 

Powers,  that  are  to  be  raised,  are  usually  denoted  by 
placing  the  index  above  the  root  or  first  power. 

So  2s  =  4  is  the  2d  power  of  2. 

23  =   8  is  the  3d  power  of  2. 

24  =  16  is  the  4th  power  of  2. 

540*         is  the  4th  power  of  540,  ozc. 

When  two  or  more  powers  are  multiplied  together,  their 
.product  is  that  power  whose  index  is  the  sum  of  the  expo- 
nent of  the  factors  or  powers  multiplied.  Or  the  multiplica- 
tion of  the  powers,  answers  to  the  addition  of  the  indices. 
Thus,  in  the  following  powers  of  2, 

1st  2d   3d    4th    5th    6th     7th     8th     9th  10th 
2     4     8     16     32     64     128     256     512  1024 
orS1    2*    2s    2*     28     2s     27      2s       2B  *10 


80 


▲XtTHXETIC. 


Here,  4  X    4  =    16,  and  2  +  2  =  4  its  index  ; 

and  8  x  16=  128,  and  3  +  4=  7  its  index; 
also  16  X  64  —  1024,  and  4  +  6  =  10  its  index. 


OTHER  EXAMPLES. 

1.  What  is  the  2d  power  of  45  1  Ans.  2025. 

2.  What  is  the  square  of  4*16  ?  Ans.  17*8056. 

3.  What  is  the  3d  power  of  3-5  ?  Ans.  42-575, 

4.  What  is  the  5th  power  of  -029  ?  Ans.  -00000002051 1149. 

5.  What  is  the  square  of  f  ?  Ans.  f . 

6.  What  is  the  3d  power  of  f  ?  Ans. 

7.  What  is  the  4th  power  of  }  ?  Ans.  ,VV- 


EVOLUTION. 


Evolution,  or  the  reverse  of  Involution,  is  the  extracting 
or  finding  the  roots  of  any  given  powers. 

The  root  of  any  number,  or  power,  is  such  a  number,  as 
being  multiplied  into  itself  a  certain  number  of  times,  will 
produce  that  power.  Thus,  2  is  the  square  root,  or  2d  root 
of  4,  because  2a  =  2  x  2  ==  4  ;  and  3  is  the  cube  root  or  3d 
root  of  27,  because  33  ==  3  X  3  X  3  =  27. 

Any  power  of  a  given  number  or  root  may  be  found  ex- 
actly, namely,  by  multiplying  the  number  continually  into 
itself.  But  there  are  many  numbers  of  which  a  proposed 
root  can  never  be  exactly  found.  Yet,  by  means  of  deci- 
mals, we  may  approximate  or  approach  towards  the  root,  to 
any  degree  of  exactness. 

Those  roots  which  only  approximate,  are  called  Surd 
Roots  ;  but  those  which  can  be  found  quite  exact,  are  called 
Rational  Roots.  Thus,  the  square  root  of  3  is  a  surd  root  ; 
but  the  square  root  of  4  is  a  rational  root,  being  equal  to  2  : 
also  the  cube  root  of  8  is  rational,  being  equal  to  2  ;  but  the 
cube  root  of  9  is  surd  or  irrational. 

Roots'  are  sometimes  denoted  by  writing  the  character  •/ 
before  the  power,  with  the  index  of  the  root  against  it. 
Thus,  the  3d  root  of  20  is  expressed  by  f/JJO ;  and  the  square 


SQUARE  ROOT. 


SI 


root  or  2d  root  of  it  is  ^/20,  the  index  2  being  always  omit- 
ted, when  only  the  square  root  is  designed. 

When  the  power  is  expressed  *»y  several  numbers,  with 
the  sign  +  or  —  beiwxeu  them,  a  line  is  drawn  from  the  top 
of  the  sign  over  all  the  parts  of  it :  thus  the  third  root  of 
-15  —  12  is  \/  45  —  12,  or  thus,  y(45— - 12),  inclosing  the 
numbers  in  parentheses. 

But  all  roots  arc  now  often  designed  like  powers,  with 

i 

fractional  indices  ;  thus,  the  square  root  of  8  is  83,  the  cube 
root  of  25  is  25»,  and  the  1th  root  of  4i>  — 18  is  (45  -  18)*. 

TO  EXTRACT  THE  SQUARE  ROOT. 

*  Divide  the  given  number  into  period"  of  two  figures 
each,  by  setting  a  point  over  the  place  of  units,  another  over 
the  place  of  hundreds,  a.id  so  on,  over  every  second  figure, 
both  to  the  left-hand  in  integers,  and  to  the  right  in  deci- 
mals. 


*  The  reason  for  separating  the  figures  of  the  dividend  into  periods 
or  portions  of  two  places  each,  U,  that  the  square  of  any  single  figure 
never  consists  of  more  than  two  places;  t tic  square  of  a  number  of  two 
figures,  <if  nmi  more  than  four  places,  and  so  on.  So  that  there  will  he 
as  many  figures  in  the  root  us  the  given  number  contains  periods  so  di- 
vided or  parted  off. 

And  the  reason  of  the  several  steps  hi  the  operation  appears  from  the 
ilgchraic  form  of  the  -quare  of  any  number  of  terms,  whether  two  or 
three  or  more.  Thus 

(«-  h)2  .  a-*  -•-  2ntt-\-  fta  _-  aa  \-(%la  f  ft)  ft,  the  square  of  two  terms  ; 
wuerc  it  appears  that  a  i*  the  first  term  of  the  root,  and  ft  the  second 
term  ;  al«*o  a  the  first  divisor,  and  'lie  new  divisor  i«  2a  j-ft,  or  double 
the  first  term  i». creased  by  the  second.  And  hence  the  manner  of  ex- 
traction is  thus : 

h:  divisor  a)  »*2  -f  Sift  -|-  ft  (a  j-  ft  the  root. 

?.a  di-;$or°.a-j-ft  .^aft-j-fts 
ft  I     ft  :-fta 


Again,  for  a  root  of  three  P'.Im,     ft.  rf  thus. 

(a  \-b-\-c)i  -■•|3"-2rtft     bi  -'r%ar-\-%bc  j  /8 

a-  -i  (m2a  ;  h)h  ■:  (2/*'  r  *2ft  j  r)c,  the 
square  of  three  terms,  where  a  is  too  fuM  term  of  the  root,  ft  the  «»rond, 
and  c  the  third  term  ;  also  a  the  fu?t  divisor,  2.i-r  ft  the  second,  and  &r 
-|  'lb  --c  the  third,  each  consi.-ting  of  the  double  of  the  root  increased 
by  thu  next  term  of 'lie  -»»m. .  And  the  mode  of  extr.ictifui  agrees  with 
iiilu.    r?«.e  far'.iier,  Case  2.  of  Kvolution  ii.  ire.  Algebra. 

 hi'  -■;  "»h       ,  . 

I* or  an  approximation  observe  that  Vul±     v  -  a.  -—   ---nearly  in 

All  cases  where  <i  it  small  in  respect  of  a. 
Vol.  J.  l'J 


82 


Find  the  greatest  square  in  the  first  period  en  the  left-hand, 
and  set  its  root  on  the  right-hand  of  the  given  number,  after 
the  manner  of  a  quotient  figure  in  Division. 

Subtract  the  square  thus  found  from  the  said  period,  and 
to  the  remainder  annex  the  two  figures  of  the  next  following 
period,  for  a  dividend. 

Double  the  root  above  mentioned  for  a  divisor ;  and  find 
how  often  it  is  contained  in  the  said  dividend,  exclusive  of  its 
right-hand  figure ;  and  set  that  quotient  figure  both  in  the 
quotient  and  divisor. 

Multiply  the  whole  augmented  divisor  by  this  last  quotient 
figure,  and  subtract  the  product  from  the  said  dividend,  bring- 
ing down  to  it  the  next  period  of  the  given  number,  for  a  new 
dividend. 

Repeat  the  same  process  over  again,  viz.  find  another  new 
divisor,  by  doubling;  all  the  figures  now  found  in  the  root ; 
from  which,  and  the  last  dividend,  find  the  next  figure  of 
the  root  as  before  ;  and  so  on  through  all  the  periods,  to  the 
last. 

iVbfe,  The  best  way  of  doubling  the  root,  to  form  the  new 
divisors,  is  by  adding  the  last  figure  always  to  the  last  divi- 
sor, as  appears  in  the  following  examples. — Also,  after  the 
figures  belonging  to  the  given  number  are  all  exhausted,  the 
operation  may  be  continued  into  decimals  at  pleasure,  by  add- 
ing any  number  of  periods  of  ciphers,  two  in  each  period. 

EXAMPLES. 

1.  To  find  the  square  root  of  20506624. 

20506624  (5432  the  root. 
25 


104 

450 

4 

416 

1083 

3466 

3 

3249 

10862  21724 
2  21724 


SQUABR  ROOT*  W 

Nero,  When  the  ml  it  to  he  extracted  to  many  places  of 
figures,  the  work  may  he  considerably  shortened,  thus  y 

.  Having  proceeded  in  the  extractioa  after  the  common 
method,  till  there  be  found  half  the  required  number  of 
figures  in  the  root,  or  one  figure  more ;  then,  for  the  retf, 
divide  the  last  remainder  by  its  corresponding  divisor,  after 
the  manner  of  the  third  contraction  in  Division  of  Deci- 
mals; thus, 

2.  To  find  the  root  of  2  to  nine  places  of  figures. 
2  (1-41421356  the  root. 
1 


24 
4 


100 


281  | 
1  I 


400 

281 


2824 
4 


11900 
11206 


60400 
56564 


3.  What 

4.  What 

5.  What 

6.  What 

7.  What 

8.  What 
0.  What 

10.  What 

11.  What 

12.  What 


28284) 


is  the  square 
is  the  square 
is  the  square 
is  the  square 
is  the  square 
is  the  square 
is  the  square 
is  the  square 
is  the  square 
is  the  square 


31936  (1356 
1008 
160 
19 
2 

root  of  2025? 
root  of  17-3056? 
root  of  -000729? 
root  of  3? 
root  of  5? 
root  of  6  ? 
root  of  7  ? 
root  of  10? 
root  of  11? 
root  of  12? 


Ads.  45« 
Ads.  416. 
Ans.  -027. 

Ans.  1-732050. 

Ans.  2*236068. 

Ans.  2*449489. 

Ans.  2-645751. 

Ans.  3-162277. 

Ads.  3-316624. 

Ans.  3-464101. 


RULES  FOR  THE  SQUARE  ROOTS  OF  VULGAR  FRACTIONS  AND 
MIXED  NUMBERS. 


First  prepare  all  vulgar  fractions,  by  reducing  \Y&m  to 
their  least  terms,  both  for  this  and  all  other  roots.  Then 


84  ARITHMETIC* 

1.  Take  the  root  of  the  numerator  and  of  the  denominator 
for  the  respective  terms  of  the  root  required ;  which  is  the 
best  way  if  the  denominator  be  a  complete  power  :  but  if  it 
be  not,  then 

2.  Multiply  the  numerator  and  denominator  together  ; 
take  the  root  of  the  product :  this  root  being  made  the  nu. 
merator  to  the  denominator  of  the  given  fraction,  or  made 
the  denominator  to  the  numerator  of  it,  will  form  the  frac- 
tional root  required. 

That  is,  ^  «      ^  =  /flft  ---L- 


b  ~~  x/b  "~   b     ~~  i/ab 

This  rule  will  serve,  whether  the  root  be  finite  or  infinite. 

3.  Or  reduce  the  vulgar  fraction  to  a  decimal,  and  extract 
its  root. 

4.  Mixed  numbers  may  be  either  reduced  to  improper 
fractions,  and  extracted  by  the  first  or  second  rule,  or  the 
vulgar  fraction  may  be  reduced  to  a  decimal,  then  joined  to 
the  integer,  and  the  root  of  the  whole  extracted. 


EXAMPLES. 


1.  What  is  the  root  of  |§? 

2.  What  is  the  root  of  TyT  ? 

3.  What  is  the  root  of  7\  ? 

4.  What  is  the  root  of  ? 

5.  What  is  the  root  of  17}  ? 


Ans.  | 
Ans.  if. 
Ans.  0-866025. 
Ans.  0-645497 
Ans.  4-16S3&3. 


By  means  of  the  square  root  also  may  readily  be  found  the 
4th  root,  or  the  8th  root,  or  the  16th  root,  <fcc.  that  is,  the 
root  of  any  power  whose  index  is  some  power  of  the  number 
2 ;  namely,  by  extruding  so  oleen  the  square  root  as  is  de- 
noted by  that  power  of  2  ;  that  is;  two  extractions  for  the  4th 
root,  three  for  the  8th  root,  and  so  on. 

So,  to  find  the  4th  root  of  the  number  21035*8,  extract  the 
square  root  two  times  as  follows  : 


CUBE  BOOT* 


85 


21035-8000  (  145  037237  (  12  0431407  the  4th  root. 
1  1 


24 
4 


110 
06 


45 
44 


285 
5 


1435 
1425 


2404 
4 


10372 
0610 


29003 


108000  24083 
87009  3 


20991  (7237 
6*7 
107 


75637 
72249 

3388  ( 1407 
980 
17 


Ex.  2.  What  is  the  4th  root  of  97-41  ? 


TO  EXTRACT  THB  CUBE  ROOT. 


I.  By  tint  Common  Rule*. 

1.  Having  divided  the  given  number  into  periods  of  three 
figures  each  (by  setting  a  point  over  the  place  of  units,  and 
also  over  every  third  figure,  from  thence,  to  the  left  hand  in 
whole  numbers,  and  to  the  right  in  decimals),  find  the  nearest 
less  cube  to  the  first  period  ;  set  its  root  in  the  quotient,  and 
subtract  the  said  cube  from  the  first  period  ;  to  the  remainder 
bring  down  the  second  period,  and  cull  this  the  resolvend. 

2.  To  three  times  the  square  of  the  root,  just  found,  add 
three  times  the  root  itself,  setting  this  one  place  more  to  the 
right  than  the  former,  and  call  this  sum  the  divisor.  Then 
divide  the  resolvend,  wanting  the  last  figure,  by  the  divisor, 
for  the  next  figure  of  the  root,  which  annex  to  the  former  ; 


*  The  reason  for  pointing  the  given  number  into  periods  of  three  fi- 
gures each,  is  because  the  cube  of  one  figure  never  amounts  to  more 
than  three  places.  And,  for  a  similar  reason,  a  given  number  is  point- 
ed into  periods  of  four  figures  for  the  4th  root,  of  five  figures  for  the  5th 
root,  and  so  on. 

The  reason  for  the  other  parts  of  the  rule  depends  on  the  algebraic 
formation  of  a  cube  :  for,  if  the  root  consist  of  the  two  parts  a  r  I 
then  its  cube  is  as  follows:  («-{-fc)3  -  aa  -j-  3a  6-f-  3a6«  -f  b*  ;  where 
a  \n  the  root  of  the  first  part  a3  ;  the  resolvend  is  3a»6-f  3a^2  -f  63  ; 
which  is  also  the  same  as  the  three  parts  of  the  subtrahend  ;  also  the 
divisor  is  3a  -7- 3a,  by  which  dividing  the  first  two  terms  of  the  resolv- 
end 3aa  6 + ab* ,  gives  b  for  the  second  part  of  the  rool  \  and  w>  on. 


86  ARITHMETIC. 

calling  this  last  figure  e,  and  the  part  of  the  root  before  found 
let  be  called  a. 

3.  Add  all  together  these  three  products,  namely,  thrice  a 
square  multiplied  by  c,  thrice  a  multiplied  by  e  square,  and 
e  cube,  setting  each  of  them  one  place  more  to  the  right  than 
the  former,  and  call  the  sum  the  subtrahend ;  which  must 
not  exceed  the  resolvend  ;  but  if  it  does,  then  make  the  last 
figure  e  less,  and  repeat  the  operation  for  finding  the  subtra- 
hend, till  it  be  less  than  the  resolvend. 

4.  From  the  resolvend  take  the  subtrahend,  and  to  the 
remainder  join  the  next  period  of  the  given  number  for  a  new 
resolvend ;  to  which  form  a  new  divisor  from  the  whole  root 
now  found  ;  and  from  thence  another  figure  of  the  root,  as 
directed  in  article  2,  and  so  on. 


EXAMPLE* 


To  extract  the  cube  root  of  48228*544. 


3  X  3»  =  27 
3  X  3  =  09 

Divisor  279 


48228-544  (  36-4  root. 
27 


21228  resolvend. 


3  X  3*  X  6  =162 
3X3   X6>=  324  )  add 
6»  =    216  f 


3  x  36J  =; 
3  X  36  =  108 


38988 


19656  subtrahend. 


1572544  resolvend. 


3  X  36»  X  4  =  15552  ) 
3  X  36  X  4*  =      1728  >  add 


43  =  64  J 


1572544  subtrahend. 


0000000  remainder. 


Ex.  2.  Extract  the  cube  root  of  571482-19. 
Ex.  3.  Extract  the  cube  root  of  1628-1582. 
Ex.  4.  Extract  the  cube  root  of  1332. 


CUBE  SOOT. 


87 


II.  Ib  extract  the  Cube  Root  by  a  short  Way*. 

1.  By  trials,  or  by  the  table  of  roots  at  p.  93,  dec.  take 
the  nearest  rational  cube  to  the  given  number,  whether  it  be 
greater  or  less  ;  and  call  it  the  assumed  cube. 

2.  Then  say,  by  the  Rule  of  Three,  As  the  sum  of  the 
given  number,  and  double  the  assumed  cube,  is  to  the  sum  of 
the  assumed  cube  and  double  the  given  number,  so  is  the 
root  of  the  assumed  cube,  to  the  root  required,  nearly.  Or, 
As  the  first  sum  is  to  the  difference  of  the  given  and  assumed 
cube,  so  is  the  assumed  root  to  the  difference  of  the  roots 
nearly. 

3.  Again,  by  using,  in  like  manner,  the  cuhe  root  of  the 
last  found  as  a  new  assumed  cube,  another  root  will  be  ob- 
tained still  nearer.  And  so  on  as  far  as  we  please  ;  using 
always  the  cube  of  the  last  found  root,  for  the  assumed 
cube. 

EXAMPLE. 

To  find  the  cube  root  of  21034-8. 

Here  we  soon  find  that  the  root  lies  between  20  and  30, 
and  then  between  27  and  28.  Taking  therefore  27,  its  cube 
is  19683,  which  is  the  assumed  cube.  Then 

19683  21035-8 
2  2 


39366  42071-6 
21035-8  19083 


As  60401-8    :     61754-6  :  :  27  :  27-6047. 
27 


4322822 
1235092 


60401-8)  1667374-2  (27-6047  the  root  nearly, 
459338 
36525 
284 
42 


*  The  method  usually  given  for  extracting  the  cube  root,  Vi  so  ev 
ceedingly  tedious,  and  difficult  to  be  remembered,  that  \w\ov\*  oXtat 


88  ARITHMETIC. 

Again,  for  a  second  operation,  the  cube  of  this  root  is 
21035-318645155823,  and  the  process  by  the*  latter  method 
will  be  thus  : 

21035-118645  &c. 


42070-637290  21035-8 
,21035-8  21035-318645  &c. 


As  63106-43729     :     difT.  -481355  :  :  27-6017  : 

thediff.  -0002^  0560. 


conseq.  the  root  req.  is  27-604910560. 

Ex.  2.  To  extract  the  cube  root  of  -67. 
Ex.  3.  To  extract  the  cube  root  of  -01. 


TO  EXTRACT  ANY  ROOT  WJIATKVER  • 

Let  p  be  the  given  power  or  number,  ?*  the  index  of  the 
power,  a  the  assumed  power,  r  its  root,  r  the  required  root 
of  p.    Then  say, 

As  the  sum  of  n  +  1  times  a  and  n  —  1  times  p, 
is  to  the  sum  of  n  +  1  times  p  and  n  —  1  times  a  ; 
so  is  the  assumed  root  r,  to  the  required  root  r, 

Or,  as  half  the  said  sum  of  n  +  1  times  a  and  n  —  1  times 
r,  is  to  the  difference  between  the  given  and  assumed  powers, 


approximating  rules  have  been  invented,  viz.  by  Newton,  Rnphson, 
Halley,  De  Lagny,  Simpson,  Emerson,  and  several  other  mathemati- 
cians ;  but  no  one  that  I  have  yet  seen  is  so  simple  in  it  form,  or  seems 
so  well  adapted  for  general  use,  as  that  above  given.  This  rule  is  the 
same  in  effect  as  Dr.  Halley's  rational  formula,  but  more  commodious- 
ly  expressed  ;  and  the  first  investigation  of  it  was  given  in  my  Tracts, 
p.  49.   The  algebraic  form  of  it  is  this: 

As  p  j  -  2a  :  a  -|-  2r  :  :  r  :  jr.  Or, 
A*  p  -(-  2a  :  p  *r   a  :  :  r  :  k  *r  r ; 

where  p  is  the  given  number,  a  is  the  assumed  nearest  cube,  r  the  cube 
root  of  a,  and  n  the  root  of  p  sought. 

*  This  is  a  very  general  approximating  rule,  of  which  that  for  the 
cube  root  is  a  particular  ca*e,  and  is  the  best  adapted  for  practice,  and 
for  memory,  of  any  that  I  have  yet  seen.  It  was  first  discovered  in  this 
form  by  myself,  and  the  investigation  and  use  of  it  were  given  at  large 
in  my  Tracts,  p.  45,  &c 


GENERAL  ROOTS. 


80 


so  is  tlss^sjhjuMd  root  r,  to  the  difference  between  the  true 
end  iMMn  roots  ;  which  difference,  added  or  subtracted, 
ee  the  case  requires,  gives  the  true  root  nearly. 
That ie, (n  4-1)  a  +  (n-l)r:  (w+1)  p.  H-(n-l)  a:  :r:a- 
Or,  (n  +  1)  Aa  +  (n — 1)      :  p^a  : :  r  :  it  ^  r. 

And  the  operation  may  be  repeated  as  often  as  we  please, 
by  using  always  the  lust  found  root  for  the  assumed  root,  and 
its  nth  power  for  the  assumed  power  a. 


example. 
To  extract  the  5th  root  of  21035& 

Here  it  appears  that  the  5th  root  is  between  7  3  and  7*4* 
Taking  7-3,  its  5th  power  is  20730  71503.  Hence  we  have 
r  «  21035-8,  n  =  5,  r  =  7-3,  and  a  =  20730-71593  ;  then 
»  +  1  .  £a  -f-  n  —  1  .  £p  :  p  ^  a  :  :  r  :  r  «^  r,  that  is, 
8  X20730-71593  +  2  x  21053-8  :  305-0*4  : :  7  3  :  -0213005 
3  2  7-3 


62192  14779 
42071-6 

104263  74779 


42071 -(J  915252 
2135568 


2227  1 13 1(  -0213605=11^ 
7  3=r,  add 


7  321360- r,  true 
to  the  last  figure. 


OTHER  EXAMPLES. 


1.  What  is  tho  3d  root  of  2  ?  Ans.  1-259921. 

2.  What  is  tho  3d  root  of  3214  ?  Ans.  14-75758. 
8.  What  is  the  4th  root  of  2  ?  Ans.  1  189207. 

1  4.  Whnt  is  the  4th  root  of  97-41  ?  Ans.  3  1415909. 

5.  Whnt  is  the  5th  root  of  2  ?  Ans.  1-148699. 

6.  What  is  the  6th  mot  of  21035-8  ?  Ans.  5-254037. 

7.  What  is  the  6th  root  of  2  ?  Ans.  1-122462. 

8.  What  is  tho  7th  root  of  21035-8  ?  Ans.  4-145392. 
0.  What  is  the  7th  root  of  2  ?  Ans.  1-104080. 

10.  What  is  the  8ih  root  of  21035-8  ?  Ans.  3-470328. 
Vol.  I.  13 


00  AStTHWCTIC. 

1 1.  What  is  the  8th  root  of  2  ?  •  •  An.  l^HK 

12.  What  is  the  9th  root  of  21035*8 1  Ana.  S^tHS9. 

13.  What  is  the  9th  root  of  2  ?  Ans.  1-080059. 


The  following  is  a  Table  of  squares  and  cubes,  and  also  the 
square  roots  and  cube  roots,  of  all  numbers  from  1  to  1000, 
which  will  be  found  very  useful  on  many  occasions,  in  nu- 
meral calculations,  when  roots  or  powers  are  concerned. 

The  use  of  this  table  may  be  greatly  extended,  either  by 
the  addition  of  ciphers,  or  by  changing  the  places  of  the 
separating  points.  The  following  examples  will  suffice  to 
suggest  the  method. 

Root.  Square.  Cube. 

36-  12<J6*  46656- 

360-  129600-  46656000- 

3600-  12960000-  46656600000- 

546-  298116-  162771336- 

54-6  2981-16  162771-330 

'546  -298116  -162771336 

For  a  simple  and  ingenious  method  of  constructing  tables 
of  square  and  cube  roots,  and  the  reciprocals  of  numbers, 
see  Dr.  Hutton's  Tracts  on  Matheirtotical  and  Philosophical 
Subjects,  vol,  i.  Tract  24,  pa.  459. 


A  TABU  OF  4QUAAU,  CUBES,  AND  ROOTS. 


91 


square. 

Square  ttooi. 

ouce  ttoot* 

1 

"  1 

1 

1  0000000 

1  000000 

i 

4 

8 

14142136 

1  259921 

9 

27 

1-7320508 

1-442250 

4 

16 

64 

2 0000000 

1-587401 

5 

25 

125 

2  2360680 

1  709976 

6 

36 

216 

24494397 

1  817121 

7 

49 

343 

2  6457513 

1-912931 

8 

64 

512 

28284271 

2  000000 

9 

81 

729 

30000000 

2  080084 

10 

100 

1000 

3 1622777 

2 154435 

11 

121 

1331 

33166248 

2  223990 

12 

144 

1728 

3  4641016 

2289428 

13 

169 

2197 

3  6055513 

2  351335 

14 

196 

2744 

37416574 

2410142 

15 

225 

3375 

38729833 

2  466212 

16 

256 

4096 

40000000 

2519842 

17 

289 

4913 

4  1231056 

2 571282 

IS 

324 

5832 

4  2426407 

2  620741 

10 

861 

6359 

4  35SS9S9 

2  668402 

30 

400 

SO  00 

4  4721360 

2714418 

21 

44  1 

9261 

4  5825757 

2  758924 

22 

434 

10643 

4  6904158 

2  802039 

23 

529 

12107 

4 795S315 

2-S43867 

24 

576 

13S24 

4  8989795 

2  884499 

25 

625 

15625 

50000000 

2 924018 

SO 

676 

17576 

5  0990195 

29G2496 

27 

729 

19683 

5 1961524 

3  000000 

28 

7S4 

21952 

5  2915026 

3036589 

29 

841 

24389 

5  385164S 

307231 7 

30 

900 

27000 

54772256 

3 107232 

31 

9G1 

29791 

5  5677644 

3  141381 

39 

1024 

32768 

5656S542 

3 174802 

33 

1089 

35937 

5  7445626 

3207534 

»  j'l 

1 1  'iJi 

1  1<JD 

35 

1225 

42875 

59160798 

3271066 

36 

12D6 

46656 

60000000 

3  301927 

37 

1369 

50653 

60827G25 

3-332222 

38 

1444 

54S72 

6  16  14140 

3  361975 

39 

1521 

59319 

62449980 

3  391211 

40 

1600 

61000 

6-3245553 

3  419952 

41 

1681 

69921 

64031242 

3  448217 

42 

1764 

7408* 

6-4807407 

3476027 

43 

1849 

79507 

6  5574385 

3 503398 

44 

i<m 

85184 

6  0332496 

3  530348 

45 

2025 

91125 

670S2039 

3  556893 

46 

2116 

97336 

0-7823300 

3  583043 

47 

2209 

103823 

68556546 

3603826 

48 

2304 

110592  , 

6  9282032 

M02 

117649 

70000000 

^  si 

2500  / 

125000 

70710678 

\  3 

AJUIBMETtC. 


Number. 

Square. 

Cube. 

Square  EooL 

 ,  

Cube  Root. 

51 

260] 

132651 

7 1414284 

3-708430 

52 

2704 

1-1  CO  US 

72111026 

3  732511 

53 

2300 

14S877 

7-2801099 

3756286 

54 

2916 

157464 

73484692 

3779763 

55 

3025 

16.G375 

7  4161985 

3802953 

56 

3136 

i  175616 

74833148 

3  825862 

57 

3249 

185193 

75498344 

3  848501 

58 

3364 

195)12 

7  6157731 

3870877 

50 

34*1 

205379 

7  681)457 

3  892996 

60 

3600 

216C0D 

77459667 

3  914863 

61 

3721 

226981 

78102497 

3936497 

62 

3844 

238328 

76740079 

3-957883 

63 

3969 

250047 

7*9372539 

3979057 

64 

4096 

262144 

800C00OO 

4 000000 

w 

4225' 

274625 

80622577 

4  020726 

60 

4356 

287496 

S12403S4 

4041240 

67 

4489 

300763 

8  1 85352S 

4061548 

6S 

4624 

314432 

8  2462113 

4-081655 

69 

4761 

3285G9 

83066239 

4101566 

70' 

4900 

343000 

83666003 

4  121285 

71 

son 

357911 

842G149S 

4  140818 

72 

5184 

373248 

8-4852814 

4 160153 

73 

5329 

399017 

8*5440037 

4 179339 

74 

5476 

405224 

86023253 

4 198336 

75 

5625 

421875 

86602540 

4217163 

76 

5776 

438976 

87177979 

4  235824 

77 

5929 

456533 

S  7749644 

4  25432J 

78 

6084 

474552 

SS317609 

4 272659 

79 

6241 

493039 

8  8881944 

4290841 

80 

6400 

512000 

S 9442719 

4  308870 

61 

6561 

531441 

90000000 

4  326749 

82 

6724 

551368 

90553S51 

4  344431 

83 

0889 

571787 

&  11 04336 

4  362071 

84 

7C56 

51)2704 

Ai  1  PSl  £  1  4 

4*379519 

65 

7225 

614125 

92195445 

4396830 

86 

7396 

636056 

0  2736185 

4414005 

87 

7569 

658503 

9  3273791 

4431047 

88 

7744 

6S1472 

936CS315 

4447960 

89 

7921 

704969 

9  4339811 

4464745 

90 

8100 

720000 

9486S:^30 

4481405 

91 

£281 

753571 

95393920 

4-497941 

92 

64JG4 

77S6SS 

9  5916630 

4-514357 

93 

S649 

S04357 

9-6436508 

4530655 

94 

8836 

8305S4 

96953597 

4  546836 

95 

9025 

857375 

97467943 

4  562903 

96 

9216 

884736 

9*7979590 

4 578857 

97 

9409 

912673 

98488578 

4-594701 

98 

9604 

941192 

9S994949 

4-610436 

99  / 

9S01 

970299 

L  9949S744 

.  4626065 

100  1 

10000 

10000GO 

\  10  moggou 

•WAftlS,  CUUS,  AlfD  BOOTf .  93 


Number. 

Square. 

Cube. 

Square  Root. 

Cube  Root. 

101 

10201 

1030301 

10' 04  98756 

4657010 

102 

10404 

106120S 

100995049 

4  672329 

103 

lCGGO 

1092727 

10  1488916 

4  687548 

104" 

10813 

1124>G4 

1  />    i  AC)  Art 

10' 1930390 

4  702t)b9 

105 

1 1 02 

1157625 

1  J"l        J  Aft  t  J  lO 

10  2469508 

4-717694 

100 

I12CG 

11010IG 

10  23o6301 

4*732624 

107 

11449 

1225043 

JO  3  I40J50* 

4  747459 

loa 

11064 

1250712 

10  3923048 

4762203 

109 

11  SSI 

1295029 

104403065 

4  77685b 

110 

12100 

1331000 

10  4880885 

4  791420 

111 

12321 

1367631 

10  5356536 

4  HO 5896 

112 

12544 

1404928 

105830052 

j  .a tin ao  * 

4 82 0284 

113 

12700 

1442S97 

10  6301459 

A  Q'li  CQQ 

4  Wo45S9 

114 

12996 

1481544 

10  67707S3 

4o4SS0S 

115 

13225 

1520875 

10  7239053 

4  00^944 

116 

13456 

1560896 

1  A^mv  aaa  nit 

1 07 703 2 06 

J    V  ""t"  ■  1  1  1  f  1 

117 

13698 

1601613 

10  8166538 

4  3905173 

11S 

13924 

1643032 

10  8627805 

4  yu4obo 

119 

14161 

1685159 

10'90S7121 

j,ni  bjjqe 

4  y 1 ooSo 

120 

14400 

1728000 

109544512 

121 

14641 

1771561 

i  rooooooo 

4  946088 

122 

149S4 

181584S 
186CS67 

11  0453610 

4  959676 

123  ; 

15120 

I  1  .Anne  'ic  r 

I I  0905365 

j   A^At  AA 

4  973 19U 
4  98663 1 

124 

15376 

1  A  A**  Cm 

1906624 

11     1  r\r  rnriH 

11  1355287 

15625 

1953125 

T  1  .  i  cm  a  a  a  a 

1 1  1803399 

o  uuuuuu 

126 

15&7G 

2000376 

1  I  2249722 

o  U  ]  a/Ho 

127 

16129 

2048383 

1 1  2694277 

t     o  OZOfr^b 

129 

16331 

2007152 

11  '3137085 

0  U3Ubb4 

129 

16641 

2146689 

I  IOC  TO  i  c  T 

I I  3o7SI67 

o 05^774 

139 

16900 

2107000 

11  4017543 

0  065797 

131 

17161 

2248091 

11     j  j  *~  ^  A  A  1 

11*4455231 

5  078753 

132 

17424 

2299908 

1 1  4891253 

c  a  a  l  i*  m  a 

5  091643 

133 

17639 

2352637 

1  lo325626 

5 104469 

134 

17956 

2406104 

11-5758369 

5 117230 

135 

18225 

2460375 

11'6189500 

5  129928 

136 

18496 

251545G 

11-6619038 

5  142563 

137 

18760 

2571353 

11  7046999 

5 155137 

138 

19044 

2628072 

11  7473444 

5  167649 

130 

19321 

2685610 

11*7898261 

5 1S0101 

140 

19600 

2744000 

11  8321596 

5 192494 

111 

198S1 

2803221 

U  8743421 

5  204828 

142 

20164 

2863283  , 

11  9163753 

5217103 

143 

20440 

2924207  i 

11  9582607 

5  220321 

144 

20736 

23859S4 

12  0000000 

5241483 

145 

21025 

3048625 

V2  0415946 

5  253583 

146 

21316 

3112136 

120830460 

5  265637 

147 

21609 

3176523 

12  1243557 

5277632 

148 

21904 

3241792 

12  1655251 

5-2S<ft&n 

149 

22201 

3307949 

122065556 

150  J 

22500  j 

3375000  j 

12-24744S7 

^»  1  rTYiltar 

Jl  ^  LI  114  Ucl  . 

Souafe 

Cube, 

Snuare  Root 

CuhA  Rrmt 

VUMC  HWl. 

151 

22801 

3442951 

12  2882037 

5325074 

15^ 

23104 

35 11808 

12-3288280 

5336303 

153 

23409 

3581577 

12  3693169 

5  348481 

154 

23716 

3652264 

124006736 

5-360108  l 

155 

24025 

3723875 

12449S996 

5  371685 

156 

24336 

3796416 

12  4899960 

5383213 

157 

24649 

3809S93 

12  5299641 

5  394691 

158 

24964 

3944312 

125693051 

5406120 

159 

25281 

4019679 

12  6095202 

5  417501 

160 

25600 

4096000 

126491106 

5428835 

Ml 

26921 

4173281 

126885776 

5440122 

16a 

26244 

425152S 

12  7279221 

5  451362 

163 

26569 

4330747 

127671453 

5462556 

164 

26896 

4410944 

12  8062485 

5473704 

165 

27225 

4492125 

128452326 

5494806 

166 

27566 

4574296 

12  8840987 

5495865 

167 

27SS9 

46*7463 

12  922S480 

5506879 

168 

4741632 

129614814 

5517S4S 

169 

2S561 

4826309 

13  0000000 

552S775 

170 

28900 

4913300 

13  0384048 

5  539658 

171 

29241 

5000211 

130766968 

5550499 

172 

29584 

5088448 

13  1148770 

5  561298 

173 

29929 

5177717 

13  1529464 

5572055 

174 

30276 

5268024 

13  1909060 

5-592770 

175 

30625 

6359375 

132287566, 

5  593445 

176 

30976 

5451776 

13  2664992 

5604079 

177 

31329 

5545233 

133041347 

5  614673 

178 

31684 

5639752 

13  3416641 

5625226 

179 

32041 

6735339 

13-3790882 

5  635741 

180 

32*00 

5932000 

13  4164079 

5  646216 

181 

,32761 

5929741 

134536240 

5656653 

182 

33124 

6028568 

134907376 

5667051 

183 

33439 

6128487 

13  5277493 

5  677411 

194 

0^29,0  04 

Jo  Ot>4bbUU 

5 687734 

185 

34225 

6331625 

13  6014705 

5699019 

186 

34596 

6434856 

136381817 

5  708267 

187 

34969 

6539203 

136747943 

5718479 

188 

35344 

6644672 

13  7113092 

5  729654 

189 

35721 

6751269 

13  7477271 

5738794 

190 

3G100 

6959000 

137840488 

5749S07 

191 

36481 

6967871 

138202750 

5758965 

192 

36864 

70778S8 

13  8564065 

5768998 

193 

37249 

7189057 

13  8924440 

5  778996 

194 

37636 

7301384 

139283883 

5  789960 

195 

38025 

7414875 

139642400 

5  798890 

196 

38416 

7529536 

1400000(10 

5S08786 

197 

3S809 

7645373 

140356688 

5  818648 

198  | 

39204 

7762302 

140712473 

5828476 

199  * 

39601 

7880599 

\  vmm 

2W  / 

40000  j 

8000000 

■40AAIS,  CUBES,  AND  ROOT*. 


/Number. 


201 
202 
203 
204 
205 
206 
207 
208 
209 
210 
211 
212 
213 
214 
215 
216 
217 
218 
219 
220 
221 
222 
223 
224 
225 
226 
227 
228 
229 
230 
231 
232 
233 
234 
235 
236 
237 
238 
239 
240 
241 
242 
243 
244 
245 
246 
247 
248 
349 


Square. 


/ 


40401 
40804 
41209 
41616 
42025 
42436 
42849 
43264 
43661 
44100 
44521 
44944 
45369 
45796 
46225 
46656 
47089 
47524 
47961 
48400 
48841 
49264 
49729 
50176 
50625 
51076 
51529 
51984 
52441 
52900 
53361 
53S24 
54289 
54756 
55225 
55696 
56169 
56644 
57121 
57600 
58061 
58564 
59049 
59536 
60025 
60516 
61009 
61504 
62001 
62500 


Cube. 


8120601 
8242408 
8365427 
8489664 
8615125 
8741816 
8869743 
8998912 
9123329 
9261000 
9393931 
9528128 
9663597 
9800344 
9938375 
10077696 
10218313 
10360232 
10503459 
10648000 
10793861 
10941048 
11089567 
11239424 
11390625 
11543176 
11697063 
11852352 
12008989 
12167000 
12326391 
12487168 
12649337 
12S12904 
12977875 
13144256 
13312053 
13481272 
13651919 
13824000 
13997521 
1417248S 
14348907 
14526789 
14706125 
14886936 
15069223 
15252992 
15438249 
15625000  1 


Square  Root.    Cube  Rogt 


141774469 
142126704 
142478068 
142828569 
14  3178211 
143527001 
143874946 
144222051 
14  4568323 
144913767 
145258390 
14  5602198 
14  5945195 
146287388 
146628783 
146969385 
14  7309199 
147648231 
147986486 
14  8323970 
148660687 
148996644 

14  9331845 
149666295 

15  0000000 
15  0332964 
150665192 
15  0996689 
15  1327460 
15- 1657509 
15  1986842 
152315462 
15  2643375 
15-2970585 
153297097 
15-3622915 
15-3948043 
15  4272486 
15  4596248 
15-4919334 
15-5241747 
155563492 
15  5884573 
156204994 
156524758 
156843871 
157162336 
157480157 
157797338 
15-3113883 


5857766 
5  867464 
5877130 
5  886765 
5896368 
5  905941 
5915482 
5924992 
5  934473 
5  943922 
5953342 
5962731 
5972091 

5  981426 
5990727 
6000000 
6009244 
6018463 
6027650 

6  036811 
6045943 
6055048 
6064126 
6073178 
6082201 
6  091199 
6 100170 
6 109115 
6 118033 
.6  126925 
6 135792 
6 144634 
6 153449 
6 162239 
6 171005 
6 179747 
6- 188463 
6 197154 
6205822 
6  214465 
6223084 
6231679 
6240251 
6248800 
6257325 
6265826 


M 


Number. 

Square, 

Cube. 

Square  Root.  1 

Cube  Root. 

251 

■  1 

63001 

15813251 

15  rS429 795  1 

b  o07994 

252 

63504 

16003G08 

15  8745079 

6'31 6359 

253 

64009 

1     C-1"    1     t\    J   a  1  -*t*f 

16134277 

1 5' 059737 

0  024704 

254 

64516 

1     1  f  r>fi A a  j 

16387064 

15  9373775 

b  0  3 302 6 

net 

65025 

1  CCDl  'ITS 

lbo3 137o 

159b37194 

b  44  1*3  2  b 

256 

65536 

lb77721b 

lb  0000000 

b  <H9b04 

257 

06049 

loy7459o 

i  c . ao  1  a  1  a  el 
1  b  Oo 1 2) 9o 

b  o57ool 

2  DO 

66564 

1  C  AC  ill  1 2  4 

lb  Ug JJ734 

o  t5bouyo 

259 

67081 

17d*3y79 

lb  0934769 

b  i>74o  1 1 

260 

67600 

17576000 

lb  1245155 

0  332504 

261 

68121 

17779591 

16  1554944 

6  390676 

262 

68644 

17934729 

161964141 

6  39S829 

263 

69169 

1S191447 

16  2172747 

6  406959 

264 

69696 

18399744 

162480768 

6  415003 

265 

70225 

1360962:> 

16*2788206 

6  423153 

266 

70756 

18821096 

^      n  a  a  p  a  n  a 

163095064 

a  ,  t  a  t  n  ftn 

b  43122S 

267 

nr  1  nan 

71289 

19034163 

16  3401346 

G 4392  /  * 

268 

71824 

1  A  A  *.  O  a  !i  »i 

19249332 

16  p37070o5 

6  447305 

269 

72361 

19465109 

te  1 Ai      i rtr 

164012195 

6  455315 

OTA 

lybSJOOO 

164316767 

(  6  463304 

271 

73441 

iyyo25i i 

16  4620776 

6  4712i4 

272 

73 934 

20123643 

16  4924225 

6  479224 

273 

74529 

20046417 

16  52271 16 

6  4S7154 

274 

75076 

2O570S24 

lb  5529454 

6  495065 

275 

75625 

207 9 6,3 7o 

16-5831240 

6  5029^6 

J76 

76176 

21 024576 

lb'6 132477 

6  510^30 

277 

76729 

it,/;  IQ'JtTn 
iD'O-ldiJl  iKJ 

b  a 1 ob34 

275 

772a  4 

4I-io4yD2 

1  D  O  r  ooo20 

b  *>2b519 

279 

77341 

Ol Tl 7KQQ 

ID  / JJ 

b  Qd4iJo5 

230 

•    7Q  4  A  A 

7&4i>u 

41 4 J4UUU 

1  ifi  .    "i  " J  fl  A  A  tl 

1  (W*5d2O0O 

0 542133 

43  1 

99  1  QCtHi  1 

ID  f OoUO-^O 

i?  -  c  j*  A,A  1  n 

-  ~ 

70*194 

1  ,fi  7Q9Q^1A 

d  Do  4  b7dt 

283 

80089 

226J51S7 

168226038 

6  565415 

234 

80656 

22906304 

16-8522995 

6573139 

285 

81225 

23149125 

16  8819430 

6-580844 

286 

81796 

23393656 

16-9115345 

6588532 

287 

82369 

23639903 

16-9410743 

6-596202 

288 

82944 

23987872 

169705627 

6603354 

289 

53521 

24137560 

17-0000000 

6  611489 

290 

84100 

24389000 

17-0293864 

6 6191 00 

291 

84631 

24642171 

17-0587221 

6  626705 

292 

85264 

24897088 

1708S0075 

6634287 

293 

85849 

25153757 

171172428 

6641852 

294 

86436 

25412184 

1T1464282 

6649399 

2&5 

87025 

25672375 

171755640 

296 

87616 

25934336 

172046505 

297 

SS209 

26198073 

172336S79 

6671940 

S&S  / 

3SS04 

26463592 

at* 

89401 

26730S99 

300  / 

90000 

27000000 

SQ.UARE8,  CUBES,  AND  ROOTS. 


97 


Number. 

Square. 

Cube.  j 

Cubo  Root. 

oUX 

one  a  1 

yUbUl 

0*70^1  IftAl  1 

■  *>  1  a  •*  "-\  i  ^  1 

0  1 u 1 / oy 

aiKS 

1*  J  ZVJ4 

Z  7 04obUS 

1  /  »5  /  ■*»  I  -1  /  — 

l*«-7AQ  1  7*i 

b  tyiji  to 

QUO' 

Ql  A  AO 

•>7tt  1  4il  07  1 

17  lA<".^iQ'i,>  1 

n-7 1  a  !%7n 

0114 

9Z4XO 

*r>Uy4-l  )4  ! 

b  /-o;*.jl 

OUO 

1  7'J.H  !•>  l0->  ' 
1  l  4b  i^-ii'Z  - 

b  /  »3 1 0 1  b 

OUU 

0OO0O 

z*>b^-5i.>  I  b 

1  7-  IOOk'%%7 

b  /  Oobbo 

QAT 

94Z4;f 

OwO'i  4  i  t  M 

1  1  •)£  1  •!  1  O'J 

b  HOyy/ 

OAO 
•JUO 

y4oo4 

2'JJISI  12 

i*.r:  ((HIOh:Q 
1  /     t\t — •  ^ 

b  /  o»5o  1 0 

QAA 

ouy 

OI%  4  Q  1 

y»481 

zl'olMojy 

b  /b0bi4 

olO 

96100 

2979 1 00(1 

1  /  bUOSJ  oil 

b  /b/syy 

Ql  1 

ol  1 

o(JU802.>l 

1  /  00  )  1 y^i  1 

rfi^T^  1  ftft 

oiZ 

y/o44 

o\K57132S 

J  7  bbo  >J1  /  . 

b  /S24zd 

«ll  *1 
Old 

oUob4297 

17  oU  LNUbU 

0  ioybbl 

ol4 

QDSnA 

yoosib 

*J  A  ft  X 1 1 1  <  ■< 

ousjoy  14  * 

1  /  /  JUO  l.ll 

b  #ub.-?v± 

QIC 

olo 

yy^zo 

OlJOO.S70 

17  /4->Jo:M  | 

b  olMUyj 

olo 

yyoob 

31554496 

1  T-T^TlIM  wCki  1 
1  /    /  /  Oo-T^*)  ' 

/••CI  1  .'JC  4 

boll  Jh4 

1  An 4  co 

Qlti':        1  •> 

0I000U 1 .3 

1  7-ViA  <  iO*>tt 

/<  vim 
b      -^4b  J 

010 

1U1 iz4 

o.)i  KT  1  -JO 

1  /  OOJO.)  1.) 

b  oj..)bJ4 

olU 

1  A  I  T/l  1 
101 / Ol 

tSJ  In 17o9 

1  "1         \       1  1  1 
J  /  nUH.)  /II 

b  80 J / 7 1 

oon 

o^u 

/  b800l» 

0^1 

1  A'<AJ.  1 

00U  /  b  1  u  L 

1  /  f  1  bt /  —  J 

17  no  1 
b  n-i  tv)jz\ 

OZJ 

i  'MU-.H 

od-*r*bi  -  s 

1*7  fl  «  1  '>  \<<  » 

b  r».J'l  1  J4 

100 
O40 

1  A  1  "*Oft 

odbii^vtb  # 

1  /  .»  /  iil.'U? 

b  nO \£l & 

oZ4 

1  A  i  A"?  ft 

'1  1  A  1  OOO  1 

1  QlUli'lfiMllM 

*io  % 
0^0 

l v'OO  JtO 

>  •.••iOj.il-,-) 

1  ~  « J«-  #  I  ...  0  1  1 

r:  w7      1 .4 

'•ton 

1  nfW7<: 

A  UU^ f  U 

O  iU-JO.I  /  b 

b  *"io(33 

f 

1  w  As;:;  Hl'l 

ft-K^QJ  1  O 
b  o^y*i  1  ;| 

1  rt7%ftJ. 

1  V/  1  »JO-± 

tc-ii  ii/70'? 
l»p  IM'// yjt* 

b  «M/b-joo 

ozy 

'\~xfl  1  1  OCA 

b  JU-HOQ 

1  option 

-*>017(  win 

ivirrVK]')'  ' 

1  A  IOQ 

b  i'  1  u-j^o 

109561 

Ml'i'^fi  0"»<i  1 

]  s*  1934054 

#VA  1  7*-lQA 

oo<s 

1 1022 l 

yvf'/J  I •  J li ~ 

fi  QO  fJ^X 

333 

1  lOSsO 

18'24S2S76  • 

i;n*i  1  oni 
0  «'•)[  1 

334 

111556 

37259704 

18  2756669  ' 

6 938232 

335 

11222.3 

37595375 

18  303U052  , 

6  945149 

336 

112896 

37933056 

1S  330302S  ; 

6  952053 

337 

113.i69 

3S272753 

18  357559S  ; 

6 958943 

338 

11  1214 

38614472 

jS  3s  17763  ! 

6  965819 

339 

114921 

3.S95S219 

i  s  4  H  9526  ! 

6  972683 

340 

115600 

39304000 

18-4390SS9  i 

6 97"532 

341 

116281 

3965 1S21 

18  4661S53 

6986368 

342 

116964 

40001 6 ss 

Is  : 93:120  ! 

6993191 

343 

11 76-1 9 

40353**0? 

18  52;:::592  j 

7O00000 

344 

118.336 

4070  :  .^4 

18  5172370  i 

7006796 

345 

119025 

41063i>25 

18  5741756  | 

7013579 

346 

119716 

41421736 

18  6010752  j 

7020349 

347 

120409 

4 178 1923 

18  6279360  j 

7  02710ft 

348 

121104 

18-6547581  1 

849  121*01 

4250S549 

18  6S15417 

\  7-^V)o^\ 

850  I 

122600  : 

42875000 

18  70S2S69 

Vol.  I 

Number. 

Cube. 

Square  Root. 

Cube  Root.  ! 

351 

123201 

43243551 

18*7349940 

7054004 

352 

123904 

43614208 

187616630. 

7060696 

353 

124609 

43936977 

18-7882942 

7067376 

354 

,  125316 

44361964 

188148S77 

7074044 

355 

126025 

44739875 

18  8414437 

7080609 

356 

126736 

45118016 

1B8679623 

7  087341 

357 

127449 

45499293 

1SS944436 

7093971 

35S 

128164 

45882712 

IS  9208879 

7100588 

359 

128881 

46268279 

189472953 

7 107194 

360 

129600 

46656000 

18  9736660 

7 113786 

361 

i  130321 

47045881 

19  0000000 

7 120367 

362 

131044 

4743792S 

19  0262976 

7 126936 

363 

131769 

47832147 

19  0525589 

7133492 

364 

132496 

48228544 

19  0787840 

7*140037 

365 

133225 

4S627125 

19' 1049732 

7146569 

366 

133956 

49027896 

19  1311265 

7  153090 

367 

134689 

49430863 

19  1572441 

7  159599 

363 

135424 

49836032 

19  1333261 

7166096 

369 

136161 

50243409 

19  2093727 

7172580 

370 

136900 

50653000 

19*2353841 

7179054 

371 

137641 

51064811 

19  2613603 

7185516 

372 

138384 

51478S48 

19  2873015 

7  191966 

373 

139129 

51895117 

193132079 

7  198405 

374 

139S7G 

52313624 

19  3390796 

7  204832 

375 

140625 

52734375 

193649167 

7-311448 

376 

141376 

53157376 

19  3907194 

7  217652 

377 

*  142129 

535S2633 

19*4164878 

7  224045  ; 

378 

142884 

54010152 

19  4422221 

7230427 

379 

143641 

54439939 

194679223 

7236797 

380 

144400 

54872000 

194935887 

7  243156 

381 

145161 

55306341 

19  5192213 

7-240504 

3S2 

145924 

55742968 

19  5448203 

7255841 

383 

146689 
147456 

561S1S87 
56623104 

195703858 

7  262167 

384 

19  5959179 

T2694&2 

3S5 

14S225 

19  0214169 

*  &  ****  i'lVf 

7-274786 

386 

14S996 

57512456 

196468827 

7281079 

397 

149769 

57960603 

19  6723156 

7287362 

388 

150544 

5841 J 072 

19  6977156 

7293633 

3S9 

151321 

58S63869 

197230829 

7-299894 

390 

152100 

59319000 

197484177 

7  306143 

391 

152S81 

59776471 

19T737199 

7  312383 

392 

153664 

60236289 

19  7989899 

7318611 

393 

154449 

60698457 

198242276 

7324829 

394 

155236 

61162984 

19  8494332 

7-331037 

395 

156025 

61629875 

198746069 

7  337234 

396 

156S16 

62099136 

198997487 

7*343420 

3t)7 

157609 

62570773 

199248588 

7349597 

39? 

158404 

63044792 

19  9499373 

7355762 

399  1 

159201 

6352 1199 

19  9749844 

7361918 

400  j 

leoooo 

64000000 

200000000 

SQUARES,  CUBES,  AND  ROOTS. 


99 


uTTkuer, 

Square. 

v>ube< 

Square  Root. 

Cube  Root, 

401 

160801 

64481201 

20  0249844 

7  37419S 

401 

161604 

64964808 

200499377 

403 
404 

162409 

65450827 

20  0748599 

7386437 

163216 

05939264 

20  0997512 

7  392542 

405 

164025 

66430125 

20  1246118 

7  39H636 

406 

16493G 

669234 16 

20  1494417 

7-404720 

407 

165649 

67419143 

20  1742410 

7  410795 

408 

166464 

U7''l 1131  2 

20  1 990099 

7  41 6859 

409 

167291 

68417929 

SO  9237481 

7-422  rna. 

|       1  Jd          H.'   J  7t 

410 

168100 

7-4  28050 

411 

163921 

60426 531 

7-434994 

412 

169744 

69934 52S 

20  2Q77A3I 

7  44  1019 

413 

170569 

70444997 

2032240 14 

7-447034 

414 

171396 

70957944 

20  3469899 

7453040 

415 

172225 

71473H75 

20  3715488 

7  459036 

416 

173056 

7' 4  65022 

417 

173889 

7251 1713 

20  4205779 

7  470999 

418 

174724 

73034632 

20  4450483 

7  476966 

419 

175561 

73560059 

204694895 

7  4S2924 

420 

176400 

740SS000 

20  4939015 

7  4B8H72 

421 

177241 

74618461 

205182845 

7  49481 1 

422 

17S0S4 

75151448 

20  5426380 

7  500741 

423 

17S929 

75G969C7 

7  506  tiG  1 

424 

179776 

76225024 

20-59 1 2603 

7  512571 

425 

180625 

76765625 

20-6)55281 

7  51S473 

426 

181476 

77308776 

20  6397674 

7  524365 

427 

182329 

77854483 

20  6639783 

7-530248 

423 

183184 

78402752 

20  6Stf 1609 

7  536 J  21 

429 

18404 I 

78953589 

20  7123152 

7  541986 

430 

184900 

79507000 

20  7364414 

7-547^42 

431 

185761 

80062991 

20  7605395 

7 553688 

432 

186624 

80621568 

207846097 

7559526 

433 

187489 

81182737 

208086520 

7  565355 

434 

188356 

61746504 

208326667 

7'57 1174 

435 

189225 

82312875 

20S566530 

7  5769*5 

436 

190096 

82381856 

208806130 

7582786 

437 

190969 

83453453 

20  9045450 

75wy579 

438 

191844 

84027672 

20  9284495 

7594363 

439 

192721 

846045 1 9 

209523268 

760013S 

440 

193600 

85184000 

209761770 

7605905 

441 

194481 

85766121 

21  0000000 

7611662 

442 

195364 

863503S8 

21  0237960 

7  617412 

443 

196249 

86938307 

21  0475652 

7623152 

444 

197136 

87528384 

210713075 

7 628884 

445 

198025 

88121125 

21  0950231 

7634607 

446 

198916 

88716536 

211187121 

7640321 

447 

199809 

89314623 

21  1423745 

7646027 

448 

200704 

21  1660105 

\  tmviw 

449 

201601 

90513849 

21-1896201 

450  I 

202500  f 

91125Q0Q  | 

21  2132034  \  TWWM 

 t-rrx- 

\ 


100 


ARITHMETIC. 


iNJ  11  m  nor 

Cube. 

451 

203401 

91733851 

21  2367606 

7668766 

452 

204304 

9234540b 

21-2602916 

7674430 

453 

205209 

92959677 

21  2837967 

7  680086 

454 

206106 

93576664 

21  3072758 

7685733 

455 

207025 

94196375 

21  3307290 

7691372 

456 

207936 

94818S16 

21  3541565 

7697002 

457 

208849 

95443993 

21  3775583 

7-702625 

458 

209764 

96071912 

21  4009346 

7  708239 

459 

210681 

96702579 

21  4242853 

7713845 

460 

211600 

97336000 

214476106 

7  719442 

461 

212521 

97972181 

21  4709106 

7725032 

462 

213444 

9S611128 

21  4941853 

7  730614 

463 

214369 

99252847 

21  517434S 

7-736188 

464 

215296 

99897344 

21  5406592 

7741753 

465 

216225 

100544625 

21  5638587 

7  747311 

466 

217156 

101194696 

21  5870331 

7  752861 

467 

218089 

101847563 

21  6101828 

•7-758402 

468 

219024 

102503232 

21-6333077 

7763936 

469 

219961 

103161709 

21  6564078 

7769462 

470 

220900 

103823000 

21-6794834 

7774980 

471 

221841 

104487111 

21  7025344 

7780490 

472 

222784 

105154048 

21  7255610 

7785993 

473 

223729 

105823817 

217485632 

7791487 

474 

224676 

106496424 

21  7715411 

7796974 

475 

225625 

107171875 

21  7944947 

7-802454 

476 

226576 

107850176 

21  8174242 

7807925 

477 

227529 

108531333 

21  8403297 

7813389 

478 

22*184 

109215352 

21  8632111 

7818846 

479 

229411 

109902239 

21  88606S6 

7S24294 

480 

230400 

110592000 

21-9089023 

7829735 

481 

231361 

111284641 

21  9317122 

7835169 

482 

232324 

111980168 

21  9544984 

7840595 

483 

233289 

11267S587 

21  9772610 

7  846013 

484 

234254 

113379904 

22  0000000 

7851424 

485 

235225 

114084125 

220227155 

7856828 

4S6 

236196 

114791256 

220454077 

7862224 

487 

237169 

115501303 

220680765 

7  867613 

488 

238144 

116214272 

220907220 

7872994 

489 

239121 

116930169 

22  1133444 

7878368 

490 

240100 

117649000 

22  1359436 

7883735 

491 

241081 

118370771 

22- 1585 198 

7889095 

492 

212064 

119095488 

22  1810730 

7894447 

493 

243049 

119823157 

22-2036033 

7899792 

494 

244036 

120553784 

22  2261108 

7905129 

495 

245025 

121287375 

222485955 

7-910460 

496 

246016 

122023936 

222710575 

7-915783 

497 

247009 

122763473 

22-2934968 

7  921100 

498 

24S004 

123505992 

223159  Vifc 

499  / 

249001 

124251499 

oOO    l  250000  1 

125000000 

\ 


SQUARES,  CUBES,  AND  ROOTS. 


101 


Number. 

Square. 

 — 

Cube. 

Square  Root. 

Cube  Root. 

u  501 

251001 

125751501 

223330293 

7942293 

502 

252004 

126506008 

224053565 

7947574 

503 

253009 

127263527 

224276615 

7-952848 

504 

254016 

128024064 

224499443 

7-958114 

505 

255025 

12S7t*7625 

224722051 

7963374 

506 

256036 

129554216 

224944438 

7968627 

507 

257049 

130323843 

225166605 

7973873 

50S 

25S064 

131096512 

225333553 

7  979112 

509 

259081 

131872229 

22  5610283 

7984344 

510 

260100 

132651000 

22  5831796 

7989570 

511 

261121 

133432831 

226053091 

7994788 

512 

262144 

134217728 

226274170 

8000000 

513 

263169 

135005697 

226495033 

8005205 

514 

264196 

135796744 

22  6715681 

8010403 

515 

265225 

136590875 

22  6936114 

8015595 

516 

266256 

137388096 

22  7156334 

8020779 

517 

267289 

138188413 

22  7376340 

8025957 

518 

26S324 

138991832 

227596134 

8  031129 

519 

269361 

139798359 

227815715 

8036293 

520 

270400 

140608000 

228035085 

8041451 

521 

271441 

141420761 

228254244 

8046603 

522 

272484 

142236643 

228473193 

8051748 

523 

273529 

143055667 

228691933 

8056886 

524 

274576 

143877824 

22  8910463 

8062018 

525 

275625 

144703125 

22  9128785 

8067143 

526 

276676 

145531576 

229346899 

8072262 

527 

277729 

146363183 

22  9564806 

8077374 

528 

278784 

147197952 

22  9782500 

8082480 

529 

279841 

148035889 

230000006 

8087579 

530 

280900 

148877000 

23  0217289 

8092672 

531 

281961 

149721291 

23  0434372 

8097759 

532 

283024 

15056S768 

230651 252 

8 102839 

533 

284089 

151419437 

230867928 

8 107913 

1  •J^Z  /  OOUi 

Q.i  1  OOQA 

535 

286225 

153130375 

23- 1300670 

8 118041 

536 

287296 

153990656 

231516738 

8123096 

537 

286369 

154854153 

23  1732605 

8128145 

538 

289444 

155720872 

23  1948270 

8 133187 

539 

290521 

156590S19 

23  2163735 

8138223 

540 

291600 

157464000 

232379001 

8 143253 

541 

292681 

158340121 

232594067 

8-148276 

542 

293764 

159220088 

232808935 

8 153294 

543 

294849 

160103007 

233023604 

8- 158305 

544 

295936 

160989184 

233238076 

8 163310 

545 

297025 

161878625 

23  3452351 

8 168309 

546 

298116 

162771336 

233666429 

8- 173302 

547 

299209. 

163667323 

23  3880311 

8- 178289 

54S 

300304 

164566592 

234093998 

549 

301401 

165469149 

23  4307490 

S-\88*44 

550  1 

302500  I 

166375000 

23-4520788 

8-19**1* 

ARITHMETIC. 


Number. 

Square. 

Cube. 

Square  Root* 

Cube  Root 

551 



303601 

167284151 

23  4733892 

8 198175 

553 

304704 

168196608 

234946802 

8  203132 

553 

305309 

169112377 

23  5159520 

8208082 

554 

306916 

170031464 

23  5372046 

8  213027 

555 

308025 

170953875 

235584380 

8  217966 

556 

309136 

171879616 

235796522 

8222898 

557 

310249 

172308693 

23-6008474 

8227825 

558 

311364 

173741112 

23  6220236 

8  232746 

559 

312481 

174676879 

23-6431303 

8  237661 

560 

313600 

175616000 

23  6643191 

8242571 

561 

314721 

176553481 

23  6854386 

8247474 

562 

315844 

177504328 

237065392 

8252371 

563 

316969 

178453547 

23  7276210 

8257263 

564 

318096 

179406144 

237486842 

8262149 

565 

319225 

180362125 

237697236 

8  267029 

566 

320356 

181321496 

237907545 

8  271904 

567 

321439 

182284263 

23  8117618 

8  276773 

568 

322624 

133250432 

23-8327506 

8-281635 

569 

323761 

184220009 

23  5537209 

3236493 

570 

324900 

135193000 

23-8746728 

8  291344 

571 

326041 

186169411 

2389560(53 

8  296190 

572 

327184 

187149248 

23  9165215 

8  301030 

573 

323329 

183132517 

23  9374184 

8305865 

574 

329476 

189119224 

239532971 

8  310694 

575 

330625 

190109375 

23  9791576 

8315517 

576 

331776 

191102976 

240000000 

3320335 

577 

332929 

192100033 

240208243 

3  325147 

578 

3340S4 

193100552 

24  04 16306 

8  329954 

579 

335241 

194104539 

24  0624183 

8  334755 

580 

336400 

195112000 

24  0831892 

8339551 

581 

337561 

196122941 

24  1039416 

8  344341 

582 

333724 

197137368 

24  1246762 

8  349126 

583 

339889 

198155287 

24  1453929 

8353905 

584 

341056 

1%  lbbU919 

W d&3o78 

585 

342225 

200201625 

24  1867732 

8363446 

586 

343396 

201230056 

24  2074369 

8-368209 

587 

344569 

202262003 

24  2230829 

8372967 

588 

345744 

203297472 

24  2487113 

8  377719 

589 

346921 

204336469 

24  2693222 

8-382465 

590 

348100 

205379000 

242899156 

8387206 

591 

349281 

206425071 

24  3104916 

3-391942 

592 

350464 

207474688 

24  3310501 

8396673 

593 

351649 

208527857 

243515913 

8-401393 

594 

352836 

209584584 

24-3721152 

8406118 

595 

354025 

210644875 

24  3926218 

8  410833 

596 

355216 

2 11 703736 

244131112 

8  415542 

597 

356409 

212776173 

24  4335334 

8420246 

598 

357604  | 

213847192 

244540335 

.  8  424945 

599  f 

358801 

214921799 

24  47447^ 

600    I  360000  \ 

216000000 

24*M4fiOT4 

SQUARES,  CUBES,  AND  ROOTS. 


103 


Numbtf. 

Square. 

Square  KooL 

Cube  Hoot, 

601 

361201 

217081801 

24  5153013  | 

3  439010 

602 

362404 

218167208 

24  5356333 

8 443688 

603 

363609 

919256227 

24  5560583 

8 448 360 

604 

364816 

220348864 

24  5764115 

8  453028  ! 

605 

366025 

221445L25 

24-5967473 

3  457691 

60S 

367236 

222545016 

24  6170673 

8  462343 

607 

36S449 

223648543 

24  6373700 

8 467000 

60S 

369664 

224755712 

24  6576560 

8  471647 

609 

37088 1 

225366529 

24  6779254 

8  476289 

610 

372 1 00 

226 9S 1000 

24698 1781 

3480426 

611 

373321 

228099131 

24 -7 134 142 

8 43 55 58 

612 

374544 

229220928 

24-7386338 

8490 185 

613 

375769 

230346397 

24-7538363 

8 4 94 806 

614 

376996 

23 1475544 

24-7790234 

8 499423 

615 

378225 

232608375 

247991935 

ft  504035 

616 

379456 

233744396 

24-31 93473 

8508642 

617 

330639 

234885113 

24-8394847 

8-513243 

618 

381924 

236029032 

24  3596053 

8 517840 

619 

3S3161 

237176659 

24  3797106 

3-522432 

620 

384400 

236328000 

24-8997992 

8 527019 

6+>l 

38564 1 

239483061 

24  9198716 

8  531601 

622 

336884 

240641848 

24  9399278 

8  536178 

623 

388129 

241804367 

24  9599679 

8510750 

624 

3S9376 

24297QG24 

24  9799920 

8  545317 

625 

390625 

244140625 

25  0000000 

8-549379 

626 

391876 

245314376 

25  0199920 

8554437 

627 

393129 

246491833 

25  0399681 

8  558990 

623 

394384 

247673152 

25  0599282 

8563533 

629 

395641 

243858189 

25079S724 

8  563081 

630 

396900 

250047000 

25  0993008 

85726 19 

631 

398161 

251239591 

25  1197134 

3  577152 

632 

399424 

252435963 

25  1396102 

8531631 

633 

400689 

253636137 

25  1594913 

8  536205 

634 

401956 

254840104 

25  1793566 

8-590724 

635 

4032*5 

256047875 

25  1992063 

8595238 

636 

404496 

257259456 

252190404 

8-599747 

637 

405769 

25S474S53 

252388539 

3604252 

638 

407044 

259694072 

25  2536GJ9 

8608753 

639 

408321 

260917119 

252784493 

8613248 

640 

409600 

262144000 

25  2982213 

8  617739 

641 

410881 

263374721 

25  3179778 

8622225 

642 

412164 

2646092S8 

25-3377189 

8626706 

643 

413449 

265347707 

253574447 

8631183 

644 

1  414736 

2670399*4 

253771551 

8635655 

645 

416025 

263336125 

25  3968502 

8  640123 

646 

417316 

269536136 

25  4165301 

8-644585 

647 

418609 

570340023 

25  4361947 

3649044 

648 

419904 

272097792 

25-4558441 

649 

421201  : 

273359449  j 

25-4754784 

I  8657946 

050  j 

422500  j  274625000  j 

25  4950976 

\  8  Wt 

104 


ARITHMETIC. 


Number. 

Square, 

Cube. 

Square  Root. 

Cube  Root. 

651 

423S01 

275894451 

25  5147016 

8666831 

652 

425104 

277167808 

25  5342907 

8671266 

653 

426409 

278445077 

25  5 538647 

8-675697* 

654 

427716 

279726264 

(CtC    C.TO  #n*l»w 

25  5734 237 

S 680 124 

655 

429025 

£\<Cjr  1  111  1  O  T  £ 

28101 14  7o 

25  5929678 

8  684540 

656 

430336 

282300416 

25  6124969 

8  68y96i> 

657 

431649 

25  63201 12 

8 69337b 

653 

432964 

2848903 12 

256515107 

8  6SJ7784 

659 

434291 

2obl91 1 TSJ 

Ac,;'  nfj'i^v  ftco 

8  7l>£  loo 

660 

4d5h00 

not i ncAAn 

2a7496000 

256904652 

b  r  Ubao 7 

661 

436921 

2 8 88 04781 

257099203 

8  7109S3 

662 
663 

43S244 

290117528 

25  7203607 

8  715373 

439569 

fin  l  ^  n  j  a  j  pv 

291434247 

25  7487864 

8  7197^9 

664 

a.  incinc 
*4U$Ub 

292754944 
29407962a 

25  7681975 

8724141 

665 

A  A a  aa  r 

442225 

25  7875939 
25S069758 

8 728518 

G66 

443556 

295408296 

8  732892 

667 

444889 

296740963 

25  8263431 

8737260 

GtiH 

446224 

298077632 

258456960 

8  741624 

669 

447561 

299418309 

25  S6 50343 

O  wf  4  t  A£5  ^ 

8  74 59 So 

670 

A  A  D  AA/\ 

44S900 

300763000 

25  8o43582 

O'7o0o40 

671 

450241 

3021 1 171 1 

25  9036677 

A    f  E  J  /■fill 

8  754691 

672 

45158! 

3 034 G 444 8 

25-9229628 

s-  ?5903S 

673 

452929 

304821217 

25  9422435 

8  76oo81 

674 

454276 

306182024 

25961 51 00 

8  767719 

675 

455625 

307546875 

25  9307621 

S  772053 

676 

456976 

308915776 

2G  0000000 

S  7/6383 

677 

45S329 

3 1 0288733 

2»  0192237 

8  780708 

67S 

459684 

31 16G5752 

2t>  Uo^4*id  1 

Q  .FT  U  &  f\ A  A 

679 

461041 

h  1  lid  i  ni'i-lA 

313046839 

2605762S4 

□  .frtfin  j  j  ■ 

680 

462400 

o  1 44  o2trO(i 

ZD  u  /onUiJb 

S /HoboU 

6S1 

4bi37b  1 

•>  1  COO  1  O  IT 

6S2 

465124 

*5 1 72 14568 

nf  i  i  Ei  rtfli-f 

2b  1 1 0  J  2*17 

8  r>02272 

683 

46G489 

31861 1987 

2b  1342GS7 

S  MJ6572 

JO  L-j.j...ipji 

o  OI  U^DEs 

685 

469225 

321419125 

261725047 

8S15160 

BSC 

470596 

322828856 

26-1916017 

8819447 

687 

471969 

324242703 

262106848 

8  823731 

683 

473344 

325660672 

262297541 

8S2S009 

689 

474721 

3270827G9 

262488095 

8-832285 

690 

476100 

32850900G  ! 

26  267851 1 

8836556 

691 

4774S1 

329939371 

262868789 

S-840823 

692 

478864 

331373S3S 

26  3058929 

8-845085 

693 

480249 

332812557 

263248932 

8849344 

694 

481636 

3342553S4 

26-3438797 

8S53598 

695 

483025 

335702375 

26-3628527 

8-857849 

696 

484416 

33715353G 

26-3818119 

8862095 

697 

485809 

338608873 

26-4007576 

SS66337 

698 

487204 

340068392 

26*4196896 

8870576 

699 

488601 

341632099 

TOO  j 

490000 

343000000 

\  MA^bm 

SQUARES,  CUBES,  AND  ROOTS. 


105 


Cube.      |  Square  Foot  j  CuLe  Root. 

701 

491401 

344472101  I 

264764046  ! 

8883266 

702 

492804 

345948088 

26  4052826  , 

8887488 

703 

494209 

347428927  i 

265141472 

8891706 

704 

495616 

348913664 
35041)2625 

265329988 

8895920 

705 

497025 

265518361  | 

8900130 

706 

498436 

351895816 

26  5706605  j 

8904336 

707 

499849 

353303243 

26  5894716  j 

8-908538  i 

i  708 

501264 

354894912 

26  6082694 

8  912737 

709 

502681 

356400*29 

26  6270539 

8916931 

710 

504 1 00 

357911000 

26  6458252  > 

8921121 

711 

505521 

359425431 

26  6645833 

8925308 

712 

506944 

360944 12^ 

266833281 

8929490 

713 

50S369 

362467097 

267020598 

8933668 

714 

509796 

363994344 

267207784 

8*937843 

715 

511225 

365525875 

26  7394839 

8  942014 

716 

512656 

367061696 

267581763 

8946181 

717 

514089 

368601813 

26  7768557 

8950344 

718 

515524 

370146232 

267955220 

8954503  i 

719 

516961 

371694959 

268141754 

8958658  j 

720 

518400 

373248000 

26  8328157 

8962809  | 

721 

519841 

374805361 

26  8514432 

8966957  ! 

722 

37636704 H 

26  8700577 

8  971101  ! 

723 

522729 
524176 

377933067 

26  8886593 

8975240 

724 

379503424 

26-90724H1  1 

8979376 

725 

525625 

381078125 

26  9258240 

8-983509 

726 

527076 

382657 176 

26-9443872 

8  9*7637 

727 

52S529 

384240583 

.  269629375 

S 991762 

728 

529984 

3S5828352 

269814751 

8 995883 

729 

531441 

3S7420489 

270000000 

9  000000 

730 

532900 

389017000 

270185122 

9  004113 

731 

534361 

390617SUI 

27  0370117 

9008223 

732 

535S24 

392223168 

270554985 

9*012328 

733 

537289 

£.1  U  tOiJ  1 41 

o.m  £1  A  M  1 
\i  i)  I  b4ol 

734 

538756 

395446904 

27  0924 344 

9 020529 

735 

540225 

397065375 

27  1108834 

9024624 

736 

541696 

398688256 

27  1293199 

9  028715 

737 

543169 

400315553 

27  1477439  , 

9-032802 

738 

544644 

401947272 

27  1661554 

9036886 

739 

546121 

403583419 

27  1S45514 

9040965 

740 

547600 

405224000 

27  2029410 

9  045041 

741 

549081 

406869021 

27  2213152 

9  049114 

742 

550564 

40851848H 

272396769 

9053183 

743 

552049 

410172407 

27  2580263 

9057248 

744 

553536 

4118307*4 

27  2763634  j 

9061310 

745 

555025 

113403625 

27  2946SS1 

9065367 

746 

556516 

i  415160936 

27  3130006  : 

9  069422 

747 

558009 

416832723 

27  3313007  « 

9073473 

748 

559504 

418508992 

!  273495K87 

/    749  1 

561001  . 

'  4201S9749 

27  367S644 

\  9-QSU-&& 

L_750  I 

562500  I 

421875000  j 

27  3861270 

Vol.  I. 

15 

106  ARITHMETIC. 
-  . — *  t  ■■  ■  *  


Number. 

Square. 

Cube. 

Square  Root. 

Cube  Root. 

751 

564001 

42o0b47ol 

274043792 

- — -  — ■  

9  089639 

752 

565504 

42525900H 

27  42261S4 

9  093672 

753 

567009 

426957777 

2744084 55 

9+ 09770 1 

754 

568516 

428661064 

27  4590604 

9 101726 

755 

570025 

430368875 

27  "4772633 

91 105748 

756 

571536 

432081216 

27" 4954542 

9109766 

757 

573049 

433798093 

MH   jr  ill  ft  A  A  A  #V 

27  5136330 

9113781 

758 

574564 

I  ■  I  •    -    1  ,  ,  -   1  l 

L^nif        ft  1  PV  ft  n  fi 

27  5317998 

9"  117793 

759 

576081 

437245479 

Afv  E  A n H E  J 

27  5499 546 

9121801 

760 

577600 

43a!J7600U 

Af¥~.  E  Jf*  OftftPV  f 

27*5680975 

9125S05 

761 

579121 

4  *  ATT  1  jn o  i 

440711081 

2 7- 5862284 

9 129606 

762 

580644 

44245Q72S 

27H 6043475 

9-133803 

763 

582169 

444194947 

27  6224546 

9*137797 

764 

58369b 

445943744 

27-6405499 

9*141788 

765 

585225 

447697125 

27  b 586334 

9' 145774 

766 

586 7a6 

449455096 

27-6767050 

9' 149757 

767 

588289 

Jt(£TA*tWji.jtA 

451217663 

276947648 

9 153737 

76S 

f£!}ft£?A  J 

589824 

452984832 

27  7128129 

9157714 

769 

591361 

454756609 

27-7308492 

9161686 

770 

r  fill nriA 

592900 

456533000 

27- 7438739 

9' 165656 

771 

594441 

458314011 

27-7668868 

91 169622 

772 

595984 

460099648 

27- 7848880 

n,     -ft  Pwn  jp  ja.  n 

9- 173585 

773 

597529 

461889917 

27  8028775 

9 177544 

774 

599076 

463bS4H24 

27S20S555 

9181500 

775 

600625 

465484375 

27*8388218 

9 185453 

776 

602176 

467288576 

A*V  A  f  nfVM  n  ^1 

27  8567766 

9- 189402 

777 

603729 

A  £3  A  J"ki  i\M  j  nil 

469097433 

27  8747197 

9 193347 

778 

605284 

4709 1 0952 

27  8 9265 14 

9' 197239 

779 

bU6341 

47272^139 

£)■*  Ai  AFrVi  r- 

279105715 

9201229 

780 

608400 

47 4 DO 2000 

Ilk          ft  AO  J  4 

2 7+ 9284801 

9 205 164 

781 

bU99bl 

4ro379541 

279463772 

9  209096 

782 

fill 524 

47821 1768 

279642629 

9  213025 

783 

j-fc  i  A  AAA 

613089 

480048687 

279921 372 

1  9216950 

784 

614656 

481890304 

280000000 

9 '220873 

785 

616225 

483736625 

280178515 

9  224791 

786 

617796 

485587656 

28  0356915 

9228707 

787 

619369 

487443403 

280535203 

9  232619 

789 

620944 

489303872 

28  0713377 

9  237528 

789 

622521 

491169069 

28  0891438 

9240433 

790 

624100 

493039000 

28  1069386 

9  244335 

791 

625681 

494913671 

28  1247222 

9243234 

792 

627264 

496793088 

28  1424946 

9252130 

793 

628849 

498677257 

28  1602557 

9256022 

794 

630436 

500566184 

28  1780056 

9  259911 

795 

632025 

502459875 

28  1957444 

9263797 

796 

633616 

504358336 

23  2134720 

9*267680 

797 

635209 

506261573 

28  231 1884 
28  2488938 

9271559 
9  275435 

798 

'  636S04 

5031 69592 

799 

63S401 

510082399 

40b0881 

9279308 

800  j 

640000  | 

512000000 

BQVAftES,  CUBES,  AND  ROOTS. 


107 


Number, 


801 
803 
803 
804 
805 
806 
807 


810 
811 
812 
813 
814 
815 
816 
817 
818 
810 
820 
831 
822 
823 
824 
825 
826 
837 
823 
820 
830 
831 
832 


835 


837 


840 
841 
842 
843 
844 
845 
846 
847 
848 
849 


Square. 


6416Q1 
643304 
644300 
646416 
643025 
649636 
651249 


654481 
656100 
657721 
659344 
660960 
662596 
664225 
665956 
6674S9 
669124 
670761 
672400 
674041 
675684 
677329 
678976 
680625 
682276 
683929 
6S5584 
637241 
688900 
690561 


697225 


848  I 
850    I  S 


700569 
702244 
703921 
705600 
707281 
708964 
710649 
712336 
714025 
715716 
717409 
719104 
720601  j 
722500  / 


Cube. 


513922401 
515849608 
517781627 
519718464 
521660125 
623606616 
525557943 
527514112 
529475120 
531441000 
533411731 
635387328 
537366797 
530353144 
541343375 
543338496 
545336513 
547343432 
540353250 
55136S000 
553387661 
555412248 
557441767 
559476224 
561515625 
563559976 
565600283 
567663552 
569722780 
571787000 
573S5G191 
575030368 
578009537 
580093704 
5821S2875 
584277056 
586376253 
5884S0472 
590589719 
592704000 
594823321 
596947683 
599077107 
601211584 
603351125 
605495736 
607645423 
!  609800192 
611960049 
614125000 


Square  Root. 


Cube  Root. 


28  3019434 
23  3106045 
283372546 
28-3543933 
28  3725210 
233901391 
28  4077454 
23-4253408 
284420253 
284604989 
23  4780617 
28  4956137 
285131549 
285306852 
23  5482048 
28  5657137 
23  5832119 

28-  6006993 
28  6181760 
236356421 
28*6530976 
28  6705424 
23  6370766 
287054002 
28  7228132 
287402157 
28  7576077 
28  7749891 
28  7923601 
238097206 
288270706 
28  8444102 
288617394 
288790582 
28  8063666 
28  9136646 
289309523 
28  9482297 
289654967 

28  9827535 
290000000 
200172363 

29  0344623 
29  0516781 
290688837 
29  0860791 
29  1032644 
29  1204396 
29*1376046 

29-  1547595 


0287044 
0290907 
9294767 
9298624 
9302477 
9  306328 
9310175 
9314019 
0  317860 
0  321697 
9325532 
9329363 
9  333192 
0  337017 
9*340838 
0344657 
0348473 
9352286 
0356095 
9359902 
9  363705 
9367505 
9  371302 
9-375096 
9-37S887 
9382675 
9386460 
9300242 
9394020 
0397796 
9401569 
9405339 
9  409105 
9  412369 
9  416630 
9  420337 
9424142 
9427894 
9431642 
9  435388 
9439131 
9  442870 
944C607 
9450341 
9454072 
945TOQQ 

9-4-WMA 
9-4*ra&9A 


108 


ARITHMETIC. 


rHUIIlUci. 

Cube. 

SnunTP  Root 

Cube  Root 

851 

724201 

616295051 

29  1719043 

9476395 

852 

725904 

618470208 

29  1690390 

9480106 

853 

727609 

620650477 

292061637 

9-483813 

854 

729316 

622835864 

292232784 

9487518 

855 

731025 

625026375 

292403830 

9491220 

856 

732736 

627222016 

292574777 

9494919 

857 

734449 

629422793 

292745623 

9  498615 

858 

736164 

631628712 

292916370 

9502308 

859 

737881 

633839779 

293087018 

9505998 

860 

739600 

636056000 

293257566 

9509685 

861 

741321 

638277381 

293428015 

9513370 

862 

743044 

640503928 

293598365 

9517051 

863 

744769 

642735647 

293768616 

9520730 

864 

746496 

644972544 

293938769 

9524406 

865 

748225 

647214625 

294108823 

9528079 

866 

749956 

649461896 

294278779 

9531749 

867 

751689 

651714363 

294446637 

9  535417 

868 

753424 

653972032 

29  4618397 

9539082 

869 

755161 

656234909 

294788059 

9542744 

870 

756900 

658503000 

294957624 

9546403 

871 

758641 

660776311 

29-5127091 

9550059 

872 

760384 

663054848 

295296461 

9553712 

873 

762129 

665338617 

295465734 

9557363 

874 

763876 

667627624 

295634910 

9561011 

875 

765625 

669921875 

295803989 

9564656 

876 

767376 

672221376 

295972972 

9568298 

877 

769129 

674526133 

296141858 

9571938 

878 

770884 

676836152 

29  6310648 

9575574 

879 

772641 

679151439 

296479325 

9579208 

880 

774400 

681472000 

296647939 

9-582840 

881 

776161 

683797841 

296616442 

9586468 

S82 

777924 

686128968 

296984848 

9590094 

883 

779689 

688465387 

297153159 

9593716 

884 

781456 

690807104 

297321375 

9597337 

885 

783225 

693154125 

297489496 

9600955 

886 

784996 

695506456 

29  7657521 

9-604570 

8S7 

786769 

697864103 

297825452 

9608182 

888 

788544 

700227072 

297993289 

9611791 

889 

790321 

702595369 

29  8161030 

9615398 

890 

792100 

704969000 

298328678 

9619002 

891 

793881 

707347971 

29  8496231 

9622603 

892 

795664 

7097322S8 

298663690 

9626201 

893 

797449 

712121957 

298831056 

9629797 

894 

799236 

714516984 

298998328 

9633390 

895 

801025 

716917375 

299165506 

9636981 

896 

802816 

719323136 

299332591 

9640569 

897 

804609 

721734273 

299499583 

9  644154 

898  I 

806404 

724150792 

I  9  647737 

899 

808201 

726572699 

900    /  810000 

729000000  \    30  OOOOWto  \  9 

•QUARKS,  CUBES,  AND  ROOTS. 


109 


Number.  Square,  Cube 


811801 
813604 
815409 
817316 
819025 
H2083G 


826281 
828100 
829921 
831744 
833569 
835396 
837225 
839056 
840889 
842724 
844561 
846400 
848241 
850084 
851929 
853776 
855625 
857476 
S59329 
861 184 
863041 
864900 
866761 
868624 
870489 
872356 
874225 
876096 
877969 
979844 
881721 
883600 
8*548] 
887364 
889249 
891136 
893025 
S9491C 
896809 
89S704 
900601  j 
902500  / 


731432701 
733870808 
736314327 
73S763264 
741217625 
743677416 
746142643 
748613312 
751039429 
753571000 
756058031 
758550528 
761048497 
763551944 
766060375 
768575296 
771095213 
773620632 
776151559 
778688000 
791229961 
783777448 
786330467 
788389024 
791453125 
794022776 
796597983 
799178752 
301765039 
804357000 
806954491 
809557568 
812166237 
314730504 
817400375 
820025856 
822656953 
825293672 
827936019 
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110 


ARITHMETIC 


951 
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WOO  / 


Square.      Cube.       Square  Root.    Cube  Root 


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1 


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31  0000000 
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31-  0805405 
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Ill 


OF  RATIOS,  PROPORTIONS,  AND  PRO- 
GRESSIONS. 

Numbers  are  compared  to  each  other  in  two  different 
ways :  the  one  comparison  considers  the  difference  of  the  two 
numbers,  and  is  named  Arithmetical  Relation ;  and  the  dif- 
ference sometimes  the  Arithmetical  Ratio  :  the  other  con- 
siders their  quotient,  which  is  called  Geometrical  Relation ; 
and  the  quotient  is  the  Geometrical  Ratio.  So,  of  these  two 
numbers  6  and  3,  the  difference,  or  arithmetical  ratio  is 
6—8  or  8,  but  the  geometrical  ratio  is  f  or  2. 

There  must  be  two  numbers  to  form  a  comparison :  the 
number  which  is  compared,  being  placed  first,  is  called  the 
Antecedent :  and  that  to  which  it  is  compared,  the  Con- 
sequent.  So,  in  the  two  number*  above,  6  is  the  antecedent, 
and  3  the  consequent. 

If  two  or  more  couplets  of  numbers  have  equal  ratios,  or 
equal  differences,  the  equality  is  named  Proportion,  and  the 
terms  of  the  ratios  Proportionals.  So,  the  two  couplets,  4,  2 
and  8,  6,  are  arithmetical  proportionals,  because  4-2  =  8 
—6  =  2;  and  the  two  couplets  4,  2  and  0,  3,  are  geome- 
trical proportions,  because  |  =  f  =  2,  the  some  ratio. 

To  denote  numbers  as  being  geometrically  proportional,  a 
colon  is  set  between  the  terms  of  each  couplet,  to  denote  their 
ratio  ;  and  a  double  colon,  or  else  a  mark  of  equality,  between 
the  couplets  or  ratios.  So,  the  four  proportionals,  4, 2,  6,  3 
are  set  thus,  4  :  2  : :  6  :  3,  which  means,  that  4  is  to  2  as  6 
is  to  3 ;  or  thus,  4:2  =  6:3,  or  thus,  |  =  |,  both  which 
mean,  that  the  ratio  of  4  to  2,  is  equal  to  the  ratio  of 
6  to  3. 

Proportion  is  distinguished  into  Continued  and  Discon- 
tinued. When  the  difference  or  ratio  of  the  consequent  of 
one  couplet,  and  the  antecedent  of  the  next  couplet,  is  not 
the  same  as  the  common  difference  or  ratio  of  the  couplets, 
the  proportion  is  discontinued.  So,  4,  2, 8,  6,  are  in  discon- 
tinued arithmetical  proportion,  because  4—2=8  —  6=2, 
whereas  8  —  2=6:  and  4,  2,  6,  3  are  in  discontinued  geo- 
metrical proportion,  because  f  =  §■  =  2,  but  -J  =  3,  which  is 
not  the  same. 

But  when  the  difference  or  ratio  of  every  two  succeeding 
terms  is  the  same  quantity,  the  proportion  is  said  to  be  Con- 
tinued, and  the  numbers  themselves  make  a  scrisa  ot  Cwv- 


112 


ARITHMETIC. 


Untied  Proportionals,  or  a  progression.  So  2,  4, 6,  8  form 
an  arithmetical  progression,  because  4  —  2  =  0  —  4  =  8  — 
6  =  2,  all  the  same  common  difference ;  and  2,  4,  8,  16,  a 
geometrical  progression,  because  f  =  }  =  Y=2,  all  the 
same  ratio. 

When  the  following  terms  of  a  progression  increase,  or 
exceed  each  other,  it  is  called  an  Ascending  Progression,  or 
Series ;  but  when  the  terms  decrease,  it  is  a  descending 
one. 

So,  0,  1,  2,  3, 4,  &c.  is  an  ascending  arithmetical  progression, 
but  9, 7, 5, 3, 1,  dec.  is  a  descending  arithmetical  progression. 
Also  1 ,2, 4, 8, 16,  dec.  is  an  ascending  geometrical  progression, 
and  16, 8, 4, 2, 1 ,  dec.  is  a  descending  geometrical  progression* 


ARITHMETICAL  PROPORTION  AND 
PROGRESSION. 

In  Arithmetical  Progression,  the  numbers  or  terms  have 
all  the  same  common  difference.  Also,  the  first  and  last 
terms  of  a  Progression,  are  called  the  Extremes ;  and  the 
other  terms,  lying  between  them,  the  Means.  The  most 
useful  part  of  arithmetical  proportion,  is  contained  in  the 
following  theorems : 

Theorem  1.  When  four  quantities  are  in  arithmetical 
proportion,  the  sum  of  the  two  extremes  is  equal  to  the  sum 
of  the  two  means.  Thus,  of  the  four  2,  4,  6,  8,  here  2  + 
8  =  4  +  6=10. 

Theorem  2.  In  any  continued  arithmetical  progression, 
the  sum  of  the  two  extremes  is  equal  to  the  sum  of  any  two 
means  that  are  equally  distant  from  them,  or  equal  to  double 
the  middle  term  when  there  is  an  uneven  number  of  terms. 

Thus,  in  the  terms  1,  3,  5,  it  is  1  +  5  =  3  +  3  =  6. 

And  in  the  series  2,  4,  6,  8,  10, 12,  14,  it  is  2  +  14  =  4 
+  12  =6  +  10  =  8  +  8  =  10. 

Theorem  3.  The  difference  between  the  extreme  terms 
of  an  arithmetical  progression,  is  equal  to  the  common  dif- 
ference of  the  series  multiplied  by  one  less  than  the  number 
of  the  terms.  So,  of  the  ten  terms,  2,  4,  6,  8,  10, 12,  14, 
16,  18,  20,  the  common  difference  is  2,  and  one  less  than 
the  number  of  terms  9  ;  then  the  difference  of  the  extremes 
is  20  -  2  =  18,  and  2  X  9  =  18  also. 


ARITHMETICAL  PHOFORTION. 


113 


Consequently  the  greatest  term  is  equal  to  the  least  term 
added  to  the  product  of  the  commoo  difference  multiplied  by 
1  less  than  the  number  of  terms. 

Theorem  4.  The  sum  of  all  the  terms,  of  any  arith- 
metical progression,  is  equal  to  the  sum  of  the  two  extremes 
multiplied  by  the  number  of  terms,  and  divided  by  2 ;  or  the 
sum  of  the  two  extremes  multiplied  by  the  number  of  the 
terms,  gives  double  the  sum  of  all  the  terms  in  the  series. 

This  is  made  evident  by  setting  the  terms  of  the  series  in 
an  inverted  order,  under  the  same  series  in  a  direct  order,  and 
adding  the  corresponding  terms  together  in  that  order.  Thus, 
in  the  series  1,  3,  5,  7,  9,  11,  13,  15; 
ditto  inverted  15,  13,  11,  9,  7,  5,  3,  1  ; 
the  sums  are  16  +10  +  16  +  16  +  16  +  16  +  16  -f- 16, 
which  must  be  double  the  sum  of  the  single  series,  and  is 
equal  to  the  sum  of  the  extremes  repeated  as  often  as  are  the 
number  of  the  terms. 

From  these  theorems  may  readily  be  found  any  one  of 
these  five  parts ;  the  two  extremes,  the  number  of  terms,  the 
common  difference,  and  the  sum  of  all  the  terms,  when  any 
three  of  them  are  given  ;  as  in  the  following  problems  : 

PROBLEM  I. 

Given  the  Extremes,  and  the  Number  of  Terms,  to find  the  Sum 
of  all  the  Terms, 

Add  the  extremes  together,  multiply  the  sum  by  the 
number  of  terms,  and  divide  by  2. 

EXAMPLES. 

1.  The  extremes  being  3  and  19,  and  the  number  of 
terms  9 ;  required  the  sum  of  the  terms  ? 

19 
3 

22 

2)  198 
Ans.  99 

2.  It  is  required  to  find  the  number  of  all  the  strokes  a 
common  clock  strikes  in  one  whole  revolution  of  the  index, 
or  in  12  hours.  Aua.nfc. 

Vox.  1.  1G 


=  ^X9=11  X  9  =  99, 
the  same  answer. 


114 


▲xinufsnc. 


Ex.  3.  How  many  strokes  do  the  clocks  of  Venice  strike 
in  the  compass  of  the  day,  which  go  continually  on  from  1 
to  24  o'clock  ?  Ana.  300. 

4.  What  debt  can  be  discharged  in  a  year,  by  weekly 
payments  in  arithmetical  progression,  the  first  payment  being 
Uy  and  the  last  or  52d  payment  5i  3t  ?  Ans.  1851 4*. 


PROBLRX  n. 


Given  the  Extremes,  and  the  Number  of  Terms  ;  t^findthe 
Common  Difference. 

Subtract  the  less  extreme  from  the  greater,  and  divide 
the  remainder  by  1  less  than  the  number  of  terms,  for  the 
common  difference. 


EXAMPLES. 


1.  The  extremes  being  3  and  19,  and  the  number  of  terms 
9 ;  required  the  common  difference  ? 

19 

Ur'  9-T  ¥ 


2.  If  the  extremes  be  10  and  70,  and  the  number  of  terms 
21  ;  what  is  the  common  difference,  and  the  sum  of  the 
series  ?  Ans.  the  com.  diff.  is  3,  and  the  sum  is  840/ 

3.  A  certain  debt  can  be  discharged  in  one  year,  by  weekly 
payments  in  arithmetical  progression,  the  first  payment  being 
1*,  and  the  last  51  Ss  ;  what  is  the  common  difference  of  the 
terms?  Ans.  2. 


PROBLEM  III. 

v 

Given  one  of  the  Extremes,  the  Common  Difference,  and  the 
Number  of  Terms  ;  to  find  the  other  Extreme,  and  the 
Sum  of  the  Series. 

Multiply  the  common  difference  by  1  less  than  the 
number  of  terms,  and  the  product  will  be  the  difference  of 
the  extremes :  Therefore  add  the  product  to  the  less  ex- 
treme to  give  the  greater  ;  or  substract  it  from  the  greater, 
to  give  the  less  extreme. 


ARITHMETICAL  PROGRESSION. 


115 


EXAMPLES. 

1.  Given  the  least  term  3,  the  common  difference  2,  of  an 
arithmetical  aeries  of  9  terms ;  to  find  the  greatest  term,  and 
the  sum  of  the  series. 

Here  2  X  (9  —  1)  +  3  =  19,  the  greatest  terra.  Theref. 
(10  +3)|  =  »}•  =99,  the  sum  of  the  series. 

2.  If  the  greatest  term  be  70,  the  common  difference  3, 
and  the  number  of  terms  21,  what  is  the  least  term,  and  the 
sum  of  the  series  ? 

Ans.  The  least  term  is  10,  and  the  sum  is  840. 

8.  A  debt  can  be  discharged  in  a  year,  by  paying  1  shilling 
the  first  week,  8  shillings  the  second,  and  so  on,  always  2 
shillings  more  every  week ;  what  is  the  debt,  and  what  will 
the  last  payment  be  ? 

Ans.  The  last  payment  will  be  5*  3*,  and  the  debt  is  1357  4s. 


PROBLEM  IV. 

To  find  an  Arithmetical  Mean  Proportional  between  two 
given  terms. 

Add  the  two  given  extremes  or  terms  together,  and  take 
half  their  sum  tor  the  arithmetical  mean  required. 

EXAMPLE. 

To  find  an  arithmetical  mean  between  the  two  numbers  4 
and  14.  Here 
14 
4 

2)  18 

Ans.     9  the  mean  required. 


problem  v. 

To  find  two  Arithmetical  Means  between  two  given 
Extremes. 

Subtract  the  less  extreme  from  the  greater,  and  divide 
the  dMfeienee  by  8,  so  will  the  quotient  be  the  coranKfli&i- 


116 


ARITHMETIC. 


ference  ;  which  being  continually  added  to  the  less  extreme, 
or  taken  from  the  greater,  will  give  the  means. 

EXAMPLE. 

To  find  two  arithmetical  means  between  2  and  3. 
Here  8 
2 

3)    6      Then  2  +  2  =  4  the  one  mean. 
— —        and  4  +  2  =  6  the  other  mean, 
com.  dif.  2 


PROBLEM  VI. 

To  find  any  Number  of  Arithmetical  Means  between  two 
given  Terms  or  Extremes. 

Subtract  the  less  extreme  from  the  greater,  and  divide 
the  difference  by  1  more  than  the  number  of  means  required 
to  be  found,  which  will  give  the  common  difference ;  then  this 
being  added  continually  to  the  least  term,  or  subtracted  from 
the  greatest,  will  give  the  mean  terms  required. 

EXAMPLE. 

To  find  five  arithmetical  means  between  2  and  14. 
Here  14 
2 

6)  12      Then  by  adding  this  com.  dif.  continually, 

  the  means  are  found  4,  6,  8,  10,  12. 

com.  dif.  2 

See  more  of  Arithmetical  progression  in  the  Algebra. 


GEOMETRICAL  PROPORTION  AND  PRO- 
GRESSION. 

If  there  be  taken  two  ratios,  as  those  of  6  to  3,  and  14 
to  7,  which,  by  what  has  been  already  said  (p.  113),  may 


GEOMETRICAL  tfftOGBBMIO*. 


117 


be  expressed  fractionally,  }  and  \f  ;  to  judge  whether  they 
are  equal  or  unequal,  we  must  reduce  them  to  a  common 
denominator,  and  we  shall  have  6X7,  and  14  X  3  for  the 
two  numerators.  If  these  are  equal,  the  fractions  or  ratios 
are  equal.  Therefore, 

Theorem  i.  If  four  quantities  be  in  geometrical  propor- 
tion, the  product  of  the  two  extremes  will  be  equal  to  the 
product  of  the  two  means. 

And  hence,  if  the  product  of  the  two  means  be  divided 
by  one  of  the  extremes,  the  quotient  will  give  the  other  ex- 
treme.  So,  of  the  above  numbers,  if  the  product  of  the  means 
42  be  divided  by  6,  the  quotient  7  is  the  other  extreme ; 
and  if  42  be  divided  by  7,  the  quotient  6  is  the  first  ex- 
treme. This  is  the  foundation  of  the  practice  in  the  Rule 
of  Three. 

We  see,  also,  that  if  we  have  four  numbers,  6,  3,  14,  7, 
such,  that  the  products  of  the  means  and  of  the  extremes  are 
equal,  we  may  hence  infer  the  equality  of  the  ratios  $  =y , 
or  the  existence  of  the  proportion  6 :  3 :  :  14  :  7.  Hence 

Theorem  n.  We  may  always  form  a  proportion  of  the 
factors  of  two  equal  products. 

If  the  two  means  are  equal,  as  in  the  terms  3,  6,  6,  12, 
their  product  becomes  a  square.  Hence 

Theorem  hi.    The  mean  proportional  between  two  num- 
bers is  the  square  root  of  their  product. 
We  may,  without  destroying  the  accuracy  of  a  proportion, 

S've  to  its  various  terms  all  the  changes  which  do  not  affect 
e  equality  of  the  products  of  the  means  and  extremes. 
Thus,  with  respect  to  the  proportion  6  :  3  :  :  14  :  7, 
which  gives  6X7  =  3X1 4,  we  may  displace  the  extremes, 
or  the  means,  an  operation  which  is  denoted  by  the  word 
AMcrnando. 

This  will  give  6  :  14  : :  3:7 

or  7  :  3  : :  14  :  6 

or  7  :  14  : :  3:6 

Or,  2dly,  we  may  put  the  extremes  in  the  places  of  the  means, 
oalled  lnvertendo. 

Thus  3  :  6  :  :  7  :  14. 

Or,  3dly,  we  may  multiply  or  divide  the  two  antecedents, 
or  the  two  consequents,  by  the  same  number,  when  propor- 
tionality will  subsist. 


118  ARITHMETIC. 

As  6  X  4  :  3  : :  14  X  4  :  7 ;  viz.  24  :  3  : :  66  :  7 
and6^-2:3::  14-t-2:7;  viz.  3:3::  7:7. 

Also,  applying  the  proposition  in  note  2,  Addition  of 
Vulgar  Fractions,  to  the  terms  of  a  proportion,  such  as 
30  :  6  : :  15  :  3,  or  y  =  y,  we  shall  have 

30±15     15     . 30+15     30-15  „ 

 =  —  and  =  .  Hence 

6±3       3        6+3  6-3 

Theorem  iv.  The  sum  or  the  difference  of  the  antece- 
dents, is  to  that  of  the  consequents,  as  any  one  of  the  ante- 
cedents is  to  its  consequent. 

Theorem  v.  The  sum  of  the  antecedents  is  to  their 
difference,  as  the  sum  of  the  consequents  is*  to  their  dif- 
ference. 

In  like  manner,  if  there  he  a  series  of  equal  ratios, 
1  =  V  =  V4  =  i  J  5  we  have 
6+10+14+30  =  14  =  30 
3+5+7+15        7      15  *nereiure, 

Theorem  vi.  In  any  series  of  equal  ratios,  the  sum  of 
the  antecedents  is  to  that  of  the  consequents,  as  any  one  an- 
tecedent is  to  its  consequent. 

Theorem  vii.  If  two  proportions  are  multiplied,  term  by 
term,  the  products  will  constitute  a  proportional. 

Thus,  if  30  :  15  ::  6  :  3 
and    2  :   3  : :  4  :  6. 

Then  30  X  2  :  15  X  3  ::  6  X  4  :  3  X  6 
or  60  :  45  ::  24  :  18  ;  or  f  J-  = 

Theorem  viii.  If  four  quantities  are  in  proportion,  their 
squares,  cubes,  &c.  will  be  in  proportion. 

For  this  will  evidently  be  nothing  else  than  assuming  the 
proportionality  of  the  products,  term  by  term,  of  two,  three, 
or  more  identical  proportions. 

The  same  properties  hold  with  regard  to  surd  or  irrational 
expressions, 

Thus,  v'TSO  :  ^80  ::  ^567  :  ^63 
and  -y/12   :-y/3    ::  :  -y/1. 


y/720  =  y'O  .  80  =  3  y/567  _  y/9X63  _  3 
y/80  "~  V  **    -v/63        y/63  1 

,  12     v/4  2 

and^3c=^-3=— =r 


GEOMETRICAL  PROGRESSION. 


119 


Theorem  ix.    The  quotient  of  the  extreme  terms  of  a 
•  geometrical  progression  is  equal  to  the  common  ratio  of  the 
series  raised  to  the  power  denoted  by  1  less  than  the  number 
of  the  terms. 

So,  of  the  ten  terms  2,  4,  8,  16,  32,  64,  128,  256,  512, 
1024,  the  common  ratio  is  2,  one  less  than  the  number  of 
terms  9 ;  then  the  quotient  of  the  extremes  is  1  °^ 4  =  512, 
and  2°  =  512  also. 

Consequently  the  greatest  term  is  equal  to  the  least  term 
multiplied  by  the  said  power  of  the  ratio  whose  index  is  1 
less  than  the  number  of  terms. 

Theorem  x.  The  sum  of  all  the  terms,  of  any  geome- 
trical progression,  is  found  by  adding  the  greatest  term  to  the 
difference  of  the  extremes  divided  by  1  less  than  the  ratio. 

So,  the  sum  of  2,  4,  8,  16,  32,  64,  128,  256,  512,  1024, 
1024-2 

(whose  ratio  is  2)  is  1024  +  -^-y- =  1024  + 1022  =2046. 

This  subject  will  be  resumed  in  the  Algebraic  part  of  this 
"work.    A  few  examples  may  here  be  added. 


EXAMPLES. 

1.  The  least  of  ten  terms,  in  geometrical  progression, 
being  1,  and  the  ratio  2  ;  what  is  the  greatest  term,  and  the 
sum  of  all  the  terms  ? 

Ans.  The  greatest  term  is  512,  and  the  sum  1023. 

2.  What  debt  may  be  discharged  in  a  year,  or  12  months, 
iy  paying  1Z  the  first  month,  21  the  second,  4Z  the  third,  and 
40  on,  each  succeeding  payment  being  double  the  last ;  and 
what  will  the  last  payment  be  ? 

Ans.  The  debt  4095Z,  and  the  last  payment  2048/. 


PROBLEM  I. 

To  find  one  Geometrical  Mean  Proportional  between  any  two 
Numbers. 

Multiply  the  two  numbers  together,  and  extract  the 
*C|uare  root  of  the  product,  which  will  give  the  mean  propor- 
tional sought. 


120 


ARITHMETIC* 


EXAMPLE. 

To  fiad  a  geometrical  mean  betweea  the  two  numbers 
3  and  12. 

12 
3 

36  (6  the  mean. 
36 


PROBLEM  II. 

To  find  two  Geometrical  Mean  Proportionals  between  any  two 
Numbers. 

Divide  the  greater  number  by  the  less,  and  extract  the 
cube  root  of  the  quotient,  which  will  give  the  common  ratio 
of  the  terms.  Then  multiply  the  least  given  term  by  the 
ratio  for  the  first  mean,  and  this  mean  again  by  the  ratio  for 
the  second  mean :  or,  divide  the  greater  of  the  two  given 
terms  by  the  ratio  for  the  greater  mean,  and  divide  this  again 
by  the  ratio  for  the  less  mean. 

EXAMPLE. 

To  find  two  geometrical  means  between  3  and  24. 

Here  3  )  24  (  8 ;  its  cube  root  2  is  the  ratio. 

Then  3  X  2  =  6,  and  6  X  2  =  12,  the  two  means. 

Or  24 +  2  =  12,  and  12  -r-  2  =  6,  the  same. 

That  is,  the  two  means  between  3  and  24,  are  6  and  12. 


problem  in. 

To  find  any  number  of  Geometrical  Means  between  two 
Numbers. 

Divide  the  greater  number  by  the  less,  and  extract  such 
root  of  the  quotient  whose  index  is  1  more  than  the  number 
of  means  required ;  that  is,  the  2d  root  for  one  mean,  the  3d 
root  for  two  means,  the  4th  root  for  three  means,  and  so  on ; 
and  that  root  will  be  the  common  ratio  of  all  the  terms. 


OF  HARJf  OXICAL  PROPORTION* 


121 


Then,  with  the  ratio,  multiply  continually  from  the  first  term, 
or  divide  continually  from  the  last  or  greatest  term. 

EXAMPLE. 

To  find  four  geometrical  means  between  3  and  96. 
Here  3)  96  (32  ;  the  5th  root  of  which  is  2,  the  ratio. 
Then  3X2=6,  dc  6X2=12,  &  t2  X 2=24,  &  24  X2=48. 
Or  96-1-2=48,  <fc  48-^2=24,  &  24^-2=12,  &  12-5-2=6. 
That  is,  6, 12, 24, 48,  are  the  four  means  between  3  and  96. 


f"  OF  HARMONIC AL  PROPORTION. 

There  is  also  a  third  kind  of  proportion,  called  Harmo- 
nical  or  musical,  which  being  but  of  little  or  no  common  use, 
a  very  short  accouut  of  it  may  here  suffice. 

Musical  Proportion  is  when,  of  three  numbers,  the  first 
has  the  same  proportion  to  the  third,  as  the  difference  be- 
tween the  first  and  second  has  to  the  difference  between  the 
second  and  third. 

As  in  these  three,  6,  8,  12  ; 
where  6  :  12  : :  8-6  :  12-8, 
that  is  6  :  12  : :  2  :  1. 

When  four  numbers  are  in  musical  proportion ;  then  the 
first  has  the  same  ratio  to  the  fourth,  as  the  difference  be- 
tween the  first  and  second  has  to  the  difference  between  the 
third  and  fourth. 

As  in  these,  6,  8,  12,  18 ; 
where  6  :  18  :  :  8-6  :  18-12, 
that  is  6  :  18  :  :  2  :  6. 

When  numbers  are  in  musical  progression,  their  recipro- 
cals are  in  arithmetical  progression ;  and  the  converse,  that 
is,  when  numbers  are  in  arithmetical  progression,  their  reci- 
procals are  in  musical  progression. 

So  in  these  musicals  6,  8,  12,  their  reciprocals,  £,  |,  yiy, 
are  in  arithmetical  progression ;  for  ^  +  =  =  i  I 
and  i  +  i  =  |  =  I  ;  that  is,  the  sum  of  the  extremes  is 
equal  to  double  the  mean,  which  is  the  property  of  arithme- 
ticals. 

Vol.  I.  17 


122 


ARITHMETIC. 


The  method  of  finding  out  numbers  in  musical  proportion 
ii  best  expressed  by  letters  in  Algebra. 


FELLOWSHIP,  OR  PARTNERSHIP. 

Fellowship  is  a  rule,  by  which  any  sum  or  quantity  may 
be  divided  into  any  number  of  parts,  which  shall  be  in  any 
given  proportion  to  one  another. 

By  this  rule  are  adjusted  the  gains  or  loss  or  charges  of 
partners  in  company  ;  or  tho  effects  of  bankrupts,  or  lega- 
cies in  case  of  a  deficiency  of  assets  or  effects  ;  or  the  shares 
of  prizes  ;  or  the  numbers  of  men  to  form  certain  detach* 
ments ;  or  the  division  of  waste  lands  among  a  number  of 
proprietors. 

Fellowship  is  either  Single  or  Double.  It  is  single,  when 
the  shares  or  portions  are  to  be  proportional  each  to  one 
single  given  number  only ;  as  when  the  stocks  of  partners 
are  all  employed  for  the  same  time;  and  Double,  when 
each  portion  is  to  be  proportional  to  two  or  more  numbers ; 
as  when  the  stocks  of  partners  are  employed  for  different 
times. 


SINGLE  FELLOWSHIP. 

GENERAL  RULE. 

Add  together  the  numbers  that  denote  tho  proportion  of 
the  shares.    Then  say, 

As  the  sum  of  the  said  proportional  numbers, 

Is  to  the  whole  sum  to  be  parted  or  divided, 

So  is  each  several  proportional  number, 

To  the  corresponding  share  or  part. 
Or,  as  the  whole  stock,  is  to  the  whole  gain  or  loss, 

So  is  each  man's  particular  stock. 

To  his  particular  share  of  the  gain  or  loss. 

To  prove  the  Work.  Add  all  the  shares  or  parts  to- 
gether, and  the  sum  will  be  equal  to  the  whole  number  to  be 
shared,  when  the  work  is  right. 


•XH6UB  FBLLOWSHIP. 


138 


EXAMPLES. 

1.  To  divide  the  number  240  into  three  such  parts,  as 
shall  be  in  proportion  to  each  other  as  the  three  numbers  1, 
Sand  3. 

Here  1  +  2  +  3  =  6,  the  sum  of  the  numbers* 
Then,  as  6  :  240  :  :  1  :   40  the  let  part, 

and  as  6  :  240  :  :  2  :   80  the  2d  part, 

also  as  6  :  240  :  :  8  :  120  the  8d  part. 

Sum  of  all  240,  the  proof. 

2.  Three  persons,  a,  b,  c,  freighted  a  ship  with  840  tuns  of 
wine,  of  which  a  loaded  100  tuns,  n  97,  and  c  the  rest :  in  a 
storm  the  seamen  were  obliged  to  throw  overboard  85  tuns  ; 
how  much  must  each  person  sustain  of  the  loss  ? 

Here    110  +  97  «  207  tuns,  loaded  by  a  and  n  ; 
theref.  340  —  207  =  133  tuns,  loaded  by  c. 

Hence,  as  840  :  85  :  :  110 

or  as  4  :  1  :  :  1 10  :  27|  tuns  =  a's  loss  ; 
and  as  4  :  1  :  :  97  :  24|  tuns  =  b's  loss  ; 
also  as    4  :    1  :  :  133  :  33}  tuns  =  c's  loss  ; 

Sum  85  tuns,  the  proof. 

8.  Two  merchants,  c  and  d,  made  a  stock  of  120/ ;  of 
irbich  c  contributed  757,  and  d  the  rest :  by  trading  they 
gained  30Z ;  what  must  each  have  of  it  ? 

Ans.  c  18/ 15*,  and  d  11/  5*. 

4.  Three  merchants,  b,  f,  g,  make  a  stock  of  700/,  of 
^vhich  b  contributed  128/,  r  358/,  and  o  the  rest :  by  trading 
fihey  gain  125/  10*  ;  what  must  each  have  of  it  ? 

Ans.  b  must  have  22/  Is  Od  2fjq. 
p    ...   64  3  8  Off. 
g    ...    30  5  3  1,V- 

5.  A  General  imposing  a  contribution*  of  700/  on  four 


*  Contribution  it  a  Ui  paid  by  provinces,  towns,  village! ,  Ac.  to  ex- 
xon  them  from  being;  plundered.  It  is  paid  in  provisions  or  in  money, 
*fcd  sometimes  in  both. 


134 


ARITHMETIC. 


villages,  to  be  paid  in  proportion  to  the  number  of  inhabitants 
contained  in  each  ;  the  first  containing  250,  the  2d  350,  the 
3d  400,  and  the  4th  500  persons  ;  what  part  must  each  vil- 
lage pay  ?  Ans.  the  1st  to  pay  116/  13s  Ad 

the  2d  -  -  163  6  8 
the  3d  -  -  186  13  4 
the  4th  -    -    233  '  6  8 

6.  A  piece  of  ground,  consisting  of  37  ac  2  ro  14  ps,  is 
to  be  divided  among  three  persons,  l,  m,  and  n,  in  propor- 
tion to  their  estates  :  now  if  l's  estate  be  worth  5002  a  year, 
m's  320/,  and  n's  75/  ;  what  quantity  of  land  must  each  one 
have  ?  Ans.  l  must  have  20  ac  3  ro  39^} {ps. 

m  -  -  -  13  1  30T\V  *. 
n    -    -    -     3     0  23tf| 

7.  A  person  is  indebted  to  o  57/  15*,  to  r  108/  3s  84,  to 
a  22/  10c/,  and  to  r  73/  ;  but  at  his  decease,  his  effects  are 
found  to  be  worth  no  more  than  170/  14s  ;  how  must  it  be 
divided  among  his  creditors  ? 

Ans.  o  must  have  37/  15*  5c/  2^/^c/. 
p  ...    70  15  2  2^V- 
q  ...    14    8  4  2flftV- 
B  -    -    -    47  14  11  2tWA. 

8.  A  ship,  worth  900/,  being  entirely  lost,  of  which  -J-  be- 
longed to  s,  I  to  t,  and  the  rest  to  v  ;  what  loss  will  each 
sustain,  supposing  540/  of  her  were  insured  ? 

Ans.  s  will  lose  45/,  t  907,  and  v  225/. 

9.  Four  persons,  w,  x,  y,  and  z,  spent  among  them  25*, 
and  agree  that  w  shall  pay  £  of  it,  x  |,  y  },  and  z  j  ;  that 
is,  their  shares  are  to  be  in  proportion  as  £,  |,  J,  and  £  : 
what  are  their  shares  t  Ans.  w  must  pay  9s  8d  3%]q. 

x  -  -  .  6  5  34$. 
y  -  -  -  4  10  14$. 
z  -    .    .  3  10  3,V- 

10.  A  detachment,  consisting  of  5  companies,  being  sent 
into  a  garrison,  in  which  the  duty  required  76  men  a  day  ; 
what  number  of  men  must  be  furnished  by  each  company,  in 
proportion  to  their  strength  ;  the  1st  consisting  of  54  men, 


DOVBU  n&LOWlBXP.  136 

» 

the  2d  of  51  men,  the  3d  of  48  men,  the  4th  of  89,  and  the 
5th  of  36  men? 

Ana.  The  1st  must  furnish  18,  the  2d  17,  the  3d  16,  the 
4th  13,  and  the  5th  12  men41. 


DOUBLE  FELLOWSHIP. 

Doubub  Fkllowbhip,  aa  has  been  said,  is  concerned  in 
cases  in  which  the  stocks  of  partners  are  employed  or  con- 
tinued for  different  times. 

RuLsf. — Multiply  each  person's  stock  by  the  time  of 
its  continuance  ;  then  divide  the  quantity,  aa  in  Single 
Fellowship,  into  shares,  in  proportion  to  these  products],  oy 
saying, 

As  the  total  sum  of  all  the  said  products, 

Is  to  the  whole  gain  or  loss,  or  quantity  to  be  parted, 

So  is  each  particular  product 

To  the  correspondent  share  of  the  gain  or  loss. 


EXAMPLES. 


1.  a  had  in  company  50f  for  4  months,  and  b  had  60J  for 
6  months ;  at  the  end  of  which  time  they  find  242  gained : 
how  roust  it  be  divided  between  them  ? 

Here   50  60 
4  5 

200  +  300  =  500 

Then  as  500  :  24  :  :  200  :  9}  =  91 12*  =  a's  share, 
and  as  500  :  24  :  :  300  :  14f  =  14   8  =  b's  share. 


*  Questions  of  this  nature  frequently  occurring  in  military  service. 
General  Haviland,  an  officer  of  great  merit,  contrived  an  ingenious  in- 
strument, for  more  expeditiously  resolving  them ;  which  is  distinguish- 
ed bv  the  name  of  I  he  inventor,  being  called  a  Haviland. 

t  Th»*  proof  of  this  rule  is  as  follows :  When  the  times  are  equal, 
the  slmres  of  the  gain  or  loss  are  evidently  as  the  stocks,  as  in  Single 
Fellowship;  and  when  the  stocks  are  equal,  the  shares  are  as  the 
times;  therefore,  when  neither  are  equal,  the  shares  must  be  esthete 
products. 


196 


ABTTH3CKTIC. 


2.  c  and  d  hold  a  piece  of  ground  in  common,  for  which 
they  are  to  pay  542.  c  put  in  23  horses  for  27  days,  and  d 
21  horses  for  30  days ;  how  much  ought  each  man  to  pay 
of  the  rent  ?  .  Ans.  c  must  pay  23/  5*  9d. 

d  must  pay  30  14  3. 

3.  Three  persons,  e,  f,  o,  hold  a  pasture  in  common, 
for  which  they  are  to  pay  30/  per  annum ;  into  which  e  put 
7  oxen  for  3  months,  f  put  9  oxen  for  5  months,  and  o  put 
in  4  oxen  for  12  months ;  "how  much  must  each  person  pay 
of  the  rent  1  Ans.  e  must  pay  57  10*  Gd  lftq. 

f  ..  11  16  10  0^V 
o    -   -    12  12  7  2ft. 

4.  A  ship's  company  take  a  prize  of  1000/,  which  they 
agree  to  divide  among  them  according  to  thejr  pay  and  the 
time  they  have  been  on  board  :  now  the  officers  and  midship- 
men have  been  on  board  6  months,  and  the  sailors  3  months ; 
the  office  re  have  40*  a  month,  the  midshipmen  30*,  and  the 
sailors  22*  a  month  ;  moreover,' there  are  4  officers,  12  mid- 
shipmen,  and  110  sailors  ;  what  will  each  man's  share  be  ? 

Ans.  each  officer  must  have  231 2s  5d  0  Yy^q. 
each  midshipman    -    17  6  9  3^. 
each  seaman     -    -     6  7  2  0fo\. 

5.  r,  with  a  capital  of  1000/,  began  trade  the  first  of 
January,  and,  meeting  with  success  in  business,  took  in  i  as 
a  partner,  with  a  capital  of  1500/,  on  the  first  of  March  fol- 
lowing. Three  months  after  that  they  admit  k  as  a  third 
partner,  who  brought  into  stock  2K007.  After  trading  toge- 
ther till  the  end  of  the  year,  they  find  there  has  been  gained 
1776/  10s ;  how  must  this  be  divided  among  the  partners  ? 

Ans.  h  must  have  475/  9s  A\d  j^q* 
i  571  16  8J 

k  -    .   -    747  3  11J  iff. 

6.  x,  y,  and  z  made  a  joint  stock  for  12  months ;  x  at 
first  put  in  20/,  and  4  months  after  20/  more  ;  y  put  in  at 
first  30/,  at  the  end  of  3  months  he  put  in  20/  more,  and  2 
months  after  he  put  in  407  more ;  z  put  in  at  first  60/,  and 
5  months  after  he  put  in  10/  more,  1  month  after  which  he 
took  out  30/ ;  during  the  12  months  they  gained  50/  ;  how 
much  of  it  must  each  have  ? 

Ans.  x  must  have  10/  18s  6d  3}  fa. 
y    ...  22    8  1  0ft. 
z    ...   16  13  4  0. 


SIMPLE  onraBST. 


SIMPLE  INTEREST. 


Interest  is  the  premium  or  sum  allowed  for  the  loan,  or 
forbearance  of  money.  The  money  lent,  or  forborn,  is 
called  the  Principal ;  and  the  sum  of  the  principal  and  its  x 
interest  added  together,  is  called  the  Amount.  Interest  is 
allowed  at  so  much  per  cent,  per  annum  ;  which  premium 
per  cent,  per  annum,  or  interest  of  100/  for  a  year,  is1  called 
the  rale  of  interest : — So, 

When  interest  is  at  3  per  cent,  the  rate  is  3 ; 

-  4  per  cent.  -  -  -  4 ; 
.    5  per  cent.    -    -    -  5 ; 

-  6  per  cent.    ...  6. 

But,  by  law,  interest  ought  not  to  be  taken  higher  than  at 
the  rate  of  5  per  cent. 

Interest  is  of  two  sorts  ;  Simple  and  Compound. 

Simple  Interest  is  that  which  is  allowed  for  the  principal 
lent  or  forborn  only,  for  the  whole  time  of  forbearance* 
As  the  interest  of  any  sum,  for  any  time,  is  directly  pro- 
portional to  the  principal  sum,  and  also  to  the  time  of  con- 
tinuance ;  hence  arises  the  following  general  rule  of  calcu- 
lation. 

As  100Z  is  to  the  rate  of  interest,  so  is  any  given  principal 
to  its  interest  for  one  year.    And  again, 

As  1  year  is  to  any  given  time,  so  is  the  interest  for  a 
year,  just  found,  to  the  interest  of  the  given  sum  for  that 
time. 

Otherwise.  Take  the  interest  of  1  pound  for  a  year, 
which  multiply  by  the  given  principal,  and  this  product 
again  by  the  time  of  loan  or  forbearance,  in  years  and  parts, 
for  the  interest  of  the  proposed  sum  for  that  time. 

Note.  When  there  are  certain  parts  of  years  in  the  time, 
as  quarters,  or  months,  or  days  :  they  may  be  worked  for, 
either  by  taking  the  aliquot  or  like  parts  of  the  interest  of  a 
year,  or  by  the  Rule  of  Three,  in  the  usual  way.  Also,  to 
divide  by  100,  is  done  by  only  pointing  off  two  figures  Cot 
decimals. 


138 


ASfHDtBTXG. 


EXAKPLK8. 


1.  To  find  the  interest  of  2801 10«,  for  1  year,  at  the  rate 
of  4  per  cent,  per  annum.„ 

Here,  As  100  :  4  ::  230/  10*  :  97  4*  4Jd. 

4 


100)  0,22  0 
20 

4-40 
12 

4  80        t  Ans.  01  4s  4f<*. 


3*20 


2.  To  find  the  interest  of  547/ 15*,  for  3  years,  at  5  per 
cent,  per  annum. 

As  100  :  5  ::  547-75 

Or  20  :  1  ::  547*75  :  27-3875  interest  for  1  year. 

3 


I  82-1625  ditto  for  3  years. 
20 


s  3-2500 
12 


<2  3-00   Ans.  82/  3*  3d. 


3.  To  find  the  interest  of 200  guineas,  for  4  years  7  months 
and  25  days,  at  4$  per  cent,  per  annum. 


SIMPLE  INTEREST. 


129 


ds      2  ds 
<  8102        As  356:  9-45:  :  25:  2 
41        or    73:9-45::  5  : -6472 

  5 

340   

105  73)  47-25  (-6472 

  345 

9-45  interest  for  1  yr.  530 
4  19 


37*80    ditto  4  years. 
6  mo  =  \  4*725  ditto  6  months. 
1  mo  =  £  -7875  ditto  1  month. 

-6472  ditto  25  days. 

I  43-9597 
20 


* 191940 
12 


d  2-3280 

4      Ans.  432 19*  2\d. 


q  1-3120 


4»  To  find  the  interest  of  450/,  for  a  year,  at  5  per  cent, 
per  annum.  Ans.  222 10*. 

5.  To  find  the  interest  of  7152 12*  6c2,  for  a  year,  at  41 
per  cent,  per  annum.  Ans.  322  4*  0}a. 

6.  To  find  the  interest  of  7202,  for  3  years,  at  5  per  cent 
per  annum.  Ans.  1082. 

7.  To  find  the  interest  of  3552 15*,  for  4  years,  at  4  per 
cent  per  annum.  Ans.  562  18*  4Jd. 

-  8.  To  find  the  interest  of  322  5*  Bd9  for  7  years,  at  4£  per 
cent  per  annum.  Ans.  92  12*  Id. 

9.  To  find  the  interest  of  1702,  for  1}  year,  at. 5  per  cent 
per  annum.  Ans.  122  15** 

10.  To  find  the  insurance  on  2052  15*,  for  J  of  a  year,  at 
4  per  cent,  per  annum.  Ans.  22  1*  lf<f. 

11.  To  find  the  interest  of  3192  6d,  for  5?  years,  at  3|  per 
cent,  per  annum.  Ans.  682  14*  9|<2. 

12.  To  find  the  insurance  on  1072,  for  117  days,  at  4f  per 
cent  per  annum.  Ana.  U  \fe  Id* 

Vol.  I.  18 


180 


ARITHMETIC 


13.  To  find  the  interest  of  172  5*,  for  117  days,  at  4f  per 
cent,  per  annum.  Ans.  5*  3d. 

It  To  find  the  insurance  on  7122  6s,  for  8  months,  at  71 
per  cent,  per  annum.  Ans.  352  1£#  3J<£ 

Note.  The  Rules  for  Simple  Interest,  serve  also  to  calcu- 
late Insurances,  or  the  Purchase  of  Stocks,  or  any  thing  else 
that  is  rated  at  so  much  per  cent. 

See  also  more  on  the  subject  of  Interest,  with  the  algebrai- 
cal expression  and  investigation  of  the  rules  at  the«adof  the 
Algebra. 


COMPOUND  INTEREST. 

Compound  Interest,  called  also  Interest  upon  Interest, 
is  that  which  arises  from  the  principal  and  interest,  taken 
together,  as  it  becomes  due,  at  the  end  of  each 'stated  time 
of  payment.  Though  it  be  not  lawful  to  lend  money  at 
Compound  Interest,  yet  in  purchasing  annuities,  pensions,  or 
leases  in  reversion,  it  is  usual  to  allow  Compound  Interest  to 
the  purchaser  for  his  ready  money. 

Rules. — 1.  Find  the  amount  of  the  given  principal,  for 
the  time  of  the  first  payment,  by  Simple  Interest.  Their 
consider  this  amount  as  a  new  principal  for  the  second  pay- 
ment, whose  amount  calculate  as  before.  And  so  on  through 
all  the  payments  to  the  last,  always  accounting  the  last  amount 
as  a  new  principal  for  the  next  payment.  The  reason  of 
which  is  evident  from  the  definition  of  Compound  Interest* 
Or  else, 

2.  Find  the  amount  of  1  pound  for  the  time  of  the  first 
payment,  and  raise  or  involve  it  to  the  power  whose  index 
is  denoted  by  tho  number  of  payments.  Then  that  power 
multiplied  by  the  given  principal,  will  produce  the  whole 
amount.  From  which  the  said  principal  being  subtracted, 
leaves  the  Compound  Interest  of  the  same.  As  is  evident 
from  the  first  Rule. 

EXAMPLES. 

1.  To  find  the  amount  of  720/,  for  4  years,  at  5  per  cent* 
per  annum. 

Here  5  is  the  20th  part  of  100,  and  the  interest  of  H  for  a 
year  is  -fa  or  *95,  and  its  amount  1*05.  Therefore, 


ALLIGATION. 


1.  By  ike  lit  Rtde.  2.  By  the  2d  Rule. 

I     s    d  1*05  amount  of  1Z. 

SO)  720   0   0   1st  yr's  princip.         1-05  * 

88   0   0    1st  yr*s  interest.       ,  tnCTe 

 J  1  1026  2d  power  of  it. 

20)756   0  0   2d  yr*s  princip.  1-1025 

97  16   0   2d  yr's  interest.-———-:^ , 
  J  1  -21550625  4th  power  of  it. 

SO)  703  16   0   3d  yr's  princip.  720 

30  13   9h  3d  yr's  interest  y 

20)  838   9   9J  4th  yr's  princip.  20 
41  13   5}  4thfr'8int«e,t.  ~~ 

£875   3   3}  the  whole  amou  12 
 or  ans.  required. 


2.  To  find  the  amount  of  502  in  5  years,  at  5  per  cent, 
per  annum,  compound  interest.  Ans.  032  16*  8jtf. 

3.  To  find  the  amount  of  50Z  in  5  years,  or  10  half-years, 
at  5  per  cent,  per  annum,  compound  interest,  the  interest 
payable  half-yearly.  Ans.  64Z  0*  Id. 

4  To  find  the  amount  of  50Z  in  5  years,  or  20  quarters, 
at  5  per  cent,  per  annum,  compound  interest,  the  interest 
payable  quarterly.  Ans.  04/  2s  (){d. 

5.  To  find  the  compound  interest  of  370Z  forborn  for  6 
years,  at  4  percent,  per  annum.  Ans.  98Z  3*  4£<Z. 

6.  To  find  the  compound  interest  of  41 OZ  forborn  for  2* 
years,  at  4£  per  cent,  per  annum,  the  interest  payable  half, 
yearly.  Ans.  48Z  4*  11  {d* 

7.  To  find  the  amount,  at  compound  interest,  of  217Z,  for* 
born  at  2{  years,  at  5  per  cent,  per  annum,  the  interest  pay- 
able quarterly.  Ans.  242/ 13*  4£rf. 


ALLIGATION. 

Alligation  teaches  how  to  compound  or  mix  together 
several  simples  of  different  qualities,  so  that  the  composition 
•nay  be  of  some  intermediate  quality,  or  rate.  It  is  com- 
monly distinguished  into  two  cases.  Alligation  Medial,  and 
Alligation  Alternate. 


1*2 


AS1THXXTIC. 


^  ALLIGATION  MEDIAL. 

Alligation  Medial  is  the  method  of  finding  the  rate  or 
quality  of  the  composition,  from  having*  the  quantities  and 
rates  or  qualities  of  the  several  simples  given.  And  it  is 
thus  performed : 

*  Multiply  the  quantity  of  each  ingredient  by  its  rate  or 

Siality  ;  then  add  all  the  products  together,  and  add  also  all 
e  Quantities  together  in  another  sum  ;  then  divide  the 
former  sum  by  the  latter,  that  is,  the  sum  of  the  products  by 
the  sum  of  the  quantities,  and  the  quotient  will  be  the  rate  or 
quality  of  the  composition  required. 

EXAMPLES. 

1.  If  three  sorts  of  gunpowder  be  mixed  together,  viz. 
601b  at  I2d  a  pound,  441b  at  9d,  and  261b  at  8d  a  pound  ; 
how  much  a  pound  is  the  composition  worth  ? 
Here  50,  44,  26  are  the  quantities, 
and    12,  9,  8  the  rates  or  qualities  ; 
then  50  X  12  =  600 
44  X    9  =  396 
26  X    8  =  208 

120)  1204       (lOrfr  =  10fV- 

Ans.  The  rate  or  price  is  lO^d  the  pound. 


•  Demonstration.   The  Rule  is  thus  proved  by  Algebra. 
Let  a,  6,  e  be  the  quantities  of  the  ingredients, 
and  m,  n,  p  their  rates,  or  qualities,  or  prices ; 
then  am,  in,  cp  are  their  several  values, 
and  am  +  bn  -\-  cp  the  sum  of  their  values, 
also  «  +  b  +  e  is  the  sum  of  the  quantities, 
and  if  r  denote  the  rate  of  the  whole  composition, 
then  (ff-f-6-fc)Xr  will  be  the  value  of  the  whole, 
conseq.  {a  -f  b  4-  c)  X  r  =  am  +  bn  +  cp, 
and  r  =  (am  -f  bn  +  cp)     (a  +  b  -f-  c),  u  hich  is  the  Rule. 

Note.  If  an  ounce  or  any  other  quantity  of  pure  gold  be  reduced 
into  94  equal  parts,  these  parts  are  called  Caracts ;  but  gold  is  often 
mixed  with  some  base  metal,  which  is  called  the  Alloy,  and  the  mixture 
is  said  to  be  of  so  many  caracts  fine,  according  to  the  proportion  of  para 

Kid  contained  in  it :  thus,  if  522  caracts  of  pure  gold,  and  2  of  a) Joy 
mixed  together,  it  is  said  to  be  32  caracts  fine. 
If  any  one  of  the  simples  be  of  little  or  no  value  with  respect  to  the 
rail,  its  rate  is  supposed  to  be  nothing  ;  as  water  mixed  with  wine,  and 
alloy  with  gold  and  silver. 


AU.IGATION  ALTERNATE. 


138 


2.  A  composition  being  made  of  51b  of  tea  at  7s  per  lb, 
91b  at  8*  64  per  lb,  and  14£lb  at  5*  lOd  per  lb  ;  what  is  a  lb 
of  it  worth?  Ana.  6*  I0\d. 

3.  Mixed  4  gallons  of  wine  at  4s  lOd  per  gall,  with  7  gal- 
Ions  at  5#  3d  per  gall,  and  9}  gallons  at  6*  Sd  per  gall ;  what 
is  a  gallon  of  this  composition  worth  ?  Ans.  5*  4{d» 

4.  Having  melted  together  7  oz  of  gold  of  22  caracts  fine, 
12 1  oz  of  21  caracts  fine,  and  17  oz  of  19  caracts  fine  :  I 
would  know  the  fineness  of  the  composition  ? 

Ans.  2(ty$  caracts  fine. 


ALLIGATION  ALTERNATE. 

Alligation  Alternate  is  the  method  of  finding  what 
quantity  of  any  number  of  simples,  whose  rates  are  given, 
will  compose  a  mixture  of  a  given  rate.  So  that  it  is  the  re- 
verse of  Alligation  Medial,  and  may  be  proved  by  it. 

RULE  i*. 

1.  Set  the  rates  of  the  simples  in  a  column  under  each 
other. — 2.  Connect,  or  link  with  a  continued  lino,  the  rate 


*  Demonst.  By  connecting  the  less  rate  with  the  greater,  and  placing 
the  difference  between  them  and  the  rate  alternately,  the  quantities  re- 
sulting are  such,  that  there  is  precisely  as  much  gained  by  one  quantity 
as  is  Inst  by  the  other,  and  therefore  the  gain  and  loss  upon  the  whole 
is  equal,  and  is  exactly  the  proponed  rate  :  and  the  same  will  be  true  of 
any  other  two  simples  managed  according  to  the  Rule. 

In  like  manner,  whatever  the  number  of  simples  may  be,  and  with 
how  many  soever  every  one  is  linked,  since  it  is  always  a  le^s  with  a 
greater  than  the  mean  price,  there  will  be  an  equal  balance  of  loss  and 
gain  between  every  two,  and  consequeutly  an  equal  balance  on  the 
whole.       s.  d. 

It  is  obvious,  from  the  Rule,  that  questions  of  this  sort  admit  of  a 
great  variety  of  answers ;  for,  having  found  one  answer,  we  may  find 
as  many  more  as  we  please,  by  only  multiplying  or  dividing  each  of 
the  quantities  found,  by  2,  or  3,  or  4,  fee. :  the  reason  of  which  is  evi- 
dent: for,  if  two  quantities,  of  two  simples,  make  a  balance  of  loss  and 
gain,  with  respect  to  the  mean  price,  so  must  also  the  double  or  treble, 
the  1  or  |  part,  or  any  other  ratio  of  these  quantities,  and  so  on  ad  w- 
Jutiltm. 

These  kinds  of  questions  are  called  by  algebraists  indeterminate  or 
unlimited  problems ;  and  by  an  analytical  process,  theorems  may  be 
raited  that  will  give  all  the  possible  answers. 


184 


ASmULETlG. 


of  each  simple,  which  is  less  than  that  of  the  compound,  with 
one,  or  any  number,  of  those  that  are  greater  than  the  com- 
pound*; and  each  greater  rate  with  one  or  any  number  of  the 
less.— -3.  Write  the  difference  between  the  mixture  rate,  and 
that  of  each  of  the  simples,  opposite  the  rate  with  which  they 
are  linked. — 4.  Then  if  only  one  difference  stand  against 
any  rate,  it  will  be  the  quantity  belonging  to  that  rate  ;  but 
if  there  be  several,  their  sum  will  be  the  quantity. 

The  examples  may  be  proved  by  the  rule  for  Alligation 
Medial. 


EXAMPLES. 

1.  A  merchant  would  mix  wines  at  16*,  at  18*,  and  at  22* 
per  gallon,  so  as  that  the  mixture  may  be  worth  20*  the  gal- 
lon ;  what  quantity  of  each  must  be  taken  ? 

1 2  at  16* 
Here  20  ?J8>v   J2  at  18* 

(22j/4  +  2  =  6at  22* 

2.  How  much  sugar  at  4d,  at  6d,  and  at  lid  per  lb,  must 
be  mixed  together,  so  that  the  composition  formed  by  them 
may  be  worth  7d  per  lb  ? 

Ans.  1  lb,  or  1  stone,  or  1  cwt,  or  any  other  equal  quan- 
tity of  each  sort. 

3.  How  much  corn  at  2*  6d,  3*  Sdy  4*,  and  4*  8d  per 
bushel  must  be  mixed  together,  that  the  compound  may  be 
worth  3*  lOd  per  bushel  ? 

Ans.  2  at  2*  6d,  3  at  3*  8d,  3  at  4*,  and  3  at  4*  Sd. 

RULE  II. 

When  the  whole  composition  is  limited  to  a  certain  quan- 
tity :  Find  an  answer  as  before  by  linking  ;  then  say,  as 
the  sum  of  the  quantities,  or  differences  thus  determined,  is 
to  the  givm  quantity  ;  so  is  each  ingredient,  found  by  link- 
ing, to  the  required  quantity  of  each. 

EXAMPLE. 

1.  How  much  gold  of  15,  17,  18,  and  22  caracts  fine,  mutt 
be  mixed  together,  to  form  a  composition  of  40  oz  of  20  cap 
racta  fino  ? 


ALLIGATION  AI/TlHUVATE. 


135 


-  2 

Here  20?  l^M  )-      .       .  2 

5  +  3+  2=10 
16 

Then  as  10  :  40  : :  2  :  5 
and  16  :  40  : :  10  :  25 
Ans.  5  oz  of  15,  of  17,  and  of  18  caracts  fine,  and  25  oz  of 
22  caracts  fine*. 

rule  inf.  t 

When  one  of  the  ingredients  is  limited  to  a  certain  quan- 
tity ;  Take  the  difference  between  each  price,  and  the  mean 
rate  as  before ;  then  say,  As  the  difference  of  that  simple, 
whose  quantity  is  given,  is  to  the  rest  of  the  differences 
severally ;  so  is  the  quantity  given,  to  the  several  quantities 
required. 


*  A  great  number  of  questions  might  be  here  given  relating  to  the 
specific  gravities  of  metals,  &c.  but  one  of  the  most  curious  may  suf- 
fice. 

Hiero,  king  of  Syracuse,  gave  orders  for  a  crown  to  be  made  entire- 
ly of  pure  gold  ;  but  suspecting  the  workmen  had  debased  it  by  mixing 
it  with  silver  or  copper,  be  recommended  the  discovery  of  the  fraud  to 
the  famous  Archimedes,  and  desiied  to  know  the  exact  quantity  of  alloy 
in  the  crown. 

Archimedes,  in  order  to  detect  the  imposition,  procured  two  other 
masses,  the  one  of  pure  gold,  the  other  of.  silvei  or  copper,  and  each  ot 
the  same  weight  with  the  former;  and  by  putting  each  separately  into 
a  vessel  full  of  water,  the  quantity  of  water  expelled  by  them  deter- 
mined their  specific  gravities :  from  which,  and  their  givr»n  weights,  the 
exact  quantities  of  gold  and  alloy  in  the  crown  may  be  determined. 

Suppose  the  weight  of  each  crown  to  be  101b,  and  that  the  water  ex- 
pelled by  the  copper  or  silver  was  921b,  by  the  gold  5*2 lb,  and  by  the 
compound  crown  C4lb  ;  what  will  be  the  quantities  of  gold  and  alloy 
Id  the  crown  ? 

The  rates  of  the  simples  are  92  and  52,  und  of  the  compound  64 ; 
therefore 

CxA  I  62  >  12  of  copper 

°*  I  62... ^28  of  gold 
And  the  sum  of  these  is  12  +  28  —  40,  which  should  have  been  10; 
therefore  by  the  Rule, 

40  :  10  ::  12 :  31b  of  copper  „„,„,„, 
40:  10:  :28  :  71b  of  «olJ     Jthe  answer 
t  Id- the  very  same  manner  questions  may  be  wrought  when  several 
•iof  the  ingredients  are  limited  to  certain  quantities,  by  finding  first  fur 
one  limit,  and  then  for  another.   The  two  last  Rules  can  need  do  de- 
monstration, as  they  evidently  result  from  the  first,  the  reason  ut 
has  been  already  explained. 


186 


ABTTHXBTIC 


EXAMPLES. 


1.  How  much  wine  at  6*,  at  5*  64,  and  6*  the  gallon,  must 
be  mixed  with  3  gallons  at  4*  per  gallon,  so  that  the  mixture  - 
may  be  worth  5*  4d  per  gallon  ? 


16+4=20 

Then  10  :  10  : :  3  :  3 
10  :  20  : :  3  :  6 
10:20::3:6 
Ads.  3  gallons  at  5*,  6  at  5s  6d9  and  6  at  6*. 
2.  A  grocer  would  mix  teas  at  12*,  10*,  and  6*  per  lb,  with 
201b  at  4s  per  lb :  how  much  of  each  sort  must  he  take  to 
make  the  composition  worth  8*  per  lb  ? 

Ans.  201b  at  4*,  101b  at  6*,  101b  at  10*,  and  201b  at  12*. 


Position  is  a  rule  for  performing  certain  questions,  which 
cannot  be  resolved  by  the  common  direct  rules.    It  is  some- 
times called  False  Position,  or  False  Supposition,  because 
it  makes  a  supposition  of  false  numbers,  to  work  with  the 
same  as  if  they  were  the  true  ones,  and  by  their  means  dis- 
covers the  true  numbers  sought.    It  is  sometimes  also  called  i 
Trial-and-Error,  because  it  proceeds  by  trials  of  f  ilse  num-  j 
bers,  and  thence  finds  out  the  true  ones  by  a  comparison  ^ 
of  the  errors. — Position  is  either  Single  or  Double. 


Single  Position  is  that  by  which  a  question  is  resolved 
by  means  of  one  supposition  only.  Questions  which  have 
their  result  proportional  to  their  supposition,  belong  to 
Single  Position  :  such  as  those  which  require  the  multiplier 


POSITION. 


SINGLE  POSITION. 


SINGLE  POSITION. 


137 


tion  or  division  of  the  number  sought  by  any  proposed  num- 
ber ;  or  when  it  is  to  be  increased  or  diminished  by  itself, 
or  any  parts  of  itself,  a  certain  proposed  number,  of  times. 
The  rule  is  as  follows  : 

Take  or  assume  any  number  for  that  which  is  required, 
and  perform  the  same  operations  with  it,  as  are  described  or 
performed  in  the  question.  Then  say,  As  the  result  of  the 
said  operation,  is  to  the  position,  or  number  assumed  ;  so  is 
the  result  in  the  question,  to  a  fourth  term,  which  will  be 
the  number  sought*. 


EXAMPLES. 


1.  A  person  after  spending  J-  and  {  of  his  money,  has  yet 
remaining  60/  ;  what  had  he  at  first  ? 

Suppose  he  had  at  first  1201.  Proof. 
Now  {  of  120  is  40  £  of  144  is  48 

J  of  it  is     30  i  of  144  is  36 

their  sum  is    70  their  sum  84 

which  taken  from  120  taken  from    1 14 

leaves    50  leaves  (50  as 

Then,  50  :  120  :  :  60  :  144  the  Answer.        per  question. 

2.  What  number  is  that,  which,  being  increased  by  »,  J, 
and  i  of  itself,  the  sum  shall  be  75?  Ans.  36. 

3.  A  general,  after  sending  out  a  foraging  i  and  £  of  his 
men,  had  yet  remaining  1000;  what  number  had  he  in 
command  ?  Ans.  6000. 

4.  A  gentleman  distributed  52  pence  among  a  number  of 
poor  people,  consisting  of  men,  women,  and  children ;  to 
each  man  he  gave  6d,  to  each  woman  4d,  and  to  each  child 
2d :  moreover  there  were  twice  as  many  women  as  men,  and 


*  The  reason  of  this  Kale  is  evident,  because  it  is  supposed  that  the 
results  are  proportional  to  the  suppositions. 

Thus,  na  :  a  :  :  nz  :  s, 


— h  —  «fcc. 

n  —  m 


a 

or 

-  :  a  : 

n 

a  a 

or 

-  - 

n —  m 

and  so  on. 
Vol.  I.  19 


138 


AJCXTHMCTTC. 


thrice  as  many  children  as  women.  How  many  were  them 
of  each  ?  Ana.  2  men,  4  women,  and  12  children. 

ft.  One  being  aaked  his  age,  said,  if  f  of  the  years  I  have 
lived,  be  multiplied  by  7,  and  §  of  them  be  added  to  the 
product,  the  sum  will  be  210.   What  was  his  age  ? 

Ana.  45  yeanr. 


DOUBLE  POSITION. 

Double  Position  is  the  method  of  resolving  certain  ques- 
tions by  means  of  two  suppositions  of  false  numbers. 

To  the  Double  Rule  of  Position  belong  such  questions  as 
have  their  results  not  proportional  to  their  positions :  such  are 
those  in  which  the  numbers  sought,  or  their  parts*  or  their 
multiples,  are  increased  or  diminished  by  some  given  absolute 
number,  which  is  no  known  part  of  the  number  sought, 

bulk*. 

Take  or  assume  any  two  convenient  numbers,  and  pro- 
ceed with  each  of  them  separately,  according  to  the  con- 


*  Dcmonstr.  The  Rule  is  founded  on  this  supposition,  namely,  tbet 
the  first  error  is  to  the  second,  as  the  difference  between  the  true  and 
first  supposed  number,  is  to  the  difference  between  the  true  end  second 
supposed  number:  when  that  is  not  the  case,  the  exact  answer  to  the 
question  cannot  be  found  by  this  Rule.— That  the  Rule  is  true,  accord- 
ing to  the  assumption,  may  be  thus  proved. 

Let a  and  6  be  the  two  suppositions,  and  A  and  a  their  results,  pro- 
duced by  similar  operation ;  also  r  and  s  their  errors,  or  the  differences 
between  the  results  a  and  a  from  the  true  result  a ;  and  let  x  denote 
the  number  sought,  answeriog  to  the  true  result  a  of  the  question. 

Then  is  k  —  a  =  r,  and  k  —  b  ~  #,  or  b  —  a  =  r— s.  Andr according 
to  the  supposition  on  which  the  Rule  is  founded,  r  :  s  ::  x  —  a :  x— 6 ; 
hence,  by  multiplying  extremes  and  means,  rx  —  rb  =  sx—  as;  then,  by 

transposition,  rx  —  #x  =  rb  —  $a ;  and,  by  division,  x  =  r^~~*g  =  the 

number  sought,  which  is  the  rule  when  the  results  are  both  too  little. 

If  the  results  be  both  too  great,  so  that  ▲  and  a  are  both  mater  than 
h  ;  then  h  —  a  =  — r,  and  a  —  a  =  —  *,  or  r  and  s  are  both  negative ; 
hence—  r  :  —  t  :  :  x  —  a  :  x— bf  but  —  r  :  —  $  t  r  -f  r  :  -4-  *,  there- 
fore r  :  s  :  :  x—a  :  x—b  \  and  the  rest  wHI  be  exactly  as  in  the  for- 
mer case. 

But  if  one  result  a  only  be  too  little,  and  the  other  a  too  great,  or 
one  error  r  positive,  and  the  other  »  negative,  then  the  theorem  be- 
comes x  =  ^4— t  which  is  the  rule  in  this  case,  or  whea  the  errors 
are  unlike. 


DOVBU  POSITION. 


180 


Virions  or  the  question,  as  in  Single  Position  ;  and  find  how 
enuch  each  remit  is  different  from  the  result  mentioned  in 
the  question,  calling  these  differences  the  errors,  noting  also 
whether  the  results  are  too  great  or  too  little. 

Then  multiply  each  of  the  said  errors  by  the  contrary 
supposition,  namely,  the  first  position  by  the  second  error, 
and  the  second  position  by  the  first  error.  Then, 

If  the .  errors  are  alike,  divide  the  difference  of  the  pro- 
ducts by  the  difference  of  the  errors,  and  the  quotient  will 
lie  the  answer. 

But  if  the  errors  are  unlike,  divide  the  sum  of  the  pro- 
ducts by  the  sum  of  the  errors,  for  the  answer. 

Note,  The  errors  are  said  to  be  alike,  when  they  are  either 
both  too  great  or  both  too  little  ;  and  unlike,  when  one  is 
too  great  and  the  other  too  little. 


SXAMPLB. 

1*  What  number  is  that,  which  being  multiplied  by  6,  the 
product  increased  by  18,  and  the  sum  divided  by  9,  the  quo- 
tient should  be  20  ? 

Suppose  the  two  numbers  18  and  30.  Then, 


First  Position.             8econd  Position. 
18   Suppose  30 
6   mult.  6 

ProoC 
27 
6 

108 
18 

add 

180 
18 

162 
18 

*)  126 

div. 

9)  198 

-0)  180 

14 

20 

results 
true  res. 

22 
20 

20 

:2d  pos. 

80 

errors  unlike 
mult. 

-2 

18  1st  pos. 

Er.  >2 
jorsyC 

\  180 

\  36 

36 

sum  8) 

216 
27 

sum  of  products 
Answer  sought. 

140 


ARITHMETIC. 


RULE  II. 

Find,  by  trial,  two  numbers,  as  near  the  true  number  as 
convenient,  and  work  with  them  as  in  the  question  ;  mark- 
ing the  errors  which  arise  from  each  of  them. 

Multiply  the  difference  of  the  two  numbers  assumed,  or 
found  by  trial,  by  one  of  the  errors,  and  divide  the  product 
by  the  difference  of  the  errors,  when  they  are  alike,  but  by 
their  sum  when  they  are  unlike.  Or  thus,  by  proportion  : 
As  the  difference  of  the  errors,  or  of  the  results,  (which  is 
the  same  thing),  is  to  the  difference  of  the  assumed  numbers, 
so  is  either  of  the  errors,  to  the  correction  of  the  assumed 
number  belonging  to  that  error. 

Add  the  quotient,  or  correction,  last  found,  to  the  number 
belonging  to  the  said  error,  when  that  number  is  too  little, 
but  subtract  it  when  too  great,  and  the  result  will  give  the 
true  quantity  sought  *. 

EXAMPLES. 

1.  So,  the  foregoing  example,  worked  by  this  2d  rule, 
will  be  as  follows  : 

30  positions  18  ;  their  diff.  12 

-2  errors    +6 ;  least  error  2 

sum  of  errors  8 )  24  (  3  subtr. 
from  the  position  30 

leaves  the  answer  27 

Or,  as  22  -  14  :  30  -  18,  or  as  8  :  12  : :  2  :  3  the  cor- 
rection, as  above. 

2.  A  son  asking  his  father  how  old  he  was,  received  this 
answer  :  Your  age  is  now  one-third  of  mine  ;  but  5  years 
ago,  your  age  was  only  one-fourth  of  mine.  What  then  are 
their  two  ages  ?  Ans.  15  and  45. 

3.  A  workman  was  hired  for  20  days,  at  3s  per  day,  for 
every  day  he  worked  ;  but  with  this  condition,  that  for  every 
day  he  did  not  work,  he  should  forfeit  1*.    Now  it  so  hap. 


•  For  since,  by  the  supposition,  r  :  t ::  x  :  —  a:x  —  b,  therefore  by 
division,  r — f :  s  ::  b —  a:  z  — 6,  or  as  b  —  a  :  6  —  a  : :  s  :x  —  6,  for  b 
—  a  if  =  r — $ :  which  is  the  2d  Rule. 


PRACTICAL  QUESTIONS. 


141 


pened,  that  upon  the  whole  he  had  27  4*  to  receive.  How 
many  of  the  days  did  he  work  ?  Ans.  16* 

4.  a  and  b  began  to  play  together  with  equal  sums  of 
money:  a  first  won  20 guineas,  but  afterwards  lost  back} 
of  what  he  then  had  ;  after  which  b  had  four  times  as  much 
as  a.    What  sum  did  each  begin  with  ?    Ans.  100  guineas. 

5.  Two  persons,  a  and  b,  have  both  the  same  income, 
a  saves  }  of  his  ;  but  b,  by  spending  60/  per  annum  more 
than  a,  at  the  end  of  4  years  finds  himself  100/  in  debt. 
"What  does  each  receive  and  spend  per  annum  ? 

Ans.  They  receive  125/  per  annum  ;  also  a  spends  100/, 
and  b  spends  150/  per  annum. 


PRACTICAL  QUESTIONS  IN  ARITHMETIC. 

Quest.  1.  The  swiftest  velocity  of  a  cannon-ball,  is 
about  2000  feet  in  a  second  of  time.  Then  in  what  time, 
at  that  rate,  would  such  a  ball  move  from  the  earth  to  the 
sun,  admitting  the  distance  to  be  100  millions  of  miles,  and 
the  year  to  contain  365  days  6  hours  ?     Ans.  8  tVtVV  years. 

Quest.  2.  What  is  the  ratio  of  the  velocity  of  light  to 
that  of  a  cannon-ball,  which  issues  from  the  gun  with  a  ve- 
locity of  1500  feet  per  second  ;  light  passing  from  the  sun 
to  the  earth  in  7£  minutes  ?  Ans.  the  ratio  of  782222$  to  1. 

Quest.  3.  The  slow  or  parade-step  being  70  paces  per 
minute,  at  28  inches  each  pace,  it  is  required  to  determine 
at  what  rate  per  hour  that  movement  is  ?     Ans.  miles. 

Qukht.  4.  The  quick-time  or  step,  in  marching,  being 
2  paces  per  second,  or  120  per  minute,  at  28  inches  each ; 
at  what  rate  per  hour  does  a  troop  march  on  a  rout,  and 
how  long  will  they  be  in  arriving  at  a  garrison  20  miles 
distant,  allowing  a  halt  of  one  hour  by  the  way  to  refresh  ? 

.  )  the  rate  is  3^T  miles  an  hour. 
'  \  and  the  time  7$  hr,  or  7h  17|  min. 
Quest.  5.  A  wall  was  to  be  built  700  yards  long  in  29 
days.  Now,  after  12  men  had  been  employed  on  it  for  11 
dtiys,  it  was  found  that  they  had  completed  only  229  yards 
of  the  wall.  It  is  required  to  determine  how  many  men  must 
be*  added  to  the  former,  that  the  whole  number  of  them  may 
just  finish  the  wall  in  the  time  proposed,  at  the  same  rate  of 
forking.  Ans.  4  men  to  be 


142 


ARITHMETIC* 


Quest.  6.  Determine  how  far  500  millions  of  guineas  will 
reach,  when  laid  down  in  a  strait  line  touching  one  an- 
other ;  supposing  each  guinea  to  be  an  inch  in  diameter,  as 
it  is  very  nearly.  Ans.  7891  miles,  728  yds,  2  ft.  8  in. 

Quest.  7.  Two  persons,  a  and  b,  being  on  opposite  sides 
of  a  wood,  which  is  536  yards  about,  they  begin  to  go  round 
it,  both  the  same  way,  at  the  same  instant  of  time  ;  a  goes  at 
the  rate  of  1 1  yards  per  minute,  and  b  34  yards  in  3  mi. 
nutes ;  the  question  is,  how  many  times  will  the  wood  be 
gone  round  before  the  quicker  overtake  the  slower  1 

Ans.  17  times. 

Quest.  8.  a  can  do  a  piece  of  work  alone  in  12  days, 
and  b  alone  in  14  ;  in  what  time  will  they  both  together  per- 
form a  like  quantity  of  work  ?  Ans.  6T0T  days. 

Quest.  9.  A  person  who  was  possessed  of  a  |  share  of  a 
copper  mine,  sold  f  of  his  interest  in  it  for  1800/ ;  what  was 
the  reputed  value  of  the  whole  at  the  same  rate  ?  Ans.  4000/. 

Quest.  10.  A  person  after  spending  20/  more  than  J  of 
his  yearly  income,  had  then  remaining  30/  more  than  the 
half  of  it ;  what  was  his  income  ?  Ans.  200/. 

Quest.  11.  The  hour  and  minute  hand  of  a  clock  are 
exactly  together  at  12  o'clock  ;  when  are  they  next  together  T 

Ans.  at  lTy  hr.  or  1  hr.  5>r  min. 

Quest.  12.  If  a  gentleman  whose  annual  income  is  15002, 
spend  20  guineas  a  week ;  whether  will  he  save  or  run  in 
debt,  and  how  much  in  the  year  ?  Ans.  save  408/, 

Quest  13.  A  person  bought  180  oranges  at  2  a  penny, 
and  180  more  at  3  a  penny  ;  after  which,  selling  them  out 
again  at  5  for  2  pence,  whether  did  he  gain  or  lose  by  the 
bargain  ?  Ans.  he  lost  6  pence. 

Quest.  14.  If  a  quantity  of  provisions  serves  1500  men 
12  weeks,  at  the  rate  of  20  ounces  a  day  for  each  man  ;  how 
many  men  will  the  same  provisions  maintain  for  20  weeks,  at 
the  rate  of  8  ounces  a  day  for  each  man  ?    Ans.  2250  men. 

Quest.  15.  In  the  latitude  of  London,  the  distance  round 
the  earth,  measured  on  the  parallel  of  latitude,  is  about  15550 
miles  ;  now  as  the  earth  turns  round  in  23  hours  56  minutes, 
at  what  rate  per  hour  is  the  city  of  London  carried  by  this 
motion  from  west  to  east  ?         Ans.  649$}}  miles  an  hour. 

Quest.  16.  A  father  left  his  son  a  fortune,  ±  of  which  he 
ran  through  in  8  months  :  $  of  the  remainder  lasted  him  12 
months  longer ;  after  which  he  had  820/  left.  What  sum 
did  the  father  bequeath  his  son  ?  Ans.  1913/  6s  8d. 

Quest.  17.    If  1000  men,  besieged  in  a  town,  with  pro* 


PRACTICAL  QUESTIONS. 


143 


visions  for  5  weeks,  allowing  each  man  16  ounces  a  day,  be 
reinforced  with  500  men  more  ;  and  supposing  that  they  can- 
not  be  relieved  till  the  end  of  8  weeks,  how  many  ounces  a 
day  must  each  man  have,  that  tho  provision  may  last  that 
time  ?  Ans.  6}  ounces. 

Qukst.  18.  A  younger  brother  received  8400/,  which 
was  just  J  of  his  elder  brother's  fortune  :  What  was  the 
lather  worth  at  his  death  ?  Ans.  19200/. 

Qukst.  19.  A  person,  looking  on  his  watch,  was  asked 
what  was  the  time  of  the  day,  who  answered,  It  is  between 
5  and  6  ;  but  a  more  particular  answer  being  required,  he 
said  that  the  hour  and  minute  hands  were  then  exactly  to- 
gether :  What  was  the  time  ?  Ans.  27^  min.  past  5. 

Quest.  20.  If  20  men  can  perforin  a  piece  of  work  in 
12  days,  how  many  men  will  accomplish  another  thrice  as 
large  in  one-fifth  of  the  time  ?  Ans.  300. 

Quest.  21.  A  father  devised  T\  of  his  estate  to  one  of 
his  sons,  and  T\  of  the  residue  to  another,  and  the  surplus  to 
his  relict  for  life.  The  children's  legacies  were  found  to  be 
514/  6*  8d  different  :  What  money  did  he  leave  the  widow 
the  use  of?  Ans.  1270/  1*  9^d. 

Quest.  22.  A  person,  making  his  will,  gave  to  one  child 

of  his  estate,  and  the  rest  to  another.  When  these  legacies 
came  to  be  paid,  the  one  turned  out  1200/  more  thun  the 
other  :  What  did  the  testator  die  worth  ?  Ans.  4000/. 

Quest.  23.  Two  persons,  a  and  b,  travel  between  Lon- 
don and  Lincoln,  distant  100  miles,  a  from  London,  and  b 
from  Lincoln,  at  the  same  instant.  After  7  hours  they  meet 
on  the  road,  when  it  appeared  that  a  had  rode  l£  miles  an 
hour  more  than  b.  At  what  rate  per  hour  then  did  each  of 
the  travellers  ride  ?  Ans.  a  7§J  and  b  miles. 

Quest.  24.  Two  persons,  a  and  n,  travel  between  Lon- 
don and  Exeter,  a  leaves  Exeter  at  8  o'clock  in  the  morn- 
ing, and  walks  at  the  rate  of  3  miles  an  hour,  without  inter- 
naission  ;  and  b  sets  out  from  London  at  4  o'clock  the  same 
evening,  and  walks  for  Exeter  at  the  rate  of  4  miles  an  hour 
constantly.  Now,  supposing  the  distance  between  the  two 
cities  to  be  130  miles,  whereabouts  on  the  road  will  they 
xtieet  ?  Ans.  09}  miles  from  Exeter. 

Quest.  25.  One  hundred  eggs  being  placed  on  the 
ground,  in  a  straight  line,  at  the  distance  of  a  yard  from  each 
other :  How  far  will  a  person  travel  who  shall  bring  them 
one  by  one  to  a  basket,  which  is  placed  at  one  yard  from  the 
first  egg?         Ans.  10100  yards,  or  5  miles  and  1300  yds. 

Quest.  26.   The  clocks  of  Italy  go  on  to       Yvoura  \ 


144 


ARITHMETIC. 


Then  how  many  strokes  do  they  strike  in  one  complete  re- 
volution of  the  index  ?  Ans.  300. 

Quest.  27.  One  Sessa,  an  Indian,  having  invented  the 
game  of  chess,  showed  it  to  his  prince,  who  was  so  delighted 
with  it,  that  he  promised  him  any  reward  he  should  ask  ;  on 
which  Sessa  requested  that  he  might  be  allowed  one  grain  of 
wheat  for  the  first  square  on  the  chess  board,  2  for  the  second, 
4  for  the  third,  and  so  on,  doubling  continually,  to  64,  the 
whole  number  of  squares.  Now,  supposing  a  pint  to  con- 
tain  7680  of  these  grains,  and  one  quarter  or  8  bushels  to  be 
worth  27^  6tZ,  it  is  required  to  compute-  the  value  of  all  the 
corn  ?  Ans.  6450468916285/  17*  3d  -Sitffff. 

Quest.  28.  A  person  increased  his  estate  annually  by 
100/  more  than  the  j-  part  of  it  ;  and  at  the  end  of  4  years 
found  that  his  estate  amounted  to  10342/  Ss  9d.  What  had 
he  at  first  ?  Ans.  4000/. 

Qukst.  29.  Paid  1012/  10*  for  a  principal  of  750/,  taken 
in  7  years  before  :  at  what  rate  per  cent,  per  annum  did  1 
pay  interest  ?  Ans.  5  per  cent. 

Quest.  30.  Divide  1000/  among  a,  b,  c  ;  so  as  to  give 
a  120  more,  and  b  95  less  than  c. 

Ans.  a  445,  b  230,  c  325. 

Quest.  31.  A  person  being  asked  the  hour  of  the  day, 
said,  the  time  past  noon  is  equal  to  £ths  of  the  time  till  mid- 
night.   What  was  the  time?  Ans.  20  min.  past  5. 

Quf.8T.  32.  Suppose  that  I  have  T^  of  a  ship  worth 
1200/;  what  part  of  her  have  I  left  after  selling  J  of  £  of 
my  share,  and  what  is  it  worth  ?         Ans.  5y„,  worth  185/. 

Quest.  33.  Part  1200  acres  of  land  among  a,  b,  c  ;  bo 
that  b  may  have  100  more  than  a,  and  c  (>4  more  than  b. 

Ans.  a  312,  b  412,  c  476. 

Quest.  34.  What  number  is  that,  from  which  if  there 
be  taken  f  of  },  and  to  the  remainder  be  added  T85-  of  \>  the 
sum  will  be  10?  Ans.  O^J. 

Quest.  35.  There  is  a  number  which,  if  multiplied  by 
f  of  |  of  1J,  will  produce  1  :  what  is  the  square  of  that 
number  ?  Ans.  1TT. 

Quest.  36.  What  length  must  be  cut  off  a  board,  8} 
inches  broad,  to  contain  a  square  foot,  or  as  much  as  12 
inches  in  length  and  12  in  breadth  ?         Ans.  16  f  $  inches. 

Quest.  37.  What  sum  of  money  will  amount  to  138/  2s 
6d,  in  15  months,  at  5  per  cent,  per  annum  simple  interest  ? 

Ans.  130/. 

Quest.  38.    A  father  divided  his  fortune  among  his  three 


nucncAft  Sjussrnoifs. 


145 


•om,  a,  a,  c,  giving  i  4  u  often  as  b  3,  and  o  5  at  often  as 
b  6 ;  what  was  the  whole  legacy,  supposing  a's  share  was 
40002?  Ans.  95002. 

Quest.  39.  A  young  hare  starts  40  yards  before  a  grey, 
bound,  and  is  not  perceived  by  him  till  she  has  been  up  40 
seconds ;  she  scuds  away  at  the  rate  of  10  miles  an  hour,  and 
the  dog,  on  view,  makes  after  her  at  the  rate  of  18  :  how 
long  will  the  course  hold,  and  what  ground  will  be  run  over, 
counting  from  the  outaetting  of  the  dog  ? 

Ans.  60^  sec.  and  530  yards  run. 

Quest.  40.  Two  young  gentlemen,  without  private  for- 
tune, obtain  commissions  at  the  same  time,  and  at  the  age  of 
18.  One  thoughtlessly  spends  102  a  year  more  than  his  pay ; 
but,  shocked  at  the  idea  of  not  paying  his  debts,  gives  his 
creditor  a  bond  for  the  money,  at  the  end  of  every  year,  and 
also  insures  his  life  for  the  amount ;  each  bond  costs  him  30 
■billings,  besides  the  lawful  interest  of  5  per  cent,  and  to  in- 
sure his  life  costs  him  6  per  cent. 

The  other,  having  a  proper  pride,  is  determined  never  to 
ran  in  debt ;  and,  that  he  may  assist  a  friend  in  need,  per. 
•everes  in  saving  102  every  year,  for  which  he  obtains  an 
interest  of  5  per  cent,  which  interest  is  every  year  added  to 
his  savings,  and  laid  out,  so  as  to  answer  the  effect  of  com- 
pound interest. 

Suppose  these  two  officers  to  meet  at  the  age  of  50,  when 
each  receives  from  Government  4002  per  annum  ;  tha  the 
one,  seeing  his  past  errors,  is  resolved  in  future  to  spend  no 
more  than  he  actually  has,  after  paying  the  interest  for  what 
he  owes,  and  the  insurance  on  his  life. 

The  other,  having  now  something  beforehand,  means  in 
future  to  spend  his  full  income,  without  increasing  his  stock* 

It  is  desirable  to  know  how  much  each  has  to  spend  per 
annum,  and  what  money  the  latter  has  by  him  to  assist  the 
distressed,  or  leave  to  those  who  deserve  it  ? 

Ana.  The  reformed  officer  has  to  spend  662  19#  1}*5389& 
per  annum. 

The  prudent  officer  has  to  spend  4372 12s  1  lj«4379cf. 

per  annum,  and 
The  latter  has  saved,  to  dispose  of,  7522  19s  9-1890& 


▼ax.  /. 


20 


146 


LOGARITHMS. 


OF  LOGARITHMS  *. 


Logarithms  are  made  to  ftrinWfe  troublesome  calcu- 
lations in  numbers.  This  they  doy  because  they  perform 
multiplication  by  only  addition,  and  division  by  subtraction, 
and  raising  of  powers  by  multiplying  the  logarithm  by  the 
index  of  the  power,  and  extracting  of  roots  by  dividing 
the  logarithm  of  the  number  by  the  index  of  the  root 
For,  logarithms  are  numbers  so  contrived,  and  adapted  to 
other  numbers,  that  the  sums  and  differences  of  the  former 
shall  correspond  to,  and  show  the  products  and  quotients  of 
the  latter,  dec. 

Or,  more  generally,  logarithms  are  the  numerical  expo- 
nents of  ratios  ;  or  they  are  a  series  of  numbers  in  arith- 


*  The  invention  of  Logarithms  is  due  to  Lord  Napier,  Baron  of 
Merchiston,  in  Scotland,  and  is  properly  considered  as  one  of  the  most 
useful  inventions  of  modern  times.  A  table  of  these  numbers  was  first 
published  by  the  inventor  at  Edinburgh,  in  the  year  1614,  in  a  treaties 
entitled  Canon  Mirificum  Logarithmorum ;  which  was  eagerly  received 
by  all  the  learned  throughout  Europe.  Mr.  Henry  Bnggs,  then  pro- 
fessor of  geometry  at  Gresham  College,  soon  after  the  discovery, 
went  to  visit  the  noble  inventor ;  after  which,  they  jointly  undertook 
the  arduous  task  of  computing  new  tables  ou  this  subject,  and  reducing 
them  to  a  more  convenient  form  than  that  which  was  at  first  thought 
of.  But  Lord  Napier  dying  soon  after,  the  whole  burden  fell  upon 
Mr.  Briggs,  who,  with  prodigious  labour  and  great  skill,  made  an  entire 
Canon,  according  to  the  new  form,  for  all  numbers  from  1  to  20000, 
and  from  90000  to  101000,  to  14  places  of  figures,  and  published  it  at 
London  in  the  year  1624,  in  a  treatise  entitled  Arithmetica  Logarithmic*, 
with  directions  for  supplying  the  intermediate  parts. 

This  Canon  was  again  published  in  Holland  by  Adrian  Vlacq,  in  the 
year  1628,  together  with  the  Logarithms  of  all  the  numbers  which  Mr. 
Briggs  had  omitted  ;  but  he  contracted  them  down  to  10  places  of  de- 
cimals.  Mr.  Briggs  also  computed  the  Logarithms  of  the  sines,  tan- 

Sents,  and  secants,  to  every  degree,  and  centestn,  or  100th  part  of  a 
egree,  of  the  whole  quadrant ;  and  annexed  them  to  the  natural  sines* 
tangents,  and  secants,  which  lie  had  before  computed,  to  fifteen  placet 
of  figures.   These  tables,  with  their  construction  and  use,  were  first 

Eublished  in  the  year  1633,  after  Air.  Briggs 's  death,  by  Mr.  Henry  Getti* 
rand,  under  the  title  of  Trigouometria  Britomiica. 


LOGARITHMS.  147 

metical  progression,  answering  to  another  series  of  numbers 
in  geometrical  progression. 

rp.  $0,1,2,3,  4,  5,  0,  Indices,  or  logarithms, 
inus  I  1,  2,  4,  8,  10,  32,  04,  Geometric  progression, 
ft  i  0,  1,  2,  3,  4,  5,  6,  Indices,  or  logarithms, 
w    £  1,  3,  9,  27,  81,  243,  729,  Geometric  progression. 

n«    $  0,    1,     2,       3,         1,  5,  Indices,  or  logs. 

w    $  1,  10,  100,  1000,  10000,  100000,  Geom.  progres. 

Where  it  is  evident,  that  the  same  indices  serve  equally 
for  any  geometric  aerie*  ;  and  consequently  there  may  be  an 
endless  variety  of  system  of  logarithms,  to  the  same  com- 
mon numbers,  by  only  changing  the  second  term,  2,  3,  or 
10,  &c.  of  the  geometrical  series  of  whole  numbers  ;  and  by 
interpolation  the  whole  system  of  numbers  may  be  made  to 
enter  the  geometric  series,  and  receive  their  proportional  loga- 
rithms, whether  integers  or  decimals. 

It  is  also  apparent,  from  the  nature  of  these  series,  that  if 
any  two  indices  be  added  together,  their  sum  will  be  the  in- 
dex of  that  number  which  is  equal  to  the  product  of  the  two 
terms,  in  the  geometric  progression,  to  which  those  in- 
dices belong.  Thus  the  indices  2  and  3,  being  added  toge- 
ther, make  5  ;  and  the  numbers  4  and  8,  or  the  terms  cor- 
responding to  those  indices,  being  multiplied  together,  make 
82,  wnich  is  the  number  answering  to  the  index  5. 

In  like  manner,  if  any  one  index  be  subtracted  from  an- 
other, the  difference  will  be  the  index  of  that  number  which 


Benjamin  Ursinus  also  gave  "a  Table  of  Napier's  Logs,  and  of  sines, 
to  every  10  seconds.  And  Chr.  Wolf,  in  his  Mathematical  Lexicon,  says 
that  one  Van  Loser  had  computed  them  to  every  single  second,  but 
Ms  untimely  death  prevented  their  publication.  Many  other  authors 
have  treated  on  this  subject ;  but  as  their  numbers  are  frequently  in  ac- 
curate and  incommodiously  disposed,  they  are  now  generally  neglect- 
ed. The  Tables  in  most  repute  at  present,  nrc  those  of  Gardiner  in 
4to,  first  published  in  the*  year  1742 ;  and  my  own  Tables  in  8vo,  first 
printed  in  the  year  1785,  where  the  Logarithms  of  all  numbers  may  be 
easily  found  from  1  to  10800000  ;  and  those  of  the  sines,  tangents,  and 
secants,  to  any  degree  of  accuracy  required. 

Mr.  Michael  Taylor's  Tables  in  large  4to,  containing  the  common 
logarithms,  and  the  logarithmic  sines  and  tangents  to  every  second  of 
the  quadrant,  are  very  valuable.  And,  in  France,  the  new  book  of 
logarithms  by  Callet;  the  2d  edition  of  which,  in  1795,  has  the 
tables  still  further  extended,  and  are  printed  with  what  are  called  stereo- 
types, the  types  in  each  page  beng  soldered  together  into  a  solid  mass 
or  block. 

Dodson's  Antiiogarithmic  Canon  is  likewise  a  very  elaborate  work, 
and  used  for  finding  the  numbers  answering  to  any  given  Vogpx\\\k\a, 
neb  to  11  places. 


148 


LOGARITHM. 


is  equal  to  the  quotient  of  the  two  feme  to  which  thoee  io« 
dices  belong.  Thai,  the  index  6,  minus  the  index  4,  is  =  2 ; 
and  the  terms  corresponding  to  those  indices  are  64  and  16, 
whose  quotient  is  =  4,  which  is  the  number  answering  to  the 
index  2. 

For  the  same  reason,  if  the  logarithm  of  any  number  be 
multiplied  by  the  index  of  its  power,  the  product  will  be  equal 
to  the  logarithm  of  that  power.  Thus,  the  index  or  loga- 
rithm of  4,  in  the  above  series,  is  2;.  ind  if  this  number  be 
multiplied  by  3,  the  product  will  be  «6  j.  which  is  the  loga- 
rithm of  64,  or  the  third  power-of  4. 

And,  if  the  logarithm  of  any  number  be  divided  by  the 
index  of  its  root,  the  quotient  will  be  equal  to  the  logarithm 
of  that  root.  Thus,  the  index  or  logarithm  of  64  is  6  ; 
and  if  this  number  be  divided  by  2,  the  quotient  will  be 
=  3 ;  which  is  the  logarithm  of  8,  or  the  square  root  of 

The  logarithms  most  convenient  for  practice,  are  such  as 
are  adapted  to  a  geometric  series  increasing  in  a  tenfold  pro- 
portion, as  in  the  last  of  the  above  forms  ;  and  are  those 
which  are  to  be  found,  at  present,  in  most  of  the  common 
tables  on  this  subject*  The  distinguishing  mark  of  this 
system  of  logarithms  is,  that  the  index  or  logarithm  of  10 
is  1  ;  that  of  100  is  2  ;  that  of  1000  is  3  ;  &c.  And,  in 
decimals,  the  logarithm  of  •!  is  —  1  ;  that  of  *01  is  —  2 ;  thai 
of  "001  is  —  3,  die.  the  log.  of  1  being  0  in  every  systesjt 
Whence  it  follows,  that  the  logarithm  of  any  number  beV" 
tween  1  and  10,  must  be  0  and  some  fractional  parts  ;  and^ 
that  of  a  number  between  10  and  100,  will  he  1  and  some? 
fractional  parts  ;  and  so  on,  for  any  other  number  whatever. 
And  since  the  integral  part  of  a  logarithm,  usually  called  the 
Index,  or  Characteristic,  is  always  thus  readily  found,  it  is 
commonly  omitted  in  the  tables ;  being  left  to  be  supplied  by 
the  operator  himself)  as  occasion  requires. 

Another  Definition  of  Logarithms  is,  that  the  logarithm  of 
any  number  is  the  index  of  that  power  of  some  other  num- 
ber, which  is  equal  to  the  given  number.  So,  if  there  be 
»-r",  then  n  is  the  log.  of  n  ;  where  n  may  be  either  po- 
sitive or  negative,  or  nothing,  and  the  root  or  base  r  any 
number  whatever,  according  to  the  different  systems  of  lo- 
garithms. When  n  is  =  0,  then  n  is  =  1,  whatever  the 
value  of  r  is ;  which  shows,  that  the  log.  of  1  is  always  0,  in 
every  system  of  logarithms.    When  n  is  =  1,  then  n  is  =  r ; 


140 


to  dial  the  radix  r  it  always  that  number  whose  log.  is  1,  in 
every  system.  When  the  radix  r  is  =  2  •718281826459  &c. 
the  indices  n  are  the  hyperbolic  or  Napier's  log.  of  the  num- 
bers ]t ;  so  that  n  is  always  the  hyp.  log.  of  the  number  if 
or  (2.718  &c.)\ 

But  when  the  radix  r  is  =  10,  then  the  index  n  becomes 
the  common  or  Briggs's  log.  of  the  number  n  :  so  that  the 
common  log.  of  any  number  10*  or  n,  is  n  the  index  of  that 
power  of  10  which  is  equal  to  the  said  number.  Thus  100, 
being  the  second  power  of  10,  will  have  2  for  its  logarithm ; 
and  1000,  being  the  third  power  of  10,  will  have  3  for  its 
logarithm  :  hence  also,  if  GO  be  =  10"**7,  then  is  1*69807 
the  common  log.  of  50.  And,  in  general,  the  following  de- 
cuple series  of  terms, 

to.  1C,  10',  109,  Iff,  10°,  io-\  10-»,  10-3,  10-4, 
or  10000,  1000,  100,  10,  1,  -1,  -01,  001,  -0001, 
have  4,  3,  2,  1,  0,  -1,  -2,  -3,  -4, 
for  their  logarithms,  respectively.  And  from  this  scale  of 
numbers  and  logarithms,  the  same  properties  easily  follow, 
as  above  mentioned. 


problem. 

To  compute  the  Logarithm  to  any  of  the  Natural  Number* 
1,  2,  3,  4,  5,  6fc. 

RULE  I*. 

Take  the  geometric  series,  1,  10,  100,  1000,  10000,  die. 
and  apply  to  it  the  arithmetic  series,  0,  1,2,  3,  4,  &c.  as 
logarithms. — Find  a  geometric  mean  between  1  and  10,  or 
/between  10  and  100,  or  any  other  two  adjacent  terms  of  the 
aeries,  between  which  the  number  proposed  lies. — In  like 
manner,  between  the  mean,  thus  found,  and  the  nearest  ex- 
treme, find  another  geometrical  mean ;  and  so  on,  till  you 
arrive  within  the  proposed  limit  of  the  number  whose  loga- 
rithm is  sought. — Find  also  as  many  arithmetical  means,  in 
the  same  order  as  you  found  the  geometrical  ones,  and  these 
will  be  the  logarithms  answering  to  the  said  geometrical 
means. 


*  The  reader  who  wishes  to  inform  himself  more  particularly  con- 
cerning the  history,  nature,  and  construction  of  Logarithms,  may  con- 
ssK  my  Mathematical  Tracts,  vol.  1,  lately  published,  where  he  wit 
sod  his  cariosity  amply  gratified. 


150 


LOGARITHMS. 


EXAMPX.B. 

Let  it  be  required  to  find  the  logarithm  of  9. 

Here  the  proposed  number  lies  between  1  and  10. 
First,  then,  the  log.  of  10  is  I,  and  the  log.  of  1  is  fr; 

theref.  (1  +  0)  -r-  2  =  %  =  *5  is  the  arithmetical  mean, 
and  -v/(10  X  1)  =  y/10  =  3*1622777  the  geom.  mean  ; 
hence  the  log.  of  0*1022777  is  '5. 

Secondly,  the  log.  of  10  is  1,  and  the  log.  of  3*  1622777  is  -5; 
theref.  (1  +  -5)     2  =  -75  ia  the  arithmetic  a!  mean, 
and  ^(10  X3-102277?)=5-6234132  is  the  geom.  mean ; 
hence  the  log.  of  5*6234132  is  »75. 

Thirdly,  the  log.  of  10  is  1,  and  the  log*  of  5*0234132  is  -75; 
theref.  (1  +  -75}  2  =  875  is  the  arithmetical  mean, 
and  v/(10  X  5*6234132)  =  7*4989422  the  geom.  mean ; 
hence  the  log.  of  7-4989422  is  -875. 

Fourthly,  the  log.of  10  is  1,  and  the  log.  of 7-4989422  is  -875; 
theref.  (1  +  -875) -r-  2  =-9375  is  the  arithmetical  mean, 
and  v/(10  X  7-4989422)  =  8-6596431  the  geom.  mean ; 
hence  the  log.  of  8-6596431  is  -9375. 

Fifthly,  the  log.  of  10  is  1,  and  the  log.  of  8-6596431  is  -9375 ; 
theref.  (l+-9375)-i-2=-96875  is  the  arithmetical  mean, 
and  v/( 10  X  8-6596431)  =  9-3057204  the  geom.  mean ; 
hence  the  log.  of  9-3057204  is  -96875. 

Sixthly,  the  log.  oT  8-6596431  is  -9375,  and  the  log.  of 
9-3057204  is -96875. 
theref.  ( -9375+  -96875) -r-2= -953 125  is  the  arith-mean, 
and  ^(8-6596431  X  9-3057204)  =  8*9768713  the  geo- 
metric mean ; 
hence  the  log.  of  8-9768713  is  -953125. 

And  proceeding  in  this  manner,  after  25  extractions,  it 
will  be  found  that  the  logarithm  of  8-9999998  is  -9542425  ; 
which  may  be  taken  for  the  logarithm  of  9,  as  it  differs  so 
little  from  it,  that  it  is  sufficiently  exact  for  all  practical  pur- 
poses. In  this  manner  were  the  logarithms  of  almost  all  the 
prime  numbers  at  first  computed. 

RUIjE  II*. 

Let  b  be  the  number  whose  logarithm  is  required  to  be 
found ;  and  a  the  number  next  less  than  b}  so  that  b  —  a  =1, 


*  For  the  demonstration  of  this  rule,  see  my  Mathematical  Tablet, 
p.  109,  &c.  and  my  Tracts,  vol.  1 . 


LOGARITHMS. 


151 


the  logarithm  of  a  being  known  ;  and  let  *  denote  the  sum 
of  the  two  numbers  a  +  b.  Then 

1.  Divide  the  constant  decimal  -8085889038  &c.  by  *, 
and  reserve  the  quotient :  divide  the  reserved  quotient  by 
the  square  of  *,  and  reserve  this  quotient ;  divide  this  last 
quotient  also  by  the  square  of  sy  and  again  reserve  the  quo- 
tient :  and  thus  proceed,  continually  dividing  the  last  quotient 
by  the  square  of  s  ,  as  long  as  division  can  be  made. 

2.  Then  write  these  quotients  orderly  under  one  another, 
the  first  uppermost,  and  divide  them  respectively  by  the  odd 
numbers,  1, 3,  5,  7,  0,  &&  as  long  as  division  can  be  made ; 
that  is,  divide  the  first  reserved  quotient  by  1,  the  second  by 
3,  the  third  by  5,  the  fourth  by  7,  and  so  on. 

8.  Add  all  these  last  quotients  together,  and  the  sum  will 
be  the  logarithm  of  b  a ;  thorefore  to  this  logarithm  add 
also  the  given  logarithm  of  the  said  next  less  number  a,  so 
will  the  last  sum  be  the  logarithm  of  the  number  b  proposed. 

That  is, 

Log.  of  b.  is  log.  a  +  i  X  ( 1  +  J-  +  -L  +  -L  +  &c. 
where  n  denotes  the  constant  given  decimal  '8085889638  dec. 


examples. 


Ex.  1.  Let  it  be  required  to  find  the  log.  of  the  number  2. 
Here  the  given  number  b  is  2,  and  the  next  less  number  a 
is  1,  whose  log.  is  0  ;  also  the  sum  2  +  1=3  =  *,  and  its 
square  *3  =  9.    Then  the  operation  will  be  as  follows  : 


3 
9 
9 
9 

9 
9 
9 
O 


•80858890-1 
•289529054 
34109902 
3571410 
397100 
44129 
4903 
515 
01 


1 
3 
5 
7 
9 
11 
13 
15 


•289529054  ( 
32109902  ( 
3574410  ( 
397100  ( 
44129  ( 
4903  ( 
545  ( 
01  ( 

log.  of  !{  - 
add  log.  1  - 


•289529(554 
10723321 
714888 
50737 
4903 
440 
42 
1 

•301029995 
•000000000 


log.  of  2 


•301029995 


LOflARITMMB. 


Ex.  3.  To  compute  the  logarithm  of  the  number  3. 

Here  b  =  3,  the  next  less  number  a  =  2,  and  the  sum 
a  +  b  =  5  =  «,  whose  square  «*  is  25,  to  divide  by  which, 
always  multiply  by  -04.    Then  the  operation  is  as  follows  : 


5 
25 
25 
25 
25 
25 


•868588964 
173717793 
6948712 
277948 
11118 
445 
18 


1  ) 
3  ) 
5  ) 
7  ) 

11  ) 


173717793 
6948712 
277948 
11118 
445 
18 


( 
[ 

Si 


log.  off 
log.  of  2  add 


173717798 
2316*37 
55590 
1588 
50 
2 

176091260 
3U1029995 


log.  of  3  sought  -477121255 


Then,  because  the  sum  of  the  logarithms  of  numbers, 
gives  the  logarithm  of  their  product ;  and  the  difference  of 
the  logarithms,  gives  the  logarithm  of  the  quotient  of  the 
numbers ;  from  the  above  two  logarithms,  and  the  logarithm 
of  10,  which  is  1,  we  may  obtain  a  great  many  logarithms, 
as  in  the  following  examples  : 


EXAMPLE  3. 

Because  2x2=  4,  therefore 
to  log.  2  .  -301029995| 
add  log.  2  -  -301029995} 


sum  is  log.  4  -602059991} 


EXAMPLE  4. 

Because  2X3  =  6,  therefore 
to  log.  2    -  -301029995 
add  log.  3  -  -477121255 


sum  is  log.  6 -778151250 


KXAMPUB  5. 

Because  2s  =  8,  therefore 
log.  2  -  -301029995 
mult,  by  3  3 


example.  6. 
Because  3"  =  9,  therefore 
log.  3    -  -477121254/, 
mult  by  2  2 


gives  log.  9  -954242509 


EXAMPLE  7. 

Because  y  =  5,  therefore 
from  log.  10 1  -000000000 
take  log.  2  -301029995} 


leaves  log.  5  -698970004} 


EXAMPLE  8. 

Because  3X4  =  12,  therefore 
to  log.  3  -  -477121255 
add  log.  4  *  -602059991 


gives  log.  8  -903089987    j     gives  log.  12  1-079181246 


LOGARITHMS. 


158 


And  thus,  computing  by  this  general  rule,  the  logarithms 
to  the  other  prime  numbers,  7,  11,  13,  17, 19,  23,  dec.  and 
then  using  composition  and  division,  we  may  easily  find  as 
many  logarithms  as  we  please,  or  may  speedily  examine  any 
logarithm  in  the  table*. 

Description  a*d  Use  if  the  Table  of  Logarithms. 

Having  explained  the  manner  of  forming  a  table  of  the 
logarithms  of  numbers,  greater  than  unity ;  the  next  thing  to 
be  done  is,  to  show  how  the  logarithms  of  fractional  quan- 
tities may  be  found.  In  order  to  this,  it  may  be  observed, 
that  as  in  the  former  case  a  geometric  series  is  supposed  to 
increase  towards  the  left,  from  unity,  so  in  the  latter  case 
it  is  supposed  to  decrease  towards  the  right  hand,  still  be- 
ginning with  unit;  as  exhibited  in  the  general  description, 
page  152,  where  the  indices  being  made  negative,  still  show 
the  logarithms  to  which  they  belong.  Whence  it  appears, 
that  as  +  1  is  the  log.  of  10,  so  —  1  is  the  log.  of  T\  or  -1  ; 
and  as  +  2  is  the  log.  of  100,  so  — 2  is  the  log.  of  T^  or  *01  : 
and  so  on. 

Hence  it  appears  in  general,  that  all  numbers  which  con- 
sist of  the  same  figures,  whether  they  be  integral,  or  frac- 
tional, or  mixed,  will  have  the  decimal  parts  of  their  loga- 
rithms the  same,  but  differing  only  in  the  index,  which  Mill 
be  more  or  less,  and  positive  or  negative,  according  to  the 
place  of  the  first  figure  of  the  number. 

Thus,  the  logarithm  of  2051  being  3-423410,  the  log.  of 
tV»  or  iiv>  or  T?!o7>  &c-  Part  °f  *t  W'M  06  113  follows : 
Numbers.  Logarithms. 


2  6  5  1 
2  0-51 
2  6  5-1 
2-651 
•2  6  5  1 
•0  2  6  5  1 
•0  0  2  6  5  1 


3-4  2  3  4  1  0 

2-4  2  3  4  1  0 

1-4  2  3  4  1  0 

0  -4  2  3  4  1  0 

-1-4  2  3  4  1  0 

-2-4  2  3  4  1  0 

-3-4  2  3  4  1  0 


*  There  are,  besides  these,  many  other  ingenious  methods,  which 
later  writers  have  discovered  for  finding  the  logarithms  of  numbers, 
la  a  much  easier  way  than  by  the  original  inventor  ;  but,  as  they  cannot 
lie  understood  without  a  kno'wledgc;  of  some  of  the  higher  branches  of 
Uie  mathematics,  it  is  thought  proper  to  omit  them,  and  to  refer  the 
a-asderto  those  works  which  are  written  e.xpres  ly  on  the  subject.  It 
Vrould  likewise  much  exceed  the  limits  of  this  compendium,  Vo 
Oat  all  the  peculiar  artifices  that  are  made  use  of  fur  COn*Vru>cftfe&u& 
Vol.  1.  21 


154 


LOGARITHMS. 


Hence  it  also  appears,  that  the  index  of  any  logarithm,  is 
always  less  by  1  than  the  number  of  integer  figures  which 
the  natural  number  consists  of:  or  it  is  equal  to  the  distance 
of  the  first  figure  from  the  place  of  units,  or  first  place  of  in- 
tegers, whether  on  the  left,  or  on  the  right,  of  it :  and  this 
index  is  constantly  to  be  placed  on  the  left-hand  side  of  the 
decimal  part  of  the  logarithm. 

When  there  are  integers  in  the  given  number,  the  index 
is  always  affirmative ;  but  when  there  are  no  integers,  the 
index  is  negative,  and  is  to  be  marked  by  a  short  line  drawn 
before  it,  or  else  above  it.  Thus, 

A  number  having      1, 2, 3, 4, 5,  &c.  integer  places, 

the  index  of  its  log.  is  0, 1, 2, 3, 4,  die.  or  1  less  than  those 
places. 

And  a  decimal  fraction  having  its  first  effective  figure  in  the 
1st,  2d,  3d,  4th,  &c,  place  of  the  decimals,  has  always 
— 1,-2, — 3, — 4,  &c.  for  the  index  of  its  logarithm. 

It  may  also  bo  observed,  that  though  the  indices  of  frac- 
tional quantities  are  negative,  yet  the  decimal  parts  of  their 
logarithms  are  always  affirmative.  And  the  negative  mark 
( — )  may  be  set  either  before  the  index  or  over  it. 

I.  TO  FIND  IN  T1IE  TABLE,  THE  LOGARITHM  TO  ANY 
NTMHER*. 

1.  If  the  given  Number  be  less  than  100,  or  consist  of  only 
two  figures ;  its  log.  is  immediately  found  by  inspection  in 
the  first  page  of  the  table,  which  contains  all  numbers  from 
1  to  100,  with  their  logs,  and  the  index  immediately  annexed 
in  the  next  column. 

So  the  log.  of  5  is  0-G9S970.  The  log.  of  23  is  1  -301728. 
The  log.  of  50.  is  1  -008070.    And  so  on. 

2.  If  the  Number  be  more  than  100  but  less  than  10000; 
that  is,  consisting  of  either  three  or  four  figures :  the  decimal 
part  of  the  logarithm  is  found  by  inspection  in  the  other 
pages  of  the  table,  standing  against  the  given  number  in  this 
manner ;  viz.  the  first  three  figures  of  the  given  number  in  the 
first  column  of  the  page,  and  the  fourth  figure  one  of  those 
along  the  top  line  of  it ;  then  in  the  angle  of  meeting  are  the 
last  lour  figures  of  the  logarithm,  and  the  first  two  figures 
of  the  same  at  the  beginning  of  the  same  line  in  the  second 


entire  table  of  these  numbers ;  but  any  information  of  this  kind,  which 
the  learner  may  wish  to  obtain,  may  he  found  in  my  Tables.    See  alto 
the  article  on  Logarithms  in  the  2d  volume,  p.  340.  &c. 
'  See  the  table  of  Logarithms,  at  the  end  of  this  volume. 


L0GABITHK8. 


156 


column  of  the  page  :  to  which  is  to  be  prefixed  the  proper 
index  which  is  always  1  less  than  the  number  of  integer 
figures. 

So  the  logarithm  of  251  is  2  399674,  that  is,  the  decimal 
•399674  found  in  the  table,  with  the  index  2  prefixed,  because 
the  given  number  contains  three  integers.  And  the  log.  of 
94-09  is  1-532627,  that  is,  the  decimal  -532627  found  in  the 
table,  with  the  index  1  prefixed,  because  tho  given  number 
contains  two  integers. 

2.  But  if  the  given  Number  contain  more  than  four  figures ; 
take  out  the  logarithm  of  the  first  four  figures  by  inspection 
in  the  table,  as  before,  as  also  the  next  greater  logarithm, 
subtracting  the  one  logarithm  from  the  other,  as  also  their 
corresponding  numbers  the  one  from  the  other.   Then  say, 

As  the  difference  between  the  two  numbers, 

Is  to  the  difference  of  their  logarithms, 

So  is  the  remaining  part  of  the  given  number, 

To  the  proportional  part  of  the  logarithm. 

Which  part  being  added  to  the  less  logarithm,  before  taken 
out,  gives  the  whole  logarithm  sought  very  nearly. 


EXAMPLE. 

To  find  the  logarithm  of  the  number  34-0926. 
Tho  log.  of  340900,  as  before,  is  532627. 
And  log.  of  341000  -  -  is  532754. 
The  ditfs.  are  100      and  127. 


Then,  as  100  :  127  :  :  26  :  33,  the  proportional  part. 

This  added  to  -    -    -  532627,  the  first  log. 

Gives,  with  the  index,  1-532660  for  the  log.  of  34-0926. 

4.  If  the  number  consist  both  of  integers  and  fractions,  or 
is  entirely  fractional ;  find  the  decimal  part  of  the  logarithm 
the  same  as  if  all  its  figures  were  integral ;  then  this,  having 
prefixed  to  it  the  proper  index,  will  give  the  logarithm  re- 
quired. 

5.  And  if  the  given  number  be  a  proper  vulgar  fraction  : 
subtract  the  logarithm  of  the  denominator  from  the  loga- 
rithm of  the  numerator,  and  the  remainder  will  be  the  loga- 
rithm sought ;  which,  being  that  of  a  decimal  fraction,  must 

*"  always  have  a  negative  index. 

6.  But  if  it  be  a  mixed  number ;  reduce  it  to  an  impro- 
per fraction,  and  find  the  difference  of  the  logarithm  of  the 
numerator  and  denominator,  in  the  same  manner  as  before. 


156 


LOGARITHMS. 


EXAMPLES. 


1.  To  find  the  log.  of  J?. 
Log,  of  87      -  1-568202 
Log.  of  94      -  1-973128 


Dif.  log.  of»  J  —1-595074 


Where  the  index  1  is  negative 


2.  To  find  the  log.  of  17$f  • 
First,  17j|  =  Then, 
Log.  of  405    .  2-807455 
Log.  of  2ft      -  1-361728 

Difl  ]p|[.  of  17iJ  1-245727 


n.  TO  FIND  THE  NATUHAX  ITDMBSS  TO  ANY  GIVEN 
LOGARITHM. 

This  is  to  be  found  in  the  tables  by  the  reverse  method 
to  the  former,  namely,  by  searching  for  the  proposed  loga- 
rithm among  those  in  the  table,  and  taking  out  the  corre- 
sponding number  by  inspection,  in  which  the  proper  number 
of  integers  are  to  be  pointed  off,  viz.  1  more  than  the  index. 
For,  in  finding  the  number  answering  to  any  given  logarithm, 
the  index  always  shows  how  far  the  first  figure  must  be 
removed  from  the  place  of  units,  viz.  to  the  left  hand,  or  in- 
tegers,  when  the  index  is  affirmative ;  but  to  the  right  hand, 
or  decimals,  when  it  is  negative. 


EXAMPLES. 


So,  the  number  to  the  log.  ]h532S82  is  34-11. 
And  the  number  of  the  log.  "l'532b82  is  -3111. 

But  if  the  logarithm  cannot  be  exactly  found  in  the  table  ; 
take  out  the  next  greater  and  the  next  less,  subtracting  the 
one  of  these  logarithms  from  the  other,  as  also  their  natural 
numbers  the  one  from  the  other,  and  the  less  logarithm  from 
the  logarithm  proposed.    Then  say, 

As  the  difference  of  the  first  or  tabular  logarithms, 
Is  to  the  difference  of  their  natural  numbers, 
So  is  the  differ,  of  the  given  log.  and  the  least  tabular  log. 
To  their  corresponding  numeral  difference. 
Which  being  annexed  to  the  least  natural  number  above  ta- 
ken, gives  the  natural  number  sought,  corresponding  to  the 
proposed  logarithm. 


EXAMPLE. 


So,  to  find  the  natural  number  answering  to  the  given 
logarithm  1*532708. 


L04AJUTHM8.  157 

Here  the  next  greater  and  next  less  tabular  logarithms, 
trith  their  corresponding  numbers,  are  as  below : 

Next  greater  532754  its  num.  341000 ;  given  log.  532708 
Next  less     532627  its  num.  340900 ;  next  less  532627 

—  81 


learly  the  numeral  differ, 
i  is  the  number  sought,  marking  off  two 
integers,  because  the  index  of  th  e  given  logarithm  is  1. 
Had  the  index  been  negative,  thus  1-532708,  its  com- 
■  number  would  have  been  340964,  wholly  decimal. 


MULTIPLICATION  BY  LOGARITHMS. 


RULE. 


Take  out  the  logarithms  of  the  factors  from  the  table, 
then  add  them  together,  and  their  sum  will  be  the  logarithm 
of  the  product  required.  Then,  by  means  of  the  table,  take 
out  the  natural  number,  answering  to  the  sum,  for  the  pro- 
duct sought. 

Take  care  to  add  what  is  to  be  carried  from  the  decimal 
part  of  the  logarithm  to  the  affirmative  index  or  indices,  or 
else  subtract  it  from  the  negative. 

Also,  add  the  indices  together  when  they  are  of  the  same 
kind,  both  affirmative  or  both  negative  ;  but  subtract  the 
less  from  the  greater,  when  the  one  is  affirmative  and  the 
other  negative,  and  prefix  the  sign  of  the  greater  to  the  re- 
mainder. 


EXAMPLES. 


1.  To  multiply  23-14  by 
5062 
Numbers.  Logs. 
23  14  .  1-364363 
5  062  .  0-704322 


2.  To  multiply  2-581926 
by  8«457291 
Numbers.  Logs. 

2-  581920  .  0-411944 

3-  457291  .  0-538786 


**rodoct  117-1347  2  068685 


Prod.  8-92648   .  0-950680 


158 


DIVISION  BY  &OGABXTHK8. 


3.  To  mult.  3-902  and  597  16 
and  -0314726  all  together. 


Numbers. 
3-902 
597  16 
•0314728 


0-59F287  ! 
2-776091 
-2-497935 


Prod.  73-3333    .  1-865313 


Here  the  —  2  cancels  the  2, 
and  the  1  to  carry  from  the 
decimals  is  set  down. 


4.  To  mult.  3-586,  and  2-1046, 
and  0-8372,  and  0-0294  all 
together. 

Numbers.  Logs. 
3  586      -  0-554610 
2-1046     -    0  323170 
0-8372  ,  -1-922829 
0-0294  -2-468347 


Prod.  01857618  - 1  -268956 


Here  the  2  to  carry  cancels 
the  -2,  and  there  remains 
the  —1  to  set  down. 


DIVISION  BY  LOGARITHMS. 

RULE. 

From  the  logarithm  of  the  dividend,  subtract  the  loga- 
rithm of  the  divisor,  and  the  number  answering  to  the  re- 
mainder will  be  the  quotient  required. 

Change  the  sign  of  the  index  of  the  divisor,  from  affirm- 
ative to  negative,  or  from  negative  to  affirmative  ;  then  take 
the  sum  of  the  indices  if  they  be  of  the  same  name,  or  their 
difference  when  of  different  signs,  with  the  sign  of  the  greater, 
for  the  index  to  the  logarithm  of  the  quotient. 

Also,  when  1  is  borrowed,  in  the  left-hand  place  of  the 
decimal  part  of  the  logarithm,  add  it  to  the  index  of  the 
divisor  when  that  index  is  affirmative,  but  subtract  it  when 
negative  ;  then  let  the  sign  of  the  index  arising  from  hence 
be  changed,  and  worked  with  as  before. 


EXAMPLES. 


1.  To  divide  24163  by  4567. 

Numbers.  Logs. 
Dividend  24163  -  4  383151 
Divisor      4567  -  3-659631 


2.  To  divide  37 -1 49  by  523-76. 

Numbers.  Logs. 
Dividend  37149  -  1-569947 
Divisor    523-76  . 2  719132 


Quot.     5-29078  0-723520 


Quot.  -0709275-2-85081* 


UfTOLUTIOM  BY  LOGARITHMS. 


150 


8.  Divide  -06314  by  -007241 

Numbers.  Logs. 
Dividend  -06314-2-800305 
Divisor  -007241-3-859799 


4.  Todivide-7438by 12-9476. 

Numbers.  Logs* 
Divid.    -7438  -1-871456 
Divisor  12-9476  1-112169 


Quo*.     8-71979   0-940506    Quot.    -057447  -  2-750267 

.  '•'  v  — «— 

Here  1  ctjjirfcd  from  •  the       Here  the  1  taken  from  the 
decimals  to  pfc    8,  jnake*  it    —  1,  makes  it  become  —2,  to 
become  —  %        wen  from    set  down, 
the  other  —2,  leaves  0  re* 
maining. 

Note.  The  RuletaftThree,  or  Rule  of  Proportion,  is  per- 
formed by  adding  the  logarithms  of  tho  2d  and  3d  terms, 
jnnd  subtracting  that  of  the  first  term  from  their  sum.  In- 
stances will  occur  in  Plain  Trigonometry. 


INVOLUTION  BY  LOGARITHMS. 


RULE. 


Take  out  the  logarithm  of  the  given  number  from  the  ta- 
ble. Multiply  the  logarithm  thus  found,  by  the  index  of  the 
power  proposed.  Find  the  number  answering  to  the  product, 
and  it  will  be  the  power  required. 


Note.  In  multiplying  a  logarithm  with  a  negative  index, 
by  an  affirmative  number,  the  product  will  be  negative.  But 
what  is  to  bo  carried  from  the  decimal  part  of  the  logarithm, 
will  always  be  affirmative.  And  therefore  their  difference 
wilj  be  the  index  of  the  product,  and  is  always  to  be  made 
of  the  same  kind  with  the  greater. 


EXAMPLES. 


1.  To  square  the  number 
2-5791. 
Numb.  Log. 
Root  2-5791  -    -  0-411468 
The  index    -    -  2 


Power  6-65174  0-822936 


2.  To  find  the  cube  of 
3-07146. 
Numb.  Log. 
Root  3  07146  -  -  0-487345 
The  index    -    -  3 


Power  28-9758  1-462035 


■VOLUTION  BY  LOGARITHMS. 


3.  To  raise  •09163  to  the 
4th  power. 
Numb.  Log. 
Root  •09163  —2-962038 
The  index   -   -  4 


Pow.  -000070494— 5-848152 


Here  4  times  the  negative 
index  being  — 8,  and  3  to 
carry,  the  difference  —  5  is 
the  index  of  the  product. 


4.  To  raise  1*0045  to  the 
365th  power. 
Numb.  Log. 
Root  1  '0045  -    -  0-001950 
Thejndex    -    .  365 


9750 
■  11700 
5850 


0-711750 


EVOLUTION  BY  LOGARITHMS. 

Take  the  log.  of  the  given  number  out  of  the  table. 
Divide  the  log.  thus  found  by  the  index  of  the  root.  Then 
the  number  answering  to  the  quotient  will  be  the  root. 

Note.  When  the  index  of  the  logarithm,  to  be  divided 
is  negative,  and  does  not  exactly  contain  the  divisor,  without 
some  remainder,  increase  the  index  by  such  a  number  as 
will  make  it  exactly  divisible  by  the  index,  carrying  the  units 
borrowed,  as  so  many  tens,  to  the  left-hand  place  of  the  deci- 
mal, and  then  divide  as  in  whole  numbers. 


EXAMPLES. 


1.  To  find  the  square  root  of 
365. 

Numb.  Log. 
Power      365  2)  2-562293 
Root  19-10496  1-281146£ 


2.  To  find  the  3d  root  of 
12345. 
Numb.  Log. 
Power    12345  3)4  091491 
Root  231116  1-363830} 


3.  To  find  the  10th  root  of 
2. 

Numb.  Log. 
Power  2    -    10)  0-301030 
Root  1-071773  0-030103 


4.  To  find  the  365th  root  of 
1-045. 
Numb.  Log. 
Power  1  045  365)  0  019116 
Root    1-000121  0-000052| 


EVOLUTION  BY  tOGA 


161 


5-  To  find  </  <m. 

Numb.  Log* 
Power  093  2) —2-968483 
Root  -304959  —1-48424!* 

Here  the  divisor  2  is  con- 
tained exactly  once  in  the  ne- 
gative index  —  2,  and  there- 
fore the  index  of  the  quotient 
it  —  1. 


6*  To  find  the  -00048. 
Numb.  Log. 
Power  -00048  3)— 4-681241 
Root    -0782973  —2-893747 

Here  the  divisor  3,  not  being  exactly 
contained  in  —4,  it  is  augmented  by  2, 
to  make  up  6,  in  which  the  divisor  is 
contained  juit  2  timet;  then  the  2, 
thus  borrowed,  being  carried  to  the  de- 
'  *  aal  figure  6,  makes  86,  which  dividV 
by  S,  gives  8,  &c. 


7.  To  find  3-1416  X  82  X  ff- 

8.  To  find  029IG  X  751-3  X  flT 

9.  Afl  7241  :  3-58  :  :  20-46  :  ? 
10,  :  -v/ff  :  :  6-927  :  ? 


Vol.  I. 


22 


ALGEBRA. 


DEFINITIONS  AND  NOTATION. 

. 

1.  Algebra  is  the  science  of  investigation  by  means  of 
symbols.  It  is  sometimes  also  called  Analysis  ;  and  is  ft 
general  kind  of  arithmetic,  or  universal  way  of  computa- 
tion. 

2.  In  this  science,  quantities  of  all  kinds  are  represented 
by  the  letters  of  the  alphabet.  And  the  operations  to  to 
performed  with  them,  as  addition  or  subtraction,  &c.  are  de- 
noted by  certain  simple  characters,  instead  of  being  express- 
ed by  words  at  length. 

3.  In  algebraical  inquiries,  some  quantities  are  known  or 

E'ven,  viz.  those  whose  values  are  known  :  and  others  un- 
iown,  or  are  to  be  found  out,  viz.  those  whose  values  are 
not  known.  The  former  of  these  are  represented  by  the 
leading  letters  of  the  alphabet,  a,  b,  c,  d,  <3uc. ;  and  the  latter, 
or  unknown  quantities,  by  the  final  letters,  *,  y, «,  tt,  &c. 

4.  The  characters  used  to  denote  the  operations,  are 
chiefly  the  following : 

+    signifies  addition,  and  is  named  plus. 

—   signifies  subtraction,  and  is  named  minus. 

X    or  •  signifies  multiplication,  and  is  named  into. 

signifies  division,  and  is  named  by. 
y/   signifies  the  square  root ;      the  cube  root ;  (/  the 
4th  root,  dtc.  ;  and     the  nth  root. 
:  :  :      signifies  proportion. 
=s   signifies  equality,  and  is  named  equal  to* 
And  so  on  for  other  operations. 

Thus  a  +  b  denotes  that  the  number  represented  by  b  is 
to  be  added  to  that  represented  by  a. 

<x  —  6  denotes  that  the  number  represented  by  b  is  to  be 
subtracted  from  that  represented  by  a. 

a*b  denotes  the  difference  of  a  and  6,  when  it  is  not 
known  which  is  the  greater. 


vzrorrnoiai  jam  HbTATiozr.  163 

Hi,  or  a  X  b,  or  a  .  bf  expresses  the  product,  by  multipli- 
cation of  the  numbers  represented  by  a  and  4. 

a  -f-  ft,  or      denotes,  that  the  number  represented  by  a 
b 

is  to  be  divided  by  that  which  is  expressed  by  b. 

a  i  b  :  :  e  :  a\  signifies  that  a  is  in  the  same  proportion  to 
b>  as  e  is  to  a\  ,  .y 

#  ■=  a  —  &  4-  *  is  an  equation,  expressing  that  *  is  equal 
to  the  difference  of  a  and  b,  added  to  the  quantity  c. 

a,  or  a*,  denotes  the  square  root  of  a.;  $/a,  or  a^,  the 

eubexoot  of  a ;  and       or  a'  the  cube  root  of  the  square  of  a ; 

JL  * 

also  ^/a,  or  aw,  is  theath  root  of  a;  and  ^/anoram  is  the 

nth  power  of  the  mth  root  of  a,  or  it  is  a  to  the  —  power. 

fn 

a1  denotes  the  square  of  a  ;  a3  the  cube  of  a ;  a4  the  fourth 
power  of  a  ;  and  an  the  nth  power  of  a. 
a  +  b  X  c,  or  (a  +  b)  c,  denotes  the  product  of  the  com- 

6wnd  quantity  a  +  b  multiplied  by  the  simple  quantity  c. 
sing  the  bar  ,  or  the  parenthesis  (  )  as  a  vinculum,  to 

connect  several  simple  quantities  into  one  compound. 

a  +  b  -f-  a  —  b9  or  a-^"  ,,  expressed  like  a  fraction,  means 
a  —  o 

the  quotient  of  a  +  b  divided  by  a— b. 

i/ab  +  cd9  or  ^ai+crf)^,  is  the  square  root  of  the  com* 

pound  quantity  ab  +  cd.  And  e  y/  ab  +  or  c  (ab  +  cd)^9 
denotes  the  product  of  c  into  the  square  root  of  the  com- 
pound quantity  ab  +  cd. 

a  +  6  —  c3,  or  (a  +  b  —  cf  denotes  the  cube,  or  third 
power,  of  the  compound  quantity  a  +  b  —  c. 

8a  denotes  that  the  quantity  a  is  to  be  taken  3  times,  and 
4(a  +  b)  is  4  times  a  +  6.  And  these  numbers,  3  or  4, 
showing  how  often  the  quantities  are  to  be  taken,  or  multi- 
plied, are  called  Co-efficients. 

Also  fx  denotes  that  x  is  multiplied  by  {  ;  thus  J  Xx  or  Jx. 

5.  Like  quantities,  are  those  which  consist  of  the  same 
letters,  and  powers.  As  a  and  3a ;  or  2ab  and  4ab ;  or  30*60 
and  —  5a*ftc. 

6.  Unlike  Quantities,  are  those  which  consist  of  different 
letters,  or  different  powers.  As  a  and  b  ;  or  2a  and  a9 ;  or 
4aP  and  3abc. 

7.  Simple  Quantities  are  those  which  consist  of  one  tettft. 
only.   As  3a,  or  bob,  or  6ak?. 


1M  .* 


ALGEBRA. 


"  8.  Compound  Quantities  are  thoae  which  consist  of  two  or 
more  terms.    As  a+b,  or  2a— 3c,  or  a+2b  -  3c. 

9.  And  when  the  compound  quantity  consists  of  two  terms, 
it  is  called  a  Binomial,  as  a+b  ;  when  of  three  terms,  it  is  a 
Trinomial,  as  a+2b —  3c  ;  when  of  four  terms,  a  Quad ri no- 
mi  al,  as  2a  —  3b+c—4d ;  and  so  on.  Also  a  Multinomial  or 
Polynomial,  consists  of  many  terms. 

10.  A  Residual  Quantity,  is  a  binomial  having  one  of  the 
terms  negative.    Asa— 2b. 

11.  Positive  or  affirmative  Quantities,  are  those  which  are 
to  be  added,  or  have  the  sign  +.  As  a  or  +  a,  or  obi  for 
when  a  quantity  is  found  without  a  sign,  it  is  understood  to 
be  positive,  or  have  the  sign  +  prefixed. 

12.  Negative  Quantities,  are  those  which  are  to  be  sub- 
tracted*   As — a,  or  —2ab,  or  —  Sab\ 

*  13.  Like  Signs,  are  cither  all  positive  (  +  ),  or  all  nega- 
tive (  -  ). 

14.  Unlike  Signs,  are  when  some  are  positive  (  +  ),  and 
others  negative  ( — ). 

15.  The  Co-efficient  of  any  quantity,  as  shown  above,  is 
the  number  prefixed  to  it.    As  3,  in  (he  quantity  Sab. 

16.  The  power  of  a  quantity  (a),  is  its  square  (a8),  or  cube 
(a3),  or  biquadrate  (a4),  &c.  ;  called  also,  the  2d  power,  or 
3d  power,  or  4th  power,  &c. 

17.  The  Index  or  Exponent,  is  the  number  which  denotes 
the  power  or  root  of  a  quantity.  So  2  is  the  exponent  of 
the  square  or  second  power  a2 ;  and  3  is  the  index  of  the 

cube  or  3d  power  ;  and  £  is  the  index  of  the  square  root,  at 

or  y/a  ;  and  \  is  the  index  of  the  cube  root,  a^,  or 

18.  A  Rational  Quantity,  is  that  which  has  no  radical  sign 
or  index  annexed  to  it.    As  a,  or  Sab. 

19.  An  Irrational  Quantity,  or  Surd,  is  that  of  which  the 
value  cannot  be  accurately  expressed  in  numbers,  as  the 
square  root  of  2,  3^J^>  Surds  are  commonly  expressed  by 

means  of  the  radical  sign  </ :  as  y/2,  or  y/a,  or  -J/a",  or  a$. 

20.  The  Reciprocal  of  any  quantity,  is  that  quantity  in- 
verted,  or  unity  divided  by  it.    So,  the  reciprocal  of  a,  or 

is  i,  the  reciprocal  of  %  is     that  of  — ~  is  ^— -. 
la  b     a*  x  +  y  a 

21.  The  letters  by  which  any  simple  quantity  is  expressed, 
may  be  ranged  according  to  any  order  at  pleasure.  So  the 
product  of  a  and  b,  may  be  cither  expressed  by  ab,  or  ba ; 


DEFINITIONS  AND  NOTATION.  *  165 


and  the  product  of  a,  6,  and  c,  by  either  abcf  or  acb,  or  hoc, 
or  bca>  or  cab,  or  cba ;  as  it  matters  not  which  quantities  are 
placed  or  multiplied  first.  But  it  will  be  sometimes  found 
convenient  in  long  operations,  to  place  the  several  letters 
according  to  their  order  in  the  alphabet,  as  a  be,  which  order 
also  occurs  most  easily  or  naturally  to  the  mind. 

22.  Likewise,  the  several  members,  or  terms,  of  which  a 
compound  quantity  is  composed,  may  be  disposed  in  any 
order  at  pleasure,  without  altering  the  value  of  the  significa- 
tion of  the  whole.  Thus,  3a  — 2a6+4a6c  may  also  be  writ- 
ten  2a+4abc—2ab,  or  4abe+oa  -2ab9  or  -2ab+3a+4abc, 
fee. ;  for  all  these  represent  the  same  thing,  namely,  the 
quantity  which  remain^,  when  the  quantity  or  term  iab  is 
subtracted  from  the  sum  of  the  terms  or  quantities  3a  and 
4abc»  But  it  is  most  usual  and  natural,  to  begin  with  a  po- 
sitive term,  and  with  the  first  letters  of  the  alphabet. 


SOXV  EXAMPLES  FOR  PRACTICE. 


In  finding  the  numeral  values  of  various  expressions,  or  com- 
binations, of  quantities. 

Supposing  a=6,  and  b =5,  and  c=4,  and  a*=l,  and  e=0. 
Then 

1.  Will  aa  +  3aft-c3=36  +  90-16  =  110. 

2.  And  2a*-3a2b  +  c3=  432-540  +  (54  =  -  44. 

3.  And  a3  x(a+6)-2ate  =  36  X  11-240=156. 

a3  21ft 

4.  And         +c==^-  +  10  =  12+  16  =  28. 

5.  And  y/2ac+cr  or  (2ac  +  c3)^  =  y/64  =  8. 

A     A     1      /    _!_  2lfC       «         0_1_40  * 

6-  An(1^c  +  7C^H^)  =  2  +  ¥  =  7- 

*   a  j  <l3~"_v/(^3~~ac)  36  —  1  35  

7*  And  Sa-v/^+^T)  "  VJZ7  "  "5  ~7' 

8.  And  t/(*3-ac)+ v^(2flc+c»)=l  +  8=9. 

9.  And  v'^cT^^+f1)  =  vT25-2*  +  8)  =  3. 

10.  And  <r&  +  c-d  =  183. 

11.  And0a6-1062  +  c=24. 

3? 

12.  And  — -  X  d  =  45. 

c 

18.  Andl±*xj  =  13J. 


166 


AMKBRA. 


14.  And 


a+b    a  —  b 


=  1|. 


15.  And— +  e  =  45. 

c 

16.  And  —  X  «  =  0. 

c 

17.  And  (&  —  c)  X  (<*— 0  =  L 
ia  And  (a+  6)  —  (c  —  4)  =  8 

19.  And  (a  +  b)  —  c  —  d  ^  Q. 

20.  And  afc  X  (P=  144. 

21.  And  acd  —  d  =  23. 

22.  And  o%  +  Ve  +  d  =  V. 


23. 


Aod^X^^lSi. 


<J — e    c  —  d 


24.  And  v^a8  +  ft2  —       —  b'  =  4-4936249. 

25.  And  3ac»  +  i/a3  —  V  =  292-497942. 

26.  And  4a1  —  3a  ^a8  —  \ab  =  72. 


ADDITION. 

Addition,  in  Algebra,  is  the  connecting  the  quantities 
together  by  their  proper  signs,  and  incorporating  or  uniting 
into  one  term  or  sum,  such  as  are  similar,  and  can  be  united. 
As  3a  -f-  26  -  2a  =  a  +  2o,  the  sum. 

The  rule  of  addition  in  algebra,  may  be  divided  into  three 
cases  :  one,  when  the  quantities  are  like,  and  their  signs  like 
also  ;  a  second,  when  the  quantities  are  like,  but  their  signs 
unlike;  and  the  third,  when  the  quantities  are  unlike. 
Which  was  performed  jftfelows*. 


•The  reasons  on  which  these  operation!  are  founded,  will  readily  ap- 
pear, by  a  little  reflection  on  the  nature  of  the  quantities  to  be  added, 
or  collected  together.  For,  with  regard  to  the  first  example,  where 
the  quantities  are  3a  and  6a,  whatever  a  represents  in  the  one  term,  it 
will  represent  the  same  thing  in  the  other;  so  that  3  times  any  thing 
and  6  times  the  same  thing,  collected  together,  must  needs  make  8  times 
thatching.  As  if  a  denote  a  shilling ;  then  3a  is  3  shillings,  and  6a  is  6 
shillings,  and  their  sum  8  shillings.  In  like  manner,  —2ab  and  —  1mb9 
or  —2  times  any  thing,  and  —7  timet  the  same  thing,  make  — f>  times 
that  thing. 

*  i 


ADDITION. 


•  167 


CASE  I. 

When  the  Quantities  are  Like,  and  have  Like  Signs. 

Add  the  co-efficients  together,  and  set  down  the  sum  ; 
after  which  set  the  common  letter  or  letters  of  the  like  quan- 
tities, and  prefix  the  common  sign  +  or  — . 

Thus,  8a  added  to  6a,  makt  a  8a. 

And  — 2ab  added  to  —  7ab,  makes  —dab. 

And  5a  +  7b  added  to  7a  +  Ut  makes  12a  +  10*. 


;  FOR  PRACTICE. 

bxy 

9a 

—  5bx 

2bxy 

5a 

—  4bx 

5fey 

12a 

—  2bx 

bxy 

a 

—  7bx 

Zbxy 

2a 

—  bx 

Uxy 

32a 

—  22bx 

18bxy 

As  to  the  second  case,  in  which  the  quantities  are  like,  but  the  signs 
unlike;  the  reason  of  its  operation  will  easily  appear,  by  reflecting, 
that  addition  means  only  the  uniting  of  Quantities  together  by  means  of 
the  arithmetical  operations  denoted  by  their  signs-)-  and  — ,  or  of  addi- 
tion and  subtraction ;  which  being  of  contrary  or  opposite  natures,  the 
one  co-efficient  must  be  subtracted  from  the  other,  to  obtain  the  incor- 
porated or  united  mass. 

As  to  the  third  case,  where  the  quantities  are  unlike,  it  is  plain  that 
such  quantities  cannot  be  united  into  one,  or  otherwise  added,  than  by 
means  of  their  signs :  thus,  for  example,  if  a  be  supposed  to  represent 
a  crown,  and  6  a  shilling ;  then  the  sum  of  a  and  u  can  be  neither  2a 
nor  2*,  that  is,  neither  2  crowns  nor  2  shillings,  but  only  1  crown  plus  1 
•Billing,  that  is  a +6. 

In  this  rule,  the  word  addition  is  not  very  properly  used ;  being  much 
too  limited  to  express  the  operation  here  performed.  The  business  of 
this  operation  is  to  incorporate  into  one  mass,  or  algebraic  expression, 
different  algebraic  quantities,  as  far  as  asUStoa)  incorporation  or  union 
is  possible ;  and  to  retain  the  algebraic  sajfkslbr  doing  it,  in  cases  where 
the  former  is  not  possible.  When  wtfjlfo  several  quantities,  some 
affirmative  and  some  negative ;  and  the  relation  of  these  quantities  can 
in  the  whole  or  In  part  be  -  discovered ;  such  incorporation  of  two  or 
more  quantities  into  one,  is  plainly  effected  by  the  foregoing  rules. 

It  may  seem  a  paradox,  that  what  is  called  addition  in  algebra,  should 
sometimes  mean  addition,  and  sometimes  subtraction.  But  the  para- 
dox wholly  arises  from  the  scantiness  of  the  name  given  to  the  alge- 
braic process;  from  employing  an  old  term  in  a  new  and  more  enlarged 
sense.  Instead  of  addition,  call  it  incorporation,  or  union,  or  g&iking  a 
Islands,  or  give  it  any  name  to  which  a  more  extensive  idea  may  be 
annexed,  than  that  which  is  usually  implied  by  the  word  addition :  and 
the  paradox  vanishes. 


168  * 


AMBMU. 


3* 

dx*+5xy 

2<i*  — 4y 

2* 

**+  xy 

4ax —  y 

4s 

2*a+4*y 

ax  —  8y 

% 

5x*+2*y 

5ax —  5y 

6x 

4x*+3*y 

7ax —  2y 

15* 

5*y 
14xy 
22xy 
Ylxy 
l\xy 

\xy 


30- 

13**- 

-3*y 

23- 

10**- 

•4xy 

14- 

14**- 

•7xy 

10- 

16**- 

•5xy 

16- 

20**- 

'  x9 

5xy  — 3x  +  4a& 
8xy— 4x  +  Sab 
3xy — 5*  +  bob 
xy— 2*  +  afc 
4*y—  *  +  7ab 


CASE  II. 


When  the  Quantities  are  alike,  ha  have  Unlike  Signs. 

Add  all  the  affinnatif^co-efficients  into  one  sum,  and  all 
the  negative  ones  into'aoother,  when  there  are  several  of  a 
kind.  Then  subtract  the  less  sum,  or  the  less  co-efficient, 
from  the  greater,  and  to  the  remainder  prefix  the  sign  of  the 
greater,  and  subjoin  the  common  quantity  or  letters. 

So  +  5fg  and  —  3a,  united,  make  +  2a. 
And — 5a  and  —  3a,  united,  make  —  2a. 


ADDITION. 


169 


OTHER  EXAMPLES  FOE  PRACTICE. 


+  Qx*  +  3y 

-  5x*  +  4y 
— 16x3  +  by 
+  3s3  —  ly 
+  2X3  —  2y 

—  8x*  +  3y 


+  4ab+  4 

—  4ab  +  l2 
+  7ab— 14 
+  ab+  3 

—  bob— 10 


—  3ox* 
+  ax* 
+  5ax* 

—  6ax* 


H-lOv/ax 

—  3v/ax 
+  Ay/ax 

—  Yty/ax 


+  3y  +  4ax* 

—  y — bax^ 
+  4y  +  2ax* 

—  2y  +  6ax* 


case  m. 
When  the  Quantities  arc  Unlike. 

Having  collected  together  all  the  like  quantities,  as  in  the 
two  foregoing  cases,  set  down  those  that  are  unlike,  one  after 
another,  with  their  proper  signs. 

:W  - 
EXAMPLES.™ 

Sxy  6xy  —  12x*        4ax  —  130  +  3x* 

2ax        -4X1  +  3xy       Sx3  +  3ax  +  9*" 

-5xy        +4x«  -  2xy       Ixy  -  4x*  +  90 
fax        -3xy  +  4r»        yx  +  40  -Ox8 

—  2xy+8ax  4xy—  8x"        7ax  +  8x*  +  7xy 


Vol.  I. 


23 


170  ALGEBRA. 

9x  Y  1 4ax  -  2x*  9  +         x  —  5y 

-li*y  5ax  +  Zry  2x  +  7-/*?  +  5y 

+  3oxy  Sif  —  tex  5y  +  3^/ax  —  4y 

— 3xa  +  26  10—  Ay/ax  +  4y 


2-v/xy  +  14x 
3x  +  2y 
—9  +  3-v/jy 


Add  a+6  and  3a  —  56  together. 

Add  5a  —  8x  and  3a  —  4x  together. 

Add  6x- 56+a+8  to  —  5a  — 4r+4fc  —  3. 

Add  a+26-3c-10  to  36 -4a  +  5c  +  10  and  56 -c. 

Add  a +6  and  a  — 6  together. 

Add  3a  +  6-10  to>c-<*-a  and  — 4c  +  2a- 36 -7. 
Add  3aa+63-cto  2rt6-3«2+6c— -6. 
Add  a3+63c-62  to  a63~a6c+63. 

Add  9a-86  -f  10x-6a*-7c  +  50  to  $r-3a-5c  +46  +6d 
-10. 


SUBTRACTION. 

Set  down  in  one  line  the  first  quantities  from  which  the 
subtraction  is  to  be  made  ;  and  underneath  them  place  all  the 
other  quantities  composing  the  subtrahend  ;  ranging  the  like 
quantities  under  each  sifter,  as  in  Addition. 

Then  change  all  the  signs  (+  and  — )  of  the  lower  line, 
or  conceive  them  to  be  changed  ;  after  which,  collect  all  the 
terms  together  as  in  the  cases  of  Addition*. 


*  This  rule  is  founded  on  (he  consideration,  that  addition  and  sub- 
traction are  opposite  to  each  other  in  their  nature  and  operation,  as  are 
the  signs -{-and  — ,  by  which  they  are  expressed  and  represented.  So 
that,  since  to  unite  a  negative  quantity  with  a  positive  one  of  the  same 
kind,  has  the  effect  of  diminishing  it,  or  subducting  an  equal  positive 


•UBTRAOTIO.N. 


1T1 


XXAXPLK3. 

From  la%—  36  9x*  ~  4y  +  8  8xy  —  3  +  6z  —  y 
Take  2aa— 86       bV+5y-4      4xy  — 7  —  6x  —  4y 

*l*y  +  4  +  12x+3y 


—  20  — 6x— 5xy 
3xy  — 9x  X  8  —  2ay 

Rem.   7xy— 12    2$f£%fc  —  8    -r-28+3x  —  8ry+2ay 


From  8x»y  +  6  5>/xy  +  2xx/xy  7x3+  2^/z-  18+  36 
Take— 2x=y  +  2    7x/xy  +  S—2xy    Ox3— 12    +  56+  ** 

Rem. 


5xy  —  30  7x3  —  2  (a  +  b)  3xy7  +  20a  +  10) 
7xy  —  50       2x3~4(a  +  6)        Ixy  +  12a  y/(xy  +  10) 


Rem.  4a*+56      3x2— 9y+12 


From  5xy—  i\5^^  —  3y — 4 
Take— 2xy  +  6  -4Qfgjb+4 


From  a  +  6,  take  a  —  b. 
From  4a  +  46,  take  b  +  a. 
From  4a  —  46,  take  3a  +  56. 
From  8a —  12x,  take  4a  —  3x* 
From  2x  — 4a  — 26  +  5,  take  8—  56  +  a  +  6x. 
From3a  +  6+c  —  d  —  10,  takec  +  Ua  —  d. 
From  3a  +  b  +  c  —  d  —  10,  take  6—  10  +  3a. 
From  2a6  +  63  —  4c  +  be  —  6,  take  3a3  —  r  +  63. 
From  a3  +  36"c  +  06*  —  a6c,  take  62  +  a6a  —  a6c. 
From  12x  +  6a— 46  +40,  take  46  —  3a  +  4x  +  6d— 10. 
•  From  2x  —  3a  +  46  +  6c  —  50,  take  9a  +  x  +  66  —  6c 
 40. 

From  6a  —  46  —  12c  +  12x,  take  2a  —  8a  +  46  —  5c. 


^De  from  it,  therefore  to  subtract  a  positive  (which  is  the  opposite  of 
^anitiog  or  adding)  is  to  add  the  equal  negative  quantity.  In  like  map. 
-^«r,  to  subtract  a  negative  quantity,  is  the  same  in  effect  as  to  add  or 
***rfte  an  equal  positive  one.  So  that,  changing  the  sign  of  a  quantity 
^*om-fto— ,  or  from  —  to  -)-,  changes  its  nature  from  a  subductive 
Quantity  to  an  additive  one ;  and  any  quantity  is  in  effect  subtracted,  by 
<k*raly  changing  its  sign. 


TO 


AL6KBKA. 


MULTIPLICATION. 


This  consists  of  several  cases,  according  as  the  factors  are 
simple  or  compound  quantities. 

cash.    When  both  the  Factors  are  Simple  Quantities. 

Fcbst  multiply  the  co-efficienti  .of  ijie  two  terms  together, 
then  to  the  product  annex  all  the  letters  in  those  terms,  which 
will  give  the  whole  product  required. 

Note*.  like  signs,  in  the  factors,  produce  +,  and  unlike 
signs  — ,  in  the  products. 

EXAMPLES. 

10a         —2a  7a  —  6* 

2b  +  2b  -4c         —  4a 


20ab        —Sab       —28ac  +24ax 


*  That  this  rule  for  the  signs  is  true,  may  be  thus  shown. 

1.  When  -f-a  is  to  be  multiplied  by  +  e;  the  meaning  is,  that  +  *  is 
to  be  taken  as  many  times  as  there  are  units  in  c ;  and  since  the  sum  of 
any  number  of  positive  terms  is  positive,  it  follows  that  -faX+o 
makes  4-  ac 

2.  When  two  quantities  are  to  be  multiplied  together,  the  result  will 
be  exactly  the  same,  in  whatever  order  they  are  placed ;  for  a  times  c 
is  the  same  as  c  times  «,  and  therefore,  when  — a  is  to  be  multiplied  by 
+  $t  or  +  e  by  — a:  this  is  the  same  thing  as  taking  —  a  as  many  times 
as  there  are  units  in  4-c ;  and  as  the  sum  of  any  number  of  negative 
terms  is  negative,  it  follows  that  —  a  X  +  c,  or  +  a  X  —  • «  make  or  pro- 
duce —  ac. 

3.  When  —  a  is  to  be  multiplied  by  —  c :  here  —  a  is  to  be  subtract- 
ed as  often  as  there  are  units  in  c:  but  subtracting  negatives  is  the  same 
thing  as  adding  affirmatives,  by  the  demonstration  of  the  rule  for  sub- 
traction ;  consequently  the  product  is  c  times  a,  or  -f-  ac. 

Otherwise.  Since  a  —  a  =  0,  therefore  (a  —  a)  X  —  c  is  also  =  0,  be- 
cause 0  multiplied  by  any  quantity,  is  sUll  but  0 ;  and  since  the  flrst 
term  of  the  product,  or  a  X  —  c  is  =  —  ac,  by  the  second  case  ;  then*1 
fore  the  last  term  of  the  product,  or  —  a  X  —  c,  must  be  -f-  ac,  to  make 
the  sum  =  0,  or  —  tu+ac  =  0;  that  in, ,  —  a  X  —  c  =  ~|-  ac. 

Other  demonstrations  upon  the  principles  of  proportion,  or  by  menus 
of  geometrical  diagrams,  have  also  been  given  ;  but  the  above  may  «tf> 
ice. 


4oc 
-3a6 

— 12a36c 


Sax  — ax         +3jcy  — 5xyz 

4x  .yi  —6c  —4  -5ax 
—  >■*  ■  "  — — 


CASE  II. 

When  ome  of  ike  Factors  is  a  Compound  Quantity. 

Multiply  every  term  of  the  multiplicand,  or  compound 
quantity,  separately,  by  the  multiplier,  as  in  the  former 
case ;  placing  the  products  one  after  another,  with  the 
proper  signs ;  and  the  result  will  be  the  whole  product  re- 
quired* 


XULTIFUGATION.  173 

9a3*  — 2x*y  —4xy 

4x            3*^  — xy 

36aV  — 6fy  +4*V 


EXAMPLES. 


5a  —  3c  3ac  —  46  2a3  —  3c  +  5 
2a  3a  6c 


lOa^-Goc      Qa^  —  12a*      2a'bc-3bcl  +  56c 


12x-2ac 
4a 


25c  — 76 
-2a 


4x  —  6  +  3a6 
2a6 


3c3  +  i 
4xy 


10s*  —  3^ 
— 4X3 


8a3  —  2x3  —  66 
2a!3 


174 


ALGEBRA. 


CASS  III. 

When  both  the  Factors  are  Compound  Quantities  : 

Multiply  every  term  of  the  multiplier  by  every  term  of 
the  multiplicand  separately  ;  setting  down  the  products  one 
after  or  under  another,  with  their  proper  signs  ;  and  add  the 
several  lines  of  products  all  together  for  the  whole  product 


required. 

.A  v 

a+b  3x+2y  2&+*y  -  2jr» 

a+b  4x— by  3x— Sy 

a*+ab  lib*+8xy  6x3+ 3x^-6*^ 

+ab+b*  -  15xy-  I0y2  —6x2y—3xy3+6ys 

a*+2ab+b2  12X3— 7xy-l(y  6x3- 3x^-9x^+6^ 

a+b  x2+y  a'+ab+b* 

a — b  x2+y  a — b 

a*+ab  xx+yx*  a3+a~b+ab2 

— ab-b2  +yx3+if  —  a**— <*>*>'— V 

a*    *  x4+2yx3+3T  «3     *     *  — 63 


Note.  In  the  multiplication  of  compound  quantities,  it  is 
the  best  way  to  set  them  down  in  order,  according  to  the 
powers  and  the  letters  of  the  alphabet.  And  in  the  actual 
operation,  begin  at  the  left-hand  side,  and  multiply  from  the 
left  hand  towards  the  right,  in  the  manner  that  we  write, 
which  is  contrary  to  the  way  of  multiplying  numbers.  But 
in  setting  down  the  several  products,  as  they  arise,  in  the 
second  and  following  lines,  range  them  under  the  like  terms 
in  the  lines  above,  when  there  are  such  like  quantities  ; 
which  is  the  easiest  way  for  adding  them  up  together. 

In  many  cases,  the  multiplication  of  compound  quantities 
is  only  to  be  performed  by  setting  them  down  one  after 
another,  each  within  or  under  a  vinculum,  with  a  sign 
multiplication  between  them.    As  {a  +  b)  X  (a  —  b)  X 
or  a  +  b  .  a  — b  .  3a&.  „ 


DTVI8ION. 


175 


EXAMPLES  TOR  PRACTTCF. 


1 .  Multiply  10ac  by  2a. 

2.  Multiply  3aa  —  26  by  36. 

3.  Multiply  3a  +  26  by  3a  —  26. 

4.  Multiply  X3  —  xy  +     by  x  +  y. 


Ans.  20aV. 
Ans.  9a*b  —  662. 
Ans.  9aa  —  4o\ 
Ans.     +  y\ 


5.  Multiply  a3  +  af6  -f  a&2  +  63  by  a  —  6.    Ans.  a4  —  64. 

6.  Multiply  a8  +  ab  +  6*  by  a3  —  «6  +  63. 

7.  Multiply  3x*  —  2xy  +  5  by  x2  +  2xy  —  6. 

8.  Multiply  3a2  —  2**  +  bx1  by  3a2  —  4ax  —  7x2. 

9.  Multiply  3x3  +  2xy  +  3y3  by  2x3  —  3xY  +  3y\ 
10.  Multiply  a3  +  a6  +  6a  by  a  —  26. 


Division  in  Algebra,  like  that  in  numbers,  is  the  converse 
of  multiplication  ;  and  it  is  performed  like  that  of  numbers 
also,  by  beginning  at  the  left-hand  side,  and  dividing  all  the 
parts  of  the  dividend  by  the  divisor,  when  they  can  be  so 
divided  ;  or  else  by  setting  them  down  like  a  fraction,  the 
dividend  over  the  divisor,  and  then  abbreviating  the  fraction 
as  much  as  can  be  done.  This  may  naturally  be  distin- 
guished into  the  following  particular  cases. 


When  the  Divisor  and  Dividend  arc  both  Simple  Quantities  : 

Set  the  terms  both  down  as  in  division  of  numbers, 
either  the  divisor  before  the  dividend,  or  below  it,  like  the 
denominator  of  a  fraction.  Then  abbreviate  these  terms  as 
much  as  can  be  done,  by  cancelling  or  striking  out  all  the 
letters  that  are  common  to  them  both,  and  also  dividing 
the  one  co-efficient  by  the  other,  or  abbreviating  them  after 
the  manner  of  a  fraction,  by  dividing  them  by  their  common 
measure. 

Noli*    Like  signs  in  the  two  factors  make  + in  *ne  <luo" 
tient ;  and  unlike  signs  make  — ;  the  same  as  in  multipli- 
cation*. 


-  *  Became  the  divisor  multiplied  by  the  quotient,  must  product  lVv% 
dfridend.  Therefore, 


DIVISION. 


CASE  I. 


170 


ALOKBBA. 


EXAMPLES. 

1.  To  divide  Gab  by  3a. 

Here  Gab  -e-  3a,  or  3a  )  Gab  ( or  ^  =  26. 

~  c     ,       ,  ,       •        abx  a 

2.  Also  c-t-c  =  -  =  1;  and  ate     wry  =  7—  = 

c  oxy  y 

3.  Divide  lBx3  by  8x.  Ans.  2*. 

4.  Divide  12a8*2  by — 3a*x.  Ans.  —  4x. 

5.  Divide—  15ay* by  3ay.  Ans.  —  5*> 

9sy 

6.  Divide  —  18ax*y  by  —  Saxx.  Ans. 


CASE.  II. 

When  the  Dividend  i*  a  Compound  Quantity,  and  the  Divitor 
a  Simple  one. 

Divide  every  term  of  the  dividend  by  the  divisor,  as  in 
the  former  case. 

EXAMFLE8. 

1.  (ai  +  fta)H-26,or^a=^  =  *a  +  i6. 

2.  (10*6  +  15a*)  -s-  5a,  or  10fl6+15fl*  =26  +  3*. 

3.  (30az->48z)  -f  *,  or  30g*~48*  =  30a-48. 

4.  Divide  6ao— 8ax  +  a  by  2a. 

5.  Divide  Sx'-lS  +  6x  +  6a  by  3x. 


1.  When  both  the  terms  are  +, tbe  quotient  must  be  + ;  because  + 
in  the  divisor  X  +  in  the  quotient,  produces  -j-  in  the  dividend. 

2.  When  the  terms  are  both  — ,  the  quotient  is  also  + ;  because  — 
in  the  divisor  X  —  in  the  quotient,  produces  -f- ia  the  dividend. 

3.  When  one  term  is-f  and  the  other—,  the  quotient  must  be--; 
because  -f  in  the  divisor  X  —  in  the  quotient  produces  —  in  the  divi- 
dend, or  —  in  the  divisor  X  +  in  the  quotient  gives  —  in  the  dividend. 

So  that  the  rule  is  general ;  vis.  that  like  signs  give  +,  and  unlike 
**ffn*  give  — ,  in  the  quotient. 


DIVISION. 


6.  Divide  6abc  +  \2abx  —  9a*b  by  Sab. 

7.  Divide  lOa*x  -  25*  by  5x. 

8.  Divide  I5a2be  —  Ibacx*  +  bad?  by  —  5ac. 

9.  Divide  15a  +  Say  -  lSy8  by  21a. 
10.  Divide  -  2(W868  +  OOab3  by  -  Qab. 


CASE  III* 

TFAen      Divisor  and  Dividend  are  both  Compound 
Quantities. 

1.  Set  them  down  as  in  common  division  of  numbers, 
the  divisor  before  the  dividend,  with  a  small  curved  line  be- 
tween them,  and  range  the  terms  according  to  the  powers  of 
aomo  one  of  the  letters  in  both,  the  higher  powers  before  the 
lower. 

2.  Divide  the  first  term  of  the  dividend  by  the  first  term 
of  the  divisor,  as  in  the  first  case,  and  set  the  result  in  the 
quotient. 

3.  Multiply  the  whole  divisor  by  the  term  thus  found,  and 
subtract  the  result  from  the  dividend. 

4.  To  this  remainder  bring  down  as  many  terms  of  the 
dividend  as  are  requisite  for  the  next  operation,  dividing  as 
before  ;  and  so  on  to  the  end,  as  in  common  arithmetic. 

Note.  If  the  divisor  be  not  exactly  contained  in  the  divi- 
dend, the  quantity  which  remains  after  the  operation  is 
%  finished  may  be  placed  over  the  divisor,  like  a  vulgar  frac- 
tion, and  set  down  at  the  end  of  the  quotient  as  in  arith- 
metic. 


EXAMPLES. 

a  -  b)  aa-  %tb  +  b*  (a  -  b 
a3  -  ab 


-ab  +  V 
-  ab  +  ^ 


Vol.  I. 


24 


178  ALGEBRA. 

a  -  c)  a3  —  4a9c  +  4^  -  c3  —  (a3  —  3ac  + 


-  3«3c  +  W 

-  3a*c  +  3'^ 


oc3  -c1 
ac3  -  c3 


«_  2)  a3  —  6a3  +  12a  -  8  (a3  -  4a  +  4 
a3 -2d3 


-  4a2  +  12a 

-  4a3  +  8a 


4a  —  8 

4a  —  8 


«  +  *)  a*  -  3x4  (a3  -  a3*  +  ax3  —  ~3  - 


a4  +  a3x  a  +  * 


—  a3*  -  3x* 

—  a3x  —  aV 


aV  -  3x4 
a3x3  -f  •  ax3 


—  ar3  -  3x* 


-  2x4 


EXAMPLES  FOB  PRACTICE. 

1.  Divide  a3  +  4ax  +  4x3  by  a  +  2x.        Ans.  a  +  2*. 

2.  Divide  a3  -  3a3z  +  3a*3  -  z3  by  a  -  z. 

Ans.  a3  —  2az  +  z\ 

3.  Divide  1  by  1  +  a.       Ans.  1  -  a  +  a2  —  a3  +  &c. 

4.  Divide  12x4  —  102  by  3x  -  6. 

Ans.  4x3  +  Sx2  +  16x  +  32. 

5.  Divide  a5  -  5a46  +  10a363  -  10a363  -f  5a64  —  b*  by 

a3  -  2a&  +  b\  Ans.  a3  -  3a36  +  Sab2  -  6'. 


FRACTIONS.  179 

6.  Divide  48s3  -  96a*3  -  64a2z  +  150a3  by  2z  -  3a. 

7.  Divide  b*  —  36  V  +  362x4  —  x*by  63  —  2b'x  +  36s3 

—  x3. 

8.  Divide  a1  —  x7  by  a  —  x. 

■    9.  Divide  a3  +  5a?x  +  5ax3  +  x3  by  a  +  x, 
10.  Divide  a4  +  4a263  —  326*  by  a  +  26. 
Ik  Divide  24a4  —  6<  by  3a  —  26. 


ALGEBRAIC  FRACTIONS. 

Algebraic  Fractions  have  the  same  names  and  rales  of 
operation,  as  numeral  fractions  in  common  arithmetic  ;  <as 
Appears  in  the  following  Rules  and  Cases. 


To  reduce  a  Mixed  Quantity  to  an  Improper  Fraction. 

Multiply  the  integer  by  the  denominator  of  the  fraction, 
and  to  the  product  add  the  numerator,  or  connect  it  with 
its  proper  sign,  4"  or  —  ;  then  tho  denominator  being  set 
under  this  sum,  will  give  the  improper  fraction  required. 

EXAMPLES. 

1.  Reduce  3},  and  a  ^-  to  improper  fractions. 

OA     (3X5) +4     15  +  4     10  ,  . 
First,  3|  =  ~- —  =  — =  —  the  Answer. 

And,  a  —  -  =  (aXar)~^_  =  — — -  the  Answer. 
xx  x 
a2  zi  aa 

2.  Reduce  a  +  -p  and  a  to  improper  fractions. 

o  a 

«.   .       ,  a2      (a  X  6)  +  a3      a6  +  a2   ,  A 


.  180  ALGEBRA. 

3.  Reduce  5f  to  an  improper  fraction.  An*.  V  • 

4.  Reduce  1  —  ^  to  an  improper  fraction.  Ans. 

5.  Reduce  2a  —  **gx     a  ^  an  improper  fraction. 

4x 
4r  18 

6.  Reduce  12  -|  jr- —  to  an  improper  fraction. 

1  —  3a  c 

7.  Reduce  x  H  —  to  an  improper  fraction. 

2r*  3a 

8.  Reduce  4  +  2x  : — —  to  an  improper  fraction. 

CA8k  II. 

To  reduce  an  Improper  Fraction  to  a  Whole  or  Mixed 
Quantity. 

Divide  the  numerator  by  the  denominator,  for  the  inte- 
gral part;  and  set  the  remainder,  if  any,  over  the  denomina- 
tor, for  the  fractional  part  ;  the  two  joined  together  will  be 
the  mixed  quantity  required. 


EXAMPLES. 

1.  To  reduce     and  to  mixed  quantities. 

o  o 

First,  y  =  16  -T-  3  =  5J,  the  answer  required. 
And,  ^^g—  =  (ab  +  a2)  -r-  b  =  a  +  Answer. 

2ac  —  3a3     ,3ax  +  4xf 

2.  To  reduce  und  ,         to  mixed  quanti- 

c  a  +  x 

ties.  « 

2ac  —  So2     M        n  nK                  3a2  _ 
First,  =  (2ac  —  3a2)     c  =  2a  .  Answer. 

3ax+4xa  x2 

And,  Ip_==(3ax+4x2Wa+s)=3x+— -  Ans. 

a+x       x  /    \       /  a+x 

_       ,      33     _  2ax  —  3x>        .  , 

3.  Reduce  —  and  to  mixed  quantities. 

3x* 

Ans.  6|,  and  2x  — . 

4aax        2n2  -f-  26 

4.  Reduce        and  — - — - —  to  whole  or  mixed  quan- 

dties. 


FRACTIONS.  181 

5.  Reduce  ****  ,  ^  and  ^     ^  to  whole  or  mixed 

x+y  x—y 

quantities. 

a  D  .      10a1  — 4a  +  6  4        .  , 

o.  Reduce  —  to  a  mixed  quantity. 

7.  Reduce  r- rr~a  «          to  a  mixed  quantity. 

Sa1  +  2a9  —  2a  —  4  n  ' 


case  in. 


To  reduce  Fractions  to  a  Common  Denominator. 

Multiply  every  numerator,  separately,  by  all  the  deno- 
minators except  its  own,  for  the  new  numerators  ;  and  all  the 
denominators  together,  for  the  common  denominator. 

When  the  denominators  have  a  common  divisor,  it  will  be 
better,  instead  of  multiplying  by  the  whole  denominators,  to 
multiply  only  by  those  parts  which  arise  from  dividing  by 
the  common  divisor.  Observing  also  tho  several  rules  and 
directions,  as  in  Fractions  in  the  Arithmetic. 


EXAMPLES. 

1.  Reduce  -  and  -  to  a  common  denominator. 

x  z 

Here  -  and  -  =  a%  and  — ,  by  multiplying  the  terms  of 
x       z      tz  xz 

the  first  fraction  by  z,  and  the  terms  of  the  2d  by  x. 

2.  Reduce  -,     and  —  to  a  common  denominator. 

x  o  c 

n      a  x      j  &      abc  ex7       ,  b*x  . 

Here  - ,  - ,  and  —  =  —  and  7 — ,  by  multiplying  the 

x    b  c       bcx  bcx         bcx  r  J  ° 

terms  of  the  1st  fraction  by  be,  of  the  2d  by  cx,  and  of  the  3d 
by  bx. 

3.  Reduce  —  and  ^  to  a  common  denominator. 

x  2c 

4ac     ,  Sbx 
Ans.  — -  and  — . 
2cx  2cx 

4.  Reduce  ^  and  — -  to  a  common  denominator. 

b  2c 

k      4ac      ,  3ab+2b* 
Ans.^and— b— , 


182  ALGEBRA. 

5a  36 

5.  Reduce     and      and  4 a*,  to  a  common  denominator. 

Sx  2c 

lOffc     ,06a:     J  24cox 
Ans.  - —  and  —  and  — —  • 
hex        ocx  ocx 

6.  Reduce  jj  and      and  26+  ~,  to  fractions  having  a  com- 

4      206     ,18a6      J  4862+72a 

mon  denominator.  Ans.  -  —  and  --r-,  and  — -rn  . 

246      246  246 

1       2a2  2tt3+63 

7.  Reduce  -  and  —  and  — r-r~  to  a  common  denomina- 

3        4  o+6 

tor. 

8.  Reduce  —  and      and  ^-  to  a  common  denominator. 

4us       3a  2a 


CASE  IV. 


Tb  find  the  greatest  common  Measure  of  tlie  Terms  of  a 
Fraction. 

Divide  the  greater  term  by  the  less,  and  the  last  divisor 
by  the  last  remainder,  and  so  on  till  nothing  remains  ;  then 
the  divisor  last  used  will  be  the  common  measure  required  ; 
just  the  same  as  in  common  numbers. 

But  note,  that  it  is  proper  to  range  the  quantities  accord- 
ing to  the  dimensions  of  some  letters,  as  is  shown  in  division. 
Note  also,  that  all  the  letters  or  figures  which  are  common 
to  each  term  of  the  divisors,  must  be  thrown  out  of  them,  or 
must  divide  them,  before  they  are  used  in  the  operation. 


EXAMPLES. 


1.  To  find  the  greatest  common  measure  of  — ^r-r  „» 

arJ+6cJ 

a6  +  63)  or2  +  be2 
or  a  +  6  )  ac2  +  bcz  (c2 
ac3  +  6c2 


Therefore  the  greatest  common  measure  is  a  +  6. 


a3— n6a 


2.  To  find  the  greatest  common  measure  of  — — -r-j-r,. 

a-+2a64-61 


FRACTIONS.  188 


a*+2ab+P)  a3— <io3  (a 


— tab— 2ab2)  a2  4-  2*6  +  63 
or       a-f    6  )  <r  +  2ab  +  b*  (a  +  b 
am  4-  a6 


oA  +  ft2 
ab  +  b1 

Therefore  a-\-b  is  the  greatest  common  divisor. 

a3— 4 

3.  To  find  the  greatest  common  divisor  of  ^q^- 

Ans.  a  —  2» 

4.  To  find  the  greatest  common  divisor  of  "r^gr- 


5.  Find  the  greatest  com.  measure  of  —-—r.-r.r-r  —r-—7-rm  • 

CASK  V. 

To  reduce  a  Fraction  to  its  lowest  Terms, 

Find  the  greatest  common  measure,  as  in  the  last  pro- 
blem. Then  divide  both  the  terms  of  the  fraction  by  the  com- 
mon measure  thus  found,  and  it  will  reduce  it  to  its  lowest 
terms  at  once,  as  was  required.  Or  divide  the  terms  by  any 
quantity  which  it  may  appear  will  divide  them  both  as  in 
arithmetical  fractious. 

EXAMPLES. 

,    n  ,       ab+b*      .  t 
1.  Reduce  — z~~r~. — :» to  its  lowest  terms. 
ac2+bc* 

ab+b2)  ar'+bc1 
or  a +6  )  ucP+bc2  (c3 
ac-+b(r 


Here  ab-\-b2  is  divided  by  the  common  factor  b. 
Therefore  a  +  b  is  the  greatest  common  measure,  and 

hence  a+b)  rf^^",^r=-?>  is  the  fraction  required. 

acr-\-bcr  <r 

S-b-c         .  , 
2.  To  reduce  -r-r-r-.    .  ...  to  its  least  terms. 
cr+%bc+b* 


184  ALOEBRA. 

Hero,  by  a  process  similar  to  that  of  Ex.  2,  Case  rv.9  we 
find  c  +  b  is  the  greatest  common  measure,  and  hence 

e  +  b)  -f      °  -;.=C  .  ^C  is  the  fraction  required. 
T  '  c*+2bc  +  b9     c+b  M 

c3— ft3  c*+bc+V 

3.  Reduce  -r — rrs  t0  its  lowest  terms.     Ans.  .-?-,-» 

 £i  J 

4.  Reduce  n to  its  lowest  terms.  Ans. 

a' — o  ar-x-or 

a1— o4  .  , 

5.  Reduce  -= — 5-^-7-0—53 — TJ to  lts  lowest  terms. 

a3 — Serb +3*oa—  oJ 

6.  Reduce  -1-T-0-~i-r.  0   ,  ,  .  to  its  lowest  terms. 

a3c +3aV+3ac3+c* 


CASE  VI. 

To  aaV2  Fractional  Quantities  together. 

If  the  fractions  have  a  common  denominator,  add  all  the 
numerators  together  ;  then  under  their  sum  set  the  common 
denominator,  and  it  is  done. 

If  they  have  not  a  common  denominator,  reduce  them  to 
one,  and  then  add  them  as  before. 

EXAMPLES. 

1.  Let  ~  and      be  given,  to  find  their  sum. 

a   .  a      4a  ,  3a     7a  . 
Here  —  +  —  =  ^  +      «F     is  the  sum  required. 

2.  Given      — ,  and      to  find  their  sum. 

be  a 

_..      a  ,    6       c     aco*  ,  66d  ,bcc  acd4-6W+occ 

Uere  y  +  7  +  7,=  kS+  6^+6^  "635" 

the  sum  required. 

3s2  2ax 
*  3.  Let  a  —      and  6  +       be  added  together. 


*  In  the  addition  of  mixed  quantities,  it  is  best  to  bring  the  fractional 
parts  only  to  a  common  denominator,  and  to  annex  their  sum  to  the  ram 
of  the  integers,  with  the  proper  sign.  And  the  same  rule  may  be  ob- 
served for  mixed  quantities  in  subtraction  also. 

See,  also,  the  note  to  Addition  of  Fractions  in  the  Arithmetic. 


FRACTIONS.  185 

Here  a  — r-  +  6  H  =  a  7  r  0  +  — — 

b  c  be  be 

.  .  ,  2abx-3cx*  .  . 

=  a  +  H  £  9  the  sura  required. 

be 

,    ...4*  .  .  20ta+6ax 

4.  Ada  jr-  and  -=r  together.  Ans.  - — — — 7 — . 

3a       56    6  15a6 

5.  Add  ~,  ~  and      together.  Ans.  £{a. 

«   AJJ  2a— 3     .5a       .  .      9a -6 

6.  Add  — - —  and  —  together.  Ans.  — - — . 

7.  Add  2a  -|  —  to  4a  -\  Ans.  Ga  Hf  ^ — . 

O  4  *U 

8.  Add  6a,  and  ^  and  -^jp  together. 

o   a^5*     j  6a  ,3a+24 

9.  Add  — ,  and  —  and  — — —  together. 

10.  Add  2a,  and  ~  and  3  +  ^  together. 

11.  Add  8a  +  ^  and  2a  — ^  together. 


,  CASE  VII. 

To  subtract  one  Fractional  Quantity  from  another. 

Reduce  the  fractions  to  a  common  denominator,  as  in 
addition,  if  they  have  not1  a  common  denominator. 

Subtract  the  numerators  from  each  other,  and  under  their 
difference  set  the  commoi  denominator,  and  the  work  is 
done. 

EXAMPLES. 


3a  4a 

1.  To  find  the  difference  of  —  andy. 

„     3a     4a     21a     16a     5a .    .    J  ir  .  , 

Here  —  —  y  =  — -  —  — -  =  ^  is  the  d  ffer.  lequired. 

2*  To  find  the  difference  of  ^7  --  -  and 

4c  36 

Vol.  I.  25 


difference  of  &»  ■»*  "4* 

4.         ^  ^  4* 

7.  T«k«  — 


9  2a 
from  4a  c 

cask  vin. 


Beto-g-Jt5     40       ,  ______ 


to* 


FRACTIONS. 


187 


2.  Required  the  product  of  |,  ~,  and  5?. 
TxTxT  "^-H^e  product  required. 

3*  Required  the  product  of  ~  and  !^p~* 

„  2m  x  (a  +  b)  2aa  +  2ab.  _  _ 
H6r6  6— (2T+T)  =  23T+-£  ^  produCt 

4a  6a 

4.  Required  the  product  of  7  and  -r-  • 

O  DC 

5.  Required  the  product  of  ^  and  —j*. 

6.  To  multiply  y,  and  ~9  and  ^  together. 

ao  3a* 

7.  Required  the  product  of  2a  +  -g^and 

o.  Required  the  product  of — — and  ^     ^  ». 

2a  4-1       2a—  1 
9.  Required  the  product  of  8a,  and  — - —  and 

10.  Multiply«  +  ±-^byr-£  +  ^. 


CASE  IX. 


To  oroide  one  Fractional  Quantity  by  another. 

Divide  the  numerators  by  each  other,  and  the  deno- 
minators by  each  other,  if  they  will  exactly  divide.  But,  if 
•Hot,  then  invert  the  terms  of  the  divisor,  and  multiply  by  it 
exactly  as  in  multiplication*. 


*  1.  If  the  fraction!  to  be  divided  have  a  common  denominator,  take 
the  numerator  of  the  dividend  for  a  new  numerator,  and  tfae  numerator 
"Of  the  divisor  for  the  new  denominator. 

ft.  When  a  fraction  is  to  be  divided  by  any  quantity,  it  is  the  tame 
thing  whether  the  numerator  be  divided  by  it,  or  the  denominator  mul- 
tiplied by  it 

8.  When  the  two  numerators,  or  the  two  denominators,  can  be  divi- 
ded by  some  common  quantity,  let  that  be  done,  and  the  ajtttUM&iwA  ' 
Instead  ef  the  fractions  first  propweiL 


188 


ALGEBRA. 


EXAMPLES. 


a  3a 

1.  Required  to  divide  -  by 

a     3a     a     8      8a      2  . 
Herei  +  T  =4  X  3a  =  I2S  "  3 *e  qU0Uent' 

2.  Required  to  divide  ?^  by 

w     3a      5c     3a     4d     I2ad     6ad  _ 

Here  »  +  45  =  26  X  5c  =  TOfc  =  56?  the  qUOUenU 

«  m  j        2a+6  _    3a+26  „ 

3.  Todmde— -6by— Here, 

2a+6  w  4a+6      8a*+6ab+b*  _ 
3a--26  X  3a+26  =  Tra*- tbe  qUOtMmt  n^md^ 

4.  To  divide  ^r-3 by-  a 


a3+63  Ja+&' 

H     —      a+6_3aaX(a+6)_  3a  . 

6  aM-6>  X    a        (a3+63)  Xa     a*  —  ab  +  6*  18 
quotient  required. 

5.  To  divide  —  by  ~. 

4  J  12 

6.  To  divide  -f  by  3x. 

5 

7.  To  divide  — - —  by  — « 

8.  To  divide  jr^--  Ly^. 

4>X. —  1  u 

9.  To  divided  by  I?. 

5  3  56 

10.  Todividc^by^-. 

4ca  oa 

„   _.  . .      5a4- to  f5a6 

11.  Dmde^-^^by 


160 


INVOLUTION. 

Involution  is  the  raising  of  powers  from  any  proposed 
root  ;  such  as  finding  the  square,  cube,  biquadrate,  &c.  of 
any  given  quantity.    The  method  is  as  follows. 

*  Multiply  the  root  or  given  quantity  by  itself,  as  many 
times  as  there  are  units  in  the  index  less  one,  and  the  last 
product  will  be  the  power  required.  Or,  in  literals,  mul- 
tiply the  index  of  the  root  by  the  index  of  the  power,  and 
the  result  will  be  the  power,  the  same  as  before. 

Note.  When  the  sign  of  the  root  is  +,  all  the  powers  of 
it  will  be  +  ;  but  when  the  sign  is  — ,  all  the  even  powers 
will  be  +,  and  all  the  odd  powers  — ;  as  is  evident  from  mul- 
tiplication. 


examples. 


a,  the  root 
a3  3=  square 
a3  =  cube 
a4  =  4th  power 
a1  =  5th  power 
6zc. 

a9,  the  root 
a4  ~  square 
a6  =  cube 
a"  =  4th  power 
a,0=  5th  power 
dec. 

— *  2a,  the  root 
+*  4aa  =  square 

—  8a3  =-  cube 

+  16a4  =  4th  power 

—  32a5  =  5ih  power 

—  3ab*,  the  root 
+    9c?b*  =  square 

—  270*6*=  cube 

+  81a46f  =  4th  power 
— 243a,6ie=  5th  power 

2ar2 
—        the  root 

,  4aV 

+  .—  =  square 

8aV 

—  =  cube 

276* 

+  -Qj-6T  4th  Power 

^g,  the  root 
aa 

4^  =  square 

?L  =cube 
a3 

1664  =  bi(luadrate 

*  Any  power  of  the  product  of  two  or  more  quantities,  is  equal  to 
the  tame  power  of  each  of  the  factors,  multiplied  together. 

And  any  power  of  a  fraction,  is  enual  to  the  same  noyr*T  cA  tab  trap 
aerator,  divided  by  the  like  power  of  the  denominator* 


190  ALOBBBA. 

x — a =root  x+  a=root 

x — a  x+a 


x2 — ax  x9  +  ax 

— at  +  a*  +ax  +  a* 


Xs — 2ax  +  a2  square  x*  +  2ax  +  a9 

x — a  x  +  a 


x5— 2axa+oax  x3  +  2a*8  f  a1* 

—ax2  +2a»x— a3  +  ax3  +  2aax  +  «* 


x3— 3ax*  "4*  Sa'x-— a3  x3  +  Sax2  +  So3*  +  a3 


the  cubes,  or  third  powers,  of  x  —  a  and  x  +  a. 


KXAMJ  LES  FOR  PRACTICE. 

1.  Required  the  cube  or  3d  power  or  3aa. 

2.  Required  the  4th  power  of  2asb.  # 

3.  Required  the  3d  power  of —  4aao3. 

Q^X 

4.  To  find  the  biquadrate  of  —  ~a. 

5.  Required  the  5th  power  of  a  —  2x. 

6.  To  find  the  6th  power  of  2a*. 

Sir  Isaac  Nekton's  Rule  for  raising  a  Binomial  to*any 
Power  whatever* :.  # 

1.  To  find  the  Terms  without,  the  Co-efficients.  The  inder. 
of  the  first,  or  leading  quantity,  begins  with  the  index  of  the 
given  power,  and  in  the  succeeding  terms  decreases  con- 
tinually by  1,  in  every  term  to  the  last  ;  and  in  the  2d  or 


Alto,  powers  or  roots  of  the  same  quantity,  are  multiplied  by  one> 
another,  by  adding  iheir  exponents ;  or  divided,  by  subtracting  their 
exponents. 

aa 

Thus,  «3  X«*  =  aa+a  =  as.   And  as  -f-aa  or — =  as— a  —  a. 

as 

*  This  rule,  expressed  in  general  terms,  is  as  follows: 
<.+x)*=a^».  a-ix+n  .  "^a^a-j-n.  'I"1 .  "^-v  ^ 

<«-^)»^-«.a»-ix4-n  .  *^la*~  z"-n.  *~l  .n^2a --y  Ac. 
/toil.   Xb*  ma  of  the  co-efficienU,  In  every  power,  it  equal  Co  ther- 


INVOLUTION. 


101 


following  quantity,  the  indices  of  the  terms  are  0t  1,2,  3,  4, 
&c.  increasing  always  by  1.  That  is,  the  first  term  will  con- 
tain only  the  1st  part  of  the  root  with  the  same  index,  or  of 
the  same  height  as  the  intended  power :  and  the  last  term-  of 
the  series  wUl  contain  only  the  2d  part  of  the  given  root, 
when  raised  also  to  the  same  height  of  the  intended  power  : 
bat  all  the  other  or  intermediate  terms  will  contain  the  pro- 
ducts of  some  powers  of  both  the  members  of  the  root,  in 
such  sort,  that  the  powers  or  indices  of  the  1st  or  leading 
member  will  always  decrease  by  1,  while  those  of  the  2d 
member  always  increase  by  1. 

2.  To  find  the  Co  efficients.  The  first  co-efficient  is  al- 
ways 1,  and  the  second  is  the  same  as  the  index  of  the  in- 
tended power ;  to  find  the  3d  co-efficient,  multiply  that  of  the 
2d  term  by  the  index  of  the  leuding  letter  in  the  same  term, 
mod  divide  the  product  by  2 ;  and  so  on,  that  is,  multiply  the 
co-efficient  of  the  term  last  found  by  the  index  of  the  leading 
quantity  in  that  term,  and  divide  the  product  by  the  number 
of  terms  to  that  place,  and  it  will  give  the  co-efficient  of  the 
term  next  following  ;  which  rule  will  find  all  the  co-efficients, 
one  after  another. 

Note.  The  whole  number  of  terms  will  be  1  more  than 
the  index  of  the  given  power  :  and  when  both  terms  of  the 
root  are  +  ,  all  the  terms  of  the  power  will  be  +  ;  but  if  the 
second  term  be  — ,  all  the  odd  terms  will  be  +  >  and  all  the 
even  terms  — ,  which  causes  the  terms  to  be  +  and  —  alter- 
nately. Also  the  sum  of  the  two  indices,  in  each  term,  is 
always  the  same  number,  viz.  the  index  of  the  required 
power ;  and  counting  from  the  middle  of  the  series,  both 
ways,  or  towards  the  right  and  left,  the  indices  of  the  two 
terms  are  the  same  figures  at  equal  distances,  but  with  mutu- 
ally changed  places.  Moreover,  the  co-efficients  are  the 
same  numbers  at  equal  distances  from  the  middle  of  the  se- 
ries, towards  the  right  and  left ;  so  by  whatever  numbers 
they  increase  to  the  middle,  by  the  same  in  the  reverse  order 
they  decrease  to  the  end. 


number  2,  when  raised  to  that  power.  Thus  1— |— 1  =  2  in  the  first  power ; 
1+2+1  =4=2- in  the  square;  1 +3  + 3  + 1  =  8  =2*  in  the  cube, 
or  third  power  :  and  so  on. 

A.  trinomial  or  a  quadrinomial  may  be  expanded  in  the  same  manner. 
Thua,  to  raise  a  —  ft  +  c — d  to  the  6th  power,  put  a — b  =  x,  e  —  d—z, 
mod  raise  i  +  z  to  the  6th  power ;  after  which  substitute  for  the  powers 
of  x  and  y  their  corresponding  values  in  terms  of  o— b,  aad  c—  d,  and 
their  powers  respectively. 


192 


AXGKBRA. 


EXAMPLES. 

1.  Let  a  +  x  be  involved  to  the  5th  power. 

The  terms  without  the  co-efficients,  by  the  1st  rule, 
will  be 

a5,  a4*,  aV,  aV,  or4,  **, 
and  the  co-efficients,  by  the  2d  rule,  will  be 
5Xj  10X3  10X2  5X1 

it  5,       ,  —  3—,  — — ,  — — ; 

or,  1, 5,   10,       10,  5,         1 ;  % 

Therefore  the  5th  power  altogether  is 

a5  +  5a4*  +  lOaV  +  lOaV  +  5a*4  +  Xs. 

But  it  is  best  to  set  down  both  the  co-efficients  and  the 
powers  of  the  letters  at  once,  in  one  line,  without  the  inter* 
mediate  lines  in  the  above  example,  as  in  the  example  here 
below.  The  operation  is  very  easily  effected  by  performing 
the  division  first. 

2.  Let  a  —  x  be  involved  to  the  6th  power. 

The  terms  with  the  co-efficients  will  be 
a8  —  6a5*  +  15aV-20aV  +  15aV  —  6a*5  +  a*. 
8.  Required  the  4th  power  of  a  —  x. 

Ans.  a4  —  4a3x  +  6aV-  4ax3  +  ac< 
And  thus  any  other  powers  may  be  set  down  at  once,  in 
the  same  manner,  which  is  the  best  way. 

4.  Involve  a  —  *  to  the  ninth  power  ;  x  —  y  to  the  tenth 
power,  and  a  +  b  —  c  to  the  fourth  power. 


EVOLUTION. 

Evolution  is  the  reverse  of  Involution,  being  the  method 
of  finding  the  square  root,  cube  root,  6zc.  of  any  given  quan- 
tity, whether  simple  or  compound. 

case  1.    To  find  the  Boots  of  Simple  Quantities. 

Extract  the  root  of  the  co-efficient,  for  the  numeral  part  *r 
and  divide  the  index  of  the  letter  or  letters,  by  the  index  oC 


EVOLUTION. 


193 


the  power,  and  it  will  give  the  root  of  the  literal  part ;  then 
annex  this  to  the  former,  for  the  whole  root  sought*. 


EXAMPLES. 


1.  The  square  root  of  4a3,  is  2a. 

2.  The  cube  root  of  8a3,  is  2a'  or  2a. 

3.  The  square  root  of  -ttt-,  or  \Z~7Tn~9  is  —  v"  5. 

16a468  2ab2 

4.  The  cube  root  of  —  -~--z-9  is  ^  -  2/2a. 

27c3       3c  v 

5.  To  find  the  square  root  of  2db\  Ans.  a63v/2. 

6.  To  find  the  cube  root  of  -  64a <68.  Ans.  -4ci63. 

~  m  ^  i  ,  „8dr6'  2a6  2 

7.  To  find  the  square  root  of  -57-7-.  Ans.  —  J  - . 

3cJ  c  3c 

a  To  find  the  4th  root  of  81aW.  Ans.  3aV&. 

9.  To  find  the  5th  root  of  —  32aW.  Ans.  —  2ab*/b. 


CASE  II. 

To  find  the  square  root  of  a  Corn-pound  Quantity. 

This  is  performed  like  as  in  numbers,  thus  : 

1.  Range  the  quantities  according  to  the  dimensions  of 
one  of  the  letters,  and  set  the  root  of  the  first  term  in  the 
quotient. 

2.  Subtract  the  square  of  the  root,  thus  found,  from  the 
first  term,  and  bring  down  ihe  next  two  terms  to  the  re- 
mainder for  a  dividend  ;  and  take  double  the  root  for  a  di- 
visor. 


*  Any  evpn  root  of  nn  affirmative  quantity,  1.  ay  be  ml'.ier -j- or  — : 
thus  the  square  root  of  -|-  a*  is  either  +  ai  or  — a »  because  -f-  a  X  + 
a  =  -f-  «a .  and  —  a  <  —  a  =  -f-  a*  aUo. 

But  an  odd  root  of  any  rj'ianti'y  will  have  the  fame  s:gn  as  the  quan- 
tity itsjlt :  thus  tbe  cube  root  of  -f-  a*  is  -J-  .i,  and  tue  cub'j  root  of  —  a  * 
k  —  a ;  for -r-  >l  X  +  «  X  +  *  -  4~  a* »  n,,d  —  a  *  —  '*  X  —  a  —  —  «3 • 

Any  evon  root  of  a  negative  quantity  ia  imp'  i«ib'e  ;  for  neithe;  -|-  a 
X+  «t  nor  —  a  v  —  a  can  prr.cHce  —  /?a. 

Any  root  of  a  prod  ict  is  cq.ial  to  the  like  root  o  each  of  l!  1  f  -jcto-s 
moltipl-pd  together.    Tor  the  root  of  a  fraction,  *ake  the  roM  of  t'ie 
numerator  and  the  ro-^t  of  the  dciominutor. 
Vol.  1. 


/ 


104  ALGEBRA* 

3.  Divide  the  dividend  by  the  divisor,  and  annex  the  re- 
sult both  to  the  quotient  and  to  the  divisor. 

4.  Multiply  the  divisor,  thus  increased,  by  the  term  last 
set  in  the  quotient,  and  subtract  the  product  from  the  divi- 
dend. 

And  so  on,  always  the  same,  as  in  common  arithmetic. 


EXAMPLES. 

1.  Extract  the  square  root  of  a4—  4a5,&+6as&»  —  4ab*+b*. 
a4  —  4a*6  +  6a»6«  —  4a6»  +  64  (a"  —  tab  +  b*  the  root. 


2f—2ab)—4a*b  +  6a263 
—  4a36  +  4a26* 

2a»_4a*  +  6s)  2a26a  —  4ab>  +  64 
2a*b2  —  4a63  +  bl 


2.  Find  the  root  of  a4  +  4tfb  +  10a26s  +  12a63  +  96*. 
a*  +  4a3*  +  lOaV  +  12a63  +  964  (a2  +  2a£  +  3^ 


2a2  +  2a6)  4a?b  +  lOa2*2 
4a36  +  4aa6a 


2aa  +  4a&  +  362)  6a862  +  12aft3  +  964 
6aW  +  12a63  +  9b* 


3.  To  find  the  square  root  of  a1  +  4a3  +  6a2  +  4a  +  I  - 

Ans.  a2  +  2a  +  1  - 

4.  Extract  the  square  root  of  a4  -  2a3  +  2a2  —  a  +  J. 

Ans.  a2  —  a  +  ■£  — 

5.  It  is  required  to  find  the  square  root  of  a3  —  ab. 


CASE  III. 

To  find  the  Boats  of  any  Powers  in  general. 

This  is  also  done  like  the  same  roots  in  numbers,  thus  ; 

Find  the  root  of  the  first  term,  and  set  it  in  the  quotie*"***' 
—Subtract  its  power  from  that  term,  and  bring  down  tJ^* 
second  term  for  a  dividend. — Involve  the  root,  last  found, 
Jbe  next  lower  power,  and  multiply  it  by  the  index  of  ***** 


EVOLUTION* 


105 


given  power,  for  a  Jivisor. — Divide  the  dividend  by  the  di- 
visor, and  set  the  quotient  as  the  next  term  of  the  root. — 
Involve  now  the  whole  root  to  the  power  to  be  extracted  ; 
then  subtract  the  power  thus  arising  from  the  given  power, 
and  divide  the  first  term  of  the  remainder  by  the  divisor  first 
found  ;  and  so  on  till  the  whole  is  finished  *. 

EXAMPLES.  ' 

1.  To  find  the  square  root  of  a4— 2a',&+3aV— 2aft3+tt 
««_2a  b  +  3a*V—  2aP  +  b*  {a3—ab  +  &*, 


2a3)—  2a  b 


**     2a  b  +  afl6>=  (a8  —  ab)' 


2a3)  2aa#» 

<t—2ab  +  3aa6a  —  2a63  +  ©4  =  (a*  -  ab  +  b3f. 

2.  Find  the  cube  root  of  a9  -  6a5  +  21a4-44a3  +  63a*  — 
54a  +  27. 

a8  —  6a»  +  2  la4  —  44a3  +  63a2  —  54a  +  27  (a3— 2a+3. 


a9 


3a1)  —  6a5 


a*—  6a5  +  12a4—  6a3  =  (a3—  2«)3 


3a4)  +  9a4 


at-fa>+*\a*--44a:±G3a3--54a+2rr=  (a3— 2a+3)\ 


*  As  this  method,  in  high  powers,  may  be  thought  too  laborious,  it 
will  not  be  improper  to  observe,  that  the  roots  of  compound  quantities 
may  sometimes  be  easily  discovered,  thus: 

Eitract  the  roots  of  some  of  the  most  simple  terms,  and  connect 
them  together  by  the  sign  -f  or  —  ,  as  may  be  judged  most  suitable  for 
the  purpose.— Involve  (he  compound  root,  thus  found,  to  the  proper 
power ;  then,  if  this  be  the  same  with  the  given  quantity,  it  is  the  root 
required. — But  if  it  be  found  to  differ  only  in  some  of  the  signs,  change 
them  from  -f  to  — ,  or  from  —  to  +  ,  till  its  power  agrees  with  the 
given  one  throughout. 

Thus,  in  the  5th  example,  the  root  3a  —  26,  is  the  difference  of  the 
toots  of  the  first  and  last  terms ;  and  in  the  3d  example,  the  mot 
ft*—1*  +  x,  is  the  sum  of  the  roots  of  the  1st,  4th,  and  6th  terms.  The 
'Ipi  nay  also  be  observed  of  the  6th  example,  where  the  KOQttofo^k 
'3HM'Umi  first  and  last  terms.  t 


106  ALGEBRA- 

3.  To  find  the  square  root  of  a'  —  2ab  +  2ax  +  P  — 
2bx  +  x*  Ans.  a  —  b  +  x. 

4.  Find  the  cube  root  of  a6  —  3a5  +  9a4  — -  l&r  +  18a3  — 
12a  +  8.  Ans.  a3—  a  +  2. 

5.  Find  the  4th  root  of  81a4  —  216a36  +  216a363  -  90a6. 
+  1664.  Ans.  3a  -  26. 

6.  Find  the  5th  root  of  as  —  10a4  +  40a3  —  80a3  +  80a 
—  32.  Ans.  a  —  2. 

7.  Required  tho  square  root  of  1  — **• 

8.  Required  the  cube  root  of  1  — x\ 


SURDS. 

Sum>s  are  such  quantities  as  have  no  exact  root ;  and  are 
usually  exprcbded  by  fractional  indices,  or  by  means  of  the 

radical  sign  y/.    Thus,  3^,  or  ^3,  denotes  tho  square  root 

of  3  ;  and  21,  or  ^/23,  or  ^/4.  the  cube  root  of  the  square  of 
2;  where  »ht  numer'or  shows  tho  power  to  w!  'zh  the 
quantity  is  to  be  raised,  and  the  denominator  its  root. 


PROHLFM  I. 


To  reduce  a  Rational  Quantify  to  the  Farm  of  a  Surd. 

R  *  ise  the  piver*  quantity  to  the  power  denoted  by  the 
index  of  the  surd  ;  then  over  or  above  the  new  quantity  set 
the  radical  sign,  an  I  it  will  be  of  the  form  required. 


EXAMPLES.  « 

1.  To  reduce  4  to  the  form  of  the  square  root. 
First,  42  —  4  X  4  ■=  10  ;  then  y/  J  6  is  the  answer. 

2.  To  reduce  3<r  to  the  form  of  the  cube  root. 
First  3<r  X  3i3  =^  X  3/7  =  \3a>) '  =  27 aG ; 

then  \y27a*  or  (27a*)*  is  the  answer. 

3.  Reduce  C  to  the  form  of  the  cube  root. 

Ans.  (210)*  or  ?/216. 

4.  Reduce  lab  to  the  form  of  the  square  root. 


8VXDI.  197 

5.  Reduce  2  to  the  form  of  the  4th  root.  Ans.  (16)*. 

6.  Reduce  a 4  to  the  form  of  the  5th  root. 

7.  Reduce  a  +  x  to  ihe  form  of  the  square  root. 

8.  Reduce  a  —  *  to  the  form  of  the  cube  root. 


PROBLEM  II. 

To  reduce  Quantities  to  a  Common  Index. 

1.  Reduce  the  indices  of  the  given  quantities  to  a  com- 
mon denominator,  and  involve  each  of  them  to  the  power 
denoted  by  its  numerator;  then  1  set  over  the  common  de- 
nominator will  form  the  common  index.  Or, 

2.  If  the  common  index  be  given,  divide  the  indices  of  the 
quantities  by  the  given  index,  and  the  quotients  will  he  the 
new  indices  for  those  quantities.  Then  over  the  said  quan- 
tities, with  their  new  indices,  set  the  given  index,  and  they 
will  make  the  equivalent  quantities  Bought. 

EXAMPLK8. 

1.  Reduce  3*  and  5*  to  a  common  index. 
Here  £  and  }  =  Jz  and  fy. 

Therefore  3^  and  5^  =  (3')^  and  (5*)^  =  V5  and  1 
=  ■ J/243  and  l{/25. 

2.  Reduce  a*  and  b*  to  the  same  common  index  |. 
Here,  f  •+  $  =  J  X  \  =  f  the  1st  index, 

and  Jr}  =  iX  \  =  |  the  2d  index. 

Therefore  (a6)'  and  (6*)',  or  yAr5  and  are  the  quanti- 
ties. 

3.  Reduce  4*  and  5*  to  the  common  index  \. 

Ans.  (256*)*  and  25*. 

4.  Reduce  afc  and  r*  to  the  common  index  j-. 

Ans.  (a1)*  and  (x')*. 

5.  Reduce  d2  and  x3  to  the  same  radical  sign. 

Ans.  y/a*  and  y/x*. 

6.  Reduce  (a  +  x)*  and  (a  —  x)^  to  a  common  index. 

7.  Reduce  (a  +  b)^  and  (a  —  t)*  to  a  comumVbfa** 


1G8 


alg::bra. 


l'RORI.r.M  nr. 

To  reduce.  Surds  to  more.  Simple  Terms. 

Divide  the  s'.ird,  if  possible,  into  two  factors,  cne  of  which 
is  a  power  of  the  kind  that  accords  wiih  the  root  sought ;  as 
a  complete  square,  if  it  be  a  square  root,  a  complete  cube, 
if  it  he  a  cube  root ;  and  so  on.  Set  the  root  f  this  com- 
plete power  before  the  surd  expression  which  indicates  the 
root  of  the  other  factor  ;  and  the  quantity  is  reduced,  ad  re- 
quired. 

If  the  surd  be  a  fraction,  the  reduction  is  effected  by  mul- 
tiplying both  its  numerator  and  denominator  by  some  number 
that  will  transform  the  denominator  into  a  complete  square, 
cube,  &c.  its  root  will  be  the  denominator  to  a  fraction  that 
will  stand  before  the  remaining  part,  or  surd.  Sec  Example 
3,  below. 

EXAMPLKS. 

1.  To  reduce  v/32  to  simpler  terms. 

Here  ^32  =  ^(10X2)  =  ^/lO  x  ^/2~4  X  v/2  =4  </2. 

2.  To  reduce  ^/3*20  to  simpler  terms. 

V320  =y(t)4  x  5)  =  yoi  x  y:>  =  i  x  y5  =^  4  ys. 

3.  Reduce  -/J*  to  simpler  terms. 

44  44  ,  4i  4.11  H  _      22.55  _ 

IB'*5' 

4.  Reduce  v/75  to  its  simplest  terms.  Ans.  5^/3. 

5.  Reduce  ^/189  to  its  simplest  terms.  Ans.  3^/7. 
0.  Reduce  '^/\;\f  to  its  simplest  terms.  Ans.  -JJ/10. 
7.  Reduce  ^/loarh  to  its  simplest  terms.  Ans.  f>tfv/36. 

Note.  There  are  other  cases  of  reducing  algebraic  surds 
to  simpler  forms,  that  are  practised  on  several  occasions  ; 
one  of  which,  on  account  of  its  simplicity  and  usefulness,  may 
be  here  noticed,  viz.  in  fractional  forms  having  compound 
surds  in  the  denominator,  multiply  both  numerator  and  de- 
nominator by  the  same  terms  of  the  denominator,  but  having 
one  sign  chanced,  from  to  —  or  from  —  to  +,  which  will 
reduce  the  fraction  »■>  a  rational  denominator. 

Ex.  To  reduce  ^2?-+-^-~,  multiply  it  bv  ^  and  it 


becomes  -  - —  =  8  +  2v/l.r>. 

49 


SURDS. 


190 


*  „  3v/15 — 4*'5       ,.  ,   .  _    «/lf>  — y5 

■  Also,  to  reduce   -     _  —  ;  multiply  it  bv       --  — — and 

y/lr  +■  v'o  *  ,/la— ^ 

.  ,  65—7,770     65  -33v/3     13— 7,/3 

it  becomes  — -  -        —  —  =  —  . 

15— o  10  2 

And  the  same  method  may  easily  be  applied  to  examples  with 
three  or  more  surds. 


PROBLK3I  IV. 

To  add  Suid  Quantities  together 

1.  Bring  all  fractions  to  a  common  denominator,  and 
reduce  the  quantities  to  their  simplest  terms,  as  in  the  last 
problem. — 2.  Reduce  also  such  quantities  as  have  unlike 
indices  to  other  equivalent  ones,  bavin"  a  common  index. — 
3.  Then  if  the  Mini  part  be  the  same  in  them  all,  annex  it 
to  the  sum  of  the  rational  pars.  \vi;h  the  sign  of  multiplica- 
tion, and  it  will  give  the  total  sum  recr-iired. 

But  if  the  surd  pan  be  not  ilu>  s«ni<'  in  all  the  quantities, 
they  can  only  be  added  by  the  signs  +  and  — . 

KX  AMI*  LI-IS. 

1.  Required  to  add  ^/IS  and  X/S2  together. 
FirstV18=V(9X2;  =  %/2;  ™<l      —  y/{WX2)^4y/2: 
Then,  3y2 +4^/2= (3+4)^/2=7^2=  sum  required. 

2.  It  is  required  to  add  */375.  and  yi92  together. 
First,y375=^/(  1 2f>  X  3 ;  =5y  3:and  y  102=^/(0.1x3)  =4^/3: 
Then,  5^3  +  4^3  =  (5+  l)y.*J     9y3  =  sum  required. 

3.  Required  the  sum  of\/27  and  x/4t\  Ans.  7  y/S, 

4.  Required  the  sum  of  \/f>0  and  >/72.        Ans.  11^/2. 

5.  Required  the  sum  of  and  v'rs-  -^ns-  t^V^' 
G.  Required  the  sum  of -y 50  and  i[/lbli.         Ans.  5|/7. 

7.  Required  the  sum  of  \/ \  and  \/  ,!f  Ans.  -Jy2. 

8.  Required  the  sum  of  3^/a-ft  and  SyMbV/j. 

fruhlfm  v. 
7'ri  t//W  the.  Diijcrvncc  of  Surd  Quantities. 

Pre  pa  it  k  th^  quantities  the  same  w:«y  as  in  the  last  rule  : 
then  subtract  the  rational  parts,  and  to  the  remainder  acuiftx. 
the  common-surd,  for  the  difference  of  the.  surtta  tec^ivt^* 


200  ALGEBRA. 

But  if  the  quantities  have  no  common  surd,  they  can  only 
be  subtracted  by  means  of  the  sign  — -. 

EXAMPLES. 

1.  To  find  the  difference  between  v/320  and  ^/80. 
First,  v/320=V(64  X  5) = 8  ✓  5;and  /S0=%/{  16X5)  =4^5. 
Then,  8^/5  —  4^/5  =  4^/5  the  difference  sought. 

2.  To  find  the  difference  between  yi'ZS  and  ^/54. 
Fint,l/128=i/(64*2)=4y2;  andy54  =  V(27x2)=3y2- 
Then,  4J/2  -  3^/2  =        the  difference  required. 

3.  Required  the  difference  of  y/75  and  ^/48.     Ans.  ^/3. 

4.  Required  the  difference  of  $/256  and  ]/32.  Ans  2^4. 

5.  Required  the  difference  of  y/%  and  Ans.  Jv'S. 

6.  Find  the  difference  of  t/|  and  yf.  Ans.  ^^/^ 

7.  Required  the  difference  of  y f  and  (/V*  Ans.fj^/75. 

8.  Find  the  difference  of  v/24a*oa  and  ^/M'*4. 

Ans.  ^/(363— 206)^/6. 

PROBLEM  VI. 

To  multiply  Surd  Quantities  together. 

Reduce  the  surds  to  the  same  index,  if  necessary ;  next 
multiply  the  rational  quantities  together,  and  the  surds  to- 
gether ;  then  annex  the  one  product  to  the  other  for  the 
whole  product  required  ;  which  may  be  reduced  to  more 
simple  terms  if  necessary. 

EXAMPLES. 

1.  Required  to  find  the  product  of  4y/\2  and  3^2. 
Here,  4*3X  y/  12x^2  =  12v/(12v2)  =  12v/24=12v/(4x6) 

=  12X2X^/6=24^/6,  the  product  required. 

2.  Required  to  multiply  \%/}  by  . 

Here  lXtf/f  xyt^iV* V*=rV Xl/«=A X*X^  18 
=Jr^/18,  the  product  required. 

3.  Required  the  product  of  SyZ  and  2^/8.        Ans.  24. 

4.  Required  the  product  of  1^/4  and  jyl2.  Ans. 

5.  To  find  the  product  of  f       and  rWi*  Ans.  jtV15. 

6.  Required  the  product  of  2^/14  and  3y4.  Ans.  12^/7. 

7.  Required  the  product  of  2a*  and  a3.  Ans.  2nf. 

8.  Required  the  product  of  (a+A)^  and  (a+&)^. 


Ml 

9.  Required  the  product  of  2x+^b  and  2x  -  y/b. 

10.  Required  the  product  of  (af  2y/6)*,  and 

11.  Required  the  product  of  2x*  and  3x'»- 

12.  Required  the  product  of  4x*  and2y". 

PSOBLEH  VII. 

7b  divide  one  Surd  Quantity  by  another. 

Reduce  the  surds  to  the  same  index,  if  necessary ;  then 
take  the  quotient  of  the  rational  quantities,  and  annex  it  to 
the  quotient  of  the  surds,  and  it  will  give  the  whole  quotient 
required  ;  which  may  be  reduced  to  more  simple  terms  if 
requisite. 

EXAMPLES. 

1.  Required  to  divide  6 1/ 90  by  3^/8. 

Here6-r- 3.^(96  +  8)  =  2^12  =2 /(4X3)  =2  X2v/3 
=  4v/3,  the  quotient  required. 

2.  Required  to  divide  12^/280  by  3$/5. 

Here  12  -5-  3  =  4,  and  280  +  5  =  56  =  8  X  7  =  23 .  7  ; 
Therefore  4x2  XV7  =         18  tne  quotient  required. 

3.  Let  4y/50  be  divided  by  2^/5.  Ann.  2^10. 

4.  Let  6 \/100  be  divided  3^5.  Ans.  2^/20. 
5  Let  fv/jV  be  divided  by  j  v'f.  Ans.  fv/5. 

6.  Let  f       be  divided  by  | \/%.  Ans. 

7.  Let  | y/a,  or  |a^,  be  divided  by  fa*.  Ans.  f  a^. 

8.  Let     be  divided  by  <A. 

9.  To  divide  3a"  by  4a". 


PROBLEM  VIII. 


To  involve  or  raise  Surd  Quantities  to  any  Power. 

Raise  both  the  rational  part  and  the  surd  part  Or  multi- 
tiply  the  index  of  the  quantity  by  the  index  of  the  power  to 
which  it  is  to  be  raised,  and  to  the  result  annex  the  power  of 
die  rational  parts,  which  will  give  the  power  Tec\uvc«A» 

Vol.  I.  27 


202 


ALGEBRA. 


EXAMPLES. 

1.  Required  to  find  the  square  of  Jo^. 

Firs',  (f  )a  =  }  X  {-  =  A>  a«d  («*)■  =  a4X2  =  ai=r^ 
Therefore,  Jafy  =  ^a,  is  the  square  required. 

2.  Required  to  find  the  square  of  J<A. 
First,  i  X  i  =  i,  and  (a*)f  =  a*  =  aj/a  ; 
Therefore  =  Ja  ^/a  is  the  square  required* 

3.  Required  to  find  the  cube  ef  }^/6  or  f  X  6^. 

First,  (*y  =  §  X  §  X  §  -      and  (6*)3  =  6*  =  6^6  ; 
Theref.  (|^tt)3  =  ft  X6V6=  V        the  cube  required. 

4.  Required  the  square  of  2^/2.  Ans.  4{/4» 

5.  Required  the  cube  of  3^,  or  </3.  Ans.  3 

6.  Required  the  3d  power  of  £  %/3.  Ans.  J  v& 

7.  Required  to  find  the  4th  power  of  Ans.  £. 

l 

8.  Required  to  find  the  with  power  of  an. 

9.  Required  to  find  the  square  of  2  +  v^3. 

PROBLEM  IX. 

To  evolve  or  extract  ihe  Roots  of  Surd  Quantities*  . 

Extract  both  the  rational  part  and  the  surd  part.  Or 
divide  the  index  of  the  given  quantity  by  the  index  of  the 


*  The  square  roet  of  a  binomial  or  residual  surd,  « -|- 6,  or  a  — K 
may  he  found  thus  :  Take  Va*  —  b2  =  c  ; 

then  Vo+T=  +  V*-^  ; 

and  V«  —  o  =  V— g  V~2~' 

Thus,  the  square  root  of  4  +  2v3  =  1  +  v3 ; 

and  the  square  root  of  6  — 2v5  =  V5  —  1. 

But  for  the  cnbe,  or  any  higher  root,  no  general  role  is  known. 

For  more  on  the  subject  of  Surds,  see  BonrycastU's  Algebra,  the  8rev 
edition,  and  the  EUmentary  Treatise  ofAbgcbra,  by  Mr.  J.  R.  Ynmg. 


ARITHMETICAL  PROGRESSION.  203 

root  to  be  extracted  ;  then  to  the  result  annex  the  root  of 
the  rational  part,  which  will  give  the  root  required. 

RXAHPLE8. 

1*  Required  to  find  the  square  root  of  16^/6. 
First,  v/16  =  4,  and  (6^)*  =  6*     *  =  6*; 
theref.  (16  y  6)*  =  4 .  6*  =  4(/G,  »  the  sq.  root  required. 

2.  Required  to  find  the  cube  root  of  ^ 
Tint,  ^  =  J,  and  (i/3)*  =  s' "5*3  =  3* ; 

theref.      ^/3^  =  | .  3^  =  it/3,  is  the  cube  root  required. 

3.  Required  the  square  root  of  6s.  Ans.  6^/6. 

4.  Required  the  cube  root  of  |a36.  Ans.  latyb. 

5.  Required  the  4th  root  of  16a* .  Ans.  2y/a. 

6.  Required  to  find  tie  mth  root  of  aA 

7.  Required  the  square  root  of  a9  —  6a  y/b  +  96. 


ARITHMETICAL  PROPORTION  AND  PRO- 
GRESSION. 

Arithmetical  Proportion  is  the  relation  whic'i  two 
quantities,  of  the  same  kind,  bear  to  each  other,  in  respect  to 
their  difference. 

Four  quantities  are  said  to  be  in  Arithmetical  Proportion, 
when  the  difference  between  the  first  and  seconJ  is  i  vju...  io 
the  difference  between  the  third  and  fourth. 

Thus,  3,  7,  12,  16,  and  a9  a  +  6,  c,  c  +  6,  are  arith- 
metically proportional. 

Arithmetical  Progression  is  when  a  series  of  quantifies 
V either  increase  or  decrease  by  the  same  common  difference. 

Thus,  1,  8,  5,  7,  9,  11,  dec.  and  a,  a  -f-  6,  a  +  26,  a  +36, 
«+ 46,  a  +  56,  &c.  are  series  in  arithmetical  progression, 
whose  common  differences  are  2  and  6. 

The  most  useful  part  of  arithmetical  proportion  and  pro. 
fwssion  has  been  exhibited  in  the  Arithmetic.  The  same 
may  be  given  algebraically,  thus : 


204  ALGEBRA. 

Let  a  denote  the  least  term, 

z  the  greatest  term, 
d  the  common  difference, 
n  the  number  of  the  terms, 
and  s  the  sum  of  the  series ; 
then  the  princip  U  properties  are  expressed  by  these  equa- 
tions, viz. 

1.  x  =  a  +  d.  (n  —  1) 

2.  a  =  z  —  €*.(»—  1) 

3.  s  =  (a  

4.  a  =  (z  —  \d  .  n  —  l)n, 

5.  «  =  (a  +  \d  .  n  —  l)n. 

Moreover,  when  the  first  term  a  is  0  or  nothing,  the 
theorems  become  z  =  d  (n  —  1) 
and  $  =  Jam. 

EXAMPLES  FOR  PRACTICE. 

1.  The  first  term  of  an  increasing  arithmetical  series  is  1, 
the  common  difference  2,  and  the  number  of  terms  21 ;  re- 
quired the  sum  of  the  series  ? 

First,  1  +  2  X  20  =  1  +  40  =  41,  is  the  last  term. 
1  4-  41 

Then  —~—  x  20  =  21  X  20  =  420,  the  sum  required. 

A 

2.  The  first  term  of  a  decreasing  arithmetical  series  is  199, 
the  common  difference  3,  and  the  number  of  terms  67  ;  re- 
quired the  sum  of  the  series  ? 

First,  199  —  3  .  66  =  199  —  198  =  1,  is  the  last  term. 
199  4-  1 

Then  X  67  =  100  X  67  =  6700,  the  sum  re- 

quired. 

3.  To  find  the  sum  of  100  terms  of  the  natural  numbers 
1,  2,  3,  4,  5,  6,  dec.  And.  505a 

4.  *  Required  the  sum  of  99  terms  of  the  odd  numbers 
1,  3,  5,  7,  9,  dec.  Ans.  9801. 


•  The  tarn  of  any  number  (w)  of  terms  of  the  Arithmetical  aerie*  of 
odd  numbers  1,  3,  5,  7, 9,  &c.  is  equal  to  the  square  (*a  )  of  that  nnfi> 
ber.   That  is,  ' 
If  1,  3,  ft.  7,  9t  &c.  be  the  numbers,  1hpn  will 
1 2s,  3f,  4\  6»,  be  the  sums  of  1, 2  3,  fcc.  terms, 
Thus»0-4-l=  1  or  1M be  sum  of  1  term, 
14-3=  4  or  2',  the  sum  of  2  terms, 
4  -j-  5  =  -9  or  3-',  the  sum  of  3  terms, 
9  +  7  =  16  or  4» ,  the  sum  oC  4  tenai,  &c 


ARITHMETICAL  PBOGBESflXON. 


90S 


5.  The  first  term  of  a  decreasing  arithmetical  series  is  10, 
the  common  difference  1,  and  the  number  of  terms  21 ;  re- 
quired the  sum  of  the  series  ?  Ans.  140. 

6.  One  hundred  stones  being  placed  on  the  ground,  in  a 
straight  line,  at  the  distance  of  2  yards  from  each  other  ; 
how  far  will  a  person  travel,  who  shall  bring  them  one  by 
one  to  a  basket,  which  is  placed  2  yards  from  the  first  stone  ? 

Ans.  11  miles  and  840  yards. 


APPLICATION  OF  ARITHMETICAL  PROGRES- 
SION. 

Qu.  i.  A  Tin  angular  Battalion  *  consists  of  thirty  ranks, 
in  which  the  first  rank  is  formed  of  one  man  only,  the  second 
of  3  ;  the  3d  of  5  ;  and  so  on :  What  is  the  strength  of  such 
*  triangular  battalion  ?  Answer,  900  men. 

Qu.  ii.  A  detachment  having  12  successive  days  to  march, 
with  orders  to  advance  the  first  day  only  2  leagues,  the 
second  3£,  and  so  on,  increasing  l£  league  each  day's  march : 
What  is  the  length  of  the  whole  march,  and  what  is  the  last 
day's  march  ? 

Answer,  the  last  day's  march  is  18J  leagues,  and  123 
leagues  is  the  length  of  the  whole  march. 

Qu.  in.  A  brigade  of  sappers*)*,  having  carried  on  15 
yards  of  sap  the  first  night,  the  second  only  13  yards,  and 


For,  by  the  1st  theorem,  1  +  2  (n  -  1)  -  1  -f2n  -  2  =  2*  -  1  » 
the  last  term,  when  the  number  of  term*  is  n ;  to  this  last  term  2*  —  1, 
■dd  the  first  term  1,  gives  2n  the  sum  of  the  extremes,  or  n  half  the  sum 
of  the  extremes ;  then,  by  the  3d  theorem,  nXn  =  n"  is  the  sum  of  all 
the  terms.  Hence  it  appears,  in  general,  that  half  the  sum  of  the  extremes 
b  always  the  same  as  the  number  of  the  terms,  n ;  and  that  the  sum  of 
alt  the  terms  is  the  same  rs  the  square  of  the  same  number,  as. 

See  more  on  Arithmetical  Proportion  in  the  Arithmetic. 

*  By  triangular  battalion,  is  to  be  understood,  a  body  of  troops  ranged 
In  the  form  of  a  triangle,  in  which  the  ranks  exceed  each  other  by  an 
equal  number  of  men:  if  the  first  rank  consist  of  one  man  only,  and 
the  difference  between  the  ranks  be  al«o  1,  then  it?  form  is  that  of  an 
equilateral  triangle;  and  when  the  difference  between  the  ranks  is 
mora  than  1,  its  form  may  then  be  an  isosceles  or  scalene  triangle. 
The  practice  of  forming  troops  in  this  order,  which  is  now  laid  aside, 
Was  formerly  held  in  greater  esteem  than  forming  them  in  a  solid  square, 
at  admitting  of  a  greater  front,  especially  when  the  troops  were  to  make 
simply  a  stand  on  all  sides. 

t  A  brigade  of  sappers  consists  generally  of  8  men,  divided  tc\\ut\V] 
feto  two  parties.   While  one  of  these  parties  is  advancing  fat  wp,  \\v<* 
•(kerb  faro  \3hwg  the  gabions,  fa*  cines,  and  other  neceuory  \m*o\atm«D\A  * 


206 


ALGEBRA. 


so  on,  decreasing  2  yards  every  night,  till  at  last  they  car*  r 
ried  on  in  one  night  only  3  yards  :  What  is  the  number  of 
nights  they  were  employed  ;  and  what  is  the  whole  length  of 
the  sap.  ||r 

Answer,  they  were  employed  7  nights,  and  the  length  of 
the  whole  sap  was  03  yards. 

Qu.  iv.  A  number  of  gabions*  being  given  to  be  placed 
in  six  ranks,  one  above  the  other,  in  such  a  manner  as  that 
each  rank  exceeding  one  another  equally,  the  first  may  con- 
sist of  4  gabions,  and  the  last  of  9  :  What  is  the  number  of 
gabions  in  the  six  ranks;  and  what  is  the  difference  between 
each  rank  ? 

Answer,  the  difference  between  the  ranks  will  be  1,  and 
the  number  of  gabions  in  the  six  ranks  will  be  39. 

Qu.  v.  Two  detachments,  distant  from  each  other  37 
leagues,  and  both  designing  to  occupy  nn  advantageous  post 
equi-distant  from  each  other's  camp,  set  out  at  different 
times  ;  the  first  detachment  increasing  every  day's  march  1 
league  and  a  half,  and  the  second  detachment  increasing  each 
day's  march  2  leagues :  both  the  detachments  arrive  at  the 
same  time  ;  the  first  after  5  days'  march,  and  the  second 
after  4  days'  march  :  What  is  the  number  of  leagues  marched 
by  each  detachment  each  day  ? 

The  progression  r7T,  2fc,  5^,  6^,  answers  the  con- 
ditions of  the  first  detachment  :  and  the  progression  If-,  3}, 
5f ,  7|,  answers  the  condition  of  the  second  detachment. 


and  when  the  first  party  is  tired,  (he  second  takes  its  place,  and  so  on, 
till  each  man  in  turn  has  been  at  (he  head  of  the  nap.  A  sap  is  a  >ma11 
ditch,  between  3  and  4  feet  in  breadth  and  depth  ;  and  is  distinguished 
from  the  trench  by  its  breadth  only,  the  trench  having  between  10  and 
15  feet  breadth.  As  an  encouragement  to  tappers,  the  pay  for  all  the 
work  carried  on  by  the  whole  brigade  is  given  to  the  survivors. 

•  Gabions  are  baskets,  open  at  both  ends,  made  of  ozier  twigs,  and 
of  a  cylindrical  form  ;  those  made  use  of  at  the  trenches  are  2  fret 
wide,  and  about  3  feet  high  ;  which,  being  filled  with  earth,  serve  aia 
shelter  from  the  enemy's  fire:  and  those  made  u«e  of  to  construct  bat- 
teries, are  generally  higherand  broader.  There  is  another  sort  of  gabion, 
made  usa  of  to  raise  a  low  parapet :  its  height  is  from  1  to  2  feel,  and  1 
foot  wide  at  top,  hut  somewhat  less  at  bottom,  to  give  room  for  placing 
the  muszle  of  a  firelock  between  them  :  these  gabions  serve  instead  0? 
sand  bags.  A  sand  bag  is  generally  made  to  contain  about  a  cubic  foot 
of  earth. 


PILIXO  OF  BALLS. 


207 


OF  COMPUTING  SHOT  OR  SHELLS  IN  A  FINISHED  PILE. 

Shot  and  Shells  are  generally  piled  in  three  different 
forms,  called  triangular,  square,  or  oblong  piles,  according 
as  their  base  is  cither  a  triangle,  a  square,  or  u  rectangle. 

Fig.  1.     C  G  Fig.  2 


abcdef,  fig.  3,  is  an  oblong  pile. 


A.  triangular  pile  is  formed  by  the  continual  laying  of  tri- 
angular horizontal  courses  of  shot  one  above  another,  in 
such  a  manner,  as  that  the  sides  of  these  courses,  called  rows, 
decrease  by  unity  from  the  bottom  row  to  the  top  row,  which 
ends  always  in  1  shot. 

A  square  pile  is  formed  by  the  continual  laying  of  square 
horizontal  courses  of  shot  one  above  another,  in  such  a  man. 
ner,  as  that  the  sides  of  these  courses  decrease  by  unity  from 
the  bottom  to  the  top  row,  which  ends  also  in  1  shot. 

In  the  triangular  and  the  square  piles,  the  sides  or  faces 
being  equilateral  triangft&,  the  shot  contained  in  those  faces 
form  an  arithmetical  progression,  having  for  first  term  unity, 
and  for  last  term  and  number  of  terms,  the  shot  CAmV&va&& 

•7 


208 


AXGKBRA. 


in  the  bottom  row  ;  for  the  number  of  horizontal  rows,  or 
the  number  counted  on  one  of  the  angles  from  the  bottom  to 
the  top,  is  always  equal  to  those  counted  on  one  side  in  the 
bottom  :  the  sides  or  faces  in  either  the  triangular  or  square 
piles,  are  called  arithmetical  triangles  ;  and  the  numbers 
contained  in  these,  arc  called  triangular  numbers  :  abc,  fig. 
1,  kfg,  fig.  2,  are  arithmetical  triangles. 

The  oblong  pile  may  be  conceived  as  formed  from  the 
square  pile  abcd  ;  to  one  side  or  face  of  which,  as  ad,  a 
number  of  arithmetical  triangles  equal  to  the  face  have  been 
added  :  and  the  number  of  arithmetical  triangles  added  to 
the  square  pile,  by  means  of  which  the  oblong  pile  is  formed, 
is  always  one  less  than  the  shot  in  the  top  row  ;  or  which  is  the 
same,  equal  to  the  difference  between  the  bottom  row  of  the 
greater  side  and  that  of  the  lesser. 

Qu.  vi.  To  find  the  shot  in  the  triangular  pile  jlbod,  fig. 
1,  the  bottom  row  ab  consisting  of  8  shot. 

Solution.  The  proposed  pile  consisting  of  8  horizontal 
courses,  each  of  which  forms  an  equilateral  triangle  ;  that  is, 
the  shot  contained  in  these  being  in  an  arithmetical  progres- 
sion, of  which  the  first  and  last  term,  as  also  the  number  of 
terms,  ore  known  ;  it  follows,  that  the  sum  of  these  particu- 
lar courses,  or  of  the  8  progressions,  will  be  the  shot  con- 
tained in  the  proposed  pile  ;  then 

The  shot  of  the  first  or  lower  ) 

triangular  course  will  be  $  (8  +  l)X4—  36 

the  second      -      -       -  -  (7  +  1)  X  3J-  =  28 

the  third        -       -       -  -  (6  +  1)  X  3   =  21 

the  fourth       -       -       -  -  (5  +  1)  X  2i  =  15 

the  fifth         -       -       -  -  (4  +  1)  X  2   =  10 

the  sixth         -       -       -  -  (3  +  1)  X  1 J  =  6 

the  seventh     -       -       -  .  (2  +  1)  X  1    =  3 

the  eighth       -       -       -  -  (1  +  1)  X    J  =  1 

Total  120  shot 

in  the  pile  proposed. 

Qu.  vn.  To  find  the  shot  of  the  square  pile  efgh,  fig.  2, 
the  bottom  row  sf  consisting  of  8  shot. 

Solution.  The  bottom  row  containing  8  shot,  and  the 
second  only  7 ;  that  is,  the  rows  farming  the  progression, 
8,  7,  6,  5,  4,  3,  2,  1,  in  which  each  of  the  terms  being  the 
square  root  of  the  shot  contained  in  each  separate  square 


FILING  OF  BALLS. 


209 


;  course  employed  in  forming  the  square  pile ;  it  follows,  that 
the  sum  of  the  squares  of  these  roots  will  be  the  shot  requir- 
ed ;  and  the  sum  of  the  squares  divided  by  8,  7,  6,  5,  4,  3, 
2, 1,  being  204,  expresses  the  shot  in  the  proposed  pile. 

Qu.  viii.  To  find  the  shot  of  the  oblong  pile  abcdep,  fig. 
3  ;  in  which  bf  =  16,  and  bc  =  7. 

Solution.  The  oblong  pile  proposed,  consisting  of  the 
square  pile  abcd,  whose  bottom  row  is  7  shot ;  besides  9 
arithmetical  triangles  or  progressions,  in  which  the  first  and 
last  term,  as  also  the  number  of  terms,  are  known ;  it  follows, 
that, 

if  to  the  contents  of  the  square  pile  -  -  140 
we  add  the  sum  of  the  9th  progression    -  252 

&\,r  their  total  gives  the  contents  required  -    -    392  shot. 

REMARK  I. 

The  shot  in  the  triangular  and  the  square  piles,  as  also 
the  shot  in  each  horizontal  course,  may  at  once  bo  ascer- 
tained by  the  following  table :  tho  vertical  column  a  con- 
tains  the  shot  in  the  bottom  row,  from  1  to  40  inclusive  ; 
the  column  b  contains  the  triangular  numbers,  or  number 
of  each  course  ;  the  column  c  contains  the  sum  of  the  tri- 
angular numbers,  that  is,  the  shot  contained  in  a  triangular 
pile,  commonly  called  pyramidal  numbers ;  the  column  n 
contains  the  square  of  tho  numbers  of  the  column  a,  that  is, 
the  shot  contained  in  each  square  horizontal  course  ;  and 
the  column  £  contains  the  sum  of  these  squares  or  shot  in  a 
square  pile. 


Vol.  I 


28 


210  ALQMBEAm 


c 

B 

A 

D 

E 

Pyramidal 

Triangular 

Natural 

Square  of 
the  natural 

Sum  of  (beta 
square 
numbers. 

number* 

d  umbers. 

numbers* 

numbers. 

1 

1 

1 

1 

1 

4 

3 

2 

A 

4 

c 
O 

10 

6 

3 

1 A 

14 

20 

10 

4 

lo 

OA 

4U 

35 

15 

5 

2d 

00 

56 

21 

6 

Qfi 

OD 

84 

28 

7 

a  n 

49 

1  Afk 

140 

120 

36 

64 

204 

165 

45 

9 

81 

AO  C 

285 

220 

55 

10 

100 

385 

286 

66 

11 

121 

506 

364 

78 

12 

144 

690 

455 

91 

13 

169 

819 

560 

105 

14 

196 

1015 

680 

120 

15 

225 

1240 

816 

136 

16 

256 

1496 

969 

153 

17 

289 

1785 

1140 

171 

18 

324 

2109 

1330 

190  • 

19 

361 

2470 

1540 

210 

20 

400 

2870 

1771 

231 

21 

441 

3311 

2024 

253 

22 

484 

3795 

9  MOO 

976 

23 

529 

4324 

2600 

300 

24 

576 

4900 

2925 

325 

25 

625 

5525 

3276 

351 

26 

676 

6201 

3654 

378 

27 

729 

6930 

4060 

406 

28 

784 

7714 

4495 

435 

29 

841 

8555 

4960 

465 

30 

900 

9455 

5456 

496 

31 

961 

10416 

5984 

528 

32 

1024 

11440 

6545 

561 

33 

1089 

12529 

7140 

595  ! 

34 

1156 

13685 

7770 

630 

35 

1225 

14910 

8436 

666 

36 

1296 

16206 

9139 

703 

37 

1369 

17575 

9880 

741 

38 

1444 

19019 

10660 

780 

39 

1521 

20540 

11480 

820 

40 

1600 

22140 

Thus,  tho  bottom  row  in  a  triangular  pile,  consisting  of 
shot,  the  contents  will  be  1330 ;  and  when  of  19  in  the  squfl»-i* 


FILING  09  BALLS. 


211 


tm.  pile,  3470.— In  die  same  manner,  the  contents  either  of  a 
71  square  or  triangular  pile  being  given,  the  shot  in  the  bottom 
row  may  be  easily  ascertained. 

The  contents  of  any  oblong  pile  by  the  preceding  table 
may  be  also  with  little  trouble  ascertained,  the  less  side  not 
exceeding  40  shot,  nor  the  difference  between  the  less  and 
the  greater  side  40.  Thus,  to  find  the  shot  in  an  oblong  pile, 
the  less  side  being  15,  and  the  greater  35,  we  are  first  to 
find  the  contents  of  the  square  pile,  by  means  of  which  the 
oblong  pile  may  be  conceived  to  be  formed  ;  that  is,  we  arc 
to  find  the  contents  of  a  square  pile,  whose  bottom  row  is 
15  shot :  which  being  0B4O,  we  are,  secondly,  to  add  these 
1240  to  the  product  2400  of  the  triangular  number  120, 
answering  to  15,  the  number  expressing  the  bottom  row  of 
the  arithmetical  triangle,  multiplied  by  20,  the  number  of 
jtito.  triangles*  and  their  sum,  being  3640,  expresses  the 
"^ppUber  of  shot  V-ihn  proposed  oblong  pile. 

•  SEHARK  II. 

The  following  algebraical  expressions,  deduced  from  the 
investigations  of  the  sums  of  the  powers  of  numbers  in 
arithmetical  progression,  which  are  men  upon  many  gunners' 
callipers'11,  serve  to  compute  with  ease  and  expedition  the  shot 
or  shells  in  any  pile. 

That  serving  to  compute  any  triangular  >  (n+2)X(n+l)Xn 
pile,  is  represented  by  $  6 

That  serving  to  compute  any  square   )  (n+l)X(2n+l)xn 
pile,  is  represented  by  $  (5 

In  each  of  these,  the  letter  n  represents  the  number  in  the 
bottom  row  :  hence,  in  a  triangular  pile,  the  number  in  the 
bottom  row  being  30 ;  then  this  pile  will  be  (30+2)  X  (30+1) 
X  V  =  4960  shot  or  shells.  In  a  square  pile,  the  number 
in  the  bottom  row  being  also  30 ;  then  this  pile  will  be 
(30  +  1)  X  (60  +  1)  X  V  =  W55  shot  or  shells. 


•  Callipers  are  large  compasses,  with  bowed  shanks,  serving  to  tnke 
the  diameters  of  convex  and  concave  bodies.  The  gunners'  callipers 
consist  of  two  thin  rules  or  plates,  which  are  moveable  quite  round  a 
Joint,  by  the  plates  folding  one  over  the  other :  the  length  of  each  rule 
or  plate  is  6  inches,  the  breadth  about  1  inch.  It  is  usual  to  represent, 
-*>tt  the  plates,  ■  variety  of  scales,  tables,  proportions,  &c.  such  as  are 
esteemed  useful  to  be  known  by  persons  employed  about  artillery ;  hut, 
«xeept  the  measuring  of  the  caliber  of  shot  and  cannon,  and  the  measur- 
ing of  salient  and  re-enterine  angles,  none  of  the  articles,  with  YiVfa>i 
the  callipers  are  usually  filled,  an  essential  to  thai  taitroxneal 


212 


ALGEBRA. 


That  serving  to  compute  any  oblong  pile,  is  represented  by 

(2n  +  1  +  3m)  X  (n  +  1)  X  n  .     «»  «  ■   «  .        ,  . 

^  !  '  — - — ' — -  ,  in  which  the  letter  n  denotes 

o 

the  number  of  courses,  and  the  letter  m  the  number  of  shot, 
less  one,  in  the  top  row ;  hence,  in  an  oblong  pile  the  num- 
ber of  courses  being  30,  and  the  top  row  31 ;  this  pile  will 
be  COTT+90  X  30  +  1  X  y  =  23405  shot  or  shells. 

REMARK  III. 

One  practical  rule,  of  easy  reelection,  will  include  the 
three  cases  of  the  triangular,  square^  and  rectangular,  com- 
plete piles. 

Thus,  recurring  to  the  diagrams  1,  2,  and  3,  we  shall 
have,  balls  in 

(bd  +  a  +  c)  X  £bdo  =  triar*  liar  pile. 

(ef  +  ef  +  g)  X  £gfh  =  aquare  pile. 

(bf  +  bf  +ae)  X  £abc  =  rectangular  pita 
Hence,  for  a  general  rule :  add  to  the  number  of  balls  or 
shells  in  one  side  of  the  base,  the  numbers  in  its  two  paral- 
lels at  bottom  and  top  (whether  row  or  ball),  the  sum  being 
multiplied  by  a  third  of  the  slant  end  or  face,  gives  the 
number  in  the  pile.  % 


GEOMETRICAL  PROPORTION,  AND  PRO- 
GRESSION. 

Geometrical  Proportion  contemplates  the  relation  of 
quantities  considered  as  to  what  part  or  what  multiple  ono 
is  of  another,  or  how  often  one  contains,  or  is  contained 
in,  another. — Of  two  quantities  compared  together,  the  first 
is  called  the  Antecedent,  and  the  second  the  Consequent, 
Their  ratio  is  tho  quotient  which  arises  from  dividing  the 
one  by  the  other. 

Four  Quantities  are  proportional,  'when  the  two  couplets 
have  equal  ratios,  or  when  the  first  is  the  same  part  or  mul- 
tiple of  the  second,  as  the  third  is  of  the  fourth.  Hius, 
3,  6,  4,  8,  and  a,  ar,  &,  fer,  are  geometrical  proportional*. 
or  hr 

For  f  =  f  =2,  and  -r  =  -y  =  r.  And  they  are  staled 

thus,  3  :  6  :  :  4  :  8,  &c.    See  the  Arithmetic. 
Geometrical  Progression  is  one  in  which  the  terms  have 


GEOMETRICAL  PROGRESSION.  213 

all  successively  the  same  ratio  ;  as  1,  2,  4,  8, 16,  dec.  where 
the  common  ratio  is  2. 

The  general  and  common  property  of  a  geometrical  pro- 
gression is,  that  the  product  of  any  two  terms,  or  the  square 
of  any  one  single  term,  is  equal  to  the  product  of  every  other 
two  terms  that  are  taken  at  an  equal  distance  on  both  sides 
from  the  former.   So  of  these  terras, 

1,  2,  4,  8, 16,  82,  64,  czc. 

1X04  =  2X  32  =  4X  16  =  8X  8=64. 

In  any  geometrical  progression,  if 
a  denote  the  least  term, 
x  the  greatest  term, 
r  the  common  ratio, 
n  the  number  of  the  terms, 
8  the  sum  of  the  series,  or  all  the  terms  ; 


any  of  these  quantities  may  be  found  from  the  others, 
by  means  of  these  general  values  or  equations,  viz. 


2.  z  =  a  X  r*~l. 

1  — 

4.  n  =        a  =  l°g»  r  +  log,  g  —  log*  a 

log.  r  log.r 

5.  *  =   X  a  =  r-  X— r  =  -. 

r  —  1  r  —  1    r*~l     r  -  1 

When  the  series  is  infinite,  then  the  least  term  a  is  nothing, 

and  the  sum  s  = 

r— 1 

In  any  increasing  geometrical  progression,  or  series  be- 
ginning with  1,  the  3d,  5th,  7th,  czc.  terms  will  be  squares ; 
the  4th,  7th,  10th,  czc.  cubes  ;  and  the  7th  will  be  both  a 
square  and  a  cube.  Thus,  in  the  series  1,  r,  r",  r3,  r*9  r5, 
r*,  r7,  r1,  r*,  &c.  r2,  r4,  r1,  r*,  are  squares ;  r*,  r",  r9,  cubes  ; 
and  r°  both  a  square  and  a  cube. 

In  a  decreasing  geometrical  progression,  the  ratio,  r,  is  a 
1— r» 

fraction,  and  then  s  =  -  -a.  If  n  be  infinite,  this  becomes 


*  =  1 — r '  a  ^>e*n8  ^  ****  termrt 


214  ALGSUU* 

When  four  quantities,  a,  or,  b,  br,  or  2,  6, 4,  12,  are  pro- 
portional ;  then  any  of  the  following  forms  of  those  quantities 
are  also  proportional,  viz. 

1.  Directly,     a  :  or  :  :  b    :  br ;  or  2  :  6  :  :    4  :  12. 

2.  Inversely,  «r  :  a  :  :  fcr   :  b  ;  or  6  :  2  :  :  12  :  4. 

3.  Alternately,  a  :  b  ;  :  or    :  br  ;  or  2  :  4  :  :    6  :  12. 

4.  Compoundedly, a : a+ar  ::b: b+br ;  or  2  :  8  :  :  4  :  10. 

5.  Dividedly,  a :  or— a  :  :  b  :  ftr—ft ;  or  2  :  4  :  :  4  :  8. 

6.  Mixed,  ar-fa:  or — a : :  br+b  :  ftr—  6 ;  or  8  :  4  : :  16 :  8. 

7.  Multiplication,  ae :  arc  : :  be  :  ftrc ;  or  2.3  : 6.3  : :  4  :  12, 

8.  Division,  —  :  —  : :  b  :  br  ;  or  1  :  3  :  :  4  :  12. 

c  c 

9.  The  numbers  a,  6,  c,  J,  are  in  harmonical  proportion, 
when  a  :  d  :  :  a     b  :  c    d  ;  or  when  their  reciprocals 

-j-,  -i,  are  in  arithmetical  proportion. 


EXAMPLES. 


1.  Given  the  first  term  of  a  geometrical  series  1,  the  ratio 
2,  and  the  number  of  terms  12  ;  to  find  the  sum  of  the  series  7 
First,  1  X  211  =  1  X  §048,  is  the  last  term. 

2048  X  2-1     4096  —  1      Ant%-  A.  .  , 

Then  :  =  =  4095,  the  sum  required. 

<£  —  1  1 

„  2.  Given  the  first  term  of  a  geometric  series  |,  the  ratio 
and  the  number  of  terms  8  ;  to  find  the  sum  of  the  series  1 
First,  |  X  (i)7  =  }XT}T  =  sly  ,  is  the  last  term. 
Then  (i - *U X i)  +  (W)  =  (*- T*T)  -7- i  =  f ff  Xf 
=  a{ { ,  the  sum  required. 

3.  Required  the  sum  of  12  terms  of  the  series  1,  3,  9,27, 
81,  &c.  Ans.  265720. 

4.  Required  the  sum  of  12  terms  of  the  series,  1,  £,  -fr. 
A.  &c.  Ans.  fflfff 

5.  Required  the  sum  of  100  terms  of  the  series,  1,  2,  4, 8, 
16, 32,  &c.       Ans.  1267650600228220401496703205375. 

See  more  of  Geometrical  Proportion  in  the  Arithmetic. 


INFINITE  SERIES. 

An  Infinite  Series  is  formed  either  from  division,  dividing 
by  a  compound  divisor,  or  by  extracting  the  root  of  a  com* 
pound  surd  quantity,  or  by  other  general  processes ;  and  is 


-  ntrnuTB  series.  215 

such  at,  being  continued,  would  run  on  infinitely,  in  the 
manner  of  a  continued  decimal  fraction*. 

But,  by  obtaining  a  few  of  the  first  terms,  the  law  of  the 
progression  will  be  manifest ;  so  that  the  series  may  thence  be 
continued,  without  actually  performing  the  whole  operation. 

problem  I. 

To  reduce  Fractional  Quantities  into  Infinite  Series  by 
Division. 

Divide  the  numerator  b)-  the  denominator,  as  in  common 
division ;  then  the  operation,  continued  as  far  as  may  be 
thought  necessary,  will  give  the  infinite  series  required. 

EXAMPLE. 

2ab 


1.  To  change  — p-r  into  an  infinite  scries. 
j7  ^  a  +  b 

2oft..(2&- 
2ab  +  2b2 


2b2     2&'  2b* 
*  +  b)2ab..{2b-  —  +  -^  —  ^  +&c. 

a      or  or 


—  2b2 

2b* 

—  2b2—  — 

a 


2b3 


a 

2P  W 
a  +  a2 


2b* 
a2 

2b*  2b9 
a2  a3 


*  The  doctrine  of  infinite  series  was  commenced  by  Dr.  Wallis ; 
who,  fn  his  arithmetical  works  published  in  1657,  first  reduced  the  frac- 
tal |-~  by  a  perpetual  division  into  the  infinite  series  a  +  ox  +  at*  + 
,  if s  +  ar4  +  &c. 


316  AL0BBJU. 

2.  Let  c^an8e^  *nto  811  infinite  series. 

1  —  a)  l....(l  +  a  +  a,+  o»  +  a«+  &c. 
a 

a  — a» 


a* -a' 


3.  Expand  — into  an  infinite  series. 


Ans.^X(l-f  +  ^-|  +  &c.) 

o  a     or  or 


4.  Expand  ^3-^  into  an  infinite  series. 


a     aa  +  a 

1  x 

5.  Expand  ^     ^  into  an  infinite  series. 

Ans.  1  —  2x  +  2*1  —  2x3  +  2x\  &c. 

aa 

6.  Expand  - — r-rr,  into  an  infinite  series. 

r      (*  +  6)a 

Ans.  1  f-  -3-  3,  &c 

a      <r  a3 

7.  Expand  ^  ^  ^  =  J,  into  an  infinite  series. 

PROBLEM  II. 

2b  reduce  a  Compound  Surd  into  an  Infinite  Series. 

Extract  the  root  as  in  common  arithmetic  ;  then  the 
operation,  continued  as  far  as  may  be  thought  necessary,  will 
give  the  series  required.  But  this  method  is  chiefly  of  use 
in  extracting  the  square  root,  the  operation  being  too  tedious 
for  the  higher  powers. 


ZHFUTITB  SERIES. 


217 


EXAMPLES. 

1.  Extract  the  root  of  a3— x2  in  an  infinite  series. 
„._*»(«____  _  —  -  _T  &c. 


2«  —  —  i 

2a) 


X4 

—  xa  +  — 
^  4a* 


Xs       X4  x4 


X4        X9  X* 

4^    §0*"  +  64a« 


X«  **      .  V 


8a4  04a° 

x8  Xs 

■  -4  &c. 

8a4  T  16a° 


dec. 


04a« 


2.  Expand  ^/(l  +  1)  =  \/2,  into  on  infinite  series. 

Ans.  l  +  £-J-  +  -,V-r5F  &c. 

3.  Expand  ^/(l  —  1)  into  an  infinite  scries. 

Ans.  i-yV— t{?  &c. 

4.  Expand  </{c?  +  x)  into  an  infinite  series. 

5.  Expand  ^/(o3— 2bx — x3)  to  an  infinite  series. 

PROBLEM  III. 

To  extract  any  Root  of  a  Binomial:  or  to  reduce  a  Binomial 
St  .  d  into  an  infinite  Series. 

This  will  be  done  by  substituting  the  particular  letters  of 
the  binomial,  with  their  proper  signs,  in  the  following  gene- 
ral theorem  or  formula,  viz. 

,    _      v^      ^  _  m  in  —  7i      ,  m  —  2ji 

(*  +  Pft)w  =  Pn  +  —  aq  +  ~2^" "Ba  "*  f*n~~Ctt  +  &c- 

Vol.  I.  29 


218 


ALCKBSA. 


and  it  will  give  the  root  required  :  observing  that  p  denotes 

m 

the  first  term,  a  the  second  term  divided  by  the  first,  «  the 
index  of  the  power  or  root ;  and  a,  b,  c,  d,  dec.  denote  the 
several  foregoing  terms  with  their  proper  signs. 


EXAMPLES. 

.  1.  To  extract  the  sq.  root  of  a1  +  V9  in  an  infinite  series* 
Here  p  «  a1,  a  =      and  —  =  g  2  therefore 

m  m 

pw=  (aa)*=  (a*)  =  a  =  a,  the  1st  term  of  the  series. 

— Aa  =  i  XaX^=^  =  b,  the  2d  term. 

m-n        1—2  v  i»  v  6»  ft*  _ . . 

-s — sa  =  —j—  x  —  X  —  =  —  ^r— 1  ■=  c,  the  3d  term.  . 
2n  4       2a     a*  2.4<r 

w_2n        1-4         i«       V       36*  t.  ... 

Hence  a  +  ^  -  g—  +  j-g-  -  &c.  or 
a  +  2«""8^  +  16^  j2^7«fec.u.the  senw  required. 

2.  To  find  the  value  of ; — ^—7^,  or  its  equal  (a — x)~~*  in  an 
(a — x)*         n     N  ' 

infinite  series*. 

Here  p=o,  q=— =-o-,«,  and  —  =  ^?  =  -2  ;  theref. 
a  n  1 


*  ATofe.  To  facilitate  the  application  of  the  rule  to  fractional  eiem- 
pies,  it  is  proper  to  observe,  that  any  surd  may  be  taken  from  the  de- 
nominator of  a  fraction  and  placed  in  the  numerator,  and  vice  versa,  by 
only  changing  the  sign  of  its  indei.  Thus, 

L  =  1  x  ar-a  or  only  x-*;  and  =  1  X  («  +       or  (a  +  *)-»; 

(o» + x») J  x  («*  -  **H ;  &c. 

The  theorem  above  given  is  only  the  Binomial  Theorem  so  expreav 
ed  as  to  facilitate  its  application  to  roots  and  series. 


INFIlCtTB  SXStES.  219 

=  [a)-9  =  a~*  =  ^-  ■=  a,  the  first  term  of  the  series. 

—  aq  =  -2X~X— =  ~=2a-^r  =  b,  the  2d  term. 
*  tr     a  or 

jr — ft  2jf    —x  3x* 

— Tjia  =-| x^X-— X  =  ^~-  =  3«-V  =  c,  the  3d. 
2»  ■    a3     a  a* 

«— 2»  4  ^Si1  ^  —  x     4x»      .    g  . 

aft  1      a4        a  a5 

Hence  or*  +  2a-3*  +  3a-4*"  +  4a-**3  +  dec.  or 

1  ,  2x  ,  3*»     4r*     5x*  .     .   .  .  , 

— r  +  —  H — —  +  — —  +  —  -  dec  is  the  series  required. 

Qi        Or        ft*         ft*  flJ 

a9 

8.  To  find  the  value  of  ,  in  an  infinite  series. 

a— a? 

X*       X9  X4 

Ans.a+*+-  +  -+-&e. 

4.  To  eqpand  ✓  „  — in  a  series. 

.       1       at*    ,  3x«      5x*  . 

5.  To  expand  t  r-ri  in  an  infinite  series. 

(«-*)" 

a     i  .  26  ,  3i»     4i»     564  . 

Ans.  1  H  h  — r  +  — ^-  H — -  <fcc. 

o      a*      a*.  a4 

6.  To  expand  ^/o1  — xa  or  (a3— x*)^  in  a  series. 

x*      x4        x*  5xf 
Ans.  «__-__ I6^~i28?^.f. 

7.  To  find  the  value  of  ?/  (a3-  6s)  or  (tf3—  63)*  in  a  series. 

63  5b9  m 

8.  To  find  the  value  of  V  (<*  +  «*)  or  (ci'+x5)*  in  a  series. 

Xs      2c10      6xl 8 

o  —  6 

9.  To  find  the  square  root  of  ^      in  an  infinite  series. 


220  ALGEBSA. 


a* 

10.  Find  the  cube  root  of  -tttt  i°  a  series. 

o»    .  2&«   

3a3     9a8  81a» 


Ans.l__+--.-  —  &c 


INFINITE  SERIES  :  PART  THE  SECOND. 


PROBLEM  I  *• 


A  series  being  given,  to  find  the  several  orders  of  dif- 
ferences of  the  successive  terms. 

Rule  i.  Subtract  the  first  term  from  the  second,  the 
second  from  the  third,  the  third  From  the  fourth,  and  so  on ; 
the  several  remainders,  will  constitute  a  new  series,  called  the 
first  order  of  differences. 

ii.  In  this  new  series,  take  the  first  terra  from  the  second, 
the  second  from  the  third,  dec.  as  before,  and  the  remainders 
will  form  another  new  series,  called  the  second  order  of  dif. 
ferences. 

in.  Proceed  in  the  same  manner  for  the  third,  fourth, 
fifth,  <3fc.  orders,  until  either  the  differences  become  0,  or  the 
work  will  be  carried  as  far  as  is  thought  necessaryf . 


EXAMPLES. 


1.  Given  the  series  1,  4,  8,  13,  19,  26,  &c.  to  find  the 
several  orders  of  differences. 


*  The  study  of  this  second  part  of  Infinite  Series  may  be  conve- 
niently postponed  till  Simple  and  Quadratic  Equations  have  been 
learnt. 

t  Let  a,  6,  e,  d,  e,  &c.  be  the  terms  of  a  given  series,  then  if  d  =  the 
first  term  of  the  nth  order  of  differences,  the  following  theorem  will 

exhibit  the  value  of  d  :  vis.  ;fc  a  =P  *6  +  n .  n"7*  .  c  +  n  .  *T"^- . 

n— 2    ,  .        11— 1  n— 2  is— 3    .  .  ,  . 

—3—  •  d  ±  *  •  — y-  •  —3—  •  —5—  •  «  Hhi  fcc-  (to  n  +  1  terms) 

=  d,  where  the  upper  signs  must  be  taken  when  n  is  an  even  number, 
and  the  lower  signs  when  it  is  odd. 

If  the  differences  be  very  great,  the  logarithms  of  the  quantities  may 
be  used,  the  differences  of  which  will  be  much  smaller  than  those  of  ^ 
the  cjuantities  themselves ;  and  at  the  close  of  the  operation  the  natural 
number  answering  to  the  logarithmical  result  will  be  the  answer.  See 
Emsnan's  ZHfnimtal  Mcihod;  prop.  1. 


INFINITE  SSBIE8.  391 

Thus  1,  4,  8,  13,  19,  26,  dec.  the  given  series. 
Then,    3,  4,  5,  6,  7,       dec.  the  first  differences. 
And        1,  1,  1,  1,         dec.  the  second  differences. 
Also         0,  0,  0,  dec.  the  third  differences, 

where  the  work  evidently  must  terminate. 

2.  Given  the  series  1,  4,  8,  16,  32,  64, 128,  dec.  to  find  the 
several  orders  of  differences. 

Here  1,  4,  8,  16,  32,  64,  128,  dec.  given  series. 

And    3,  4,  8,  16,  32,  64,  dec.  1st  diff. 

1,  4,  8,  16,  .32,  &c  2nd  diff. 

3,  4,  8,  16,  &c.  3rd  diff. 

1,  4,  8,  dec.  4th  diff. 

3,  4,  fcc.  5th  diff. 

1,  &c.  6th  diff. 

3.  Find  the  several  orders  of  differences  in  the  series 
1, 2,  3,  4,  &c. 

Ans.  First  diff.  1,  1,  1,  1,  &c.  Second  diff.  0,  0,  0,  &c. 

4.  To  find  the  several  orders  of  differences  in  the  series 
1,  4,  9,  16,  25,  &c.  of  squares. 

Ans.  First  differences  3,  5,  7,  9,  dec.    Second,  2,  2,  2, 
&c.    Third,  0,  0,  dec. 

5.  Required  the  orders  of  differences  in  the  series  1,  8, 
27,  64,  125,  &c.  being  cubes. 

6.  Given  1,  6,  20,  50,  105,  dec.  to  find  the  several  orders 
of  differences* 


PROBLEM,  n. 


To  Find  any  term  of  a  given  series. 

Rule  i.  Let  a,  ft,  c,  d,  e,  dec.  be  the  given  series ;  dr,  d", 
dm,  <Z*V,  dec.  respectively,  the  first  term  of  the  first,  second, 
third,  fourth,  dec.  order  of  differences,  as  found  by  the  ore- 
ceding  article;  n  =  the  number  denoting  the  place  or  the 
term  required. 

n.  Then  will  a  +  ^1.  d'  +  ^=1 .  ^ .  d>  + 

1  1  A  1 

w— 2  n— 3  n— 1   n-2  n-3  n — i 

■     to  the  nth  term  required. 


388  ALGEBRA* 


XX  AMPLE  8* 


1.  To  find  the  10th  term  of  the  series  2,  5,  9,  14,  20,  dec 
Here  2,  5,  9,  14,  20,  dec.  series. 
3,  4,  5,  6,     dec.  1st  diff. 
1,  1,  1,       dec.  2nd  diff. 
0,  0,        dec  3rd  diff. 
Where  d'  =  3,  d'  =  1,  d'"  =  0,  also  a  =  2,  n  =  10  ; 

wherefore  a  H  j— .  d'  H  —  ---g—  .  df  =  (2  -|  j — 

X3  +  12pIxi^?Xl=)2+27  +  86  =  e6  =  the 

10th  term  required. 

2.  To  find  the  20th  term  of  the  series  2,  6, 12,  20,  30,  dee. 
Here  a  =  2,  n  =  20 ;  and  Art.  12. 

2,  6,  12,  20,  30,  dec.  series. 
4,  6,  8,  10,     dec.  1st  diff. 
2,  2,  2,       dec.  2nd  diff.  or  d'  =  4,  d'  =  2  ; 

whence  a  -\  j—  .  a'  +  — p- .  — ^— .  d"  =  (2  +  —  X  4+ 

^  X  ^X2  =  )2  +  76  +  342  =  420  =  the  20th  term 
required. 

3.  Required  the  5th  term  of  the  series,  1,  3,  6,  10,  dec. 

Ans.  16. 

4.  To  find  the  10th  term  of  the  series,  1,  4,  8,  13,  19,  dee. 

Ans.  64. 

5.  Required  the  20th  term  of  the  series,  1,  8,  27,  64,  125, 
dec.  Ans.  8000. 


PROBLEM  HI. 


If  the  succeeding  terms  of  a  given  series  be  at  an  unit's 
distance  from  each  other,  to  find  any  intermediate  term  by 
interpolation. 

Rule  1.  Let  y  be  the  term  to  be  interpolated,  x  its 
distance  from  the  beginning  of  the  series,  d',  d%  dh\  dir,  dec* 
the  tint  terms  of  the  several  orders  of  differences. 


INFINITE  SEBIES.  223 

2.  Then willa  +  *d'  +  * .  ^ . d'  +*. ^  .  <T"+ 
* .        .  ^-jp  •  ^-j^ .  <#v  +  &c.  =  y,  the  term  required. 

EXAMPLES. 

1.  Given  the  logarithmic  sines  of  3°  4',  3°  5',  3°  6',  8°  7', 
and  3°  8',  to  find  the  sine  of  3°  6'  16*. 

Series.    Logarithm*.    Istdiff.   2nddiff.  3rddif. 

8*4'  8-7283366   23516  1QA 

3  5  8-7306882  23390      ~ifl  1 

3  6  8-7330272   23263      ~\ZL       —  * 

3  7         8-7353535   23140      ~  KM 

3  8  8-7876675 

Here  x "=  (3*6'  15'-  3°  4'  =  2'  15'  = )  f  =  the  distance 
of  the  term  y,  to  be  interpolated;  a  =  8-7283366,  d'  = 
23516,  d"  =  -  126,  d'"  =  1,  and  y  =  a  +  <rd'  +  *. 

2=1'  *  +  x  ?=1.        .       =  (a  +  K  +  Hd'  + 

M*"  = )  8-7283366  +  0052911  —  -00001771875  + 
•0000000117  =  8-73360999296,  the  log.  sine  required. 

2.  Given  the  series  -fa,  fa,  iV  iV>  t0  find  the  tenn 
which  stands  in  the  middle,  between  fa  and  fa.     Ans.  y|T. 

3.  Given  the  logarithmic  sines  of  1°  0',  1°  \', 1Q  2',  and 
1°  3',  to  find  the  logarithmic  sine  of  1°  1'  40".  Ans.  8-2537533. 


PROBLEM  IV. 

2b  find  any  intermediate  Term  by  Interpolation,  when  the 
first  Differences  of  a  Series  of  equidifferent  Terms  are 
small. 

Rule  1.  Let  a,  b,  c,  d,  e,  <kc.  represent  the  given  series, 
and  n  =  the  number  of  terms  given. 

2.  Then  will  a — nb  +  n  .  n~1  .  c  —  n*.         .  n~2 

.  d  +  n . n^-^  .        .        .  e  +  dec.  =  0,  from  whence 
55        o  4 

by  transportation,  dec.  any  required  term  may  be  obtained*. 


•  For  the  investigation  of  these  roles,  see  Emenon't  Diffemdiel 
Msthod. 


▲L0JBBJU. 


EXAJCPLBS. 

1.  Given  the  square  root  of  10, 11,  12, 13,  and  15,  to  find 
the  square  root  of  14. 

Here  n  =  5,  and  e  is  the  term  required. 
a  =  (-/10  = )  31622776 
b  =  (^11  =  )  3-3166248 
c  =  (v/12=)  8-4641016 
d  =  L/12  = )  3-6055512 
/  =  (^15=)  8-8729833 
And  since  n  =  5,  the  series  must  be  continued  to  6  terms. 

Therefore  a — nft  +  n.— .  c — n  .  — . .d  + 
n — 1  n — 2  n — 3  n — 1   n  —  2  n  —  3  n  —  4 

./=0. 

Whence,  by  transposition,  in  order  to  find  c  we  shall  have 

n — 1   n  — 2  n— 8  ,    .  n — 1  , 

n.    g    .    3    .  —j—  .e  =  — a  +  nft  —  n.  — .c  +  n 

n— 1  9i — 2   ,  .      n  -1  n — 2  n  —  3  n  —  4  r 

.-2-.-3~,<*+».-2-.-3  j-.-g-./;  *" 

in  numbers  becomes  5c  =  —  3-1622776  +  (5  X  3-3166248) 
—  (10  x  3-4641016)  +  (10  X  3-6055512)  +  3-8729833  =* 

56-5116193— 37-8032936=18-7088257,  and  e=  18  7083257 

5 

ss  3-74166514  =  the  root,  nearly. 

2.  Given  the  square  roots  of  37,  38,  39,  41,  and  42,  to 
find  the  square  root  of  40.  Ans.  6-32455532. 

3.  Given  the  cube  roots  of  45,  46,  47,  48,  and  49,  to  find 
the  cube  root  of  50.  Ans.  3-684033. 


PROBLEM  V. 


7b  revert  a  given  Series. 

When  the  powers  of  an  unknown  quantity  are  contained 
in  the  terms  of  a  aeries,  the  finding  the  value  of  the  unknown 
quantity  in  another  series,  which  involves  the  powers  of  the 


nornriTE  series. 


225 


quantity  to  which  the  given  series  is  equal,  and  known  quan- 
tities only,  is  called  reverting  the  series*. 

Rule  1.  Assume  a  series  for  tho  value  of  the  unknown 
quantity,  of  the  same  form  with  the  series  which  is  required 
to  be  reverted. 

2.  Substitute  this  series  and  its  powers,  for  the  unknown 
quantity  and  its  powers,  in  the  given  series. 

3.  Make  the  resulting  terms  equal  to  the  corresponding 
terms  of  the  given  series,  whence  the  values  of  the  assumed 
co-efficients  will  be  obtained. 


examples. 


1.  Let  ax  +  bx*  +  cr*  +  dx*  +  &c.  =  z  be  given,  to  find 
the  value  of  x  in  terms  of  z  and  known  quantities. 

Let  z*=  x,  then  it  is  plain  that  if  zn  and  its  powers  be  sub- 
stituted in  the  given  series  for  x  and  its  powers,  the  indices 
of  z  will  be  n,  2n,  3n,  4n,  &c.  and  1  ;  whence  n=  1,  and 
the  differences  of  these  indices  are  0, 1,  2,  3, 4,  &c.  Where- 
fore the  indices  of  the  series  to  be  assumed,  must  have  the 
same  differences  ;  let  therefore  this  series  be  az  +  bz3  +  cz3 
+  dz4  +  ©zc.  =  x.  And  if  this  series  be  involved,  and  sub- 
stituted for  the  several  powers  of  x,  in  the  given  series,  it  will 
become 

axz  +  obz2  +  acz3  +  avz*  +  dec. 

*  +  6aV  +  26ab*3  +  2b  ac  zK  +  dec. 

*  *  *     +  £hV  +  dec. 

*  *     +  CA3Z3  +  3cAaHZl  +&C 

*  *  *       +  dA4Z4.       +  &C 

Whence,  by  equating  the  terms  which  contain  like  powers 
of  *,  we  obtain  (oaz  =  z,  or)  a  =  -i- ;  {aitz2  +  6a  V  =  0, 

whence)  b  =  ( —       =  )  -  ~,  (acz*+  2  W+  caV=0, 

t     2oab+ca3  KW-ac 
whence)  c  =  (  =  )  -  —5- —  ;  J>  =  ( —  - 

&bAC+bi?+3cAaB+dA*     .  5abc-5b3-a>d  _  . 

 1  x=  )  ,  &c.  and  conse- 


*  Other  methods  of  reversion  are  given  by  different  mathemalic;axv%» 
Tltie  above  is  selected  for  it*  simplicity. 
Vol.  I.  30 


326  ALGEBRA. 

quently  x=(\z+Bz>+czi+  &c.=)-^  ^  +  — s*— 

 =  .  2*  +  sc.  the  senes  required. 

a 

This  conclusion  forms  a  general  theorem  for  every  similar 
series,  involving  the  like  powers  of  the  unknown  quantity. 

2.  Let  the  series  x  —  x2  +  x3  —  x*  +  dec.  =  *,  be  propos- 
ed l'>r  reversion. 

Here  a  =  1,  b  =  —  1,  c  =  1,  d  =  —  1,  &c.  these  values 
being  substituted  in  the  theorem  derived  from  the  preceding 
example,  we  thence  obtain  x  =  z  +  z2  +  z3  +z4  +  &c.  the 
answer  required. 

^2         x3  jgi 

3.  Let  x  —  +  - —  —  +       =  y,  be  given  for  rever- 

sion. 

Substituting  as  before,  we  have  a  =  l,6=  —  |,  c  =4, 
and  d  =—  £,  &c.    These  values  being  substituted,  we  shall 

y2  y3  yA 

have  x  =  y  +     +  ~r  +        &c.  from  which  if  y  be  given, 
2       0  24 

and  sufficiently  small  for  the  series  to  approximate,  the  value 
of  x  will  be  known. 


PROBLEM  VI. 

To  find  the  Sum  of  n  Terms  of  an  Infinite  Series. 

Rule  1.  Let  a,  b,  c,  d,  c,  &c.  be  the  given  scries,  s  =  the 
sum  of  n  terms,  and  d',  d%  d"\  dw,  &c.  respectively  the  first 
terms  of  the  several  orders  of  differences,  found  by  prob.  1. 

2.  Then  will  na  +  n  .  ^  .  d'  +  n  .  5=1  .  ^  .  d*+ 

n-l    n-2   n-3  n— 1    n— 2   n— 3   n— 4 

.  dlv  +  &c.  =  s,  the  sum  of  n  terms  of  the  series,  as  was  re- 
quired. 

Case  1.  To  find  the  sum  of  n  terms  of  the  series  1,  2, 
3,  4,  5,  dec. 

First,  1,  2,  3,  4,  5,  &c.  the  given  series. 
1,  1,  1,  1,  &c,  first  differences. 
0,  0,  0,  &c.  second  differences. 

Here  o=l,  d'=l,  <T=0 ;  then  will  na  +  n  .  ^  .  cT 


INFINITE  SERIES.  22ff 

^  ^""^ '  — ,  which,  (since  a  and  d'  each  =  1)  = 

2n+«* — *    v» .  a  +  1        A,  .  , 

 =  )  ~  =  8,  the  sum  required. 

EXAMPLES. 

1.  Let  the  sum  of  20  terms  of  the  above  series  be  re- 
quired. 

„  on     j        n^n+T     20X21     01A  . 

Here  »  =  20,  and  *  =  — ^—  =  — - —  =  210,  the  ans. 

2.  Let  the  sum  of  1000  terms  be  required.   Ans.  500500. 

3.  Let  the  sum  of  12345  terms  be  required. 

Case  2.  To  find  the  sura  of  n  terms  of  the  series,  1,  3, 
5,7,9,  <&c. 

Here  1,  3,  5,  7,  9,  &c.  the  given  series. 

2,  2,  2,  2,    &c.  .  .  .  first  difference. 
0,  0,  0,     &c. . . .  second  difference. 

Wherefore  a  =  1,  dr  =  2,  <T  =  0,  and  na  +  n  .  <*' 

ft3  — ft 

==  (na  H  —  .  d'  =  (since  a  =  1  and  a*  =  2)  n  +  n3  — 

n  =)**  =  *,  the  sum  required. 

EXAMPLE. 

To  find  the  sum  of  10  terms  of  the  above  series. 

Here  »  =  10,  and  s  =-  (ft3  =)  100,  the  answer. 
Case  3.   To  find  the  sum  of  it  terms  of  the  series  of 
squares  1,  4,  9,  16,  25,  &c. 

Here  1,  4,  9,  16,  25,  ©zc.  the  series. 

3,  5,  7,  9,      &c  1st  difF. 

2,2,2,       <fcc  2nddi(F. 

0,  0,        &c  3rd  diff. 

Whence  a  =*  1,  d'  =  3,  d"  =  2,  d'"  =  0,  and  na  +  n  . 

_.^  +  ._._.^  =  (w+.3^..  —  .  +  2n. 


n— 2  _  3a* -n      n*-3n?-f-2n      n.AiT  l.-'n  1 1 
~'  "3  T~  +        3        "  '        ft  * 

4hs  sum  required. 


838  ALGEBRA. 


EXAMPLE. 


Let  the  sum  of  30  terms  of  the  above  series  be  required. 
Here  „=  30;  wherefore^l^±i)=?^«- 
9455,  the  answer.    See  the  table,  pa.  210, 


PROBLEM  VII. 

To  find  the  Sums  of  Series,  by  the  Method  of  Subtraction. 

This  method  will  be  rendered  evident  by  two  or  three 
simple  examples. 

EXAMPLE  1. 

Let  1  +  i  +  ±  +  }  +  ozc.  in  inf.  =  s 
then    \  +  J  +  }  +  I  +  ozc.  in  inf.  =  *  —  1. 

by  sub.  ig  +  i-4+  i-  +  &c.  mm/.  =  1. 

EXAMPLE  2. 

Let  1  +  |  +  *        +  &c.  =  * 
then    i  +  i  +  i  +  i  +  <&c.  =  s  =  |. 

2       2        2  2 
*  8ub-  O  +  274.  +  375  +  4T6  +  &C'  =  * 

°'-5-2'i!3+^4  +  315+i  +  &C-  =  *- 

EXAMPLE  3. 


1 

1.2 

+ 

1 

2.3 

+ 

1 

3.4 

1 

2.3 

+ 

1 

3.4 

+ 

1 

4.5 

by8Ub-r|-3+2li+ro  +  &c-e=* 


INFINITE  SBBXE8. 


EXAMPLE  4. 

Find  the  s»m  of  the  series  ^  +  ji-g  +  — + &c. 

Take  away  the  last  factor  out  of  each  denominator,  and 
1,1    ,  1    ,  - 
"rane23+0+678  +  *C-S!!* 

* >ub OS  +  SXft  +  £§X0  +  *C'  -  * 


KXAKFLK  4. 

Find  the  sum  of  the  infinite  series 

_1       ,      1  1        ,  I 

8.4.6.8     4.6.8.10     6.8.10.12  8.10.12.14 

Ans.  ^t- 

EXAMPLE  5. 

Find  the  sum  of  the  infinite  series 

1       ,  1  ,  1_       ,  . 

*"  *  q  ll  i^      q  n  ia  l*  ■  n  ia  inr  oa  '  flcc« 


3.5.8.11  4  5.8.11.14  4  8.11.14.17  r  11.14.17.20 

Ans. 

PROBLEM  vni. 

To  sum  an  infinite  series  by  supposing  it  to  arise  from  the 
expansion  of  some  fractional  expression. 

Rule.  Assume  the  series  equal  to  a  fraction,  whose  de- 
nominator is  such,  that  when  the  series  is  multiplied  by  it, 
the  product  may  be  finite  ;  this  product  being  equal  to  the 
numerator  of  the  assumed  fraction,  determines  its  ^jue. 

EXAMPLES. 

1.  Required  the  sum  of  the  infinite  series  x     a?  * 


280  ALGEBRA. 

Assume  the  series  =  -r^— 
1 — x 

then  x  +  x2  +  x3  +  d&c. 
into  1  —  x 

x  +  x3  +  x3  +  d&c. 
—  x*  —  x3  —  dec. 

2  =  X 

.\  x  +  x*  +  x3  +  dec*  =  j-^-. 

Thus,  if  x  =  J,  then  i  +  *  +  i  +  &c  =  |  -^  j  =  1  ; 
if  x  =  J,  then  i  +  i  +  ft  +  &c.  =  $  -r  |  =  J. 

2.  Required  the  sum  of  the  infinite  series  x  +  2xa  +  8r* 
+  dec. 


Assume  the  series  = 


(l—x)a  1— 2x+xa  ' 
then  x  +  2x*  +  3X3  +  dec. 
into  1  —  2x  xa 


x  +  2ra  +  3r»  +  dtc. 
_2x3  — 4i3  —  dec. 
+  V  +  d:c. 


V  x  +  2ia  +  3x3  +  dec.  =  -a. 

(1— x) 

If  x  =  J,  then  ^  +  f  +  |  +  TV  +  dec.  =  i  -T-  -J  =  2. 
If  x  =  J,  then  J  +  J  +  ft  +  ?*r  +  dtc.  =  |  -j-  J  =  f. 
And  so  on,  in  other  cases  *. 

3.  Find  the  sum  of  the  infinite  series  x  +  4x2  +  9x*  + 
16x4  +  dcc.  .  *(l+x) 


*  TbvPpfrfeceding  is  only  a  sketch  of  an  inexhaustible  subject.  For 
the  algebraical  investigation  of  infinite  series,  consult  Dodson's  Math* 
malical  Repository,  and  Mr.  J.  R.  Younu's  Mnebra.  The  subject,  how- 
ever, is  much  more  extensively  treated  by  means  of  the  flaiional 
•BjJjsift 


231 


SIMPLE  EQUATIONS. 

An  Equation  is  the  expression  of  two  equal  quantities 
with  the  sign  of  equality  (=)  placed  between  them.  Thus 
10  —  4  =  6  is  an  equation,  denoting  the  equality  of  the 
quantities  10  —  4  and  6. 

Equations  are  either  simple  or  compound.  A  Simple 
Equation,  is  that  which  contains  only  one  power  of  the  un- 
known quantity,  without  including  different  powers.  Thus, 
x  —  a  =  b  +  c,  or  axa  =  b9  is  a  simple  equation,  containing 
only  one  power  of  the  unknown  quantity  x.  But  x2  —  2ax 
■=  b2  is  a  compound  one. 

GENERAL  RULE. 

Reduction  of  Equations,  is  the  finding  the  value  of  the 
unknown  quantity.  And  this  consists  in  disengaging  that 
quantity  from  the  known  ones;  or  in  ordering  the  equa- 
tion so,  that  the  unknown  letter  or  quantity  may  stand 
alone  on  one  side  of  the  equation,  or  of  the  mark  of  equality, 
without  a  co-efficient ;  and  all  the  rest,  or  the  known  quan- 
ties,  on  the  other  side. — In  general,  the  unknown  quantity 
is  disengaged  from  the  known  ones,  by  performing  always 
the  reverse  operations.  So,  if  the  known  quantities  arc  con- 
nected with  it  by  +  or  addition,  they  must  be  subtracted  ;  if 
by  minus  ( — ),  or  subtraction,  they  must  be  added  ;  if  by 
multiplication,  we  must  divide  by  them ;  if  by  division,  we 
must  multiply ;  when  it  is  in  any  power,  wo  must  extract 
the  root ;  and  when  in  any  radical,  we  must  raise  it  to  the 
power.  As  in  the  following  particular  rules ;  which  are 
founded  on  the  general  principle,  that  when  equal  operations 
are  performed  on  equal  quantities,  the  results  must  still  be 
equal ;  whether  by  equal  additions,  or  subtractions,  or  mul- 
tiplications, or  divisions,  or  roots,  or  powers. 

PAB^ftcULAR  BULK  T. 

When  known  quantities  arc  connected  with  the  unknown 
hy  +  or  — ;  transpose  them  to  the  other  side  of  the  equa- 
tion, and  change  their  signs.  Which  is  only  adding  or  sab- 
tracting  the  same  quantities  on  both  sides,  vu  ottat  to 


232 


all  the  unknown  terms  on  one  side  of  the  question,  and  all 
the  known  ones  on  the  other  side*. 

Thus,  if  x  +  5  =  8 ;  then  transposing  5  gives  x=8  — 5=3. 

And  if  x— 3  +  7  =  9;  then  transposing  the  3  and  7,  gives 
x=9  +  3  — 7  =  5. 

Also,  if*  —  a  +  b^cd9  then  by  transpc  sing  a  and  ft,  it 

is  x  =»  a  —  b  +  cd. 
In  like  manner,  if  5x  —  6  =  4x  +  10,  then  by  transposing 
6  and  4x,  it  is  5x  —  4x  —  10  +  6,  or  x  =  1G. 

RULE  II. 

When  the  unknown  term  is  multiplied  by  any  quantity  ; 
divide  all  the  terms  of  the  equation  by  it. 

Thus,  if  ax=ab — 4a;  then  dividing  by  a,  gives  x=&— 4. 

And,  if  3x  +  5  =  20 ;  then  first  transposing  5  gives 
3x  =  15  ;  and  then  by  dividing  by  3,  it  is  x  =  5. 

In  like  manner,  if  ax+3a6=4ca ;  then  by  dividing  by  a,  it 

4e*  4c2 
is  x+36=  —  ;  and  then  transposing  36,  gives  x  =  36. 


RULE  III. 

WiiEif  the  unknown  term  is  divided  by  any  quantity ; 
we  must  then  multiply  all  the  terms  of  the  equation  by  that 
divisor  ;  which  takes  it  away. 

Thus,  if  |  =  3  +  2:  then  mult,  by  4,  gives  x  =  12  +  8=20. 

And,  if-  =  3b  +  2c  —  d: 
a 

then  mult,  by  a,  it  gives  x  =  Sab  +  2ac  —  ad. 


*  Here  it  is  earnestly  recommended  that  the  pupil  be  accustomed, 
at  every  line  or  step  in  the  reduction  of  the  equations,  to  name  the  par- 
ticular operation  to  be  performed  in  the  equation  in  the  last  line,  in  or- 
der to  produce  the  next  form  or  state  of  the  equation,  in  applying  each 
of  these  rules,  according  as  the  particular  form  of  the  equation  may 
require ;  applying  them  according  to  the  order  in  which  they  are  here 
placed :  and  beginning  every  line  with  the  words  Then  by,  as  in  the 
following  specimens  of  Examples;  which  two  words  will  always  bring 
to  his  recollection,  that  he  is  to  pronounce  what  particular  operation 
he  is  to  perform  on  the  last  line,  in  order  to  give  the  next ;  allotting 
always  a  single  line  for  each  operation,  and  ranennq  the  equations  neat- 
ly just  under  each  other,  in  the  several  line*,  as  they  are  successively 
prodaced. 


SIMPLE  EQUATIONS. 


238 


Then  by  transposing  3,  it  is  *  r 
And  multiplying  by  5,  it  is  3r 
Lastly,  dividing  by  3,  gives  x 


10. 

50. 


RULE  IV. 


When  the  unknown  quantity  is  included  in  any  root  or 
surd  :  transpose  the  rest  of  the  terms,  if  there  he  any,  by 
Rule  1  ;  then  raise  each  side  to  such  n  power  as  is  denoted 
by  the  index  of  the  surd  ;  viz.  square  each  hide  when  it  is 
the  square  root ;  cube  each  side  when  it  is  the  cube  loot  ; 
&c.  which  clears  that  radical. 

Thus,  if  y/x  —  3=4;  then  transposing  3,  gives  y/x  =  7  ; 

And  squaring  both  sides  gives  x  =  40. 

And,  if  y/(2r+  10)  =  8: 

Then  by  squaring  it,  it  becomes  2r  +  10  =  04  ; 

And  by  transposing  10,  it  is  2r  =  54  ; 

Lastly,  dividing  bv  2.  gives  x  27. 

Also,  if  3/(3r  +  4/+  3  =  0  ; 
Then  by  transposing  3,  it  is  y(3r  +  4)  =  3  ; 
And  by  cubing,  it  is  3x  -f-  4  —  'SI  : 
Also,  by  transp>  ;:ig4,  it  h  !>r  =  23  ; 
Lastly,  dividing  by  3,  gives  x  =  7J. 


When  that  side  of  the  equation  which  contains  the  un- 
known o/jantity  is  a  complete  power,  or  can  easily  be  reduced 
to  one,  by  rule  1,  2,  or  3  ;  then  extract  the  runt  of  the  said 
power  on  both  sides  of  the  equation  ;  lhat  is,  extract  the 
square  root  when  it  is  a  square  power,  or  the  cube  root  when 
it  is  a  cube,  &c. 

Thus,  if  x2  +  8t  +  1G  =  30,  or  (x      4)a  =  30  ; 
Then  by  extracting  the  root,  it  is  x  +  4  =  0  ; 
And  by  transposing  4,  it  is  x  =  0  —  4  =  2. 

And  if  3x:  —  10  =  21  +  35. 
Then,  by  transposing  If),  it  is  3<2  =  75  ; 
And  dividing  by  3,  gives  x1  ~  25  ; 
And  extracting  the  root,  gtv«:s  i  =  5. 

Also,  if  Jx3  —  fl  =  24. 
Then  transposing  0,  jives  J.r*  =  30  ; 


KT.LK  v. 


Vol.  L 


31 


284 


ALGEBRA. 


And  multiplying  by  4,  gives  3s3  =  120  ; 

Then  dividing  by  3,  gives  x*  =  40  ; 

Lastly,  extracting  the  root,  gives  x  =  ^40  =  6*824556* 


RULE  VI. 

Whe.v  there  is  any  analogy  or  proportion,  it  is  to  be 
changed  into  an  equation,  by  multiplying  the  two  extreme 
terms  together,  and  the  two  means  together,  and  making  the 
one  product  equal  to  the  other. 

Thus,  if  2x  :  9  :  :  3  :  5. 
Then  mult,  the  extremes  and  means,  gives  10*  =  27  ; 
And  dividing  by  10,  gives  x  =  2T7T. 

And  if  Jx  :  a  :  :  56  :  2c. 
Then  mult.  c.\!rcmes  and  means,  gives  jcx  =  bob  ; 
And  multiplying  by  2,  gives  3cx  =  10ad; 

t     i     r    r     i    o  l0ab 
Lastly,  dividing  by  3c,  gives  x  = 

Also,  if  10—  x  :  lx  :  :  3  :  1. 
Then  mult,  extremes  and  means,  gives  10  —  x  =  2x  ; 
And  transposing  x,  gives  10  =■=  3x  ; 
Lustly,  dividing  by  3,  gives  3£  =  x. 


RULE  VII. 

When  the  same  quantity  is  found  on  both  sides  of  an  equa- 
tion, with  the  same  sign,  cither  plus  or  minus,  it  may  be  left 
out  of  both  :  and  when  every  term  in  an  equation  is  either 
multiplied  or  divided  by  the  same  quantity,  it  may  be  struck 
out  of  them  all. 

Thus,  if  3x  +  2a  =  2a  +  b  : 
Then,  by  taking  away  2a,  it  is  3x  =  b. 
And,  dividing  by  8,  it  is  x  =  ±b. 

Also,  if  there  be  4ax  +  6ab  =  7ac. 
Then  striking  out  or  dividing  by  a,  gives  4x  +  Gb  =  7c. 
Then  by  transposing  66,  it  becomes  4x  =  7c  —  6b; 
And  then  dividing  by  4,  gives  x  =  jc  —  $6. 

Again,  if  fx  —  f  =  V  —  f  - 
Then,  taking  away  the  £,  it  becomes  fx  =  fs°  ; 
And  taking  away  the  3's,  it  is  2x  =  10  ; 
Lastly,  dividing  by  2,  gives  x  =  5. 


SIMPLE  EQUATIONS. 


286 


MISCELLANEOUS  EXAMPLES. 

1.  Given  7* —  18  =  4x  +  6  ;  to  find  the  value  of  x. 
Firsts  transposing  18  and  4x  gives  3x  =  24  ; 
Then  dividing  by  3,  gives  x  =  8. 

2.  Given  20 — 4*  — 12  =  02  — 10* ;  to  find  x. 
First,  transposing  20  and  12  and  lOx,  gives  6x  =  84 ; 
Then  dividing  by  6,  gives  x  =  14. 

3.  Let  4ax  —  5b  =  Sdx  +  2c  be  given :  to  find  x. 
First,  by  trans.  56  and  9dx9  it  is  4ax  —  3cfx  =  55  +  2c : 

Then  dividing  by  4a  —  3d,  gives  x  =  |~~~^» 

4.  Let  5x" —  12x  =  9x  +  2X3  be  given  ;  to  find  x. 
First,  by  dividing  by  x,  it  is  5x  —  12  =  9  -f-  2x ; 
Then  transposing  12  and  2x,  gives  3x=21  ; 
Lastly,  dividing  by  3,  gives  x  =■•  7. 

5.  Given  9ax3  —  15abx*  =  Gar*  +  12ax3 ;  to  find  x. 
First,  dividing  by  Sax3,  gives  3x  —  56  =  2x  +  4  ; 
Then  transposing  56  and  2x,  gives  x=56  -fi. 

—  XXX 

6*  Let  -  —  -  +  ^  =:  2  be  given,  to  find  x. 

First,  multiplying  by  3,  gives  x  —  f  r-f-3!x -  6 ; 
Then,  multiplying  by  4,  gives  x  +  V*x  =24. 
Also  multiplying  by  5,  gives  17x  =  120 : 
Lastly,  dividing  by  17,  gives  x  =  7yT. 

~  ^-      x — 5  ,  x     ,  _     x — 10       „  , 

7.  Given  — — f-  -  =  12  — ;  to  find  x. 

First,  mult,  by  3,  gives  x  —  5  +  £r=3G  —  x  +  10  ; 
Then  transposing  5  and  x,  gives  *2»,4--,;r=-51  ; 
And  multiplying  by  2,  gives  7x  =  102 ; 
Lastly,  dividing  by  7,  gives  x=l  1$. 

3x 

8.  Let  v^-j-  +  7  =  10,  be  given  ;  to  find  x. 

First,  transposing  7,  give3  ^^=3  ; 
Then  squaring  the  equation,  gives  J x  —9 


236  ALGEBRA* 

Then  dividing  by  3,  gives  \x  =  3  ; 
Lastly,  multiplying  by  4,  gives  x  =  12. 

6a3 

9.  Let  2x  +  2v/(a2  +  x3)  =  ,  be  given,  to  find*. 

First,  mult,  by  ^/(a2+xt)9  gives  2s  v/(a2+xa)+2a,+2x> 
=  5a3. 

Thentransp.  2a3  and  2X3,  gives  2x  v^(aa+r,)=3a1— 2x»; 
Then  by  squaring,  it  is  4x*  X  (a*  +  x3)  =  (3a1—  2*")1; 
That  is,  4aV  -f-  4x4  =  9a4— 12aV  +  4x4 ; 
By  taking  4x4  from  both  sides,  it  is  4a3x3=9a4  —  12aV; 
Then  transposing  12aax3,  gives  16a3x3=9a4 ; 
Dividing  by  a3  gives  lCx3  =  9a3 ; 
And  dividing  by  16,  gives  x2=f9a9 ; 
Lastly,  extracting  the  root,  gives  x=Ja. 

EXAMPLES  FOR  PIIACTICK. 

1.  Given  2r  —  5  +  16  =  21  ;  to  find  x.  Ans.  x=5. 

2.  Given  Ox  —  15  =  x  +  6  ;  to  find  x.  Ans.  *=4i. 
5.  Given  8— 3x  r  12  =  30-5x+4 ;  to  find  x.    Ans.  x=7. 

4.  Given  x  +  Jx  —  Jx=rl3  ;  to  find  x.  Ans.  x— 12. 

5.  Given  3x+ Jx+2=5x—  4;  to  find  x.  Ans,  *=4. 

6.  Given  4ax+Ja — 2=ax — bx  ;  to  find  x. 

AnS'X=:9a+3S- 

7.  Given  -}x —     -f  \x  =  J  ;  to  find  x.       Ans.  x  —  ff. 

8.  Given  v/(4-fx)=4— v/x  ;  to  find  x.        Ans.  x  =  2J. 

X" 

9.  Given  4a  +  x  =  ;  to  deter,  x.    Ans.  x  =  — 2a. 

4(7  -f-  x 

10.  Given  x/{lal+  x3)=  «/(4&4+  x4) ;  to  find  x. 

Ans.  x  =  \/— sT' 
2a" 

11.  Given  y/x  +  y/(2a+x)  =  — ~— ,  ;  to  find  x. 

</{Za-\-x) 

Ans.  x  =  |a. 

12.  Given  —V  +  -----  =  2b  ;  to  find  x. 

l+2x     1 — 2x 

Ans.  x=£  \/"^"# 

13.  Given  a+x=  v/(a3-fx  ^/^P+a*))  ;  to  find  x. 

Ans.  x  =  —  —  <*• 
a 


SIMPLE  EQUATIONS. 


287 


OF  REDUCING  DOUBLE,  TRIPLE,  &C.  EQUATIONS,  CONTAINING 
TWO,  THREE,  OR  MORE  UNKNOWN  QUANTITIES. 

PROBLEM  I. 

lb  exterminate  two  Unknown  Quantities;  Or,  to  reduce  the 
two  Simple  Equations  containing  them,  to  a  Single  one. 


RULE  I. 

Find  the  value  of  one  of  the  unknown  letters,  in  terms  of 
the  other  quantities,  in  each  of  the  equations,  by  the  methods 
already  explained.  Then  put  those  two  values  equal  to 
each  other  for  a  new  equation,  with  only  one  unknown  quan- 
tity in  it,  whose  value  is  to  be  found  as  before. 

Note.  It  is  evident  that  we  must  first  begin  to  find  the 
values  of  that  letter  which  is  easiest  to  be  found  in  the  two 
proposed  equations. 

EXAXPLE8. 

1.  Given  ^  5^     2y  =  14  |  ;  t0  find  x  and  y* 
In  the  1st  equat.  trans.  3y  and  div.  by  2,  gives  x  =  ^   ^ ; 

14+2y 

In  the  2d  trans.  2y  and  div.  by  5,  gives  x  =  — —  £ ; 

o 

.      1.  .  1    •      14+2y  l?-3y 

Putting  these  two  values  equal,  gives  — — ~  =  — ^  i 

Then  mult,  by  2  and  5,  gives  28  +  Ay  =  85  —  15y ; 
Transposing  28  and  15y,  gives  1%  =  57 ; 
And  dividing  by  19,  gives  y  =  3. 
And  hence  x  =  4. 

Or,  effect  the  same  by  finding  two  values  of  y,  thus 

17-2x 

In  the  1st  equat.  tr.  2x  and  div.  by  3,  gives  y  =  — g —  ; 

5x— 14 

In  the  2d  tr.  2y  and  14,  and  div.  by  2,  gives  y  =  — —  ; 

5a; -14  17— 2x 
Putting  these  two  values  equal,  gives  — — —  =  — g — \ 


288  ALGEBRA. 

Mult,  by  2  and  by  3,  gives  15x  —  42  =  34  —  4x ; 
Transp.  42  and  4x9  gives  19x  =  76 ; 
Dividing  by  19,  gives  x  =  4. 
,  Henoe  y  =  8,  as  before. 

2.  Given  {  jjlSfa*  j  5  tofindxandy. 

Ans.  x  =  a  +  b9  and  y  =     —  Ji. 

3.  Given  3*  +  y  =  22,  and  3y  +  x  =  18;  tofindxandy. 

Ans.  x  =s  6,  and  y  «  4. 

4.  Given        +  jy  =  3J  |  ?  to  ^n<*  x  y# 

Ans.  x  =  6,  and  y  =  3. 

,  2a:  .  3y     22     _  3a?  .  2y    .  67         „  _ 

5.  GivenT  +  ^=yand-  +  ^=-;  to  find. 

and  y.  Ans.  a?  =3,  and  y  =  4. 

6.  Given  x  +  2y  =  sy  and  x*  —  4y*  =  <P ;  to  find  x  and  y. 

An»-  *  =  — ^— ,  and  jf  =  — ^— . 

7.  Given  x  —  2y  =  d>  and  x  :  y : :  a :  b  ;  to  find  x  and  y. 

^•^^^^^ 

RULE  II. 

Find  the  value  of  one  of  the  unknown  letters,  in  only  one 
of  the  equations,  as  in  the  former  rule;  and  substitute  this 
value  instead  of  that  unknown  quantity  in  the  other  equation, 
and  there  will  arise  a  new  equation,  with  only  one  unknown 
quantity,  whose  value  is  to  be  found  as  before. 

Note.  It  is  evident  that  it  is  best  to  begin  first  with  that 
letter  whose  value  is  easiest  found  in  the  given  equations. 

EXAMF  E8. 

1.  Given  |*J  + 1*        |  ;  to  find  x  and  y. 

This  will  admit  of  four  ways  of  solution ;  thus ;  First, 

17  3tf 

in  the  1st  eq.  trans.  3y  and  div.  by  2,  gives  x  =  — — - . 

This  val.  subs,  for  x  in  the  2d,  gives  85  —  2y  =  14; 
Hub.  by  2,  this  becomes  86  —  15y  —  4y  =  28; 


snmx  equations.  289 

Transp.  15y  and  4y  and  28,  gives  57  =  19y ; 
And  dividing  by  19,  gives  3  =  y. 

l*en,  =  ^  =  4. 

14  +  2v 

Hly,  in  the  3d  trans.  2y  and  div.  by  5,  gives  x  =  — - — -  ; 

*  This  subst.  for  *  in  the  1st,  gives  ^jtl?  +  3y  =s  17 ; 

Mult,  by  5,  gives  28  +  4y  +  15y  =  85  ; 
Transpo.  2*5,  gives  19y  =  57 ; 
And  dividing  by  19,  gives  y  =  3. 
14  +  2y 

Then  *  =  — -  s=  4,  as  before. 

o 


8d1y,  in  the  1st  trans.  2x  and  div.  by  3,  gives  y  =  ? 

34  4X 

This  subst  for  y  in  the  2d,  gives  Ex  ^  =  14  ; 

Multiplying  by  3,  gives     15x  —  34  +  4x  =  42  ; 
Transposing  34,  gives       19x  =  76  ; 
And  dividing  by  19,  gives     x  =  4. 
17  2x 

Hence  y  =  —  =  3,  as  before. 

3 


5x  — 14 

4thly,  in  the  2d  tr.  2y  and  14  and  div.  by  2,  gives  y  =  — - — . 

15x  42 

This  substituted  in  the  1st,  gives  2x  H  -  =  17 ; 

Multiplying  by  2,  gives  19x  —  42  =  34 ; 
Transposing  42,  gives  19x  =  70  ; 
And  dividing  by  19,  gives  x  =  4 ; 
5X  14 

Hence  y  =  —  =  3,  as  before. 


2.  Given  2x  +  3y  =  29,  and  3x  —  2y  =  11  :  to  find  x 
and  y.  Ans.  x  =  7,  and  y  =  5. 

,3.  Given  |  *  *  ^Z.  l\  ^  ;  to  find  x and  y. 

Ans.  x  atv^^^^ 


MO  ALGEBRA. 

4.  Given  |  ^^20  |  ;*<>  find  x  and  y. 

Ans.  x  =  6,  and  y  =  4. 

5.  Given  g  +  3y  =  21,  and  |  +  3x  =  29  ;  to  find  r 
and  y.  Ans.  x  =  9,  and  y  =  6L 

6.  Given  10  -  |  =  |  +  4,  and  +  f  -  2  =  ' 
3y  —  x 

-~r  1  ;  to  find  x  and  y.         Ans.  x  =  8,  and  y  =■  6. 

7.  Given  x  :  y  :  :  4  :  3,  and  x3  —  y1  =  37  ;  to  find  % 
and  y.  Ans.  x  =  4,  and  y  =  8.^ 


RULE  III. 


Lbt  the  given  equations  be  so  multiplied,  or  divided,  &c. 
and  by  such  numbers  or  quantities,  as  will  make  the  terms 
which  contain  one  of  the  unknown  quantities  the  same  in 
both  equations  ;  if  they  are  not  the  same  when  fir3t  pro- 
posed. 

Then  by  adding  or  subtracting  the  equations,  according 
as  the  signs  may  require,  there  will  result  a  now  equation, 
with  only  one  unknown  quantity,  as  before.  That  is,  add 
the  two  equations  when  the  signs  are  unlike,  but  subtract 
them  when  the  signs  are  alike,  to  cancel  that  common 
term. 

Note.  To  make  two  unequal  terms  become  equal,  as 
above,  multiply  each  term  by  the  co-efficient  of  the  other. 


EXAMPLES. 


r   g,.  __.    9  ^ 

Given  i  2x  +  5y  =  16  \  '  t0  find  x  and  y' 

Here  we  may  either  make  the  two  first  terms,  containing  rr  , 
equal,  or  the  two  2d  terms,  containing  y,  equal.    To  mak.^ 
the  two  first  terms  equal,  we  must  multiply  the  1st  equation 
by  2,  and  the  2d  by  5 ;  but  to  make  the  two  2d  terms  equaT, 
we  must  multiply  the  1st  equation  by  5,  and  the  2d  by  3  ; 
Ma  follows. 


SIMPLE  EQUATIONS. 


241 


1.  By  making  the  two  first  terms  equal : 

Mult  the  1st  equ.  by  2,  gives  lOx  —  6y  =  18 

And  mult,  the  2d  by  5,  gives  lOx  +  25y  =  80 

Subtr.  the  upper  from  the  under,  gives  Sly  =  62 
And  dividing  by  31,  gives  y  =  2. 

Hence,  from  the  1st  given  equ.  *  =  — -— ?  =  3. 

2.  By  making  the  two  2d  terms  equal : 

Mult,  the  1st  equat.  by  5,  gives  25x  —  15y  =  45 ; 
And  mult,  the  2d  by  3,  gives  Ox  +  15y  =  48  ; 
Adding  these  two,  gives  31x  =  93  ; 

And  dividing  by  31,  gives  x  =  3. 

c  y   9 

3     Hence,  from  the  1st  equ.  y  =  — - —  =  2.' 


MISCELLANEOUS  EXAMPLES. 


1.  Given  +  6y  =  21,  and  ^  +  5x  =  23  ;  to  find 
x  and  y.  Ans.  x  =  4,  and  y  =  3. 

2.  Given  + 10  =  13,  and  +  5=  12 ;  to  find 
x  and  y.  Ans.  a:  =  5,  and  y  =  3. 

3.  Give„?^+*=10,and^  +  ?  =  14;tofind 

5         4  o  o 

x  and  y.  Ans.  x  =  8,  and  y  =  4. 

4.  Given  3x+4y=38,  and  4r  —  3y  ~  9  ;  to  find  x  and  y. 

Ans.  x  =  6,  and  y  =  5. 


problem:  hi. 

y 

To  exterminate  three  or  more  Unknotcn  Quantities ;  Or,  to 
reduce  the  simple  Equations,  containing  them,  to  a  Single 
one* 

RULE. 

This  may  be  done  by  any  of  the  three  methods  in  the  last 
problem :  viz. 

1.  After  the  manner  of  the  first  rule  in  the  last  problem, 
find  the  value  of  one  of  the  unknown  letters  in  each  of  the 
given  equations  ;  next  put  two  of  these  values  equal  to  each 
other,  and  then  one  of  these  and  a  third  value  equal,  and  so 
on  for  all  the  values  of  it ;  which  gives  a  new  set  of  c^ftvcycA, 

Vol.  1.  32 


243 


AXGEBSJU 


with  which  the  same  process  is  to  be  repeated,  and  so  on  till 
there  is  only  one  equation,  to  be  reduced  by  the  rules  for  a 
single  equation. 

2.  Or,  as  in  the  2d  rule  of  the  same  problem,  find  the  value 
of  one  of  the  unknown  quantities  in  oue  of  the  equations  only; 
then  substitute  this  value  instead  of  it  in  the  other  equations ; 
which  gives  a  new  set  of  equations  to  be  resolved  as  before, 
by  repeating  the  operation. 

3.  Or,  as  in  the  3d  rule,  reduce  the  equations,  by  multi- 
plying or  dividing  them,  so  as  to  make  some  of  the  terms  to 
agree :  then,  by  adding  or  subtracting  them,  as  the  signs 
may  require,  one  of  the  letters  may  be  exterminated,  dec.  as 
before. 


EXAMPLES. 


Cx  +  y  +  z  =  91 
I.  Given  <  x  4-  2y  +3z  =  16  >  ;  to  find  x9  y,  and  z. 

(x  +  3y  +4*  =  21) 
1.  By  the  1st  method : 
Transp.  the  terms  containing  y  and  z,  in  each  cqua.  gives 
x  =  9  —  y  —  2, 
*=  16  —  2y  —  3z, 
x  =  21  —  3y  — 4z; 

Then  putting  the  1st  and  2d  values  equal,  and  the  2d  and  3d 
values  equal,  give 

9—  y—  z  =  16— 2?/  — 32, 
16  _2y  —32  =21  -  3y  —  4z  ; 
In  the  1st  trans.   9,  2,  and  2y,  gives  y  =  7  —  2z ; 
In  the  2d  trans.  16,  3z,  and  3y,  gives  y  =  5  —   z  ; 
Putting  these  two  equal,  gives  5  —  z  =  7  —  22. 
Trans.  5  and  2z,  gives  2  =  2. 
Hence  y  =  5  —  2  =  3,  and  x  =  9  —  y  —  2  —  4- 
2dly.  By  the  2d  method  : 

From  the  1st  equa.  x  =•  9  —  y  —  2 ; 
This  value  of  x  substit.  in  the  2d  and  3d,  gives 
9  +   y  +  22  =  16, 
9  +  2y  +  32  =  21  ; 
lii  the  1st  trans.  9  and  22,  gives  y  =  7  —  2z ; 
This  substit.  in  the  last,  gives  23  —2  =  21; 
Trans,  z  and  21,  gives  2  =  2. 
Hence  again  y  =  7  —  22  =  3,  and  a:  =  9  —  y  —  *  — 


SIMPLE  EQUATIONS.  248 

8d1y.  By  the  3d  method  :  subtracting  the  1st  equ.  from 
the  2d,  and  the  2d  from  the  3d,  gives 
y  +  2z  =  7, 
y+  *  ==  5  ; 
Subtr.  the  latter  from  the  former,  gives  z  =  2. 
Hence  y  =  5  —  z  =  3,  and  x  =  9  —  y  —  :  =  4. 


(*+  y+  *  =  18) 
2.  Given ^x  +  3y  +  2*  =  38V; 

+    +  i*  =  i<0 

Ans.  x  = 
+  4y  +  i*  =  27) 
+  Jy  +  i*  =  20  }  ;  to 

+  *y  +    =  16  J 


to  find  x,  y,  and  z. 


Ads.  x  =  4,  y  =  6,  z  =  8. 

>  +  4y  +  i*  =  27, 

3.  Given  <  *  +  |y  +  |z  =  20  J. ;  to  find  x,  y,  and  z, 

Ans.  x  =  1,  y  =  12,  z  =  60. 

4.  Given  *  —  y  =  2,  x  —  z  =  3,  and  y  +  z  =  9  •  to 
find  x,  y,  and  z.  Ans.  x  =  7,  y  =  5,  z  =  4. 


5.  Given  <  3x  +  4y  +  5z  =  46  )  ;  to  find  x,  y,  and  z. 

(  2x  +  6y  +  8z  =  68  ) 
ix(x  +  y  +  z)=  4jL^ 

6.  Given  J  y  (x  +  y  +  z)  =         ;  to  find  x,  y,  and  z. 

+  *  +     =  10?J 

J 

A  COLLECTION  OF  QUESTIONS  PRODUCING  SIMPLE 
EQUATIONS. 

Quest.  1.  To  find  two  numbers,  such,  that  their  sum 
shall  be  10,  and  their  difference  6. 

Let  x  denote  the.greater  number,  and  y  the  less"" 
Then,  by  the  1st  condition  x  +  y  =  10, 
And  by  the  2d     -    -    .   x  —  y  =  6, 
Transp.  y  in  each,  gives    x  =■=  10  —  y, 
and  x  =  6  +   y  ; 
Put  these  two  values  equal,  gives  6  +  y=  10  —  y; 
Transpos.  6  and  — y,  gives    -    2y  =  4  ; 
Dividing  by  2,  gives       -     -     y  =  2. 
And  hence      -      -     •     -     x  =  6  -f-  y  =  8. 


*  la  these  solutions,  as  many  unknown  letters  are  always  used  as 
there  are' unknown  numbers  to  be  found,  purposely  for  exercise  in  the 
nodes  of  reducing  the  equations :  avoiding  the  short  ways  of  notation, 
which,  though  they  may  give  neater  solutions,  afford  less  eiertV6«\u 
practising  the  several  rules  in  reducing  equations, 


244 


AL€SBBA. 


Quest.  2.  Divide  100Z  among  a,  b,  c,  so  that  ▲  may  hate 
20Z  more  than  b,  and  b  10/  more  than  c. 

Let  x  =  a's  share,  y  =  b's,  and  z  =  c's. 
Then  x  +  y  +   %  —  100, 
x  =  y  +  20, 
y  =  z  +  10. 

In  the  1st  suhstit.  y  +  20  for  x,  gives  2y  +  z  +  20  =  100  ; 
'  In  this  substituting  z  +  10  for  y,  gives  3*  +  40  =  100  ; 
By  transposing  40,  gives       -     -     3z  =  60  ; 
And  dividing  by  3,  gives       -     -      z  =  20. 
Hence  y  =  z  +  10  =  30,  and  x  =  y  +  20  =  50. 

Quest.  3.  A  prize  of  500Z  is  to  be  divided  between  two 
persons,  so  as  their  shares  may  be  in  proportion  as  7  to  8 ; 
required  the  share  of  each. 

Put  x  and  y  for  the  two  shares  ;  then  by  the  question, 

7  :  8  :  :  x  :  y,  or  mult,  the  extremes, 
and  the  means,  7y  =  8x, 

and  x  +  y  =  500  ; 
Transposing  y,  gives  x  =  500  —  y  ; 
This  substituted  in  the  St,  gives  7y  =  4000  —  Sy  ; 
By  transposing  8y,  it  is*f  5y  =  4000  ; 
By  dividing  by  15,  it  gives  y  =  266f  ; 
And  hence  x  =  500^-  y  =  233£. 

Quest.  4.  What  fraction  is  that,  to  the  numerator  of 
which  if  1  be  added,  the  value  will  be  \  ;  but  if  1  be  added 
to  the  denominator,  its  value  will  be  £  ? 

x 

Let  —  denote  the  fraction. 

y 

Then  by  the  quest.  *  ^  1  =  4,  and  — =  4. 

The  1st  mult,  by  2  and  y,  gives  2x  +  2  =  y  ; 
The  2d  mult,  by  3  and  y  +  1,  is  3x  =  y  +  1  ; 
The  upper  taken  from  the  under  leaves  x  —  2  =  1; 
By  transpos.  2,  it  gives  x  =  3. 
And  hence  y  =  2x  +  2  =  8  ;  and  the  fraction  is  f . 

Quest.  5.  A  labourer  engaged  to  serve  for  30  days  oflK 
these  conditions  :  that  for  every  day  he  worked,  he  was 
receive  20d,  but  for  every  day  he  played,  or  was  absent,  he» 
was  to  forfeit  lOd.    Now  at  the  end  of  the  time  he  had  t» 
receive  just  20  shillings,  or  240  pence.   It  is  required  ts» 


SIMPLE  EQUATIONS. 


2*5 


find  how  many  days  he  worked,  and  how  many  he  was 
idle? 

Let  x  he  the  days  worked,  and  y  the  days  idled. 
Then  20x  is  the  pence  earned,  and  lOy  the  forfeits  ; 
Hence,  by  the  question    -    x  +  y  =  30, 

and  20x  -  lOy  =  240  ; 
The  1st  mult,  by  10,  gives  lOx  +  lOy  =  300  ; 
These  two  added,  give  -  30x  =■  540  ; 
This  div.  by  30,  gives    .    x  =  18,  the  days  worked  ; 
Hence       -      y  =  30  —  x  =  12,  the  days  idled. 

Quest.  6.  Out  of  a  cask  of  wine  which  had  leaked  away 
30  gallons  were  drawn  ;  and  then,  being  guaged,  it  appear- 
ed to  be  half  full ;  how  much  did  it  hold? 

Let  it  he  supposed  to  have  held  x  gallons, 

Then  it  would  have  leaked  }x  gallons, 

Conseq.  there  had  been  taken  away  }x  +  30  gallons. 

Hence  Jx  =  \x  +  30  by  the  question. 

Then  mult,  by  4,  gives  2x  =  x  +  120  ; 

And  transposing  x,  gives  x  =  120  the  gallons  it  held. 

Quest.  7.  To  divide  20  into  rVo  such  parts,  that  3  times 
tlie  one  part  added  to  5  times  the  other  may  make  76. 

Let  x  and  y  denote  the  two  parts. 
Then  by  the  question       -       -    x  +   y  =  20, 

and  3x  +  by  =  76. 
Mult,  the  1st  by  3,  gives  -  3x  +  3y  =  60  ; 
Subtr.  the  latter  from  the  former,  gives  2y  =  16  ; 
And  dividing  by  2,  gives  -  -  y  =  8. 
Hence,  from  the  1st,      -      x  =  20  —  y  =  12. 

Quest.  8.  A  market  woman  bought  in  a  certain  number 
of  eggs  at  2  a  penny,  and  as  many  more  at  3  a  penny,  and 
•old  them  all  out  again  at  the  rate  of  5  for  two-pence,  and 
so  doing,  contrary  to  expectation,  found  she  lost  3d ;  what 
number  of  eggs  had  she  ? 

Let  x  =  number  of  eggs  of  each  sort, 
Then  will  -£x  =  cost  of  the  first  sort, 
And  \x  =  cost  of  the  second  sort ; 
But  5:2  : :  2x  (the  whole  number  of  eggs)  :  |* ; 
Hence  jx  =  price  of  both  sorts,  at  5  for  2  pence  ; 
Then  by  the  question  |r  +  J*  —  f  x  =  3  ; 
JVfult.  by  2,  gives    -     x  +  \x  —  -fx  =  6  ; 
And  mult,  by  3,  gives  5x  —  *£x  —  IB; 
Also  mult,  by  5,  gives  x  =  90,  the  number  of  tfjgt  *t 
each  sort. 


246 


ALGEBRA* 


Quest.  9.  Two  persons,  a  and  b,  engage  at  play.  Be- 
fore they  begin,  a  has  80  guineas,  and  b  has  60.  After  a 
Certain  number  of  games  won  and  lost  between  them,  a  rises 
with  three  times  as  many  guineas  as  b.  Query,  how  many 
guineas  did  a  win  of  b  ? 

Let  x  denote  the  number  of  guineas  a  won. 
Then  a  rises  with  80  +  x> 
And  n  rises  with  60  —  x ; 
Theref.  by  the  quest.  80  +  x  =  180  —  Sx  ; 
Transp.  80  and  3x,  gives  Ix  =  100  ; 
And  dividing  by  1,  gives  x  =  25,  the  guineas  won. 


QUESTIONS  FOB  PRACTICE. 

1.  To  determine  two  numbers  such,  that  their  difference 
may  be  4,  and  the  difference  of  their  squares  64. 

Ans.  6  and  10. 

2.  To  find  two  numbers  with  these  conditions,  viz.  that 
half  the  first  with  a  third  part  of  the  second  may  make  9, 
and  that  a  4lh  part  of  the  first  with  a  5th  part  of  the  second 
may  make  5.  Ans.  8  and  15. 

3.  To  divide  the  number  20  into  two  such  parts,  that  a 
3d  of  the  one  part  added  to  a  5th  of  the  other,  may  make  6. 

Ans.  15  and  5. 

4.  To  find  three  numbers  such,  that  the  sum  of  the  1st 
and  2d  shall  be  ?,  the  sum  of  the  1st  and  3d  8,  and  the  sum 
of  the  2tl  and  3d  0.  Ans.  3,  4,  5. 

5.  A  father,  dying,  bequeathed  his  fortune,  which  was 
2800/,  to  his  son  and  daughter,  in  this  manner  ;  that  for  eve- 
ry half  crown  the  son  might  have,  the  daughter  was  to  have 
a  shilling.    What  then  were  their  two  shares  ? 

Ans.  The  son  2000/  and  the  daughter  800L 

6.  Three  persons,  a,  b,  c,  make  a  joint  contribution,  which 
in  the  whole  amounts  to  400/ :  of  which  sum  b  contributes 
twice  as  much  as  a  and  20/  more  ;  and  c  as  much  as  a  and 
b  together.    What  sum  did  each  contribute  ? 

Ans.  a  60/,  b  140/,  and  c  2001. 

7.  A  person  paid  a  bill  of  100/  with  half  guineas  and 
crowns,  using  in  all  202  pieces  ;  how  many  pieces  were  there 
of  each  sort  ?  Ans.  180  half  guineas,  and  22  crowns. 


SIMPLE  EQUATIONS. 


247 


8.  Says  a  to  u,  if  you  give  me  10  guineas  of  your  money, 
,  I ,  Bhall  then  have  twice  ?.s  much  us  you  will  have  left  :  but 

says  n  to  a,  give  me  10  of  your  guineas,  and  then  I  shall 
have  3  times  as  many  as  you.    How  many  had  each  ? 

A  us.  a  22,  n  2G. 

9.  A  person  goes  to  a  tavern  with  a  curtain  quantity  of 
money  in  his  poc!:et,  where  ho  spends  2  .shillings  ;  he  then 
borrows  as  much  money  as  h:j  had  left,  and  going  to  another 
tavern,  he  there  spends  '2  shillings  also  ;  then  borrowing 
again  as  much  money  as  was  left,  he  went  to  a  third  tavern, 
where  likewise  he  spent  2  shillings  ;  and  thus  repeating  tho 
same  at  a  fourth  tavern,  he  then  had  nothing  remaining. 
What  sum  had  he  at  first  !  A  us.  3*.  Orf. 

10.  A  man  with  his  wife  and  child  dine  together  at  an 
inn.  The  landlord  charged  1  shilling  for  the  child  ;  and  for 
the  woman  he  charged  as  much  as  for  the  child  and  \  as 
much  as  for  the  man  ;  and  for  the  man  he  charged  as  much 
as  for  the  woman  and  child  together.  How  much  was  that 
for  each  ?  Ans.  The  woman  20c/  and  the  man  32</. 

11.  A  cask,  which  held  (50  gallons,  was  tilled  with  a 
mixture  of  brandy,  wine,  and  cyder,  in  this  manner,  viz. 
the  cyder  was  0  gallons  more  than  tho  brandy,  and  the 
wine  was  as  much  as  the  cyder  and  \  of  the  brandy.  How 
much  was  there  of  each  ? 

Ans.  Brandy  15,  cyder  21,  wine  24. 

12.  A  general,  disposing  his  armv  into  a  square  form, 
finds  that  he  has  2 SI  men  more  than  a  perfect  square  :  but 
increasing  the  side  by  1  niau,  he  men  wants  25  men  to  be  a 
complete  square.  How  iininv  men  had  lie  under  his  com- 
mand ?  "  Ans.  '24000. 


13.  What  number  is  that,  to  which  if  3.  5,  and  8,  bo 
severally  added,  the  three  Minis  shall  be  in  geometrical  pro- 
gression ?  Ans.  1. 

14.  The  stock  of  three  traders  amounted  to  7*50/  :  the 
shares  of  the  first  and  second  exceeded  that  of  the  third 
by  240  :  and  the  sum  of  the  2d  and  3d  exceeded  the  first 
by  360.    What  was  the  share  of  each  .' 

Ans.  The  1st  200,  the  2d  300,  the  3d  200. 

15.  What  two  numbers  are  those,  which,  !;cing  in  the 
ratio  of  3  tu  1,  their  product  is  equal  to  12  times  their  sum 


248 


ALGEBRA. 


16.  A  certain  company  at  a  tavern,  when  they  came  to 
settle  their  reckoning,  found  that  had  there  been  4  more  in 
company,  they  might  have  paid  a  shilling  each  less  than 
they  did  ;  but  that  if  there  had  been  3  fewer  in  company, 
they  must  have  paid  a  shilling  each  more  than  they  did. 
What  then  was  the  number  of  persons  in  company,  what 
each  paid,  and  what  was  the  whole  reckoning  ? 

Ans.  24  persons,  each  paid  7s,  and  the  whole 
reckoning  8  guineas. 

17.  A  jockey  has  two  horses  :  and  also  two  saddles,  the 
one  valued  at  18/.  the  other  at  3/.  Now  when  he  sets  the  - 
better  saddle  on  the  1st  horse,  and  the  worse  on  the  2d,  it 
makes  the  first  horse  worth  double  the  2d  ;  but  when  he 
places  the  better  saddle  on  the  2d  horse,  and  the  worse  on 
the  first,  it  make*  the  2d  horse  worth  three  times  the  1st. 
What  then  were  the  values  of  the  two  horses  ? 

Ans.  The  1st  0/,  and  the  2d  9/. 

18.  What  two  numbers  arc  as  2  to  3,  to  each  of  which  if 
6  be  added,  the  sums  will  be  as  4  to  5  ?         Ans.  0  and  O. 

19.  What  arc  those  two  numbers,  of  which  the  greater  is 
to  the  less  as  their  sum  is  to  20,  and  as  their  difference  is  to 
10?  Ans.  15  and  45. 

20.  What  two  numbers  are  those,  uhosc  difference,  sum, 
and  product,  are  to  each  other,  as  the  three  numbers  2, 
3,  5  ?  Ans.  2  and  10. 

21.  To  find  three  numbers  in  arithmetical  progression,  of 
which  the  first  is  to  the  third  as  5  to  0,  and  the  sum  of  all 
three  is  03.  Ann.  15,  21,  27. 

22.  It  is  required  to  divide  the  number  2i  into  two  such 
parts,  that  the  quotient  of  the  greater  part  divided  by  the 
less,  may  be  to  the  quotient  of  the  less  part  divided  by  the 
greater,  as  4  to  1.  Ans.  10  and  8. 

23.  A  gentleman  being  asked  the  age  of  his  two  sons, 
answered,  that  if  to  the  sum  of  their  ages  18  be  added,  the 
result  will  be  double  the  age  of  the  elder ;  but  if  0  be  taken 
from  the  difference  of  their  ages,  the  remainder  will  be  equal 
to  the  age  of  the  younger.    What  then  were  their  ages  ? 

Ans.  30  and  12. 

24.  To  find  four  numbers  such,  that  the  sum  of  the  1st, 
2d,  and  3d  shall  be  13  ;  the  sum  of  the  1st,  2d,  and  4th, 
15  ;  the  sura  of  the  1st,  3d,  and  4th,  18  ;  and  lastly,  the  sum 
of  the  2d,  3d,  and  4th,  20.  Ans.  2,  4,  7,  9. 


4/  / 


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QUADRATIC  EQUATIONS. 


249 


• 

25.  To  divide  48  into  4  such  parts,  that  the  first  increased 
by  3,  the  second  diminished  by  3,  the  third  multiplied  by  3, 
and  the  4th  divided  by  3,  may  be  all  equal  to  each  other. 

Ans.  6,  12,  3,  27. 


QUADRATIC  EQUATIONS. 

Quadratic  Equations  are  either  simple  or  compound. 

A  simple  quadratic  equation,  is  that  which  involves  the 
square  only  of  the  unknown  quantity.  As  ax3  =  b.  The 
solution  of  such  quadratics  has  been  already  given  in  simple 
equations. 

A  compound  quadratic  equation,  is  that  which  contains 
the  square  of  the  unknown  quantity  in  one  term,  and  the 
first  power  in  another  term.    As  or1  +  bx  =  c. 

All  compound  quadratic  equations,  after  being  properly 
reduced,  fall  under  the  three  following  forms,  to  which  they 
must  always  be  reduced  by  preparing  them  for  solution. 

1.  x3  +  ar  =  6 

2.  xa—  ax  =  b 

3.  x*  —  ax  =  —b 

The  general  method  of  solving  quadratic  equations,  is  by 
what  is  called  completing  the  square,  which  is  as  follows  : 

1.  Reduce  the  proposed  equation  to  a  proper  simple  form, 
as  usual,  such  as  the  forms  above  ;  namely,  by  transposing 
all  the  terms  which  contain  the  unknown  quantity  to  one 
aide  of  the  equation,  and  the  known  terms  to  the  other  ; 
placing  the  square  term  firs.,  and  the  single  power  scr  md  ; 
dividing  the  equation  by  the  co-efficient  of  the  square  or 
first  term,  if  it  has  one,  and  changing  the  signs  of  all  the 
terms,  when  that  term  happens  to  be  negative,  as  that 
term  must  always  be  made  positive  before  the  solution. 
Then  the  proper  solution  is  by  completing  the  square  as 
follows,  viz. 

2.  Complete  the  unknown  side  to  a  square,  in  this  man. 
ner,  viz.  Take  half  the  co-efficient  of  the  socond  term,  «r»d 
square  it ;  which  square  add  to  both  sides  of  the  equation, 
then  that  side  which  contains  the  unknown  quantity  will  be 
a  complete  square. 

Vol.  L  33 


250 


ALGEBRA. 


3.  Then  extract  the  square  root  on  both  sides  of  the 
equation*,  and  the  value  of  the  unknown  quantity  will  be 
determined,  making  the  root  of  the  known  side  either  +  or 
— ,  which  will  give  two  roots  of  the  equation,  or  two  values  of 
the  unknown  quantity. 


*  As  the  square  root  of  any  quantity  may  be  cither  +  or—;  there- 
fore all  quadratic  equations  admit  of  two  solutions.  Thus,  the  square 
root  of  -j-  n* 's  either  -j-  n  or  —  n;  for  -j-  n  X  +  «  and  —  n  X  —  • 
are  each  equal  to  -|-  na.  But  the  square  root  of  —  n8,  or  V  —  is 
imaginary  or  impossible,  as  neither  -j-  n  nor  —  n,  when  squared,  gives 

—  i* 

So.  in  the  first  form,  x*~±-az  -  ft,  where  x  -j-  fa  is  found  =  V(b  + 
the  root  may  be  either  -J-  V(b  +  fa2),  or  —  V(b  -j-  fa2\  since  either 
of  them  being  multiplied  by  itself  produces  b -\-  fa\   And  this  ambi- 
guity is  expressed  by  writing  the  uncertain  or  double  sign  +  before 
V(b  4-  fa*)  ;  thus  x  =  ±  V(b  +  fa2)  —  fa. 

In  this  form,  where  i  -  Hh  V(b  -\-  fa2) —  fa,  the  first  value  of  a:,  via. 
x  =  -j-  V(6  +  d«v)  —  4»  is  always  affirmative  ;  for  since  J«y-f  b  is 
greater  than  fa-,  the  greater  square  must  necessarily  have  the  greater 
root;  therefore  v(b  fa7),  will  always  be  greater  than  Vjir3,  or  its 
equal  fa  ;  and  consequently -j-  V(b-\-  fa*)  —  fa  will  always  be  affirm- 
ative. 

The  second  value,  viz.  x  —  —  \/(b  -)-  fa2)  —  fa  will  always  \te  nega- 
tive, because  it  is  composed  of  two  negative  terms.  Therefore  when 
x9  -}-  ax  =  b,  we  shall  have  x  —  -j-  \'{b  -f-  ja3)  —  for  the  affirmative 
value  of  x%  and  x  =  —        -f-  Ja2)  —      for  the  negative  value  of  x. 

In  the  second  form,  where  x  =  ±  V(6  -f-  -f-  fa  tne  fi^t  value, 
viz.  i  —  +  H"  ~r  ?la  is  always  affirmative,  since  it  is  composed 
of  two  affirmative  terms.  But  the  second  value,  viz.  x  =  —  V(6-f  fa7) 
•4-  £a,  will  always  be  negative;  for  since  b-\-  fa2  is  greater  than  4«*t 
therefore  v(6  -{-  fa")  will  be  greater  than  vfa2,  or  its  equal  ^cr ;  and 
consequently  —  V(n  -|-  fa':)  \-  fa  is  always  a  negative  quantity. 

Therefore,  when  x2  —  ar  —  0,  we  shall  havez  —  -j-  \ '(b  -j-  fa2)  fa 
for  the  affirmative  value  of  x ;  and  x  =  — -  v(&  -)-  fa'<)  -j-  j«  for  toe 
negative  value  of  x;  so  that  in  both  the  first  arid  second  forms,  the  un- 
known quantity  has  always  two  value>,  one  of  which  is  positive,  and 
the  other  negative. 

But,  in  the  third  form,  whero  .t  -  -±  \  '(fa2  —  b) -'r  fa,  both  the 
values  of  x  will  be  positive,  when  fa2  is  greater  than  b.  For  the  first 
value,  viz.  x  =z  +  V(\al  —  b)  -f-  fa  will  then  be  affirmative,  being  com- 
posed of  two  affirmative  terms. 

The  second  value,  viz.  s  -  —  V(fa-  —  b)  -i-  fa  is  affirmative  also  ; 
for  since  fa2  is  greater  than  fa2—  b,  therefore  Vfa-  or  fa  is  greater  than 
V(fa2 —  b)  ;  and  consequently  —  v'(i«-  —  6)  -f-  A<i  will  always  be  an 
affirmative  quantity.    So  that,  when  x*  —  ax  —  —  b,  wc  shall  have  z 

—  +  v(fal  —  M  4a.  and  also  x  —  \  {fa2—  b)  -f-  fa,  for  the 
values  of  x,  both  positive. 

But  in  this  third  form,  if  b  be  greater  than  fa1,  the  solution  of  the  pro- 
posed question  will  be  i n  possible.  For  bince  the  square  of  any  quan- 
tity (whether  that  quantity  be  affirmative  or  negative)  is  always  affirma- 
tive, the  square  root  of  a  negative  quantity  is  impossible,  and  cannot 
be  assigned.  But  when  b  is  greater  than  fa\  then  fa*  —  b  is  a  nega- 
tive quuntity ;  and  therefore  its  root  V(faJ  —  b)  is  impossible,  or  ima- 
ginary ;  consequently,  in  that  case,  z  =  fa  +  V(fa~  —  b),  or  the  two 
rood  or  values  of  x,  are  both  impo^'ible^  or  ioiaginary  quantities. 


QUADRATIC  KQUATIONS. 


251 


Note,  1.  The  root  of  the  first  side  of  the  equation,  is 
always  equal  to  the  root  of  the  first  term,  with  half  the  co- 
efficient of  the  second  term  joined  to  it,  wi;ii  its  sign,  whether 
+  or — . 

2.  All  equations,  in  which  there  are  two  terms  including 
the  unknown  quantity,  and  which  have  the  index  of  the  one 
just  double  that  of  the  other,  are  resolved  like  quadratics,  by 
completing  the  square,  as  above. 

Thus,  x*  +  ax2  6,  or  x**  +  axn  =  b,  or  x  +  ax*  =  6, 
or  (x2  ±  ax)2  ±.  m{x2  :£  ax)  =  6,  are  analsgous  to  quadra- 
tics, and  the  value  of  the  unknown  quantity  may  be  deter, 
mined  accordingly. 

3.  For  the  construction  of  Quadratics,  see  vol.  ii. 

EXAMPLES. 

1.  Given  x*  +  4x  =  60 ;  to  find  x. 

First,  by  completing  the  square,  x'2  +  4r  +  4  =  64 ; 

Then,  by  extracting  the  root,  x  +  2  =  ±.  8  ; 

Then,  transpos.  2,  gives  x  =  6  or  — 10,  the  two  roots* 

9   2.  Given  xa  —  6x  +  10  =  65 ;  to  find  x. 
First,  trans.  10,  gives  x2  —  6x  =  55 ; 
Then  by  complet.  the  sq.  it  is  x2  —  6x  +  9  =  64  ; 
And  by  extr.  the  root,  gives  x  —  3  =  ±  8 ; 
Then  trans.  3,  gives  x  =  1 1  or  —  5. 

3.  Given  3x2  —  3*  +  9  *=  8|  ;  to  find  x. 
First  div.  by  3,  gives  x2  —  x  +  3  =  2 J  ; 
Then  transpos.  3,  gives  x2  —  x  =  —  J  ; 
And  compl.  the  sq.  gives  x2  —  x  +  J  =  ^ ; 
Then  extr.  the  root  gives  x  —  ^  =      i  ; 
And  transp.  J,  gives  x  =  |  or 

4.  Given  i*2  —  £r  +  30J  =  52£ ;  to  find  x. 
First  by  transpos.  30J,  it  is  \x2  —  \x  =  22$  ; 
Then  mult,  by  2  gives  x2—  §x=44£  ; 

And  by  compl.  the  sq.  it  is  x2— §x4-J=44J. 
Then  extr.  the  root  gives  x  —  £  =  tt  6} ; 
And  trans.  £,  gives  x  =  7  or  <—  6£  ; 

5.  Given  ax2  —  bx  =  c ;  to  find  x. 
First  by  div.  by  a,  it  is  x1 —  -  s  =  —  ; 


9B&  AXGBBRA. 

Then  compl.  the  sq.  gives  a*—-  a:  +^f=- 

b  4ac+  b* 

And  extrnc.  the  root,  gives  *  —  ^  =  :£  — ^ —  ; 

Then  transp.      gives  *  =  ±  + 

6.  Given  a* — 20**=  6  ;  to  find  a?. 

First  by  compl.  the  sq.  gives  a?— 2ox+oa==aa4-o ; 
And  extract,  the  root,  gives  a*—  a  =  ±  ^/(a2— b) ; 
Then  transpos.  a,  gives  a*  =  ±  ^/(a1  +  6)  +  a ; 
And  extract,  the  root,  gives  a?  =  +  ^/[a  +  ^/(a'+i)]. 


SXAMFLB8  FOR  PRACTICE*. 

J.  Given  a?— 62-7  =  33 ;  to  find  2.     Ans.  2  =  10  or-4. 


*  1.  Cubic  equations  when  occurring  in  pairs,  may  usually  be  reduced 
to  quadratic*,  by  extermination.  Thus, 

Suppose  4z  4-  3x*  -r-  6z  =  150  > 
and  3z*-f  2xa  +  2l  =  106  5 
Then  molt.  1st  equa.  by  3,  and  2d  by  4, 

1223  4-  9xa  4-  15z  =  450 
12x3  4-8**  +  gz  =420 

By  aobtr.        z*  4-  7x  =  30 

Compl.  the  sq.  z»  4-  7x  +      =  30  +  ±f.  =  xfi. 

Extr.  the  root  z   +  f  =  ±  V 

z   =  £=3  or  —  10. 

2.  Sometines,  when  the  unknown  square  has  a  co-efficient,  the  fol- 
lowing method  may  be  advantageously  adopted :  viz. 

Having  transposed  the  known  terms  to  one  side  and  the  unknown 
terms  to  the  other,  multiply  each  side  by  4  times  the  co-efficient  of  the 
unknown  square. 

Add  the  square  of  the  co-efficient  of  the  simple  power  of  the  un- 
known quantity,  to  both  sides;  the  first  side  will  then  be  a  complete 
square. 

Extract  the  root,  and  the  value  of  the  unknown  quantity  will  be  ob- 
tained. 

Thus,  if  5xa  +  4z  =  28. 

Then  mult,  by  4  X  5t  lOOx*  4-  80x  =  660 
Add    42.    .    100x2  4-  80x4-16*  =  576 
Eitr.  the  root,   lOz  -f  4  =  ±  24 
Transposing   .  lOz  =  20  or  —  28 
Dividing  by  10,    x  =  2,  or  —  2  8. 
The  principal  advantage  of  this  method,  which  is  due  to  the  Indians, 
Is  that  it  dots  not  introduce  fractions  into  the  operation.   It  will  have 
the  same  advantage  in  cases  where  the  square  has  00  co-efficient,  if  that 
of  the  simple  fwwer  be  an  odd  number. 


QUADRATIC  EQUATIONS. 


208 


2.  Given  X1— 5x— 10  =  14 ;  to  find  x.    Ans.  x  =  8  or  —  3. 

3.  Given  5x*  +  Ax  —  90  =  114  ;  to  find  x. 

Ans.  a?  =  6  or  —  ftf  • 

4.  Given  Jx1 — $x  +  2  =»  9  ;  to  find  x.  Ana.  x  =  4  or  -  3J. 

5.  Given  3x*  —  2x"  =  40  ;  to  find  a?.  Ans.  x  =  2  or  —2. 

6.  Given  Jx—  J^/x  =  1J ;  to  find  x.  An*,  x  =9  or  2}. 

7.  Given  ix*  +  fx  =  J  ;  to  find  x.  * 

Ans.  x  =  — |  ±  |  */70  —  -7277668  or  —2-0611000. 

8.  Given  x8  +  4x*  =  12  ;  to  find  x. 

Ans.  x  =       =  1-259921,  or  y  —  6  =  -  1-817121. 

9.  Given  X2  +  4x  =  a*  +  2  ;  to  find  x. 

Ans.  x  —  v'(«2+6)^2. 

questions  pboduoing  quadratic  equations. 

1.  To  find  two  numbers  whose  difference  is  2,  and  pro- 

duct 80. 

Let  x  and  y  denote  the  two  required  numbers. 
Then  the  first  condition  gives  x  —  y  =  2, 
And  the  second  gives  xy  •=  80. 
The  n  transp.  y  in  the  1st  gives  x  =  y  +  2  ; 
This  value  of  x  suhstitut.  in  the  2d,  is  y3  +  2y  =  80  ; 
Then  comp.  the  square  gives  y3  +  2y  +  1  =  81  ; 
And  extrac.  the  root  gives  y  +  1  =  9  ; 
And  transpos.  1  gives  y  =  8  ; 
And  therefore  x  =  y  +  2  =  10. 

2.  To  divide  the  number  14  into  two  such  parts,  that  their 

product  may  be  48. 
Let  x  and  y  donote  the  two  parts. 
Then  the  1st  condition  gives  x  +  y  *=  14, 
And  the  2d  gives  xy  =  48. 
Then  transp.  y  in  the  first  gives  x  =-*  14  —  y  ; 
This  value  subst.  for  x  in  the  2d,  is  14y  —  j/5  =  48  ; 
Changing  all  the  signs,  to  make  the  square  positive, 
gives  y2  —  14y  =  —  48  ; 
Then  com  pi.  the  square  gives  y3  —  14y  +  49  =  1  ; 
And  extrac.  the  root  gives  y  —  7  =  4-1; 
Then  transpos.  7,  gives  y  =  8  or  6,  the  two  parts. 

3.  What  two  numbers  are  those,  whose  sum,  product,  and 
difference  of  their  squares,  are  all  equal  to  each  other  ? 

Let  x  and  y  denote  the  two  numbers. 

Then  the  1st  and  2d  expression  give  x  +  y  =.  xy* 

And  the  1st  and  3d  give  x  +  y  =  a?— . 


254 


ALGEBRA. 


Then  the  last  equa.  div.  by  x  +  y,  gives  1  =  x  —  y ; 
And  transpos.  y,  gives  y  +  1  =  x  ; 
This  val.  substit.  in  the  1st  gives  2y  +  1  =  y'  +  y ; 
And  transpos.  2y,  gives  1  =  y2  —  y  ; 
Then  complet.  the  sq.  gives  f  =  y*  —  y  +  j  ; 
And  extracting  the  root  gives  J  ^5  =  y  —  £ ;  ■ 
And  transposing  \  gives  i  v/5  +  J  =  y  ; 
And  therefcre  x  =  y  +  1  =  J  + 
And  if  these  expressions  be  turned  into  numbers,  by  ex- 
tracting the  root  of  5,  &c.  they  give  x  =  2-6180  +,  and 
y=  1-6180  +. 

4.  There  are  four  numbers  in  arithmetical  progression,  of 
wtth  the  product  of  the  two  extremes  is  22,  and  that  of  the 
means  40 ;  what  are  the  numbers  ? 

Let  x  =  the  less  extreme, 

and  y  =  the  common  difference  ; 
Then  r,  x+y,  x-f 2y,  x-fc3y,  will  be  the  four  numbers. 
Hence,  by  the  1st  condition  .t2  +  3.ry  =  22, 
And  by  the  2d  x2  +  Sry  +  2ya  =  40. 
Then  subtracting  the  first  from  the  2d  gives  2y*  =  18  ; 
And  dividing  by  2  gives  y1  =  9 ; 
And  extracting  the  root  gives  y  =  3. 
Then  substit.  3  for  y  in  the  1st,  gives  x2  r|n  9x  =  22  ; 
And  completing  the  square  gives  x3 "+  9x  +  V  =  "f 9  ; 
Then  extracting  the  root  gives  x  -f-  J-  =  y  ; 
And  transposing  g-  gives  a:  =  2  the  least  number. 
Hence  the  four  numbers  are  2,  5,  8,  11. 

5.  To  find  3  numbers  in  geometrical  progression,  whose 
sum  shall  be  7,  and  the  sum  of  their  squares  21. 

Let  x,  y,  and  z  denote  the  Ihree  numbers  sought.  * 
Then  by  the  1st  condition  xz  =  y2, 
And  by  the  2d  x  +  y  +  z  =  7, 
And  by  the  3d  xa  +     +  z*  =  21. 
Transposing  y  in  the  2d  gives  x  +  z  =  7  —  y ; 
Sq.  this  equa.  gives  x2  ■+  2xx  +  2a  =  49  —  14y  +  y"; 
Substi.  2y2  for  2xs,  gives  x3  +  2y=  +  z2  =  49  —  14y     f ; 
Subtr.  y2  from  each  side,  leaves  x3  +  y2  +  z2  =  49 — 14y ; 
Pulling  the  two  values  of  x2  +  y3  +  z3  >  21  =  49_  -  m 
equal  to  each  other,  gives  $  y* 
Then  transposing  21  and  14y,  gives  14 v  =  28  ; 
And  dividing  by  14,  gives  y  =  2. 
Then  substit.  2  for  //  in  the  1st  equa.  gives  xz  =  4, 
And  in  the  4th,  it  gives  x  +  z  =  5 ; 
Transposing  z  in  the  last,  gives  x  =  5  —  z  ; 
This  subst.  in  the  next  above,  gives  bz — z*  =  4 ; 


QUADRATIC  EQUATIONS. 


255 


Changing  all  the  signs,  gives  r1  —  hz  =  —  4 ; 

Then  completing  the  square,  gives  z2  —  5z  +  V  =  {  ? 

And  extracting  the  root  gives  z  —  \  =  ±:  \\ 

Then  transposing  £,  gives  *  and  i  =  4  and  1,  the  two 

other  numbers* ; 
So  that  the  three  numbers  are  1,  2,  1. 

QUESTIONS  KOR  FRACTICK. 

1.  What  number  is  that  which  added  to  its  square  makes 
42?  Ans.  C,  or  —  7. 

2.  To  find  two  numbers  such,  that  the  less  may  be  to  \jfie 
greater  as  the  greater  is  to  12,  and  that  the  sum  of  Jhf  ir 
squares  may  be  45.  j\ns.  3  anR>. 

3.  What  two  numbers  are  those,  whose  difference  is  2, 
and  the  difference  oi' their  cubes  98?  Ans.  3  and  5. 

4.  WThat  two  numbers  arc  those,  whose  sum  is  0,  and  the 
sum  of  their  cubes  72  ?  *  Ans.  2  and  4. 

5.  What  two  numbcis  are  those,  whose  product  is  20,  and 
the  difference  of  their  cubes  (51  Ans.  4  and  5. 

6.  To  divide  the  number  11  into  two  such  parts,  that  the 
product  of  their  squares  may  be  784.  Ans.  4  and  7. 

7.  To  divide  the  number  5  into  two  such  parts,  that  the 
sum  of  their  alternate  quotients  may  b«;  that  is  of  the 
two  quotients  of  each  part  divided  by  the  other. 

Ans.  i  rsnd  4. 

8.  To  divide  12  into  two  such  parts,  Ihsit  their  product 
may  be  equal  to  8  limes  their  dilfei'Micc.         Ans.  1  and  8. 

1).  To  divide  the  number  10  into  two  such  parts,  that  the 
square  of  4  times  the  less  part,  may  be  112  more  than  the 
square  of  2  times  the  greater.  Ans.  4  and  6. 

10.  To  find  two  numbers  such,  that  the  sum  of  their 
squares  may  be  80,  and  their  sum  multiplied  by  the  greater 
may  produce  104.  J^ns.  5  and  8. 

11.  What  number  is  that,  which  bcin<*  divided  by  the 
product  of  its  two  dibits,  the  quotient  is  V;  ;  but  when  9  is 
subtracted  from  it,  there  remains  a  uurnher  Laving  the  same 
digits  inverted  ?  A  ns.  32. 

12.  To  divide  20  into  three  !>;•  its  suc:i.  the  continual 
product  of  all  throe  may  b*  2"0,  ;nnl  th.it  th«  difference  of 
the  first  and  second  may  b^  2  h  <..*  than  thi*  diflc  re  nee  of  the 
second  and  third.  Ans.  5,  6,  9. 

13.  To  find  three  numbers  in  arithmetical  progression^ 
such  that  the  sum  of  their  squares  may  he       wuixYifc  tori 


256  ALGEBRA. 

arising  by  adding  together  3  times  the  first  and  2  times  the 
second  and  3  times  the  third,  may  amount  to  32. 

Ans.  2, 4,  6. 

14.  To  divide  the  number  13  into  three  such  parts,  that 
their  squares  may  have  equal  differences,  and  that  the  sum 
of  those  squares  may  be  75.  Ans.  1,  5,  7. 

15.  To  find  three  numbers  having  equal  differences,  so 
mat  their  sum  may  be  12,  and  the  sum  of  their  fourth  powers 
062.  Ans.  3,  4,  5.. 

16.  To  find  three  numbers  having  equal  differences,  and 
such  that  the  square  of  the  least  added  to  the  product  of  the 
two  greater  may  make  28,  but  the  square  of  the  greatest 
adflsd  to  the  product  of  the  two  less  may  make  44. 

W  Ans.  2,  4,  0. 

17.  Three  merchants,  a,  r,  c,  on  comparing  their  gains 
find,  that  among  them  all  they  have  gained  1444/  ;  and  that 
b's  gained  added  to  the  square  root  of  a's  made  920/ ;  but  if 
added  to  the  square  root  of  c*s  it  made  912/.  What  were 
their  several  gains  ?  Ans.  a  400,  b  900,  c  144. 

.18.  To  find  three  numbers  in  arithmetical  progression,  so 
that  the  sum  of  their  squares  shall  be  93  ;  also  if  il  e  first 
be  multiplied  by  3,  the  second  by  4,  and  the  third  by"  5, 
the  sum  of  the  products  may  be  66."  Ans.  2,  5,  8. 

19.  To  find  two  numbers  such,  that  their  product  added 
to  their  sum  may  make  47,  and  their  sum  taken  from  the 
sum  of  their  squares  mr.y  leave  02.  Ans.  5  and  7* 


RESOLUTION  OF  CUBIC  AND  HIGHER 
EQUATIONS. 

A  Cubic  Equation,  or  Equation  of  the  3d  degree  or 
power,  is  one  that  contains  the  third  power,  of  the  unknown 
quantity.    As  i3  -  ar-  +  bx  =  c. 

A  Biquadratic,  or  Double  Quadratic,  is  an  equation  that 
contains  the  4th  power  of  the  unknown  quantity  : 
As  x*  —  ax3  -f  bxJ  —  cx  =  d. 
An  Equation  of  the  5th  Power  or  Decree,  is  one  that 
contains  the  5th  power  of  the  unknown  quantity. 

As  x3—  uxA  +  W  —  cx2  +  clx  =-=  e. 
And  so  on,  for  all  other  higher  powers,    \fhere  it  is 
to  be  noted,  however,  that  all  the  powers,  or  terms,  in  the 


=4  y=J" 


 ne  <     —  **- 


\  . «*-  •••• 


CUBIC,  X4UAT10X8. 


equation,  are  supposed  to  be  freed  from  surds  or  fractional 
exponents. 

There  are  many  particular  and  prolix  rules  usually  given 
for  the  solution  of  some  of  the  above-mentioned  powers 
or  equations.  But  they  may  be  all  readily  solved  by  the 
following  easy  rule  of  Double  Position,  sometimes  called 

Trial -and-E  rror  *. 

i 

RULE. 

1.  Find,  by  trial,  two  numbers,  as  near  the  true  root  as 
you  can,  and  substitute  them  separately  in  the  given  equa- 
tion, instead  of  the  unknown  quantity  ;  and  find  how  much 
the  terms  collected  together,  according  to  their  signs  7-  or 
— ,  differ  from  the  absolute  known  term  of  the  equation, 
marking  whether  these  errors  are  in  excess  or  defect. 

2.  Multiply  the  difference  of  the  two  numbers,  found  or 
taken  by  trial,  by  either  of  the  errors,  and  divide  the  pro- 
duct by  the  difference  of  tho  errors,  when  they  are  alike, 
but  by  their  sum  when  they  arc  unlike.  Or  say,  As  the 
difference  or  sum  of  the  errors,  is  to  the  difference  of  the 
two  numbers,  so  is  either  error  to  the  correction  of  its  sup- 
posed number. 

3.  Add  the  quotiont,  last  found,  to  the  number  belonging 
to  that  error,  when  its  supposed  number  is  too  little,  but 
subtract  it  when  too  great,  and  the  result  will  give  tho  true 
root  nearly. 

4.  Take  this  root  and  the  nearest  of  the  two  former,  or 
any  other  that  may  be  found  nearer :  and,  by  proceeding  in 
like  manner  as  above,  a  root  will  be  had  still  nearer  than 
before.    And  so  on,  to  any  degree  of  exactness  required. 

Note  1.  It  is  best  to  employ  always  two  assumed  num- 
bers that  shall  differ  from  each  other  only  by  unity  in  the 
last  figure  on  the  right  hand  ;  because  then  the  difference, 
or  multiplier,  is  only  1.  It  is  also  best  to  use  always  the 
least  error  in  the  above  operation. 

NoU  2.  It  will  be  convenient  also  to  begin  with  a  single 


*  See,  farther,  that  portion  of  vol.  ii.  which  relates  to  equations,  their 
construction,  be. 

A  new  and  ingenious  general  method  of  solving  equations  has  been 
recently  discovered  by  Messrs.  //.  Atkinson,  Holared,  and  Horner,  inde- 
pendently of  each  other.   For  the  best  pratical  view  of  this  new  <Ki«\ta&. 
and  its  applications,  consult  the  Elementary  Treatise  of  Algebra,  TAx, 
J.  R,  Young;  a  work  which  deserves  our  cordial  reuimoiefedtttoft* 
Vol.  L  34 


258 


-"ALGEBRA. 


figure  at  first,  trying  several  single  figures  till  thero  be  found 
the  two  nearest  the  truth,  the  one  too  little,  and  the  other 
too  great ;  and  in  working  witli  them,  find  only  one  more 
figure.  Then  substitute  this  corrected  result  in  the  equation, 
for  the  unknown  letter,  and  if  the  result  prove  too  little, 
substitute  also  the  number  next  greater  for  the  second  sup. 
position  ;  but  contrarywise,  if  the  former  prove  too  great, 
then  take  the  next  less  number  for  the  second  supposition  ; 
and  in  working  with  the  second  pair  of  errors,  continue  the 
quotient  only  so  far  as  to  have  the  corrected  number  to  four 
places  of  figures.  Then  repeat  the  same  process  again  with 
this  last  corrected  number,  and  the  next  greater  or  less,  as 
the  case  may  require,  carrying  the  third  corrected  number 
to  tight  figures ;  because  each  new  operation  commonly 
doubles  the  number  of  true  figures.  And  thus  proceed  to 
any  extent  that  may  be  wanted. 


EXAMPLES. 


Ex.  1.  To  find  the  root  of  the  cubic  equation  ar1  +  jr  + 
x=  100,  or  the  value  of  x  in  it. 


Here  it  is  soon  found  that 
x  lies  between  i  and  5.  As- 
sume therefore  these  two  num- 
bers, and  the  operation  will  be 
as  follows  : 
k  1st  Sup.  2d  Sup. 

4  -  x  5 
Hi  -  Xs  -  25 
61       -  -  125 


84 
100 

—10 


sums  - 
but  should  be 

-    errors  - 


+55 


the  sum  of  which  is  71. 
Then  as  71  :  1  :  :  1G  :  -2 
Hence  x  =  4 '2  nearly. 


Again,  suppose  4*2  and  4-3, 
and  repeat  the  work  aa  fol- 
lows : 


155 
100 


1st  Sup. 
42 
1704 
74  088 

05-928 
100 


x 

x2 

X3 

sums 


2d  Sup. 
4-3 
.  18-49 
.  79-507 

102-297 
100 


072    errors  +2-297 


the  sum  of  which  is  &l 
!  As  0-309  :-l  :  :  2-297:  0-036 
I  This  taken  from     -  4-300 


loaves  x  nearly 


=  4-264 


CUBIC,  Ac.  EQUATIONS. 


250 


Again,  suppose  4*264,  and  4*265,  and  work  as  follows: 


4*264 

X 

4*265 

18181696 

X* 

18*100225 

77-526752 

x1 

77*581310 

99-972448 

sums 

100036535 

100 

100 

-0027552 

errors  - 

+0  036535 

tbe  sum  of  which  is  -064087. 
Then  as  -064087  :  -001  :  :  027552  :  0  0004299 


To  this  adding      -  4*264 
gives  x  very  nearly  =  4-2644209 


The  work  of  the  example  above  might  have  been  much 
shortened,  by  the  use  of  the  Table  of  Powers  in  the  Arith- 
metic, which  would  have  given  two  or  three  figures  by  in- 
spection. But  the  example  has  been  worked  out  so  particu- 
larly as  it  is,  the  better  to  show  the  method. 

Ex.  2.  To  find  the  root  of  the  equation  z3  —  15x2  +  63x 
=  50,  or  the  value  of  x  in  it. 

Here  it  soon  appears  that  x  is  very  little  above  1. 


Suppose  therefore  1  *0and  1*1, 
and  work  as  follows : 


10 


1*1 


63  0  -   63x     -  69*3 
—15      — 15*1  —1815 
1     .      Xs    -  1-331 


49 

50 


~   sums   •  52*481 
50 


—l    -  errors  +2*481 
3*481  sum  of  the  errors. 
As  8*481 : 1 : :  *1 :  -03correct. 
1*00 

Hence  xa  1-03 nearly. 


Again,  suppose  the  two  num. 
bers  1*03  and  1-02,  &c.  as 
follows  : 
1*03    .       i  -  1-02 

64*89    -  63*  64*26 
—15*9135- IS*3— 15*6060 
1-092727    x3    1 -061208 


50  069227 sums  49-715208 
50  50 


+ •0(S9227er  rors — -284792 
•284792* 


As   -354019 :  -01  : :  -069227: 
•0019555 
This  taken  from     1  -03 


leaves  x  nearly  =  1*02804 


960 


Note  3.  Every  equation  has  as  many  roots  as  it  contains 
dimensions,  or  as  there  are  units  in  the  index  of  its  highest 
power.  That  is,  a  simple  equation  has  only  one  value  of 
the  root ;  but  a  quadratic  equation  has  two  values  or  roots, 
a  cubic  equation  has  three  roots,  a  biquadratic  equation  has 
four  roots,  and  so  on. 

When  one  of  the  roots  of  an  equation  has  been  found  by 
approximation,  as  above,  the  rest  may  be  found  as  follows. 
Take,  for  a  dividend,  the  given  equation,  with  the  known 
term  transposed,  with  its  sign  changed,  to  the  unknown  side 
of  the  equation ;  and,  for  a  divisor,  take  x  minus  the  root 
just  found.  Divide  the  said  dividend  by  the  divisor,  and 
the  quotient  will  be  the  equation  depressed  a  degree  lower 
than  the  given  one. 

Find  a  root  of  this  new  equation  by  approximation,  as  be- 
fore, or  otherwise,  and  it  will  be  a  second  root  of  the  origin- 
al equation.  Then,  by  means  of  this  root,  depress  the  se- 
cond equation  one  degree  lower,  and  from  thence  find  a  third 
root ;  and  so  on,  till  the  equation  be  reduced  to  a  quadratic  ; 
then  the  two  roots  of  this  being  found,  by  the  method  of  com- 
pleting the  square,  they  will  make  up  the  remainder  of  the 
roots.  Thus,  in  the  foregoing  equation,  having  found  one 
root  to  be  1  '02804,  connect  it  by  minus  with  x  for  a  divisor, 
and  the  equation  for  a  dividend,  &c.  as  follows : 

x  —  1-02804  )  s3  -  15r»  +  63*  —  50  (  x*  -  13-97196*  + 

48-63627  =  0. 

Then  the  two  roots  of  this  quadratic  equation,  or  -  -  - 
Xs—  13-97196*  =  —  48-63627,  by  completing  the  square, 
are  6-57653  and  7*39543,  which  are  also  the  other  two  roots 
of  the  given  cubic  equation.  So  that  all  the  three  roots  of 
that  equation,  viz.  r1-  Ibx2  +  63j?  =  50, 

and  the  sum  of  all  the  roots  is  found  to  be 
15,  being  equal  to  the  co-efficient,  of  the  2d 
term  of  the  equation,  which  the  sum  of  the 
roots  always  ought  to  be,  when  they  are 
right. 

Note  4.  It  is  also  a  particular  advantage  of  the  foregoing 
rule,  that  it  is  not  necessary  to  prepare  the  equation,  as  for 
other  rules,  by  reducing  it  to  the  usual  final  form  and  state 
of  equations.  Because  the  rule  may  be  applied  at  once  to  an 
unreduced  equation,  though  it  be  ever  so  much  embarrassed 


arc  1  02804 
and  6-57653 
and  7-39543 


sum  15-00000 


CUBIC. 


mvATiont. 


9tl 


by  mid  and  compound  quantities.  As  in  the  following  ex- 
ample: 

Ex.  3.  Let  k  be  required  to  find  the  root  x  of  the  equation 
y(144**  —  (jr»  +  20)»)  +  +  24)1)  »  114,  or 

the  value  of  x  in  it. 

By  a  few  trials  it  is  soon  found  that  the  value  of  x  is  but 
little  above  7.  Suppose  therefore  first  that  x  is=7,  and  then 
x  =  8. 

First,  when  x  =  7,  Second,  when  *  =  8. 

47-906   .   -/[144*1— («»  +  20)n     -  46-476 
65-384   .   v/flOO*1  — (xa  +  24)«] 


113-  290 

114-  000 

—0-710 
+1759 


-  the  sums  of  these 

-  the  true  number 

•   the  two  errors 


115-750 
114-000 

+1-750 


As  2-469  :  1 


0-710  :  0-2  nearly. 
70 


Therefore  x  =  7-2  nearly. 


Suppose  again  x  =  7-2,  and  then,  because  it  turns  out  too 
great,  suppose  x  also  =  7-1,  dec.  as  follows : 


Supp.  x  =  7-2, 

47-990  .  v/[144xa—  (s8  +  20)2] 
66-402    .     ^[196**—  (x*  +  24)2] 

414*392    -   the  sums  of  these 
114-000    -   the  true  number 


+0-392 
0123 


the  two  errors 


Supp.  *  =  7-l, 
-  47-973 
.  65-904 


113-  877 

114- 000 

—0128 


As   -515  :  1 


*123  :  -024  the  correction, 
7-100  add 


Therefore  x  =  7*124  nearly  the  root  required. 

Nate  5.  The  same  rule  also,  among  other  more  difficult 
forms  of  equations,  succeeds  very  well  in  what  are  caiUd 
exponential  ones,  or  those  which  have  an  *^a*a&« 


an 


ALGEBRA. 


ty  in  the  exponent  of  the  power ;  as  in  the  following  ex- 
ample : 

Ex.  4.   To  find  the  value  of  x  in  the  exponential  (equation 

For  more  easily  resolving  such  kinds  of  equations,  it  is 
convenient  to  take  the  logarithms  of  them,  and  then  com- 
pute the  terms  by  means  of  a  table  of  logarithms.  Thus, 
the  logarithms  of  the  two  sides  of  the  present  equation  are 
x  X  log.  of  x  =  2,  the  log.  of  100.  Then,  by  a  few  trials, 
it  is  -soon  perceived  that  the  value  of  x  is  somewhere  be- 
tween the  two  numbers  3  and  4,  and  indeed  nearly  in  the 
middle  between  them,  but  rather  nearer  the  latter  than  the 
former.  Taking  therefore  first  x  =  3  5,  and  then  =■  3*6, 
and  working  with  the  logarithms,  the  operation  will  be  as 
follows : 


First  Supp.  x  =  3-5.  . 
Log.  of  3-5  =  0-544068 
then  3-5 Xlog.3  5=1  -904238 


Second  Supp.  x  =  3*6. 
Log.  of  3  6  =  0*556303 
then  3-6  X  log.  3  6=2-002689 


the  true  number  2-000000  I       the  true  number  2*000000 


error,  too  little,  —  -095762 
•002689 


error,  too  great,  +  -002689 


•098451  sum  of  the  errors.  Then. 


As  -098451  :  -1  :  :  -002689  :  0  00273  the  correction 
taken  from  3-60000 


leaves   -    3*59727  =  x  nearly. 


By  repeating  the  operation  with  a  larger  table  of  loga- 
rithms, a  nearer  value  of  x  may  be  found  3*597285. 

This  method,  indeed,  may  be  a  little  improved  in  practice : 
for  since  x*  =  a,  we  have  by  logarithms  x  X  log.  x  =  log.  a ; 
and  again,  log.  x  +  log.  log.  x  =  log.  log.  a.  We  have 
therefore  only  to  find  a  number,  which,  added  to  its  log.  will 
will  be  equal  to  the  log.  of  the  log.  of  the  given  number  ; 
and  the  natural  number  answering  to  this  number,  is  the  va- 
lue of  x  required. 

In  illustration  of  the  above,  take  the  12th  example  :  — 
«•  =  123456789.  First,  log.  123456789  =  8 -0915143,  and 
log.  8*0915148  =  -9080298.  Searching  in  a  table  of  loga- 
liSaoB,  we  find  the  nearest  number  -93651 ;  which  added  to 


CUBIC,  AiCrn  EQUATIONS.  263 

its  logarithm  —  1-0715124  =  -9080224.  The  next  higher 
number  '93652  +  its  log.  =  -9080371.  Hence 

-9080371  -9080298 

•9080224         -9080224       74  —  147  =  -503 


147  74 


Therefore,  the  number  sought  is  '93651503,  the  natural 
number  answering  to  which  is  8-640026  the  value  of  x, 
which  is  true  to  the  last  figure,  the  value  given  by  Dr.  Hut* 
ton  being  8-6400268. 

The  common  logarithmic  solution  fails  when  a  is  less  than 
unity,  its  log.  being  then  negative.  In  this  case,  assume 
x  =  1  -f-  y,  and  a  =- 1  e,  which  transforms  the  given  equa. 
x*  =  af  to  &  =  y.  Taking  the  logs,  twice,  we  get  y  log. 
t  =  log.  y,  and  log.  y  +  log.  of  log.  e  =  log.  of  log.  y  ;  or, 
putting  log.  y  =  »,  and  log.  of  log.  e  =  *,  we  have  v  +  *  = 
log.  v,  an  equation  easy  to  solve. 

Ex.  5.  To  find  the  value  of  x  in  the  equation  x3  +  lOx3 
+  5*  =  260.  Ans.  x  =  4-1 179857. 

Ex.  6.  To  find  the  value  of  x  in  the  equation  x3 — 2x=50. 

Ans.  3-8648854. 

Ex.  7.  To  find  the  value  of  x  in  the  equation  x3  +  2x2  — 
23x  =  70.  Ans.  x  =  5-13457. 

Ex.  8.  To  find  the  value  of  x  in  the  equation  x3 — 17x2 
+  54x  =  350.  Ans.  x  =  14-95407. 

Ex.  9.  To  find  the  value  of  x  in  the  equation  x4  —  3x*  — 
75x  =  10000.  Ans.  x  =  10-2609. 

Ex.  10.  To  find  the  value  of  x  in  the  equation  2x4 —  16x3 
+  40X3  —  30x  =  —  1.  Ans.  x  =  1-284724. 

Ex.  11.  To  find  the  value  of  x  in  the  equation  Xs  +  2x4 
+  Sx3  +  4X8  +  5x  =  54321 .  Ans.  x  =  8*414455. 

Ex.  12.  To  find  the  value  of  x  in  the  equation  x*  = 
123456789.  Ans.  x  =  8  6400268. 

Ex.  13.  Given  2x4  —  7x3+  llx3  —  3x  =  11,  to  find  *. 

Ex.  14.  To  find  the  value  of  x  in  the  equation. 

(3x*  —  2y/x  +  1)?  —  (x2  —  4*v/x  +  3v'x)*  =  56. 

Ans.  x  =  18-360877. 


90* 


To  resolve  Cubic  Equations  bp  Cardan's  Rule. 

Though  the  foregoing  general  method,  by  the  application 
of  Double  Position,  be  the  readiest  way,  in  reul  practice,  of 
finding  the  roots  in  numbera  of  cubic  equations,  as  well  as 
of  all  the  higher  equations  universally,  we  may  here  add  the 
particular  method  commonly  called  Cardan's  Rule,  for  re- 
solving cubic  equations,  in  case  any  person  should  choose 
occasionally  to  employ  that  method  ;  although  it  is  only  ap- 
plicable when  two  of  the  roots  are  impossible. 

The  form  that  a  cubic  equation  ihust  necessarily  have,  to 
be  resolved  by  this  rule,  is  this,  viz.  z1  +  az  =  6,  that  is, 
wanting  the  second  term,  or  the  term  of  the  2d  power  z*. 
Therefore,  after  any  cubic  equation  hns  been  reduced  down 
to  its  final  usual  form,  x3  +  px*  +  qx  =  r,  freed  from  the 
co-efficient  of  its  first  term,  it  will  then  be  necessary  to  take 
away  the  2d  term  px2 ;  which  is  to  be  done  in  this  manner ; 
Take  Jp,  or  £  of  the  co-efficient  of  the  second  term,  and 
annex  it,  with  the  contrary  sign,  to  another  unknown  letter 
z,  thus  z  —  Jp ;  then  substitute  this  for  x,  the  unknown 
letter  in  the  original  equation  x3  +  px2  +  qx  =  r,  and  there 
will  result  this  reduced  equation  z'J  ±az  b,  of  the  form 
proper  for  applying  the  following,  or  Cardan's  rule.  Or 
take  c  =  J  a,  and  d  =  J6,  by  which  the  reduced  equation 
takes  this  form,  z3  +  3cz  =  2d. 

Then  substitute  the  values  of  c  and  d  in  this 

form,  %  =  V[d  +         +  J)]  +  V[d  -  y/{*  +  O],  > 

or  ,  =  „[*  +        +  O]  -  w^w+^y  \ 

and  the  value  of  the  root  z,  of  the  reduced  equation  z3  + 
az  =  b,  will  be  obtained.  Lastly,  take  x  =  z  —  |p,  which 
will  give  the  value  of  r,  the  required  root  of  the  original 
equation  x3  +  px3  +  qx  =  r,  first  proposed. 

One  root  of  this  equation  being  thus  obtained,  then  de- 
pressing the  original  equation  one  degree  lower,  after  the 
manner  described,  p.  260,  the  other  two  roots  of  that  equa- 
tion will  be  obtained  by  means  of  the  resulting  quadratic 
equation. 

Note.  When  the  co-efficient  a,  or  c,  is  negative,  and  c3  is 
greater  than  this  is  called  the  irreducible  case,  because 
then  the  solution  cannot  be  generally  obtained  by  this  rule*. 


*  Suppose  a  root  to  consist  of  the  two  parts  z  and  y,  so  that  (x  +  y) 
as  jr;  which  sum  substituted  for  z,  in  the  given  equation  *3  +  a*  = 


cubic,  4ce»  MVAirom.  985 

Ex.  To  find  the  roots  of  the  equations3  —  6ac*  +10*  =  8. 
First  to  take  away  the  2d  term,  its  co-efficient  being  —  6, 
its  3d  part  is  —  2 ;  put  therefore  x  =  *  +  2 ;  then 

=  z3  +  6s9  +  12z  +  8 
-  6**=  -6*1  —  24*  —  24 
+  10*  =  +  10*  +  20 


theref.  the  sum  z3   #    -  2* +  4  =  8 
or  z3   *    —  2*  =  4 

Here  then  a  =  —  2, 6  =  4,  c  =  —  |,  d  =  2. 

Theref.  V[rf+^(W)]-l/[2+^(4-A)]«l/(2+^  W)^ 

and  Vt^-^+c3)]  ^/[2-v/(4-A)]-l/(2-^  W)» 
3/(2-  yv/3)=0-42265  ^ 

then  the  sum  of  these  two  is  the  value  of  *  =  2.  Hence 
x  =  *  +  2  =  4,  one  root  of  *  in  the  eq.  a3  —  Ox*  +  lOx  =  8. 

To  find  the  two  other  roots,  perform  the  division,  Sec.  as 
in  p.  261,  thus: 

x  _  4 )  x3  —  6xa  +  lOx  —  8  (  Xs  —  2x  +  2  =s  0 
x3  —  4x" 


—  2**+  lOx 

—  2r»  +  8x 


2r  — 8 
2x  — 8 


it  becomes  x3  +  y3  +  3xy  (x+  v)  +a  (x  +  y)  =  6.  Again,  suppose 
3sjf  =  —  a ;  which  substituted,  the  last  equation  becomes  x3  -|-  =  6. 
Now,  from  the  square  of  this  equation  subtract  four  times  the  equation 
xy  =  —  Ja,  and  there  results  x8  —  2xy  +  3^  =  *9  +  aS*3* tbe  square 
root  of  which  is  x3  —  y3  =  V  (6*  +  Afli)-  This  being  added  to  and 
taken  from  the  equation  x3  +  y3  =  6,  gives 

•      C  2xs  =  6  +  V  (6a  +  A  *)  =  6  4-  2  V  [(J6)3  4-  (J*)3!, 
i  2y*  =  6  -  V  (6*  —  aS  «  )  =  *  — 2  V         +  (J*)3] ;  or 

{  S!  =  5S  ±  »  V  [S  J  ^  }  •  Hence'  di*d'"*  *  *  — 
extracting  the  cube  roots,  we  have  x  =  l/d  -f-  v  (d2  -f  c1),  and  y  =s 
%/d  —  V(d2  +  c3)  ;  the  sum  of  these  two  gives  the  first  form  of  the  root 
s  above  stated.  And  that  the  2d  form  is  equal  to  the  first  will  be  evident 
by  reducing  the  two  2d  quantities  to  the  same  denominator. 

When  c  is  negative,  and  c3  greater  than  o*f  the  root  *pp*axiY*w& 
imaginary  form. 

Vox.  I.  35 


906  of  BiKPix  umnunr. 

Hence  x3  —  2*  =  —  2,  or  **  —  2*+  1  «=  —  1,  and  *— 1 
=  rhv'  — 1      =  lor=l  —     —  l,thetwo 

other  roots  sought. 

Ex.  2.  Given  Xs  —  6a*  +  36x  =  44,  to  find  *. 

Ans.  *  =  2*32748. 
Ex.  3.  To  find  the  roots  of  x>  —  7x*  +  14x*=  20. 

Ans.  x  =  5,  or  =  1  +  ^/ —  3,  or  =  1  —  ^/  —  3. 

Ex.  4.  Find  the  three  roots  of  x3  +  6x  =  20. 


OF  SIMPLE  INTEREST. 

As  the  interest  of  any  sum,  for  any  time,  is  directly  pro- 
portional  to  the  principal  sum,  and  to  the  time ;  therefore 
the  interest  of  1  pound,  for  1  year,  being  multiplied  by  any 
given  principal  sum,  and  by  the  time  of  its  forbearance,  in 
years  and  parts,  will  give  its  interest  for  that  time.  That  is, 
if  there  be  put 

r  =  the  rate  of  interest  of  1  pound  per  annum, 
p  =  any  principal  sum  lent, 
t  =  the  time  it  is  lent  for,  and 

a  =  the  amount  or  sum  of  principal  and  interest ;  then 
is  pfi  =  the  interest  of  the  sum  p,  for  the  time  t,  and  conseq. 
p  +  prt  or  p  X  (1  +  rt)  =  dy  the  amount  for  that  time. 

From  this  expression,  other  theorems  can  easily  be  de- 
duced, for  finding  any  of  the  quantities  above  mentioned : 
which  theorems,  collected  together,  will  be  as  follows  : 

1st,  a  =  p  +  prt  the  amount ;  2d,  p  =  ■  J*  ■  the  principal  ; 

3d,  r  =          the  rate  ;  4th,  t  =          the  time. 

pt  pr 

For  Example.  Required  to  find  in  what  time  any  princi- 
pal sum  will  double  itself,  at  any  rate  of  simple  interest. 

In  this  case,  we  must  use  the  first  theorem,  o  =-p  +  prt, 
in  which  the  amount  a  must  be  made  =  2p,  or  double  the 
principal,  that  is,  p  +  prt  =  2p,  or  prt  =  p,  or  rt  =  1 ; 

and  hence  t  =  -. 

r 

Hence  r  being  the  interest  of  11  for  1  year,  it  follows,  that 
the  doubling  at  simple  intern^  ia         to  the  quotient  of 


COMPOUND  INTEREST.  907' 

any  sum  divided  by  its  interest  for  1  year.  •  So,  if  the  rate  of 
interest  be  5  per  cent,  then  100  -s-  5  =  20,  is  the  time  of 
doubling  at  that  rate.    Or  the  4th  theorem  gives  at  once 

#     a—p     2p—p      2-1     1   .  '  r 

t  =          =  — — — =   =     the  same  as  before. 

pr         pr  r  r 


COMPOUND  INTEREST. 

Besides  the  quantities  concerned  in  Simple  Interest, 
namely, 

p  =  the  principal  sum, 

r  =  the  rate  of  interest  of  11  for  1  year, 

a  =  the  whole  amount  of  the  principal  and  interest, 

t  =  the  time* 

there  is  another  quantity  employed  in  Compound  Interest, 
viz.  the  ratio  of  the  rate  of  interest,  which  is  the  amount  of 
II  for  1  time  of  payment,  and  which  here  let  be  denoted  by 
B,  viz. 

K  =  1  +  r,  the  amount  of  11  for  I  time. 

Then  the  particular  amounts  for  the  several  times  may 
be  thus  computed,  viz.  As  II  is  to  its  amount  for  any  time, 
so  is  any  proposed  principal  sum,  to  its  amount  for  the  same 
time ;  that  is,  as 

}l  :  R  :  :  p  :  pa,  the  1st  year's  amount, 
1Z  :  R  :  :  pn  :  pRa,  the  2d  year's  amount, 
11  :  R  :  :  pR2  :  J>R3,  the  3d  year's  amount, 
and  so  on. 

Therefore,  in  general,  pn1  =  a  is  the  amount  for  the 
t  year,  or  t  time  of  payment.  Whence  the  following  genera! 
theorems  are  deduced  : 

1st,  a  =  j>r«  the  amount ;  2d,  p  =  ~  the  principal ; 

Jd,K  =  y-theratio;  4tM  =  ^0^4°---^^ 
'       v  p  loe.  of  r  *  -  ■ 


OOXPOTCTD 

From  which,  any  one  of  the  quantities  may  bo  found, 
when  die  rest  are  given. 

As  to  the  whole  interest,  it  is  found  by  barely  subtracting 
die  principal/)  from  the  amount  a. 

Example.  Suppose  it  be  required  to  find,  in  how  many 
years  any  principal  sum  will  double  itself,  at  any  proposed 
rate  of  compound  interest. 

In  this  case  the  4th  theorem  must  be  employed,  making 
m  a*  2p ;  and  then  it  is 

I  log*  a~log.jp     log,  2p — log.  p  _  log.  2 

leg.  n  log.  n  log.  r" 

So,  if  the  rate  of  interest  be  5  per  cent  per  annum ;  then 
B  =  1  +  -06  -»  1*05  ;  and  henee 


log.  2  '301030 
log.  1-05  *  -021189 


14-2067  nearly  ; 


that  is,  any  sum  doubles  itself  in  14£  years  nearly,  at  the 
rate  of  5  per  cent,  per  annum  compound  interest. 

Hence,  and  from  the  like  question  in  simple  interest,  above 
given,  are  deduced  the  times  in  which  any  sum  doubles  itself, 
at  several  rates  of  interest,  both  simple  and  compound  ;  viz. 


At" 
3 

f 

4 

4* 

5 

6 

7 

8 

9 

10  J 

per  cent. -per  annum 
interest,  1/.  or  any 

other  sum,  will 
double  itself  in  the 

following  years. 

AtSimp.Int. 

At  Comp.Int 

in  50 
40 
33i 
28| 
25 

22J  Kj 
20  2 
16|  ? 
14| 
12* 

Hi 

I  10 

in  35  0028 
28-0701 
23-4498 
201488 
17-6730 
15-7473  h- 
14-2067 1 
11-8957? 
10-2448 
9  0065 
8  0432 
7-2725 

The  following  Table  will  very  much  facilitate  calculations 
of  compound  interest  on  any  sum,  for  any  number  of  years, 
at  various  rates  of  interest. 


cokpouhd  iivtibxst.  968 
The  Amounts  of  12  in  any  Number  of  Tears. 


Yrs. 

3 

3} 

4 

5 

6 

1 

1*0300 

1-0350 

1-0400 

1-0450 

1-0500 

1-0600 

2 

1-0609 

10712 

1-0816 

1-0920 

1-1025 

11236 

3 

1-0927 

11087 

1-1249 

11412 

1-1576 

11910 

4 

1-1255 

1-1475 

1-1699 

1-1925 

1-2155 

1-2625 

* 

1-1593 

1-1877 

1-2167 

1-2462 

1-2763 

1-3382 

6 

1-1948 

1-2293 

1-2653 

1-3023 

1-3401 

1-4185 

7 

1-2299 

1-2723 

1-3159 

1-3609 

1-4071 

1-5036 

8 

1-2668 

1-3168 

1-3686 

1«4221 

1-4775 

1-5939 

9 

1-3048 

1-3629 

1-4233 

1-4861 

1-5513 

1-6895 

10 

1-3439 

1-4106 

1-4802 

1-5530 

1-6289 

1-7909 

11 

1-3842 

1-4600 

1-5895 

1-6229 

1-7103 

1-8983 

12 

1-4258 

1-5111 

1-6010 

1-6959 

1.7959 

2-0122 

13 

1-4685 

1-5640 

1-6651 

1-7722 

1-8856 

21329 

14 

1-5126 

1-6187 

1-7317 

1-8519 

1-9799 

2-2609 

15 

1-5580 

1-6753 

1-8009 

1-9353 

20789 

2-3966 

16 

1-6047 

1-7340 

1-8730 

2  0224 

21829 

2-5404 

17 

1-6528 

1-7947 

1-9479 

21134 

2-2920 

2-6928 

18 

1-7024 

1-8575 

2  0258 

2-2085 

2-4066 

2-8543 

19 

1-7535 

1-9225 

2-1068 

2-3079 

2-5270 

30256 

20 

1-8061 

1-9828 

21911 

2-4117 

2-6533 

3-2071 

The  use  of  this  Table,  which  contains  all  the  powers,  r', 
to  the  20th  power,  or  the  amounts  of  1Z,  is  chiefly  to  calcu- 
late the  interest,  or  the  amount  of  any  principal  sum,  for  any 
time,  not  more  than  20  years. 

For  example,  let  it  be  required  to  find,  to  how  much  5231 
will  amount  in  15  years,  at  the  rate  of  5  per  cent,  per  annum 
compound  interest. 

In  the  table,  on  the  line  15,  and  in  the  column  5  per  cent 
is  the  amount  of  1/,  viz.         .       -    2  0789 
this  multiplied  by  the  principal       -  523 

gives  the  amount         -      -  1087-2647 
or        ....  1087Z5*3J<*. 
and  therefore  the  interest         564Z  5*  3\d. 

Note  1.  When  the  rate  of  interest  is  to  be  determined  to 
any  other  time  than  a  year  ;  as  suppose  to  £  a  year,  or  J  a 
year,  dec. :  the  rules  are  still  the  same  ;  but  then  t  will  ex- 
press that  time,  and  k  must  be  taken  the  amount  foe  tihsX 
time  also. 


270 


ANNUITIES. 


Nole  2,  When  the  compound  interest,  or  amount,  of  any 
sum,  is  required  for  the  parts  of  a  year ;  it  may  be  determin- 
ed in  the  following  manner : 

1st,  For  any  time  which  is  some  aliquot  part  of  a  year : — 
Find  the  amount  of  11  for  1  year,  as  before  ;  then  that  root 
of  it  which  is  denoted  by  the  aliquot  part,  will  be  the  amount 
of  11.  This  amount  being  multiplied  by  the  principal  sum, 
will  produce  the  amount  of  the  given  sum  as  required. 

2d,  When  the  time  is  not  an  aliquot  part  of  a  year : — 
Reduce  the  time  into  days,  and  take  the  365th  root  of  the 
amount  of  11  for  1  year,  which  will  give  the  amount  of  the 
same  for  1  day.  Then  raise  this  amount  to  that  power  whose 
index  is  equal  to  the  number  of  days,  and  it  will  be  the 
amount  for  that  time.  Which  amount  being  multiplied  by 
the  principal  sum,  will  produce  the  amount  of  that  sum  as 
before. — And  in  these  calculations,  the  operation  by  loga- 
rithms will  be  very  useful. 


OF  ANNUITIES. 


Annuity  is  a  term  used  for  any  periodical  income,  arising 
from  money  lent,  or  from  houses,  lands,  salaries,  pensions, 
&c.  payable  from  time  to  time,  but  mostly  by  annual  pay- 
ments. 

Annuities  are  divided  into  those  that  are  in  Possession, 
and  those  in  Reversion :  the  former  meaning  such  as  have 
commenced  ;  and  the  latter  such  as  will  not  begin  till  some 
particular  event  has  happened,  or  till  after  some  certain  time 
has  elapsed. 

When  an  annuity  is  forborn  for  some  years,  or  the  pay- 
ments not  made  for  that  time,  the  annuity  is  said  to  be  in 
Arrears. 

An  annuity  may  also  be  for  a  certain  number  of  years ; 
or  it  may  be  without  any  limit,  and  then  it  is  called  a  Per- 
petuity. 

The  Amount  of  an  annuity,  forborn  for  any  number  of 
years,  is  the  sum  arising  from  the  addition  of  all  the  annui- 
ties for  that  number  of  years,  together  with  the  interest  due 
upon  each  after  it  becomes  due. 


ANNUITIES.  271 

The  Present  Worth  or  Value  of  an  annuity,  is  the  price 
or  sum  which  ought  to  be  given  for  it,  supposing  it  to  be 
bought  off,  or  paid  all  at  once. 

Let  a  =  the  annuity,  pension,  or  yearly  rent ; 
n  =  the  number  of  years  forborn,  or  lent  for ; 
R  =  the  amount  of  11  for  1  year  ; 
m  =s  the  amount  of  the  annuity  ; 
v  =  its  value,  or  its  present  worth. 

Now,  1  being  the  present  value  of  the  sum  b,  by  propor- 
tion  the  present  value  of  any  other  sum  a,  is  thus  found : 

as  r  :  1  : :  a  :  ~  the  present  value  of  a  due  1  year  hence. 
In  like  manner  ~  is  the  present  value  of  a  due  2  years 
hence  ;  for  r  :  1  : :  -  :         So  also  ~,  — ,  —,  &c.  will 

R      Ra  R3    R*  R4 

be  the  present  values  of  a,  due  at  the  end  of  3,  4,  5,  &c. 
years  respectively.    Consequently  the  sum  of  all  these,  or 

aiaiaiaic         ,1.1.1.1.    X  ^ 

a  continued  to  n  terms,  will  be  the  present  value  of  all  the  n 
years'  annuities.  And  the  value  of  the  perpetuity,  is  the  sum 
of  the  series  to  infinity. 

But  this  series,  it  is  evident,  is  a  geometrical  progression, 

having  ~  but  for  its  first  term  and  common  ratio,  and  the 

number  of  its  terms  n  ;  therefore  the  sum  v  of  all  the  terms, 
or  the  present  value  of  all  the  annual  payments,  will  be 

„  =  *     *     R"  X  a,  or  —  J*—^-^-  X 

^       1  R        1  Rn 

R 

When  the  annuity  is  a  perpetuity ;  n  being  infinite,  r* 
is  also  infinite,  and  therefore  the  quantity  ~  becomes  =  0, 

therefore  — ^-j-  X  ~  also  =  0 ;  consequently  the  expression 

becomes  barely  v  =  — — _  ;  that  is,  any  annuity  divided  by 

R  "™ ■ ~  •* 

the  interest  of  11  for  1  year,  gives  the  value  of  tto  \*%T^etoai- 
ty.    So,  if  the  rate  of  Interest  be  5  per  cent. 


372  ANNUITIES. 

Then  100a  -f-  5  =  20a  is  the  value  of  the  perpetuity  at 
5  per  cent :  Also  100a  -f-  4  =  25a  is  the  value  of  the  per- 
petuity  at  4  per  cent. :  And  100a  -r-  3  =  33£a  is  the  value 
of  the  perpetuity  at  3  per  cent. :  and  so  on. 

Again,  because  the  amount  of  11  in  n  years,  is  Rn,  its 
increase  in  that  time  will  be  Rn  —  1 ;  but  its  interest  for  one 
single  year,  or  the  annuity  answering  to  that  increase,  is 
r  —  1 ;  therefore,  as  r  —  1  is  to  ra  —  1,  so  is  a  to  m  ;  that 
nn  —  1 

is,  m  =   —  X  a.    Hence,  the  several  cases  relating  to 

r  —  1 

Annuities  in  Arrear,  will  be  resolved  by  the  following 
equations : 


m  = 


v  = 


n  = 


Rn— 1 
R— 1 

X  a  = 

CR«  ; 

R»  —  1 

X-  = 

m 

R— 1 

X  R" 

?? 

R  — 1 
Rn    1 

X  m  = 

R—  1 
Rn—  1 

log.  m  - 

-log.  V 

'log. 

a  =  —  ^  X  m  =  — — ^  x  vr*  ; 

77iR  —  m  +  a 


log.  R  log.  R 

Log   &  —  *0^*  m — v 


Rp        Rn'       R  1 

In  this  last  theorem,  r  denotes  the  present  value  of  an 
annuity  in  reversion,  after  p  years,  or  not  commencing  till 
after  the  first  p  years,  being  found  by  taking  the  difference 

between  the  two  values  ——4  X  —  and  =  — ,  for  n 

R—  1        Rn         R—  1  RP 

years  and  p  years. 

But  the  amount  and  present  value  of  any  annuity  for  any 
number  of  years,  up  to  21,  will  be  most  readily  found  by  the 
two  following  tables. 


ANNUITIES. 


273 


TABLE  I. 

The  Amount  of  an  Annuity  of  1/  at  Compound  Interest. 


YrB. 

at  3  per  c. 

31  perc. 

4  per  c. 

4  J  perc. 

5  per  c. 

6  per  c. 

1 

10000 

10000 

1  0000 

1  0000 

10000 

10000 

2 

20300 

2  0350 

20400 

2  0450 

20500 

20600 

3 

3  0909 

3*1062 

3*1216 

3- 1370 

3  1525 

31836 

4 

41836 

4-2149 

42465 

42782 

43101 

43746 

5 

5  3091 

53625 

5  4163 

5-4707 

55256 

56371 

6 

64684 

65502 

66330 

67169 

68019 

69753 

7 

76625 

77794 

78983 

80192 

8  1420 

83938 

8 

88923 

90517 

92142 

9  3800 

95491 

98975 

9 

10  1591 

103685 

10-5828 

10-8021 

110266 

11  4913 

10 

114639 

117314 

120061 

122882 

12  5779 

131808 

11 

12-8078 

131420 

13  4864 

138412 

14-2068 

149716 

12 

14  1920 

146020 

150258 

15-4640 

159171 

16-8699 

13 

156178 

16  1130 

16  6268 

171599 

17-7130 

18*8821 

14 

170863 

17  6770 

182919 

189321 

19  5986 

21  0151 

15 

18-5989 

19  2957 

203236 

20  7841 

21  5786 

232760 

16 

20  1569 

209710 

21  8245 

22  7193 

236575 

25-6725 

17 

21  7616 

22-7050 

236975 

24-7417i  25  8404 

282129 

IS 

234144 

244997 

25  6454 

268551 

28  1324 

309057 

19 

25  1169 

26  3572 

276712 

290636 

305390 

3376C0 

20 

268704 

282797 

29*7781 

31  3714 

33  0660 

367856 

21 

286765 

302695 

31  9692 

33  7831 

35  7193 

399927 

table  ii.    The  Present  Value  of  un  Annuit}'  of  1/. 


Yrs. 

at  3  perc. 

3£  per  c. 

4  per  c. 

1 

09709 

09662 

09615 

2 

1  9135 

1-8997 

1*8861 

3 

28286 

2*8016 

27751 

4 

37171 

36731 

36299 

5 

4-5797 

4*5151 

44518 

6 

5-4172 

5*3286 

52421 

7 

62303 

61145 

60020 

8 

70197 

6*8740 

77327 

9 

77861 

7-6077 

74353 

10 

8*5302 

8*3166 

8  1109 

11 

9-5256 

90016 

8-7605 

12 

9-9540 

96633 

93851 

13 

10-6350 

10  3027 

9-9857 

14 

11  2961 

10*9205 

105631 

15 

11  9379 

11  5174 

11  1181! 

16 

12  5611!  120941 

11-65231 

17 

131661 

126513 

12  1657 

18 

13-7535 

13  1S97 

12-659?! 

19 

143238 

13*7098 

13  1339 

20 

148775 

142124 

135903 

21 

154150/ 

14  69801 

14  0292 

4}  por  c.  I  5  per  c. 


09569 
1  8727 
27490 
3*5875 

4-  3^C0 
51579 

5-  8927 
65959 
7-2688i 
7*9127| 
8*5289' 
91 186! 
9*6S29| 

10  2228: 
10-7396| 

11  2340. 

11  7072: 

12  16001 
1259331 

13  0079 
13  4047' 


09524 
1-8594 
27233 
35460 
4  :)23b 
50757 
57864 
64632 
7*  1078 
7  7217 
83G54 
88633 
9-3S3S 
989S6 
10-3797 


6  per  c. 


0  95.  4 

2  (>7oC 
34651 
42124 
49173 
55824 
62095- 
68017 
73601 
78869 
8-3838 
88527 
92950 
971*3 
10  8378:  10  1069 


11-2741 
11  6S96 
120853 


10-4773 
10*8276 
11  158V 


Vol.  I. 


36 


274 


ANNUITIES. 


To  find  the  Amount  of  any  Annuity  forlorn  a  certain  number 
of  years. 

Take  out  the  amount  of  12  from  the  first  table,  for  the 
proposed  rate  and  time ;  then  multiply  it  by  the  given 
annuity  ;  and  the  product  will  be  the  amount,  for  the  same 
number  of  years,  and  rate  of  interest.  And  the  converse  to 
find  the  rate  of  time. 

Exam.  To  find  how  much  an  annuity  of  507  will  amount 
to  in  20  years,  at  3£  per  cent,  compound  interest. 

On  the  line  of  20  years,  and  in  the  column  of  3 J  per  cent, 
stands  28*2797,  which  is  the  amount  of  an  annuity  of  12  for 
the  20  years.  Then  28-2797  X  50,  gives  1413-9851  = 
1413/  19*  8d  for  the  answer  required. 

To  find  the  Present  Value  of  any  Annuity  for  any  number 
of  years. — Proceed  here  by  the  2d  table,  in  the  same  manner 
us  above  for  the  1st  table,  and  the  present  worth  required 
will  be  found. 

Exam.  1.  To  find  the  present  value  of  an  annuity  of  502, 
which  is  to  continue  20  years,  at  3J  per  cent. — By  the  table, 
the  present  value  of  11  for  the  given  rate  and  time,  is 
14-2124;  therefore  14-2124  X  50  =  710-022  or  7102  12*  4d 
is  the  present  value  required. 

Exam  2.  To  find  the  present  value  of  an  annuity  of  202, 
to  commence  10  years  hence,  and  then  to  continue  for  11 
years  longer,  or  to  terminate  21  years  hence,  at  4  per  cent, 
interest. — In  such  cases  as  this,  we  have  to  find  the  difference 
between  the  present  values  of  two  equal  annuities,  for  the 
two  given  times ;  which  therefore  will  be  done  by  subtracting 
the  tabular  value  of  the  one  period  from  that  of  the  other, 
and  then  multiplying  by  the  given  annuity.  Thus, 
tabular  value  for  21  years  14*0292 
ditto  for  10  years  8*1109 


the  difference  5-9183 
multiplied  by  20 


gives     -  118*3602 
or     -     -     1 1 8Z  7*  3 £c2  the  answer. 


END  OF  THE  ALGEBRA. 


275 


GEOMETRY, 


DEFINITIONS. 

1.  A  Point  is  that  which  has  position,  bat 
no  magnitude,  nor  dimensions ;  neither  length, 
breadth,  nor  thickness. 

2.  A  Line  is  length,  without  breadth  or 
thickness. 

S.  A  Surface  or  Superficies,  is  an  extension 
or  a  figure  of  two  dimensions,  length  and 
breadth ;  but  without  thickness. 

4.  A  Body  or  Solid,  is  a  figure  of  three  di- 
mensions, namely,  length,  breadth,  and  depth, 
or  thickness. 

5.  Lines  are  either  Right,  or  Curved,  or 
Mixed  of  these  two. 

6.  A  Right  Line,  or  Straight  Line,  lies  all  iu 
the  same  direction,  between  its  extremities ; 
and  is  the  shortest  distance  between  two  points. 

When  a  Line  is  mentioned  simply,  it  means 
a  Right  Line. 

7.  A  Curve  continually  changes  its  direction 
between  its  extreme  points. 

8.  Lines  are  either  Parallel,  Oblique,  Per- 
pendicular,  or  Tangential. 

.  9.  Parallel  Lines  are  always  at  the  same 
perpendicular  distance ;  and  they  never  meet, 
though  ever  so  far  produced. 

10.  Oblique  lines  change  their  distance,  and 
would  meet,  if  produced  on  the  side  of  the  least 
distance. 

11.  One  line  is  Perpendicular  to  another, 
when  it  inclines  not  more  on  the  one  side 


276 


GEOMETRY. 


than  the  other,  or  when  the  angles  on  both 
sides  of  it  are  equal. 

12.  A  line  or  circle  is  Tangential,  or  is  a 
Tangent  to  a  circle,  or  other  curve,  when  it 
touches  it,  without  cutting,  when  bath  are 
produced. 

13.  An  Angle  is  the  inclination  or  open- 
ing of  two  lines,  having  different  directions, 
and  meeting  in  a  point. 

14.  Angles  are  Right  or  Oblique,  Acute 
or  Obtuse. 

15.  A  Right  Angle  is  that  which  is  made 
by  one  line  perpendicular  to  another.  Or 
when  the  angles  on  each  side  are  equal  to 
one  another,  they  are  right  angles. 

16.  An  Oblique  Angle  is  that  which  is 
made  by  two  oblique  lines ;  and  is  either  less 
or  greater  than  a  right  angle. 

17.  An  Acute  Angle  is  less  than  a  right 
angle. 

18.  An  Obtuse  Anglo  is  greater  than  a 
right  angle. 

19.  Superfices  are  either  Plane  or  Curved. 

20.  A  Plane  Superficies,  or  a  Plane,  is  that  with  which 
a  right  line  may,  every  way,  coincide.  Or,  if  the  line  touch 
the  plane  in  two  points,  it  will  touch  it  in  every  point.  But, 
if  not,  it  is  curved. 

21.  Plane  Figures  are  bounded  either  by  right  lines  or 
curves. 

22.  Plane  figures  that  are  bounded  by  right  lines  have 
names  according  to  the  number  of  their  sides,  or  of  their 
angles ;  for  they  have  as  many  sides  as  angles ;  the  least 
number  being  three. 

83.  A  figure  of  three  sides  and  angles  is  called  a  Triangle. 
And  it  receives  particular  denominations  from  the  relations 
of  its  sides  and  angles. 

24.  An  Equilateral  Triangle  is  that  whose 
three  sides  are  all  equal. 

' 

25.  An  Isosceles  Triangle  is  that  which  has 
two  sides  equal. 


DEFINITIONS. 


277 


26.  A  Scalene  Triangle  is  that  whose  three 
sides  are  all  unequal. 

27.  A  Right-angled  Triangle  is  that  which 
has  one  right  angle.  ^ 

28.  Other  triangles  are  Oblique-angled,  and 
are  either  obtuse  or  acute. 

20.  An  Obtuse-angled  Triangle  has  one  ob- 
tuse angle. 

30.  An  Acute-angled  Triangle  has  all  its 
three  angles  acute. 

31.  A  figure  of  Four  sides  and  angles  is  call- 
ed a  Quadrangfe,  or  a  Quadrilateral. 

32.  A  Parallelogram  is  a  quadrilateral  which 
has  both  its  pairs  of  opposite  sides  parallel. 
And  it  takes  the  following  particular  names, 
viz.  Rectangle,  Square,  Rhombus,  Rhomboid. 

33.  A  Rectangle  is  a  parallelogram,  having 
a  right  angle. 

34.  A  Square  is  an  equilateral  rectangle ; 
having  its  length  and  breadth  equal. 

35.  A  Rhomboid  is  an  oblique-angled  paral- 
lelogram. 

36.  A  Rhombus  is  an  equilateral  rhomboid  ; 
having  all  its  sides  equal,  but  its  angles  ob- 
lique. 

37.  A  Trapezium  is  a  quadrilateral  which 
hath  not  its  opposite  sides  parallel. 

88.  A  Trapezoid  has  only  one  pair  of  oppo- 
site sides  parallel. 

39.  A  Diagonal  is  a  line  joining  any  two  op* 
poaite  angles  of  a  quadrilateral. 


□ 

/J 

40.  Plane  figures  that  have  more  than  four  sides  are,  in 
general,  called  Polygons  :  and  they  receive  other  particular 
names,  according  to  the  number  of  their  sides  or  angles. 
Thus, 

41.  A  Pentagon  is  a  polygon  of  five  sides ;  a  Hexagon,  of 
six  sides;  a  Heptagon,  seven;  an  Octagon,  eight;  %ttocu 
agon,  nine ;  a  Decagon,  ten ;  an  Undecagon,  tawa  \ 
vodeoagon,  twelve  sides. 


278 


GEOMETRY. 


42.  A  Regular  Polygon  has  all  its  sides  and  all  its  angles 
equal. — If  they  are  not  both  equal,  the  polygon  is  Irregular. 

43.  An  Equilateral  Triangle  is  also  a  Regular  Figure  of 
three  sides,  and  the  Square  is  one  of  four  :  the  former  being 
also  called  a  Trigon,  and  the  latter  ^tetragon. 

44.  Any  figure  is  equilateral,  when  all  its  sides  are  equal : 
and  it  is  equiangular  when  all  its  angles  arc  equal.  When 
both  these  arc  equal,  it  is  a  regular  figure. 

45.  A  Circle  is  a  plane  figure  bounded  by 
a  curve  line,  called  the  Circumference,  which 
is  every  whore  equidistant  from  a  certain  point 
within,  called  its  Centre. 

The  circumference  itself  is  often  called  a 
circle,  and  also  the  Periphery. 

46.  The  Radius  of  a  circle  is  a  line  drawn 
from  the  centre  to  the  circumference. 

47.  The  Diameter  of  a  cirle  is  a  line  drawn 
through  the  centre,  and  terminating  at  the 
cireumfcrencc  on  both  sides. 


48.  An  Arc  of  a  circle  is  any  part  of  the 
circumference. 


49.  A  Chord  is  a  right  line  joining  the  ex. 
tremitics  of  an  arc. 


50.  A  Segment  is  any  part  of  a  circle 
bounded  by  an  arc  and  its  chord. 

51.  A  Semicircle  is  half  the  circle,  or  a 
segment  cut  off  by  a  diameter. 

The  half  circumference  is  sometimes  called 
the  Semicircle. 

52.  A  Sector  is  any  part  of  a  circle  which 
is  bounded  by  an  arc,  and  two  radii  drawn  to 
its  extremities. 

•  53.  A  Quadrant,  or  Quarter  of  a  circle  is 
a  sector  having  a  quarter  of  the  circumference 
for  its  arc,  and  its  two  radii  are  perpendicular 
to  each  other.  A  quarter  of  the  circumference 
is  sometimes  called  a  Quadrant. 


DEFINITIONS. 


279 


B    A  d 


54.  Tho  Height  or  Altitude  of  a  figure  is 
a  perpendicular  let  fall  from  an  angle,  or  its 
vertex,  to  the  opposite  side,  called  the  base. 

55.  In  a  right-angled  triangle,  the  side  op- 
posite the  right  angle  ailed  the  Hypothc- 
nuse ;  and  the  other  two  sides  are  called  the 
Legs,  and  sometimes  the  Base  and  Perpen- 
dicular. 

56.  When  an  angle  is  denoted  by  three 
letters,  of  which  one  stands  at  the  angular 
point,  and  the  other  two  on  the  two  sides, 
that  which  stands  at  the  angular  point  is  read 
in  the  middle. 

57.  The  circumference  of  every  circle  is 
supposed  to  be  divided  into  360  equal  parts 
called  degrees ;  and  each  degree  into  60  Mi- 
nutes, each  Minute  into  60  Seconds,  and  so 
on.  Hence  a  semicircle  contains  160  degrees, 
and  a  quadrant  90  degrees. 

58.  The  Measure  of  an  angle,  is  an  arc  of 
any  circle  contained  between  the  two  lines 
which  form  that  angle,  the  angular  point 
being  the  centre  ;  and  it  is  estimated  by  the 
number  of  degrees  contained  in  that  arc. 

59.  Lines,  or  chords,  are  said  lo  be  Equi- 
distant from  the  centre  of  a  circle,  when  per- 
pendiculars drawn  Lo  them  from  the  centre 
are  equal. 

69.  And  the  right  line  on  which  the  Great- 
er Perpendicular  falls,  is  said  to  be  farther 
from  the  centre. 

61.  An  Angle  In  a  Segment  is  that  which 
is  contained  by  two  lines,  drawn  from  any 
point  in  the  arc  of  the  segment,  to  the  two 
extremities  of  that  arc. 

62.  An  Angle  On  a  segment,  or  an  are,  is  that  which  is 
contained  by  two  lines,  drawn  from  anv  point  in  the  opposite 
or  supplemental  part  of  the  circumference,  to  tho  extremities 
of  the  arc,  and  containing  the  arc  between  (hem. 

63.  An  Angle  at  the  circumference,  is  that  S^/V^ 
whose  angular  point  or  summit  is  any  where        (  f\ 
in  the  circumference.    And  an  angle  at  the        '  /  ^  v 
centre,  is  that  whose  angular  point  is  at  the 
centre. 


280 


GEOMETRY. 


64.  A  right-lined  figure  is  Inscribed  in  a 
circle,  or  the  circle  Circumscribes  it,  when 
all  the  angular  points  of  the  figure  are  in  the 
circumference  of  the  circle. 

65.  A  right-lined  figure  Circumscribes  a 
circle,  or  the  circle  is  Inscribed  in  it,  when  all 
the  sides  of  the  figure  touch  the  circumference 
of  the  circle. 

66*  One  right-lined  figure  is  Inscribed  in 
another,  or  the  latter  circumscribes  the  former, 
when  all  the  angular  points  of  the  former  are 
placed  in  the  sides  of  the  latter. 


67.  A  Secant  is  a  line  that  cuts  a  circle, 
lying  partly  within,  and  partly  without  it. 

66.  Two  triangles,  or  other  right-lined  figures,  are  said  to 
be  mutually  equilateral,  when  all  the  sides  of  the  one  are 
equal  to  the  corresponding  sides  of  the  other,  each  to  each  ; 
and  they  are  said  to  be  mutually  equiangular,  when  the 
angles  of  the  one  are  respectively  equal  to  those  of  the  other. 

68.  Identical  figures  are  such  as  are  both  mutually  equi- 
lateral and  equiangular  ;  or  that  have  all  the  sides  and  all  the 
angles  of  tho  one,  respectively  equal  to  all  the  sides  and  all 
the  angles  of  the  other,  each  to  each  ;  so  that  if  the  one  figure 
were  applied  to,  or  laid  upon  the  other,  all  the  sides  of  the  one 
would  exactly  fall  upon  and  cover  all  the  sides  of  the  other  ; 
the  two  becoming  as  it  were  but  one  and  the  same  figure. 

70.  Similar  figures,  are  those  that  have  all  the  angles  of 
the  one  equal  to  all  the  angles  of  the  other,  each  to  each,  and 
the  sides  about  the  equal  angles  proportional. 

71.  The  Perimeter  of  a  figure,  is  the  sum  of  all  its  sides 
taken  together. 

72.  A  Proposition,  is  something  which  is  either  proposed 
to  be  done,  or  to  be  demonstrated,  and  is  either  a  problem  or 
a  theorem. 

73.  A  Problem,  is  something  proposed  to  be  done. 

74.  A  Theorem,  is  something  proposed  to  be  demonstrated. 

75.  A  Lemma,  is  something  which  is  premised,  or  demon- 
trated,  in  order  to  render  what  follows  more  easy. 

76.  A  Corollary,  is  a  consequent  truth,  gained  immediate- 
ly from  some  preceding  truth,  or  demonstration. 

77.  A  Scholium,  is  a  remark  or  observation  made  upon 
something  going  before  it. 


281 


,  AXIOMS. 

1.  Things  which  are  equal  to  the  aame  thing  arc  equal  to 
each  other. 

2.  When  equals  are  added  to  equals,  the  wholes  are 
equal. 

3.  When  equals  are  taken  from  equals,  the  remainders 
are  equal. 

4.  When  equals  are  added  to  uncquals,  the  wholes  are  un- 
equal. 

5.  When  equals  are  taken  from  unequal*,  the  remainders 
are  unequal, 

6.  Things  which  are  double  of  the  same  thing,  or  equal 
things,  are  equal  to  each  other.  ^ 

7.  Things  which  are  halves  of  the  same  thing,  are  equal. 
.  .8.  Every  whole  is  equal  to  all  its  parts  taken  together. 

0.  Things  which  coincide,  or  fill  the  same  space,  are  iden- 
tical, or  mutually  equal  in  all  their  parts. 

20.  All  right  angles  are  equal  to  ono  another. 

21.  Angles  that  have  equal  measures,  or  arcs,  are  equal. 


TIIEOREX  T. 


in 
all 


If  two  triangles  have  two  sides  and  the  included  angle 
in  the  one,  equal  to  two  sides  and  the  included  angle 
the  other,  the  triangles  will  be  identical,  or  equal  in 
respects. 

In  the  two  triangles  jlbc,  def,  if 
the  side  ac  be  equal  to  the  side  dp, 
and  the  side  bc  equal  to  the  side  ef, 
and  the  angle  c  equal  to  the  angle  f  ; 
then  will  the  two  triangles  be  identical, 
or  equal  in  all  respects.  ^ 

For  conceive  the  triangle  abc  to  be  applied  to,  ot  ^Yas&& 
on,  the  triangle  def,  in  such  a  manner  that  the  pov&l  c  m*$ 

Vol  1  37 


\ 


482  •EOXETftT. 

coincide  with  the  point  r,  and  the  side  ac  with  the  side  sv9 
which  is  equal  to  it. 

Then,  since  the  angle  f  is  oqunl  to  the  angle  c  (by  hyp.), 
the  side  bc  w«ill  fall  on  the  side  r.r.  Also,  because  ac  is 
equal  to  or,  and  nc  equal  to  kf  (by  hypO,  the  point  a  will 
co»»cido  witn  the  point  i>,  and  ihe  jx  inr  a  with  the  point  k  ; 
consequently  the  side  An  will  coincide  with  the  side  dk. 
Therefore  the  two  triangles  are  ilt-nlical,  and  have  all  their 
other  corresponding  parts  equal  (ax.  ?)),  namely,  the  side  ab 
equal  to  the  side  de,  the  angle  a  to  the  angle  d,  and  the  angle 
b  to  the  angle  e.    q.  e.  d. 

THEOREM  II. 

When  two  triangles  have  two  angles  and  the  included 
side  in  the  one,  equal  to  two  angles  and  the  included  side  in 
the  other,  the  triangles  are  identical,  or  have  their  other  sides 
and  angle  equal. 

Let  the  two  triangles  abc,  def,  q  -g 

have  the  angle^i  equal  to  the  anglo 

D,  the  angle  b  equal  to  tL-  1 — 

and  the  side  ab  equal  to  1 
then  these  two  triangles  1 
tical. 

For,  conceive  the  triangle  abc  to  be  placed  on  the  triangle 
def,  in  such  manner  that  the  side  ab  muy  lull  exactly  on  the 
equal  side  dk.  Then,  since  the  angle  a  is  equal  to  the  angle 
i>  (by  hyp.)}  the  side  ac  must  fall  on  the  side  df  ;  and,  in 
like  manner,  because  the  angle  h  is  equal  to  the  angle  >:,  the 
side  bc  must  fall  on  the  side  kf.  Thus  the  three  sides  of  the 
triangle  a»c  will  be  exactly  placed  on  the, three  sides  of  the 
triangle  dkf  :  consequently  the  two  triangles  are  identical 
(ax.  9),  having  the  other  two  sides  ac,  bu,  equal  to  the  two 
df,  rf,  and  the  remaining  angle  c  equal  to  the  remaining 
angle  f.    q.  e.  d. 

theorem  III. 

In  an  isosceles  triangle,  the  angles  at  the  base  are  equal. . 
Or,  if  a  triangle  have  two  sides  equal,  their  opposite  angles 
will  also  bc  equal. 

If  the  triangle  abc  have  the  side  ac  equal 
to  the  side  bc  :  then  will  the  angle  b  be  equal 
to  the  angle  a. 

For,  conceive  the  angle  c  to  be  bisected, 
or  divided  into  two  equal  parts,  by  the  line 
cd,  making  the  angle  acd  equal  to  the  angle  — jj- 

BCD. 


I  to  the  anglo  A 

the  angle  e,  /  I 

>  the  side  df.  ;  /  I 

\  will  be  iden-     *   t, 


THEOREM. 


Then,  the  two  triangles,  acd,  bci>,  have  two  sides  and 
the  contained  angle  of  tho  one,  equal  to  two  sides  and  the 
contained  angle  of  tho  other,  viz.  the  side  ac  equal  to  Br, 
the  angle  acd  equal  to  bcd,  and  the  side  cd  common  ;  there- 
fore these  two  triangles  arc  identical,  or  equal  in  all  respocts 
(th.  1)  ;  and  consequently  tho  angle  a  equal  to  the  angle  b. 
q.  E.  1). 

Carol.  1.  Hence  the  lino  which  hisects  the  vertical  angle 
of  an  isosceles  triangle,  bisects  the  base,  and  is  also  perpen- 
dicular to  it. 

Carol .  2.  Hence  too  it  appears,  that  every  equilateral  tri- 
angle, is  also  equiangular,  or  has  all  its  angles  equal. 


THEOREM  IT, 

When  a  triangle  has  two  of  its  angles  equal,  the  sides 
opposite  to  them  are  also  equal. 


If  the  triangle  abc,  have  the  angle  cab 
equal  to  the  angle  cba,  it  will  also  have  the 
side  ca  equal  to  the  side  ch. 

For,  if  ca  and  cb  he  not  equal,  let  ca  be 
the  greater  of  tho  two,  and  let  da  be  equal 


t3  en,  and  join  db.  Then,  because  da,  ab, 
arc  equal  to  cb,  ba,  each  to  each,  and  the  angle  dab  to 
cba  (hyp.),  the  triangles  dab,  cba,  are  equal  in  all  respects 
(th.  1),  a  part  to  the  whole,  which  is  absurJ  ;  therefore 
ca  is  not  greater  than  cb.  fn  the  same  way  it  may  be 
proved,  that  cb  is  not  greater  than  ca.  They  are  therefore 
equal.       f.  d. 

Cord.  Hence  every  equiangular  triangle  is  also  cquu 
lateral. 

THEOREM  V. 

Whex  two  triangles  have  all  the  three  sides  in  the  one, 
equal  to  all  the  three  sides  in  the  other,  the  triangles  are 
identical,  or  have  also  their  three  triangles  equal,  each  to  each* 

Let  the  two  triangles  abc,  abd, 
have  their  three  sides  respectively, 
equal,  viz.  the  side  ab  equal  to  ab, 
ac  to  ad,  and  nc  to  bd  ;  then  shall 
the  two  triangles  be  identical,  or  have 
their  angles  equal,  viz.  those  anglos 


•K0ML1KV. 


that  are  opposite  to  the  equal  sides  ;  g 

namely,  the  angle  bac  to  the  angle 

bad,  the  angle  abc  to  the  angle  abd, 

and  the  angle  c  to  the  angle  d.  A 
For,  conceive  the  two  triangles  to 

be  joined  together  by  their  longest  j) 

equal  sides,  and  draw  the  line  cd. 

Then,  in  the  triangle  acd,  because  the  side  ac  is  equal 

to  ad  (by  hyp.),  the  angle  acd  is  equal  to  the  angle  adc 

(th.  3).    In  like  manner,  in  the  triangle  rcd,  the  angle  BCD 

is  equal  to  the  angle  bdc,  because  the  side  bc  is  equal  to  bd. 
Hence  then,  the  angle  acd  being  equal  to  the  angle  adc, 
and  the  angle  bcd  to  the  angle  bdc,  by  equal  additions  the 
sum  of  the  two  angles  acd,  bcd,  is  equal  to  the  sum  of  the 
two  adc,  bdc,  (ax.  2),  that  is,  the  whole  angle  acb  equal  to 
the  whole  angle  adb. 

Since  then,  the  two  sides  ac,  cb,  are  equal  to  the  two 
sides  ad,  db,  each  to  each,  (by  hyp.),  and  their  contained 
angles  acb,  adb,  also  equal,  the  two  triangles  abc,  abd, 
are  identical  (th.  1),  and  have  the  other  angles  equal,  viz. 
the  angle  bac  to  the  angle  bad,  and  the  angle  abc  to  the 
angle  akd.    u.  l.  d. 

TilKOKJ  m  VI. 

Win:*  one  line  meets  another,  the  angles  which  it  makes 
on  the  same  side  of  the  otli^r,  are  together  equal  to  two  right 
angles. 

Let  the  line  ah  meet  the  line  cd  :  then 
will  the  two  angles  abc,  abd,  taken  to- 
gether, ho  equal  to  two  right  angles. 

For,  first,  when  the  two  angles  abc,  abd, 
are  equal  to  each  other.  tlic\  are  both  of 
them  right  angles  (def.  15.) 

But  when  the  angles  are  unequal,  suppose  bb  drawn  per- 
pendicular to  cd.  Then,  since  the  two  angles  ebc,  fbd,  are 
right  angles  (def.  15),  and  the  an^le  ebd  is  equal  to  the  two 
angles  eba,  add,  together  (ax.  8),  the  three  angles,  ebc,  kba, 
and  abd,  arc  equal  to  two  right  angles. 

But  the  two  angles  ebc,  eba,  arc  together  equal  to  the 
angle  abc  (ax.  8).  Consequently  the  two  angles  abc,  abd, 
are  also  equal  to  two  right  angles,    q.  e.  d. 

Corol.  1.  Hence  also,  conversely,  if  the  two  angles  abc, 
abd,  on  both  sides  of  the  line  ab,  make  up  together  two 
right  angles,  then  cb  and  bd  form  one  continued  right 
line  cd. 


THEOREMS. 


385 


Corol.  2.  Hence,  alt  the  angles  which  can  be  made,  at 

any  point  b,  by  any  number  of  linos,  on  the  same  side  of 
the  right  line  cd,  are,  when  taken  all  together,  equal  to  two 
right  angles. 

Cord.  3.  And,  ns  all  the  angles  that  can  be  made  on  the 
other  side  of  the  line  cn  are  also  equal  to  two  right  angles  ; 
therefore  all  the  angles  that  can  be  made  quite  round  a  point 
b,  by  any  number  of  lines,  are  equal  to  four  right  angles. 

Coral.  4.  Hence  also  the  whole  circumfer- 
ence of  a  circle,  being  the  sum  of  the  mea- 
sures of  all  the  angles  that  can  be  made  about 
the  centre  f  (def.  57),  is  the  measure  of  four 
right  angles.  Consequently,  a  semicircle,  or 
180  degrees,  is  the  measure  of  two  right  an- 
gles ;  and  a  quadrant,  or  90  degrees,  the  measure  of  one 
right  angle. 

THEOREM  VII. 

When  two  lines  intersect  each  other,  the  opposite  angles  are 
equal. 

Let  the  two  lines  ad,  vu,  intersect  in 
the  point  e  ;  then  will  the  angle  aec  be  /C 
equal  to  the  angle  bed,  and  the  angle     >  i 
aed  equal  to  the  angle  ceb.  a   }  /TQ 

For,  since  the  lino  cc  meets  the  line  / 
ab,  the  two  angles  aec,  bec,  taken  to-  D 
gethcr,  arc  equal  to  two  ricjht  angles  (lli.  6). 

In  like  manner,  the  line  he,  meeting  the  line  cd,  makes 
the  two  angles  dkc,  red,  equal  to  two  right  angles. 

Therefore  the  sum  of  the  two  angles  aec,  bec,  is  equal  to 
the  sum  of  the  two  bec,  ki  d  (ax.  1  ;■. 

And  if  the  angle  nr.c,  which  is  common,  be  taken  away 
from  both  these,  the  remaining  angle  aec  will  be  equal  to 
the  remaining  angle  bed  (ax.  3). 

And  in  like  manner  it  may  be  shown,  that  the  angle  aid 
is  equal  to  the  opposite  angle  bec. 

theorem  viii. 

When  one  side  of  a  triangle  is  produced,  the  outward 
angle  is  greater  than  either  of  the  two  vkw&x&  c^c*\\» 
angles. 


980 


ozomnr. 


Let  abo  be  a  triangle,  having  the 
aide  ab  produced  to  i> ;  then  will  the 
outward  angle  cno  be  greater  than 
cither  of  the  inward  opposite  angles  a 
or  c. 

For,  conceive  the  side  bc  to  be  bi- 
sected in  the  point  e,  and  draw  the 


line  ak,  producing  it  till  ef  bc  equal 
to  ak  ;  and  join»BF. 

Then,  since  the  two  triangles  aec,  hf.f,  have  the  side 
ae  —  the  side  kf,  and  the  side  ce  =  the  side  be  (by  suppos.) 
and  the  included  or  opposite  angles  at  e  also  equal  (th.  7}, 
therefore  those  two  triangles  arc  equal  in  all  respects 
(th.  1),  and  have  the  angle  c  =  the  corresponding  angle 
ebf.  But  the  angle  crd  is  greater  than  the  angle  ebf  ; 
consequently  the  said  outward  angle  cbd  is  afso  greater  than 
the  angle  <:. 

In  like  manner,  if  cb  bo  produced  to  g,  and  ab  b?  1  i- 
sected,  it  may  bc  shown  that  the  outward  angle  abc,  or  it* 
equal  cbd,  is  greater  than  the  other  angle  a. 

THEOREM  IX. 

TnE  greater  side,  of  cvrry  triangle,  is  oiprs'tc  to  the 
greater  ungle  ;  and  the  greater  angle  opposite  to  the  greater 
aide. 

Lot  abc  be  a  triangle,  having  the  side  q 


ab  greater  than  the  side  ac  ;  then  will  the 
angle  acb,  opposite  the  greater  side  ab,  be 
greater  than  the  angle  b,  opposite  the  less 
aide  ac. 


For,  on  the  greater  side  ab,  take  the 
part  ad  equal  to  the  less  side  ac,  and  join  cd.  Then,  since 
bcd  is  a  triangle,  the  outward  angle  Anc  if.  greater  than  the 
inward  opposite  angle  b  (th.  8).  But  the  angle  acd  is  equal 
to  the  said  outward  angle  abc,  because  ad  is  eqal  to  ac 
(th.  3).  Consequently  the  angle  acd  also  is  greater  than  the 
angle  b.  And  since  the  angle  acd  is  only  a  part  of  acb, 
much  more  must  the  whole  angle  acb  be  greater  than  the 
angle  n.    a.  k.  d. 

Again,  conversely,  if  the  angle  c  he  greater  than  the  angle 
b,  then  will  the  side  ab,  opposite  the  former,  be  greater  than 
the  side  ac,  opposite  the  latter. 

For,  if  ab  bc  not  greater  than  ac,  it  must  bo  cither 
eguai  to  it,  or  leas  than  k.    But  it  cannot  be  equal,  for 


TRSOBEKB- 


then  the  angle  c  would  be  equal  to  the  angle  b  (th-  3),  which 
it  is  not,  by  the  supposition.  Neither  can  it  bo  less,  for  then 
the  angle  c  would  be  less  than  the  angle  n,  by  the  former 
part  of  this  ;  which  is  also  contrary  to  the  supposition.  Tho 
aide  ab,  then,  being  neither  equal  to  ac,  nor  less  than  it, 
must  necessarily  be  greater,    a.  u.  d. 


tiieobem  x. 


The  sum  of  any  two  sidtes  of  a  triangle  is  greater  than  the 
third  side. 

Let  abc  be  a  triangle  ;  then  will  the 
sum  of  any  two  of  its  sides  be  greater 
than  the  third  side,  as  for  instance, 
ac  +  cb  greater  than  ab. 

For,  produce  ac  till  cn  be  equal  to 
CB,  or  ad  equal  to  the  sum  of  the  two 
AC  +  cb;  and  join  bi>  Then,  because 
CD  is  equal  to  en  (by  constr.),  the  angle  i>  is  equal  to  the 
angle  cbd(iIi.  3).  But  the  angle  ahd  is  greater  than  the 
angle  cbd,  consequently  it  must  also  be  greater  than  the 
angle  in  And,  since  the  greater  side  of  any  triangle  is  op. 
posite  to  the  greater  nngle  (th.  9),  the  side  ai>  (of  the  tri- 
angle ahd)  is  greater  tbun  the  side  au.  But  ad  is  equal  to 
ac  and  cd,  or  ac  and  cb,  taken  together  (by  constr.)  ;  there- 
fore ac  +  cb  is  also  greater  than  ab.    q.  e.  d. 

Carol.  The  shortest  distance  between  two  points,  is  a 
single  right  line  drawn  from  the  one  point  to  the  other. 


THE0BE3I  XI. 


The  difference  of  any  two  sides  of  a  triangle,  is  less  than 
the  third  side. 

Let  abc  be  a  triangle  ;  then  will  the  D 
difference  of  any  two  sides,  as  ab  —  ac, 
be  less  than  the  third  side  sc. 

For,  produce  the  less  side  ac  to  d, 

till  ad  be  equal  to  the  greater  side  ab,   .  

so  that  <"D  may  be  the  difference  of  tl.o      -A.  B 
two  sides  ah  —  ac  ;  and  join  bd.  Then, 
because  ad  is  equal  to  ab  (by  constr.),  the  opposite  angels  D 
and  abd  are  equal  (th.  3).    J  kit  the  angle  cbd  is  less  than 
the  angle  abd,  and  consequently  also  less  than  the  eaual 
angle  d.   And  since  the  greater  side  of  any  \xv»&$& 


OEOatCTKT. 


opposite  to  the  greater  angle  (th.  9),  the  side  cd  (of  the  tri- 
anglo  bcd)  is  less  than  the  side  bc.    a.  e.  d. 

Otherwise*  Set  off  upon  ah  a  distance  ai  equal  to  ao. 
Then  (th.  |0)  ac  +  cb  is  greater  than  ab,  that  is,  greater 
than  ai  +  ib.  From  these,  take  away  the  equal  parts  AC, 
Ai,  respectively ;  and  there  remains  cb  greater  than  ic.  Con* 
sequently,  ic  is  less  than  cb.    a.  e>-  d. 

THEOREM  XII. 

When  a  lino  intersects  two  parallel  lines,  it  makes  the 
alternate  angles  equal  to  each  other. 

Let  the  line  ef  cut  the  two  parallel 
line  ab,  cd  ;  then  will  the  angle  aef  be 
equal  to  the  alternate  angle  efd. 

For  if  they  are  not  equal,  one  of  them 
must  be  greater  than  the  other;  let  it  be 
efd  for  instance,  which  is  the  greater,  if 
possible ;  and  conceive  the  line  fh  to  bc 
drawn,  cutting  off  the  part  or  angle  efb  equal  to  the  angle 
AEF,  and  meeting  the  line  ab  in  the  point  n. 

Then,  since  the  outward  angle  aef,  of  the  triangle  bef, 
is  greater  than  the  inward  opposite  angle  efb  (th.  8)  ;  and 
since  these  two  angles  also  are  equal  (by  the  constr.)  it  fol- 
lows, that  those  angles  are  both  equal  and  unequal  at  the 
same  time  :  which  is  impossible.  Therefore  the  angle  efd 
is  not  unequal  to  the  alternate  angle  aef,  that  is,  they  are 
equal  to  each  other,    q.  e.  d. 

Corol.  Right  lines  which  are  perpendicular  to  one,  of  two 
parallel  lines,  are  also  perpendicular  to  the  other. 

THEOREM  XIII. 

When  a  lino,  cutting  two  othrr  lines,  makes  the  alter- 
nate  angles  equal  to  each  oilier,  those  two  lines  are  paral- 
lel. 

Let  the  lino  F.r,  cutting  the  two  lines 
ab,  cn,  make  the  alternate  angles  aef, 
dfe,  equal  to  each  other ;  then  will  ab 
be  parallel  to  cd. 

For  if  they  be  not  parallel,  let  some 
other  line,  as  fg,  be  parallel  to  ab. 
Then,  because  of  these  parallels,  the 
angle  aef  is  equal  to  the  alternate  angle  efg  (th.  12).  But 
the  angle  aef  is  equal  to  the  angle  efd  (by  hyp.)  There- 
fore the  anglo  efd  is  equal  to  the  angle  efg  "(ax.  1) ;  that  is, 
a  part  is  equal  to  the  whole,  which  is  impossible.  Therefore 
oo  line  but  cd  can  be  parallel  to  ab.   q.  e.  d. 


THEOREMS. 


280 


Cord.  Those  lines  which  are  perpendicular  to  the  same 
lines,  are  parallel  to  each  other. 


THEOREM  XIV. 

When  a  line  cuts  two  parallel  lines,  the  outward  angle  is 
equal  to  the  inward  opposite  one,  on  the  same  side  ;  and 
the  two  inward  angles,  on  the  sume  side,  equal  to  two  right 
angles. 

Let  the  line  ef  cut  the  two  parallel 
lines  ab,  cd  ;  then  will  the  outward  an- 
gle eob  be  equal  to  the  inward  oppo- 
site angle  ghd,  on  the  same  side  of  the 
line  ef  ;  and  the  two  inward  angles 
bgh,  ghd,  taken  together,  will  be  equal 
to  two  right  angles. 

For  since  the  two  lines  ab,  cd,  are 
parallel,  the  angle  agh  is  equal  to  the  alternate  angle  cud, 
(th.  12.)  But  the  angle  agh  is  equal  to  the  opposite  angle 
egb  (th.  7).  Therefore  the  angle  egb  is  also  equal  to  the 
angle  ghd  (ax.  1).    q.  e.  d. 

Again,  because  the  two  adjacent  angles  egb,  bgh,  are  to- 
gether equal  to  two  right  angles  (th.  (5; ;  of  which  the  angle 
xgb  has  been  shown  to  be  equal  to  the  angle  ghd  ;  therefore 
the  two  angles  bgh,  gud,  taken  together,  are  also  equal  to 
two  right  angles. 

Carol.  1.  And,  conversely,  if  one  line  meeting  two  other 
lines,  make  the  angles  on  the  same  side  of  it  equal,  those 
two  lines  are  parallels. 

Corol.  2.  If  a  line,  cutting  two  other  lines,  make  the  sum 
of  the  two  inward  angles  on  the  same  side,  less  than  two 
right  angles,  those  two  lines  will  not  be  parallel,  but  will 
meet  each  other  when  produced. 

THEOREM  XV. 

Those  lines  which  arc  parallel  to  the  same  line,  are 
parallel  to  each  other. 

Let  the  lines  ab,  cd,  be  each  of  them  G  -p 

parallel  to  the  line  ef  ;  then  shall  the  lines  A  iS 


ab,  cd,  be  parallel  to  each  other.  C  35 

For,  let  the  line  Gibe  perpendicular  jr      """I  p 
to  ef.    Then  will  this  line  be  also  per-  I 
pendicular  to  both  the  lines  ab,  cn  (corol.  th.  12),  and  con- 
sequently the  two  lines  ab,  cd,  are  parallels  (corol.  th.  13\. 

a.  i>. 

Vol.  I.  38 


390 


OKOKETAY. 


THEOREM  XVI. 


Whex  one  sido  of  a  triangle  is  produced,  the  outward 
angle  is  equal  to  both  the  inward  opposite  angles 
together. 

Let  the  side  ab,  of  the  triangle 
ahc,  be  produced  to  d  ;  then  will  the 
outward  angle  cbd  be  equal  to  the  sum 
of  the  two  inward  opposite  angles  a 
and  c. 

For,  conceive  be  to  be  drawn  pa- 
rallel to  the  side  ac  of  the  triangle. 
Then  iic,  meeting  the  two  parallels  ac,  be,  makes  the  alter- 
nate angles  c  and  cbe  equal  (th.  12).  And  ab,  cutting  the 
same  two  parallels  ac,  be,  makes  the  inward  and  outward 
angles  on  the  same  side,  a  and  ebd,  equal  to  each  other 
(th.  14).  Therefore,  by  equal  additions,  the  sum  of  the  two 
angles  a  and  c,  is  equal  to  the  sum  of  the  two  cbe  and  : 
that  is,  to  the  whole  angle  cbd  (by  ax.  2),   <i»  E.  D. 


THEOREM  XVII. 


In  any  triangle,  the  sum  of  all  the  three  angles  is  equal  to 
two  right  angles. 

Let  abc  be  any  plane  triangle  ;  then 
the  sum  of  the  three  angles  a  +  b  +  c 
is  enuul  to  two  right  angles. 

For,  let  the  side  ab  he  produced  to  D. 
Then  the  outward  angle  cbd  is  equal 
to  the  sum  of  the  two  inward  opposite 
angles  a  +  c  (th.  16).  To  each  of  these  equals  add  the  in- 
ward angle  b,  then  will  the  sum  of  the  three  inward  angles 
a  +  b  +  c  be  equal  to  the  sum  of  the  two  adjacent  angles 
abc  +  cbd  (ax.  2).  But  the  sum  of  these  two  last  adjacent 
angles  is  equal  to  two  right  angles  (th.  6).  Therefore  aba 
the  sum  of  the  three  angles  of  the  triangle  a  +  b  +  c  ii 
equal  to  two  right  angles  (ax.  1).    q.  e.  d. 

Carol.  1.  If  two  angles  in  one  triangle,  be  equal  to  two 
angles  in  another  triangle,  the  third  angles  will  also  be  equal 
(ax*  3),  and  the  two  triangles  equiangular. 

Cord.  2.  If  one  angle  in  one  triangle,  be  equal  to  mm 
angle  in  another,  the  sums  of  the  remaining  angles  will  afcj» 
be  equal  (ax.  3). 


THEOREMS. 


291 


CoroZ.  3.  If  one  angle  of  n  triangle  be  right,  the  sum  of 
the  other  two  will  also  be  equal  to  a  right  angle,  and  each  of 
them  singly  will  be  acute,  or  less  thun  a  right  angle. 

Cmxi.  4.  The  two  least  angles  of  every  triangle  are  acute, 
or  each  less  thaa  a  right  angle. 


THEOREM  XVIII. 


Iff  any  quadrangle,  the  sum  of  all  the  four  inward  angles,  is 
equal  to  four  right  angles. 
Let  a bcd  be  a  quadrangle ;  then  the 
sum  of  the  four  inward  angles,  a  +  b  + 
c  +  d  is  equal  to  four  right  angles. 

Let  the  diagonal  ac  be  drawn,  dividing 
the  quadrangle  into  two  triangles,  abc,  adc. 
Then,  because  the  sum  of  the  three  angles 
of  each  of  these  triangles  is  equal  to  two 
right  angles  (th.  17)  ;  it  follows,  that  the  sum  of  all  (he 
angles  of  both  triangles,  which  make;  up  the  lour  angles  of 
the  quadrangle,  must  be  equal  to  four  ri*» In  angles  (ax.  2). 

ci.  K.  D. 

Cord.  1.  Hence,  if  three  of  the  angles  be  right  ones,  tl.e 
fourth  will  also  be  a  right  angle. 

Carol.  2.  And  if  the  sum  of  two  of  the  four  angles  be 
equal  to  two  right  angles,  the  sum  of  the  remaining  two  will 
also  be  equal  to  two  right  angles. 


THEOREM  XIX. 

In  any  figure  whatever,  the  sum  of  all  the  inward  angles, 
taken  together,  is  equul  to  twice  as  many  right  angles, 
wanting  four,  as  the  figure  has  sides. 

Let  abcde  be  any  figure  ;  then  the 
eum  of  all  its  inward  angles,  a  +  h  + 
c  +  D  +  E,  is  equal  to  twice  as  many 
right  angles,  wanting  four,  as  the  figure 
lias  sides. 

For,  from  any  point  r,  within  it,  draw 
lines,  pa,  i»b,  re,  &c.  to  all  the.  angles, 
dividing  the  polygon  into  as  m  iny  tri- 
angles as  it  has  sides.  Now  the  sum  of  the  three  angles  of 
each  of  these  triangles,  is  equal  to  two  riijht  angles  (h.  17)  ; 
therefore  the  sum  of  the  angles  of  alt  the  triangles  is  equal 
to  twice  as  many  right  angles  as  the  figure  has  sides.  But 
the  sum  of  all  the  angles  about  the  point     nYikh  m  w> 


292 


GEOMETRY. 


many  of  f lie  angles  of  the  triangles,  but  no  part  or  the  to- 
ward angles  of  the  polygon,  is  equal  to  four  right  angles 
(corol.  3,  th.  6),  and  must  he  deducted  out  of  the  former 
sum.  Hence  it  follows  that  the  sum  of  all  the  inward  angles 
of  the  polygon  alone,  a  +  b  +  c  +  i>  +  e»  is  equal  to  twice 
as  many  right  angles  as  the  figure  has  sides,  wanting  the 
said  four  right  angles,    u.  e.  d. 

TI1EOREX  XX. 

When  every  side  of  any  figure  is  produced  out,  the  sum 
of  all  the  outward  angles  thereby  made,  is  equal  to  four  right 
angles. 

Let  a,  b,  c,  dtc.  be  the  outward 
angles  of  any  polygon,  made  by  pro- 
ducing all  the  sides  ;  then  will  the  sum 
a  +  b  +  c  +  i)  +  e,  of  all  those  outward 
angles,  be  equal  to  four  right  angles. 

For  every  one  of  these  outward  an- 
gles, together  with  its  adjacent  inward 
angle,  make  up  two  right  angles,  as 
A+a  equul  to  two  right  angles,  being 
the  two  angles  made  by  one  line  meeting  another  (th.  6). 
And  there  being  as  many  outward,  or  inward  angles,  as  the 
figure  has  sides  ;  therefore  the  sum  of  all  the  inward  and 
outward  angles,  is  equal  to  twice  as  many  right  angles  as 
the  figure  has  sides.  But  the  sum  of  all  the  inward  angles 
with  four  right  angles,  is  equal  to  twice  as  many  right  angles 
as  the  figure  has  sides  (th.  19).  Therefore  the  sum  of  all 
the  inward  and  all  the  outward  angles,  is  equal  to  the  sum 
of  all  the  inward  angles  and  four  right  angles  (by  ax.  1). 
From  each  of  these  take  away  all  the  inward  angles,  and 
there  remains  all  the  outward  angles  equal  to  four  right  angles 
(by  ax.  3j. 

THEOREM  XXI. 

A  perpendicular  is  the  shortest  line  that  can  be  drawn 
from  a  given  point  to  an  indefinite  line.  And,  of  any  other 
linos  drawn  from  the  same  point,  those  that  are  nearest  the 
perpendicular  are  less  than  those  more  remote. 

If  ab,  ac,  ad,  &c.  be  lines  drawn  from 
the  given  point  a,  to  the  indefinite  line  de, 
of  which  ab  is  perpendicular  ;  then  shall 
the  perpendicular  ab  be  less  than  ac,  and 
ac  less  than  ad,  &c. 

For,  the  angle  b  being  a  t\gV\t  quo,  the 


TREOBEKI. 


298 


angle  c  is  acute  (by  cor.  3,  th.  17),  and  therefore  less  than 
the  angle  b.  But  the  less  angle  of  a  triangle  is  subtended 
by  the  leas  side  (th.  9).  Therefore  the  side  ab  is  less  than 
the  side  ac. 

Again,  the  angle  acb  being  acute,  as  before,  the  adjacent 
angle  acd  will  be  obtuse  (by  th.  tf)  ;  consequently  the  angle 
d  is  acute  (corol.  3,  th.  17),  and  therefore  is  less  than  the 
angle  c.  And  since  the  less  side  is  opposite  to  the  less  angle, 
therefore  the  side  ac  is  less  than  the  side  ad*  q.  s.  d. 


Carol.  A  perpendicular  is  the  least  distance  of  a  given 
point  from  a  line. 


THEOREM  XXII. 

Thb  opposite  sides  and  angles  of  any  parallelogram  are 
equal  to  each  other  ;  and  the  diagonal  divides  it  into  two 
equal  triangles. 

Let  abcd  be  a  parallelogram,  of  which 
the  diagonal  is  bd  ;  then  will  its  opposite 
sides  and  angles  be  equal  to  each  other, 
and  the  diagonal  bd  will  divide  it  into  two 
equal  parts,  or  triangles. 

For,  since  the  sides  ab  and  dc  are  pa- 
rallel, as  also  the  sides  ad  and  bc  (defin. 


32),  and  the  line  bd  meets  them  ;  therefore  the  alternate 
angles  are  equal  (th.  12),  namely,  the  angle  abd  to  the  angle 
cdb,  and  the  angle  adb  to  the  angle  cbd.  Hence  the  two 
triangles,  having  two  angles  in  the  one  equal  to  two  angles 
in  the  other,  have  also  their  third  angles  equal  (cor.  1,  th.  17), 
namely,  the  angle  a  equal  to  the  angle  c,  which  are  two  of 
the  opposite  angles  of  the  parallelogram. 

Also,  if  to  the  equal  angles  abd,  cdb,  be  added  the  equal 
angles  cbd,  abd,  the  wholes  will  be  equal  (ax.  2),  namely, 
the  whole  angle  abc  to  the  whole  ado,  which  are  the  other 
two  opposite  angles  of  the  parellelogram.  ft.  e.  d. 

Again,  since  the  two  triangles  are  mutually  equiangular 
and  have  a  side  in  each  equal,  viz.  the  common  side  bd  ; 
therefore  the  two  triangles  are  identical  (th.  2),  or  equal  in 
all  respects,  namely,  the  side  ab  equal  to  the  opposite  side 
dc,  and  ad  equal  to  the  opposite  side  bc,  andlta^fata 
triangle  abd  equal  to  the  whole  triangle  bcd.   <fc-  fe«  t>% 


294 


GEOMETRY. 


Corol.  1.  Hence,  if  one  angle  of  a  parallelogram  be  a  right 
angle,  ail  the  other  three  will  also  be  right  angles,  and  the 
parallelogram  a  rectangle. 

Corol.  2.  Henc;  also,  the  sum  of  any  two  adjacent  angles 
of  a  parallelogram  is  equal  to  two  right  angles. 

THEOREM  XXIII. 

Every  quadrilateral,  whose  opposite  sides  are  equal,  is  a 
parallelogram,  or  has  its  opposite  sides  parallel. 


Let  a bcd  be  a  quadrangle,  having  the 
opposite  sides  equal,  namely,  the  side  ab 
equal  to  nc,  and  ad  equal  to  hc  ;  then 
shall  these  equal  sides  be  also  parallel, 
and  the  figure  a  parallelogram. 


For,  let  the  diagonal  bd  he  drawn. 
Then,  the  triangles,  abd,  cud,  being 
mutually  equilateral  (by  hyp.),  they  are 
also  mutually  equiangular  (th.  5),  or  have  their  corresponding 
angles  equal ;  consequently  the  opposite  sides  are  parallel 
(th.  13) ;  viz.  the  side  ah  parallel  to  nc,  and  ad  parallel  to 
bc,  and  the  figure  is  a  parallelogram,    a.  k.  d. 

THEORKM  XXIV. 

Those  lines  which  join  the  corresponding  extremes  of 
two  equal  and  parallel  lines,  are  themselves  equal  and 
parallel. 

Let  ab,  nc,  be  two  equal  and  parallel  lines  ;  then  will 
the  lines  ad,  bc,  which  join  their  extremes,  be  also  equal 
and  parallel.    [Sec  the  fig.  above.] 

For,  draw  the  diagonal  bd.  Then,  because  ab  and  dc  are 
parallel  (by  hyp.),  the  angle  abd  is  equal  to  the  alternate 
angle  bdc  (th.  12).  Hence  then,  the  two  triangles  having 
two  sides  and  the  contained  alines  equal,  viz.  the  side  ab 
equal  to  the  aide  dc,  and  the  side  bo  common,  and  the  con- 
tained angle  abd  equal  to  the  contained  angle  bdc,  they 
have  the  remaining  sides  and  angles  also  respectively  equal 
(th.  1) ;  consequently  ad  is  equal  to  bc,  and  also  parallel  to 
it  (th.  12).    u.  £.  d. 

THEORKM  XXV. 

Parallelograms,  as  also  triangles,  standing  on  the 
same  base,  and  between  the  samo  parallels,  are  equal  to 
each  other. 


THEOREMS. 


295 


Let  abcd,  abep,  be  two  parallelograms,  J>     C  T  E 
and  abc,  abf,  two  triangles,  standing  on    V     A  A  7 
the  same  base  ab,  and  between  the  same     \    /  V ;  / 
parallels  ab,  de  ;  then  will  the  parallelo-      \  / 
gram  abcd  be  equal  to  the  parallelogram       y/  V/ 
abbp,  and  the  triangle  abc  equal  to  the     Js^  JJ 
triangle  abf* 

For,  since  the  line  de  cuts  the  two  parallels  af,  be,  and 
the  two  ad,  bc,  it  makes  the  angle  e  equal  to  the  angle  afd, 
and  the  angle  d  equal  to  the  angle  bce  (th.  14) ;  the  two 
triangles  adf,  bce,  are  therefore  equiangular  (cor.  1,  th.  17) ; 
and  having  the  two  corresponding  sides  ad,  bc,  equal 
(th.  22),  being  opposite  sides  of  a  parallelogram,  these  two 
triangles  are  identical,  or  equal  in  all  respects  (th.  2).  If 
each  of  these  equal  triangles  then  be  taken  from  the  whole 
space  abed,  there  will  remain  the  parallelogram  abef  in 
the  one  case,  equal  to  the  parallelograms  abcd  in  the  other 
(by  ax.  3). 

Also  the  triangles  abc,  abf,  on  the  same  base  ah,  and 
between  the  same  parallels,  are  equal,  being  the  halves  of 
the  said  equal  parallelograms  (th.  22).    q.  r.  d. 

CoroL  1.  Parallelograms,  or  triangles,  having  the  same 
base  and  altitude,  are  equal.  For  tho  altitude  is  the  same  as 
the  perpendicular  or  distance  between  the  two  parallels,  which 
is  every  where  equal,  by  the  definition  of  parallels. 

Corel.  2.  Parallelograms,  or  triangles,  having  equal  bases 
and  altitudes,  are  equal.  For,  if  the  one  figure  be  applied 
with  its  base  on  the  other,  the  bases  will  coincide  or  be  the 
same,  because  they  are  equal :  and  so  the  two  figures,  having 
the  same  base  and  altitude,  are  equal. 

theorem  xxvi. 

If  a  parallelogram  and  a  triangle,  stand  on  the  same 
base,  and  between  the  same  parallels,  the  parallelogram 
will  be  double  the  triangle,  or  the  triangle  half  the  paral- 
lelogram. 

Let  abcd  be  the  parallelogram,  and  abe  a 
triangle,  on  the  same  base  ab,  and  between 
the  same  parallels  ab,  de  ;  then  will  the 
parallelogram  abcd  he  double  the  triangle 
abe,  or  the  triangle  half  the  parallelo- 
gram. 

For,  draw  the  diagonal  ac  of  the  parallelogram,  divid\\i% 
it  into  two  equal  parts  (th.  22).   Then  bec&uafe  lY\&  XxwoqgtK* 


296 


GEOMETRY. 


abc,  abe,  on  the  same  base,  and  between  the  same  parallels, 
are  equal  (th.  25)  ;  and  because  the  one  triangle  abc  is  half 
the  parallelogram  abcd  (th.  22),  the  other  equal  triangle 
abe  is  also  equal  to  half  the  same  parallelogram  abcd. 
q.  e.  d. 

Card.  1.  A  triangle  is  equal  to  half  a  parallelogram  of  the 
same  base  and  altitude,  because  the  altitude  is  the  perpendi- 
cular distance  between  the  parallels,  which  is  every  where 
equal,  by  the  definition  of  parallels. 

Carol.  2.  If  the  base  of  a  parallelogram  be  half  that  of  a 
triangle,  of  the  same  altitude,  or  the  base  of  the  triangle  be 
double  that  of  the  parallelogram,  the  two  figures  will  be 
equal  to  each  other. 


THEOREM  XXVn. 


0 


Rectangles  that  are  contained  by  equal  lines,  are  equal 
to  each  other. 

Let  bd,  fh,  be  two  rectangles,  having       jj    C  H  G 
the  sides  ab,  bc,  equal  to  the  sides  ef,  "7 
fo,  each  to  each ;  then  will  the  rectangle  / 
bd  be  equal  to  the  rectangle  fh.  / 

For,  draw  the  two  diagonals  ac,  eg,  A.  B  £  F 
dividing  the  two  parallelograms  each  into 
two  equal  parts.  Then  the  two  triangles  abc,  efg,  are 
equal  to  each  other  (th.  1),  because  they  have  the  two  sides 
ab,  bc,  and  the  contained  angle  b,  equal  to  the  two  sides 
ef,  fg,  and  the  contained  angle  f  (by  hyp.}.  But  these 
equal  triangles  are  the  halves  of  the  respective  rectangles. 
And  because  the  halves,  or  the  triangles,  are  equal,  the 
wholes,  or  the  rectangles  db,  hf,  are  also  equal  (by  ax.  6). 
a.  e.  d. 

Carol.  The  squares  on  equal  lines  are  also  equal ;  for 
every  square  is  a  species  of  rectangle. 


THEOREM  XXVIII. 


The  complements  of  the  parallelograms,  which  are  about 
the  diagonal  of  any  parallelogram,  are  equal  to  each  other. 

Let  ac  be  a  parallelogram,  bd  a  dia- 
gonal, eif  parallel  to  abof  dc,  and  <;iu  J)  G 
parallel  to  "ad  or  bc,  making  ai,  ic,  com-  K  j 
plements  to  the  parallelograms  eg,  iif,  E 


which  are  about  the  diagonal  db  :  then  /  ~j 

will  the  complement  ai  be  equal  to  the  h 
complement  xc 


i 


THEOREMS.  207 

For,  since  the  diagonal  db  bisects  the  three  parallelograms 
ac,  eg,  hp  (th.  22) ;  therefore,  the  whole  triangle  dab  being 
equal  to  the  whole  triangle  dcb,  and  the  parts  dei,  ihb,  re* 
sportively  equal  to  the  parts  dgi,ifb,  the  remaining  parts  Ar, 
ic,  must  also  be  equal  (by  ax.  3).    q.  e.  d. 


THEOREM  XXIX. 


A  trapezoid,  or  trapezium  haying  two  sides  parallel,  is 
equal  to  half  a  parallelogram,  whose  base  is  the  sum  of  those 
two  sides,  and  its  altitude  the  perpendicular  distance  between 
them. 

Let  abcd  be  the  trapezoid,  having  its 
two  sides  ab,  dc,  parallel ;  and  in  ah 
produced  take  be  equal  to  dc,  so  that 
ae  may  be  the  sum  of  the  two  parallel 
sides ;  produce  dc  also,  and  let  kf,  gc,  G  B  E 

bh,  be  all  three  parallel  to  ad.    Then  is 
af  a  parallelogram  of  the  same  altitude  with  the  trapezoid 
abcd,  having  its  base  ae  equal  to  the  sum  of  the  parallel 
sides  of  the  trapezoid  ;  and  it  is  to  be  proved  that  the  trape- 
zoid abcd  is  equal  to  half  the  parallelogram  af. 

Now,  since  triangles,  or  parallelograms,  of  equal  bases  and 
altitude,  are  equal  (corol.  2,  th.  25),  the  parallelogram  no  is 
equal  to  the  parallelogram  he,  and  the  triangle  cob  equal  to 
the  triangle  chb  ;  consequently  the  line  bc  bisects,  or  equal- 
ly divides,  the  parallelogram  af,  and  abcd  is  the  half  of  it. 

Q.  E.  D. 


THEOREM  XXX. 


J3     G  H  C 


The  sum  of  all  the  rectangles  contained  under  one  whole 
line,  and  the  several  parts  of  another  line,  any  way  divid- 
ed, is  equal  to  the  rectangle  contained  under  the  two  whole 
lines. 

Let  ad  be  the  one  line,  and  ab  the 
other,  divided  into  the  parts  ae,  ef, 
fb  ;  then  will  the  rectangle  contained 
by  ad  and  ab,  be  equal  to  tlio  sum  of 
the  rectangles  ot  ad  and  ae,  and  ad  and 
ef,  and  ad  and  fb  :  thus  expressed, 

AD  •  AB  =  AD  .  AE  +  AD  .  EF  +  AD  .  FB. 

For,  make  the  rectangle  ac  of  the  two  whole  lines  ad, 
ab  ;  and  draw  eg,  fh,  perpendicular  to  ab,  or  parallel  to 
ad,  to  which  they  are  equal  (th.  22).    Then  \ta  ^iWAa 
rectangle  ac  is  made  up  of  all  the  other  TectaaeW 

Vol.  I.  39 


A.    E  f  B 

208 


GEOMETBY. 


G  H  C 


fc.  Hut  these  rectangles  arc  contain- 
ed by  ad  and  ae,  eg  and  ef,  i  n  and  fb  ; 
which  aro  equal  to  the  rectangles  of  ad 
and  ae,  ad  and  ef,  ad  and  fb,  because 
ad  is  equal  to  each  of  the  two  eg,  fh. 
Therefore  the  rectangle  \d.  ab  is  equal 
to  the  sum  of  all  l  he  other  rectangles  ad  • 

AE,  AD  .  EF,  AD  .  FB.     Q.  E.  D. 

Corol.  If  a  right  line  be  divided  into  any  two  parts,  the 
square  on  the  whole  line,  is  equal  to  both  the  rectangles  of 
the  whole  line  and  each  of  the  parts. 


X  FB 


THEOREM  XXXI. 

The  square  of  the  sum  of  two  lines,  is  greater  ti.an  the 
sum  of  their  squares,  by  twice  the  rectangle  of  the  said 
lines.  Or,  the  square  of  a  whole  line,  is  equal  to  the 
squares  of  its  two  parts,  together  with  twice  the  rectangle  of 
those  parts. 

Let  the  line  ab  be  the  sum  of  any  two 
lines  ac,  ch  ;  then  will  the  square  of  ab  js-      H  ij 

be  equal  to  the  squares  of  .u?,  cb,  together 
with  twice  the  rectangle  of  ac  .  cb.  That 
1S,  ABa=  AC2  +  cb3  +  2ac  .  cn. 


I 


For,  lot  \ni)E  be  the  square  on  the  sum  *       C  B 

or  whole  line  ab,  and  acfg  the  square 
on  the  part  ac.    Produce  cf  and  ar  to  the  other  sides  at  H 
and  i. 

From  the  lines  ch,  ci.  which  are  equal,  being  each  equal 
to  the  biiVs  of  the  square  ab  or  bd  (th.  22),  take  the  parts 
CF,  gf,  which  arc  also  equal,  being  the  sides  of  the  square 
Ai'.  am1  there  remains  *u  equal  to  fx,  which  are  also  equal 
to  mi.  or,  being  the  opposite  sides  of  the  parallelogram, 
fleucc  the  figure  hi  is  equilateral  :  and  it  has  all  its  angles 
riiiht  onus  teorol.  1,  th.  22) :  it  is  therefore  a  square  on  the 
line  fi,  or  the  square  of  its  equal  cn.  Also  the  figures  ef, 
fb,  arc  equal  to  two  rectangles  under  ac  and  cb,  because 
c;r  is  equal  to  ac.  and  fh  or  fi  equal  to  cb.  But  the 
whole  square  ad  is  made  up  of  the  four  figures,  viz.  the  two 
tiquarch  af,  id,  and  the  two  equal  rectangles  ef,  fb.  That 
i??  the  .-square  of  aji  is  equal  to  the  squares  of  ac,  cb,  toge- 
ihcr  with  twice  th"  rectangle  of  ac,  cb.    a.  u.  d. 

0>r.  /.  Hence,  if  a  line  be  divided  into  two  equal  parts  ; 
the  .square  of  the  whole  line  will  be  equal  to  four  times  the 
square  of  half  the  hue. 


I 

THEOREMS. 


299 


E 


ID 


THEOREM  XXXII. 

The  square  of  the  difference  of  two  lines,  is  less  than  the 
sum  of  their  squares,  by  twice  the  rectangle  of  the  said 
lines. 

Let  ac,  bc,  be  any  two  lines,  and  ab 

their  difference  :  then  will  the  square  of  ab  &  

be  less  than  the  squares  of  ac,  bc,  by 
twice  the  rectangle  of  ac  and  bc.  Or, 

AB*  s*  AC1  +  BC1 — 2AC  .  BC. 

For,  let  abde  be  the  square  on  the  dif- 
ference ab,  and  acfo  the  square  on  the        A.  B 
line  ac.    Produce  ed  to  h  ;  also  produce  K  I 

db  and  hc,  and  draw  ki,  making  bi  the  square  of  the  other 
line  bc. 

Now  it  is  visible  that  the  square  ad  is  less  than  the  two 
squares  af,  bi,  by  the  two  rectangles  ef,  di.  But  gf  is 
equal  to  the  one  line  ac,  and  ue  or  fii  is  equal  to  .the  other 
line  bc  ;  consequently  the  rectangle  kf,  contained  under  i:« 
and  of,  is  equal  to  the  rectangle  of  ac  and  bc. 

Again,  fh  being  equal  to  ci  or  bc  or  Dir,  by  adding  the 
common  part  hc,  the  whole  hi  will  bo  equal  to  the  whole  rc, 
or  equal  to  ac  ;  and  consequently  the  figure  di  is  equal  to 
the  rectangle  contained  by  ac  and  bc. 

Hence  the  two  figures  ef,  di,  arc  two  rectangles  of  the 
two  lines  ac,  bc  ;  and  consequently  the  square  of  vn  is 
less  than  the  squares  of  ac,  bc,  by  twice  the  rectangle 

AC  .  BC.     Q.  E.  B. 

THEOREM  XXXUI. 

The  rectangle  under  the  sum  and  difference  of  two  lines,  is 
equal  to  the  difference  of  the  squares  of  those  lines*. 
Let  ab,  ac,  be  any  two  unequal  lines  ; 

then  will  the  difference  of  the  squares  of 

ab,  ac,  be  equal  to  a  rectangle  under 

their  sum  and  difference    That  is, 

AB1—  AC3  =  AB  -f-  AC  .  AB  —  AC. 

For,  let  abde  be  the  square  of  ab,  and 
acfo  the  square  of  ac.  Produce  db 
till  bh  be  equal  to  ac  ;  draw  hi  parallel 
to  ab  or  ed,  and  produce  fc  both  ways 
to  i  and  k. 


E 
G 


C 


F 


*  This  and  the  two  preceding  theorems,  arc  evinced  algebraically, 
by  the  three  expression! 

( a  +  6 ) J  =  a '  +  %ib  +  6»  a*  +  6»  -f-  2ab 
(«  —  6  )3  =  a>  —  2a6  4  fta  =  a>  +  63  —  2a6 
(a  +  6)(ft-6):=«*—  6*. 


800 


GEOMETRY. 


Then  the  difference  of  the  two  squares  ad,  af,  is  evi- 
dently the  two  rectangles  ef,  kb.  But  the  rectangles  ef, 
bi  are  equal,  being  contained  under  equal  lines ;  for  ex  and 
bh  are  each  equal  to  ac,  and  ge  is  equal  to  cb,  being  each 
equal  to  the  difference  between  ab  and  ac,  or  their  equals 
ae  and  ag.  Therefore  the  two  ef,  kb,  are  equal  to  the  two 
xb9  bi,  or  to  the  whole  kh  ;  and  consequently  kh  is  equal 
to  the  difference  of  the  squares  ad,  af.  But  kh  is  a  rect- 
angle contained  by  dh,  or  the  sum  of  ab  and  ac,  and  by  kd, 
or  the  difference  of  ab  and  ac.  Therefore  the  difference  of 
the  squares  of  ab,  ac,  is  equal  to  the  rectangle  under  their 
sum  and  difference.    Q.  e.  d. 

theorem  xxxiv. 

In  any  right  angled  triangle,  the  square  of  the  hypo- 
thenuse,  is  equal  to  the  sum  of  the  squares  of  the  other  two 
sides* 

Let  abc  be  a  right-angled  triangle,  Q 
having  the  right  angle  c ;  then  will  the 
square  of  the  hypothenuse  ab,  be  equal 
to  the  sum  of  the  squares  of  the  other  -° 
two  sides  ac,  cb.     Or  ab3  =  ac* 

+  BCa. 

For,  on  ab  describe  the  square  ae, 
and  on  ac,  cb,  the  squares  ag,  bh  ; 
then  draw  ck  parallel  to  ad  or  be  ; 
and  join  ai,  bf,  cd,  ck. 

Now,  because  the  line  ac  meets  the  two  cg,  cb,  so  as  to 
make  two  right  angles,  these  two  form  one  straight  line  gb 
(corol.  1,  th.  6).  And  because  the  angle  fac  is  equal  to  the 
angle  dab,  being  each  a  right  angle,  or  the  angle  of  a  square ; 
to  each  of  these  equals  add  the  common  angle  bac,  so  will 
the  whole  angle  or  sum  fab,  be  equal  to  the  whole  angle  or 
sum  cad.  But  the  line  fa  is  equal  to  the  line  ac,  and  the 
line  ab  to  the  line  ad,  being  sides  of  the  same  square ;  so 
that  the  two  sides  fa,  ab,  and  their  included  angle  fab.  are 
equal  to  the  two  sides  ca,  ad,  and  the  contained  angle  cad, 
each  to  each  :  therefore  the  whole  triangle  afb  is  equal  to 
the  whole  triangle  acd  (th.  1). 

But  the  square  ag  is  double  the  triangle  afb,  on  the 
same  base  fa,  and  between  the-  same  parallels  fa,  ob 
(th.  26) ;  in  like  manner  the  parallelogram  ak  is  double  the 
triangle  acd,  on  the  same  base  ad,  and  between  the  same 
parallels  ad,  ck.  And  since  the  doubles  of  equal  things, 
are  equal  (by  ax.  6) ;  therefore  the  square  ag  is  equal  to  the 
parallelogram  ak. 


THEOREMS. 


301 


la  like  manner,  the  other  square  bh  is  proved  equal  to 
the  other  parallelogram  bk.  Consequently  the  two  squares 
ag  and  bh  together,  are  equal  to  the  two  parallelograms  ak 
and  bk  together,  or  to  the  whole  square  ak.  That  is,  the 
sum  of  the  two  squares  on  the  two  less  sides,  is  equal  to  the 
square  on  the  greatest  side.    a.  e.  d. 

Cord.  1.  Hence,  the  square  of  either  of  the  two  less  sides, 
is  equal  to  the  difference  of  the  squares  of  the  hypothenuse 
and  the  other  side  (ax.  3)  ;  or,  equal  to  the  rectangle  con- 
tained by  the  sum  and  difference  of  the  said  hypothenuse 
and  other  side  (th.  33). 

Carol.  2.  Hence  also,  if  two  right-angled  triangles  have 
two  sides  of  the  one  equal  to  two  corresponding  sides  of  the 
other  ;  their  third  sides  will  also  be  equal,  and  the  triangles 
identical. 


THEOREM  XXXV. 


In  any  triangle,  the  difference  of  the  squares  of  the 
two  sides,  is  equal  to  the  difference  of  the  squares  of  the 
segments  of  the  base,  or  of  the  two  lines,  or  distances, 
included  between  the  extremes  of  the  base  and  the  perpen- 
dicular. 

Let  abc  be  any  triangle,  having 
cd  perpendicular  to  ab  ;  then  will 
the  difference  of  the  squares  of  ac, 
bc,  be  equal  to  the  difference  of 

the  squares  of  ad,  bd  ;  that  is,  _  _    A     ^  ^ 

AC*  BC3  =  AD2  BD2.  A     BD   A  DB 

For,  since  ac2  is  equal  to  ad2  +  cd2  >        ,  „.N 

and  bc2  is  equal  to  bd2  +  c  d2  \  W  ihm  M>  ; 
Theref.  the  difference  between  ac2  and  bc2, 
is  equal  to  the  difference  between  ad2  +  cd2 

and  bd2  +  cd2, 

or  equal  to  the  difference  between  ad2  and  bd3, 

by  taking  away  the  common  square  cd3.  q.  e.  d. 

Carol.  The  rectangle  of  the  sum  and  difference  of  the  two 
sides  of  any  triangle,  is  equal  to  the  rectangle  of  the  sum 
and  difference  of  the  distances  between  the  perpendicular 
and  the  two  extremes  of  the  base,  or  equal  to  the  rectangle 
of  the  base  and  the  difference  or  sum  of  the  segments, 
according  as  the  perpendicular  falls  within  or  without  the 
triangle. 


302 


GEOMETRY. 


That  is,  (ac+bc)  .  (ac — bc)  =  (ad+bd)  .  (ad — bd) 
Or,  (ac+bc)  .  (ac — bc)  =  ab  .  (ad — bd)  in  the  2d  fig. 
And  (ac+bc)  .  (ac— bc)  =  ab  .  (ad+bd)  in  the  lrt  fig. 


THEOREM  XXXVI. 


In  any  obtuse-angled  triangle,  the  square  of  the  side  sub- 
tending the  obtUBe  angle,  is  greater  than  the  sum  of  the 
squares  of  the  other  two  sides,  by  twice  the  rectangle  of 
the  base  and  the  distance  of  the  perpendicular  from  the  ob- 
tuse angle. 

Let  abc  be  a  triangle,  obtuse  angled  at  b,  and  cd  perpen- 
dicular to  ab  ;  then  will  the  square  of  ac  be  greater  than  the 
squares  of  ab,  bc,  by  twice  the  rectangle  of  ab,  bd.  That 
is,  ac3  =  ab3  +  bc8  +  2a n  .  bd.  See  the  1st  fig.  above,  or 
below. 

For,  ad2  =  ab2  +  bd3  +  2ab  .  bd  (th.  31). 

And  ad1  +  en8  =  ab3  +  bd*  +  cd2  +  2ab  .  bd  (ax.  2). 

But  ad2  +  cd2  =  ac3,  and  bd2  +  cd*  =  bc2  (th.  34). 
Therefore  ac2  =  ab2  +  bc2  +  2a b  .  bd.    q.  e.  d. 


THEOREM  XX XVI I. 


In  any  triangle,  the  square  of  the  side  subtending  an  acute 
angle,  is  less  than  the  squares  of  the  base  and  the  other  aide, 
by  twice  the  rectangle  of  the  base  and  the  distance  of  the 
perpendicular  from  the  acute  angle. 

Let  abc  be  a  triangle,  having  ^  „ 

the  angle  a  acute,  and  cd  perpen-  ^ 
dicular  to  ab  ;  then  will  the  square  ''■ 
of  bc,  be  less  than  the  squares 

of  ab,  ac,  by  twice  the  rectangle  

of  ab,  ad.  That  is,  bc===  ab2+  W  .B  D  A.  J)B 
ac*  —  2ad  .  AB. 

For  BD3  =  AD3  +  AB2  —  2ad  .  AB  (th.  32). 

And  BD3  +  DC2  =  AD2  +  DC2  +  AB2 — 2 AD  .  AB  (aX.  2), 

Therefore  bc3  =  ac2  +  ab2  —  2ad  .  ab  (th.  34).    q.  s.  d. 


THEOREM  XXXVIII. 


Ik  any  triangle,  the  double  of  the  square  of  a  line  drawn 
from  the  vertex  to  the  middle  of  the  base,  together  with 


THEOREMS. 


303 


double  the  square  of  the  half  base,  is  equal  to  the  sum  of  the 
squares  of  the  other  two  sides. 

Let  abc  be  a  triangle,  and  <;d  the  line 
drawn  from  the  vertex  to  the  middle  of  9 
the  base  ab,  bisecting  it  into  the  two  equal 
parts  ad,  db  ;  then  will  the  sum  of  the 
squares  of  ac,  ch,  be  equal  to  twice  the 
sum  of  the  squares  of  <;«,  ad  ;  or  ac3  + 
cb3  =  2cd3  +  2\Da. 


/ 
'  j 


A  DEB 


For  AC8  =  CD3  +  ad3  +  2ad  •  de  (th.  36). 
And  bc3  =  CD*  +  bd2  —  2ad  .  db  (th.  37). 
Therefore  ac3  +  bc3  =  2cd3  +  ad3  +  bd3 

=  2cd3  -f-  2ad3  (ax.  2).    <j.  e.  d. 


tiikork;i  xxxix. 

In  an  isosceles  triangle,  the  square  of  a  line  drawn  from 
the  vertex  to  any  point  in  the  base,  together  with  the  rect- 
angle of  the  segments  of  the  base,  is  equal  to  the  square  of 
one  of  the  equal  sides  of  the  trim.gle. 

Let  abc  be  the  isosceles  triangle,  and  cd  c 
a  line  drawn  from  the  vertex  to  any  point 
D  in  the  base  :  then  will  the  square  of  ac, 
be  equal  to  the  square  of  ci>,  together 
with  the  rectangle  of  ad  and  on.    That  is, 

AC3  =  CD3  +  AD  .  DB. 

For  AC3— CD3  =  AE3  —  DE3  (th.  35). 

=  AD  .  DB  (th.  33). 

Therefore,  ac2  =  cd2  -f-  ad  .  db  (ax.  2).    a.  k.  d. 


A  13 


THEOREM  XL. 

In  any  parallelogram,  the  two  diagonals  bisect  each  other ; 
and  the  sum  of  their  squares  is  equal  to  the  sum  of  the 
squares  of  all  the  four  sides  of  the  parallelogram. 

Let  abcd  be  a  parallelogram,  whost;  "JJ  C 
diagonals  intersect  each  other  in  e  :  then 
will  ae  be  equal  to  ec,  and  be  to  i:i>  :  and 
the  sum  of  the  squares  of  ,u\  m>,  will  be 
equal  to  the  sum  of  the  square  s  of  ab,  ik\ 
cd,  da.  That  is, 

ae  =  ec,  and  bj:  —  ed, 
and  ac3+  bd'  =  abs  +  bc3-t  ci>  r  ua  • 


804 


GEOMETRY. 


For,  the  triangles  aeb,  dec,  are  equiangular,  because 
they  have  the  opposite  angles  at  e  equal  (th.  7),  and  the  two 
lines  ac9  bd,  meeting  the  parallels  ab,  dc,  make  the  angle 
bae  equal  to  the  angle  dce,  and  the  angle  abe,  equal  to  the 
angle  cde,  and  the  side  ab  equal  to  the  side  dc  (th.  22) ; 
therefore  these  two  triangles  are  identical,  and  have  their 
corresponding  sides  equal  (th.  2),  viz.  ae  =  ec,  and  be  a  ed. 

Again,  since  ac  is  bisected  in  e,  the  sum  of  the  squares 
ad3  +  DC3  =  2AE3  +  2des  (th.  38). 

In  like  manner,  ab'  +  bc*  =■  2aes  +  2be3  or  2de3. 

Theref.  abs  +  bc3  +  CD*  +  da1  =  4  a  e3  +  4de3  (ax.  2). 

But,  because  the  square  of  a  whole  line  is  equal  to  4 
times  the  square  of  half  the  line  (cor.  th.  31),  that  is,  ac*  = 
4ae\  and  bd3  =  4de3  : 

Theref.  ab3  +  bc3  +  cd3  -4  da3  =  ac2  f  bd3  (ax.  1). 

Q.  E.  D. 

Cor.  1.  If  ad  =  dc,  or  the  parallelogram  be  a  rhombus; 
then  ad3  =  ae3  +  ED3,  CD3  =■  de*  +  ce1,  dsc. 

Cor.  2.  Hence,  and  by  th.  34,  the  diagonals  of  a  rhom- 
bus intersect  at  right  angles. 


THEOREM  XLI. 


If  a  line,  drawn  through  or  from  the  centre  of  a  circlet 
bisect  a  chord,  it  will  bc  perpendicular  to  it;  or,  if  it  be 
perpendicular  to  the  chord,  it  will  bisect  both  the  chord  and 
the  arc  of  the  chord. 

Let  ab  be  any  chord  in  a  circle,  and  ct> 
a  line  drawn  from  the  centre  <-  to  the 
chord.  Then,  if  the  chord  be  bisected  in 
the  point  d,  cd  will  bc  perpendicular  to 
ab. 

Draw  the  two  radii  ca,  cb.  Then  the 
two  triangles  acd,  bcd,  having  ca  equal  to 
cb  (def.  44),  and  cd  common,  also  ad  equal 
to  db  (by  hyp.) ;  they  have  all  the  three  sides  of  the  one, 
equal  to  all  the  three  sides  of  the  other,  and  so  have  their 
angles  also  equal  (th.  5).  Hence  then,  the  angle  ado  being 
equal  to  the  angle  bdc,  these  angles  are  right  angles,  and  the 
line  cd  is  perpendicular  to  ab  (def.  11). 

Again,  if  cd  bo  perpendicular  to  ah*  then  will  the  chord 


THEOUM*. 


Mft 


ab  be  bisected  at  the  point  d,  or  have  ad  equal  to  db  ;  and 
the  arc  abb  bisected  in  the  point  e,  or  have  ae  equal  bb. 

For,  having  drawn  ca,  cb,  as  before  :  Then,  in  the  tri- 
angle abc,  because  the  side  ca  is  equal  to  the  side  cb,  their 
opposite  angles  a  and  b  are  also  equal  (th.  3).  Hence  then, 
in  the  two  triangles  acd,  bcd,  the  angle  a  is  equal  to  the 
angle  b,  and  the  angles  at  d  are  equal  (def.  11) ;  therefore 
the  third  angles  are  also  equal  (corol.  1.  th.  17).  And 
having  the  side  cd  common,  they  have  also  the  side  ad  equal 
to  the  side  db  (th.  2). 

Also,  since  the  angle  ace  is  equal  to  the  angle  bob,  the 
arc  ae,  which  measures  the  former  (def.  57),  is  equal  to  the 
arc  be,  which  measures  the  latter,  since  equal  angles  must 
have  equal  measures. 

Corol.  Hence  a  line  bisecting  any  chord  at  right  angles, 
passes  through  the  centre  of  the  circle. 


THEOREM  XLII. 


If  more  than  two  equal  lines  oan  be  drawn  from  any 
point  within  a  circle  to  the  circumference,  that  point  will  bo 
the  centre. 

Let  abc  be  a  circle,  and  d  a  point 
within  it :  then  if  any  three  lines,  da, 
db,  dc,  drawn  from  the  point  d  to  the 
circumference,  be  equal  to  each  other, 
the  point  d  will  be  the  centre. 

Draw  the  chords  ab,  bc,  which  let 
be  bisected  in  the  points  e,  f,  and  join 
de,  df. 

Then,  the  two  triangles,  dak,  dbe, 
have  the  side  da  equal  to  the  side  db  by  supposition,  and 
the  side  ae  equal  to  the  side  eb  by  hypothesis,  also  the  side 
db  common  :  therefore  these  two  triangles  are  identical,  and 
have  the  angles  at  e  equal  to  each  other  (th.  5) ;  conse. 
quently  de  is  perpendicular  to  the  middle  of  the  chord  ab  . 
(def.  11),  and  therefore  passes  through  the  centre  of  the 
circle  (corol.  th.  41). 

In  like  manner,  it  may  be  shown  that  df  passes  through 
the  centre.  Consequently  the  point  d  is  the  centre  of  the 
circle,  and  the  three  equal  lines  da,  db,  dc,  are  radii. 

0» 

Vol.  1.  40 


306 


•KOMETRY. 


THEOREM  XLIII. 


If  two  circles  placed  one  within  another,  touch,  the  centre* 
of  the  circles  and  the  point  of  contact  will  be  all  in  the  same 
right  line. 

Let  the  two  circles  abc,  ade,  touch  one  A. 
anottier  internally  in  the  point  a  ;  then 
will  the  point  a  and  the  centres  of  those 
circles  be  all  in  the  same  right  line. 

Let  f  be  the  centre  of  the  circle  ahc, 
through  which  draw  the  diameter  afc. 
Then,  if  the  centre  of  the  other  circle  g 
can  be  out  of  this  line  ac,  let  it  be  sup- 
posed  in  some  other  point  as  o  ;  through  which  draw  the  line 
fis,  cutting  the  two  circles  in  b  and  d. 

Now  in  the  triangle  afg,  the  sum  of  the  two  sides  fgt 
ca,  is  greater  than  the  third  side  af  (th.  10),  or  greater  than 
its  equal  radius  fb.  From  each  of  these  take  away  the 
common  part  fg,  and  the  remainder  ga  will  be  greater 
than  the  remainder  gb.  But  the  point  g  being  supposed 
the  centre  of  the  inner  circle,  its  two  radii,  ga,  gd,  are  equal 
to  each  other  ;  consequently  od  will  also  be  greater  than  gb. 
But  ade  being  the  inner  circle,  gd  is  necessarily  less  than 
gb.  So  that  up  is  both  greater  and  less  than  gb  ;  which  is 
absurd.  Consequently  the  centre  o  cannot  be  out  of  the 
lino  afc.    q.  e.  n. 


THEOREM  XLIV. 


If  two  circles  touch  one  another  externally,  the  centres  of 
the  circles  and  the  point  of  contact  will  be  all  in  the  same 
right  line. 

Let  the  two  circles  ybc,  ape,  touch  one 
another  externally  at  the  point  \  :  then  will         /  ^ 
the  point  of  contact  a  and  the  centres  of  the         I  i 
two  circles  be  all  in  the  same  right  line.  \w  /I 

Let  f  be  the  centre  of  the  circle  aim:. 
through  which  draw  the  diameter  afc,  and  / 
produce  it  to  the  other  circle  at  e.  Then,  if  \ 


F 


*  -  -  —  ..v,   ...  . 

the  centre  of  the  other  circle  ade  can  be  out  \C 
ofyhc  line  fk,  let.  i(,  if  possible,  be  supposed 
in  some  other  point  as  g  ;  and  draw  the  lines 
a«:,  rune,  cutting  the  two  circles  in  b  and  d. 


./ 


THEOREMS. 


507 


Then,  in  the  triangle  afg,  the  sum  of  the  two  sides  af, 
ao,  is  greater  than  the  third  side  fg  (th.  10).  But,  f  and  o 
being  the  centres  of  the  two  circles,  the  two  radii  ga,  gd, 
•are  equal,  as  are  also  the  two  radii  af,  fb.  Hence  the  sura 
of  ga,  af,  is  equal  to  the  sum  of  ou,  bf  ;  and  therefore  this 
latter  sum  also,  od,  bf,  is  greater  than  gf,  which  is  absurd. 
Consequently  the  centre  o  cannot  be  out  of  the  line  ef. 

4.B.D. 


THEOREM  XLV. 

Asnc  chords  in  a  circle,  which  are  equally  distant  from 
the  centre,  are  equal  to  each  other  ;  or  if  they  be  equal  to 
each  other,  they  will  be  equally  distant  from  the  centre. 

Let  ab,  cd,  be  any  two  chords  at  equal  C 
distances  from  the  centre  g  ;  then  will  /7\A\ 
these  two  chords  ab,  cd,  be  equal  to  each       fcl  \  /  VpV 
other.  I  /   qT  \  J 

Draw  the  two  radii  ga,  gc,  and  the       V  V/ 
two  perpendiculars  ge,  of,  which  are  the      B  >s*_^>T3 
equal  distances  from  the  centre  g.  Then, 
the  two  right-angled  triangles,  gae,  gcf,  having  the  side  ga 
equal  the  side  gc,  and  the  side  ge  equal  the  side  gf,  and 
the  angle  at  e  equal  to  the  angle  at  f,  therefore  those  two 
triangles  are  identical  (cor.  2,  th.  34),  and  have  the  line 
ae  equal  to  the  line  cf.    But  ab  is  the  double  of  ae,  and 
cd  is  the  double  of  cf  (th.  41)  ;  therefore  ab  is  equal  to  cd 
(by  ax.  6).    u.  e.  d. 

Again,  if  the  chord  ab  be  equal  to  the  chord  cd  ;  then 
will  their  distances  from  the  centre,  ge,  gf,  also  be  equal 
to  each  other. 

For,  since  ab  is  [equal  cd  by  supposition,  the  half  ai:  is 
equal  the  half  cf.  Also  the  radii  ga,  gc,  being  equal,  as 
well  as  the  right  angles  e  and  f,  therefore  the  third  sides  are 
equal  (cor.  2,  th.  34),  or  the  distance  ge  equal  the  distance 
of.    a.  fi.  d. 


theorem  xlvi. 

A  line  perpendicular  to  the  extremity  of  a  radius^  va 
tangent  to  the  circAe. 


906 


•BOMBTBY. 


Let  the  line  adb  be  perpendicular  to  the 
radius  cd  of  a  circle ;  then  shall  ab  touch 
the  circle  in  the  point  d  only. 

From  any  other  point  s  in  the  line  ab 
draw  cfb  to  the  centre,  cutting  the  circle 
in  f. 

Then,  because  the  angle  d,  of  the  trian- 

51e  cde,  is  a  right  angle,  the  angle  at  e  is  acute  (cor.  3,  th. 
7),  and  consequently  less  than  the  angle  d.  But  the  greater 
side  is  always  opposite  to  the  greater  angle  (th.  9)  ;  there* 
fore  the  side  ce  is  greater  than  the  Bide  cd,  or  greater  than 
its  equal  cf.  Hence  the  point  e  is  without  the  circle  ;  and 
the  same  for  every  other  point  in  the  line  ab.  Consequently 
the  whole  line  is  without  the  circle,  and  meets  it  in  the  point 
d  only. 


J  THEOREM  XLVIZ. 

Whew  a  line  is  a  tangent  to  a  circle,  a  radius  drawn  to 
the  point  of  a  contact  is  perpendicular  to  the  tangent. 

Let  the  line  ab  touch  the  circumference  of  a  circle  at  the 
point  d  ;  then  will  the  radius  cd  be  the  perpendicular  to  the 
tangent  ab.    [See  the  last  figure.] 

For  the  line  ab  being  wholly  without  the  circumference 
except  at  the  point  d,  every  other  line,  as  ce,  drawn  from 
the  centre  c  to  the  line  ab,  must  pass  out  of  the  circle  to 
arrive  at  this  line.  The  line  cd  is  therefore  the  shortest  that 
can  be  drawn  from  the  point  c  to  the  line  ab,  and  conse- 
quently (th.  21)  it  is  perpendicular  to  that  line. 

Carol.  Hence,  conversely,  a  line  drawn  perpendicular  to 
a  tangent,  at  the  point  of  contact,  passes  through  the  centre 
of  the  circle. 

THEOREM  XLVIII. 

The  angle  formed  by  a  tangent  and  chord  is  measured  by 
half  the  arc  of  that  chord. 

Let  ab  be  a  tangent  to  a  circle,  and  cd  a  chord  drawn 
from  the  point  of  contact  c  ;  then  is  the  angle  bcd  measured 
by  half  the  arc  cfd,  and  the  angle  acd  measured  by  half  the 
arc  con. 

Draw  the  radius  ec  to  the  point  of  contact,  and  the  radios 
bf  perpendicular  to  the  chord  at  h. 


i 


THEOREMS.  809 

Then  the  radius  kf,  being  perpendicular 
to  the  chord  cd,  bisects  the  arc  cfd  (th. 
41 ).   Therefore  cf  is  half  the  arc  cfd. 

In  the  triangle  ceh ,  the  angle  h  being  a 
right  one,  the  sum  of  the  two  remaining 
angles  e  and  c  is  equal  to  a  right  angle  (cor. 
3,  th.  17),  which  is  equal  to  the  angle  bce, 
because  the  radius  ce  is  perpendicular  to 
the  tangent.  From  each  of  these  equals  take  the  common 
part  or  angle  c,  and  there  remains  the  angle  e  equal  to  the 
angle  bcd.  But  the  angle  b  is  measured  by  the  arc  cf  (def. 
57),  which  is  the  half  of  cfd  ;  therefore  the  equal  angle 
bcd  must  also  have  the  same  measure,  namely,  half  the 
arc  cfd  of  the  chord  cd. 

Again,  the  line  gef,  being  perpendicular  to  the  chord  cd, 
bisects  the  arc  cod  (th.  41).  Therefore  co  is  half  the  arc 
cod.  Now,  since  the  line  ce,  meeting  fo,  makes  the  sum 
of  the  two  angles  at  s  equal  to  two  right  angles  (th.  6),  and 
the  line  cd  makes  with  ab  the  sum  of  the  two  angles  at  c 
equal  to  two  right  angles  ;  if  from  these  two  equal  sums 
there  be  taken  away  the  parts  or  angles  ceh  and  bch, 
which  have  been  proved  equal,  there  remains  the  angle 
ceo  equal  to  the  angle  ach.  Rut  the  former  of  these, 
cfo,  being  an  angle  at  the  centre,  is  measured  by  the  are 
cg  (def.  57)  ;  consequently  the  equal  angle  acd  must  also 
have  the  same  measure  co,  which  is  half  the  arc  cod  of  the 
chord  CD.     Q.  E.  D. 

Carol.  1.  The  sum  of  two  right  angles  is  measured  by 
half  the  circumference.  For  the  two  angles  bcd,  acd, 
which  make  up. two  right  angles,  are  measured  by  the  arcs 
cf,  co,  which  make  up  half  the  circumference,  fo  being  a 
diameter. 

Carol.  2.  Hence  also  one  right  angle  must  have  for  its 
measure  a  quarter  of  the  circumference,  or  90  degrees. 


THE  OBEX  XLIX. 

Ah  angle  at  the  circumference  of  a  circle  is  measured  by  half 
the  arc  that  subtends  it. 


Let  bac  be  an  angle  at  the  circumference ;   3)    A  18 
it  has  for  its  measure,  half  the  arc  bc  which 
subtends  it. 

For,  suppose  the  tangent  db  passing 
through  the  point  of  contact  a  ;  then,  the 


3)    A.  IS 


GEOMETRY. 


angle  dac  being  measured  by  half  the  arc  arc,  and  the  angle 
dab  by  half  the  arc  ab  (th.  48)  ;  it  follows,  by  equal  tub. 
traction,  that  the  difference,  or  angle  bag,  must  be  measured 
by  half  the  arc  bc,  which  it  stands  upon.    a.  e.  d. 

THEOREM  L. 

All  angles  in  the  same  segment  of  a  circle,  or  standing  on 
the  same  arc,  are  equal  to  each  other. 

Let  c  and  d  be  two  angles  in  the  game 
segment  acdb,  or,  which  is  the  same  thing, 
standing  on  the  supplemental  arc  aeb  ;  then 
will  the  angle  c  be  equal  to  the  angle  d. 

For  each  of  these  angles  is  measured  by 
half  the  arc  aeb  ;  and  thus,  having  equal  B 
measures,  they  are  equal  to  each  other  (ax.  11). 


THEOREM  LI. 


An  angle  at  the  centre  of  a  circle  is  double  the  angle  at  the 
circumference,  when  both  stand  on  the  same  arc. 

Let  c  be  an  angle  at  the  centre  c,  and  d 
an  angle  at  the  circumference,  both  standing 
on  the  same  arc  or  same  chord  ab  :  then  will 
the  angle  c  bo  double  of  the  angle  i>,  or  the 
angle  d  equal  to  half  the  angle  c. 

For,  the  angle  at  the  centre  c  is  measured 
by  the  whole  arc  aeb  (def.  57),  and  the  angle  at  the  circum- 
ference d  is  measured  by  half  the  same  arc  aeb  (th.  49)  ; 
therefore  the  angle  d  is  only  half  the  angle  c,  or  the  angle  c 
doubles  the  angle  d. 


THEOREM  LII. 


An  angle  in  a  semicircle,  is  a  right  angle. 

If  abc  or  adc  be  a  semicircle  ;  then  any  D 
angle  d  in  that  semicircle,  is  a  right  angle. 

For,  the  angle  d,  at  the  circumference, 
is  measured  by  half  the  arc  abc  (th.  49), 
that  is,  by  a  quadrant  of  the  circumference. 
But  a  quadrant  is  the  measure  of  a  right 
angle  (cor.  4,  th.  6;  or  cor.  2,  th.  48). 
Therefore  the  angle  d  is  a  rigtit  angle. 


THE0REHS. 


311 


THEOREM  LIU. 

The  angle  formed  by  a  tangent  to  a  circle,  and  a  chord 
drawn  from  the  point  of  contact,  is  equal  to  the  angle  in  the 
alternate  segment. 

If  ab  be  a  tangent,  and  ac  a  chord,  and 
D  any  angle  in  the  alternate  segment  adc  ; 
then  will  the  angle  d  be  equal  to  the  angle 
bac  made  by  the  tangent  and  chord  of  the 
arc  a ec. 

For  the  angle  d,  at  the  circumference, 
is  measured  by  half  the  arc  aec  (th.  49) ; 
and  the  angle  bac,  made  by  the  tangent  and  chord,  is  also 
nfeasured  by  the  same1  half  arc  aec  (th.  48) ;  therefore  these 
two  angles  are  equal  (ax.  11). 

THEOREM  LIV. 

The  sum  of  any  two  opposite  angles  of  a  Quadrangle  in- 
scribed in  a  circle,  is  equal  to  two  right  angles. 

Let  abcd  be  any  quadrilateral  inscribed 
in  a  circle  ;  then  shall  the  sum  of  the  two 
opposite  angles  a  and  c,  or  u  and  d,  be  equal 
to  two  right  angles. 

For  the  angle  a  is  measured  by  half  the 
arc  dcb,  which  it  stands  on,  and  the  angle 
c  by  half  the  arc  dab  (th.  49)  ;  therefore 
the  sum  of  the  two  angles  a  and  c  is  measured  by  half  the 
sum  of  these  two  arcr.,  that  is,  by  half  the  circumference. 
But  half  the  circumference  is  the  measure  of  two  right  angles 
(cor*  4,  th.  G) ;  therefore  the  sum  of  the  two  opposite  angles 
a  and  c  is  equal  to  two  right  angles.  In  like  manner  it  is 
dhown,  that  the  sum  of  the  other  two  opposite  angles,  d  and 
B,  is  equal  to  two  right  angles,    u.  k.  d. 

THEOREM  LV. 

Ir  any  side  of  a  quadrangle,  inscribed  in  a  circle,  be  pro- 
duced out,  the  outward  angle  will  be  equal  to  the  inward 
opposite  angle. 

If  the  side  An,  of  the  quadrilateral 
abcd,  inscribed  in  a  circle,  be  produced 
to  e  ;  the  outward  angle  dak  will  bo  equal 
to  the  inward  opposite  angle  c. 


ns 


GEOMETRY. 


For,  the  mim  of  the  two  adjacent  angles  dab  and  dab  is 
equal  to  two  right  angles  (th.  6)  ;  and  the  sum  of  the  two 
opposite  angles  c  and  dab  iB  also  equal  to  two  right  angles 
(th.  54) ;  therefore  the  former  sum,  of  the  two  angles  dab 
and  dab,  is  equal  to  the  latter  Bum,  of  the  two  c  and  dab  (ax. 
1).  From  each  of  these  equate  taking  away  the  common 
angle  dab,  there  remains  the  angle  dab  equal  the  angle  c. 

Q.  E.  D. 


THEOREM  LVI. 


Awv  two  parallel  chords  intercept  equal  arcs. 

Let  the  two  chords  ab,  cd,  be  parallel : 
then  will  the  arcs  ac,  bd,  be  equal ;  or 

AC  =  BD. 

Draw  the  line  bc.  Then,  because  the 
lines  ae,  cd,  are  parallel,  the  alternate  an- 
gleB  b  and  c  are  equal  (th.  12}.  But  the 
angle  at  the  circumference  b,  is  measured  by  half  the  arc 
ac  (th.  49) ;  and  the  other  equal  angle  at  the  circumference 
c  is  measured  by  half  the  arc  bd  :  therefore  the  halves  of  the 
arcs  ac,  bd,  and  consequently  the  arcs  themselves,  are  also 
equal,    q.  e.  d. 


THEOREM  LVII. 


When  a  tangent  and  chord  are  parallel  to  each  other,  they 
intercept  equal  arcs. 

Let  the  tangent  abc  be  parallel  to  the 
chord  df  ;  then  are  the  arcs  bd,  bf,  equal ; 
that  is,  bd  =  bf. 

Draw  the  chord  bd.  Then,  because  the 
lines  ab,  df,  are  parallel,  the  alternate 
angles  d  and  b  are  equal  (th.  12).  But 
the  angle  b,  formed  by  a  tangent  and  chord,  is  measured  by 
half  the  arc  bd  (th.  48)  ;  and  the  other  angle  at  the  circum- 
ference d  is  measured  by  half  the  arc  bf  (th.  49) ;  therefore 
the  arcs  bd,  bf,  are  equal,    a.  e.  d. 


THBOBJUC8. 


313 


THEOREM  LVin. 


Tn  angle  formed,  within  a  circle,  by  the  intersection  of 
(wo  chords,  is  measured  by  half  the  sum  of  the  two  inter- 
cepted arcs.  * 

Let  the  two  chords  ab,  cd,  intersect  at 
the  point  e  :  then  the  angle  aec,  or  deb,  is 
measured  by  half  the  sum  of  the  two  arcs 

AC,  DB. 

Draw  the  chord  ap  parallel  to  cd.  Then 
because  the  lines  ap,  cd,  are  parallel,  and  ab 
cuts  them,  the  angles  on  the  same  side  a 
and  deb  are  equal  (th.  14).  But  the  angle  at  the  circumfer- 
ence a  is  measured  by  half  the  arc  bf,  or  of  the  sum  of  fd 
and  db  (th.  49) ;  therefore  the  angle  £  is  also  measured  by 
half  the  sum  of  fd  and  db* 

Again,  because  the  chords  af,  cd,  are  parallel,  the  arcs  acv 
fd,  are  equal  (th.  56) ;  therefore  the  sum  of  the  two  arcs  ac, 
db,  is  equal  to  the  sum  of  the  two  fd,  db  ;  and  consequently 
the  angle  e,  which  is  measured  by  half  the  latter  sum,  is  also 
measured  by  half  the  former,    q.  e.  d. 


theorem:  lix. 


The  angle  formed,  out  of  a  circle,  by  two  secants,  is  mea- 
sured by  half  the  difference  of  the  intercepted  arcs. 

Let  the  angle  e  be  formed  by  two  se- 
cants eab  and  ecd  ;  this  angle  is  measur- 
ed by  half  the  difference  of  the  two  arcs 
Ac,  db,  intercepted  by  the  two  secants. 

Draw  the  chord  af  parallel  to  cd.  Then, 
because  the  lines  af,  cd,  are  parallel,  and 
ab  cuts  them,  the  angles  on  the  same  side  a 
«nd  bed  are  equal  (th.  14).  But  the  angle  a,  at  the  circum- 
ference, is  measured  by  half  the  arc  bf  (th.  49),  or  of  the 
difference  of  df  and  db  :  therefore  the  equal  angle  b  is  also 
measured  by  half  the  difference  of  df,  db. 

Again,  because  the  chords,  af,  cd,  are  parallel,  the  arcs 
ac,  fd,  are  equal  (th.  56) ;  therefore  the  diffettfic*  ot  ^* 

Vol.  I.  41 


314 


GEOMETRY. 


two  arcs  AC)  db,  is  equal  to  the  difference  of  the  two  »r,  db. 
Consequently  the  angle  e,  which  is  measured  by  half  the 
latter  difference,  is  also  measured  by  half  the  former. 

q.  e.  d. 


THEOREM  LX. 


The  angle  formed  by  two  tangents,  is  measured  by  half  the 
difference  of  the  two  intercepted  arcs. 

Let  eb,  ed,  be  two  tangents  to  a  circle 
at  the  points  a,  c;  then  the  angle  e  is 
measured  by  half  the  difference  of  the  two 

arcs  CFA,  CGA. 

Draw  the  chord  af  parallel  to  ed. 
Then,  because  the  lines,  af,  ed,  are  pa- 
rallel,  and  eb  meets  them,  the  angles  on 
the  same  side  a  and  e  are  equal  (th.  14). 
But  the  angle  a,  formed  by  the  chord  af  and  tangent  ab, 
is  measured  by  half  the  arc  af  (th.  48) ;  therefore  the  equal 
angle  e  is  also  measured  by  half  the  same  arc  af,  or  half  the 
difference  of  the  arcs  cfa  and  cf,  or  cga  (th.  57). 


Carol.  In  like  manner  it  is  proved,  that 
the  angle  e,  formed  by  a  tangent  ecd, 
and  a  secant  eab,  is  measured  by  half 
the  difference  of  the  two  intercepted  arcs 
ca  and  cfb. 


theorem  lxi. 


When  two  lines,  meeting  a  circle  each  in  two  points,  cut 
one  another,  either  within  it  or  without  it;  the  rectangle 
of  the  parts  of  the  one,  is  equal  to  the  rectangle  of  the 
parts  of  the  other ;  the  parts  of  each  being  measured  from 
the  point  of  meeting  to  the  two  intersections  with  the  cir- 
cumference. 


THEOREMS. 


815 


Let  the  two  lines  ab,  cd,  meet  each 
trther  in  e  ;  then  the  rectangle  of  ae,  eb, 
will  be  equal  to  the  rectangle  of  ce,  ed. 

Or,  AE  .  EB  =  CE  .  ED. 

For,  through  the  point  e  draw  the  dia- 
meter fo  ;  also,  from  the  centre  h  draw 
the  radius  dh,  and  draw  hi  perpendicular 
to  CD. 

Then,  since  dbh  is  a  triangle,  and  the 
perp.  hi  bisects  the  chord  cd  (th.  41),  the 
line  cb  is  equal  to  the  difference  of  the 
segments  di,  ei,  the  sum  of  them  being 
be.  Also,  because  h  is  the  centre  of  the 
circle,  and  the  radii  dh,  fh,  oh,  are  all  equal,  the  line  eg 
is  equal  to  the  sum  of  the  sides  dh,  he  ;  and  ef  is  equal  to 
their  difference. 

But  the  rectangle  of  the  sum  and  difference  of  the  two 
sides  of  a  triangle  is  equal  to  the  rectangle  of  the  sum  and 
difference  of  the  segments  of  the  base  (th.  35) ;  therefore 
the  rectangle  of  fe,  eo,  is  equal  to  the  rectangle  of  ce,  ed. 
In  like  manner  it  is  proved,  that  the  same  rectangle  of  fe, 
eg,  is  equal  to  the  rectangle  of  ae,  eb.  Consequently  the 
rectangle  of  ae,  eb,  is  also  equal  to  the  rectangle  of  ce,  ed 
(ax.  1).    Q.  E.  D. 

Coral.  1.  When  one  of  the  lines)  in  the 
second  case,  as  de,  by  revolving  about  the 
point  e,  comes  into  the  position  of  the  tan- 
gent ec  or  ed,  the  two  points  c  and  d  run- 
ning into  one ;  then  the  rectangle  of  ce,  ed, 
becomes  the  square  of  ce,  because  ce  and  de 
are  then  equal.  Consequently  the  rectangle 
of  the  parts  of  the  secant,  ae  .  eb,  is  equal 
to  the  square  of  the  tangent,  ce9. 

Carol.  2.  Hence  both  the  tangents  ec,  ef,  drawn  from 
the  same  point  e,  are  equal ;  since  the  square  of  each  is  equal 
tolhe  same  rectangle  or  quantity  ae  •  eb. 


THEOREM  LXII. 

In  equiangular  triangles,  the  rectangles  of  the  corresponding 
or  like  sides,  taken  alternately,  are  equal. 


816 


GKOVETMT. 


Let  abc,  dbf,  be  two  equiangular 
triangles,  having  the  angle  a  =  the 
angle  d,  the  angle  b  =  the  angle  e, 
and  the  angle  c  =  (he  angle  f  ;  also 
the  like  si-les  ab,  de,  and  ac,  df,  be- 
ing those  opposite  the  equal  angles  : 
then  will  the  rectangle  of  ab,  df,  be 
equal  to  the  rectangle  of  ao,  de. 

In  ba  produced  take  ag  equal  to  or ;  and  through  the 
three  points  b,  c,  g,  conceive  a  circle  bcoh  to  be  described, 
meeting  ca  produced  at  h,  and  join  oh. 

Then  the  angle  o  is  equal  to  the  angle  c  on  the  same  arc 
bh,  and  the  angle  h  equal  to  the  angle  b  on  the  same  arc 
co  (th.  50) ;  also  the  opposite  angles  at  a  are  equal  (th.  7)  : 
therefore  the  triangle  agh  is  equiangular  to  the  triangle 
acb,  and  consequently  to  the  triangle  dfb  also.  But  the 
two  like  sides  ao,  df,  are  also  equal  by  supposition  ;  conse- 
quently the  two  triangles  aoh,  dfk,  are  identical  (th.  2), 
having  the  two  sides  ao,  ah,  equal  to  the  two  df,  de,  each 
to  each. 

But  the  rectangle  ga  .  ab  is  equal  to  the  rectangle  ha  •  ac 
(th.  61)  :  consequently  the  rectangle  df  .  ab  is  equal  to  the 
rectangle  de  .  ac.    a.  e.  d. 


THEOREM  LXI1I. 


The  rectangle  of  the  two  sides  of  any  triangle,  is  equal 
to  the  rectangle  of  the  perpendicular  on  the  third  side  and 
the  diameter  of  the  circumscribing  circle. 

Let  cd  be  the  perpendicular,  and  ce 
the  diameter  of  the  circle  about  the  triangle 
abc  ;  then  the  rectangle  ca  .  cb  is  =  the 
rectangle  cd  •  ce. 

For,  join  be  :  then  in  the  two  triangles 
acd,  ecb,  the  angles  a  and  e  are  equal, 
standing  on  the  same  arc  bc  (th.  50)  ;  also 
the  right  angle  d  is  equal  the  angle  b,  which  is  also  a  right 
angle,  being  in  a  semicircle  (th.  52)  :  therefore  these  two 
triangles  have  also  their  third  angles  equal,  and  are  equian- 
gular. Hence,  ac,  ce,  and  cd,  cb,  being  like  sides,  nib- 
tending  the  equal  angles,  the  rectangle  ac  .  cb.  of  the  first 
and  last  of  them,  is  equal  to  the  rectangle  ce  .  cd,  of  the 
other  two  (th.  62). 


THEOREMS. 


317 


THEOREM  LXIV. 

The  square  of  a  line  bisecting  any  angle  of  a  triangle, 
together  with  the  rectangle  of  the  two  segments  of  the  oppo- 
site side,  is  equal  to  the  rectangle  of  the  two  other  sides  in- 
cluding the  bisected  angle. 


Let  cd  bisect  the  angle  c  of  the  triangle 
abc  ;  then  the  square  cd9  +  the  rectangle 
ad  .  db  is  =  the  rectangle  ac  .  cb. 

For,  let  cd  be  produced  to  meet  the  cir- 
cumscribing circle  at  e,  and  join  ae. 


Then  the  two  triangles  ace,  bcd,  are 
equiangular  :  for  the  angles  at  c  are  equal 
by  supposition,  and  the  angles  b  and  e  are  equal,  standing 
on  the  same  arc  ac  (th.  50)  ;  consequently  the  third  angles 
at  a  and  Dare  equal  (cor.  1,  th.  17)  :  also  ac,  cd,  and  ce, 
cb,  are  like  or  corresponding  sides,  being  opposite  to  equal 
angles  :  therefore  the  rectangle  ac  .  cb  is  =  the  rectangle 
cd  .  ce  (th.  62).  But  the  latter  rectangle  cd  .  ce  is  =  cd*  + 
the  rectangle  cd  .  de  (th.  30)  ;  therefore  the  former  rect- 
angle ac  .  cb  is  also  =  cd3  +  cd  .  de,  or  equal  to  cd2  + 
ad  .  db,  since  cd  .  de  is  =  ad  •  db  (th.  61).    a.  e.  d. 


theorem  lxv. 

The  rectangle  of  the  two  diagonals  of  any  quadrangle 
inscribed  in  a  circle,  is  equal  to  the  sum  of  the  two  rect- 
angles of  the  opposite  sides. 

Let  abcd  be  any  quadrilateral  inscribed 
in  a  circle,  and  ac,  bd,  its  two  diagonals  : 
then  the  rectangle  ac  .  bd  is  =  the  rect- 
angle ab  .  dc  +  the  rectangle  ad  .  sc. 

For,  let  ce  be  drawn,  making  the  angle 
bce  equal  to  the  angle  dca.  Then  the  two 
triangles  acd,  bce,  are  equiangular  ;  for 
the  angles  a  and  b  are  equal,  standing  on  the  same  arc  dc  ; 
and  the  angles  dca,  bce,  are  equal  by  supposition  ;  conse- 
quently the  third  angles  adc,  bec,  are  also  equal :  also,  ac, 
bc,  and  ad,  .be,  are  like  or  corresponding  sides,  being  oppo- 
site to  the  equal  angles  :  therefore  the  rectangle  ac  .  be  it 

the  rectangle  ad  .  bc  (th.  62). 


318 


GEOMETRY* 


Again,  the  two  triangles  abc,  dec,  are  equiangular :  for 
the  angles  bac,  bdc,  are  equal,  standing  on  the  same  arc  bc  ; 
and  the  angle  dce  is  equal  to  the  anglo  bca,  by  adding  the 
common  angle  ace  to  the  two  equal  angles  dca,  bce  ;  there- 
fore  the  third  angles  e  and  abc  are  also  equal :  but  ac,  dc, 
and  ab,  de,  are  the  like  sides :  therefore  the  rectangle  AC  . 
de  is  =  the  rectangle  ab  .  dc  (th.  62). 

Hence,  by  equal  additions,  the  sum  of  the  rectangles 
ac  .  be  +  ac  .  de  is  =  ad  .  bo  +  ab  .  dc.  Hut  the  for- 
mer sura  of  the  rectangles  ac  .  be  +  ac  .  de  is  =  the  rect- 
angle ac  .  bd  (th.  30) :  therefore  the  same  rectangle  ac  • 
bd  is  equal  to  the  latter  sum,  the  rect.  ad  .  bc  +  the  rect. 
ab  .  dc  (ax.  1).    Q.  E.  D. 

CoroL  Hence,  if  abd  be  an  equilateral  triangle,  and  c 
any  point  in  the  arc  bcd  of  the  circumscribing  circle,  we  have 
ac  =  bc  +  dc.  For  ac  .  bd  being  =  ad  .  bc  +  ab  -  dc  ; 
dividing  by  bd  ==  ab  =  ad,  there  results  ac  =  bc  +  dc* 


OF  RATIOS  AND  PROPORTIONS. 


DEFINITIONS. 

Dep.  76.  Ratio  is  the  proportion  or  relation  which  one 
magnitude  bears  to  another  magnitude  of  the  same  kind, 
with  respect  to  quantity. 

Note*  The  measure,  or  quantity,  of  a  ratio,  is  conceived, 
by  considering  what  part  or  parts  the  leading  quantity,  called 
the  Antecedent,  is  of  the  other,  called  the  Consequent ;  or 
what  part  or  parts  the  number  expressing  the  quantity  of  the 
former,  is  of  the  number  denoting  in  like  manner  the  latter. 
So,  the  ratio  of  a  quantity  expressed  by  the  number  2,  to  a 
like  quantity  expressed  by  the  number  6,  is  denoted  by  2 
divided  by  6,  or  |  or  £ :  the  number  2  being  3  times  con- 
tained in  6,  or  the  third  part  of  it.  In  like  manner,  the  ratio 
of  the  quantity  3  to  0,  is  measured  by  £  or  £  ;  the  ratio  of 
4  to  6  is  }  or  |;  that  of  6  to  4  is  $  or  £  ;  &c. 

77.  Proportion  is  an  equality  of  ratios.  Thus, 

78.  Three  quantities  are  said  to  be  proportional,  when  the 
ratio  of  the  first  to  the  second  is  equal  to  the  ratio  of  the 


THEOREMS. 


319 


second  to  the  third.    As  of  the  three  quantities  a  (2),  b  (4), 
c  (8),  where  $==1  =  1,  hoth  the  same  ratio. 

79.  Four  quantities  are  said  to  be  proportional,  when  the 
ratio  of  the  first  to  the  second,  is  the  same  as  the  ratio  of  the 
third  to  the  fourth.  As  of  the  four,  a  (4),  n  (2),  c  (10),  o  (5), 
where  a  =  y>  =  2,  both  the  same  ratio. 

Note*  To  denote  that  four  quantities,  a,  b,  c,  d,  are  pro* 
portional,  they  are  usually  stated  or  placed  thus,  a  :  b  : :  c  :  d; 
and  read  thus,  a  is  to  b  as  c  is  to  d.  But  when  three  quan- 
tities are  proportional,  the  middle  one  is  repeated,  and  they 
are  written  thus,  a  :  b  :  :  b  :  c. 

The  proportionality  of  quantities  may  also  be  expressed 
very  generally  by  the  equality  of  fractions,  as  at  pa.  118. 

Thus,  if  -  =     then  a  :  b  :  :  c  :  d,  also  b  :  a  :  r  c  :  p,  and 

B  D 

A  :  o  :  :  b  :  d,  and  c :  a  : :  b  :  d. 

80.  Of  three  proportional  quantities,  the  middle  one  is 
said  to  be  a  Mean  Proportional  between  the  other  two  ;  and 
the  last,  a  Third  Proportional  to  the  first  and  second. 

81.  Of  four  proportional  quantities,  the  last  is  said  to  be 
a  Fourth  Proportional  to  the  other  three,  taken  in  order. 

82.  Quantities  are  said  to  be  Continually  Proportional,  or 
in  Continued  Proportion,  when  the  ratio  is  the  same  between 
every  two  adjacent  terms,  viz.  when  the  first  is  to  the  second, 
as  the  second  to  the  third,  as  the  third  to  the  fourth,  as  the 
fourth  to  the  fifth,  and  so  on,  all  in  the  same  common  ratio. 

As  in  the  quantities  1,  2,  4,  8,  16,  &c. ;  where  the  com- 
mon ratio  is  equal  to  2. 

83.  Of  any  number  of  quantities,  a,  b,  c,  d,  the  ratio  of 
the  first  a,  to  the  last  d,  is  said  to  be  Compounded  of  the 
ratios  of  the  first  to  the  second,  of  the  second  to  the  third, 
and  so  on  to  the  last. 

84.  Inverse  ratio  is,  when  the  antecedent  is  made  the 
consequent,  and  the  consequent  the  antecedent. — Thus,  if 
1  :  2  :  :  3  :  6  ;  then  inversely,  2  :  1  :  :  6  :  3. 

85.  Alternate  proportion  is,  when  antecedent  is  compared 
with  antecedent,  and  consequent  with  consequent. — As,  if 
1  :  2  :  :  3  :  6  ;  then,  by  alternation,  or  permutation,  it  will  be 
1  :  3  :  :  2  :  6. 

86.  Compound  ratio  is,  when  the  sum  of  the  antecedent 
and  consequent  is  compared,  either  with  the  to\u&qp£feV>  « 


820 


GEOMETRY* 


with  the  antecedent.— Thus,  if  1  :  2  : :  3  :  6,  then  by  com- 
position,  l+2:l::3  +  6:3,  an(]  1  -f  2  :  2  : :  3  + 
6  :  6. 

87.  Divided  ratio,  is  when  the  difference  of  the  antecedent 
and  consequent  is  compared,  either  with  the  antecedent  or 
with  the  consequent. — Thus,  if  1  :  2  : :  3  :  6,  then,  by  di- 
vision, 2  —  1:1  : :  6—  3  :  3,  and  2  —  1  :  2  : :  6  —  3:6. 

Nate.  The  term-Divided,  or  Division,  here  means  subtract, 
ing,  or  parting ;  being  used  in  the  sense  opposed  to  com- 
pounding, or  adding,  in  def.  86. 

THEOREM  LXVI. 

Equimultiples  of  any  two  quantities  have  the  same  ratio  as 
the  quantities  themselves. 

Let  a  and  b  be  any  two  quantities,  and  m\,  j»b,  any  equi- 
multiples of  them,  m  being  any  number  whatever :  then  will 
wia  and  mB  have  the  same  ratio  as  a  and  b,  or  a  :  b  :  :  jra  : 

fllB. 

mB      b  . 
For  —  =  -,  the  same  ratio. 

HIA  A 

Cord.  Hence,  like  parts  of  quantities  have  the  same  ratio 
as  the  wholes  ;  because  the  wholes  are  equimultiples  of  the 
like  parts,  or  a  and  r  are  like  parts  of  ma  and  ms. 

THEOREM  LXVII. 

If  four  quantities,  of  the  same  kind,  be  proportionals ; 
they  will  be  in  proportion  by  alternation  or  permutation, 
or  the  antecedents  will  have  the  same  ratio  as  the  conse- 
quents*. 


*  The  author's  object  in  these  propositions  was  to  simplify  the  doc- 
trine of  ratios  and  proportions,  by  imagining  that  the  antecedents  and 
consequences  may  always  be  divided  into  parts  that  are  commensura- 
ble. But  it  is  known  to  mathematicians  that  there  are  certain  quantities 
or  magnitudes,  such  as  the  side  and  the  diagonal  of  a  square,  which 
cannot  possibly  be  divided  in  that  manner  by  means  of  a  common  mf* 
sure.  The  theorems  themselves  are  true,  nevertheless,  when  applied  to 
these  incommensurabUs ;  since  no  two  quantities  of  the  same  kind  can 
possibly  be  assigned,  whose  ratio  cannot  be  expressed  by  that  of  two 
numbers,  so  near,  that  the  difference  shall  be  less  than  the  least  number 
that  can  be  named.  From  the  greater  of  two  unequal  magnitudes  we 
may  take,  or  suppose  taken,  its  Hoify  from  the  remaining  half,  its  half, 


THEOREMS.  821 

Let  a  :  b  : :  uiA  :  »iB ;  then  will  a  :  wia  : :  b  :  jrb. 

For  —  =  —i  and  — -  =  ~>  both  the  same  ratio. 
a       1  b  1 


and  so  on,  by  continual  bisections,  until  there  shall  at  length  be  left  a 
magnitude  less  than  the  least  of  two  magnitudes ;  or.  indeed,  less  than 
the  least  magnitude  that  can  be  assigued ;  and  this  principle  furnishes  a 
ground  of  reasoning. 

Or,  somewhat  differently,  let  a  and  b  be  two  constant  quantities,  a 
and  b  two  variable  quantities,  which  we  can  render  as  small  as  we 
please,  if  we  have  an  equality  between  i-j-fl,  and  b  -}-  6,  or,  in  other 
words,  if  the  equation  a+o  =  b-|-6  holds  good  whatever  are  the  va- 
lues of  a  and  6,  it  may  be  divided  into  two  others,  a  =  b,  between  the 
constant  quantities,  and,  a  =  bt  between  the  variable  quantities,  and 
which  latter  must  obtain  for  all  their  states  of  magnitude.  For  if,  on 
the  contrary,  we  suppose  a  =  b  ^  q,  we  shall  have  I  —  b  =  6  —  a  = 
q,  an  absurd  result ;  since  the  quantities  a  and  6  being  susceptible  of 
diminishing  indefinitely*  their  difference  cannot  always  be  =  q.  This 
is  the  principle  which  constitutes  the  method  of  limits.  In  general,  one 
magnitude  is  called  a  limit  of  another,  tchen  we  can  make  this  latter  ap- 
proach so  near  to  the  former,  that  their  difference  shall  be  less  than  any  given 
magnitude*  and  yet  so  that  the  two  magnitudes  shall  never  become  strictly 
equal. 

Let  us  here  apply  the  principle  to  the  demonstration  of  this  proposi- 
tion, that  the  ratio  of  two  angles  acb,  nop,  is  equal  to  that  of  the  arcs, 
o6,  np,  comprised  between  their  sides,  and  drawn  from  their  respective 
summits  as  centres  with  equal  radii. 

If  the  'arcs  pnf  ba,  are 
commensurable,  their 
common  measure  6m 
will  be  contained  n 
times  in  iro,  r  times  in 
ba ;  so  that  we  shall  - 
have  the  equal  ratios 

¥L  =  -.  Through  each 
6a  r 

point  of  division,  m,  n',  <fcc.  draw  the  lines  mc,  n'c,  &c.  to  the  summits 
c,  and  o,  the  angles  proposed  will  be  divided  into  n,  and  r,  equal  angles, 

6cm,  men',  poq,  qor,  be.   We  shall,  therefore,  have       =  *.  Hence 
'         r  '  boa  r 

is  =?—,  since  each  of  tbem  is  equal  to  the  ratio  -. 
bca        6a  r 

If  the  arcs  are  incommensurable,  divide  one  of  them,  6a,  into  a  num- 
ber r  of  equal  parts,  6m,  mn',  be.  and  set  off  equal  parts  pq,  qr}  &c.  upon 
the  other  arc pn;  and  let  s  be  the  point  of  division  that  falls  nearest  to  n. 
Draw  oss.   Then,  by  the  preceding,  6a,  ps,  being  commensurable,  we 

shall  have  ?—  =      the  angle  pos  =  pon  +  iros,  arc  ps  =  pn  +  ns. 
bca  ba 

Therefore, 

pon      ifos      pn_  ns 
bca      bca  ~  ba  ba' 
Here  nos  and  ns  are  susceptible  of  indefinite  variation,  according  as 
we  change  the  common  measure,  6m,  of  6a ;  they  may,  therefore,  ba 
Vol.  I.  42 


832  GEOMETRY. 

Otherwise.    Let  a  :  b  :  :  c  :  d  ;  then  shall  b  r  a  : 

A  C 

For,  let  -  =  -  =  r ;  then  a  =  bt,  and  c  =  dt  :  there- 

B  D 


fore  b 


A,  CTT         bI.d  1 

-,  and  d  =■  -.    Hence  -  =      and  -  =  — , 


B  D 

'  Whence  it  is  evident  that  —  =  —  (ax.  1),  or  b  :  a  :  :  d  :  c» 

A  C  ' 

In  a  similar  manner  may  most  of  the  other  theorems  he 
demonstrated. 

THEOREM  LXTUI. 

If  four  quantities  be  proportional ;  they  will  be  in  proportion 
by  inversion,  or  inversely. 

Let  a  :  b  :  :  ira  :  ms ;  then  will  b  :  a  :  :  mB  :  ma. 

For  —  =  — ,  both  the  same  ratio. 
mB  b 

THEOREM  LXIX. 

If  four  quantities  be  proportional ;  they  will  be  in  proportion 
by  composition  and  division. 

Let  a  :  b  :  :  mx  :  mB  ;  1 
Then  will  b  ±  a  :  a  :  :  ms  ±  mx  :  mx, 
and  b  ±  a  :  b  :  :  kb  dfc  mx  :  mB. 
_  mx  A  ,       f»B  B 

For  —  =*  — — ;  and  —  =  — — . 

«iB  rb  m\     b±a         mB±.m\     b  rb  a 

Carol.  It  appears  from  hence,  that  the  sum  of  the  greatest 
and  least  of  four  proportional  quantities,  of  the  same  kind, 
exceeds  the  sum  of  the  other  two.  For,  since  .  -  -  - 
a  :  a  +  b  :  :  m\  :  mx  +  ms,  where  a  is  the  least,  and 
fflA  +  «»b  the  greatest ;  then  m  +  1  .  a  +  «b,  the  sum  of 
the  greatest  and  least,  exceeds  m  +  1  .  a  +  b,  the  sum  of 
the  two  other  quantities. 

THEOREM  JLXX. 

If,  of  four  proportional  quantities,  there  be  taken  any 
equimultiples  whatever  of  the  two  antecedents,  and  any  equi- 

rendered  as  small  as  we  please,  while  the  other  quantities  remain  the 
same.  Consequently,  by  the  nature  of  limits,  as  above  explained,  we 

have  the  equal  ratios  -~  =      or  for  :  bac  ::pn:  ba. 

bca      oa  r 


THEOREMS.  323 

multiples  whatever  of  the  two  consequents ;  the  quantities 
resulting  will  still  be  proportional. 

Let  a  :  b  :  :  «a  :  wib  ;  also,  let  pA  and  pmA  be  any 
equimultiples  of  the  two  antecedents,  and  qs  and  qmB  any 
equimultiples  of  the  two  consequents ;  then  will  .... 
px  :  qB  :  :  pmA  :  qmB. 

For  VOIL  =  2?  both  the  same  ratio. 
pmA  pA 

■  t 

THEOREM  LXXI. 

If  there  be  four  proportional  quantities,  and  the  two  con- 
sequents be  either  augmented  or  diminished  by  quantities 
that  have  the  same  ratio  as  the  respective  antecedents ;  the 
results  and  the  antecedents  will  still  be  proportionals. 

Let  a  :  b  :  :  wa  :  mn,  and  n\  and  nmA  any  two  quan- 
tities having  the  same  ratio  as  the  two  antecedents ;  then  will 
a  :  b  ±  nA     mA  :  ms  ±  nmA. 

„    mi*  ±  nmA     b  ±  tia  , 

For  =  ,  -both  the  same  ratio. 

IRA  A 

THEOREM  LXXII. 

If  any  number  of  quantities  be  proportional,  then  any 
one  of  the  antecedents  will  be  to  its  consequent,  as  the 
sum  of  all  the  antecedents,  is  to  the  sum  of  all  the  conse- 
quents.    ^  * 

Let  a  :  b  :  :  mA  :  wib  :  :  tiA  :  ub,  &c.  ;  then  will  -  -  . 
a  :  b  :  :  a  +  wa  +  iia  :  b  +  mB  +  iib,  &c.  ' 

B+ma+itB      (l+ro+n)B      b  , 

For   :  =  77-;  ; — r~  =  — ,  the  same  ratio. 

A+roA+ftA      (l+m+n)A  A 


THEOREM  LXXHI. 


If  a  whole  magnitude  be  to  a  whole,  as  a  part  taken  from 
the  first,  is  to  a  part  taken  from  the  other  ;  then  the  re- 
mainder will  be  to  the  remainder,  as  the  whole  to  the 
whole. 


Let  a  :  b  :  : 


then  will  a  b  ; ;  a  a  :  b  b. 

n  % 


324 


GEOMETRY. 


m 

B—  —  B 

For  as  — ,  both  the  same  ratio. 

m  a 

A  —   A 

theorem:  lxxiv. 

If  any  quantities  be  proportional  ;  their  squares,  or  cubes, 
or  any  like  powers,  or  roots,  of  them,  will  also  be  propor- 
tional. 

Let  a  :  b  :  :  i?ia  :  i?ib  ;  then  will  a*  :  b*'  :  :  mnAn  :  m*B". 

_    mnBn     b»  .    .  . 
r  or  — — -  =  — ,  both  the  same  ratio. 
ro*Aw  a" 

See  also,  th.  vni.  pa,  118. 

THEOREM  LXXV. 

If  there  be  two  sets  of  proportionals  ;  then  the  products 
or  rectangles  of  the  corresponding  terms  will  also  be  pro- 
portional. 

Let  a  :  b  :  :  wa  :  mB, 

and  c  :  d  :  :  nc  :  hd  ; 

then  will  ac  :  bd  :  :  mnAC  :  uitibd. 

mnBD      bd  .    ,  . 
ror  =  — ,  both  the  same  ratio. 

fflttAC  AC 

THEOREM  LXXVI. 

If  four  quantities  be  proportional ;  the  rectangle  or  pro- 
duct of  the  two  extremes,  will  be  equal  to  the  rectangle  or 
product  of  the  two  means.    And  the  converse. 

Let  a  :  b  :  :  ota  :  ms  ; 
then  is  a  X  wb  =  b  Xj»a  =  hiae,  as  is  evident. 

THEOREM  LXXVII. 

If  three  quantities  be  continued  proportionals  ;  the  rect- 
angle or  product  of  the  two  extremes,  will  be  equal  to  the 
square  of  the  mean.    And  the  converse. 

Let  a,  «a,  m9A  be  three  proportionals, 
or  a  :  tfiA  :  :  mA  ;  maA  ; 
then  is  a  X  vp?k  =*  mV,  a»  \*  owtaciSi. 


THEOREMS. 


325 


THEOREM  LXXVI11. 

If  any  number  of  quantities  be  continued  proportionals 
the  ratio  of  the  first  to  the  third,  will  be  duplicate  or  the 
square  of  the  ratio  of  the  first  and  second  ;  and  the  ratio  of 
the  first  and  fourth  will  be  triplicate  or  the  cube  of  that  of 
the  first  and  second ;  and  so  on. 
'  Let  a,  mA,  jti'a,  jti3a,  dec.  be  proportionals  ; 

then  is  —  =  — ;  but  -4-  =  —7  ;  and  -4-  =  \  ;  dtc. 
mA     m       maA     mr          wta  mr 

THEOREM  LXXIX. 

Triangles,  and  also  parallelograms,  having  equal  altitudes, 
are  to  each  other  as  their  bases. 

Let  the  two  triangles  adc,  def,  have  I  CK. 
the  same  altitude,  or  be  between  the  same 
parallels  ae,  ce  ;  then  is  the  surface  of 
the  triangle  adc,  to  the  surface  of  the 
triangle  def,  as  the  base  ad  is  to  the  AB  BOH  is 
base  de.  Or,  ad  :  de  :  :  the  triangle 
adc  :  the  triangle  def. 

For,  let  the  base  ad  be  to  the  base  de,  as  any  one  num- 
ber m  (2),  to  any  other  number  n  (3) ;  and  divide  the 
respective  bases  into  those  parts,  ab,  bd,  do,  gm,  he,  all 
equal  to  one  another ;  and  from  the  points  of  division  draw 
the  lines  bc,  fg,  fh,  to  the  vertices  c  and  f.  Then  will 
these  lines  divide  the  triangles  adc,  dkf,  into  the  same 
number  of  parts  as  their  bases,  each  equal  to  the  triangle 
abc,  because  those  triangular  parts  have  equal  bases  and 
altitude  (cor.  2,  th.  25) ;  namely,  the  triangle  abc  equal  to 
each  of  the  triangles  bdc,  dfg,  gfh,  hfe.  So  that  the  tri- 
angle adc,  is  to  the  triangle  dfe,  as  the  number  of  parts  m 
(2)  of  the  former,  to  the  number  n  (3)  of  the  latter,  that  is, 
as  the  base  ad  to  the  base  de  (def.  79)*. 

In  like  manner,  the  parallelogram  adki  is  to  tho  parallelo- 
gram defk,  as  the  base  ad  is  to  the  base  de  ;  each  of  these 
having  the  same  ratio  as  the  number  of  their  parts,  m  to  ft* 

Q.  E.  D. 


*  If  the  bases  ad,  de,  of  two  triangles  that  have  a  common  ^%t\VL%, 
aire  incommensurable  to  each  other,  the  ratio  of  tto  trvi&tjto Ha* wjM^ 
gUnd'wg,  equal  to  that  of  their  bases. 


926 


GEOMETRY* 


THEOREM  LXXX. 

Triangles,  and  also  parallelograms  having  equal  bases,  are 
to  each  other  as  their  altitudes. 


Let  abc,  bep,  be  two  triangles 
having  the  equal  bases  ab,  be,  and 
whose  altitudes  are  the  perpendicu- 
lars co,  fh  ;  then  will  the  triangle 
abc  :  the  triangle  bef  :  :  co  :  fh. 

For,  let  bk  be  perpendicular  to 


ab,  and  equal  to  cg  ;  in  which  let 
there  be  taken  bl  =  fh  ;  drawing  ak  and  al. 

Then  triangles  of  equal  bases  and  heights  being  equal 
(cor.  2,  th.  25),  the  triangle  abk  is  =  abc,  and  the  triangle 
abl  =  bef.  But,  considering  now  abk,  abl,  as  two  tri- 
angles on  the  bases  bk,  bl,  and  having  the  same  altitude  ab, 
these  will  be  as  their  bases  (th.  79),  namely,  the  triangle 
abk  :  the  triangle  abl  :  :  bk  :  :  bl. 

But  the  triangle  abk  =  *abo,  and  the  triangle  abl  =  bef, 

also  bk  =  cg,  and  bl  =  fh. 
Theref.  the  triangle  abc  :  triangle  bef  : :  cg  :  fh. 

And  since  parallelograms  are  the  doubles  of  these  triangles, 
having  the  same  bases  and  altitudes,  they  will  likewise  have 
to  each  other  the  same  ratio  as  their  altitudes,    q.  e.  d. 

Corel.  Since,  by  this  theorem,  triangles  and  parallelo- 
grams, when  their  bases  are  equal,  arc  to  each  other  as  their 
altitudes;  and  by  the  foregoing  one,  when  their  altitudes  are 
equal,  they  are  to  each  other  as  their  bases ;  therefore  uni- 


For,  first,  if  possible,  let  the  triangle  kcd 
be  to  the  triangle  acd,  not  as  ed  to  ad,  but 
as  some  other  line  bd  greater  than  ed,  is  to 

AD. 

Let  ah  be  a  part,  or  measure  of  ad.  less 
than  be,  and  let  di  be  that  multiple  frf  ah, 
which  least  exceeds  de,  and  which  by  the  note      B  I  E  .D  MA 
to  th.  67,  may  be  made  as  small  as  we  please. 

Let  cb,  ci,  be  drawn,  i  evidently  falls  between  e  and  b,  because  (by 
hyp.)  ei  is  less  than  am.  But  icd  :  acd  : :  id  :  ad,  by  th.  79.  Also, 
by  hyp.  ecd  :  acd  :  :  bd  :  ad,  greater  than  the.  ratio  of  id  :  ad,  or  of 
Ico  :  acd  ;  and  consequently,  ecd  is  greater  than  icd  :  which  is  impoui-  - 
bU,  By  a  like  reasoning  it  may  be  shown,  that  ecd  cannot  be  to  acd, 
.as  a  line  feu  than  ed,  is  to  ad.  Consequently,  it  must  be  ecd  :  acd  :  :  *D 
I  ad. 

Similar  reasoning,  founded  upon  vYte  \rc*wdvcv^  tvoU,  &$oUes  alto  te 
the  case  of  parallelograms. 


THEOREM!. 


327 


versally,  when  neither  are  equal,  they  are  to  each  other  in 
the  compound  ratio,  or  as  the  rectangle  or  pibduct  of  their 
bases  and  altitudes. 


  c 

~~A 

Q 
B 

r  d 

THEOREM  LXXXI. 

If  four  lines  be  proportional ;  the  rectangle  of  the  ex- 
tremes will  be  equal  to  the  rectangle  of  the  means.  And, 
conversely,  if  the  rectangle  of  the  extremes,  of  four  lines, 
be  equal  to  the  rectangle  of  the  means,  the  four  lirttes,  taken 
alternately,  will  be  proportional. 

Let  the  four  lines  a,  b,  c,  d,  be  A  

proportionals,  or  a  :  b  :  :  c  :  d  ;  B 
then  will  the  rectangle  of  a  and  d  be  ^ 
equal  to  the  rectangle  of  b  and  c ; 
or  the  rectangle  a  .  d  =  b  .  c. 

For,  let  the  four  lines  be  placed 
with  their  four  extremities  meeting 
in  a  common  point,  forming  at  that 

point  four  right  angles  ;  and  draw  lines  parallel  to  them  to 
complete  the  rectangles  p,  q,  r,  where  p  is  the  rectangle  of 
a  and  d,  a  the  rectangle  of  b  and  c,  and  r  the  rectangle  of 
b  and  d.  " 

Then  the  rectangles  r  and  r,  being  between  the  same 
parallels  are  to  each  other  as  their  bases  a  and  b  (th.  79)  ; 
and  the  rectangles  q  and  r,  being  between  the  same  parallels, 
are  to  each  other  as  their  bases  c  and  d.  But  the  ratio  of 
a  to  b,  is  the  same  as  the  ratio  of  c  to  n,  by  hypothesis  : 
therefore  the  ratio  of  p  to  a,  is  the  same  as  the  ratio  of  q  to 
r  ;  and  consequently  the  rectangles  f  and  q  are  equal. 

Q.  E.  D# 

Again,  if  the  rectangle  of  a  and  d,  be  equal  to  the 
rectangle  of  b  and  c  ;  these  lines  will  be  proportional,  or 
a  :  b  :  :  c  :  D.j 

For,  the  rectangles  being  placed  the  same  as  before  :  then, 
because  parallelograms  between  the  same  parallels,  are  to  one 
another  as  their  bases,  the  rectangle  r  :  r  :  :  a  :  b,  and 
q  :  r  :  :  c  :  d.  But  as  p  and  a  are  equal,  by  supposition, 
they  have  the  same  ratio  to  n,  that  is,  the  ratio  of  a  to  b  is 
equal  to  the  ratio  of  c  to  d,  or  a  :  b  : :  c  :  d.    q.  e.  d. 

Carol.  1.  When  the  two  means,  namely,  the  second  and 
third  terms,  are  equal,  their  rectangle  becomes  a  square  of 
the  second  term,  which  supplies  the  place  of  both  the  second 
and  third,    And  hence  it  follows,  that  when  three  lines  an 


828 


GEOMETRY. 


proportionals,  the  rectangle  of  the  two  extremes  is  equal  to 
the  square  of  the  mean  ;  and,  conversely,  if  the  rectangle  of 
the  extremes  be  equal  to  the  square  of  the  mean,  the  three 
lines  are  proportionals. 

Corel.  2.  Since  it  appears,  by  the  rules  of  proportion  in 
Arithmetic  and  Algebra,  that  when  four  quantities  are  pro* 
portional,  the  product  of  the  extremes  is  equal  to  the  product 
of  the  two  means  ;  and,  by  this  theorem,  the  rectangle  of  the 
extremes  is  equal  to  the  rectangle  of  the  two  means  ;  it  fol- 
lows, that  the  area  or  space  of  a  rectangle  is  represented  or 
expressed  by  the  product'  of  its  length  and  breadth  multiplied 
together.  And,  in  general,  a  rectangle  in  geometry  is  similar 
to  the  product  of  the  measures  of  its  two  dimensions  of  length 
and  breadth,  or  base  and  height.  Also,  a  square  is  similar 
to,  or  represented  by,  the  measure  of  its  side  multiplied  by 
itself.  So  that,  what  is  shown  of  such  products,  is  to  be  un- 
derstood of  the  squares  and  rectangles. 

CoroL  3.  Since  the  same  reasoning,  as  in  this  theorem, 
holds  for  any  parallelograms  whatever,  as  well  as  for  the 
rectangles,  the  same  property  belongs  to  all  kinds  of  paral- 
lelograms, having  equal  angles,  and  also  to  triangles,  which 
are  the  halves  of  parallelograms  ;  namely,  that  if  the  sides 
about  the  equal  angles  of  parallelograms,  or  triangles,  be 
reciprocally  proportional,  the  parallelograms  or  triangles  will 
be  equal ;  and,  conversely,  if  the  parallelograms  or  triangles 
be  equal,  their  sides  about  the  equal  angles  will  be  recipro- 
cally proportional. 

Corol.  4.  Parallelograms,  or  triangles,  having  an  angle  in 
each  equal,  are  in  proportion  to  each  other  as  the  rectangles 
of  the  sides  which  arc  about  these  equal  angles. 


THEOREM  LXXXII. 


If  a  line  be  drawn  in  a  triangle  parallel  to  one  of  its  sides, 
it  will  cut  the  other  two  sides  proportionally.        £  / 

Let  de  be  parallel  to  the  side  bc  of  the  A 
triangle  abc  ;  then  will  ad  :  db  :  :  ae  :  ec.  /\ 

For,  draw  be  and  cd.    Then  the  tri-  X)/  \j£ 

angles  dbe,  dce,  are  equal  to  each  other,  /x^\A 
because  they  have  the  same  base  de,  and  ^\ 
are  between  the  same  parallels  de,  i:c      B  C 
(th.  25).    But  the  two  triangles,  ade,  bde, 
on  the  bases  ad,  db,  have  the  same  altitude  ;  and  the  two 
triangles  ade,  cde,  on  the  bases  ae,  ec,  have  also  the  same 


THEOREMS.  329 

altitude  ;  and  because  triangles  of  the  same  altitude  are  to 
each  other  as  their  bases,  therefore 

the  triangle  ade  :  bde  :  :  ad  :  db, 
and  triangle  ade  :  cde  : :  ae  :  ec. 

But  bde  is  ~  cde  ;  and  equals  roust  have  to  equals  the 
same  ratio  ;  therefore  ad  :  db  : :  ae  :  ec.    a*  e.  d. 

Carol.  Hence,  also,  the  whole  lines  as,  ao,  are  propor- 
tional to  their  corresponding  proportional  segments  (corol. 
th.  60), 

viz.  ab  :  ac  :  :  ad  :  ae, 
and  ab  :  ac  :  :  bd  :  ce. 


theorem  lxxxiii. 


A  Line  which  bisects  any  angle  of  a  triangle,  divides  the 
opposite  side  into  two  segments,  which  are  proportional  to 
the  two  other  adjacent  sides. 

Let  the  angle  acb,  of  the  triangle  abc, 
be  bisected  by  the  line  cd,  making  the 
angle  r  equal  to  the  angle  s  :  then  will  the 
segment  ad  be  to  the  segment  db,  as  the 
side  ac  is  to  the  side  cb.  Or,  -  -  -  - 
ad  :  db  : :  ac  :  cb. 

For,  let  be  be  parallel  to  cd,  meeting 
AC  produced  at  e.  Then,  because  the  line  bc  cuts  the  two 
parallels  cd,  be,  it  makes  the  angle  cbe  equal  to  the  alter- 
nate angle  s  (th.  12),  and  therefore  also  equal  to  the  angle 
r,  which  is  equal  to  *  by  the  supposition.  Again,  because 
the  line  ae  cuts  the  two  parallels  uc,  be,  it  makes  the  angle 
E  equal  to  the  angle  r  on  the  same  side  of  it  (th.  14).  Hence, 
in  the  triangle  bck,  thfjangles  b  and  e,  being  each  equal  to 
the  angle  r,  are  equal  to  each  other,  and  consequently  their 
opposite  sides  cb,  ce,  are  also  equal  (th.  3). 

But  now,  in  the  triangle  abe,  the  line  cd,  being  drawn 
parallel  to  the  side  be,  cuts  the  two  other  sides  ab,  ae,  pro- 
portionally (th.  82),  making  ad  to  db,  as  is  ac  to  ce  or  to 
its  equal  cb.    q.  e.  d. 

Vol.  L  43 


830 


GEOXETXT. 


THEOREM  LXXXIV. 


Euuiangular  triangles  are  similar,  or  have  their  like  sides 
proportional- 
Let  abc,  def,  be  two  equiangular  tri- 
angles, having  the  angle  a  equal  to  the 
angle  d,  the  angle  b  to  the  angle  e,  and 
consequently  the  angle  c  to  the  angle  f  ; 
then  will  ab  :  ac  :  :  de  :  df.  A.  B 

For,  make  dg  =  ab,  and  dh  =  ac,  and  F 
join  gii.  Then  the  two  triangles  abc, 
dgh,  having  the  two  sides  ab,  ac,  equal 
to  the  two  dg,  dii,  and  the  contained  an- 
gles a  and  d  also  equal,  are  identical,  or 
equal  in  all  respects  (th.  1),  namely,  the 
angles  b  and  c  are  equal  to  the  angles  g  and  n.  But  the 
angles  b  and  c  are  equal  to  the  angles  e  and  f  by  the  hypo- 
thesis ;  therefore  also  the  angles  g  and  11  are  equal  to  the 
angles  e  and  f  (ax.  1),  and  consequently  the  line  qh  ia  paral- 
lel to  the  sido  ef  (cor.  1,  th.  14). 

Hence  then,  in  the  triangle  def,  the  line  gh,  being  parallel 
to  the  side  ef,  divides  the  two  other  sides  proportionally, 
making  do  :  dii  :  :  de  :  df  (cor.  th.  82).  But  dg  and 
dh  are  equal  to  ab  and  ac  ;  therefore  also  -  -  -  -  • 
ab  :  ac  :  :  de  :  df.    a.  e.  d. 


THEOREM  LXXXV. 


Triangles  which  have  their  sides  proportional,  arc  equi- 
angular. 

In  the  two  triangles  abc,  def,  if 
ab  :  de  :  :  ac  :  df  :  :  bc  :  ef  ;  the  two 
triangles  will  have  their  corresponding  /\ 
angles  equal. 

For,  if  the  triangle  abc  bc  not  equian-  A  B 
gular  with  the  triangle  dkf,  suppose  some  <*•  P 

other  triangle,  as  deg,  to  be  equiangular 
with  abc.  But  this  is  impossible  :  for  if 
the  two  triangles  abc,  deg,  were  equian- 
gular, their  sides  would  be  proportional 
(th.  84).  So  that,  ab  being  to  de  as  ac 
to  dg,  and  ab  to  de  as  bc  to  eg,  it  follows  that  do  and  eg, 
being  fourth  proportionals  to  the  same  three  quantities,  as 
well  as  the  two  df,  ef,  the  Conner,  dg,  eg,  would  be  equal 


THEOREMS. 


881 


to  the  latter,  df,  bp*  Thus,  then,  the  two  triangles  def, 
deg,  having  their  three  sides  equal,  would  be  identical 
(th.  5) ;  which  is  absurd,  since  their  angles  are  unequal. 

THEOREM  LXXXVI. 

Triangles,  which  have  an  angle  in  the  one  equal  to  an 
angle  in  the  other,  and  the  sides  about  these  angles  pro- 
portional, are  equiangular. 

Let  ABO,  def,  be  two  triangles,  having  the  angle  a  =  the 
angle  d,  and  the  sides  ab,  ac,  proportional  to  the  sides 
db,  dp  :  then  will  the  triangle  abc  be  equiangular  with  the 
triangle  dep. 

For,  make  do  =  ab,  and  dh  =  ac,  and  join  on. 

Then,  the  two  triangles  abc,  doh,  having  two  sides  equal, 
and  the  contained  angles  a  and  d  equal,  are  identical  and 
equiangular  (th.  1),  having  the  angles  o  and  h  equal  to  the 
angles  b  and  c.  But,  since  the  sides  dg,  du,  are  proportional 
to  the  sides  dk,  dp,  tho  line  air  is  parallel  to  ef  (th.  82) ; 
hence  the  angles  e  and  f  are  equal  to  the  angles  o  and  h 
(th.  14),  and  consequently  to  their  equals  b  and  c.  Q.  e.  d. 
[See  fig.  th.  lxxxiv.] 

THEOREM  LXXXV1I. 

In  a  right-angled  triangle,  a  perpendicular  from  the 
right  angle,  is  a  mean  proportional  between  the  segments  of 
the  hypothenuse;  and  each  of  the  sides,  about  the  right 
angle,  is  a  mean  proportional  between  the  hypothenuse  and 
the  adjacent  segment. 

C 

Let  abc  be  a  right-angled  triangle,  and 
cd  a  perpendicular  from  the  right  angle  c 
to  the  hypothenuse  ab  ;  then  will  A       D  B 

cd  be  a  mean  proportional  between  ad  and  db  ; 
ac  a  mean  proportional  between  ab  and  ad  ; 
bc  a  mean  proportional  between  ab  and  bd. 

Or,  ad  :  cd  :  :  cd  :  db  ;  and  ab  :  bc  :  :  bc  :  bd  ;  and 
ab  :  ac  :  :  ac  :  ad. 

For,  the  two  triangles,  abc,  adc,  having  the  right  angles 
at  c  and  d  equal,  and  the  angle  a  common,  have  their  third 
angles  equal,  and  are  equiangular,  (cor.  1,  th.  17).  In,  tikfe 
manner,  the  two  triangles  abc,  bdc,  having  xY&TUjgoX  wct^e* 


382 


GEOMETRY. 


at  c  and  d  equal,  and  the  angle  b  common,  hare  their  third 
angles  equal,  and  are  equiangular. 

Hence  then,  all  the  three  triangles,  abc,  adc,  bdc,  being 
equiangular,  will  have  their  like  sides  proportional  (th.  84) ; 

viz.  ad  :  CD  :  :  cd  :  db; 
and  xr:  ac  :  :  ac  :  ad; 
and  ab  :  bc  :  :  bc  :  bd.  q.  e  .d. 

Carol.  1.  Because  the  angle  in  a  semicircle  is  a  right 
angle  (th.  52) ;  it  follows,  that  if,  from  any  point  c  in  the 
periphery  of  the  semicircle,  a  perpendicular  be  drawn  to  the 
diameter  ab  ;  and  the  two  chords  ca,  cb,  be  drawn  to  the 
extremities  of  the  diameter :  then  are  ac,  bc,  cd,  the  mean 
proportionals  as  in  this  theorem,  or  (by  th.  77),  .... 

CD*  =  AD  .  DB  ;    AC3  =  AB  .  AD  ;  and  BC1  =  AB  .  BD. 

Corol.  2.    Hence  ac3  :  bc9  :  :  ad  :  bd. 

Corol.  3.  Hence  we  have  another  demonstration  of 
th.  34. 

For  since  ac3  =  ab  .  ad,  and  bc3  =  ab  .  bd  ; 
By  addition  ac3  +  bc9  =  ab  (ad  +  bd)  =  ab3. 


THEOREM  LXXXVIII. 


Equiangular  or  similar  triangles,  are  to  each  other  as  the 
squares  of  their  like  sides. 

Let  abc,  def,  be  two  equiangular 
triangles,  ab  and  de  being  two  like 
sides  :  then  will  the  triangle  abc  be  to 
the  triangle  def,  as  the  square  of  ab 
is  to  the  square  of  dk,  or  as  ah2  to  de2. 

For,  the  triangles  being  similar,  they 
have  theirlikesidesproportional  (th.84), 
and  are  to  each  other  as  the  rectangles 
of  the  like  pairs  of  their  sides  (cor.  4, 
th.  81) ; 

theref.  ab  :  de  :  :  ac  :  df  (th.  84), 

and  ab  :  de  :  :  ab  :  de  of  equality  : 
theref  ab3  :  de9  :  :  ab  •  ac  :  de  .  df  (th.  75). 
But  A  abc  :  A  def  :  :  ab  .  ac  :  de  .  df  (cor.  4,  th.  81), 
theref.  A  abc  :  A  def  :  :  ab3  :  de9.  a.  s.  d. 


a  £ 


THEOREMS  • 


383 


THEOREM  LXXX1X. 


All  similar  figures  are  to  each  other,  as  the  squares  of  their 
like  sides. 


Let  abcde,  fohik,  be 
any  two  similar  figures,  the 
like  sides  being  ab,  fg,  and 
bc,  oh,  and  so  on  in  the 
same  order:  then  will  the 
figure  abcde  be  to  the  figure 
fohik,  as  the  square  of  ab 
to  the  square  oft     or  as  ab3  to  fo9. 

For,  draw  be,  bd,  ok,  01,  dividing  the  figures  into  an 
equal  number  of  triangles,*  by  lines  from  two  equal  angles 
b  and  g. 

The  two  figures  being  similar  (by  suppos.),  they  are  equi- 
angular, and  have  their  like  sides  proportional  (def.  67). 

Then,  since  the  angle  a  is  =  the  angle  f,  and  the  sides 
ab,  ae,  proportional  to  the  sides  fo,  fk,  the  triangles 
abe,  fok,  are  equiangular  (th.  88).  In  like  manner,  the 
two  triangles  bcd  ghi,  having  the  angle  c  =  the  angle  h, 
and  the  sides  bc,  cd,  proportional  to  the  sides  gh,  hi,  are 
also  equiangular.  Also,  if  from  the  equal  angles  aed,  fkj, 
there  be  taken  the  equal  angles  aeb,  fko,  there  will  remain 
the  equals  bed,  gki  ;  and  if  from  the  equal  angles  cde,  hik, 
be  taken  away  the  equals  cdb,  hio,  there  will  remain  the 
equals  bde,  oik  ;  so  that  the  two  triangles  bde,  gik,  having 
two  angles  equal,  are  also  equiangular.  Hence  each  trian- 
gle of  the  one  figure,  is  equiangular  with  each  corresponding 
triangle  of  the  other. 

But  equiangular  triangles  arc  similar,  and  are  proportional 
to  the  squares  of  their  like  sides  (th.  88). 

Therefore  the  A  abb  :  A  fgk  : :  ab3  :  fg3, 
and  A  bcd  :  A  ohi  : :  nc3 :  gii2, 
and  A  bde  :  A  gik  : :  de3  :  iKa. 

But  as  the  two  polygons  are  similar,  their  like  sides  are 
proportional,  and  consequently  their  squares  also  propor- 
tional ;  so  that  all  the  ratios  ab2  to  fg3,  and  bc9  to  oh9,  and 
dm9 to  ik9,  are  equal  among  themselves,  antlxonsequently 
the  corresponding  triangles  also,  abe  to  fob*  and  bcd  to 
ohi,  and  bde  to  gik,  have  all  the  same  ratio,  viz.  that  of 
ab9  to  fg3  :  and  hence  all  the  antecedents,  or  the  figure 
abcde,  have  to  all  the  consequents,  or  the  figure  fghik, 
the  same  ratio,  viz.  that  of  ab3  to  fo9  QCh.  T&y    o..  i>» 


384 


GEOMETRY* 


THEOREM  XC. 


Similar  figures  inscribed  in  circles,  have  their  like  sides, 
and  also  their  whole  perimeters,  in  the  same  ratio  as  the 
diameters  of  the  circles  in  which  they  are  inscribed. 

.    Let    ABCDE,  FGHIK,  T>  1 

be  two  similar  figures,  ^^>J* 
inscribed  in  the  circles 
whose  diameters  are  al 
andFM;  then  will  each 
side  ab,  bc,  die.  of  the 
one  figure  be  to  the  like 
side  gf,  oh,  &c.  of  the 

other  figure,  or  the  whole  perimeter  ab  +  bc  +  die.  of  the 
one  figure,  to  the  whole  perimeter  fg  +  oh  +  dec.  of  the 
other  figure,  as  the  diameter  al  to  the  diameter  fm. 

For,  draw  the  two  corresponding  diagonals  ac,  fh,  as 
also  the  lines  bl,  gm.  Then,  since  the  polygons  are  similar, 
they  are  equiangular,  and  their  like  sides  have  the  same  ratio 
(def.  67) ;  therefore  the  two  triangles  abc,  fgh,  have  the 
angle  b  =  the  angle  g,  and  the  sides  ab,  bc,  proportional 
to  the  two  sides  fg,  Gir,  consequently  these  two  triangles 
are  equiangular  (th.  80),  and  have  the  angle  acb  =  fhg. 
But  the  angle  acb  =  alb,  standing  on  the  same  arc  ab  ; 
and  the  angle  fhg  =  fmg,  standing  on  the  same  arc  fg  ; 
therefore  the  angle  alb  =  fmg  (ax.  1).  And  since  the 
angle  abl  =  fgm,  being  both  right  angles,  because  in  a 
semicircle  ;  therefore  the  two  triangles  abl,  fgm,  having 
two  angles  equal,  are  equiangular ;  and  consequently  their 
like  sides  are  proportional  (th.  84)  ;  hence  ab  :  fg  : :  the 
diameter  al  :  the  diameter  fm. 

In  like  manner,  each  side  bc,  cd,  dec.  has  to  each  side 
oh,  in,  dec.  the  same  ratio  of  al  to  fm  ;  and  consequently 
the  sums  of  them  are  still  in  the  same  ratio,  viz.  ab  +  bc  + 
cd,  &c.  :  fg  +  gh  +  hi,  dec.  :  :  the  diam.  al  :  the  diam. 
fm  (th.  72).    Q.  E.  D. 


THEOREM  XCI. 

Similar  figures  inscribed  in  circles,  are  to  each  other  a»  the 
squares  of  the  diameters  of  those  circles. 

Let  abcde,  foiiis,  be  two  similar  figures,  inscribed  in 
the  circles  whose  diameters  are  al  and  fm  ;  then  the  surface 
of  the  polygon  abode  will  be  to  the  surface  of  the  polygon 

FGHIK,  as  AL3  to  FM3. 


THEOREMS. 


385 


For,  the  figures  being  similar,  are  to  each  other  as  the 
squares  of  their  like  sides,  ab2  to  Ft;3  (th.  86).  But,  by  the 
last  theorem,  the  sides  ab,  fg,  are  as  the  diameters  al,  fm  ; 
and  therefore  the  squares  of  the  sides  ab3  to  fg3,  as  the 
squares  of  the  diameters  al*  to  fx1  (th.  74).  Consequently 
the  polygons  abcde,  fohik,  are  also  to  each  other  as  the 
squares  of  the  diameters  al3  to  fm3  (ax.  1).  u.  e.  d. 
[See  fig.  th.  xc] 

THEOREM  XCII. 

The  circumferences  of  all  circles  are  to  each  other  as  their 
diameters1'. 


*  The  truth  of  theorems  92, 93,  and  94,  may  be  established  more 
satisfactorily  than  in  the  text,  upon  principles  analogous  to  those  of  the 
two  last  notes. 

Theorem.  The  area  of  any  circle  abd  is  equal  to  the  rectangle  con- 
tained by  the  radius,  and  a  straight  line  equal  to  half  the  circumference. 

If  not,  let  the  rectangle  be  lest  than  the  circle 
aid,  or  equal  to  the  circle  fhh  :  and  imagine  ed 
drawn  to  touch  the  interior  circle  in  f,  and  meet 
the  circumference  abd  in  e  and  d.  Join  cd, 
cutting  the  arc  of  the  interior  circle  in  k.  Let 
fii  be  a  quadrantal  arc  of  the  inner  circle,  and 
from  it  take  its  half,  from  the  remainder  Us  half, 
and  so  on,  until  an  arc  fi  is  obtained,  less  than 
fit.  Join  ci,  produce  it  to  cut  ed  in  l,  and  make 
fo  =  fl  :  so  snail  lo  be  the  side  of  a  regular  polygon  circumscribing  the 
circle  frh.  It  is  manifest  that  this  polygon  is  less  than  the  circle  abd, 
because  it  is  contai.ud  within  it  Because  the  trinngle  gcl  is  half  the 
rectangle  of  base  gl  and  altitude  cf,  the  whole  polygon  of  which  gcl 
is  a  constituent  triangle,  is  equal  to  half  the  rectangle  whose  base  is  the 
perimeter  of  that  polygon  and  altitude  cf-  But  that  perimeter  is  less 
than  the  circumference  abd,  because  each  portion  of  it,  such  as  gl,  Is 
less  than  the  corresponding  arch  of  circle  having  radius  cl,  and  there- 
fore, *  fortiori,  less  than  the  corresponding  arch  of  circle  with  radius 
ca.  Also  ce  is  less  than  ca.  Therefore  the  polygon  of  which  one  side 
is  ol,  is  less  than  the  rectangle  whose  base  is  half  the  circumference  abd 
and  altitude  ca;  that  is,  (by  hyp.)  less  than  the  circle  fwh,  which  it 
conta  *s:  which  is  absurd.  Therefore,  the  rectangle  under  the  radius 
and  half  the  circumference  is  not  less  than  the  circle  abd.  And  by  a 
similar  process  it  may  be  shown  that  it  is  not  greater.  Consequently, 
H  is  equal  to  that  rectangle,  q.  e.  d. 

Theorem.  The  circumferences  of  two  circles  abd,  abd,  are  as  their 
radii. 

If  possible,  let  the  radius  ac, 
be  to  the  radius  ac,  as  the  cir- 
cumference abd  to  a  circum- 
ference ihk  less  than  abd.  Draw 
the  radius  cic,  and  the  straight 
line/tg- a  chord  to  the  circle 
abd,  and  a  tangent  to  the  circle 
ihk  in  i.  From  eb,  a  quarter  of 
the  circumference  ofa&t,  take 


336 


GEOMETRY. 


Let  d,  dy  denote  the  diameters  of  two  circles,  and  c,  e9 
their  circumferences ; 

then  will  d  :  d  :  :  c  :  c,  or  d  :  c  : :  d  :  c. 

For  (by  theor.  90),  similar  polygons  inscribed  in  circles 
have  their  perimeters  in  the  same  ratio  as  the  diameters  of 
those  circles. 

Now  as  this  property  belongs  to  all  polygons,  whatever 
the  number  of  the  sides  may  be ;  conceive  the  number  of  the 
sides  to  be  indefinitely  great,  and  the  length  of  each  inde- 
finitely small,  till  they  coincide  with  the  circumference  of 
the  circle,  and  be  equal  to  it,  indefinitely  near.  Then  the 
perimeter  of  the  polygon  of  no  infinite  number  of  sides,  is 
the  same  thing  as  the  circumference  of  the  circle.  Hence  it 
appears  that  the  circumferences  of  the  circles,  being  the  same 
as  the  perimeters  of  such  po  /gone,  are  to  each  other  in  the 
same  ratio  as  the  diameters  of  the  circles,    a-  e.  d. 

THEOREM  XCIII. 

The  areas  or  spaces  of  circles,  arc  to  each  other  as  the 
squares  of  their  diameters,  or  of  their  radii. 

Let  a,  a,  denote  the  areas  or  spaces  of  two  circles,  and 
d,  d,  their  diameters ;  then  a  :  a  : :  d3  :  d2. 

For  (by  theorem  91)  similar  polygons  inscribed  in  circles 
are  to  each  other  as  the  squares  of  the  diameters  of  the 
circles. 


away  its  half,  and  then  the  half  of  the  remainder,  and  so  on,  until  there 
be  obtained  an  arc  ed  less  than  eg;  and  from  d  draw  ad  parallel  to//, 
it  will  be  the  side  of  a  regular  polygon  inscribed  in  the  circle  abd,  yet 
evidently  greater  than  the  circle  ihk,  because  each  of  its  constituent  tri- 
angles, as  acd  contains  the  corresponding  circular  sector  eno.  Let  ad 
be  the  side  of  a  similar  polygon  inscribed  in  the  circle  adb,  and  join  ac, 
cd,  similarly  to  ac,  ed.  The  similar  triangles  acd,  acdt  give  ac  :  ac : : 
ad  :  ad,  and  : :  perim.  of  polygon  in  abd  :  perim.  of  polygon  in  abd. 
But,  by  the  preceding  theorem,  ac  :  ac  : :  circumf.  abd  :  circumf.  abd. 
The  perimeters  of  the  polygons  are,  therefore,  as  the  circumferences  of 
the  circles.  But,  this  is  impossible ;  because,  (by  hyp.)  the  perim.  of 
polygon  in  abd  is  less  than  the  circumf. ;  while,  on  the  contrary,  the 
perim.  of  polygon  in  adb  is  greater  than  the  circumf.  ihk.  Conse- 
quently, ac  is  not  to  ac,  as  circumf.  adb,  to  a  circumference  Ust  than 
adb.  And  by  a  similar  process  it  may  be  shown,  that  ac  is  not  to  ac,  as 
the  circumf.  dbd,  to  a  circumference  less  than  abd.  Therefore  ac  :  ac 
::  circumf.  abd  :  circumf.  abd.       e.  d. 

Corol.  Since  by  this  theorem,  we  have  c  :  c  : :  r  :  r,  or,  if  c  =  »R, 
c  =  *r ;  and,  by  the  former,  area  (a)  :  area  (a)  : :  £rc  :  |rc  :  we  btvo 
a  :  a  :  :  fan? :  far* :  :  R*  :  t*       •.  d*    c» :  A 


THEOREMS. 


837 


Hence,  conceiving  the  number  of  the  sides  of  the  polygons 
to  be  increased  more  and  more,  or  the  length  of  the  sides  to 
become  less  and  less,  the  polygon  approaches  nearer  and 
nearer  to  the  circle,  till  at  length,  by  an  infinite  approach, 
they  coincide,  and  become  in  effect  equal  ;  and  then  it  fol- 
lows, that  the  spaces  of  the  circles,  which  are  the  same  as  of 
the  polygons,  will  be  to  each  other  as  the  squares  of  the 
diameters  of  the  circles,    q.  e.  d. 

Carol.  The  spaces  of  circles  are  also  to  each  other  as  the 
squares  of  the  circumferences ;  since  the  circumferences  are 
in  the  same  ratio  as  the  diameters  (by  theorem  92). 

THEOREM  XCIV. 

% 

Thb  area  of  any  circle,  is  equal  to  the  rectangle  of  half  its 
circumference  and  half  its  diameter. 

Conceive  a  regular  polygon  to  be  in- 
scribed in  the  circle  ;  and  radii  drawn  to 
all  the  angular  points,  dividing  it  into  as 
many  equal  triangles  as  the  polygon  has 
sides,  one  of  which  is  abc,  of  which  the 
altitude  is  the  perpendicular  cd  from  the 
centre  to  the  base  ab. 

Then  the  triangle  abc,  being  equal  to  a  rectangle  of  half 
the  base  and  equal  altitude  (th.  26,  cor.  2),  is  equal  to  the 
rectangle  of  the  half  base  ad  and  the  altitude  cd  ;  con- 
sequently the  whole  polygon,  or  all  the  triangles  added  to- 
gether which  compose  it,  is  equal  to  the  rectangle  of  the 
common  altitude  cd,  and  the  halves  of  all  the  sides,  or  the 
half  perimeter  of  the  polygon. 

Now  conceive  the  number  of  sides  of  the  polygon  to  be 
indefinitely  increased  ;  then  will  its  perimeter  coincide  with 
the  circumference  of  the  circle,  and  consequently  the  altitude 
cd  will  become  equal  to  the  radius,  and  the  whole  polygon 
equal  to  the  circle.  Consequently  the  space  of  the  circle,  or 
of  the  polygon  in  that  state,  is  equal  to  the  rectangle  of  the 
radius  and  half  the  circumference,   a.  e.  d. 


Vol.  I. 


44 


338 


OF  PLANES  AND  SOLIDS. 


DEFINITIONS. 


Def.  88.  The  Common  Section  of  two  Planes,  is  the 
line  in  which  they  meet,  or  cut  each  other. 

80.  A  Line  is  Perpendicular  to  a  Plane,  when  it  is  per* 
pendicular  to  every  line  in  that  plane  which  mmka  it* 

90.  One  Plane  is  Perpendicular  to  Another,  when  eray 
line  of  the  one,  which  is  perpendicular  to  the  line  of  their 
common  section,  is  perpendicular  to  the  other. 

91.  The  Inclination  of  one  Plane  to  another,  or  the  angle 
they  form  between  them,  is  the  angle  contained  by  two  lines, 
drawn  from  any  point  in  the  common  section,  and  at  right 
angles  to  the  same,  one  of  these  lines  in  each  plane. 

92.  Parallel  Planes,  are  such  as  being  produced  ever  so 
far  both  ways,  will  never  meet,  or  which  are  every  where  at 
an  equal  perpendicular  distance. 

93.  A  Solid  Angle,  is  that  which  is  made  by  three  or 
more  plane  angles,  meeting  each  other  in  the  same  point. 

94.  Similar  Solids,  contained  by  plane  figures,  are  such  as 
have  all  their  solid  angles  equal,  each  to  each,  and  are  bounded 
by  the  same  number  of  simitar  planes,  alike  placed. 

95.  A  Prism,  is  a  solid  whose  ends  are  parallel,  equal,  and 
like  plane  figures,  and  its  sides,  connecting  those  ends,  are 
parallelograms. 

96.  A  Prism  takes  particular  names  according  to  the  figure 
of  its  base  or  ends,  whether  triangular,  square,  rectangular, 
pentagonal,  hexagonal,  &c. 

97.  A  Right  or  Upright  Prism,  is  that  which  .has  the 
planes  of  the  sides  perpendicular  to  the  planes  of  the  erifa 
or  base. 

98.  A  Parallelopiped,  or  Parallelopipedon,  is 
a  prism  bounded  by  six  parallelograms,  every 
opposite  two  of  which  are  equal,  alike,  and  pa- 
rallel. 


DEFINITIONS. 


889 


A 


DO.  A  Rectangular  Parallelopidedon,  is  that  whose  bound- 
ins  planes  are  all  rectangles,  which  are  perpendicular  to  each 
other. 

100.  A  Cube,  is  a  square  prism,  being  bound- 
ed by  six  equal  square  sides  or  faces,  and  are 
perpendicular  to  each  other. 

101.  A  Cylinder  is  a  round  prism,  having 
circles  for  its  ends ;  and  is  conceived  to  be  form- 
ed by  the  rotation  of  a  right  line  about  the  cir- 
cumferences of  two  equal  and  parallel  circles, 
always  parallel  to  the  axis. 

102.  The  Axis  of  a  Cylinder,  is  the  right 
line  joining  the  centres  of  the  two  parallel  circles,  about 
which  the  figure  is  described. 

108.  A  Pyramid,  is  a  solid,  whose  base  is  any 
right-lined  plane  figure,  and  its  sides  triangles, 
having  all  their  vertices  meeting'  together  in  a 
point  above  the  base,  Called  the  vertex  of  the 
pyramid. 

104.  A  pyramid,  like  the  prism,  takes  particular  names 
from  the  figure  of  the  base. 

105.  A  Cone,  is  a  round  pyramid,  having  a 
circular  base,  and  is  conceived  to  be  generated 
by  the  rotation  of  a  right  line  about  the  circum- 
ference of  a  circle,  one  end  of  which  is  fixed  at 
a  point  above  the  plane  of  that  circle. 

106.  The  Axis  of  a  cone,  is  the  right  line,  joining  the 
vertex,  or  fixed  point,  and  the  centre  of  the  circle  about 
which  the  figure  is  described. 

107.  Similar  Cones  and  Cylinders,  are  such  as  have  their 
altitudes  and  the  diameters  of  their  bases  proportional. 

108.  A  Sphere,  is  a  solid  bounded  by  one  curve  surface, 
which  is  every  where  equally  distant  from  a  certain  point 
within,  called  the  Centre.  It  is  conceived  to  be  generated 
by  the  rotation  of  a  semicircle  about  its  diameter,  which  re- 
mains fixed. 

109.  The  Axis  of  a  Sphere,  is  the  right  line  about  which 
the  semicircle  revolves  ;  and  the  centre j  is  the  same  as  that 
of  the  revolving  semicircle. 

110.  The  Diameter  of  a  Sphere,  is  any  right  line  passing 
through  the  centre,  and  terminated  both  ways  by  the  surface. 

111.  The  Altitude  of  a  solid,  is  the  perpendicular  drawn 
from  the  vertex  to  the  opposite  side  or  base. 


840 


GEOMETRY. 


THEOREM  XCV. 

A  perpendicular  is  the  shortest  line  which  can  be  drawn 
from  any  point  to  a  plane. 

Let  ab  be  perpendicular  to  the  plane 
db  ;  then  any  other  line,  as  ac,  drawn 
from  the  same  point  a  to  the  plane,  will 
be  longer  than  the  line  ab. 

In  the  plane  draw  the  line  bo,  joining  d 
thepoints  m . 

Then,  because  the  line  ab  is  perpendi- 
cular to  the  plane  de,  the  angle  b  is  a  right  angle  (de£  90), 
and  consequently  greater  than  the  angle  c ;  therefore  the 
line  ab,  opposite  to  the  less  angle,  is  less  than  any  other  line 
ac,  opposite  the  greater  angle  (th.  21).    q.  e.  d. 

THEOREM  ZCVI. 

A  perpendicular  measures  the  distance  of  any  point  from  a 
plane. 

The  distance  of  one  point  from  another  is  measured  by  a 
right  line  joining  them,  because  this  is  the  shortest  line  which 
can  be  drawn  from  one  point  to  another.  So,  also,  the  dis- 
tance from  a  point  to  a  line,  is  measured  by  a  perpendicu- 
lar, because  this  line  is  the  shortest  which  can  be  drawn 
from  the  point  to  the  line.  In  like  manner,  the  distance 
from  a  point  to  a  plane,  must  be  measured  by  a  perpendicu- 
lar drawn  from  that  point  to  the  plane,  because  this  is  the 
shortest  line  which  can  be  drawn  from  the  point  to  the 
plane. 

THEOREM  XCVII. 

The  common  section  of  two  planes,  is  a  right  line. 

Let  acbda,  aebfa,  be  two  planes  cut- 
ting each  other,  and  a,  b,  two  points  in 
which  the  two  planes  meet ;  drawing  the 
line  ab,  this  line  will  be  the  common  in- 
tersection of  the  two  planes. 

For,  because  the  right  line  ab  touches 
the  two  planes  in  the  points  a  ajd  b,  it 


THEOREMS. 


841 


touches  them  in  all  other  points  (def.  20)  ;  this  line  is  there- 
fore common  to  the  two  planes.  That  is,  the  common  in- 
tersection of  the  two  planes  is  a  right  line.    a.  b.  d. 

Cord.  From  the  same  point  in  a  plane,  there  cannot  be 
drawn  two  perpendiculars  to  the  plane  on  the  same  side  of 
it.  For,  if  it  were  possible,  each  of  these  lines  would  be 
perpendicular  to  the  straight  line  which  is  the  common  inter- 
section of  the  plane  and  another  plane  passing  through  the 
two  perpendiculars,  which  is  impossible. 


THEOREM  XCVIII. 

If  a  line  be  perpendicular  to  two  other  lines,  at  their  com- 
mon point  of  meeting  ;  it  will  be  perpendicular  to  the  plane 
of  those  lines. 

Let  the  line  ab  make  right  angles  with  -q 
the  lines  ac,  ad  ;  then  will  it  be  per- 
pendicular  to  the  plane  cde  which  passes 
through  these  lines.  y^^Ty^ 

If  the  line  ab  were  not  perpendicular  to  E^^sT/) 
the  plane  cde,  another  plane  might  pass 
through  the  point  a,  to  which  the  line  ab 
would  be  perpendicular.    But  this  is  im- 
possible ;  for,  since  the  angles  bac,  bad,  are  right  angles, 
this  other  plane  must  pass  through  the  points  c,  d.  Hence, 
this  plane  passing  through  the  two  points  a,  c,  of  the  line 
ac,  and  through  the  two  points  a,  d,  of  the  line  ad,  it  will 
pass  through  both  these  two  lines,  and  therefore  be  the  same 
plane  with  the  former,   a.  e.  d. 


THEOREM  XCIX. 


If  two  planes  cut  each  other  at  right  angles,  and  a  line 
be  drawn  in  one  of  the  planes  perpendicular  to  their 
common  intersection,  it  will  be  perpendicular  to  the  other 
plane. 

Let  the  two  planes  acbd,  aebf,  cut 
each  other  at  right  angles  ;  and  the  line 
co  be  perpendicular  to  their  common  sec- 
tion ab  ;  then  will  co  be  also  perpendicu- 
lar to  the  other  plane  aebf. 

For,  draw  eg  perpendicular  to  ab. 
Then,  because  the  two  lines,  ac,  ox,  are 
perpendicular  to  the  common  intersection 


53 


GEOXETftY. 


ab,  the  angle  cge  is  the  angle  of  inclination  of  the  two 
planes  (def.  92).  But  since  the  two  planes  cut  each  other 
perpendicularly,  the  angle  of  inclination  oge  is  a  right 
angle.  And  since  the  line  cg  is  perpendicular  to  the  two 
Jines  oa,  oe,  in  the  plane  aebf,  it  is  therefore  perpendicular 
to  that  plane  (th.  98).    a.  e.  d. 

Carol.  1.  Every  plane,  ACB,'passing  through  a  perpendicular 
<jg  to  another  plane  aebf,  wiH  be  perpendicular  to  that  other 
plane.  For,  if  acb  be  not  perpendicular  to  the  plane  aebf, 
some  other  plane  on  the  same  side  of  aebf,  and  passing 
through  ab,  will  be  perpendicular  to  it.  Then,  if  from  the  point 
g  a  straight  line  be  drawn  in  this  other  plane  perpendicular  to 
the  common  intersection,  it  will  be  perpendicular  to  the  plane 
abbf.  But  (hyp.)  co  is  perpendicular  to  that  plane.  There- 
fore, there  will  be,  from  the  same  point  g,  two  perpendicu- 
lars to  the  same  plane  on  the  same  side  of  it,  which  is  im- 
possible (cor.  97). 

Carol.  2.  If  from  any  point  g  in  the  common  intersection 
of  the  two  planes  acb  and  aebf  perpendicular  to  each  other, 
a  line  be  drawn  perpendicular  to  either  plane,  that  line  will 
be  in  the  other  plane. 


THEOBEM  C. 


If  two  lines  be  perpendicular  to  the  same  plane,  they  will  be 
parallel  to  each  other. 

Let  the  two  lines  ab,  cd,  be  both  per- 
pendicular to  the  same  plane  ebdf  ;  then 
will  ab  be  parallel  to  cd.  .    ■  ■■ 

For,  join  b,  d,  by  the  line  bd  in  the  El  B '  h>  B 
plane.  The  plane  abd  is  perpendicular  to  I  ■■  •  J 
the  plane  ef  (cor.  1,  th.  99) ;  and  therefore 
the  line  cd,  drawn  from  a  point  in  the  common  intersection 
of  the  two  planes,  perpendicular  to  ef,  will  be  in  the  plane 
abd  (cor.  2,  th.  99).  But,  because  the  lines  ab,  cd,  are 
perpendicular  to  the  plane  ef,  they  are  both  perpendicular 
to  the  line  bd  in  that  plane,  and  they  have  been  proved  to 
be  in  the  same  plane  abd  ;  consequently,  they  are  paral- 
lel to  each  other  (cor.  th.  13).    a.  e.  d. 

Carol.  If  two  lines  be  parallel,  and  if  one  of  them  be  per- 
pendicular to  any  plane,  the  other  will  also  be  perpendicular 
to  the  same  plane. 


THE0RBMS. 


348 


THEOREM  CI. 

If  one  plane  meet  another  plane,  it  will  make  angles 
with  that  other  plane,  which  are  together  equal  to  two  right 
angles. 

Let  the  plane  acbd  meet  the  plane  aebf  ;  these  planes 
make  with  each  other  two  angles  whose  sum  is  equal  to  two 
right  angles. 

For,  through  any  point  g,  in  the  common  section  ab, 
draw  cd,  ef,  perpendicular  to  ab.  Then,  the  line  cg 
makes  with  ef  two  angles  together  equal  to  two  right  angles. 
But  these  two  angles  are  (by  def.  92)  the  angles  of  inclina* 
tion  of  the  two  planes.  Therefore  the  two  planes  make  an- 
gles with  each  other,  which  are  together  equal  to  two  right 
angles. 

Corel.  In  like  manner,  it  may  be  demonstrated,  that  planes 
which  intersect  have  their  vertical  or  opposite  angles  equal ; 
also,  that  parallel  planes  have  their  alternate  angles  equal  ; 
and  so  on,  as  in  parallel  lines. 


•  %  THEOREM  CII. 

If  two  planes  be  parallel  to  each  other  ;  a  line  which  is 
perpendicular  to  one  of  the  planes,  will  also  be  perpendicular 
to  the  other. 


Let  the  two  planes  cd,  ef,  be  parallel, 
and  let  the  line  ab  be  perpendicular  to  the 
plane  cd  ;  then  shall  it  also  be  perpendi- 
cular to  the  other  plane  ef. 

For,  from  any  point  g,  in  the  plane  ef, 
draw  gh  perpendicular  to  the  plane  cd,  and 
draw  ah,  bg. 


Then,  because  ba,  gh,  are  both  perpendicular  to  the 
plane  cd,  the  angles  a  and  h  are  both  right  angles.  And 
because  the  planes  cd,  ef,  are  parallel,  the  perpendiculars 
ba,  gh,  are  equal  (def.  93).  Hence  it  follows  that  the  lines 
bg,  ah,  are  parallel  (def.  9).  And  the  line  ab  being  per- 
pendicular to  the  line  ah,  is  also  perpendicular  to  the  parallel 
fine  bg  (cor.  th.  12). 

In  like  manner  it  is  proved,  that  the  line  ab  is  perpendicu- 
lar to  all  other  lines  which  can  be  drawn  from  Ita^wsiX  Vto. 


844 


OEOXBTET. 


the  plane  ef.  Therefore  the  line  ab  is  perpendicular  to  the 
whole  plane  ef  (def.  00).   q.  b.  d. 


theobek  cm. 

If  two  lines  be  parallel  to  a  third  line,  though  not  in  the 
same  plane  with  it ;  they  will  be  parallel  to  each  other. 


Let  the  lines  ab,  cd,  be  each  of  them 
parallel  to  the  third  line  ef,  though  not  in 
the  same  plane  with  it ;  then  will  ab  be  pa-  J) 
rallel  to  cd. 

For,  from  any  point  o  in  the  line  ef,  let 
oh,  01,  be  each  perpendicular  to  ef,  in  the  H 
planes  eb,  id,  of  the  proposed  parallels. 

Then,  since  the  line  ef  is  perpendicular 
to  the  two  lines  gh,  01,  it  is  perpendicular 
to  the  plane  ghi  of  those  lines  (th.  98).  And  because  ef 
is  perpendicular,  to  the  plane  cm,  its  parallel  ab  is  also  per- 
pendicular to  that  plane  (cor.  th.  99).  For  the  same  reason, 
the  line  cd  is  perpendicular  to  the  same  plane  ghi.  Hence, 
because  the  two  lines  ab,  cd,  are  perpendicular  to  the  same 
plane,  these  two  lines  are  parallel  (th.  99).    q.  e.  d. 


THEOREM  CIV. 


If  two  lines,  that  meet  each  other,  be  parallel  to  two 
other  lines  that  meet  each  other,  though  not  in  the  same 
plane  with  them  ;  the  angles  contained  by  those  lines  will  be 
equal. 

^*et  the  two  lines  ab,  bc,  be  parallel  to  B 
the  two  lines,  de,  ef  ;  then  will  the  angle  ^ 
abc  beequal  to  the  angle  def.  ^ 

For,  make .  the  lins  ab,  bc,  de,  ef,  all 
equal  to  each  other,  and  join  ac,  df,  ad, 
be,  cf. 

Then,  the  lines  ad,  be,  joining  the  equal  £> 
and  parallel  lines  ab,  de,  are  equal  and 
parallel  (th.  24).  For  the  same  reason,  cf,  be,  are  equal 
and  parallel.  Therefore  ad,  cf,  are  equal  and  parallel 
(th.  15)  ;  and  consequently  also  ac,  df  (th.  24).  Hence, 
the  two  triangles  abc,  def,  having  all  their  sides  equal, 
each  to  each,  have  their  angles  also  equal,  and  consequently 
the  angle  abc  ==  the  angle  def.   a.  e.  d. 


THEOREMS. 


845 


THEOREM  CV. 


Tax  sections  made  by  a  plane  cutting  two  other  parallel 
planes,  are  also  parallel  to  each  other. 

Let  the  two  parallel  planes  ab,  cd,  be 
cut  by  the  third  plane  efhg,  in  the  lines 
sr,  oh  :  these  two  sections  kf,  oh,  will 
be  parallel. 

Suppose  eo,  fh,  be  drawn  parallel  to 
each  other  in  the  plane  efhg  ;  also  let 
ei,  FK,  be  perpendicular  to  the  plane 
cd  ;  and  let  ig,  kh,  be  joined. 

Then  eg,  fh,  being  parallels,  and  ei,  fk,  being  both 
perpendicular  to  the  plane  cd,  are  also  parallel  to  each  other 
(th.  99)  ;  consequently  the  angle  hfk  is  .equal  to  the  angle 
gei  (th.  104).  But  the  angle  fkh  is  also  equal  to  the  angle 
big,  being  both  right  angles  ;  therefore  the  two  triangles  are 
equiangular  (cor.  1,  th.  17) ;  and  the  sides  fk,  ei,  being  the 
equal  distances  between  the  parallel  planes  (def.  93),  it  fol- 
lows that  the  sides  fh,  eg,  are  also  equal  (th.  2).  But  these 
two  lines  are  parallel  (by  suppos.),  as  well  as  equal;  con" 
sequently  the  two  lines  ef,  gh,  joining  those  two  equal 
parallels,  are  also  parallel  (th.  24).    a.  e.  d. 


theorem  cvi. 


If  any  prism  be  cut  by  a  plane  parallel  to  its  base,  the  sec- 
tion will  be  equal  and  like  to  the  base. 

Let  ag  be  any  prism,  and  il  a  plane 
parallel  to  the  base,  ac  ;  then  will  the  plane 
il  be  equal  and  like  to  the  base  ac,  or  the 
two  planes  will  have  all  their  sides  and  all 
their  ancles  equal. 

For,  the  two  planes  ac,  il,  being  parallel 
by  hypothesis  ;  and  two  parallel  planes,  cut 
by  a  third  plane,  having  parallel  sections 
(th.  105) ;  therefore  nt  is  parallel  to  ab,  and 
xjl  to  bc,  and  lm  to  cd,  and  im  to  ad.  But  ai  and  bk  are 
parallels  (by  def.  95) ;  consequently  ak  is  a  parallelogram ; 
and  the  opposite  sides  ab,  ik,  are  equal  (th.  22).  In  like 
manner,  it  is  shown  that  kx  is  =  bc,  and  lm  =  cd,  and  im 
s=  ad,  or  the  two  planes  ac,  il,  are  mutually  equilateral.  But 
these  two  planes  having  their  corresponding  side*  ^an&&, 

Vol.  I.  45 


846 


GEOMETRY. 


have  the  angles  contained  by  them  also  equal  (th.  104), 
namely,  the  angle  a  =  the  angle  i,  the  angle  b  «  the 
angle  k,  the  angle  c  =  the  angle  l,  and  the  angle  »  =  the 
angle  m.  So  that  the  two  planes  ac,  il,  have  all  their 
corresponding  sides  and  angles  equal,  or  they  are  equal  mwA 
like.   a.  b.  d. 


THBOBKM  CVII* 


If  a  cylinder  be  cut  by  a  plane  parallel  to  its  base,  the 
section  will  be  a  circle,  equal  to  the  base. 

Let  af  be  a  cylinder,  and  ghi  any  sec- 
tion parallel  to  the  base  abc  ;  then  will  0111 
he  a  circle,  equal  to  abc. 

Forf  let  the  planes  kb,  kf,  pass  through 
the  .axis  of  the  cylinder  mk,  and  meet  the 
section  ghi  in  the  three  points  h,  i,  l  ;  and 
join  the  points  as  in  the  figure. 

Then,  since  kl,  ci,  are  parallel  (by  def. 
102)  ;  and  the  plane  ki,  meeting  the  two 
parallel  planes  abc,  ghi,  makes  the  two  sections  kg,  li,  pa- 
rallel (th.  105) ;  the  figure  klic  is  therefore  a  parallelogram, 
and  consequently  has  the  opposite  sides  li,  kc,  equal,  where 
kc  is  a  radius  of  the  circular  base. 

In  like  manner  it  is  shown  that  lh  is  equal  to  the  radius 
kb;  and  that  any  other  lines,  drawn  from  the  point  L  to 
the  circumference  of  the  section  ghi,  are  all  equal  to  radii 
of  the  base ;  consequently  ghi  is  a  circle,  and  equal  to  abc. 

B.  D. 


THEOREM  CV1II. 


All  prisms  and  cylinders,  of  equal  bases  and  altitudes,  ate 
equal  to  each  other. 

Let  ac,  df,  be  two 
prisms,  and  a  cylinder, 


on  equal  bases,  ab,  de, 
and  having  equal  alti- 
tudes bc,  ef  ;  then  will  P 
the  solids  ac,  df,  be 
equal*. 

For,  let  pq,  bs,  be 


7 


©J 


S  It 


E 


*  This,  and  some  other  demonstrations  relative  to  solids,  are  upon  the 
defective  principle  of  Indivisibles,  introduced  by  CaodUriuM  in  tie  year 
1635.  Unfortunately,  demonstrations  npon  sounder  principles  would 
sot  accord  with  the  brevity  of  this  Course. 


847 


may  two  sections  parallel  to  the  bases,  and  equidistant  from 
them.  Then,  by  the  last  two  theorems,  the  section  pq  is 
equal  to.  the  base,  ab,  and  the  section  rs  equal  to  the  base 
bb.  But  the  bases,  ab,  db,  are  equal,  by  the  hypothesis  ; 
therefore  the  sections  pq,  rs,  are  equal  also.  In  like  manner, 
it  may  be  shown,  that  any  other  corresponding  sections  are 
equal  to  one  another. 

Since  then  every  section  in  the  prism  ac  is  equal  to  its 
corresponding  seetion  in  the  prism  or  cylinder  df,  the  prisms 
and  cylinder  themselves,  which  are  composed  of  an  equal 
number  of  all  those  equal  sections,  must  also  be  equal. 

Q.  K.  D. 

Corol.  Every  prism,  or  cylinder,  is  equal  to  a  rectangular 
parallelopipedon,  of  an  equal  base  and  altitude. 


THEOREM  CIZ. 


Rectangular  parallelopipedons,  of  equal  altitudes,  are  to 
each  other  as  their  bases3". 

Let  ac,  eo,  be  two  rectan- 
gular parallelopipedons,  having 
the  equal  altitudes  ad,  eh  ; 
then  will  the  solid  ac  be  to  the 
solid  bo,  as  the  base  ab  is  to  the 
base  bp. 


Q   R  5  C 

HO 


A  LIS' 


For,  let  the  proportion  of  the 
base  ab  to  the  base  ef,  be  that 
of  any  one  number  m  (3)  to 

any  other  number  n  (2).  And  conceive  ab  to  be  divided 
into  m  equal  parts,  or  rectangles,  ai,  lk,  mb  (by  dividing  an 
into  that  number  of  equal  parts,  and  drawing  il,  km,  paral- 
lel to  bit).  And  let  ef  be  divided,  in  like  manner,  into  n 
equal  parts,  or  rectangles,  eo,  pf  :  all  of  these  parts,  of  both 
bases,  being  mutually  equal  among  themselves.  And  through 
the  lines  of  division  Jet  the  plane  sections  lb,  ms,  pv,  pass 
parallel  to  aq,  et. 

Then  the  parallelopipedons  ar,  ls,  mc,  ev,  pg,  are  aU 
equal,  having  equal  bases  and  altitudes.  Therefore  the  solid 
ac  ia  to  the  solid  eg,  as  the  number  of  parts  in  the  former, 
to  the  number  of  equal  parts  in  the  latter ;  or  as  the  number 


*  Here,  also,  the  principle  of  former  notes  may  readily  be, 
the  case  of  ineommeasorablef. 


848  GBOBBTRT. 

of  parts  in  ab  to  the  number  of  equal  parts  in  Br,  that  is,  as 
the  base  ab  to  the  base  bf.   q.  b.  d. 

Carol.  From  this  theorem,  and  the  corollary  to  the  last,  it 
appears  that  all  prisms  and  cylinders  of  equ  Jl  altitudes,  are 
to  each  other  as  their  bases ;  every  prism  and  cylinder  being 
equal  to  a  rectangular  parallelopipeaon  of  an  equal  base  and 
altitude. 


THEOREM  CZ. 


V 


Rectangular  parallelopipedons,  of  equal  bases,  are  to  each 
other  as  their  altitudes. 

Let  ab,  cd,  be  two  rectan-  n 
gular  parallelopipedons,  stand, 
ing  on  the  equal  bases  ae,  cf  ; 
then  will  the  solid  ab  be  to  the 
solid  cd,  as  the  altitude  eb  is  to 
the  altitude  fd. 

For,  let  ag  be  a  rectangular 
parallelopipedon  on  the  base  **  ^ 

ab,  and  its  altitude  eg  equal  to  the  altitude  fd  of  the  solid 

CD. 

Then  ag  and  cd  are  equal,  being  prisms  of  equal  bases  and 
altitudes.  But  if  hb,  hg,  be  considered  as  bases,  the  solids 
ab,  ag,  of  equal  altitude  ah,  will  be  to  each  other  as  those 
bases  hb,  hg.  But  these  bases  hb,  hg,  being  parallelograms 
of  equal  altitude  he,  are  to  each  other  as  their  bases  eb, 
bo  ;  therefore  the  two  prisms,  ab,  ag,  are  to  each  other  as 
the  lines  eb,  eg.  But  ag  is  equal  to  cd,  and  eg  equal  to  fd  ; 
consequently  the  prisms  ab,  cd,  are*to  each  other  as  their  al<* 
titudes,  eb,  fd  ;  that  is,  ab  :  cd  :  :  eb  :  fd.    q.  e.  d. 


Corol.  1.  From  this  theorem,  and  the  corollary  to  theorem 
108,  it  appears,  that  all  prisms  and  cylinders,  of  equal  bases, 
are  to  one  another  as  their  altitudes.  * 

Corol.  2.  Because,  by  corollary  1,  prisms  and  cylinders 
are  as  their  altitudes,  when  their  bases  are  equal.  And  by 
the  corollary  to  the  last  theorem,  they  are  as  their  bases, 
when  their  altitudes  are  equal.  Therefore,  universally, 
when  neither  are  equal,  they  are  to  one  another  as  the  pro- 
duct of  their  bases  and  altitudes.  And  hence  also  these 
products  are  the  proper  numeral  measures  of  their  quantities 
or  magnitudes. 


THEOREMS. 


849 


THEOREM  CXI. 


Sdolaji  prisma  and  cylinders  are  to  each  other,  at  the 
cubes  of  their  altitudes,  or  of  any  other  like  linear  dimensions. 

Let  abcd,  efgh,  be  two  similar 
prisms ;  then  will  the  prism  cd  be 
to  the  prism  oh,  as  ab3  to  ef3  or 
ad3  to  EH3. 

For  the  solids  are  to  each  other 
as  the  product  of  their  bases  and 
altitudes  (th.  110,  cor.  2),  that  is, 
as  ac  •  ad  to  so  •  ih.  But  the 
bases,  being  similar  planes,  are  to  each  other  as  the  squares 
of  their  like  sides,  that  is,  ac  to  eg  as  ab3  to  ef1;  therefore 
the  solid  cd  is  to  the  solid  oh,  as  ab3  .  ad  to  ef3  .  eh.  But 
bd  and  fh,  being  similar  planes,  hare  their  like  sides  pro. 

portional,  that  is,  ab  :  ef  :  :  ad  :  eh,  -  or  ab3  : 

ef3  :  :  ad3  :  eh3  :  therefore  ab3  .  ad  :  ef3  .  eh  :  :  ab3  :  ef3, 
or  :  :  ad3  :  eh3  ;  conseq.  the  solid  cd  :  solid  oh  :  :  ab3  :  ef3  : : 
ad3  :  eh3,    a.  E.  D. 


B 


THEOREM  CXII. 

In  any  pyramid,  a  section  parallel  to  the  base  is  similar  to 
the  base  ;  and  these  two  planes  are  to  each  other  as  the 
squares  of  their  distances  from  the  vertex. 

Let  abod  be  a  pyramid,  and  efo  a  sec. 
tion  parallel  to  the  base  bcd,  also  aih  a 
line  perpendicular  to  the  two  planes  at  h 
and  i :  then  will  bd,  eg,  be  two  similar 
planes,  and  the  plane  bd  will  be  to  the 
plane  eg,  as  ah1  to  ai3. 

For,  join  ch,  fi.  Then  because  a  plane 
cutting  two  parallel  planes,  makes  parallel 
sections  (th.  105),  therefore  the  plane  abc, 
meeting  the  two  parallel  planes  bd,  eg,  makes  the  sections 
bc,  ef,  parallel  :  In  like  manner,  the  plane  acd  makes  the 
sections  cd,  fg  parallel.  Again,  because  two  pair  of  parallel 
lines  make  equal  angles  (tb.  104),  the  two  ef,  fg,  which 
are  parallel  to  bc,  cd,  make  the  angle  efo  equal  the  angle 
bcd.  And  in  like  manner  it  is  shown,  that  each  angle  in 
the  plane  eg  is  equal  to  each  angle  in  the  plane  bd,  and  con- 
sequently those  two  planes  are  equiangular. 


OBOXBTBY. 


Again,  the  three  lines  as,  ac,  ad,  making  with  the 
parallels  bc,  bf,  and  cd,  fo,  equal  angles  (th.  14),  and 
*  we  angles  at  a  being  eommon,  the  two  triangles  abc,  ad, 
are  equiangular,  as  also  the  two  triangles  acd,  afg,  and 
.%fm  therefore  their  like  sides  proportional,  namelyt  *  -  -  - 
40  f  ajt  ; :  bo  :  bf  : .  2  cd  :  re.  And  in  like  manner  it 
way  be  shown,  that  all  the  lines  in  the  plane  fo,  are  pro- 
portional to  all  the  corresponding  lines  in  the  base  bd. 
Hence  these  two  planes,  haying  their  angles  equal,  and  their 
sides  proportional,  are  similar,  by  def.  68. 

But,  similar  planes  being  to  each  other  as  the  squares  of 
their  like  sides,  the  plane  bd  :  bo  :  :  bc9  :  bf?,  or  :  {  ac9  : 
AT*,  by  what  is  shown  above.  Also,  the  two  IfAPttfAf* 
.abc,  aif,  having  the  angles  h  and  1  right  ones  ph.  m\ 
wad  the  angle  a  common,  are  equiangular,  and  have  there- 
fore their  luce  sides  proportional,  namely,  ac  :  af  : :  ah  :  Afc 
or  AC*  ;  af*  : :  Ad9 :  ai9.  Consequently  the  two  planes  bd, 
30,  which  are  as  the  former  squares  ac9,  af8,  will  be  also  as 
the  latter  squares  ah3,  ai9,  that  is  bd  :  bo  : : 

AH9  :  AI9.     Q.  E.  D. 

THEOREM  CX1II. 

In  a  cone,  any  section  parallel  to  the  base  is  a  circle ;  and 
this  section  is  to  the  base,  as  the  squares  of  their  distances 
from  the  vertex. 

Let  abod  be  a  cone,  and  ohi  a  secti  on  A. 
parallel  to  the  base  bcd  ;  then  will  ghi 
be  a  circle,  and  bcd,  obi,  will  be  to  each 
other,  as  the  squares  of  their  distances 
from  the  vertex. 

For,  draw  alf  perpendicular  to  the  two 
parallel  planes  ;  and  let  the  planes  ace, 
adb,  pass  through  the  axis  of  the  cone 
akb,  meeting  the  section  in  the  three  points 

,     H,  I,  K. 

9  Then,  since  the  section  ohi  is  parallel  to  the  base  bcd,  and 

the  planes  ck,  dk,  meet  tbem,  hk  is  parallel  to  cb,  and 
IK  to  ps  (th.  105).  And  because  the  triangles  formed  by 
these  lines  are  equiangular,  kh  :  bc  : :  ax  :  ab  :  :  ki  :  bd. 
But  bc  is  equal  to  bd,  being  radii  of  the  same  circle  ;  there- 
fore xi  is  also  equal  to  kh.  And  the  same  may  be  shown  of 
driy  other  lines  drawn  from  the  point  k  to  the  perimeter  of 
the  section  ohi,  which  is  therefore  a  circle  (def.  44). 

Again,  bv  similar  triangles,  al  :  af  : :  ax  :  ab,  or 
;  ;  XI :  bd,  hence  al9  :  af3  ; :  ki9  :  bd9  ;  but  ki9  :  ed1  : 2 


THEOREMS. 


circle  ohi  :  circle  bcd  (tb.  OS)  ;  therefore  al9  :  af3  : : 
circle  obi  :  circle  bcd.    q.  e.  d. 


THEOREM  CXIV. 


All  pyramids,  and  cones,  of  equal  bases  and  altitudes,  are 
equal  to  one  another. 

Let  abc,  def,  be 
any  pyramids  and 
cone,  of  equal  bases 
bc,  ef,  and  equal 
altitudes  ao,  dh  : 
then  will  the  pyra- 
mids and  cone  abc 
and  def,  be  equal. 

For,  parallel  to  the  bases  and  at  equal  distances  \x,  do, 
from  the  vertices,  suppose  the  planes  ik,  lm,  to  be  drawn. 

Then,  by  the  two  preceding  theorems,  - 

do*  :  dh8  :  :  lm  :  ef,  and 
an3  :  ao2  : :  ik  :  bc. 

But  since  an-,  ao2,  are  equal  to  do3,  dh3,  respectively, 
therefore  ik  :  bc  :  :  lm  :  ef.  But  bc  is  equal  to  ef, 
by  hypothesis  :  therefore  ik  is  also  equal  to  lm. 

In  like  manner  it  is  shown,  that  any  other  sections,  at 
equal  distance  from  the  vertex,  are  equal  to  each  other. 

Since  then,  every  section  in  the  cone,  is  equal  to  the  cor- 
responding  section  in  the  pyramids,  and  the  heights  are  equal, 
the  solids  abc,  def,  composed  of  all  those  sections,  must  be 
equal  also.    q.  e.  d. 


THEOREM  CXV. 

Every  pyramid  is  the  third  part  of  a  prism  of  the  same  base 
and  altitude. 

Let  abcdef  be  a  prism,  and  bdef  a 
pyramid,  on  the  same  triangular  base  def  : 
then  will  the  pyramid  bdef  be  a  third  part 
of  the  prism  abcdef. 

For,  in  the  planes  of  the  three  sides  of 
the  prism,  draw  the  diagonals  bf,  bd,"  cd. 
Then  the  two  planes  bdf,  bcd,  divide  the 
whole  prism  into  the  three  pyramids  bdef, 
dabc,  dbcf,  which  are  proved  to  be  all  equal  to  one  another, 
as  follows. 

Since  the  opposite  ends  of  the  prism  are  equal  to  eu&Vk^fabT, 


V 


Mt  OBOJCXTBY. 

the  pyramid  whoM  base  is  abc  and  vertex  d,  if  equal  to  the 
pyramid  whose  base  is  dbf  and  vertex  b  (th.  114),  being 
pyramids  of  equal  base  and  altitude. 
'  But  the  latter  pyramid,  whose  base  is  dbf  and  vertex  B, 
is  the  wne  solid  as  the  pyramid  whose  base  is  bxf  and 
vertex  n,  and  this  is  equal  to  the  third  pyramid  whose  base 
is  bcf  and  vertex  d,  being  pyramids  of  the  same  altitude  and 
equal  bases  bef,  bcf. 

Consequently  all  the  three  pyramids,  which  compose  the 
prism,  are  equal  to  each  other,  and  each  pyramid*  is  the 
third  part  of  the  prism,  or  the  prism  is  triple  of  the  pyramid. 

4.  X.  D. 

Hence  also,  every  pyramid,  whatever  its  figure  may  be,  is 
the  third  part  of  a  prism  of  the  same  base  and  attitudes 
since  the  base  of  the  prism,  whatever  be  its  figure,  my  be 
divided  into  triangles,  and  the  whole  solid  into  triangular 
prisms  and  pyramids. 

Cord.  Any  cone  is  the  third  part  of  a  cylinder,  or  of  a 
prism,  of  equal  base  and  altitude  ;  since  it  has  been  proved 
that  a  cylinder  is  equal  to  a  prism,  and  a  cone  equal  to  a 
pyramid,  of  equal  base  and  altitude. 

Scholium.  Whatever  has  been  demonstrated  of  the  pro- 
portionality  of  prisms,  or  cylinders,  holds  equally  true  of 
pyramids,  or  cones ;  the  former  being  always  triple  the 
latter ;  viz}  that  similar  pyramids  or  cones  are  as  the  cubes 
of  their  like  linear  sides,  or  diameters,  or  altitudes,  fcc. 
And  the  same  for  all  similar  solids  whatever,  viz.  that  they 
are  in  proportion  to  each  other,  as  the  cubes  of  their  like 
linear  dimensions,  since  they  are  composed  of  pyramids  every 
way  similar. 

THEOREM  CXVI. 

If  a  sphere  be  cut  by  a  plane,  the  section  will  be  a  circlet. 

Let  the  sphere  abbf  be  cut  by  the  plane  B 
aub  ;.then  will  the  section  adb  be  a  circle* 

If  the  section  pass  through  the  centre  of 
the  sphere,  then  will  the  distance  from  the 
centre  to  every  point  in  the  periphery  of 
that  section  be  equal  to  the  radius  of  the 
sphere,  and  consequently  such  section  is  a 

carafe.   Such,  in  truth,  is  the  circle  safb  ¥   

in  the  figure. 

Draw  the  chord  ab,  or  diameter  of  the  section  adb  ;  per* 
psndicnhr  to  which,  or  to  the  said  section,  draw  the  axis  of 


# 


THKOSXM8.  358 

the  sphere  ecgf,  through  the  centre  c,  which  will  bisect  the 
chord  ab  in  the  point  «  (th.  41).  Also,  join  ca,  cb  ;  and 
draw  cd,  od,  to  any  point  d  in  the  perimeter  of  the  sec- 
tion ADB. 

Then,  because  co  is  perpendicular  to  the  plane  adb,  it  is 
perpendicular  both  to  ga  and  od  (def.  90).  So  that  coa, 
cod  are  two  right-angled  triangles,  having  the  perpendi- 
cular co.  common,  and  the  two  hypothenuses  ca,  cd,  equal, 
being  both  radii  of  the  sphere ;  therefore  the  third  sides  ga, 
gd,  are  also  equal  (cor.  2,  th.  34).  In  like  manner  it  is 
shown,  that  any  other  line,  drawn  from  the  centre  o  to  the 
circumference  of  the  section  adb,  is  equal  to  ga  or  gb  ;  con- 
sequently that  section  is  a  circle. 

Scholium.  The  section  through  the  centre,  having  the 
same  centre  and  diameter  as  the  sphere,  is  called  a  great 
circle  of  the  sphere  ;  the  other  plane  sections  being  little 
circles. 

THEOREM.  CXVn. 

Evert  sphere  is  two.thirds  of  its  circumscribing  cylinder. 

Let  abcd  be  a  cylinder,  circumscribing    \       J  g 
the  sphere  efgh  ;  then  will  the  sphere 
sfgh  be  two-thirds  of  the  cylinder  abcd.  0 

For,  let  the  plane  ac  be  a  section  of  the 
sphere  and  cylinder  through  the  centre  i. 
Join  ai,  bi.  Also,  let  fih  be  parallel  to 
ad  or  bc,  and  eig  and  kl  parallel  to  ab 
or  dc,  the  base  of  the  cylinder ;  the  latter  ■ 
line  kl  meeting  bi  in  m,  and  the  circular  section  of  the 
sphere  in  w.  « 
-  Then,  if  the  whole  plane  hfbc  be  conceived  to  revolve 
about  the  line  rf  as  an  axis,  the  square  fg  will  describe 
a  cylinder  ag,  and  the  quadrant  ifg  will  describe  a  hemi- 
sphere efg,  and  the  triangle  ifb  will  describe  a  cone  lab. 
Also,  in  the  rotation,  the  three  lines  or  parts  kl,  kit,  km,  as 
radii,  will  describe  corresponding  circular  sections  of  those 
solids,  namely,  kl  a  section  of  the  cylinder,  kn  a  section  of 
the  sphere,  and  km  a  section  of  the  cone. 

Now,  fb  being  equal  to  n  or  ig,  and  kl  parallel  to  fb, 
then  by  similar  triangles  ik  is  equal  to  km  (th.  82^~>  And 
since,  in  the  right-angled  triangle  ikn,  in*  is  equal  to  ik1 
+  kn3  (th.  34)  ;  and  because  kl  is  equal  to  the  radius  io 
or  in,  and  km  =  ik,  therefore  kl2  is  equal  to  km3  +  xir*9 
or  the  square  of  the  longest  radius,  of  tto  8t&~V\t&\^ 

Vol.  I  •  46 


864  GEOMETRY. 

sections,  is  equal  to  the  sum  of  t^e  squares  of  the  two  others* 
And  because  circles  are  to  each  other  as  the  squares  of  their 
diameters,  or  of  their  radii,  therefore  the  circle  described  by 
kl  is  equal  to  both  the  circles  described  by  km  and  kn  ;  or 
the  section  of  the  cylinder,  is  equal  to  both  the  corresponding 
sections  of  the  sphere  and  cone.  And  as  this  is  always  the. 
case  in  every  parallel  position  of  kl,  it  follows,  that  the  cy- 
linder eb,  which  is  composed  of  all  the  former  sections,  is 
equal  to  the  hemisphere  efg  and  cone  iab,  which  are  com- 
posed  of  all  the  latter  sections. 

But  the  cone  iab  is  a  third  part  of  the  cylinder  eb  (cor.  2, 
th.  115)  ;  consequently  the  hemisphere  efg  is  equal  to  the 
remaining  two-thirds  ;  or  the  whole  sphere  efgh  equal  to 
two-thirds  of  the  whole  cylinder  abcd.    q.  e.  d. 

Coral.  1.  A  cone,  hemisphere,  and  cylinder  of  the  same 
base  and  altitude,  are  to  each  other  as  the  numbers  1,  2,  3. 

CoroL  2.  All  spheres  are  to  each  other  as  the  cubes  of 
their  diameters ;  all  these  being  like  parts  of  their  circum- 
scribing cylinders. 

CoroL  3.  From  tho  foregoing  demonstration  it  also  ap- 
pears, that  the  spherical  zone  or  frustum  egxf,  is  equal  to 
the  difference  between  the  cylinder  eglo  and  the  cone  in  a, 
all  of  the  same  common  height  ik.  And  that  the  spherical 
segment  pfn,  is  equal  to  the  difference  between  the  cylinder 
ablo  and  the  conic  frustum  aqmb,  all  of  the  same  common 
altitude  fk. 


355 


PROBLEMS. 


PROBLEM  I. 

To  bisect  a  line  ab  ;  that  is,  to  divide  it  into  two  equal  parts. 

From  the  two  centres  a  and  b,  with  any  c 
equal  radii,  describe  arcs  of  circles,  inter, 
secting  each  other  in  c  and  d  ;  and  draw 
the  line  cd,  which  will  bisect  the  given  line  A 
ab  in  the  point  e. 

For,  draw  the  radii  ac,  bc,  ad,  bd. 
Then,  because  all  these  four  radii  are  equal, 
and  the  side  cd  common,  the  two  triangles 
acd,  bcd,  are  mutually  equilateral  :  consequently  they  are 
also  mutually  equiangular  (th.  5),  and  have  the  angle  ace 
equahto  the  angle  bce. 

Hence,  the  two  triangles  ace,  bce,  having  the  two  sides 
ac,  ce,  equal  to  the  two  sides  bc,  ce,  and  their  contained 
angles  equal,  are  identical  (th.  1),  and  therefore  have  the 
side  ae  equal  to  eb.    q.  e.  d. 


problem  n. 

To  bisect  an  angle  bac*. 

From  the  centre  a,  with  any  radius,  de- 
scribe an  arc,  cutting  off  the  equal  lines 
ad,  ae  ;  and  from  the  two  centres  d,  e, 
with  the  same  radius,  describe  arcs  inter, 
secting  in  f  ;  then  draw  af,  which  will 
bisect  the  angle  a  as  required. 


*  A  very  ingenious  instrument  for  trisecting  an  angle,  is  described  in 
the  Mechanic's  Magasioe,  No.  22,  p.  344. 


A 


For,  join  df,  if.  Then \  the  two  triangles  isr,  a»f. 
baring  the  two  aide*  ad9  df,  equal  to  the  two  ae,  bf  (beiag 
equal  radii),  and  the  side  af  common,  they  are  mutuafiy 
equilateral ;  consequently  they  are  also  mutually  equiangular 
(th.  5),  and  have  the  angle  bat  equal  to  the  angle  oaf. 

Scholium.  In  the  same  manner  is  an  arc  of  a  circle  bi- 
sected. 

fboblex  m. 

At  a  given  point  o,  in  a  line  ab,  to  erect  a  perpendicular. 

From  the  given  point  o,  with  any  radius, 
cut  off  any  equal  parts  cd,  cb,  of  the  given 
line  ;  and,  from  the  two  centres  d  and  s, 
with  any  one  radius,  describe  arcs  intersect-  _ 
ing  in  f  ;  then  join  of,  which  will  be  per-  -4tT"0"TtB 
pendicular  as  required* 

For,  draw  the  two  equal  radii  df,  ef.  Then  the  two 
triangles  cdf,  cef,  having  the  two  sides  cd,  df,  equal  to 
the  two  ok,  bf,  and  cf  common,  are  mutually  equilateral ; 
consequently  they  are  also  mutually  equiangular  (th.  5),  and 
have  the  two  adjacent  angles  at  c  equal  to  each  other ;  there- 
fore the  line  cf  is  perpendicular  to  ab  (def.  11). 

Otherwise* 

Whew  the  given  point  c  is  near  the  end  of  the  line* 

From  any  point  d  assumed  above  the 
line,  as  a  centre,  through  the  given  point 
c  describe  a  circle,  cutting  the  given  line 
at  e  ;  and  through  e  and  the  centre  d, 
draw  the  diameter  edf;  then  join  cf, 
which  will  be  the  perpendicular  required. 

For  the  angle  at  c,  being  an  angle  in  a  semicircle,  is  a 
right  angle,  and  therefore  the  line  cf  is  a  perpendicular  (by 
def.  15). 

PROBLEM  IV. 

From  a  given  point  a,  to  let  fall  a  perpendicular  on  a  given 
line  bc. 

From  the  given  point  a  as  a  centre,  with 
any  convenient  radius,  describe  an  arc,  cut- 
ting  the  given  line  at  the  two  points  d  and 
b  ;  and  from  (he  two  centres  d,  e,  with  any 
radius,  describe  two  arcs,  intersecting  at  f  ; 
then  draw  aof,  which  will  be  perpendicular 
to  bc  as  required. 


S07 


For,  draw  the  equal  radii  ad,  as,  and  df,  ep.  Then  the 
two  triangles  adf,  aef,  having  the  two  sides  ad  df,  equal 
to  the  two  ab,  bf,  and  af  common,  are  mutually  equilateral ; 
consequently  they  are  also  mutually  equiangular  (th.  5),  and 
have  the  angle  dag  equal  the  angle  bag.  Hence  then,  the 
two  triangles  ado,  abg,  having  the  two  sides  ad,  ao,  equal 
to  the  two  ab,  ao,  and  their  included  angles  equal,  are  there- 
fore equiangular  (th.  1),  and  have  the  angles  at  o  equal ; 
consequently  ao  is  perpendicular  to  bc  (def.  11). 

Otherwise. 

WftEN  the  given  point  is  nearly  opposite  the  end  of  the  line. 

From  any  point  d,  in  the  given  line 
bc,  as  a  centre,  describe  the  arc  of  a 
circle  through  the  given  point  a,  cutting 
bc  in  e  ;  and  from  the  centre  e,  with  the 
radius  ba,  describe  another  arc,  cutting 
the  former  in  f  ;  then  draw  agf,  which 
will  be  perpendicular  to  bc  as  required.  3f 

For,  draw  the  equal  radii  da,  df,  and  ea,  bf.  Then  the 
two  triangles  dak,  dfe,  will  be  mutually  equilateral ;  conse- 
quently they  are  also  mutually  equiangular  (th.  5),  aqd  have 
the  angles  at  d  equal.  Hence,  the  two  triangles  dag,  dfo, 
having  the  two  sides  da,  dg,  equal  to  the  two  df,  do,  and 
the  included  angles  at  d  equal,  have  also  the  angles  at  o 
equal  (th.  1)  ;  consequently  those  angles  at  o  are  right 
angles,  and  the  line  ag  is  perpendicular  to  dg. 


PROBLEM  V. 


At  a  given  point  a,  in  a  line  ab,  to  make  an  angle  equal  to 
a  given  angle  c. 

From  the  centres  a  and  c,  with  any  one  •  jg^ 

radius,  describe  the  arcs  de,  fg.  Then, 
with  radios  de,  and  centre  f,  describe  an 


arc,  cutting  fg  in  g.    Through  g  draw       C  D 
the  line  ag,  and  it  will  form  the  angle  re*  ~ 
quired.  \ 

For,  conceive  the  equal  lines  or  radii,       j±  jtjj 
db,  fg,  to  be  drawn.    Then  the  two  trian- 
gles CDs,  afg,  being  mutually  equilateral,  are  mutually  equi- 
angular (th.  5),  and  have  the  angle  at  a  eqiud  to  ta*  vu^a  fe» 


868 


GEOMETRY* 


PROBLEM  VI. 


Through  a  given  point  a,  to  draw  a  line  parallel  to  a  given 
line  bo. 

From  the  given  point  a  draw  a  line  ad  EA 
to  an j  point  in  the  given  line  bc.  Then 
draw  the  line  eaf  making  the  angle  at  a 
equal  to  the  angle  at  d  (by  prob.  5)  ;  bo  j5~C 
shall  ef  be  parallel  to  bc  as  required. 

For,  the  angle  d  being  equal  to  the  alternate  angle  a,  the 
lines  bc,  ef,  are  parallel,  by  th.  13. 


problem  vii. 


To  divide  a  line  ab  into  any  proposed  number  of  equal 
parts. 

Draw  any  other  line  ac,  forming  any 
angle  with  the  given  line  ab  ;  on  which  EVA 
set  off  as  many  of  any  equal  parts  ad,  de,  \ 
ef,  fc,  as  tho  line  ab  is  to  be  divided  into.  3\V  \  \ 

Join  bc  ;  parallel  to  which  draw  the  other  ^IHCKB 
lines  fg,  eh,  di  :  then  these  will  divide  ab 
in  the  manner  as  required. — For  those  parallel  lines  divide 
both  the  sides  ab,  ac,  proportionally,  by  th.  82. 


PROBLEM  Vin. 

To  find  a  third  proportional  to  two  given  lines  ab,  ac. 

Place  the  two  given  lines  ab,  ac, 

forming  any  angle  at  a  ;  and  in  ab  take        A  B 

also  ad  equal  to  ac.    Join  bc,  and        A-  ^ 
draw  de  parallel  to  it ;  so  will  ae  be 
the  third  proportional  sought. 

For,  because  of  the  parallels,  bc,  de,       A  2)  '0 

the  two  lines  ab,  ac,  are  cut  propor- 
tionally (th.  82) ;  so  that  ab  :  ac  : :  ad  or  ac  :  ae  ;  there- 
fore ae  is  the  third  proportional  to  ab,  ac. 

PROBLEM  IX. 

To  find  a  fourth  proportional  to  three  lines  ab,  ac,  ad. 

Place  two  of  the  given  lines  ab,  ac,  making  any  angle  at 
A ;  also  place  ad  on  ab.    Join  bc  ;  and  parallel  to  it  draw 


PROBLEMS. 


850 


de  :  so  shall  ae  be  the  fourth  propor- 
tional as  required. 

For,  because  of  the  parallels  bc,  de, 
the  two  sides  ab,  ac,  are  cut  propor- 
tionally (th.  82)  ;  so  that  .... 
ab  :  ac  : :  ad  :  ae. 

PROBLEM  X. 

To  find  a  mean  proportional  between  two  lines  ab,  bc. 

Place  ab,  bc,  joined  in  one  straight 
line  ac  :  on  which,  as  a  diameter,  describe 
the  semicircle  adc  ;  to  meet  which  erect 
the  perpendicular  bd  ;  and  it  will  be  the 
mean  proportional  sought,  between  ab  and 
bc  (by  cor.  th.  87).  . 

problem  XI. 

To  find  the  centre  of  a  cii 

Draw  any  chord  ab  ;  and  bisect  it  p 
pendicularly  with  the  line  cd,  which  will 
a  diameter  (th.  41,  cor.).  Therefore 
bisected  in  o,  will  give  the  centre,  as  reqi 
ed. 

PROBLEM  XII. 

To  describe  the  circumference  of  a  circle  through  three  given 
points  a,  b,  c. 

From  the  middle  point  b  draw  chords 
ba,  bc,  to  the  two  other  points,  and  bi-  •"-Hs^JL-JK--* 
sect  these  chords  perpendicularly  by  lines  ^^T^Si 
meeting  in  o,  which  will  be  the  centre.  A<^^y[^5\C 
Then  from  the  centre  o,  at  the  distance       I    /q\  J 
of  any  one  of  the  points,  as  oa,  describe       \.  J 
a  circle,  and  it  will  pass  through  the  two 
other  points  b,  c,  as  required. 

For  the  two  right-angled  triangles  oad,  obd,  having  the 
sides  ad,  db,  equal  (by  constr.),  and  od  common,  with  the 
included  right  angles  at  d  equal,  have  their  third  sides  oa, 
ob,  also  equal  (th.  1).  And  in  like  manner  it  is  shown  that 
oc  is  equal  to  ob  or  oa.  So  that  all  the  three  oa,  ob,  go*  tid- 
ing equal,  will  be  radii  of  the  same  circta. 


OROMSTRY. 


PROBLEM  XIII. 

To  draw  a  tangent  to  a  circle,  through  a  given  point 

When  the  given  point  a  is  in  the  circum- 
ference of  the  circle  :  Join  a  and  the  centre 
o ;  perpendicular  to  which  draw  bac,  and  it 
will  be  the  tangent,  by  th.  46. 

But  when  the  given  point  a  is  out  of  the 
circle :  Draw  ao  to  the  centre  o ;  on  which 
as  a  diameter  describe  a  semicircle,  cutting 
the  given  circumference  in  d  ;  through  R 
which  draw  badc,  which  will  be  the  tangent  1 
cs  required. 

For,  join  do.  Then  the  angle  ado,  in  a 
semicircle,  is  a  right  angle,  and  consequent- 
ly ad  is  perpendicular  to  the  radius  do,  or 
is  a  tangent  to  the  circle  (th.  46). 

PROBLEM  xiv. 

On  a  given  line  b  to  describe  a  segment  of  a  circle,  to  contain 
a  given  angle  c. 

At  the  ends  of  the  given  line  make 
angles  dab,  dba,  each  equal  to  the 
given  angle  c.  Then  draw  ae,  be, 
perpendicular  to  ad,  bd  ;  and  with  the 
centre  e,  and  radius  ea  or  eb,  describe 
a  circle ;  so  shall  afb  be  the  segment 
required,  as  any  angle  f  made  in  it  will 
be  equal  to  the  given  angle  c. 

For,  the  two  lines  ad,  bd,  being 
perpendicular  to  the  radii  ea,  eb  (by  constr.),  are  tangents 
to  the  circle  (th.  46) ;  and  the  angle  a  or  b,  which  is  equal  to 
the  given  angle  c  by  construction,  is  equal  to  the  angle  f  in 
the  alternate  segment  aeb  (th.  53). 

problem  xv. 

To  cut  off  a  segment  from  a  circle,  that  shall  contain  a  given 
angle  c. 

Draw  any  tangent  ab  to  the  given 
circle  ;  and  a  chord  ad  to  make  the  E 
angle  dab  equal  to  the  given  angle  c ; 
then  dka  will  be  the  segment  required, 
any  angle  s  made  in  it  being  equal  to 
the  given  angle  c. 


PROBLEMS. 


861 


For  the  angle  a,  made  by  the  tangent  and  chord,  whioh 
ia  equal  to  the  given  angle  c  by  construction,  is  also  equal  to 
any  angle  a  in  the  alternate  segment  (th.  63). 


problem  zvi. 

To  make  an  equilateral  triangle  on  a  given  line  ab. 

From  the  centres  a  and  b,  with  the 
distance  ab,  describe  arcs,  intersecting  in 
c.  Draw  ac,  bo,  and  abc  will  be  the 
equilateral  triangle. 

For  the  equal  radii,  ac,  bc,  are,  each  of 
them,  equal  to  ab. 


problem  xvn. 

To  make  a  triangle  with  three  given  lines  ab,  ac,  bc 

With  the  centre  a,  and  distance  ac, 
describe  an  arc.  With  the  centre  b,  and 
distance  bc,  describe  another  arc,  cutting 
the  former  in  c.  Draw  ab,  bc,  and  abc 
will  be  the  triangle  required. 

For  the  radii,  or  sides  of  the  triangle, 
ac,  bc,  are  equal  to  the  given  lines  ac, 
ac,  by  construction. 


A 


PROBLEM  XVIII. 

To  make  a  square  on  a  given  line  ab. 

Raise  ad,  bc,  each  perpendicular  and  j>_ 
equal  to  ab  ;  and  join  dc  ;  so  shall  abcd  be 
the  square  sought. 

For  all  the  three  sides  ab,  ad,  bc,  are 
equal,  by  the  construction,  and  dc  is  equal 
and  parallel  to  ab  (by  th.  24) ;  so  that  all  the 
four  sides  are  equal,  and  the  opposite  ones  are  parallel. 
Again,  the  angle  a  or  b,  of  the  parallelogram,  being  a  right 
angle,  the  angles  are  all  right  ones  (cor.  1,  th.  22).  Hence, 
then,  the  figure,  having  all  its  sides  equal,  and  alL'towGq&a* 
right,  is  a  square  (def.  34). 

Vol.  I  47 


GEOMETRY. 


problem  XIX. 


To  make  a  rectangle,  or  a  parallelogram,  of  a  given  length 
and  breadth,  ab,  bc. 

Erect  ad,  bc,  perpendicular  to  ab,  and 
each  equal  to  bc  ;  then  join  dc,  and  it  is 
done. 

The  demonstration  is  the  same  as  the    _ 

last  problem.  B— —  C 

And  in  the  same  manner  is  described  any  oblique  paral- 
lelogram,  only  drawing  ai>  and  bc  to  make  the  given  oblique 
angle  with  ab,  instead  of  perpendicular  to  it. 


PROBLEM  xx* 

To  inscribe  a  circle  in  a  given  triangle  abc. 

Bisect  any  two  angles  a  and  b,  with 
the  two  lines  ad,  bd.  From  the  inter- 
section d,  which  will  be  the  centre  of 
the  circle,  draw  the  perpendiculars  db, 
df,  DU,  and  they  will  be  the  radii  of  the 
circle  required. 

For,  since  the  angle  dae  is  equal  to 
the  angle  dag,  and  the  angles  at  e,  o, 
right  angles  (by  const r.),  the  two  triangles,  adb,  ado,  are 
equiangular ;  and,  having  also  the  side  ad  common,  they  are 
identical,  and  have  the  sides  de,  do,  equal  (th.  2).    In  like 
manner  it  is  shown,  that  df  is  equal  to  de  or  do. 

Therefore,  if  with  the  centre  d,  and  distance  de,  a  circle 
be  described,  it  will  pass  through  all  the  three  points,  e,  f,  g, 
in  which  points  also  it  will  touch  the  three  sides  of  the  tri- 
angle (th.  46),  because  the  radii  de,  df,  do,  are  perpendicu- 
lar to  them. 

PROBLEM  XXI. 

To  describe  a  circle  about  a  given  triangle  abc. 

Bisect  any  two  sides  with  two  of  the 
perpendiculars  de,  df,  do,  and  d  will 
be  the  centre. 

For,  join  da,  db,  dc  Then  the  two 
right-angled  triangles  dae,  dbe,  have 
the  two  sides,  de,  ea,  equal  to  the  two 
de,  eb,  and  the  included  angles  at  e 
equal :  those  two  triangles  are  therefore 


P10BLEHS. 


383 


identical  (th.  1%  and  have  the  side  da.  equal  to  db.  In  like 
manner  it  it  shown,  that  dc  is  also  equal  to  da  or  db.  So 
that  all  the  three  da,  db,  dc,  being  equal,  they  are  radii  of 
a  circle  passing  through  a,  b,  and  c. 


fgOBLBH  XXII. 


To  inscribe  an  equilateral  triangle  in  a  given  circle. 

Through  the  centre  c  draw  any  diameter  a 
ab.    From  the  point  b  as  a  centre,  with  the  y^/fV^N, 
radius  bc  of  the  given  circle,  describe  an   f  /  |\  \ 
arc  dcb.   Join  ad,  as,  db,  and  ade  is  the  f  X-JsA  ) 
equilateral  triangle  sought  x^^l^^v/ 

For,  join  db,  dc,  bb,  bc.    Then  dcb  ^  X^TT^^E 
is  an  equilateral  triangle,  having  each  side  ^jj^ 
equal  to  the  radius  of  the  given  circle.  In 
like  manner,  bcb  is  an  equilateral  triangle.    But  the  angle 
ade  is  equal  to  the  angle  abb  or  cbe,  standing  on  the  same 
arc  ae  ;  also  the  angle  akd  is  equal  to  the  angle  cbd,  on  the 
same  arc  ad  ;  hence  the  triangle  dab  has  two  of  its  angles, 
adb,  aed,  equal  to  the  angles  of  an  equilateral  triangle,  and 
therefore  the  third  angle  at  a  is  also  equal  to  the  same  ;  so 
that  the  triangle  is  equiangular,  and  therefore  equilateral. 


PROBLEM  XXIII. 


To  inscribe  a  square  in  a  given  circle* 


Draw  two  diameters  ac,  rd,  crossing 
at  right  angles  in  the  centre  e.  Then 
join  the  four  extremities  a,  b,  c,  d,  with 
right  lines,  and  these  will  form  the  in- 
scribed square  abcd. 

For  the  four  right-angled  triangles 
aeb,  bp.c,  ced,  dea,  are  identical  be- 
cause they  have  the  sides  ea,  eb,  ec,  ed, 
all  equal,  being  radii  of  the  circle,  and 
the  four  included  angles  at  e  all  equal, 
being  right  angles,  by  the  construction.  Therefore  all  their 
third  sides  ab,  bc,  cd,  da,  are  equal  to  one  another,  and  the 
figure  abcd  is  equilateral.  Also,  all  its  four  angles,  a,  b,  c,  d, 
are  right  ones,  being  angles  in  a  semicircle.  Cooaec^t&Vj 
the  figure  is  a  square. 


GEOMETRY. 


PROBLEM  XXIV. 


To  describe  a  square  about  a  given  circle. 

Draw  two  diameters  ac,  bd,  crossing 
at  right  angles  in  the  centre  s.  Then 
through  their  four  extremities  draw  fg, 
ib,  parallel  to  ac,  and  fi,  oh,  parallel 
to  bd,  and  they  will  form  the  square 

FGHI. 

For,  the  opposite  sides  of  parallelo- 
grams being  equal,  fg  and  in  are  each 
equal  to  the  diameter  ac,  and  fi  and  on  each  equal  to  the 
diameter  bd  ;  so  that  the  figure  is  equilateral.  Again,  be- 
cause the  opposite  angles  of  parallelograms  are  equal,  all  the 
four  angles  f,  c,  h,  i,  are  right  angles,  being  equal  to  the 
opposite  angles  at  e.  So  that  the  figure  fgmi,  having  its 
sides  equal,  and  its  angles  right  ones,  is  a  square,  and  its  sides 
touch  the  circle  at  the  four  points  a,  b,  c,  d,  being  perpen- 
dicular to  the  radii  drawn  to  those  points. 


PROBLEM  XXV. 


To  inscribe  a  circle  in  a  given  square. 

Bisect  the  two  sides  fg,  fi,  in  the  points  a  and  b  (last  fig.). 
Then  through  these  two  points  draw  ac  parallel  to  fc  or  ih, 
and  bd  parallel  to  fi  or  gh.  Then  the  point  of  intersection 
x  will  be  the  centre,  and  the  four  lines  ea,  eb,  ec,  ed,  radii 
of  the  inscribed  circle. 

For,  because  the  four  parallelograms  ef,  eg,  kh,  ei,  have 
their  opposite  sides  and  angles  equal,  therefore  all  the  four 
lines  ea,  eb,  ec,  ed,  are  equal,  being  each  equal  to  half  a 
side  of  the  square.  So  that  a  circle  described  from  the  centre 
E,  with  the  distance  ea,  will  pass  through  all  the  points 
a,  b,  c,  d,  and  will  be  inscribed  in  the  square,  or  will  touch 
its  four  sides  in  those  points,  because  the  angles  there  are 
right  ones. 

PROBLEM  XXVI. 

To  describe  a  circle  about  a  given  square. 
(See  fig.  Prob.  xxiii.) 
Draw  the  diagonals  ac,  bd,  and  their  intersection  s  will 
be  the  centre. 

For  the  diagonals  of  a  square  bisect  each  other  (th.  40), 
making  ea,  eb,  ec,  ed,  all  equal,  and  consequently  these 
are  radii  of  a  circle  naasin^  vUtou^U  the  four  points  a,  b,  c,  p. 


FftOBUMS. 


805 


FKOBLEM  XXVII. 

To  cut  a  given  line  in  extreme  and  mean 

Let  ab  be  the  given  line  to  be  divided 
in  ex  I  re  me  and  mean  ratio,  that  is,  so  as 
that  the  whole  line  may  be  to  the  greater 
part,  as  the  greater  part  is  to  the  less  part. 

Draw  bc  perpendicular  to  AR/and  equal 
to  half  ab.  Join  ac  ;  and  with  centre  c 
and  distance  cb,  describe  the  circle  bd  ; 
then  with  centre  a  and  distance  ad,  de- 
scribe the  arc  dk  ;  so  shall  ab  be  divided 
in  e  in  extreme  and  mean  ratio,  or  so  that 
ab  :  ae  :  :  ab  :  eb. 

Produce  ac  to  the  circumference  at  f.  Then,  auf  being 
a  secant,  and  ab  a  tangent,  because  b  is  a  right  angle  :  there- 
fore the  rectangle  af  .  ad  is  equal  to  ab9  (cor.  1,  th.  61) ;  con* 
sequently  the  means  and  extremes  of  these  are  proportional 
(th.  77),  viz.  ab  :  af  or  ad  +  df  :  :  ad  :  ab.  But  ab 
is  equal  to  ad  by  construction,  and  ab  =  2bc  =  df  ; 
therefore,  ab  :  ae  +  ab  :  :  ae  :  ab  ; 

and  by  division,  ab  :  ae  :  :  ae  :  eb. 

PROBLEM  XXVIII. 

To  inscribe  an  isosceles  triangle  in  a  given  circle,  that 
shall  have  each  of  the  angles  at  the  base  double  the  angle  at 
the  vertex.  ^ 


Draw  any  diameter  ab  of  the  given 
circle ;  and  divide  the  radius  cb,  in  the 
point  d,  in  extreme  and  mean  ratio,  by  the 
last  problem.  From  the  point  b  apply  the 
chords  be,  bf,  each  equal  to  the  greater 
part  cd.  Then  join  ae,  af,  ef  ;  and  akf 
will  be  the  triangle  required. 


For,  the  chords  be,  bf,  being  equal, 
their  arcs  are  equal ;  therefore  the  supplemental  arcs  and 
chords  ae,  af,  are  also  equal ;  consequently  the  triangle  aef 
is  isosceles,  and  has  the  angle  e  equal  to  the  angle  f  ;  alto 
the  angles  at  u  are  right  angles. 

Draw  cf  and  df.  Then,  bc  :  cd  :  :  cd  :  bd,  or 
bc  :  bf  :  :  bf  :  bd  by  constr.  And  ba  :  bf  :  :  bf  :  bo 
(by  th.  87).  But  bc  =  £ba  ;  therefore  bo  =  £bo  =  go  \ 
therefore  the  two  triangles  gbf,  ©df,  ara  VtouvicaX  VJ3fc%\V 


ratio. 


A 


t 


c 

806     .  C  GEOMETRY. 

£ 

and  each  equiangular  to  arf  and  agf  (th.  87).  Therefore 
their  doubles,  bfd,  afe,  are  isosceles  and  equiangular,  as 
well  as  the  triangle  hcf  ;  having  the  two  sides  bc,  cf,  equal, 
and  the  angle  b  common  with  the  triangle  bfd.  But  cd 
is  =  df  or  bf  ;  therefore  the  angle  c  =  the  angle  dpc 
(th.  4)  ;  consequently  the  angle  bdf,  which  is  equal  to  the 
sum  of  these  two  equal  angles  (th.  16),  is  double  of  one  of 
them  c  ;  or  the  equal  angle  b  or  ceb  double  the  angle  c. 
So  that  cbf  is  an  isosceles  triangle,  having  each  of  its  two 
equal  angles  double  of  the  third  angle  c.  Consequently  the 
triangle  arf  (which  it  has  been  shown  is  equiangular  to  the 
triangle  c  f)  has  al*o  each  of  its  angles  at  the  base  double 
the  angle  a  at  the  vertex. 

PROBLEM  XXIX. 

To  inscribe  a  regular  pentagon  in  a  given  circle. 

Inscribe  the  isosceles  triangle  abc, 
having  each  of  the  angles  abc,  acr, 
double  the  angle  bac  (prob.  28).  Then 
bisect  the  two  arcs  adr,  arc,  in  the 
points  d,  e  ;  and  draw  the  chords  ad,  dr, 
ar,  ec,  so  shall  adrce  be  the  inscribed 
equilateral  pentagon  required. 

For,  because  equal  angles  stand  on 
equal  arcs,  and  double  angles  on  double  arcs,  also  the  angles 
abc,  acb,  being  each  double  the  angle  bac,  therefore  the 
arcs  adr,  arc,  subtending  the  two  former  angles,  are  each 
double  the  arc  bc  subtending  the  latter.  And  since  the  two 
former  arcs  are  bisected  in  d  and  r  it  follows  that  all  the 
five  arcs  ad,  dr,  rc,  ck,  ea,  are  equal  to  each  other,  and  con- 
sequently  the  chords  also  which  subtend  them,  or  the  live 
sides  of  the  pentagon,  are  a1  I  equal. 

Note.  In  (he  constniction,  the  points  d  and  e  are  most 
easily  found,  by  applying  bd  and  ce  each  equal  to  bc. 

problem  xxx. 

To  inscribe  a  regular  hexagon  in  a  circle. 

Apply  the  radius  ao  of  the  given  circle 
as  a  chord,  ar,  rc,  cd,  &c.  quite  round 
the  circumference,  and  it  will  complete 
the  regular  hexagon  abcdef. 

Draw  the  radii  ao,  ho,  co,  do,  eo,  fo, 
completing  six  equal  triangles  ;  of  which 
any  one,  as  abo,  being  equilateral  (by 
const r.)  its  three  angles  are  all  equal  (cor. 
2,  tb.  3),  and  any  one  of  them,  as  aob,  is  one-third  of  the' 


FB0BLEMS. 


987 


whole,  or  of  two  right  angles  (th.  17),  or 
one-sixth  of  four  right  angles.  But  the 
whole  circumference  is  the  measure  of  four 
right  angles  (cor.  4,  th.  6).  Therefore  the 
arc  ar  is  one.sixth  of  the  circumference  of 
the  circle,  and  consequently  its  chord  ab  one 
aide  of  an  equilateral  hexagon  inscribed  in  the 
circle.    And  the  same  of  the  other  chords. 

Corel.  The  side  of  a  regular  hexagon  is  equal  to  the 
radius  of  the  circumscribing  circle,  or  to  the  chord  of  one- 
sixth  part  of  the  circumference*. 

PROBLEM  XXXI. 

To  describe  a  regular  pentagon  or  hexagon  about  a  circle. 

Izv  the  given  circle  inscribe  a  regular 
polygon  of  the  same  name  or  number 
of  sides,  as  abcdk,  by  one  of  the  fore- 
going problems.  Then  to  all  its  angular 
points  draw  tangents  (by  prob.  13),  and 
these  will  form  the  circumscribing  poly- 
gon required. 

For  all  the  chords,  or  sides  of  the 
inscribed  figure,  ab,  bc,  dec.  being  equal,  and  all  the  radii 
oa,  ob,  dec.  being  equal,  all  the  vertical  angles  about  the 
point  o  are  equal.  But  the  angles  oef,  oaf,  oao,  obg, 
made  by  the  tangents  and  radii,  are  right  angles  ;  therefore 
oef  +  oaf  =  two  right  angles,  and  oao  +  obg  =  two  right 
angles  ;  consequently,  also,  aoe  +  afe  =  two  right  an- 
gles, and  oab  +  a«b  «  two  right  angles  (cor.  2,  th.  18). 
Hence,  then,  the  angles  aoe  +  afe  being  =  aob  +  aob,  of 
which  aob  is  =  aoe  ;  consequently  the  remaining  angles  r 
and  o  are  also  equal.  In  the  same  manner  it  is  shown,  that  all 
Hthe  angles  f,  g,  h,  i,  k,  are  equal. 

Again,  the  tangents  from  the  same  point  fe,  fa,  are  equal, 
as  also  the  tangents  ao,  gb,  (cor.  2,  th.  61)  ;  and  the  angles 
f  and  g  of  the  isosceles  triangles  afe,  agb,  are  equal,  as  well 
as  their  opposite  sides  ae,  ab  ;  consequently  those  two  tri- 
angles are  identical  (th.  1),  and  have  their  other  sides  ef,  fa, 
ag,  gb,  all  equal,  and  fg  equal  to  the  double  of  any  one  of 
them.  In  like  manner  it  is  shown,  that  all  the  other  sides 
gh,  hi,  ik,  ki,  are  equal  to  fg,  or  double  of  the  tangents  gb, 
bh,  &c. 


*  The  bent  way  to  describe  n  polygon  of  any  number  of  sides,  the 
length  of  one  side  being  given,  is  to  find  the  radius  of  the  cATOraMafa» 
log  circle  by  means  of  the  table,  at  pa.  413,  and  \ta  t*\»  «t  \*. 


368 


GKOKETBY. 


Hence,  then,  the  circumscribed  figure  is  both  equilateral 
and  equiangular,  which  was  to  be  shown. 

Cord*  The  inscribed  circle  touches  the  middle  of  the  sides 
of  the  polygon. 

PSOBLEX  XXXII. 


To  inscribe  a  circle  in  a  regular  polygon. 

Bisect  any  two  sides  of  the  polygon 
by  the  perpendiculars  go,  fo,  and  their 
intersection  o  will  be  the  centre  of  the 
inscribed  circle,  and  oo  or  of  will  be  the 
radius. 

For  the  perpendiculars  to  the  tangents 
af,  ao,  pass  through  the  centre  (cor.  r 
th.  47) ;  and  the  inscribed  circle  touches  C 
the  middle  points  f,  o,  by  the  last  corollary.  Also,  the  two 
sides,  ao,  ao,  of  the  right-angled  triangle  aog,  being  equal 
to  the  two  sides  af,  ao,  of  the  right-angled  triangle  aof,  the 
third  sides  of,  oo,  will  also  be  equal  (cor.  th.  45).  There- 
fore  the  circle  described  with  the  centre  o  and  radius  og,  will 
pass  through  f,  and  will  touch  the  sides  in  the  points  g  and  f. 
And  the  same  for  all  the  other  sides  of  the  figure. 


PROBLEM  XXXIII. 


To  describe  a  circle  about  a  regular  polygon. 

Bisect  any  two  of  the  angles,  c  and  d, 
with  the  lines  co,  do  ;  then  their  inter, 
section  o  will  be  the  centre  of  the  circum- 
scribing circle ;  and  or,  or  od,  will  be  the 
radius. 

For,  draw  ob,  oa,  of,  &c.  to  the  an- 
gular points  of  the  given  polygon.  Then 
the  triangle  ocd  is  isosceles,  having  the  angles  at  c  and  D 
equal,  being  the  halves  of  the  equal  angles  of  the  polygon 
BCD,  cdb  ;  therefore  their  opposite  sides  co,  do,  are  equal, 
(th.  4).  But  the  two  triangles  oci>,  ocb,  having  the  two  sides 
oc,  cd,  equal  to  the  two  oc,  cb,  and  the  included  angles  ocd, 
Ocb,  also  equal,  will  be  identical  (th.  1),  and  have  their  third 
•ides  bo,  od,  equal.  In  like  manner  it  is  shown,  that  all  the 
lines  oa,  ob,  oc,  od,  or,  aro  equal.  Consequently  a  circle 
described  with  the  centre  o  fjnd  radius  oa,  will  pass  through 
all  the  other  angular  points,  b,  c,  d,  dec.  and  will  circum- 
msribe  the  polygon. 


PROBLEMS. 


PROBLEM  XXXIV. 


To  make  a  square  equal  to  the  sum  of  two  or  more  given 
squares. 

Let  ib  and  ac  be  the  sides  of  two 
given  squares.  Draw  two  indefinite 
lines  ap,  aq,  at  right  angles  to  each 
other ;  in  which  place  the  sides  ab,  ac, 
of  the  given  squares  ;  join  bc  ;  then  a 
square  described  on  bc  will  be  equal  to 
the  sum  of  the  two  squares  described 
on  ab  and  ac  (th.  34). 

In  the  same  manner,  a  square  may  be  made  equal  to  the 
sum  of  three  or  more  given  squares.  For,  if  ab,  ac,  ad,  be 
taken  as  the  sides  of  the  ffiven  squares,  then,  making  ae=bc, 
ad  =  ad,  and  drawing  he,  it  is  evident  that  the  square  on  db 
will  be  equal  to  the  sum  of  the  three  squares  on  ab,  ac,  ad. 
And  so  on  for  more  squares. 


PROBLEM  XXXV. 


To  make  a  square  equal  to  the  difference  of  two  given 
squares. 

Let  ab  and  ac,  taken  in  the  same 
straight  line,  be  equal  to  the  sides  of  the 
two  given  squares. — From  the  centre  a, 
with  the  distance  ab,  describe  a  circle ; 
and  make  cd  perpendicular  to  ab,  meet-  A  C  *B 

ing  the  circumference  in  d  :  so  shall  a  square  described  on 
cd  be  equal  to  ad'j — ac\  or  ab3 — ac9,  as  required  (cor.  th.  34). 


PROBLEM  XXXVI. 


To  make  a  triangle  equal  to  a  given  quadrangle  abcd. 

Draw  the  diagonal  ac,  and  parallel  j)  q 

to  it  de,  meeting  ba  produced  at  e,  and  /P  J9\ 

join  ce  ;  then  will  the  triangle  ceb  be  st* 
equal  to  the  given  quadrilateral  abcd.  •/ 


XL 


For,  the  two  triangles  ace,  acd,         E     A  B 
being  on  the  same  base  ac,  and  between 
the  same  parallels  ac,  de,  are  equal  (th.  25)  ;  therefore,  if 
abc  be  added  to  each,  it  will  make  bce  eqaaUo  kwct>  Ujl^v 
•Vol.  I.  48 


870  OBOMBTBY. 


PROBLEM  XXXVII. 


To  make  o  triangle  equal  to  a  given  pentagon  abcds. 

Draw  da  and  db,  and  also  ef,  co, 
parallel  to  them,  meeting  ab  produced 
at  v  and  o ;  then  draw  dp  and  do  ;  so 
shall  the  triangle  dfo  be  equal  to  the 
given  pentagon  abcde. 

For  the  triangle  dfa  =  dka,  and 
the  triangle  dob  =  dcb  (th.  25)  ; 
therefore,  by  adding  dab  to  the  equals, 
the  sumw  are  equal  (ax.  2),  that  is,  dab  +  dap  +  dbg»  dab 
+  dae  +  dbc,  or  the  triangle  dfo  =  to  the  pentagon  . 


problem  xxxviii. 


To  make  a  rectangle  equal  to  a  given  triangle  abc. 

Bisect  the  base  ab  in  d  :  then  raise 
de  and  bf  perpendicular  to  ab,  and 
meeting  cf  parallel  to  ab,  at  e  and  f  : 
so  shall  dp  be  the  rectangle  equal  to  the 
given  triangle  abc  (by  cor.  2,  th.  26). 


problem  xxxix. 

To  make  a  square  equal  to  a  given  rectangle  abcd. 

Produce  one  side  ab,  till  be  be 

equal  to  the  other  side  bc.    On  ae  as  O  .  V 

a  diameter  describe  a  circle,  meeting  3)    rJ  j^,... 

bc  produced  at  f  :  then  will  bp  be  the  \    \  I 

side  of  the  square  bfoh,  equal  to  the  f__  j  !  j 

given  rectangle  bd,  as  required ;  as  AH  B  E 
appears  by  cor.  th.  87,  and  th.  77. 


871 


APPLICATION  OF  ALGEBRA 


TO 


GEOMETRY. 


Whbx  it  is  proposed  to  resolve  a  geometrical  problem 
algebraically,  or  by  algebra,  it  is  proper,  in  the  first  place, 
to  draw  a  figure  that  shall  represent  the  several  parts  or  con- 
ditions of  the  problem,  and  to  suppose  that  figure  to  be  the 
true  one.  Then  having  considered  attentively  the  nature 
of  the  problem,  the  figure  is  next  to  be  prepared  for  a  solu- 
tion,  if  necessary,  by  producing  or  drawing  such  lines  in  it  as 
appear  most  conducive  to  that  end.  This  done,  the  usual 
symbols  or  letters,  for  known  and  unknown  quantities,  are 
employed  to  denote  the  several  parts  of  the  figure,  both  the 
known  and  unknown  parts,  or  as  many  of  them  as  necessary, 
as  also  such  unknown  line  or  lines  as  may  be  easiest  found, 
whether  required  or  not.  Then  proceed  to  the  operation, 
by  observing  the  relations  that  the  several  parts  of  the  figure 
have  to  each  other  ;  from  which,  and  the  proper  theorems 
in  the  foregoing  elements  of  geometry,  make  out  as  many 
equations  independent  of  each  other,  as  there  are  unknown 
quantities  employed  in  them  :  the  resolution  of  which  equa- 
tions, in  the  same  manner  as  in  arithmetical  problems,  will 
determine  the  unknown  quantities,  and  resolve  the  problem 
proposed. 

As  no  general  rule  can  be  given  for  drawing  the  lines,  and 
selecting  the  fittest  quantities  to  substitute  for,  so  as  always 
to  bring  out  the  most  simple  conclusions,  because  different 
problems  require  different  modes  of  solution  ;  the  best  way 
to  gain  experience,  is  to  try  the  solution  of  the  same  problem 
in  different  ways,  and  then  apply  that  which  succeeds  best, 
to  other  cases  of  the  same  kind,  when  they  afterwards  occur. 
The  following  particular  directions,  however,  may  be  of 
some  use. 

l«t,  In  preparing  the  figure,  by  drawing  lines,  let  them  be 
either  parallel  or  perpendicular  to  other  lines  in  the  figure, 
or  so  as  to  form  similar  triangles.  And  if  an  angle  be  given, 
it  will  be  proper  to  let  the  perpendicular  be  opposite  to  that 
-angle,  and  to  fall  from  one  end  of  a  given  line,  if  ^awfttat* 


372 


APPLICATION  or  ALGEBRA 


2d,  In  selecting  the  quantities  proper  to  substitute  for, 
those  are  to  be  chosen,  whether  required  or  not,  which  lie 
nearest  the  known  or  given  parts  of  the  figure,  and  by  means 
of  which  the  next  adjacent  parts  may  be  expressed  by  addi- 
tion and  subtraction  only,  without  using  surds. 

3d,  When  two  lines  or  quantities  are  alike  related  to  other 
parts  of  the  figure  or  problem,  the  best  way  is,  not  to  make 
use  of  either  of  them  separately,  but  to  substitute  for  their 
sum,  or  difference,  or  rectangle,  or  the  sum  of  their  alternate 
quotients,  or  for  some  line  .or  lines,  in  the  figure,  to  which 
they  have  both  the  same  relation. 

4th,  When  the  area,  or  the  perimeter,  of  a  figure  is  given, 
or  such  parts  of  it  as  have  only  a  remote  relation  to  the  parts 
required  :  it  is  sometimes  of  use  to  assume  another  figure 
similar  to  the  proposed  one,  having  one  side  equal  .to  unity, 
or  some  other  known  quantity.  For,  hence  the  other  parts 
of  the  figure  may  be  round,  by  the  known  proportions  of  the 
like  sides,  or  parts,  and  so  an  equation  be  obtained.  For 
examples,  take  the  following  problems. 

PROBLEM  I. 

In  a  right-angled  triangle,  having  given  the  base  (8),  and 
the  sum  of  the  hypotenuse  and  perpendicular  (9)  ;  to  find 
both  these  two  sides. 

Let  abc  represent  the  proposed  triangle 
right-angled  at  b.  Put  the  base  ab  =  3  =  b, 
and  the  sum  ac  +  bc  of  the  hypothenuse 
and  perpendicular  =  9  =  s  ;  also,  let  x  de- 
note the  hypothenuse  ac,  and  y  the  perpen- 
dicular BC. 

Then  by  the  question  -  .  .  x  +  y  =  s, 
and  by  theorem  34,  -  -  .  .  x*  =  y%  +  b*, 
By  tr»:nspos.  y  in  the  1st  equ.  gives x  =  s  —  yt 
This  value  of  x  substi.  in  the  2d, 

gives     ....       s^-Qsy  +  y1  =  f  +  b*9 
Taking  away  y*on  both  sides  leaves  j*...  2sy  =  b*, 
By  transpos.  Usy  and  6j,  gives  -  s^b'  =  Usy, 

*3  —  b2 

And  dividing  by  2s,  gives   -    -    — —  =  y  =  4  =  bc. 
Hence  x  =  *  —  y  =  5  =  ac. 

^  N.  B.  In  this  solution,  and  the  following  ones,  the  nota. 
tkm  is  made  by  using  as  many  unknown  letters,  x  and  jr,  as 


TO  OEOMKBT. 


378 


there  are  unknown  tides  of  the  triangle,  a  separate  letter  for 
each  ;  in  preference  to  using  only  one  unknown  letter  for 
one  side,  and  expressing  the  other  unknown  side  in  terms 
of  that  letter  and  the  given  sum  or  difference  of  the  sides  ; 
though  this  latter  way  would  render  this  solution  shorter  and 
sooner  ;  because  the  former  way  gives  occasion  for  more  and 
better  practice  in  reducing  equations ;  which  is  the  very  end 
and  reason  for  which  these  problems  are  given  at  all. 

PROBLsk'lI. 

In  a  right-angled  triangle,  having  given  the  hypothenuse  (5)  ; 
and  the  sum  of  the  base  and  perpendicular  (7) ;  to  find  both 
these  two  sides. 

Let  abc  represent  the  proposed  triangle,  right-angled  at 
B.  Put  the  given  hypothenuse  ac  =  5  =  a,  and  the  sum 
ab  +  bc  of  the  base  and  perpendicular  =  7  =  s  ;  also  let  x 
denote  the  base  ab,  and  y  the  perpendicular  bc. 

Then  by  the  question    -    -    -    x  +  y  =  st 
and  by  theorem  34      ...   x*+  y*=  a2, 
By  transpos.  y  in  the  1st,  gives   x  =  s  —  y, 
By  substitu.  this  value  for  x,  gives  **—  2sy  4-  2ya  =  a\ 
By  transposing  s*,  gives  -    -    2y*  —  2sy  —  a*  —  s7, 
By  dividing  by  2,  gives  -   -     y2—  sy  =  \a*  —  ±s*9 
By  completing  the  square,  gives  y*  —  sy  +  Js*  =  }a*  —  \s*f 
By  extracting  the  root,  gives  -   y  —  \s  =  %/(ia3  ~"  i*9) 
By  transposing  is,  gives  -    -   y  =  J*  ±  y/\\a2  —  \s*)  = 

4  and  3,  the  values  of  x  and  y. 

problem  in. 

In  a  rectangle,  having  given  the  diagonal  (10\  and  the  peri- 
meter,  or  sum  of  all  the  four  sides  (28)  ;  to  find  each  of  the 
sides  severally* 

Let  abcd  be  the  proposed  rectangle  ; 
and  put  the  diagonal  ac  =  10  =  d,  and 
half  the  perimeter  ab  +  bc  or  ad  + 
dc  —  14  =.  a  :  also  put  one  side  ab  =  ar, 
and  the  other  side  bc  =  y.  Hence,  by 
right-nngled  triangles,  -  -  -  .  -  x*  +  y7  =  d\ 
And  by  the  question  -  -  -  .  -  x+y  —  a, 
Then  by  transposing  y  in  the  2d,  gives  x  —  a  —  y, 
This  value  substituted  in  the  1st,  gives   a?  —  <SUu)V*^=^ 


874 


APPLICATION  OF  ALGEBRA 


Transposing  a*,  gives    .    -    2y' —  2ay  =  d1 — «*, 
And  dividing  by  2,  gives    -     y1  —  ay  =  \dl —  ±a\ 
By  completing  the  square,  it  is  y*  — ay  +  \a*  =  \<P —  \a\ 
And  extracting  the  root,  gives  y  —  ±a  =  y/(±dl  —  Ja1), 
And  transposing  \a,  gives    -    y  =  £a  2:  v^(i^J — l*1)3^ 
or  6,  the  values  of  x  and  y. 


problem  IV. 

Having  given  the  base  anfoerpendicular  of  any  triangle  ;  to 
find  the  side  of  a  square  inscribed  in  the  same. 

Let  abc  represent  the  given  triangle,  q 
and  EFGit  its  inscribed  square.  Put  the 
base  ab  =■  by  the  perpendicular  cd  =  a, 
and  the  side  of  the  square  gf  or  on  = 
Di  x  ;  then  will  ci  =  cd  —  di  = 
a  —  x. 

Then,  because  the  like  lines  in  the 
similar  triangles  abc,  gpc,  are  propor- 
tional (by  theor.  84,  Geom.),  ab  :  cd  :  :  ge  :  ci,  that 
is,  6  :  a  :  :  x  :  a  —  x.  Hence,  by  multiplying  extremes  and 
means,  qb  —  bx  =  ax,  and  transposing  bx,  gives  ab  =  ax 

ab 

+  bx ;  then  dividing  by  a  +  b,  gives  x  =  a  ^  ^  =  gf  otch 

the  side  of  the  inscribed  square  :  which  therefore  is  of  the 
same  magnitude,  whatever  the  species  or  the  angles  of  the 
triangles  may  be. 


problem  v. 


In  an  equilateral  triangle,  having  given  the  lengths  of  the 
three  perpendiculars,  drawn  from  a  certain  point  within,  on 
the  tlirce  sides ;  to  determine  the  sides. 

Let  abc  represent  the  equilateral  tri- 
angle, and  oe,  df,  dg,  the  given  per- 
pendiculars from  the  point  d.  Draw  the 
lines  da,  dh,  dc,  to  the  three  angular 
points  ;  and  let  fall  the  perpendicular  cu 
on  the  base  ab.  Put  the  three  given  per- 
pendiculars, de  =  a,  df  =  b,  d<;  =  c, 
and  put  x  =  a  11  or  bii,  half  the  side  of 
the  equilateral  triangle.  Then  is  ac  or  bc  =  2.r,  and  by 
right-angled  triangles  the  perpendicular  cu  =  */(ac2  —  ah1) 


•S3T 


c 

)  - 

TO  GEOMETRY. 


375 


Now,  since  the  area  or  space  of  a  rectangle,  is  expressed 
by  the  product  of  the  buse  arid  height  (cor.  2,  th  81,  Geom.), 
and  that  a  triangle  is  equal  to  half  a  rectangle  of  equal  baso 
and  height  (cor.  1,  th.  ^6),  it  follows  that, 
the  whole  triangle  abc  is  =  Jab  X  cn  =  x  X  x  y/3  =  x2  ^3, 
the  tnungle  abd  =  Jab  X  do  =  x  X  c  =  cr, 
the  triangle  bcd  =■  Jbc  X  dk  =  x  X  a  =  ax, 
the  triangle  acd  =  \ac  X  df  =  *  X  b  =  bx. 
But  the  three  last  triangles  make  up,  or  are  equal  to,  the 
whole  former,  or  great  tnungle  ; 

that  is,  x*       =  ax  +  br  +  cx  ;  hence,  dividing  by  *,  gives 
r  y/3  =  a  +6   +  c,  and  dividing  by  ^/3,  gives 
a-f.  &  +  r 

x  =  6 — ,  half  the  side  of  the  triangle  sought. 

Also,  since  the  whole  perpendicular  cn  is  =-  x  y/3,  it  is 
therefore  =  a  +  b  +  c.  That  is,  the  whole  perpendicular 
cn,  is  just  equal  to  the  sum  of  all  the  three  smaller  perpen- 
diculars db  +  nr  +  do  taken  together,  wherever  the  point 
d  ii  situated. 

PROBLEM  VI. 

In  a  right-angled  triangle,  having  given  the  base  (3\  and 
the  difference  between  the  hypoihenuse  and  perpendicular 
(1)  ;  to  find  both  these  two  sides. 

PROBLEM  VII. 

In  a  right-angled  triangle,  having  given  the  hypothenuse 
5),  and  the  difference  between  the  base  and  perpendicular 
1)  ;  to  determine  both  these  two  sides. 

problem  viu. 

Having  given  the  area,  or  measure  of  the  space,  of  a  rect. 
angle,  inscribed  in  a  given  triangle  ;  to  determine  the  sides 
of  the  rectangle. 

problem  u. 

In  a  triangle,  having  given  the  ratio  of  the  two  sides, 
together  with  both  the  segments  of  the  base,  made  by  a  per- 
pendicular from  the  vertical  angle  ;  to  determine  the  sides  of  - 
the  triangle. 

problem  x. 

In  a  triangle,  having  given  the  base,  the  sum  of  the  other 
two  sides,  and  the  length  of  a  line  drawn  ftom\Yi«  <<i«*ta*\ 


376  APPLICATION  OF  ALGEBRA 

angle  to  the  middle  of  the  base  ;  to  find  the  sides  of  the 
triangle. 

PROBLEM  XI. 

In  a  triangle,  having  given  the  two  sides  about  the  verti- 
cal angle,  with  the  line  bisecting  that  angle,  and  terminating 
in  the  base  ;  to  find  the  base. 

PROBLEM  XII. 

To  determine  a  right-angled  triangle  ;  having  given  the 
lengths  of  two  lines  druwn  from  the  acute  angles,  to  the 
middle  of  the  opposite  sides. 

PROBLEM  XIII. 

To  determine  a  right-angled  triangle  ;  having  given  the 
perimeter,  and  the  radius  of  its  inscribed  circle. 

PHOBLEM  XIV. 

To  determine  a  triangle  ;  having  given  the  base,  the  per- 
pendicular, and  the  ratio  of  the  two  sides. 

PROBLEM  xv. 

To  determine  a  right-angled  triangle  ;  having  given  the 
hypothenuse,  and  the  side  of  the  inscribed  square. 

PROBLEM  XVI. 

To  determine  the  radii  of  three  equal  circles,  described  in 
a  given  circle,  to  touch  each  other  and  also  the  circum- 
ference of  the  given  circle. 

PROBLEM  XVII. 

In  a  right-angled  triangle,  having  given  the  perimeter,  or 
sum  of  all  the  sides,  and  the  perpendicular  let  fall  from  the 
right  angle  on  the  hypothenuse  ;  to  determine  the  triangle, 
that  is,  its  sides. 

PROBLEM  XVIII. 

To  determine  a  right-angled  triangle ;  having  given  the 
hypothenuse,  and  the  difference  of  two  lines  drawn  from  the 
two  acute  angles  to  the  centre  of  the  inscribed  circle. 


-$&~  i-$A  t&^h.  w-a+yi-  t  t 


I  "IT 


If- 


 hZe^dr^ 


1 


to 


TO  GEOMETRY.  377 
PROBLEM  XIX. 

To  determine  a  triangle  ;  having  given  the  base,  the  per- 
pendicular, and  the  difference  of  the  two  other  sides. 

PROBLEM  XX. 

To  determine  a  triangle  ;  having  given  the  base,  the  per- 
pendicular, and  the  rectangle  or  product  of  the  two  sides* 

PROBLEM  XXL 

To  determine  a  triangle  ;  having  given  the  lengths  of  three 
lines  drawn  from  the  three  angles,  io  the  middle  of  the  oppo* 
site  sides. 

PROBLEM  XXXI. 

In  a  triangle,  having  given  all  the  three  sides ;  to  find  the 
radius  of  the  inscribed  circle. 

PROBLEM  XXIII. 

To  determine  a  right-angled  triangle  ;  having  given  the 
aide  of  the  inscribed  square,  and  the  radius  of  the  inscribed 
circle. 

PROBLEM  XXIV. 

To  determine  a  triangle,  and  the  radius  of  the  inscribed 
circle  ;  having  given  the  lengths  of  three  lines  drawn  from 
the  three  angles,  to  the  centre  of  that  circle. 

PROBLEM  XXV. 

To  determine  a  right-angled  triangle  ;  having  given  the 
hypothenuse,  and  the  radius  of  the  inscribed  circle. 

PROBLEM  XXVI. 

To  determine  a  triangle  ;  having  given  the  base,  the  line 
bisecting  the  vertical  angle,  and  the  diameter  of  the  circum. 
scribing  circle. 


Vol.  I. 


49 


97 


PLANE  TRIGONOMETRY. 


DEFIMTIOX8. 

1.  Plank  Trigonometry  treats  of  the  relations  and  cal- 
culations  of  the  sides  and  angles  of  plane  triangles. 

2.  The  circumference  of  every  circle  (as  before  observed 
in  Geom.  Def.  56)  is  supposed  to  be  divided  into  360  equal 
parts,  called  Degrees  ;  also  each  degree  into  60  Minutes, 
and  each  minute  into  60  Seconds,  and  so  on.  Hence  a  se- 
micircle contains  180  degrees,  and  a  quadrant  90  degrees. 

3.  The  Measure  of  an  angle  (Def.  57,  Geom.)  is  an  arc 
-of  any  circle  contained  between  the  two  lines  which  form 
that  angle,  the  angular  point  being  the  centre  ;  and  it  is  esti- 
mated by  the  number  of  degrees  contained  in  that  arc. 

Hence,  a  right  angle,  being  measured  by  a  quadrant,  or 
quarter  of  the  circle,  is  an  angle  of  90  degrees  ;  and  the 
sum  of  the  three  angles  of  every  triangle,  or  two  right  an* 
gles,  is  equal  to  180  degrees.  Therefore,  in  a  right-angled 
triangle,  taking  one  of  the  acute  angles  from  90  degrees, 
leaves  the  other  acute  angle  ;  and  the  sum  of  the  two  angles, 
in  any  triangle,  taken  from  180  degrees,  leaves  the  third 
angle  ;  or  one  angle  being  taken  from  180  degrees,  leaves 
the  sum  of  the  other  two  angles. 

4.  Degrees  arc  marked  at  the  top  of  the  figure  with  a 
small  °,  minutes  with ',  seconds  with  *,  and  so  on.  Thus, 
57°  30'  12",  denote  57  degrees  30  minutes  and  12  seconds. 

5.  The  Complement  of  an  arc,  is 
what  it  wants  of  a  quadrant  or  90°. 
Thus,  if  ad  be  a  quadrant,  then  bd  is 
the  complement  of  the  arc  ab  ;  and, 
reciprocally,  ab  is  the  complement  of 
bd.  So  that,  if  ab  be  an  arc  of  50°,  & 
then  its  complement  bd  will  be  40°. 

6.  The  Supplement  of  an  arc,  is 
what  it  wants  of  a  semicircle,  or  180°.  T 
Thus,  if  ade  be  a  semicircle,  then 
bde  is  the  supplement  of  the  arc  ab  ;  and,  reciprocally,  ab 


DJEFiirrnoifs. 


87V 


is  the  supplement  of  the  arc  bde.  So  that,  if  ab  be  an  arc 
of  50°,  then  its  supplement  bob  will  be  130°. 

7.  The  Sine,  or  Right  Sine,  of  an  arc,  is  the  line  drawn 
from  one  extremity  of  the  arc,  perpendicular  to  the  diameter 
which  passes  through  the  other  extremity.  Thus,  bf  is  the 
sine  of  the  arc  ab,  or  of  the  supplemental  arc  bde.  Hence 
the  sine  (bf)  is  half  the  chord  (bo)  of  the  double  arc 
(bao). 

8.  The  Versed  Sine  of  an  arc,  is  the  part  of  the  diameter 
intercepted  between  the  arc  and  its  sine.  So,  af  is  the  versed 
sine  of  the  arc  ab,  and  ef  the  versed  sine  of  the  arc  edb. 

9.  The  Tangent  of  an  arc,  is  a  line  touching  the  circle  in 
one  extremity  of  that  arc,  continued  from  thence  to  meet  a 
line  drawn  from  the  centre  through  the  other  extremity  ; 
which  last  line  is  called  the  Secant  of  the  same  arc.  Thus, 
ah  is  the  tangent,  and  en  the  secant,  of  the  arc  ab.  Also, 
ei  is  the  tangent,  and  ci  the  secant,  of  the  supplemental  arc 
bob.  And  this  latter  tangent  and  secant  are  equal  to  the 
former,  but  are  accounted  negative,  as  being  drawn  in  an 
opposite  or  contrary  direction  to  the  former. 

10.  The  Cosine,  Cotangent,  and  Cosecant,  of  an  arc, 
are  the  sine,  tangent,  and  secant  of  the  complement  of  that 
arc,  the  Co  being  only  a  contraction  of  the  word  comple- 
ment Thus,  the  arcs  ab,  bi>,  bein  *  the  complements  of 
each  other,  the  sine,  tangent,  or  secant  of  the  one  of  these, 
is  the  cosine,  cotangent,  or  cosecant  of  the  other.  So,  bf, 
the  sine  of  ab,  is  the  cosine  of  bd  ;  and  bk,  the  sine  of  bd, 
is  the  cosine  of  ab  :  in  like  manner,  ah,  the  tangent  of  ab, 
is  the  cotangent  of  bd  ;  and  dl,  the  tangent  of  db,  is  the 
cotangent  of  ab  ;  also,  ch,  the  secant  of  ab,  is  the  cosecant 
of  bd  ;  and  cl,  the  secant  of  bd,  is  the  cosecant  of  ab. 

Cord.  Hence  several  important  properties  easily  follow 
from  these  definitions  ;  as, 

1st,  That  an  arc  and  its  supplement  have  the  same  sine, 
tangent,  and  secant  ?  but  the  two  latter,  the  tangent  und 
secant,  are  accounted  negative  when  the  arc  is  greater  than 
a  quadrant  or  90  degrees. 

2d,  When  the  arc  is  0,  or  nothing,  the  sine  and  tangent 
are  nothing,  but  the  secant  is  then  the  radius  oa,  the  least  it 
can  be.  As  the  arc  increases  from  0,  the  sines,  tangents, 
and  secants,  all  proceed  increasing,  till  the  arc  becomes  a 
whole  quadrant  ad,  and  then  the  sine  is  tkc  greatest  it  can 
be,  being  the  radius  en  of  the  circle ;  and  both  the  tangent 
and  secant  are  infinite. 

3d,  Of  any  arc  ab,  the  versed  sine  af,  and  cosine  bk, 
or  cf,  together  make  up  the  radius  ca  of  the  evecta.— 


•80 


FLAHK  TUOONOVXTBT. 


adius  ca,  the  tangent  ah,  and  the^  secant  ch,  form  a  right» 
angled  triangle  c  %  h.  So  also  do  the  radius,  sine,  and  conn** 
form  another  right-angled  triangle  chf  or  cbk.  As  also  the 
radius,  cotangent,  and  cosecant,  another  right-angled  triangle 
cdl.  And  all  these  right-angled  triangles  are  similar  to  each 
other. 

11.  The  sine,  tangent,  or 
secant  of  aa  angle,  is  the  sine, 
tangent,  or  secant  of  the  arc 
by  which  the  angle  is  mea- 
sured, or  of  tho  degrees,  dic- 
ta the  same  arc  or  angle. 

12.  The  method  of  con- 
structing the  scales  of  chords, 
sines,  tangents,  and  secants, 
usually  engraven  on  instru- 
ments, for  practice,  is  exhi- 
bited in  the  annexed  figure. 

13.  A  Trigonometrical 
Canon,  is  a  table  showing 
the  length  of  the  sine,  tan- 

Sent,  and  secant,  to  everyjg 
egree  and  m  minute  of  the 
quadrant,  with  respect  to  the 
radius,  which  is  expressed  by 
unity  or  1,  with  any  number 
of  ciphers.  The  logarithms 
ef  these  sines,  tangents,  and 
secants,  are  also  ranged  in  the 
tables  ;  and  these  are  most  commonly  used,  as  they  perform 
the  calculations  by  only  addition  and  subtraction,  instead  of 
the  multiplication  and  division  by  the  natural  sines,  etc.  ac- 
cording to  the  nature  of  logarithms.  Such  tables  of  log. 
sines  and  tangents,  as  well  as  the  logs  of  common  numbers, 
greatly  facilitate  trigonometrical  computations,  and  are  now 
very  common.  Among  the  most  correct  are  those  published 
by  the  author  of  this  Course. 


PROBLEM  I. 


To  compute  the  Natural  Sine  and  Cosine  of  a  Given  Arc. 

Tni9  problem  is  resolved  after  various  ways.  One  of  these 
is  as  follows,  viz.  by  means  of  the  ratio  between  the  diameter 


PBOBLSK*.  881 

and  circumference  of  a  circle,  together  with  the  known  series 
for  the  sine  and  cosine,  hereafter  demonstrated.    Thus,  the 
aemicircumference  of  the  circle,  whose  radius  is  1,  being 
3-14169^653589703  &c,  the  proportion  will  therefore  be, 
as  the  number  of  degrees  or  minutes  in  the  semicircle, 
is  to  the  degrees  or  minutes  in  the  proposed  arc, 
so  is  3  14169265  dec,  to  the  length  of  the  said  arc. 
This  length  of  the  arc  being  denoted  by  the  letter  a ;  and 
its  sine  and  cosine  by  «  and  c ;  then  will  these  two  be  ex- 
pressed by  the  two  following  series,  viz. 

_   _  jrr  ,  _a*_  a*   _ 

9     a      2.3  +  2.3.4.5  2.3.4.5.0.7 

=   a3  ,   a*        a7    ,  . 

°     6      120  5040 

2  ^2.3.4     2.3.4.5.6  T  C 
a9     o*  a8 
=  l— 2+34-720  +  &C- 

Exam.  1.  If  it  be  required  to  find  the  sine  and  cosine  of 
1  minute.  Then,  the  number  of  minutes  in  180°  being 
10800,  it  will  be  first,  as  10600  :  1  : :  3  14150205  dec.  : 
•000290888208665  =  the  length  of  an  arc  of  one  minute. 
Therefore,  in  this  case, 

a=  -0002908882 
and^a3=  -000000000004  dec. 
the  diflT.  \ss=    0002908882  the  sine  of  1  minute. 
Also,  from  1- 

take  ia*  =  0  0000000423079  dec. 

leaves  c  =  -9999999577  the  cosine  of  1  minute. 

Exam.  2.  For  the  sine  end  cosine  of  5  degrees. 
Here  as  1H)°  :  5«  :  :  3  141 59205  &c.  :  -08726646  =  a  the 
length  of  5  degrees.    Hence  a  ==  -08726K46 
—  Ja*  *  -  -00011076 
+  ^  as  =  -00000004 


these  collected  give  $  =  '08715574  the  sine  of  5\ 

And,  for  the  cosine,  1  =  1* 

—  ±a2  =  —  -00380771 
+        =  -00000241 


these  collected  give  c  = 


•99619470  the  cosine  of  5°. 


383 


PL  ARB  TBIGOXOXXTBY. 


After  the  same  manner,  the  sine  and  cosine  of  any  other 
arc  may  be  computed.  Rut  the  greater  the  arc  is,  the  slower 
the  series  will  converge,  in  which  case  a  greater  number  of 
terms  must  be  taken,  to  bring  out  the  conclusion  to  the  same 
degree  of  exactness. 

Or,  having  found  the  sine,  the  cosine  will  be  found  from 
it,  by  the  property  of  the  right-angled  triangle  cbf,  vis.  the 
cosine  cp  =  y/{cu* —  bp11),  or  c  =•  y/{l  —  ?). 

There  are  also  other  methods  of  constructing  the  canon 
of  sines  and  cosines,  which,  for  brevity's  sake,  are  here 
omitted  :  some  of  them,  however,  are  explained  under 
the  analytical  trigonometry  in  the  second  volume  of  this 
Course. 


problem  n. 

To  compute  the  Tangents  and  Secants. 

Tub  sines  and  cosines  being  known,  or  found  by  the 
foregoing  problem  ;  the  tangents  and  secants  will  be  easily 
found,  from  the  principle  of  similar  triangles,  in  the  follow, 
ing  manner : 

In  the  first  figure,  where,  of  the  arc  ab,  bf  is  the  sine, 
cf  or  bk  the  cosine,  ah  the  tangent,  ch  the  secant,  dl  the 
cotangent,  and  cl  the  cosecant,  the  radius  being  ca  or  cb  or 
cd  ;  the  three  similar  triangles  cfb,  cah,  cdl,  give  the  fol- 
lowing proportions : 

1**,  cf  :  fb  :  :  ca  :  ah  ;  whence  the  tangent  is  known, 
being  a  fourth  proportional  to  the  cosine,  sine,  and  radius. 

2d,  cp  :  cb  :  :  ca  :  ch;  whence  the  secant  is  known, 
being  a  third  proportional  to  the  cosine  and  radius :  or, 
being,  indeed,  the  reciprocal  of  the  cosine  when  the  radius 
is  unity. 

3d,  bf  :  fc  :  :  cd  :  dl  ;  whence  the  cotangent  is  known, 
being  a  fourth  proportional  to  the  sine,  cosine,  and  radius. 

Or,  aii  ;  ac  i  i  cd  :  dl  ;  whence  it  appears  that  the  co- 
tangent is  a  third  proportional  to  the  tangent  and  radius ; 
or  the  reciprocal  of  the  tangent  to  radius  1. 

4th  bf  :  bc  :  :  cd  :  cl  ;  whence  the  cosecant  is  known, 
being  a  third  proportional  to  the  sine  and  radius  ;  or  the  re- 
ciprocal of  the  sine  to  radius  1. 

As  for  the  log.  sines,  tangents,  and  secants,  in  the  tables, 
they  are  only  the  logarithms  of  the  natural  sines,  tangents, 
and  secants,  calculated  as  above. 

Having  given  an  idea  of  the  calculation  and  use  of  sines, 
tangents,  and  secant*,  wt>  may  uow  proceed  to  resolve  the 


PROBLEMS. 


889 


several  cases  of  Trigonometry  ;  previous  to  which,  however, 
it  may  be  proper  to  add  a  few  preparatory  notes  and  ob- 
servations, as  below. 

Note  1.  There  are  three  methods  of  resolving  triangles, 
or  the  cases  of  trigonometry  ;  namely,  Geometrical  Con- 
struction, Arithmetical  Computation,  and  Instrumental  Opera- 
tion ;  of  which  the  first  two  will  here  be  treated. 

In  the  First  Method,  The  triangle  is  constructed,  by 
making  the  parts  of  the  given  magnitudes,  namely,  the  sides 
from  a  scale  of  equal  parts,  and  the  angles  from  a  scale  of 
chords,  or  by  some  other  instrument.  Then  measuring  the 
unknown  parts  by  the  same  scales  or  instruments,  the  solu- 
tion will  be  obtained  near  the  truth. 

In  the  Second  Method,  Having  stated  the  terms  of  the 
proportion  according  to  the  proper  rule  or  theorem,  resolve 
it  like  any  other  proportion,  in  which  a  fourth  term  is  to  fie 
found  from  three  given  terms,  by  multiplying  the  second 
and  third  together,  and  dividing  the  product  by  the  first, 
in  working  with  the  naturul  numbers  ;  or,  in  working  with 
the  logarithms,  add  the  logs,  of  the  second  and  third  terms 
together,  and  from  the  sum  take  the  log.  of  the  first  term  ; 
then  the  natural  number  answering  to  the  remainder  is  the 
fourth  term  sought. 

Note  2.  Every  triangle  has  six  parts,  viz.  three  sides  and 
three  angles.  And  in  every  triangle  proposed,  there  must 
be  given  three  of  these  parts,  to  find  the  other  three.  Also, 
of  the.  three  parts  that  are  given,  one  of  them  at  least  must 
be  a  side ;  because,  with  thf  same  angles,  the  sides  may  be 
greater  or  less  in  any  proportion. 

Note  3.  All  the  cases  in  trigonometry,  may  be  comprised 
in  three  varieties  only  ;  viz. 

1**,  When  a  side  and  its  opposite  angle  are  given. ' 
■  2d,  When  two  sides  and  the  contained  angle  are  given. 

3d,  When  the  three  sides  are  given. 

For  there  cannot  possibly  be  more  than  these  three  varie- 
ties of  cases ;  for  each  of  which  it  will  therefore  be  proper 
to  give  a  separate  theorem,  as  follows  : 


THEOREM  I. 

When  a  Side  and  Us  Opposite  Angle  are  two  of  the  Give* 
Parts. 

Then  the  unknown  parts  will  be  found  by  this  theorem  : 
viz.  The  sides  of  the  triangle  have  the  same  proportion,  to 
each  other,  as  the  sines  of  their  opposite  ua^tatYm*. 


884 


PLANE  TRIGONOMETRY. 


That  is.  As  any  one  aide, 

la  to  the  sine  of  its  opposite  angle  ; 

So  is  any  other  side, 

To  the  sine  of  its  opposite  angle. 
Demonstr.    For,  let  abc  be  the  pro-  C 
posed  triangle,  having  ab  the  greatest  Y^f\ 
aide,  and  bc  the  least.    Take  ad  =         sSv*  \ 

bc,  considering  it  as  a  radius ;  and  let  |\i  \ 

fall  the  perpendiculars  dk,  cf,  which  £  3£  Jf  B 
will  evidently  be  the  sines  of  the  an- 

§lea  a  and  a,  to  the  radius  ad  or  bc. 
Tow  the  triangles  ade,  acf,  are  equiangular  ;  they  therefore 
have  their  like  sides  proportional,  namely,  ac  :  cf  :  :  ad  or 
Be  :  de  ;  that  is,  the  side  ac  is  to  the  sine  of  its  opposite  an- 
gle b,  as  the  aide  bc  is  to  the  sine  of  its  opposite  angle  a. 

Note  1.  In  practice,  to  find  an  angle,  begin  the  proportion 
with  a  side  opposite  to  a  given  angle.  And  to  find  a  aide, 
begin  with  an  angle  opposite  to  a  given  side. 

Note  2.  An  angle  found  by  this  rule  is  ambiguous,  or  un- 
certain whether  it  be  acute  or  obtuse,  unless  it  be  a  right 
angle,  or  unless  its  magnitude  be  such  as  to  prevent  the 
ambiguity  ;  because  the  sine  answers  to  two  angles,  which 
are  supplements  to  each  other  ;  and  accordingly  the  geome- 
trical construction  forms  two  triangles  with  the  same  parts 
that  are  given,  as  in  the  example  below  ;  and  when  there  is 
no  restriction  or  limitation  included  in  the  question,-  either 
of  them  may  be  taken.  The  number  of  degrees  in  the  table, 
answering  to  the  sine,  measurc%he  acute  angle  ;  but  if  the 
angle  be  obtuse,  subtract  those  degrees  from  180°,  and  the 
remainder  will  be  the  obtuse  angle.  When  a  given  angle  if 
obtuse,  or  a  right  one,  there  can  be  no  ambiguity  ;  for  then 
neither  of  the  other  angles  can  be  obtuse,  and  the  geometri- 
cal construction  will  form  only  one  triangle. 


EXAMPLE  I. 

In  the  plane  triangle  abc, 

I  ab  345  yards 
Given  {  bc  232  yards 
a  37"  20' 
Required  the  other  parts. 

1.  Geometrically. 

Draw  an  indefinite  line  ;  on  which  set  off  ab  =  345, 
from  some  convenient  scale  of  equal  parts. — Make  the  angle 


THEOREM  I . 


885 


a  =  37°i. — With  a  radius  of  232,  taken  from  the  same 
scale  of  equal  parts,  and  centre  b,  cross  ac  in  the  two 
points,  c,  c. — Jjastly,  join  bc,  bo,  and  the  figure  is  construct, 
ed,  which  gives  two  triangles,  and  shows  that  the  case  is  am. 
biguous. 

Then,  the  sides  ac  measured  by  the  scale  of  equal  parts, 
and  the  angles  b  and  c  measured  by  the  line  of  chords,  or 
other  instrument,  will  be  found  to  be  nearly  as  below  ;  viz. 

ac  174  z.b27«  Z.cll5ft|. 

or  3741  or    78}  or     64  J. 

2.  Arithmetically. 

First,  to  find  the  angles  at  c. 

As  side      bc  232  .  log.  2-3654880 

To  sin.  op.  £  a  37°  20'     .      .  9*78^7958 

So  side     ab  345          -  25378191 

To  sin.  op.     c  1 1 5'  36*  or  61°  24'  9  9551269 

add        Z.A  37  20      37  20 

the  sum        152  56  or  101  44 

taken  from     180  00     180  00 

leaves       b  27  04  or  78  16 

Then,  to  find  the  side  ac. 

As  sine     Z  a   37°  20' 

To  op.  side  bc  2S2 

„  .  .  i 270  0* 
So  sin.     Z  b  J78  16 

To  op.  side  ac    174  07 
or  374*56 


-  log.  9-7827956 

-  '  2-3654*80 

9*6580371 
9*9908291 
'84407*93 
2-5735218 


EXAMPLE  II. 


In  the  plane  triangle  abc, 

C  ab  365  poles 
Given  <  £a  57°  12' 
24  45 

Required  the  other  parts. 

EXAMPLE  III. 

In  the  plane  triangle  abc, 

(  ac  120  feet 
Given  <   bc  112  feet 
(  Za  57"  27' 

Required  the  other  parts. 
Vol.  I.  50 


Ans.  <  a 


c 

AC 
BC 


98°  3' 
154 


f  £b  64*34'  21' 
or  115  25  39 
£c57  58  39 
or     7   7  21 
ab  112-65  feet 

lor   16-47  fa*. 


386 


PLANE  TBIOOH  OMETXY. 


THEOREM  II. 


When  too  Sides  and  their  Contained  Angle  are  given* 

F1S8T  find  the  sum  and  the  difference  of  the  given  sides. 
Next  subtract  the  given  angle  from  180°,  and  the  remainder 
will  be  the  sum  of  the  two  other  angles ;  then  divide  that 
by  2,  which  will  give  the  half  sum  of  the  said  unknown  an- 
gles.   Then  say, 

As  the  sum  of  the  two  given  sides, 

Is  to  the  difference  of  the  same  sides ; 

So  is  the  tang,  of  half  the  sum  of  their  op.  angles. 

To  the  tang,  of  half  the  diff.  of  the  same  angles. 

Add  the  half  difference  of  the  angles,  so  found,  to  their 
half  sum,  and  it  will  give  the  greater  angle,  and  subtracting 
the  same  will  leave  the  less  angle  :  because  the  half  sum  of 
any  two  quantities,  increased  by  their  half  difference,  gives 
the  greater,  and  diminished  by  it  gives  the  less. 

All  the  angles  being  thus  known,  the  unknown  side  will 
be  found  by  the  former  theorem. 

Note.  Instead  of  the  tangent  of  the  half  sum  of  the  un. 
known  angles,  in  the  third  term  of  the  proportion,  may  be 
used  the  cotangent  of  half  the  given  angle,  which  is  the 
same  thing. 

Demon.  Let  abc  be  a  plane  triangle  of  which  ac,  ci, 
and  the  included  angle  c  are  given :  c  being  acute  in  the 
first  figure,  obtuse  in  the  second. 

On  ac,  the  longer  side,  set  off  cd  =  cb  the  shorter ;  join 


bd,  and  bisect  it  in  e  ;  also,  bisect  ad  in  o,  and  join  »,  cs, 
producing  the  latter  to  r. 

Now  J(ac  +  cb)  =  £(2gd  +  2dc)  =  co 
and  ^(ac  —  cb)  =  |(2ag)  =  ag 

also  {(a  +  b)  =  £(cdb  +  CBD)  x  cm 
and  |(b  —  a)  ==  abc  —  J  sum  =  abd: 


C 


THEOREM  II.  397 

also,  because  cs  bisects  the  base  of  the  isosceles  triangle  cbd, 
it  is  perpendicular  to  it : 

Therefore  ec  =  tangent  of  cbd  )  .  M 
kp  =  tangent  of  abd  5  t0radMI8BB- 
Lastly,  because  in  the  triangle  acf,  oe  is  parallel  to  af 
(Geom.  th.  82)  we  have 

co  :  oa  :  :  ce  :  ef  ;  that  is, 
J(ac  +  cb)  :  |(ac —  cb)  :  :  tan.  £(b  +  a)  :  tan.  J(b  —  a)  ; 
or,  siuce  doubling  both  the  antecedent  and  consequent  of 
the  first  ratio  does  not  change  the  mutual  relatiou  of  its 
terms,  we  have 

ac  +  cb  :  ac  —  cb  : :  tan.  J(b  +  a)  :  tan.  J(b  —  a),  q.  e.  d. 


EXAMPLE  I. 


In  the  plane  triangle  abc, 
C  ab  345  yards 
Given  <  ac  174*07  yards 
(  £  a  37°  20' 
Required  the  other  parts. 


1.  Geometrically. 

Draw  ab  =  345  from  a  scale  of  equal  parts.  Make  the 
angle  a  ==  37°  20'.  Set  off  ac  =  174  by  the  scale  of  equal 
parts.   Join  bc,  and  it  is  done. 

Then  the  other  parts  being  measured,  they  are  found  to 
be  nearly  as  follow  ;  viz.  the  side  bc  232  yards,  the  angle 
b  27°,  and  the  angle  c  115°{. 


2.  Arithmetically. 

The  side  ab  345  From  180°  00' 

the  side  ac  174*07  take  Lk    37  20 

their  sum     519*07  sum  of  c  and  b  142  40 

their  differ.  170*93  half  sum  of  do.     71  20 

As  sum  of  sides  ab,  ac,    -    -  519  07  log.  2*7152259 

Todiff.ofsides  ab.ac,    -    -  170*93    -  2*2328183 

So  tang,  half  num^flc  and  b  71-  2ff    -  10  4712979 

To  tang,  half  diff.  L  s  c  and  b  44  10   -  9-9888903 

these  added  give  115  36 

and  subtr.   give  z.  b  27  4 


888 


PLANK  TKJOOMOXKTBY. 


Then,  by  the  former  theorem. 

As  sin  Z  c  1 15"  3ff  or  64  24'       -  log.  0-95518S0 

To  its  ou.  side  ar  345  -       -       -  2-53781M 

Sown.  ofZ  a37  2ff  •       -      -  07827U58 

To  its  op.  side  bc  232  -      •      -  2-3054880 

EXAMPLE  n. 

In  the  plane  triangle  abc, 

(  ab  365  poles  (  bc  800-86 

Given  I  ac  154-33            Ana.  {  L  b  24«  45' 

a  57"  12*  file  08  3 
Required  the  other  parts. 

EXAMPLE  III* 

In  the  plane  triangle  abc, 

(  ac  120  yards  i  ab  112-65 
Given  I  bc  112  yards          Ans.  1  Z±  57e  2T  0" 

(  Zc  57"  58'  39"  (  ^b  65  34  21 
Required  the  other  parts. 


TIIEOREM  III. 

When  the  Three  Sides  of  a  Triangle  a  r  give  a. 

First,  let  full  a  perpendicular  from  the  greatest  angle  on 
the  opposite  side,  or  base,  dividing  it  into  two  segments,  and 
the  whole  triangle  into  two  right-angled  triangles  :  then  the 
proportion  will  be, 

As  the  base,  or  sum  of  the  segments, 
Is  to  the  sum  of  the  other  two  sides  ; 
So  is  the  difference  of  those  sides, 
To  the  diff.  of  the  segments  of  the  base. 

Then  take  half  this  difference  of  the  segments,  and  add 
it  to  the  half  sum,  or  the  half  base,  for  the  greater  segment, 
and  subtract  the  same  for  the  less  segment. 

Ht  nee,  in  each  of  the  two  right-angled  triangles,  there 
will  be  known  two  sides,  and  the  right  angle  opposite  to  one 
of  them  ;  consequently  the  other  angles  will  be  found  by  the 
first  theorem. 

Demonsfr.  By  theor.  35,  Geom.  the  rectangle  of  the  sum 
and  difference  of  the  two  sides,  is  equal  to  the  rectangle  of 
the  sum  and  difference  of  the  two  segments.  Therefore,  by 
forming  the  sides  of  these  rectangles  into  a  proportion  by 


THfOREV  Iff. 


389 


tbeor.  76,  Geometry,  it  will  appear  that  the  sums  and  dif- 
ferences are  proportional  as  in  this  theorem. 

N.  B.  Before  you  commence  a  solution  of  an  example  to 
this  case,  ascertain  whether  the  triangle  be  rigta-angled  or 
not,  by  determining  whether  the  square  of  the  rongest  side 
be  equal  or  unequal  to  the  sums  of  the  squares  of  the  other 
two.  If  equal,  the  exircple  may  be  referred  to  the  notes 
to  theorem  nr. 


EXAMPLE  i. 

In  the  plane  triangle  abc, 
Given  4     345  yards 

*•  ~de8  J  bc  174-07 
To  find  the  angles. 

1.  Geometrically. 


Draw  the  base  ab  =  345  by  a  scale  of  equal  parts.  With 
radius  232,  and  centre  a,  describe  an  arc  ;  and  with  radius, 
174,  and  centre  b,  describe  another  arc,  cutting  the  former 
in  c.   Join  ac,  bc,  and  it  is  done. 

Then,  by  measuring  the  angles, ,  they  will  be  found  to  be 
nearly  as  follows,  vie. 

Z  a  27%  L  b  37°i,  and  Lc  11 5° J. 


2.  Arithmetically* 

Having  let  fall  the  perpendicular  cp,  it  will  be, 
As  the  base  ab  :  ac  +  bc  : :  ac  —  bc  :  ap  —  bp, 
that  is,  as  345  :  406  07  : :  57  03  :  68-18  =  ap  —  bp, 
its  half  is      -        34  09 
the  half  base  is  172-50 
the  sum  of  these  is  206-59  =  ap. 
and  their  diff.  is     138*41  =  bp. 


Then,  in  the  triangle  apc,  right-angled  at  p, 

As  the  side      ac   -      -  232    -  log.  2-3054880 

To  sin.  op.      iiP    .       .  90s  .  -  10*0000000 

So  is  the  side    ap    .      -  208-59  .  2-3151093 

To  sin.  op.  L  acp    .      -  62°  56'  .  9-94t6213 

which  taken  from        -  90  00 

leaves  the  Lh.  27  04 


990 


plaice  naooHoxmr. 


Again,  in  the  triangle  bpc,  right-angled  at  p9 

As  the  aide      bc   .      .  174-07  -  log.  2-2407230 

Toain.  op.      £p   -  00"  .   .  10-0000000 

8oiaaide        bp   -      -  188-41  .   .  2-1411675 

To  ein  op.  L  bcp   -      -  52°  40'  .   .  9-0004486 

which  taken  from        -  90  00 

leaves  the  Lb  87  20 

Also  the  /acp  62°  66' 

added  to  Zbcp  52  40 

gives  the  whole  £acb  115  36 

So  that  all  the  three  angles  are  as  follow,  viz. 
the  iLA27'4';  the  Z.B3T20';  the  Lc  115* 36'. 

The  angles  a  and  b  may  also  easily  be  found  by  the  ex- 

»  AC  BO 

pressions  sec.  a  =  — ,  sec.  b  =  — ,  or  the  equivalent  logs. 


EXAMPLE  II. 


In  the  plane  triangle  abc, 


r (  ab  365  poles  {  L  a  57*  12' 

ss-issa  Has- 

To  find  the  angles 


exampw  in. 


r;w«n     (ab120  (^a  57*27'  0' 

\  AC  112-65  Ans.  <  /1b  57  58  39 
the  sides  JBcU2  (^c  64  34  21 

To  find  the  angles. 


The  three  foregoing  theorems  include  all  the  eases  of 
plane  triangles,  both  right-angled  and  oblique.  But  there 
are  other  theorems  suited  to  some  particular  forms  of  tri- 
angles (see  vol.  ii.),  which  are  sometimes  more  expeditious 
in  their  use  than  the  general  ones ;  one  of  which,  as  the  case 
for  which  it  serves  so  frequently  occurs,  may  be  here  ex- 
plained. 


TRSOBBM  IV. 


4 

an 


THEOREM  IV. 

When  a  Triangle  is  Right-angled ;  any  of  the  unknown  part* 
may  be  found  by  the  following  proportions :  viz. 

As  radius 

Is  to  either  leg  of  the  triangle  ; 
So  is  tang,  of  its  adjacent  angle, 
To  its  opposite  leg ; 
And  so  is  secant  of  the  same  angle, 
To  the  hypothenuse. 

Demonstr.  ab  being  the  given  leg,  in  the  * 
right-angled  triangle  abc  :  with  the  centre 
a,  and  any  assumed  radius  ad,  describe  an 
arc  de,  and  draw  dp  perpendicular  to  ab, 
or  parallel  to  bc.  Then  it  is  evident,  from 
the  definitions,  that  df  is  the  tangent,  and 
af  the  secant  of  the  arc  de,  or  of  the 
angle  a  which  is  measured  by  that  arc,  to  the  radius  ad. 

Then,  because  of  the  parallels  bc,  df,  it  will  be  - 

as  ad  :  ab  : :  df  :  bc  and  : :  af  :  ac,  which  is  the  same  as 
the  theorem  is  in  words. 

Note.  The  radius  is  equal,  either  to  the  sine  of  90°,  or  the 
tangent  of  45r ;  and  is  expressed  by  1,  in  a  table  of  natural 
sines,  or  by  10  in  the  log.  sines. 

EXAMPLE  I. 


In  the  right-angled  triangle  abc, 

Given  \  TAf  48'  \  To       A0  and  B& 

1.  Geometrically. 

Make  ab  =  162  equal  parts,  and  the  angle  a=53*  7'  48' ; 
then  raise  the  perpendicular  bc,  meeting  ac  in  c.  So  shall 
ac  measure  270,  and  bc  216. 


2.  Arithmetically. 

As  radius  log.  10*0000000 

To  leg  ab                162  2-2005150 

So  tang.                   53°  7  48"  10-1240871 

TolegBc               216  -  S-S&M&fllY 


S03 


PLANE  raieONOMBTRY. 


So  secant  Lk  -  53°  T  48 7  -  10  2218477 
To  hyp.  ac  270  .  2-4318627 


EXAMPLE  H. 


In  the  right-angled  triangle  abc, 

n.       5  the  leg  ab  180  .      (ac  302-0146 

UlTcn  )  the  Z  a  62  40'  An8,  I  bc  348-2464 

To  find  the  other  two  side*. 

Note.  There  is  sometimes  given  another  method  for  right- 
angled  triangles,  which  is  this : 

abc  being  such  a  triangle,  make  one 
leg  ab  radius  ;  that  is,  with  centre  a, 
and  distance  ab,  describe  an  arc  bf. 
Then  it  is  evident  that  the  other  leg  bc 
represents  the  tangent,  and  the  hypo- 
thenuse  ac  the  secant,  of  the  arc  bf,  or 
of  the  angle  a. 

In  like  manner,  if  the  leg  bc  be  made 
radius ;  then  the  other  leg  ab  will  re- 
present the  tangent,  and  the  hypothenuse  ac  the  secant,  of 
the  arc  bo  or  angle  c. 

But  if  the  hypothenuse  be  made  radius ;  then  each  leg 
will  represent  the  sine  of  its  opposite  angle  ;  namely,  the  leg 
ab  the  sine  of  the  arc  ae  or  angle  c,  and  the  leg  bc  the  sine 
of  the  arc  cd  or  angle  a. 

Then  the  general  rule  for  all  these  cases  is  this,  namely, 
that  the  sides  of  the  triangle  bear  to  each  other  the  same 
proportion  as  the  parts  which  they  represent. 

And  this  is  called,  Making  every  side  radius. 

Note  2.  When  there  are  given  two  sides  of  a  right-angled 
triangle,  to  find  the  third  side  ;  this  is  to  be  found  by  the 
property  of  the  squares  of  the  sides,  in  theorem  34,  Geom. 
vis*  that  the  square  of  the  hypothenuse,  or  longest  side,  is 
equal  to  both  the  squares  of  the  two  other  sides  together. 
Therefore,  to  find  the  longest  side,  add  the  squares  of  the 
two  shorter  sides  together,  and  extract  the  square  root  of 
that  sum  ;  but  to  find  one  of  the  shorter  sides,  subtract  the 
one  square  from  the  other,  and  extract  the  root  of  the  re- 
mainder. Or,  when  the  hypothenuse,  h,  and  either  the  base, 
b,  or  the  perpendicular,  p,  are  given  :  then  half  the  sum  of 
log.  (a  +  p)  and  log.  (u  —  p)  —  log.  b  ;  and  half  the  sum 
ofJog.  (h  -f  b)  and  log.  (h  —  b)  =  log.  p. 


QflSFUL  JPOftMGUB* 


When  b  and  p  are  given,  the  following  logarithmic  ope- 
ration may  sometimes  be  advantageously  employed ;  viz. 
Find  n  the  number  answering  to  the  log.  diff.,  2  log.  p  —  log. 
b  ;  and  make  b  +  *  =  x  :  then,  £  (log.  m  +  log.  b)  =  log.  h, 
the  hypothenuse. 

The  truth  of  this  rule  is  evident :  for,  from  the  nature 


of  logarithms.  —  =  if; 


whence  b  +  n  =  b  +  -t-  = 


b9+p9 

— - —  =*  m;  and  £  (log.  n  +  log.fl)  =  J  log.  mb  =  |  log. 
(B*  +  p>)  =  log.  i/(Ba  +  p*)  =  log.  H. 

Or,  stall  more  simply,  find  10  +  the  diff.  (log.  p  —  log.  b) 
in  the  log.  tangents.  The  corresponding  log.  secant  added 
to  log.  b  ==  log.  H. 

Note,  also,  as  many  right-angled  triangles  in  integer  num- 
bers as  we  please  may  be  found  by  making 
»*  +  a9  5=  hypothenuse 
m9  —  n9  =  perpendicular 
2mn  ■=  base 
m  and  n  being  taken  at  pleasure,  m  greater  than  ft. 

Before  we  proceed  to  the  subject  of  Heights  and  Distances 
"  we  shall  give, 

A  CONCISE  INVESTIGATION  OF  SOME  OF  THE  MOST  USEFUL 
TRIGONOMETRICAL  FORMULAE. 

Let  ab,  ac,  ad,  be  three  arches,  such  that  bc  =  c*,  aud 
o  the  centre.    Join  ao,  oc,  bo.    Draw  deq  and  oi  per- 
pendicular, and  bdc  ||  to  oa.    Join  Ma  and  bisect  it  by  the 
radius  on  ;  and  draw  ah  ||  to  bp. 
Then  is  ah  =  sin.  ac 
oh  =  cos.  ac; 

alSO  DE  =  EQ  =  8in.  AD 

EK  =  oi  =  sin.  ab 
ojk  =  sin.  ad  +  sin.  ab 
dk  =  sin.  ad  —  sin.  ab 

BI  =  IM  =  COS.  AB 
OR  =>  KI  =  COS.  AD 
MK  =  COS.  AB  +  COS.  AD 
BK  =  COS.  AB  —  COS.  AD 

Because  the  angles  at  k  are  right  angles  : 
arc  bd  +  arc.Mli  =  180*,  and  arc  dc  +  arc  mn  =  Ifr 

.%  MP  =  VH  =  OG  =  COS.  DC  =  COS.       \     '  V 

Vol,  I  51  %  V 


394  PLANE  TRIGONOMETRY. 

also,  because  ao  =  4(ab  +  ad)  =  £baq  =  angle  aoc  (at 
centre)  =  bdq  (at  circumf.)  =  bmq  (on  same  arc) 
.%  triangles  aoh,  bdk,  qmk,  are  equiangular. 

Hence — 

I.  oa  :  ah  :  :  mq  :  qk  ; 
that  is,  rad.  :  sin.  ac  :  :  2  cos.  bc  :  sin.  ad  +  sin.  ab 

II.  ao  :  oh  :  :  bd  :  dk  ; 

or,  rad.  :  cos.  ac  :  :  2  sin.  bc  :  sin.  ad  —  siii.  ab 

III.  ao  :  oh  :  :  on  :  kk  ; 

or,  rad.  :  cos.  ac  :  :  2  cos.  bc  :  cos.  ab  +  cos.  ad 

IV.  ao  :  ah  :  :  db  :  dk  ; 

or,  rad.  :  sin.  ac  :  :  2  sin.  bc  :  cos.  ab  —  cos  ad  ; 

also, 

V.  BK  .  KM  =  DK  .  KQ,  that  is  (COS.  AB          COS.  AD) 

(cos.  ab+cos.  ad)  =  (sin.  ad— sin.  ab)  (sin.  AD+sin.  ab). 

By  reducing  the  above  four  proportions  into  equations, 
making  rad.  =  1,  we  obtain  two  distinct  classes  of  formula*, 
thus  :— 

First  Class,  ac  =  a,  cb  =  b  ;  then  ad  =  a  +  6,  ab  =  a— bl 

1.  sin.  (a  +  b)  +  sin.  (a  —  I)  =  2  sin.  a  cos.  b 

2.  sin.  (a  +  b)  —  sin.  (a  —  b)  =  2  cos.  a  sin.  6 

3.  cos.  (a  —  6)  +  cos.  (a  +  6)  =  2  cos.  a  cos.  6 

4.  cos.  (a  —  b)  —  cos.  (a  +  b)  =  2  sin.  a  sin.  b 

Second  Class,  ad  =  a,  ab  =  b  ;  then  ac  =  £(a  +  6), 
bc  =  £(a  —  6). 

5.  sin.  a  +  sin.  6=2  sin.  i(a  +  b)  cos.  £(a  —  b) 

6.  sin.  a  —  sin.  6  =  2  cos.£(a  +  b)  sin.  £(a  —  b) 

7.  cos.  6  +  cos.  a  ss2  cos.£(a  +  b)  cos.  \\a  —  6) 

8.  cos.  b  —  cos.  a  =  2  sin.  i(a  +  &)  sin,  £(a  —  6) 

The  first  class  is  useful  in  transforming  the  products  of 
sines  into  simple  sines,  and  the  contrary. 

The  second  facilitates  the  substitution  of  sums  or.  differ- 
ences of  sines  for  the  products,  and  the  contrary. 

Taking  the  sum  and  the  difference  of  equations  1  and  2, 
also  of  3  and  4,  remembering  that  sin.  =  cos.  tan.  we  obtain 
the  following  : 

Third  Class. 

9.  sin.  (a  +  b)  =  sin.  a  cos.  b  +  sin.  b  cos.  a 
=  cos.  a  co*.  h  (tan.  a  +  tan.  b) 


USEFUL  FOBKiflLfi.  305 

10.  sin.  (a  —  6)  =  sin.  a  cos.  b  —  sin.  b  cos.  a 

=  cos.  £i  cos.  6  (tan.  a  —  tan.  b) 

11.  cos.  (a  +  b)  =  cos.  a  cos.  &  — -  sin.  a  sin.  b 

■s  cos.  a  cos.  6  (1  —  tan.  a  tan.  b) 

12.  cos.  (ci  —  b)  =  cos.  a  cos.  6  +  sin.  a  sin.  b. 

=  cos.  a  cos.  b  (1  +tan.  a  tan.  b). 

From  these,  making  a  =  6,  we  readily  obtain  the  ex- 
pressions for  sines  and  cosines  of  double  arcs ;  also  dividing 
equation  9  by  11,  and  equation  10  by  12,  we  obtain  ex- 
pressions for  the  tangents  of  a  +  b  and  a  —  b.  Thus  we 
have  : — 

Fourth  Class. 

13.  sin.  2a  =  2  sin.  a  cos.  a  =  2  ooe.'a  tan.  a 

14.  cos.  2a  =  cos.2  a  —  sin.2  a  =  cos.2  a  (1  —  tan.2  a) 

sin.  ,    .  .v  /    •  t\     tan.  a  +  tan.  6 

15.   (a  +  6)  =  tan.  (a  +  6)  =  - — —  z 

cos.  v  '      1—  tan.  a  tan.  6 

sin.  ,       ,v  /ix      tan.  o  —  tan.  b 

 (a  —  b)  =  tan.  (a  —  ft)  =  r  . 

cos.  v        '  '     1  +  tan.  a  tan.  6  . 


16 


_  4  0  2  tan.  a 
17.  tan.  2a  = 


18.  cot.  2a  = 


1—  tan.2  a 
1—  tan.2  a 
2  tan.  a 


Substituting  in  the  second  class, 

for  sin.  i(a+b),  cos.  i(a  +  b)  tan.  $(a+b), 
.and  for  sin.  i(a— b),  cos.  £(a —  b)  tan.  we  have : — 

Fifth  Class. 

19.  cos.  &+cos.  a=2  cos.  £(a+&)cos.  4(a— 6). — Seeequa.  7. 

20.  cos.  6  — cos.a  =  tan.  $(a+b)  tan.  £(a—  5)  2  cos.  |(a+&) 
cos.  £(a-&)  =  ton- tan.  i(a— &)(cos.&+cos.  a) 

21.  sin.  a+sin.  6  =  tan.  ±(a+&}  2  cos.  i(a+&)  cos.  i(a-5) 

=  tan.  £(a+6)  (cos.  a+cos.  b) 

22.  sin.  a  -sin.  b  =  tan.  ^(a-6)  2  cos.  J(a+&)  cos.  }(*—*) 

=  tan.  |(a—  6)  (cos.  a+cos.  6) 

^0  sin.  a+sin.  5     tan.  i{a+b) 

23.  r — r  =  - — 77 — 7x  -  from  21  and  22. 

sin.  a— sm.  o     tan.  J(a— 6) 

^  sin.  a+sin.  6  w    .        r  rt« 

24.  r  =  tan.  Ua  +  6)  :  from  21. 

cos.a+cos.  o 

^  sin.  a— sin.  i     A      , ,  r  M 

25.   ;  r  =  tan.  Ua  —6) :  from  22. 

cos.a+cos.  b  ,v 


300  o*  nktolm 


Excunplts  for  Exercise. 

1.  Demonstrate  that  in  any  right-angled  plane  triangle  tiur 
following  properties  obtain :  viz. 

oerp.  base 

(1.)  £_£.=£tan*  ang.  at  base.  (2.)  =tan.  ang.  at  vertex* 

*  'base  *  v  'perp.  ^ 

(3.)  j^EL'sssin.  ang.  at  base.  (4.)        —sin.  ang.  at  vertex* 

(5. )        « sec.  ang.  at  base.  (6.)        =sec.  ang.  at  vertex* 

2.  Demonstrate  that  tan<  a  +  sec.  a  =  tan.  (45*  +  i^)* 

l*4"tan  *  a 

3.  Demonstrate  that  sec.  2a  =  - — - — Vi>  tnat 

1 — tanv  * 

l+tan.8A      sec.9  a 


cosec, 


2a  = 


2  tan.  a      2  tan.  a 

4.  Given  Axy  =  ay8  +  ns* ;  to  find  x  and  y  the  sine  and 
cosine  of  an  arc. 

5.  Demonstrate  that  of  any  arc,  tan.a  —  sin.2  =  tan.2  sin.2- 

6.  Demonstrate  that  if  the  tan.  of  an  arc  be  =  ^/n,  the 

sine  of  the  same  arc  is  =  y/  n 


n+1" 


OF  HEIGHTS  AND  DISTANCES,  &c. 

6y  the  mensuration  and  protraction  of  lines  and  angles, 
are  determined  the  lengths,  heights,  depths,  and  distances  of 
bodies  or  objects. 

Accessible  lines  are  measured  by  applying  to  them  some 
certain  measure  a  number  of  times,  as  an  inch,  or  a  foot,  or 
yard.  But  inaccessible  lines  must  be  measured  by  taking 
angles,  or  by  such-like  method,  drawn  from  the  principles  of 
geometry. 

When  instruments  are  used  for  taking  the  magnitude  of  the 
angles  in  degrees,  the  lines  are  then  calculated  by  trigonome- 
try :  in  the  other  methods,  the  lines  are  calculated  fr#m  the 
principle  of  similar  triangles,  or  some  other  geometrical 
property,  without  regard  to  the  measure  of  the  angles* 


AlfD  MBTANCEf . 


397 


Angles  of  elevation,  or  of  depression,  are  usually  taken 
either  with  a  theodolite,  or  with  a  quadrant,  divided  into  de- 
grees and  minutes,  and  furnished  with  a  plummet  suspended 
from  the  centre,  and  two  open  sights  fixed  on  one  of  the  radii, 
or  else  with  telescopic  sights. 


To  lake  an  Angle  of  Altitude  and  Depression  with  tike 
Quadrant. 


Let  a  be  any  object,  as  the  sun, 
inoon,  or  a  star,  or  the  top  of  a 
tower,  or  hill,  or  other  eminence : 
and  let  it  be  required  to  find  the 
measure  of  the  angle  abc,  which  a 
line  drawn  from  the  object  makes 
above  the  horizontal  line  bc. 

Place  the  centre  of  the  quadrant 
in  the  angular  point,  and  move  it 
round  there  as  a  oentre,  till  with  one  eye  at  n,  the  other 
being  shut,  you  perceive  the  object  a  through  the  sights ; 
then  will  the  arc  gh  of  the  quadrant,  cut  off  by  the  plumb- 
line,  bii,  be  the  measure  of  the  angle  abc  as  required. 

The  angle  abc  of  depression  of 
any  object  a,  below  the  horizontal 
line  bc,  is  taken  in  the  same  manner; 
except  that  here  the  eye  is  applied  to 
the  centre,  and  the  measure  of  the 
angle  is  the  arc  gh,  on  the  other 
side  of  the  plumb-liner 

The  following  examples  are  to  be  constructed  and  calcu- 
lated by  the  rules  of  Trigonometry. 


B  


EXAMPLE  t. 


Having  measured  a  distance  of  200  feet,  in  a  direct  hori- 
zontal line,  from  the  bottom  of  a  steeple,  the  angle  of  eleva- 
tion of  its  top,  taken  at  that  distance,  was  found  to  be  47°  30' ; 
hence  it  is  required  to  find  the  height  of  the  steeple. 


Construction. 

Draw  an  indefinite  line ;  on  which  set  off  ac  a  200  equal 
parts,  for  the  measured  distance.  Erect  the  indefinite  per- 
pendicular ab  ;  and  draw  cb  so  as  to  make  the  an&la,$  «a 


OF  HEIGHTS 


47°  SO7,  tho  angle  of  elevation ;  and  it  is  done.  Then  ab, 
measured  on  the  scale  of  equal  parts,  is  nearly  218J. 

Calculation. 


As  radius      -  10-0000000 

To  ac  200     -       -  2-3010300 

So  tang.  L  c  47°  80'  10-0379475 

To  ab  218-26  required  2-3380775 


Or,  by  the  nat.  tangents,  we  have  ac  X  tan.  bca  = 
200  X  1-091308  =  218-2616  =  ab. 

EXAMPLE  It. 

What  was  the  perpendicular  height  of  a  cloud,  or  of  a 
balloon,  when  its  angles  of  elevation  were  35°  and  64°,  as 
taken  by  two  observers,  at  the  same  time,  both  on  the  same 
side  of  it,  and  in  the  same  vertical  plane  ;  the  distance  be* 
tween  them  being  half  a  mile  or  880  yards  ?  And  what  was 
its  distance  from  the  said  two  observers  ? 

Construction. 

Draw  an  indefinite  ground  line,  on  which  set  off  the 
given  distance  ab  =  880 ;  then  a  and  b  are  the  places  of 
the  observers.  Make  the  angle  a  =  35°,  and  the*  angle 
B  =  64° ;  then  the  intersection  of  the  lines  at  c  will  be  the 
place  of  the  balloon :  whence  the  perpendicular  cd,  being  let 
fall,  will  be  its  perpendicular  height.  Then,  by  measure- 
ment are  found  the  distances  and  height  nearly  as  follow , 
viz.  ac  1631,  bc  1041,  dc  936. 


C 


Calculation. 

First,  from  L  b  64' 
take  L  a  35 
leaves   L.  acb  29 


— ' —  /  ; 

A            33  D 
Then  in  the  triangle  abc, 
As  sin.  Zacb       29°        ...  0-6855712 

To  op.  side  ab     880         -  2-9444827 

So  sin.  Lk          35°        -  9-7585913 

To  op.  side  bc    1041-125  3-0175028 


AND  DISTANCES. 


399 


As  sin.  ^acb       29°  -       .       -  9-6855712 

To  op.  side  ab     880  ...  2-9444827 

So  sin.  Z.B  1 16°  or  64°  -  9-9536602 

To  op.  side  ac   1631-442          -       -  3-2125717 


And  in  the  triangle  bcd,  ( 

As  sin.  L  d          90°        -  -  -  10-0000000 

To  op.  side  bc    1041-125  -  .  3-0175028 

So  sin.  L  b           64°        -  -  -  0-9536602 

To  op.  side  cd     935-757  -  -  2-9711630 


EXAMPLE  in. 


Having  to  find  the  height  of  an  obelisk  standing  on  the 
top  of  a  declivity,  I  first  measured  from  its  bottom  a  distance 
of  40  feet,  and  there  found  the  angle,  formed  by  the  oblique 
plane  and  a  line  imagined  to  go  to  the  top  of  the  obelisk, 
41  ° ;  but  after  measuring  on  in  the  same  direction  60  feet 
farther,  the  like  angle  was  only  23°  45'.  What  then  was 
the  height  of  the  obelisk  ?  » 


Construction. 

Draw  an  indefinite  line  for  the  sloping  plane  or  declivity, 
in  which  assume  any  point  a  for  the  bottom  of  the  obelisk, 
from  which  set  off  the  distance  ac  =  40,  and  again  cd  =  60 
equal  parts.  Then  make  the  angle  c  =  41°,  and  the  angle 
d  =  23°  45' ;  and  the  point  b  where  the  two  lines  meet  will 
be  the  top  of  the  obelisk.  Therefore  ab  joined,  wilr  be  its 
height. — Draw  also  the  horizontal  line  de  perp.  to  ab. 

Calculation. 

From  the  L  c  41°  00' 
take  the  /d  23  45 
loaves  the  £  dbc  17  15 


Then  in  the  triangle  dbc, 

As  sin.  /.dbc  17°  15' 
To  op.  side  dc  60 
So  sin.  L  d     23  45 
To  op.  side  cb  8M88 


9-4720856 

1-7781513. 

9-6050320 

i-9\vwn 


400 


OF  1IBEGHTS 


And  in  the  triangle  abc, 


As  sum  of  sides  cb,  ca 
To  diff.  of  sides  cb,  ca 
So  tang.  }(a  +  b) 
To  tang.  ]  (a  —  b) 


121*488  -  20845333 

41-488  .  1-6179225 

60*  3C  -  10-4272623 

42  24}  -  9*9606516 


the  diff.  of  these  is  £cba  27  5} 
the  sum  is  L  cab  111  54} 


Lastly,  as  sin.  £cba  27°  5'}  .  -  9*0582842 

To  op.  side  ca         40  .  1*6020600 

So  sin.  Lc       -      41°  0'  -  -  9*8169429 

To  op.  side  ab         57-623  -  -  1*7607187 


Also  the  L  ade  ^=  bac  —  90r  =  21°  54'}. 


EXAMPLE  IV. 


Wanting  to  know  the  distance  between  two  inaccessible 
trees,  or  other  objects,  from  tho  top  of  a  tower  120  feet  high, 
which  lay  in  the  same  right  line  with  the  two  objects,  I  took 
the  angles  formed  by  the  perpendicular  wall  and  lines  con* 
ceived  to  be  drawn  from  the  top  of  the  tower  to  the  bottom 
of  each  tree,  and  found  them  to  be  33°  and  64°}.  What  is 
the  distance  between  the  two  objects  ? 

Construcliou. 

Draw  the  indefinite  ground  line 
bd,  and  perpendicular  to  it  ba  = 
120  equal  parts.  Then  draw  the 
two  lines  ac,  ad,  making  the  two 
angles  bac,  bad,  equal  to  the 
given  measures  33'  and  64°£.  So 
shall  c  and  d  be  the  places  of  the 
two  objects. 

Calculation.  ^St- 

First,  in  the  right-angled  triangle  abi  , 

As  radius             -  10-0000000 

To  ab       .       190  ...  4i    2  0791812 

Sotaug.  /I  bac    33l»  -       -       .  9-8125174 

Tob<;       .   77-«»  -      -  1-8916980 


ASD  DISTANCES. 


401 


Then  in  the  right-angled  triangl*  abd, 

As  radius   10 'OOOOOOO 

To  ab      •      -        120            .  2  0701812 

So  tang.  L  bad  -         64°  3a  -      -  10*3215089 

To  bd      •         251-586     -      .  2*4006851 
From  which  take  bc  77*929 
leaves  the  dist.  cd  173*056,  as  required. 

Or  thus,  by  the  natural  tangents, 

From  nat.  tan.  dab  -     64°  30'  =  2*0905436 

Take  nat.  tan.  cab       -      .     33    0  =0  6494076 


Difference  -         •         -  1*4471360 

If  drawu  into  ab  -  120 


The  result  gives  cd         -  =  173-05632 


EXAMPLE  V. 

Being  on  the  side  of  a  river,  and  wanting  to  know  the 
distance  to  a  house  which  was  seen  on  the  other  side,  I  mea- 
sured 200  yards  in  a  straight  line  by  the  side  of  the  river ; 
and  then,  at  each  end  of  this  line  of  distance,  took  the  hori- 
zontal angle  formed  between  the  house  and  the  other  end  of 
the  line ;  which  angles  were,  the  one  of  them  68°  2 ,  and  the 
other  73°  15'.  What  were  the  distances  from  each  end  to 
the  house  ? 


Construction. 

Draw  the  line  ab  =  200  equal  parts. 
Then  draw  ac  so  as  to  make  the  angle 
a  =  68  2',  and  bc  to  make  the  angle 
b=73'  15 .  So  shall  the  point  c  be  the 
place  of  the  house  required. 


The  calculation,  which  i*  left  for  the  student's  exercise, 
gives  ac  =  30619,  bc  =  296  54. 

Exam.  vi.  From  the  edge  of  a  ditch,  of  36  feet  wide, 
surrounding  a  fort,  having  taken  the  angle  of  elevation  of 
the  top  of  the  wall,  it  was  found  to  be  62*40' :  required  the 
height  of  the  wall,  and  the  length  of  a  ladder  to  reach  from 
my  station  to  the'top  of  it  ?       Att  height  of  wall  69-64, 

Ans"  {ladder, 7%Afe*\. 

Vol.  I.  52 


Or  KXZOHTt 


Exam,  vii.  Required  the  length  of  a  shoar,  which  being 
to  strut  11  feet  from  the  upright  of  a  building,  will  support 
a  jamb  23  feet  10  inches  trooMhe  ground  7. 

Ans.  26  feet  3  inches. 

Exam.  viii.  A  ladder,  40  feet  long,  can  be  so  placed,  that 
it  shall  reach  a  window  33  feet  from  the  ground,  on  one  side 
of  the  street ;  and  by  turning  it  over,  without  moving  the 
foot  out  of  its  place,  it  will  do  the  same  by  a  window  21  feet 
high,  on  the  other  side  :  required  the  breadth  of  the  street  T 

Ans.  56-649  feet. 

Exam.  ix.  A  maypole,  whose  top  was  broken  off  by  a 
blast  of  wind,  struck  the  ground  at  15  feet  distance  from  the 
foot  of  the  pole  :  what  was  the  height  of  the  whole  maypole, 
supposing  the  broken  piece  to  measure  39  feet  in  length  ? 

Ans.  75  feet 

Ex  ax.  x.  At  170  feet  distance  from  the  bottom  of  a  tower, 
the  angle  of  its  elevation  was  found  to  be  52°  30* :  required 
the  altitude  of  the  tower  ?  Ans.  221-55  feet 

Exam.  xi.  From  the  top  of  a  toner,  by  the  sea-side,  of 
143  feet  high,  it  was  observed  that  the  angle  of  depression 
of  a  ship's  bottom,  then  at  anchor,  measured  35° ;  what  was 
the  ship's  distance  from  the  bottom  of  the  wall  ? 

Ans.  204-22  feet. 

Exam.  xii.  What  is  the  perpendicular  height  of  a  hifl ; 
its  angle  of  elevation,  taken  at  the  bottom  of  it,  being  46°, 
and  200  yards  farther  off,  on  a  level  with  the  bottom,  the 
angle  was  31  °  ?  Ans.  286-28  yards. 

Exam.  xiii.  Wanting  to  know  the  height  of  an  inacces- 
sible tower  ;  at  the  least  distance  from  it,  on  the  same  hori- 
zontal plane,  I  took  its  angle  of  elevation  equal  to  58° ;  then 
going  300  feet  directly  from  it,  found  the  angle  there  to  be 
only  32° :  required  its  height,  and  my  distance  from  it  at  the 
first  station  ?  k      i  height  307-53 

An8#  }  distance  198-15 

Exam.  xiv.  Being  on  a  horizontal  plane,  and  wanting  to 
know  the  height  of  a  tower  placed  on  the  top  of  an  inacces- 
sible hill  ;  I  took  the  angle  of  elevation  of  the  top  of  the  hill 
40",  and  of  the  top  of  tha  tower  51°  ;  the  measuring  in  a 
line  directly  from  it  to  the  distance  of  200  feet  farther,  I 
found  the  angle  to  the  top  of  the  tower  to  be  33°  45'.  What 
is  the  height  of  the  tower  ?  Ans.  93-33148  feet 

Exam.  xv.  From  a  window  near  the  bottom  of  a  house, 
which  seemed  to  be  on  a  level  with  the  bottom  of  a  steeple, 


AND  MSTANCM. 


I  took  the  angle  of  elevation  of  the  top  of  the  steeple  equal 
40° ;  then  from  another  window,  18  feet  directly  above  the 
former,  the  like  angle  was  37*  10'  :  required  the  height  and 
distance  of  the  steeple.  A     t  height    21(1 44 

An   }  distance  250-79 

Exam.  xvi.  Ranting  to  know  the  height  of,  and  my 
distance  frofn,  an  object  on  the  other  side  of  a  river,  which 
appeared  to  be  on  a  level  with  the  place  where  1  stood, 
close  by  the  side  of  the  river ;  and  not  having  room  to 
measure  backward,  in  the  same  line,  because  of  the  im. 
mediate  rise  of  the  bank,  I  placed  a  mark  where  I  stood, 
and  measured  in  a  direction  from  the  object,  up  the  ascend, 
ing  ground,  to  the  distance  of  264  feet,  where  it  was  evi. 
dent  that  I  wan  above  the  level  of  the  top  of  the  object ; 
there  the  angles  of  depression  were  found  to  be,  viz.  of  the 
mark  left  at  the  river's  side  42°,  of  the  bottom  of  the  object 
27°,  and  of  its  top  19*.  Required  the  height  of  the  object, 
and  the  distance  of  the  mark  from  its  bottom  ? 

a  \  height  57-26 
Ans"  I  distance  150-56 

Exam.  xvii.  If  the  height  of  the  mountain  called  the 
Peak  of  Teneriffe  be  2£  miles,  as  it  is  very  nearly,  and  the 
angle  taken  at  the  top  of  it,  as  formed  between  a  plumb-line 
and  a  line  conceived  to  touch  the  earth  in  the  horizon,  or 
farthest  visible  point,  be  88°  2  ;  it  is  required  from  these 
measures  to  determine  the  magnitude  of  the  whole  earth, 
and  the  utmost  distance  that  cpn  be  seen  on  its  surface  from 
the  top  of  the  mountain,  supposing  the  form  of  the  earth  to 
be  perfectly  globular  ? 

.      (dist.    185-943 1  ji 
in,-Jdiam.  7918!mLCS- 

Exam.  xvui.  Two  ships  of  war,  intending  to  cannonade 
a  fort,  are,  by  the  shallowness  of  the  water,  kept  so  fur  from 
it,  that  they  suspect  their  guns  cannot  reach  it  with  effect. 
In  order  therefore  to  measure  the  distance,  they  separate 
from  each  other  a  quarter  of  a  mile,  or  440  yards  ;  then  each 
ship  observes  and  measuses  the  angle  which  the  other  ship 
and  the  fort  subtends,  which  angles  are  83"  45'  and  85°  15'- 
What  is  the  distance  between  each  ship  and  the  fort  ? 

.  $2292  26  yards. 
An*'  {2296-05 

Exam.  xix.  Wanting  to  know  the  breadth  of  a  river,  I 
measured  a  base  of  500  yards  in  a  straight  line  close  by  one 
aide  of  it ;  and  at  each  end  of  this  line  I  found  the  anglea 
Mbtended  by||be  other  end  and  a  tree,  close  to  the  haok** 


404 


OF  HEIGHT!  AMD  DISTAXCBS. 


the  other  side  of  the  river,  to  be  53°  and  79*  VH*  What  was 
the  perpendicular  breadth  of  the  river  t 

Ana.  520-48  yards. 

Exam.  xx.  Wanting  to  know  the  extent  of  a  piece  of  water, 
or  distance  between  two  headlands ;  I  measured  from  each 
of  them  to  a  certain  point  inland,  and  found^the  two  distances 
to  be  786  yards  and  840  yards ;  also  the  horizontal  angle 
subtended  between  these  two  lines  was  55°  40.  What  was 
the  distance  required  ?  Ans.  741  -2  yards. 

Exam.  xxi.  A  point  of  land  was  observed,  by  a  ship  at 
sea,  to  bear  east-by .south  ;  and  after  sailing  north-east  12 
miles,  it  was  found  to  bear  south.east-by-east.  It  is  required 
to  determine  the  place  of  that  headland,  and  the  ship's  dis- 
tance from  it  at  the  last  observation  ?     Ans.  26-0728  miles. 

Exam.  xxii.  Wanting  to  know  the  distance  between  a 
house  and  a  mill,  which  were  seen  at  a  distance  on  the  other 
side  of  a  river,  I  measured  a  base  line  along  the  side  where 
I  was,  of  000  yards,  and  at  each  end  of  it  took  the  angles 
subtended  by  the  other  end  and  the  house  and  mill,  which 
were  as  follow,  viz.  at  one  end  the  angles  were  58°  2tf  and 
95°  20',  and  at  the  other  end  the  like  angles  were  53°  3a  and 
98°  45'.  What  then  was  the  distance  between  die  house  and 
mill  ?  Ans.  959-5866  yards. 

Exam,  xxiii.  Wanting  to  know  my  distance  from  an  in. 
accessible  object  o,  on  the  other  side  of  a  river  ;  and  having 
no  instrument  for  taking  angles,  but  only  a  chain  or  cord  for 
measuring  distances  ;  from  each  of  two  stations,  a  and  b, 
which  were  taken  at  500  yards  asunder,  I  measured  in  a  di- 
rect like  from  the  object  o  100  yards,  viz.  ac  and  bd  each 
equal  to  100  yards  ;  also  the  diagonal  ad  measured  550 
yards,  and  the  diagonal  bc  560.  \\  hat  was  the  distance  of 
the  object  o  from  each  station  a  and  b  ? 

ao  536-81 


n'  \  bo  500-47 

Exam.  xxiv.  In  a  garrison  besieged  are  jjjiree  remarkable 
objects,  a,  b,  c,  the  distances  of  which  frrtm  each  other  are 
discovered  by  means  of  a  map  of  the  place,  and  are  as  fol- 
low, viz.  ab  266],  ac  530,  bc  327 £  yards.  Now,  having  to 
erect  a  battery  against  it,  at  a  certain  spot  without  th(?  place, 
and  being  desirous  to  know  whether  my  distances  from  the 
three  objects  be  such,  as  that  they  may  from  thence  be  bat- 
tered with  effect,  I  took,  with  an  instrument,  the  horizontal 
angles  subtended  by  these  objects  from  the  station  s,  and 
found  them  to  be  as  follow,  viz.  the  angle  asb  13°  30,  and 
the  angle  B8c28°5tf.   Refuted  the  three  distances,  a  a, 


MX2ISUBATIOX  OF  ttAlfBS. 


406 


ib,  sc  ;  the  object  b  being  situated  nearest  me,  and  between 
the  two  others  a  and  c.  i  sa  757*14 

Ans.  <  sb  587*10 
(sc  655-80 

Exam.  xxv.  Required  the  same  as  in  the  last  example, 
when  the  object  a  is  the  farthest  from  my  station,  but  still  seen 
between  the  two  others  as  to  angular  position,  and  those  an* 
gles  being  thus,  the  angle  asb  88  45',  and  bsc  2*4  80  ,  also 
the  three  distances,  ab  600,  ac  800,  bc  400  vaids  ? 

(•a  710-3 
Ans.  {sb  1041*85 
(sc  93414 

Exam.  xxvi.  If  db  in  the  figure  at  pa.  378  represent  a  por- 
tion of  the  earth's  surface,  and  n  the  point  where  the  level* 
ling  instrument  is  placed,  then  lb  will  be  the  difference 
between  the  true  and  the  apparent  level  ;  and  you  nre  re- 
quired to  demonstrate  that,  for  distances  not  exceeding  5  or 
6  miles  measured  on  the  earth's  surface,  bl,  estimated  in 
feet,  is  equal  to  }  of  the  square  of  bd,  taken  in  miles. 


MENSURATION  OF  PLANES. 


The  Area  of  any  plane  figure,  is  the  measure  of  the  space 
contained  within  its  extremes  or  bounds  ;  without  any  re- 
gard to  thickness. 

This  area,  or  the  content  of  the  plane  figure,  is  estimated 
by  the  number  of  little  square*  that  may  be  contained  in  it ; 
the  side  of  those  little  measuring  squares  being  an  inch,  or  a 
foot,  or  a  yard,  or  any  other  fixed  quantity.  And  hence  tl  e 
area  or  content  is  said  to  be  so  many  square  inches,  or  square 
feet,  or  square  yards,  &c. 

Thus,  if  the  figure  to  be  measured  be 
the  rectangle  abcd,  and  the  little  square 
b,  whose  side  is  one  inch,  be  the  mea- 
suring unit  proposed  :  then  as  often  as 
the  said  little  square  is  contained  in  the 
rectangle,  so  many  square  inches  the 
rectangle  is  said  to  contain,  which  in 
the  present  case  is  12. 


D 

4 

c 

J 

A. 

B 

m 

406 


PROBLEM  I. 

7b  find  the  Area  of  any  Parallelogram ;  whether  it  be  a  Square, 
a  Rectangle,  a  Rhombus,  or  a  Rhomboid. 

Multiply  the  length  by  the  perpendicular  breadth,  or 
height,  and  the  product  will  be  the  area*. 

EXAMPLES. 

Ex*  1  •  To  find  Ihe  area  of  a  parallelogram,  the  length  being 
12*25,  and  breadth  or  height  8*5. 

12*25  length 
8*5  breadth 


C125 
0800 


104*125  area. 


Ex.  2.  To  find  the  area  of  a  squire,  whose  side  is  35*25 
chains.  Ans.  124  acres,  1  rood,  1  perch. 

Ex.  3.  To  find  the  area  of  a  rectangular  board,  whose 
length  is  12}  feet,  and  breadth  9  inches.  Ans.  9f  feet 

Ex.  4.  To  find  the  content  of  a  piece  of  land,  in  form  of  a 
rhombus,  its  length  being  6-20  chains,  and  perpendicular 
breadth  5*45.  Ans.  3  acres,  1  rood,  20  perches. 

Ex.  5.  To  find  the  number  of  square  yards  of  painting  in 
a  rhomboid,  whose  length  is  37  feel,  and  height  5  feet  S 
inches.  Ans.  21^  square  yards. 


*  The  truth  of  this  rule  is  proved  in  the  Geom.  theor.  81.  cor.  9. 

The  same  is  otherw.e  proved  ihu*:  Let  thts  foregoing  met  Angle  he 
the  figure  piopnsed ;  and  let  the  length  end  lirenrith  he  dvided  inlmeft* 
nil  purls,  each  equal  to  lite  linear  measuring  imitt  being  here  4  forth* 
length,  and  H  for  th»»  hreadtli ;  and  let  the  opposite  points  of  division  bt 
connected  hy  right  line*.— Then  it  is  evident  that  three  Hues  divide  tbt 
rectangle  into  a  n um her  of  little  -squares,  each  eniial  to  the  sqoait 
measuring  unit  i ;  and  further,  that  the  n  urn  her  of  these  little  squares, 
or  the  area  of  the  figure,  is  eq-ial  to  the  tuimher  of  linear  measuring  spin 
in  the  length,  related  at  olten  as  there  are  linear  measuring  units  in  the 
hrearlth,  or  height;  thai  h,  equal  to  the  length  drawn  into  the  height; 
whirh  here  is  4  X  3  or  I '2. 

And  it  is  proved  (Geom  theor.  25,  cor.  2),  that  any  oblique  parallelo- 
gram if  equal  to  a  rectangle,  of  equal  length  and  perjtendirular  breadth. 
Therefore  the  rale  U  general  for  all  |*railelograiofl  whatever. 


0F  NAHM. 


PBOB1  EM  II. 


To  find  the  Area  of  a  Triangle. 

Rulk  im  Multiply  the  base  by  the  perpendicular  height, 
and  take  half  the  product  for  the  area*.  Or,  multiply  the 
one  of  these  dimensions  by  half  the  other. 


EXAMPLES. 

Ex.  1.  To  find  the  area  of  a  triangle,  whose  J>ase  is  625* 
and  perpendicular  height  520  links  ? 

Here  6^5  X  260  =  162500  square  links, 

or  equal  1  acre,  2  roods,  20  perches,  the  answer. 
Ex.  2.  How  many  square  yards  contains  the  triangle, 
whose  base  is  40,  and  perpendicular  30  feet  ? 

A ns.  66}  square  yards. 
Ex.  3.  To  find  the  number  of  square  yards  in  a  triangle, 
whose  base  is  49  feet,  and  height  25J  feet. 

Ans.  684},  or  68*7361. 
Ex.  4.  To  find  the  area  of  a  triangle,  whose  base  is  18 
feet  4  inches,  and  height  11  feet  10  inches  ? 

Ans.  108  feet,  5}  inches. 
Rule  n.  When  two  sides  and  their  contained  angle  are 

S'ven :  Multiply  the  two  given  sides  together,  and  take  half 
eir  product :  Then  say,  as  radius  is  to  the  sine  of  the  given 
angle,  so  is  that  half  product,  to  the  area  of  the  triangle. 

Or,  multiply  that  half  product  by  the  natural  sine  of  the 
■aid  angle,  for  the  areaf. 


*  The  truth  of  this  rule  is  evident,  because  any  triangle  it  the  half  of 
a  parallelogram  of  equal  base  and  altitude,  by  Geom.  theor.  26, 

t  For.  let  ab,  ac,  be  the  two  given  sides,  in-  Q 
eluding  the  given  angle  a.  Now  £  ab  X  cp  is  the 
area,  by  the  first  rule,  cr  being  the  perpendicular. 
But  by  trigonometry,  as  sin.  JL  r,  or  radius : 
ac  : :  sin.  ^  a  :  cr,  which  is  therefore  =  ac  X 
era.  Z.  a,  taking  radius  =  1.  Therefore  the  area 
£a*  X  cp  is  =  Iab  X  ac  X  tin.  £  a,  lo  radius  I ; 
•r,  as  radios :  sis.  4  a x  :  Jab  x  ac  :  the  area. 


408 


X I2UU  RATI05 


Ex.  1.  What  hi  the  area  of  a  triangle,  whose  two  sides  are 
80  and  40,  and  their  contained  angle  28*  57'  ? 

By  Natural  Number*.  By  Lcgariikm. 
First,  J  X  40  X  30  =  600, 

then,  1  :  600  : :  -484046  sin.  28-  57'  log.  0-684887 

600  2  778151 


Anawer  290-4276  the  area  answ.  to    2  468088 

Ex.  3*  How  many  square  yards  contains  the  triangle  of 
which  one  angle  is  45%  and  its  containing  sides  25  and  21} 
feet  ?  Ans.  20-86047. 

Ruue  in.  When  the  three  sides  are  given  :  Add  all  the 
three  sides  together,  and  take  half  that  sum.  Next,  subtract 
each  aide  severally  from  the  said  half  sum,  obtaining  three 
remainders.  Then  multiply  the  said  half  sum  and  those  three 
remainders  all  together,  and  extract  the  square  root  of  the 
last  product,  for  the  area  of  the  triangle  f. 


t  For,  let  6  denote  the  base  a  a  of  the  triangle  abc  (see  the  last  fig.), 
also  a  the  side  ac,  and  e  the  side  ac.   Then,  by  Ibeor.  3, 

Trigon.  as  6  : «  +  e  : : «  —  ei  **~  -  =  ap  —  pb  the  diff.  of  the  seg> 
ments; 

-     ,      ,  oa — ec    bb  4-  aa  —  cc  4l_ 
theref.  J6-f  — —  =  —  =  the  segment  ap  ; 

hence  V^ao1  —  ap*)  =  the  perp.  cr,  that  is, 


CP. 


66  +  ««  —  «» 
V(as-(— ^  ))=  - 

Wb->~a<  +2b€i  —  »i-f  g«y  —  fi  _ 
V  466  " 

Bot  Jab  X  cp  is  the  area,  that  is, 

16  X  cp  =  V-  J — jg  1  

_  vima-bb-cc  +  2bc^-na  +  bb  +  cc  +  V>c)  (A) 

.  ( « +J±f  y  ii+  *±!  x  —  *±-e  v  tt*  r  •% 

—  v\      2  2  2      x  2 

=  V  { t X  (f  —  «)  X  («  —  A)  X  (•  —  c)  J,  which  is  toe  role, 
denotes  half  the  sum  of  the  three  sides. 

The  espressioa  marked  (A),  if  we  put  s  =  6  +  e,  and  d  for  6  —  f,  to 
equivalent  to  J  V  \  —  d  —  di)  j ;  which,  in  most  cases,  furnishes 
a  satire  commodious  rale  for  practice  than  rule  in.  here  gfren ;  espe- 
Ssatyv  t£  the  computet  have  a  table  of  squares  at  band, 


OF  PLANES. 


409 


If  the  aides  of  the  triangle  be  large,  then  add  the  logs,  of 
the  half  sum,  and  of  the  three  remainders  together,  and  half 
their  sum  will  be  the  log.  of  the  area. 

Ex.  1.  To  find  the  area  of  the  triangle  whose  three  sides 
are  20,  30, 40. 

20            45  45  45 

30            20  30  40 

40            —  —  — 

  25  1st  rem.  15  2d  rem.  5  3d  rem. 

2)  00            —  —  — 
45  half  sum 

Then  45  X  25  X  15  X  5  =  84375, 
The  root  of  which  is  290-4737,  the  area* 

Ex.  2.  How  many  square  yards  of  plastering  are  in  a 
triangle,  whose  sides,  are  30, 40,  50  feet  ?  Ans.  66}. 

Ex.  3.  How  many  acres,  &c.  contains  the  triangle,  whose 
aides  are  2569, 4900,  5025  links  ? 

Acs.  61  acres,  1  rood,  39  perches. 


PROBLEM  III. 

To  find  the  Area  of  a  Trapezoid. 

Add  together  the  two  parallel  sides  ;  then  multiply  their 
sum  by  the  perpendicular  breadth,  or  the  distance  between 
them  ;  and  take  half  the  product  for  the  area.  By  Geora. 
theor.  29. 

Ex.  1.  In  a  trapezoid,  the  parallel  sides  are  750  and  1225, 
and  the  perpendicular  distance  between  them  1540  links ;  to 
find  the  area. 
1225 
750 

1975  X  770  =  152075  square  links  —-15  arc.  33  perc. 

Ex.  2.  How  many  square  feet  are  contained  in  the  plank, 
whose  length  is  12  feet  6  inches,  the  breadth  at  the  greater 
end  15  inches,  and  at  the  less  end  11  inches  ? 

Ans.  13}}  feet. 

Ex.  3.  In  measuring  along  one  side  ab  of  a  quadrangular 
field,  that  side,  and  the  two  perpendiculars  let  fall  on  it  from 
the  two  opposite  corners,  measured  as  foUqw  \ 
content. 

Vol.  I  53 


410 


WCWITftATTOXf 


ap  =  110  links 


Ads.  4  acres,  1  rood,  5*792  perches. 


au=  745 

AB  =  1110 

cp  =  352 
pa-  595 


PROBLEM  IT* 


To  find  the  Area  of  any  Trapezium. 


Divide  the  trapezium  into  two  triangles  by  a  diagonal ; 
then  find  the  areas  of  these  triangles,  and  add  them  together. 

Or  thus,  let  fall  two  perpendiculars  on  the  diagonal  from 
the  other  two  opposite  angles  ;  then  add  these  two  perpen- 
diculars together,  and  multiply  that  sum  by  the  diagonal, 
taking  half  the  product  for  the  area  of  the  trapezium. 

Ex.  1.  To  find  the  area  of  the  trapezium,  whose  diagonal 
is  42,  and  the  two  perpendiculars  on  it  16  and  18. 

Here  16+18=  34,  its  half  is  17. 
Then  42  X  17  =  714  the  area. 

Ex.  2.  How  many  square  yards  of  paving  are  in  the  tra* 
pezium,  whose  diagonal  is  65  fe<;t,  and  the  two  perpendicu- 


Ex.  3.  In  the  quadrangular  field  abcd,  on  account  of  ob- 
structions there  could  only  be  taken  the  following  measures, 
viz.  the  two  sides  bc  265  and  ad  220  yards,  the  diagonal 
ac  378,  and  the  two  distances  of  the  perpendiculars  from  the 
ends  of  the  diagonal,  namely,  ae  160,  and  cf  70  yards.  Re- 
quired the  construction  of  the  figure,  and  the  area  in  acres, 
when  4840  square  yards  make  an  acre  ? 


To  find  the  Area  of  an  Irregular  Polygon. 

Draw  diagonals  dividing  the  proposed  polygon  into  tra» 
peziums  and  triangles.  Then  find  the  areas  of  all  these  se- 
parately, and  add  them  together  for  the  content  of  the  whole 
polygon. 


lars  let  fall  on  it  28  and  33£  feet  ? 


Ans.  222y9  yards. 


Ans.  17  acres,  2  roods,  21  perches. 


problem  v. 


or  PLAinct. 


abcdefga,  in  which  are  given  the  following  diagonals  and 
perpendiculars:  namely, 


To  find  the  Area  of  a  Regular  Polygon. 

Rule  i.  Multiply  the  perimeter  of  the  polygon,  or  sum 
of  its  sides,  by  the  perpendicular  drawn  from  its  centre  on 
one  of  its  sides,  and  take  half  the  product  for  the  area3". 

Ex.  1.  To  find  the  area  of  a  regular  pentagon,  ench  side 
being  25  feet,  and  the  perpendicular  from  the  centre  on  each 
side  17-2047737. 

Here  25  X  5  =  125  is  the  perimeter. 
And  17-2047737  X  125  =  2150  5967125. 
Its  half  1075*208356  is  the  area  sought^ 

Rule  n.  Square  the  side .  of  the  polygon  ;  then  multiply 
that  square  by  the  tabular  area,  or  multiplier  set  against  its 
name  in  the  following  table,  and  the  product  will  be  the 
areaf. 


•  This  is  only  in  effect  resolving  the  polygon  into  as  ninny  equal  tri- 
angles as  it  has  sides,  hy  drawing  lines  from  ihe  cent  re  to  all  the  angles; 
then  finding  their  areas,  and  adding  them  all  together. 

t  This  rule  is  founded  on  the  property,  thitt  like  polvgon«,  being  simi- 
lar figures,  are  to  one  another  as  the  Mpiares  of  their  Ifke  sides :  w»»icb 
is  proved  in  the  Geora.  theor.  89.  Now,  the  multipliers  iu  the  table, 
«re  the  areas  of  the  respective  polygons  to  the  side  1.  Whence  tLe 
rule  is  manifest. 


ac  55 


Ads.  1878}. 


fd  52 
€0  44 
em  13 

BR  18 

oo  12 
sp  8 
d?23 


PROBLEM  VI. 


413 


XXRtCBATIOIf 


No.  of 
Side*. 

Names. 

3~ 

Trigon  or  triangle 

4 

Tetragon  or  square 

5 

Pentagon 

6 

Hexagon 

7 

Heptagon 

8 

Octagon 

9 

Nonagon 

10 

Decagon 

11 

Undccagon 

12 

Dodecagon 

Areas,  or 

Radius  ot  cir- 

Multipliers. 

cum.  cin  !e. 

0-4330127 

05778503 

1-0000000 

0-7071068 

1-7204774 

0-8506508 

2-5980762 

1-0000000 

: -6339124 

1  1523824 

4-828*271 

1-3065628 

6-1818242 

1-4619022 

7-6942088 

1-6180340 

9-3656399 

1-7747324 

11  1961524 

1-9318517 

Exam.  Taking  here  the  same  example  as  before,  namely, 
a  pentagon,  whose  side  is  25  feet.  9 
Then  252  being  =  625, 
And  the  tabular  area  1  7204774  ; 
Theref.  1-7204774  X  625  =  1075-298375,  as  before. 
Ex.  2.  To  find  the  area  of  the  trigon  or  equilateral  tri- 
angle, whose  side  is  20.  Ans.  173-20508. 
Ex.  &•  To  find  the  area  of  the  hexagon  whose  side  is  20. 

Ans.  1039-23048. 
Ex.  4.  To  find  the  area  of  an  octagon  whose  side  is  20. 

Ans.  1931-37084. 
Ex.  5.  To  find  the  area  of  a  decagon  whose  side  is  20. 

Ans.  3077-68352. 

Note.  If  ab  *  1,  and  n  the  number  of  sides  of  the  poly- 
gon, then  area  of  polygon  —  n  times  area  of  the  triangle 
abc  =  ft  ad  .  dc  —  n  ad  tan.  c?ad  (to  rad.  ad)  =  in  tan.  cad 

180° 

=  in  cot.  ai  d  =  Jn  cot.   .    The  ra- 
ft 

dius  of  the  circumscribing  circle,  to  side  1, 
is  evidently  equal  fo  J  si*c.  cad.  Mulri-' 
plying,  therefore,  the  radius  of  the  table  by 
the  numeral  value  of  any  proposed  side,  the 
product  is  the  radius  of  a  circle  in  which 
that  polygon  may  be  inscribed ;  and  from  which  it  may 
readily  be  constructed. 


OF  PLANES. 


41S 


PROBLEM  VII. 

To  find  the  Diameter  and  Circumference  of  any  Circle,  the 
one  from  the  other. 

This  may  be  done  nearly,  by  either  of  the  four  following 
proportion*, 

viz.  As  7  is  to  22,  so  is  the  diameter  to  the  circumference. 
Or,  As  1  is  to  3-1410,  so  is  the  diam.  to  the  circumf. 
Or,  As  113  to  355,  so  is  the  diam.  to  the  circumf.* 
And,  as  1  :  '318309  : :  the  circumf.  :  the  diameter. 


*  For  let  abcd  benny  circle,  whose  centre  is 
z,  and  lei  ab,  bc,  he  any  two  equal  arcs.  Draw 
the  several  chords  as  in  the  figure,  and  join  be; 
also  draw  the  diameter  da.  which  produce  to  r, 
till  bp  be  equal  to  the  chord  bd. 

Then  the  two  isosceles  triangles  df.r,  dbf,  are 
equiangular,  because  they  have  the  angle  at  d 
common;  consequently  de  :  db  : :  dr  :  df.  But 
the  two  triangles  afb,  dcb,  are  identical,  or  equal 
in  all  re«pects,  because  they  have  the  angle  f  — 
the  an^le  biic,  being  each  equal  to  the  angle 
adb,  these  being  subtended  by  the  equal  arcs  ab, 
bc;  also  the  exterior  angle  fab  of  the  quadrnn-  . 
gle  abcd,  is  equal  to  the  opposite  interior  angle 
at  c  ;  and  the  two  triangles  have  also  the  side  bf  =  the  side  bd  ;  there- 
fore the  side  af  is  also  equal  in  the  side  dc.  Hence  the  proportion  above, 
viz.  de  :  db  : :  db  :  df  =  da  -J-  af,  becomes  dk  :  db  : :  db  :  2de  -|-  dc. 
Then,  by  taking  the  rectangles  of  the  extremes  and  means,  it  is  db->  = 
2db:-|-dk  .  DC. 

Now,  if  the  radius  de  be  taken  =  1,  this  exprestUafv becomes  db3  = 
2-|-  i>c.  and  hence  the  root  db  =.  V(2-f  dc).   That  is,  if  the  measure 
of  the  supplemental  chord  of  any  arc  be  increased  by  the  number  2,  the. 
sq  tare  root  of  the  sum  will  be  the  supplemental  chord  of  half  that  arc 
N  »w,  to  apply  this  to  the  calculation  of  the  circumference  of  the  cir- 
cle, let  the  arc  ac  be  taken  equal  to  \  of  the  circumference,  and  be  suc- 
cessively bisected  by  the  above  theorem :  thus  the  chord  ac  of  -J-  of  the 
1  circumference,  is  the  side  of  the  inscribed  regular  hexagon,  and  is  there- 
,  fore  equ.il  to  the  radius  ae  or  I  :  hence,  in  the  right-angled  triangle  a  CD, 
it  «  ill  be  dc  ^  V(ad  -  ac  )  =  V(  ,i—  1)  =  V3  =  1-7320508U76,  the 
supplemental  chord  of  X  of  the  periphery. 

Then,  by  the  foregoing  theorem,  by .  always  bisecting  the  aces,  end 
adding  2  to  the  last  square  root,  there  will  be  found  the  supplemental 
chords  of  the  l2th,  the  24th,  the  48th,  the  96th,  &c,  parts  of  the  peri- 
phery ;  thus. 


V  3 -7320 108076  : 
^/ 3-93 1 85 165*5  : 
^3  9828897227  : 
^3-9957178165  : 
v/3-9989291743  : 
v/3-9997322757  : 
v/3-9999330678  : 
V3-9999832669  - 


1-9318516525 
1-9828097227 
1-9957178465 

:  1-9939291743 
1*9997322757 

;  1-9999330G78 
1-9999832669 


°  1 

r  ^  i 

US 
—  o 

T¥ 

J8 

c 

3  JX  ' 

*u 

414 


MBIfSITBATIOlT 


1  .    .       '  V 

Ex.  1.  To.findtfie  circumference  of  the  circle  whose  dia- 
meter is  20. 

By  the  first  rale,  as  7  :  22  :  :  20  :  62j,  the  answer. 

Ex.  2.  If  the  circumference  of  the  earth  be  24877-4  miles, 
what  is  its  diameter  ? 

By  the  2d  rule,  as  3-1416  :  1  : :  24877-4  :  7918-7  nearly 
the  diameter. 

By  the  3d  rule,  as  355  :  113  :  :  24877-4  :  7918-7  nearly. 
i>;  u.e4lhrule,asl  :  -318309  :  :  24877  4  :  7918-7  nearly. 


PROBLEM  VIII. 

To  find  the  Length  of  any  Arc  of  a  Circle. 

Multiply  the  decimal  -017453  by  the  degrees  in  the 
given  arc,  and  that  product  by  the  radius  of  the  circle,  for  the 
length  of  the  arc*. 

Since  then  it  is  found  that  3*9999832669  is  the  square  of  fhe  supple- 
mental chord  of  the  1536th  part  of  the  periphery,  let  this  number  be 
Inker-  from  4,  which  is  the  square  of  the  diameter,  nnd  the  remainder 
0-0000167331  will  tie  the  square  of  the  chord  of  the  said  1 546th  part  of 
the  periphery,  and  consequently  the  root  \/O  00O0 167331  =  0-OO40906  U2 
is  the  length  of  that  chord;  this  number  then  being  multiplied  by  1536 
gives  6  2S3I7BS  for  the  perimeter  of  a  regular  polygon  of  1536  sides  in* 
scribed  in  the  circle;  which,  as  the  sides  of  the  polygon  nearly  coin- 
cide  with  the  circumference  of  the  circle,  must  also  express  the  length 
of  the  circumference  itself,  very  nearly. 

But  now,  to  show  how  near  this  determination  is  to 
the  truth,  let  a^p  =  0-0040906 1 12  represent  one  side 
of  such  a  regular  polygon  of  1536  side*,  and  «rt  a  side 
of  another  similar  polygon  described  about  the  circle; 
and  from  the  centre  e  let  the  perpendicular  zqR  be 
drawn,  bisecting  a p  and  st  in  q  nud  r.  Then  >ince 
a<i  is  =  4  ap  -  0  00i»  »4Vi05rt.  and  ka  =  I.  therefore 
»q'i  —  ka'—  ai^1  =  -9991)958167,  and  consequently  its 
root  gives  ei  =  -99991)791)8-1 ;  then  because  of  the  pa- 
rallels ap,  st,  it  is  p.q  :  kr  : :  ap  :  st  : :  as  the  whole  in- 
scribed perimeter:  to  the  circumscribed  one.  that  is, 
as  -9999979084  :  1  : :  6  283176*  :  6  28*1920  the  perime- 
ter of  the  circumscribed  polygon.  Now,  the  circum- 
ference of  the  circle  being  greater  than  the  perimeter  of  the  inner  poly- 
gon, but  less  limn  that  of  the  outer,  it  must  consequently  b«  greater 
than  6-283178& 

but  less  than  6-2831940, 

and  must  therefore  be  nearly  equal  to  £  their  sum,  <>r  6-2831854,  which 
%in  fact  is  true  to  the  last  figure,  which  fhould  be  a  3,  instead  of  the  4. 
Hence  the  circumference  heing  6-2831854  w  hen  the  diameter  is  2,  it 
will  be  the  half  of  that,  or  3  1415^27.  when  the  diameter  is  I,  to  which 
the  ratio  in  the  rule,  viz.  1  to  3- 14 16.  is  very  near.  Also  the  first  ratio 
in  the  rule,  7  to  22  or  1  to  3f  3- 1428  &c.  is  another  near  a pproii na- 
tion.   But  the  third  ratio,  1 13  to  355,  —  1  to  3- 14 15929,  is  the  nearest. 

*  It  having  been  found,  in  the  demonstration  of  the  foregoing  problem, 
that  when  the  radius  of  a  cArc\e\t  \,\V&  ItugLh  of  the  whole  circumie- 


OF  FLANKS. 


415 


Ex.  1.  To  find  the  length  of  an  arc  of  30  degrees,  the 
radius  being  0  feet.  Ans.  4-71231. 

Ex.  2.  To  find  the  length  of  an  arc  of  12  10',  or  12  J,  the 
radius  being  10  feet.  Ans.  2*1234. 

PROBLEM  IX. 

To  find  the  Area  of  a  Circle*. 

Rule  i.  Multiply  half  the  circumference  by  half  the 
diameter.  Or  multiply  the  whole  circumference  by  the  whole 
diameter,  and  take  \  of  the  product. 

Rule  ft.  Square  the  diameter,  and  multiply  that  square 
by  the  decimal  a7854,  for  the  area. 

Rule  in.  Square  the  circumference,  and  multiply  that 
square  by  the  decimal  -07958. 

Ex.  1.  To  find  the  area  of  a  circle  whose  diameter  is  1Q> 
and  its  circumference  31  '416. 

By  Rule  1.  By  Rule  2.  By  Rule  3. 

31-416  -7854  31-416 

10  103=   100  31-416 


4)314 16  ~*  986-965 

78-54  70  34  -07958 


78-54 


So  that  the  area  is  78*54  by  all  the  .three  rules. 


rence  is  6  2831854,  which  consists  of  360  degrees ;  therefore  as  3*0"  : 
6-2831854: :  1  :  017453,  kc.  the  length  of  the  arc  of  I  degree.  Hence  the 
decimal  -017453  multiplied  hy  any  number  of  degrees,  will  give  the  length 
of  the  arc  of  those  degrees.  And  because  the  circumferences  and  arcs  are 
in  proportion  as  the  diameters,  or  as  the  radii  of  the  circles,  therefore  as 
the  radius  1  is  to  any  other  radius  r,  so  is  the  length  of  the  arc  above 
mentioned,  to  '017453  X  degrees  in  the  arc  X  r>  which  is  the  length  of 
that  arc,  as  in  the  rule. 

*  The  first  rule  is  proved  in  the  Geom.  theor.  94. 

And  the  9d  and  3 1  rules  are  deduced  from  the  first  rule,  in  this  man- 
ner.—By  that  rule,  de  -i-  4  is  the  area,  when  d  denote*  the  diameter,  and 
t  the  circumference.  But, by  prob.  7,  e  is  =  3- 14 IrW ;  therefore  ihe  said 
area  de  -r  4,  becomes  (tX*14lfi<*-r>4  =  -78544',  which  gives  the  2d 
rale. — Also,  by  tho  snme  prob.  7,  d  is  =  c  -f-  3  1416;  therefore  again 
the  same  first  area  dr.  -f-  4,  becomes  (c  3*1416)  X  (c  4)  =  e- 
12-5664,  which  is  =  c*  X  07958,  by  taking  the  reciprocal  of  12  5664,  or 
changing  ibat  divisor  into  the  inuitipler  -07958 ;  which  gives  the  3d  rule. 

CoroL  Hence  the  areas  of  different  circles  are  in  proportion  to  one 
another,  as  the  square  of  their  diameters  or  as  the  square  oC  Umax  ^maNtr 
fereoces-  as  before  proved  in  the  Geom.  Iheor. 


416 


MEKST7IUTI0N 


Ex.  2.  To  find  the  area  of  a  circle,  whose  diameter  is  7, 
and  circumference  22.  Ans.  38$. 

Ex.  3.  How  many  square  yards  are  in  a  circle,  whose 
diameter  is  3  J  feet  ?  Ans.  1  -069. 

Ex.  4.  To  find  the  area  of  a  circle,  whose  circumference 
is  12  feet.  Ans.  11-4595. 


PROBLEM  X. 


To  find  the  Area  of  a  Circular  Ring,  or  of  the  Space  included 
between  the  Circumferences  of  two  Circles ;  tlie  "bite  being 
contained  within  the  other. 

Take  the  difference  between  the  areas  of  the  two  circles, 
as  found  by  the  last  problem,  for  the  area  of  the  ring. — Or, 
which  is  the  same  thing,  subtract  the  square  of  the  less  dia- 
meter from  the  square  of  the  greater,  and  multiply  their  dif- 
ference by  -7854. — Or,  lastly,  multiply  the  sum  of  the  dia- 
meters by  the  difference  of  the  same,  and  that  product  by 
•7854  ;  which  is  still  the  same  thing,  because  the  product  of 
the  sum  and  difference  of  any  two  quantities,  is  equal  to  the 
difference  of  their  squares. 

Ex.  1.  The  diameters  of  two  concentric  circles  being  10 
and  6,  required  the  area  of  the  ring  contained  between  their 
circumferences. 

Here  10  +  6  =  16  the  sum,  and  10  —  6  =  4  the  diff. 
Therefore  -7854  X  10  X  4  ^=  -7854  X  64  -  50  2656, 
the  area. 

Ex  2.  What  is  the  area  of  the  ring,  the  diameters  of  whose 
bounding  circles  are  10  and  20  ?  Ans.  235  62. 

PROBLEM  XI. 

To  find  the  Area  of  the  Sector  of  a  Circle. 

Rule  i.  Multiply  the  radius,  or  half  the  diameter,  by  half 
the  arc  of  the  sector,  for  the  area.  Or,  multiply  the  whole 
diumeter  by  the  whole  arc  of  the  sector,  and  take  £  of  the 
product.  The  reason  of  which  is  the  same  as  for  the  first 
rule  to  problem  9,  for  the  whole  circle. 

Rule  ii.  Compute  the  area  of  the  whole  circle  :  then  say, 
as 360  is  to  the  degrees  in  the  «rc  of  the  sector,  so  is  the  area 
of  the  whole  circle,  to  X\ve       <rt  toa  «&&&t. 


OP  PLAICES. 


41? 


This  is  evident,  because  the  sector  is  proportional  to  the 
length  of  the  arc,  or  to  the  degrees  contained  in  it. 

Ex.  1.  To  find  the  area  of  a  circular  sector,  whose  arc 
contains  18  degrees ;  the  diameter  being  3  feet. 
1.  By  the  first  Rule. 
First,  3-1416  X  3  =  0-4248,  the  circumference. 
And  360  :  18  : :  0-4848  :  -47124,  the  length  of  the  arc. 
Then  -47124  X  3  ^4=  1-41372  +  4  « -35343,  the  area. 

2;  By  the  2d  Rule. 
First,  -7854  X  3"  =  7-0686,  the  area  pf  the  whole  circle. 
Then,  as  360  :  18  :  :  7  0686  :  -35343,  the  area  of  the 
sector. 

Ex.  2.  To  find  the  area  of  a  sector,  whose  radius  is  10, 
and  arc  20.  Ans.  100. 

Ex.  3.  Required  the  area  of  a  sector,  whose  radius  is  25, 
and  its  arc  containing  147°  20'.  Ans.  804-3086. 


PROBLEM  XII. 


To  find  the  Area  of  a  Segment  of  a  Circle. 

Rule  I.  Find  the  area  of  the  sector  having  the  same  arc 
with  the  segment,  by  the  last  problem. 

Find  also  the  area  of  the  triangle,  formed  by  the  chord  of 
the  segment  and  the  two  radii  of  the  sector. 

Then  add  these  two  together  for  the  answer,  when  the 
segment  is  greater  than  a  semicircle :  or  subtract  them  when 
it  is  less  than  a  semicircle. — As  is  evident  by  inspection. 

Ex.  1.  To  find  the  area  of  the  segment  acbda,  its  chord 
▲b  being  12,  and  the  radius  ae  or  ce  10. 

First,  As  af  :  sin.  L.  d  00° :  :  ad  :  sin. 
86°  52'  J  =  36*87  degrees,  the  degrees  in  the 
aec  or  arc  ac.   Their  double,  73*74,  are 
the  degrees  in  the  whole  arc  acb.  \  J 

Now  -7854  X  400  =  314-16,  the  area  of  VX-/ 

the  whole  circle.  .  /  ' 

Therefore  360° :  73-74  : :  31416  :  ^3504,  area  of  the 
sector  acre. 

Again,  ^/(ab»  —  ad2)  =  ^(100  —  36)  =  ^/64  =  8  =  de. 
Theref.  ad  X  de  =*  6  X  8  =  48,  the  area  of  the  triangle 

AEB. 

Hence  sector  acbe  —  triangle  akb  =  16-3504,  area  of 
seg.  acbda. 

Rule  n.  Multiply  the  square  of  the  radius  of  the  circle 
by  either  half  the  difference  of  the  arc  acb  and  its  sine  (Jrtdrt 
Vol.  I.  54 


418 


MHIUBJkUOM 


to  the  radius  1),  or  half  the  sum  of  the;  arc  and  its  sine,  Ac* 
cording  as  the  segment  is  less  or  greater  than  a  semicircle ; 
the  product  will  be  the  area. 

The  reason  of  this  rule,  also*  is  evident  from  an  mspcetioo 
of  the  diagram. 

Exam,  the  same  as  before,  in  which  am  «  IS,  ax  a*  10 ; 
and  from  the  former  computation  are  acb  =  78*  44'f- 

Then,  by  Button's  Mathematical  Tables,  pp.  840,  ccc 
arc  73°  44'f,  to  radius  1  =*  1-2870059 
sin.  78°  44'},  to  radius  1  =  -9600010 


2)  -3270009 


•1685084 


whence,  -1635034  X  10*  =  16-35034,  the  area  of  thcseg- 

ment ;  very  nearly  as  before. 

Ex.  2.  What  is  the  area  of  the  segment,  whose  height  is 
18,  and  diameter  of  the  circle  50  ?  Ans.  636-375. 

Ex.  3.  Required  the  area  of  the  segment  whose  chord  is 
16,  the  diameter  being*  20  ?  Ans.  44-728,  or  269-432. 

PROBLEM  XIII. 

To  measure  long  Irregular  Figures. 

Take  or  measure  the  breadth  at  both  ends,  and  at  several 
places,  at  equal  distances.  Then  add  together  all  these  ia* 
termediate  breadths  and  half  the  two  extremes,  which  sum 
multiply  by  the  length,  and  divide  by  the  number  of  parts, 
for  the  area*. 


5  {jlj^t? 


*  This  rule  is  made  out  as  follows: 
— Let  abcd  be  the  irregular  piece ; 
having  the  several  breadths  ad,  bf,  oh, 
iKy  bc,  at  the  equal  distances  ak,  eg, 
oi,  u.  Let  the  several  breadths  in  or-  . 
der  be  denoted  by  the  corresponding  A  E  &  I  B 
letters  a,  bt  c,  d.  c,  and  the  whole  length 

ab  by  l\  then  compute  the  areas  of  the  parti  into  which  the  Store  » 
divided  by  the  perpendiculars,  as  so  many  trapezoids,  by  prob.  3,  aid 
add  them  all  together.   Thus,  the  sum  of  the  parts  is, 

=      x  it + tjf  x  y+ -  x  ii+Sf •  x  * 

=  «•  +  &  +  c  +  4  +  ft  X  V  =  <JR  -V  »  +  «  +  <*)  V. 


or  rums. 


JVbfe.  If  the  perpendiculars  or  breadths  be  not  at  equal 
distances,  compute  all  the  parts  separately,  as  so  many  trape- 
zoids, and  add  them  all  together  for  the  whole  area. 

Or  else,  add  all  the  perpendicular  breadths  together,  and 
divide  their  sum  by  the  number  of  them  for  the  mean 
breadth,  to  multiply  by  the  length ;  which  will  give  the  whole 
area,  not  fiur  from  the  truth. 

Ex.  1.  The  breadths  of  an  irregular  figure,  at  five  equi. 
distant  places,  being  8-2,  7-4,  9-2, 10-2,  8-6 ;  and  the  whole 
length  39 ;  required  the  area. 

8*2  35-2  sum. 

8-6  39 

2  )  16-8  sum  of  the  extremes.  8168 

8-4  mean  of  the  extremes.  1066 


7-4  4  )  1372-8 

9-2                                  343-2  An*. 
10-2   

36-2  sum. 

Ex.  2.  The  length  of  an  irregular  figure  being  84,  and  the 
breadths  at  six  equidistant  places  17*4,20-6, 14-2, 16-5, 20*1, 
24-4 ;  what  is  the  area?  Ana.  1550-64. 


FBOBLBM  XIV. 

To  find  Ae  Area  of  an  Ellipsis  or  Oval 

Multiply  the  longest  diameter,  or  axis,  by  the  shortest ; 
then  multiply  the  product  by  the  decimal  -7854,  for  the  area. 
As  appears  from  cor.  2,  theor.  3,  of  the  Ellipse,  in  the  Conic 
Sections. 

Ex.  1.  Required  the  area  of  an  ellipse  whose  two  axes  are 
70  and  50.  Ans.  2748-9. 

Ex.  2.  To  find  the  area  of  the  oval  whose  two  axes  are  24 
and  18.  Ans.  339-2928. 


which  if  the  whole  area,  agreeing  with  the  rule :  m  being  the  arithmeti- 
cal memo  between  the  extremes,  or  half  the  sum  of  them  both,  and  4 
the  number  of  the  parti.  And  the  same  for  any  other  aombet  «C  ?ute 
whatever. 


480  XBMlUBAnOIC 


NKOBLXH  XV. 

To  find  ike  Area  of  an  Elliptic  Segment. 

Find  the  area  of  a  corresponding  circular  segment,  having 
the  same  height  and  the  same  vertical  axis  or  diameter.  Then 
say,  as  the  said  vertical  axis  is  to  the  other  axis,  parallel  to 
the  segment's  base,  so  is  the  area  of  the  circular  segment 
before  found,  to  the  area  of  the  elliptic  segment  sought. 
This  rule  also  comes  from  cor.  2,  theor.  3,  of  the  Ellipse. 

Ex.  1.  To  find  the  area  of  the  elliptic  segment,  whose 
height  is  20,  the  vertical  axis  being  70,  and  the  parallel  axis 
60.  ins.  648  13. 

Ex.  2.  Required  the  area  of  an  elliptic  segment,  cut  off 
parallel  to  the  shorter  axis  ;  the  height  being  10,  and  the  two 
axes  25  and  35.  Ans.  162-03. 

Ex.  3.  To  find  the  area  of  the  elliptic  segment,  cut  off  pa- 
rallel to  the  longer  axis  ;  the  height  being  5,  and  the  axes  25 
and  35.  Ans.  97-8425. 

PROBLEM  XVI. 

To  find  the  Area  of  a  Parabola,  or  iU  Segment. 

MultiAy  the  base  by  the  perpendicular  height;  then 
take  two-thirds  of  the  product  for  the  area.  As  is  proved  in 
theorem  17  of  the  Parabola,  in  the  Conic  Sections. 

Ex.  1.  To  find  the  area  of  a  parabola ;  the  height  being  2, 
and  the  base  12. 

Here  2  X  12  =  24.    Then  %  of  24  =  16,  is  the  area. 

Ex.  2.  Required  the  area  of  the  parabola,  whose  height  is 
10,  and  its  base  16.  Ans.  106f. 


MENSURATION  OF  SOLIDS. 

By  the  Mensuration  of  Solids  are  determined  tho  spaces 
included  by  contiguous  surfaces ;  and  the  sum  of  the  met* 
sures  of  these  including  surfaces  is  the  whole  surface  or  su. 
perficies  of  the  body. 

The  measure  of  a  solid,  is  called  its  solidity,  capacity,  or 
content. 


o»  solids,  431 

Solids  are  measured  by  cubes,  whose  sides  are  inches,  or 
feet,  or  yards,  dec.  And  hence  the  solidity  of  a  body  is  said 
to  be  so  many  cubic  inches,  feet,  yards,  dec.  as  will  fill  its 
capacity  or  space,  or  another  of  an  equal  magnitude. 

The  least  solid  measure  is  the  cubic  inch,  other  cubes 
being  taken  from  it  according  to  the  proportion  in  the  fol- 
lowing table,  which  is  formed  by  cubing  the  linear  pro* 
portions. 

Table  of  Cubic  or  Solid  Measures. 

1728  cubic  inches  make '  1  cubic  foot 

27  cubic  feet        -  1  cubic  yard 

166|  cubic  yards     -  1  cubic  pole 

04000  cubic  poles      .  1  cubic  furlong 

512  cubic  furlongs  1  cubic  mile. 

PROBLEM  1. 

To  find  the  Superficies  of  a  Prism  or  Cylinder. 

Multiply  the  perimeter  of  one  end  of  the  prism  by  the 
length  or  height  of  the  solid,  and  the  product  will  be  the  sur- 
face of  all  its  sides.  To  which  add  also  the  area  of  the  two 
ends  of  the  prism,  when  required*. 

Or,  compute  the  areas  of  all  the  sides  and  ends  separately, 
and  add  them  all  together. 

Ex.  1.  To  find  the  surface  of  a  cube,  the  length  of  each 
side  be  ng  20  feet.  Ans.  2400  feet. 

Ex.  2.  To  find  the  whole  surface  of  a  triangular  prism, 
whose  length  is  ,  20  feet,  and  each  side  of  its  end  or  base  18 
inches.  Ans.  91*048  feet. 

Ex.  3.  To  find  the  convex  surface  of  a  round  prism,  or 
cylinder,  whose  length  is  20  feet,  and  the  diameter  of  its  base 
is  2  feet.  Ans.  125-664. 

Ex.  4.  What  must  be  paid  for  lining  a  rectangular  cistern 
with  lead,  at  3d.  a  pound  weight,  the  thickness  of  the  lead 
being  such  as  to  weigh  71b.  for  each  square  foot  of  surface  ; 
the  inside  dimensions  of  the  cistern  being  as  follow,  viz.  the 
length  3  feet  2  inches,  the  breadth  2  feet  8  inches,  and  depth 
2  feet  6  inches?  Ans.  32.  5s.  9jd. 


*  The  truth  of  this  will  easily  Appear,  by  considering  that  the  sides  of 
any  prism  are  parallelograms,  whose  common  length  is  the  same  as  Ibe 
length  of  the  solid,  and  their  breadths  taken  all  together  make  op  the 
perimeter  of  the  ends  of  the  same. 

And  the  rale  is  evidently  the  tame  for  the  tatta*  oAiqjYk&ki. 


MJUOTJRATSOIf 


PBOBLBMII. 


To  find  the  Surface  of  a  Pyramid  or  Cone. 

Multiply  the  perimeter  of  the  bate  by  the  riant  height, 
or  length  of  the  side,  and  half  the  product  will  evidently  be 
the  surface  of  the  sides,  or  the  sum  of  the  areas  of  all  the  tri- 
angles which  form  it.  To  which  add  the  area  of  the  end  or 
base,  if  requisite. 

Ex.  1.  What  is  the  upright  surface  of  a  triangular  pyra- 
mid, the  slant  height  being  20  feet,  and  each  side  of  the  base 
3  feet?  Ana.  90 feet. 

Ex.  2.  Required  the  convex  surface  of  a  cone,  or  circular 
pyramid,  the  slant  height  being  50  feet,  and  the  diameter  of 


To  find  the  Surface  of  the  Frustum  of  a  Pyramid  or  Cone, 
being  the  lower  pari,  when  the  top  is  cut  off  by  a  plane  pa- 
rallel to  the  base. 

Add  together  the  perimeters  of  the  two  ends,  and  multiply 
their  sum  by  the  slant  height,  taking  half  the  product  for  the 
answer. — As  is  evident,  because  the  sides  of  the  solid  are 
trapezoids,  having  the  opposite  sides  parallel. 

Ex.  1.  How  many  square  feet  are  in  the  surface  of  the 
frustum  of  a  square  pyramid,  whose  slant  height  is  10  feet ; 
also  each  side  of  the  base  or  greater  end  being  3  feet  4  inches, 
and  each  side  of  the  less  end  2  feet  2  inches  ?  Ans.  110  feet. 

Ex.  2.  To  find  the  convex  surface  of  the  frustum  of  a 
cone,  the  slant  height  of  the  frustum  being  12±  feet,  and 
the  circumferences  of  the  two  ends  6  and  8*4  feet. 


To  find  the  Solid  Cohtent  of  any  Prism  or  Cylinder. 

Find  the  area  of  the  base,  or  end,  whatever  the  figure  of 
it  may  be  ;  and  multiply  it  by  the  length  of  the  prism  or  cylin- 
der, for  the  solid  content*. 


Ans.  607-511. 


PROBLEM  m. 


Ans.  90  feet. 


PROBLEM  IV. 


•  This  rale  appears  from  the  Geom.  tbeor.  110,  cor.  2.  The  fMBe  » 
more  particularly  shown  at  follows:  Let  the  annexed  rectangular  parti 


OF  MUM. 


Note.  For  a  cube,  take  the  cube  of  its  aide  by  multiplying 
this  twice  by  itaelf ;  and  for  a  parallelopipedon,  multiply  the 
length,  breadth,  and  depth  all  together,  for  the  content. 

Ex.  1.  To  find  the  solid  content  of  a  cube,  whose  side  is 
24  inches.  Ans.  18834. 

Ex.  2.  How  many  cubic  feet  are  in  a  block  of  marble,  its 
length  being  3  feet  2  inches,  breadth  2  feet  8  inches,  and 
thickness  2  feet  6  inches  ?  Ans.  21}. 

Ex.  3.  How  many  gallons  of  water  will  the  cistern  con- 
tain, whose  dimensions  are  the  same  as  in  the  btst  example, 
when  277}  cubic  inches  are  contained  in  one  gallon  ? 

Ans.  131-53. 

Ex.  4.  Required  the  solidity  of  a  triangular  prism,  whose 
length  is  10  feet,  and  the  three  sides  of  its  triangular  end  or 
base  are  3, 4,  5  feet.  Ans.  60. 

Ex.  5.  Required  the  content  of  a  round  pillar,  or  cylinder, 
whose  length  is  20  feet,  and  circumference  5  feet  6  inches. 

Ans.  48*1450  feet. 


PROBLEM  V. 

To  find  the  Content  of  any  Pyramid  or  Cone. 

Find  the  area  of  the  base,  and  multiply  that  area  by  the 
perpendicular  height ;  then  take  £  of  the  product  for  the 
content*. 


lelopipedon  be  the  solid  to  be  measured, 
and  the  cube  r  the  solid  measuring  unit,  its 
side  being  1  inch,  or  1  foot,  Jtc. ;  also,  let 
the  length  and  breadth  of  the  base  abcd, 
and  also  the  height  ah,  be  each  divided 
into  spaces  equal  to  the  length  of  the  base 
of  the  cube  p,  namely,  here  3  in  the  length 
and  2  in  the  breadth,  matins;  3  times  2  or  6 
squares  in  the  base  ac,  each  equal  to  the 
base  of  the  cube  p.  Hence  it  is  manifest 
that  the  parallelopipedon  will  contain  the 
cube  p,  as  many  times  as  the  base  ac  con- 
tains the  base  of  the  cube,  repeated  as  often 
as  the  height  ah  contains  the  height  of  the  cube.  That  is,  the  contest 
of  any  parallelopipedon  is  found,  by  multiplying  the- are  a  of  the  base  by 
the  altitude  of  that  solid. 

And  because  all  prisms  and  cylinders  are  equal  to  parallelopfoedom 
of  equal  bases  and  altitudes,  by  Geom.  theor.  108,  it  follows  that  tne  rale 
b  general  for  all  such  solids,  whatever  the  figure  of  the  base  may  be. 

*  This  rule  follows  from  that  of  the  prism,  because  any  pyramid  if  -l 
of  a  prism  of  equal  base  and  altitude ;  by  Geom.  theot  AvVout. 


XBSrsVBATIOZf 


Ex.  1.  Required  the  solidity  of  a  square  pyramid,  each 
aide  of  its  base  being  30,  and  its  perpendicular  height  25. 

Ads.  7500. 

Ex.  2.  To  find  the  content  of  a  triangular  pyramid,  whose 
perpendicular  height  is  30,  and  each  side  of  the  base  8. 

Ans.  38-971143. 

Ex.  3.  To  find  the  content  of  a  triangular  pyramid,  its 
height  being  14  feet  6  inches,  and  the  three  sides  of  its  base 
5,  6, 7  feet.  Aim.  71*0352. 

Ex.  4.  What  is  the  content  of  a  pentagonal  pyramid,  its 
height  being  12  feet,  and  each  side  of  its  base  2  feet  ? 

Ans.  27-5276. 

Ex.  5.  What  is  the  content  of  the  hexagonal  pyramid, 
whose  height  is  6*4  feet,  and  each  side  of  its  base  6  inches  1 

Ans.  1-38564  feet. 

Ex.  6.  Required  the  content  of  a  cone,  its  height  being 
lty  feet,  and  the  circumference  of  its  base  9  feet, 

Ans.  22-56093. 


PROBLEM  VI. 


To  find  the  Solidity  of  a  Frustum  of  a  Cone  or  Pyramid. 

Add  into  one  sum,  the  areas  of  the  two  ends,  and  the 
mean  proportional  between  them  :  and  take  \  of  that  sum 
for  a  mean  area  ;  which  being  multiplied  by  tne  perpen- 
dicular height,  or  length  of  the  frustum,  will  give  its  con- 
tent*. 


*  Let  abcd  be  any  pyramid,  of  which  bcdofe  is 
a  frustum.  And  put  a2  for  the  area  of  I  he  base  rcd, 
b9  the  area  of  the  top,  rfo,  A  the  height  ih  of  the 
frustum,  and  c  the  height  ai  of  the  top  part  above 
it.  Then  c  -\-  A  =  ah  is  the  height  of  the  whole 
pyramid. 

Hence,  by  the  last  prob.  (c-fM  is  the  content 
of  the  whole  pyramid  abcd.  and  {b'c  the  content 
of  the  top  part  akfo  ;  therefore  the  difference  -  -  - 
|a*(c  +  A)  —  J6?c  is  the  content  of  the  frustum 
bcdgfjc.  fiat  the  quantity  c  being  no  dimension  of 
the  frustum,  it  mutt  be  expelled  from  this  formula,  by  substituting  iti 
value,  found  in  the  following  manner.  By  Geom.  theor.  1 12,  «  J :  £» : : 
(c  +  A)« :  c\  or  « :  b  : :  e  +  A :  c,  hence  (ficom.  th.  69)  a  —  b  :  b  : :  A  :  c, 

6A  cA 

and«  —  b  :  a  : :  A :  c  4-  A ;  hence  therefore  c  =  —j-  and  c  -f-  A  =  — . ; 


OP  SOLIDS. 


435 


Note.  This  general  rule  may  be  otherwise  expressed,  as 
follows,  when  the  ends  of  the  frustum  arc  circles  or  regular 
polygons.  In  this  latter  case,  square  one  side  of  each  poly, 
gon,  and  also  multiply  the  one  side  by  the  other ;  add  all 
these  three  products  together ;  then  multiply  their,  sum  by 
the  tabular  area  proper  to  the  polygon,  and  take  one-third  of 
the  product  for  the  mean  area,  to  be  multiplied  by  the  length, 
to  give  the  solid  content.  And  in  the  case  of  the  frustum- 
of  a  cone,  the  ends  being  circles,  square  the  diameter  or  the 
circumference  of  each  end,  and  also  multiply  the  same  two 
dimensions  together ;  then  take  the  sum  of  the  three  pro- 
ducts, and  multiply  it  by  the  proper  tabular  number,  viz.  by 
•7854  when  the  diameters  are  used,  or  by  '07958  in  using 
the  circumferences ;  then  taking  one-third  of  the  product,  to 
multiply  by  the  length,  for  the  content. 

Ex.  1.  To  find  the  number  of  solid  feet  in  a  piece  of  tim- 
ber, whose  bases  are  squares,  each  side  of  the  greater  end 
being  15  inches,  and  each  side  of  the  less  end  6  inches ;  also, 
the  length  or  the  perpendicular  altitude  24  feet.     Ans.  19 J. 

Ex.  2.  Required  the  content  of  a  pentagonal  frustum, 
whose  height  is  5  feet,  each  side  of  the  base  18  inches  ;  and 
each  side  of  the  top  or  less  end  6  inches.    Ans.  9-31925  feet. 

Ex.  3.  To  find  the  content  of  a  conic  frustum,  the  altitude 
being  18,  the  greatest  diameter  6,  and  the  least  diameter  4. 

Ans.  527-788P. 

Ex.  4.  What  is  the  solidity  of  the  frustum  of  a  cone,  the 
'  altitude  being  25,  also  the  circumference  at  the  greater  end 
being  20,  and  at  the  less  end  10  ?  Ans.  464-216. 

Ex.  5.  If  a  cask,  which  is  two  equal  conic  frustums  joined 
together  at  the  bases,  have  its  bung  diameter  28  inches,  the 
bead  diameter  20  inches,  and  length  40  inches ;  how  many 
gallons  of  wine  will  it  hold  ?  Ans.  79-0613. 


then  these  values  of  c  and  e  +h  being  substituted  for  them  in  the  ex- 
pression for  the  content  of  the  frustum  gives  that  content 

=  *a> - Xfl-^j  =  V*  X^=p  =  lhx(*  +  ab  +  b*);  which 

to  the  rale  above  given ;  ak  being  the  mean  between  a9  and  a*. 

Note.  If  d,  d  be  the  corresponding  linear  dimensions  of  ihe  ends,  6 
their  difference,  m  the  appropriate  multiplier,  h  the  height  of  the  frus- 
tum, then  is  the  content  =  JmA  (3ixf  +  6)  ;  which  is  a  coavenieot  prac- 
tical expression. 


Vol-  I.  55  ' 


426 


MKIfttJBATIOIf 


PROBLEM  VII. 

To  find  the  Surface  of  a  Sphere,  or  any  Segment. 

Rule  i.  Multiply  the  circumference  of  the  sphere  by 
its  diameter,  and  the  product  will  be  the  whole  surface  of 
it*. 

Rulk  u.  Square  the  diameter  and  multiply  that  square  by 
3*1416,  for  the  surface. 

Rulk  hi.  Square  the  circumference  ;  then  either  multi- 
ply that  square  by  the  decimal  '31 83,  or  divide  it  by  8-1416, 
for  the  surface. 

Note.    For  the  surface  of  a  segment  or  frustum,  multiply 


*  These  rules  come  from  the  following  theorems  for  the  surface  of  a 
sphere,  viz.  That  the  said  surface  is  equal  to  the  curve  surface  of  ^cir- 
cumscribing cylinder;  or  Hint  it  is  equal  to  4  great  circles  of  the  same 
sphere,  nr  of  l he  ?ame  diameter;  which  are  thus  proved. 

Let  abcd  be  a  cylinder,  circumscribing  the 
Sphere  eioh  ;  the  former  genertitr d  by  the  J± 
rotation  of  the  rectangle  fbch  about  the  axis 
or  dimeter  fii  ;  and  the.  latter  by  the  rota- 
tion of  the  semicircle  fgh  about  the  same  di- 
ameter fh.  Draw  two  lines  kl,  mi»,  perpen- 
dicnlar  to  the  axis,  intercepting  the  paits  i.n, 
op,  of  the  cylinder  and  sphere  ;  then  will  the 
ring  or  cylindric  surface  generated  by  the  ro- 
tation of  i  n,  be  equal  to  the  ring  or  fpherical 
surface  generated  by  the  arc  op.  For,  first,  ™ 
suppose  the  parallels  ki.  and  ms  to  be  indefi- 
nitely near  together;  drawing  10,  and  also  oo.  parallel  to  iji.  Then  the 
t\\  o  triangles  iko.  oqp,  being  equiangular,  it  is,  as  op  :  oq  or  LR  : :  so  or 
ki-  :  ko  ::  circumference  described  by  kl  :  circiimf.  described  by  so; 
therefore  the  rectangle  op.xcirciimf.  of  ko  is  equal  to  the  rectangle  l*X 
circumf.  of  ki.;  that  is,  the  ring  described  by  op  on  the  sphere,  iseqoal 
to  the  ring  described  by  l.n  on  the  rylindt-r. 

And  as  this  is  every  where  the  case,  therefore  the  sums  of  any  corres- 
ponding number  of  tln-se  are  also  equal ;  that  is.  the  whole  surface  of 
the  sphere,  described  by  the  whole  semicircle  fgh,  is  equal  to  the  whole 
curve  surface  of  the  cylinder,  described  by  the  height  bc  ;  as  well  as  the 
surface  of  any  >  cement  described  by  fo,  equal  to  the  surface  of  the  cor- 
responding segment  described  by  el. 

Corol.  I.  Hence  'he  smface  of  the  sphere  is  equal  to  4  of  its  great  cir- 
cles or  equal  to  the  circumference  efgh,  or  of  dc,  multiplied  by  tat 
height  bc.  or  by  the  diameter  fh. 

Corol.  2.  Hence  also,  the  surface  of  any  such  part,  as  a  segment  or 
frustum,  or  zone,  is  equal  to  the  same  circumference  of  the  sphere,  mal- 
tiplied  by  the  height  of  the  said  part.  And  consequently  such  spheri- 
cal curve  surfaces  are  to  one  auotber  in  the  same  proportion  as  their 
altitudes. 


OP  SOLIDS. 


437 


the  whole  circumference  of  the  sphere  by  the  height  of  the 
part  required. 

Ex.  1.  Required  the  convex  superficies  of  a  sphere,  whose 
diameter  is  7,  and  circumference  22.  Ans.  154. 

Ex.  2.  Required  the  superficies  of  a  globe,  whose  diameter 
is  24  inches.  Ans.  1809-5616. 

Ex.  3.  Required  the  area  of  the  whole  surface  of  the 
earthy  its  diameter  being  71)57 J  miles,  and  its  circumferenco 
25000  miles.  Ans.  198943750  sq.  miles. 

Ex.  4.  The  axis  of  a  sphere  being  42  inches,  what  is  the 
convex  superficies  of  the  segment  whose  height  is  9  inches  ? 

Ans.  1187-5248  inches. 

Ex.  5.  Required  the  convex  surface  of  a  spherical  zone, 
whose  breadth  or  height  is  2  feet,  and  cut  from  n  sphere  of 
12»  feet  diameter.  Ans.  78-54  feet. 


PROBLEM  Vin. 

7b  find  the  Solidity  of  a  Sphere  or  Globe. 

Rule  i.  Multiply  the  surface  by  the  diameter,  and  take 
|  of  the  product  for  the  content*.  Or,  which  is  the  same 
thing,  multiply  the  square  of  the  diameter  by  the  circum. 
ference,  and  take  }  of  the  product. 

Rulr  H.  Take  the  cube  of  the  diameter,  and  multiply  it 
by  the  decimal  '5236,  for  the  content. 

Rule  in.  Cube  the  circumference,  and  multiply  by 
•01688. 

Ex.  1.  To  find  the  solid  content  of  the  globe  of  the  earth, 
supposing  its  circumference  to  be  25000  miles. 

Ans.  263750000000  miles. 

Ex.  2.  Supposing  that  a  cubic  inch  of  cast  iron  weighs 
•269  of  a  lb.  avoird.  what  is  the  weight  of  an  iron  bull  of 
5-04  inches  diameter  ? 


*  For.  nnt  d  =  the  diameter,  c  =  the  circumference,  end  t  —  the 
surface  of  the  sphere,  or  of  its  circumscribing  cylinder  ;  also,  a  —  the 
number  3-1416. 

Then,  \t  is  =.  the  base  of  the  cylinder,  or  one  gre«t  circle  of  the 
sphere ;  and  d  is  the  height  of  the  cylinder :  then-fore  \ds  is  lite  cniifent 
of  the  cylinder.  But  {  of  the  cylinder  is  the  sphere,  liy  th.  117,  Gcom. 
that  it,  §  of  $d$%  or^ds  is  the  sphere ;  which  is  the  first  rule. 

Again,  because  the  surface  « is  =  ad*;  iherefore  ±*h  _  \nd*  —  5MM\ 
U  the  content,  as  in  the  2d  rule.  Also,  d  being  =  c  a,  therefore 
t*d*  =         a*  =  •01088,  the  3d  rule  for  the  content* 


488 


MJBH  S  UKATfON 


PROBLEM  K. 


7b  find  the  Solid  Content  of  a  Spherical  Segment. 

*  Rule  i.  From  3  tiroes  the  diameter  of  the  sphere 
take  double  the  height  of  the  segment;  then  multiply  the  re* 
mainder  by  the  square  of  the  height,  and  the  product  by  the 
decimal  -5230,  for  the  content. 

Rule  ii.  To  3  tiroes  the  square  of  the  radius  of  the 
segment's  base,  add  the  square  of  its  height ;  then  multiply 
the  sum  by  the  height,  and  the  product  by  '5236,  for  the 
content. 

Ex.  1 .  To  find  the  content  of  a  spherical  segment,  of  2 
feet  in  height,  cut  from  a  sphere  of  8  feet  diameter. 

Ans.  41-888. 


0 

•  By  corol.  3,  of  theor.  117,  Geom.  it  ap- 
pears thnt  the  spheiic  segment  prit,  is  equal 
to  the  difference  between  the  cylinder  ablo, 
and  the  conic  frustum  abmq. 

But,  putting  d  =  ab  or  fh  the  diameter  of  £ 
the  sphere  or  cylinder,  /*  =  fk  the  height  of 
the  segment,  r  =  pk  the  radius  of  its  lm«c, 
and  a  =  3*1416;  ihen  the  content  of  the 
tone  abi  is  =  \ad*  X  Jfi  —  :  and  by 

the  similar  cones  abi,   qmi,  as  ri1:  si1  : : 

^adx :  ^ad*  X  (r-^j—)1  =  the  cone  <*m ;  therefore  the  cone  abi  — 

the  cone  qsti  =  &ad*  —  J^i  X  (*-""-  V  =  iad*  —  b*dk*  +  J**1 

is  =  the  conic  frustum  of  abm<*. 
And  \atl  h  is  —  the  cylinder  ablo. 

Then  the  difference  of  these  tw  o  is  jmfti  —  \ah^  =  \ah*  X  (3rf  —21), 
for  the  spheric  segment  pfn  ;  whirh  is  ihe  first  rule. 
Again,  because  pk*  =  fk  X  kh  (cor.  to  theor.  87,  Geom.)  or  r1  =  k 

(d- A), therefore =         /*,  and  2d  -  <J>  =  ^+«=^L+i; 

3ri  -4-  A* 

which  being  substituted  in  the  former  rule,  it  becomes  \ah*  X  —  ^  — 

=  +*A  X  (  *r'-M  ),  which  is  (he  2d  rule. 

Note.  By  subtracting  a  segn  ent  from  n  half  sphere,  or  from  another 
tegmeiit,  the  content  o(  my  faiiitam  or  tone  may  be  found. 


or  MUM.  429 

*Ex.  2.  What  is  the  solidity  of  the  segment  of  a  sphera,  its 
height  being  9,  and  the  diameter  of  its  base  20  ? 

Ana.  1795*4344. 


Arte.  The  general  rules  for  measuring  the  most  useful 
figu-es  having  been  now  delivered,  we  may  proceed  to  apply 
them  to  the  several  practical  uses  in  life,  as  follows. 


[  430  ] 


LAND  SURVEYING. 


SECTION  I. 

DESCRIPTION  AND  USE  OF  THE  INSTRUMENTS. 

1.  OF  THE  CHAIN. 

Land  is  measured  with  a  chain,  called  Gunter's  Chain, 
from  its  inventor,  the  length  of  which  is  4  poles,  or  22  yards, 
or  66  feet.  It  consists  of  100  equal  links ;  and  the  length 
of  each  link  is  therefore  j'fo  of  a  yard,  or  of  a  foot,  or 
7 -92  inches. 

Land  is  estimated  in  acres,  roods,  and  perches.  An  acre 
is  equal  to  10  square  chains,  or  as  much  as  10  chains  in  length 
and  1  chain  in  hreadth.  Or,  in  yards,  it  is  220  X  22  =  4840 
square  vards.  Or,  in  poh»s,  it  is  40  X  4  =  160  square  poles. 
Or,  in 'links,  it  is  1000  X  100  —  100000  square  links: 
these  being  all  the  same  quantity. 

Also,  an  acre  is  divided  into  4  parts  called  roods,  and  a 
rood  into  40  parts  called  perches,  which  are  square  poles,  or 
the  square  of  a  pole  of  yards  long,  or  the  square  of  £  of  a 
chain,  or  of  25  links,  which  is  625  square  links.  So  that  the 
divisions  of  land  measure  will  be  thus  : 

625  sq.  links  —  1  pole  or  perch 
40  perches  =  1  rood 
4  roods      =  1  acre. 

The  lengths  of  lines  measured  with  a  chain,  are  best  set 
down  in  links  as  integers,  every  chain  in  length  being  100 
links  ;  and  not  in  chains  and  decimals.  Therefore,  after  the 
content  is  found,  it  will  he  in  square  links;  then  cut  off  five 
of  the  figures  on  the  right  h;ind  for  decimals,  and  the  rest  will 
be  acres.  These  decimals  are  then  multiplied  by  4  for  roods, 
and  the  decimals  of  these  again  by  40  for  perches. 


LAUD  SUB  YE  TING. 


481 


Exam.  Suppose  tho  length  of  a  rectangular  piece  of  ground 
be  ?£2  Lnks,  and  its  breadth  385  ;  to  fi.ul  the  area  in  acres, 
roods,  aud  perches. 

792  3  04020 

385  4 


•K680 

6336  40 
2376   


3  (49*0 


7-8*200 


Ans.  3  aores,  0  roods,  7  perches. 

2.  OF  THE  PLAIN  TABLE. 


This  instrument  consists  of  a  plain  rectangular  board,  of 
any  convenient  size  :  the  centre  of  which,  when  used,  is  fixed 
by  means  of  screws  to  a  three-legged  stand,  having  a  hall 
and  socket,  or  other  joint,  at  the  top,  by  means  of  which, 
when  the  legs  are  fixed  on  the  ground,  the  table  is  inclined 
in  any  direction. 

To  the  table  belong  various  parts,  as  follow. 

1.  A  frame  of  wood,  made  to  fit  round  its  edges,  and  to 
be  taken  off,  for  the  convenience  of  putting  a  sheet  of  paper 
on  the  table.  One  side  of  this  frame  is  usually  divided  into 
equal  parts,  for  drawing  lines  across  the  table,  parallel  or 
perpendicular  to  the  sides  ;  and  the  other  side  of  the  frame 
is  divided  into  360  degrees,  to  a  centre  in  the  middle  of  the 
table ;  by  means  of  which  the  table  may  be  used  as  a  theo- 
dolite, dec. 

2.  A  magnetic  needle  arid  compass,  either  screwed  into  the 
side  of  the  table,  or  fixed  beneath  its  centre,  to  point  out  the 
directions,  and  to  be  a  check  on  the  sights. 

3.  An  index,  which  is  a  brass  two-foot  scale,  with  either 
a  small  telescope,  or  open  sights  set  perpendicularly  on  the 
ends.  These  sights  and  one  edge  of  the  index  are  in  the  same 
plane,  and  that  is  called  the  fiducial  edge  of  the  index. 

To  use  this  instrument,  take  a  sheet  of  paper  which  will 
cover  it,  and  wet  it  to  make  it  expand  ;  then  spread  it  flat  on 
the  table,  pressing  down  the  frame  on  the  edges,  to  stretch 
it  and  keep  it  fixed  there  ;  and  when  the  paper  is  become 
dry,  it  will,  by  contracting  again,  stretch  itself  smooth  and 
flat  from  any  cramps  and  unevenness.  On  this  paper  is  to 
be  drawn  the  plan  or  form  of  the  thing  measured. 

Thus,  begin  at  any  proper  part  of  the  ground,  and  make 
a  point  on  a  convenient  part  of  the  paper  or  tabic,  to  reore. 
sent  that  place  on  the  ground  ;  then  fix.  vu  \tax  ^oveft. 


482 


LAND 


leg  of  (he  compasses,  or  a  fine  steel  pin,  and  apply  to  it  the 
fiducial  edge  of  the  index,  moving  it  round  till  through  the 
aights  you  perceive  some  remarkable  object,  as  the  corner  of 
a  field,  dtc.  ;  and  from  the  station-point  draw  a  line  with  the 
point  of  the  compasses  along  the  fiducial  edge  of  the  index, 
which  is  called  setting  or  taking  the  object :  than  set  another 
object  or  corner,  and  draw  its  line  ;  do  the  same  by  another ; 
and  so  on,  till  as  many  objects  are  taken  as  may  be  thought 
fit*  Then  measure  from  the  station  towards  as  many  of  toe 
objects  as  may  be  necessary,  but  not  more,  taking  the  requi- 
site offsets  to  corners  or  crooks  in  the  hedges,  laying  the 
measures  down  on  their  respective  lines  on  the  table.  Then 
at  any  convenient  place  measured  to,  fix  the  table  in  the 
same  position,  and  set  the  objects  which  appear  from  that 
place  ;  and  so  on,  as  before.  And  thus  continue  till  the 
work  is  finished,  measuring  such  lines  only  as  are  necessary, 
and  determining  as  many  as  may  be  by  intersecting  lines  of 
direction  drawn  from  different  stations. 

Of  shifting  the  Paper  on  the  Plain  Table. 

When  one  paper  is  full,  and  there  is  occasion  for  more, 
draw  a  line  in  any  manner  through  the  farthest  point  of  the 
last  station  line,  to  which  the  work  can  be  conveniently  laid 
down  ;  then  take  the  sheet  off  the  table,  and  fix  another 
on,  drawing  a  line  over  it,  in  a  part  the  most  convenient  for 
the  rest  of  the  work  ;  then  fold  or  cut  the  old  sheet  by  the 
line  drawn  on  it,  applying  the  edge  to  the  line  on  the  new 
sheet,  and,  as  they  lie  in  that  position,  continue  the  last  sta- 
tion line  on  the  new  paper,  placing  on  it  the  rest  of  the 
measure,  beginning  at  where  thu  old  sheet  left  off.  And  so 
on  from  sheet  to  sheet. 

When  the  work  is  done,  and  you  would  fasten  all  the 
sheets  together  into  one  piece,  or  rough  plan,  the  aforesaid 
lines  are  to  be  accurately  joined  together,  in  the  same  man* 
ncr  a8  when  the  lines  were  transferred  from  the  old  sheets 
to  the  new  ones.  But  it  is  to  be  noted,  that  if  the  said  join, 
ing  lines,  on  the  old  and  new  sheets,  have  not  the  same  in- 
clination to  the  side  of  the  table,  the  needle  will  not  point  to 
the  original  degree  when  the  table  is  rectified  ;  and  if  the 
needle  be  required  to  respect  still  the  same  degree  of  the 
compass,  the  easiest  way  of  drawing  the  line  in  the  same 
position,  is  to  draw  them  both  parallel  to  the  same  sides  of 
the  table,  by  means  of  the  equal  divisions  marked  on  the 
other  two  sides. 


SUItVBYlNQ. 


m 


3.  OF  THE  THEODOLITE. 

The  theodolite  is  a  brazen  circular  ring,  divided  into  360 
degrees,  &c.  and  having  an  index  with  sights,  or  a  telescope, 
placed  on  the  centre,  about  which  the  index  is  moveable  ; 
also  a  compass  fixed  to  the  centre,  to  point  out  courses  and 
check  the  sights  ;  the  whole  being  fixed  by  the  centre  on  a 
stand  of  a  convenient  height  for  use. 

In  using  this  instrument,  an  exact  account,  or  field-book, 
of  all  measures  and  things  necessary  to  be  remarked  in  the 
plan,  ntust  be  kept,  from  which  to  make  out  the  plan  on  re- 
turning home  from  the  ground. 

Ilegin  at  such  part  of  the  ground,  and  measure  in  such 
directions  as  are  judged  most  convenient ;  taking  angles  or 
directions  to  objects,  and  measuring  such  distances  as  appear 
necessary,  under  the  same  restrictions  as  in  the  use  of  the 
plain  table.  And  it  is  safest  to  fix  the  theodolite  in  the 
original  position  at  every  station,  by  means  of  fore  and  back 
objects,  and  the  compass,  exactly  as  in  using  the  plain  table ; 
registering  the  number  of  degrees  cut  off  by  the  index  when 
directed  to  each  object  ;  and,  at  any  station,  placing  the 
index  at  the  same  degree  as  when  the  direction  towards  that 
station  was  taken  from  the  last  preceding  one,  to  fix  the 
theodolite  there  in  the  original  position. 

The  best  method  of  laying  down  the  aforesaid  lines  of 
direction,  is  to  describe  n  pretty  large  circle  ;  then  quarter  it, 
and  lay  on  it  the  several  numbers  of  degrees  cut  off  by  the 
index  in  each  direction,  and  drawing  lines  from  the  centre  to 
all  these  marked  points  in  the  circle.  Then,  by  means  of  a 
parallel  ruler,  draw  from  station  to  station,  lines  parallel  to 
the  aforesaid  lines  drawn  from  the  centre  to  the  respective 
points  in  the  circumference. 

4.  OF  THE  CROSS. 

The  cross  consists  of  two  pair  of  sights  set  at  right  angles 
to  each  other,  on  a  staff  having  a  sharp  point  at  the  bottom, 
to  fix  in  the  ground. 

Tho  cross  is  very  useful  to  measure  small  and  crooked 
pieces  of  ground.  The  method  is,  to  measure  a  base  or  chief 
line,  usually  in  the  longest  direction  of  the  piece*  from  corner 
to  corner  ;  and  while  measuring  it,  finding  the  places  where 
perpendiculars  would  fall  on  this  line,  from  the  several  cor- 
nere  and  bends  in  the  boundary  of  the  piece,  with  the  cross, 
by  fixing  it,  by  trials,  on  such  parts  of  the  line,  as  that 
through  one  pair  of  the  sights  both  ends  of  the  line  may 
appear,  and  through  the  other  pair  the  rom«^uKv&%taro&i 

Vol.  I.  66 


m 


urn 


or  corners  :  and  then  measuring  die  lengths  of  the  eni  Tp«  r 

pendiculors. 

BEXAMS* 

Besides  the  fore*mentioned  instruments,  whic't  ere  mcst 
commonly  used,  there  are  some  others ;  as, 

The  perambulator,  used  for  measuring  roads,  and  other 
great  distances,  level  ground,  and  by  the  sides  of  rivers.  It 
has  a  wheel  of  8}  feet,  or  half  a  pole,  in  circumference*  by 
the  turning  of  which  the  machine  goes  forward  ;  and  the 
.  distance  measured  is  pointed  out  by  an  index,  which  is  moved 
round  by  clock-work. 

Levels,  with  telescopic  or  other  sights,  are  used  to  find 
the'  level  between  place  and  place,  or  how  much  one  place 
is  higher  or  lower  than  another.  And  in  measuring  any 
sloping  or  oblique  line,  either  ascending  or  descending,  a  small 
pocket  level  is  useful  for  showing  how  many  links  lor  each 
chain  are  to  be  deducted,  to  reduce  the  tine  to  the  hori- 
zontal length. 

An  offset. staff  is  a  very  useful  instrument,  for  measuring 
the  offsets  and  other  short  distances.  It  is  10  links  in  length, 
being  divided  and  marked  at  each  of  the  10  links. 

'J  en  small  arrows,  or  rods  of  iron  or  wood,  are  used  to 
mark  the  end  of  every  chain  length,  in  measuring  lines. 
And  sometimes  pickets,  or  staves  with  flags,  are  set  up  as 
marks  or  objects  of  direction. 

Various  scales  are  also  used  in  protracting  and  measuring 
on  the  plan  or  paper  ;  such  as  plane  scales,  line  of  chords, 
protractor,  compasses,  reducing  scale,  parallel  and  pc  rpen- 
dicular  rules,  dec.  Of  plane  scales,  there  should  be  several 
sizes,  as  a  chain  in  1  inch,  a  chain  in  }  of  an  inch,  a  chain 
in  £  an  inch,  &c.  And  of  these,  the  best  for  use  are  those 
that  are  laid  on  the  very  edges  of  the  ivory  scale,  to  mark  off 
distances,  without  compasses. 


SECTION  IL 

THE  PRACTICE  OF  SURVEYING. 

This  part  contains  the  several  works  proper  to  be  dc  n*»  in 
the  field,  or  the  ways  of  measuring  by  all  the  instaiaeots, 
aud  in  all  situations. 


•UBVBViire, 


PBO^EH  I. 

7b  measure  a  Line  or  Distance. 

To  measure  a  line  on  the  ground  with  the  chain  :  Having 
provided  a  chain,  with  10  small  arrows,  or  rods,  to  fix  one 
into  the  ground,  as  a  mark,  at  the  end  of  every  chain  ;  two 
persons  take  hold  of  the  chain,  one  at  each  end  of  it  ;  nnd 
all  the  10  arrows  are  taken  by  one  of  them,  who  goes  fore- 
most, and  is  called  the  leader ;  the  other  being  called  the 
follower,  for  distinction's  sake. 

A  picket,  or  station-staff,  being  set  up  in  the  direction  of 
the  line  to  be  measured,  if  there  do  not  appear  some  murks 
naturally  in  that  direction,  they  measure  straight  towards  it, 
4he  leader  fixing  down  an  arrow  at  the  end  of  every  chain, 
which  the  follower  always  takes  up,  as  he  comes  at  it,  till 
all  the  ten  arrows  are  used.  'They  are  then  all  returned  to 
the  leader,  to  use  over  again.  And  thus  the  arrows  are 
changed  from  the  one  to  the  other  at  every  10  chains  length, 
till  the  whole  line  is  finished  ;  then  the  number  of  changes 
of  the  arrows  shows  the  number  of  tens,  to  which  the  fol. 
lower  adds  the  arrows  he  holds  in  his  hand,  and  the  number 
of  links  of  another  chain  over  to  the  mark  or  end  of  the 
line.  So,  if  there  have  been  3  changes  of  the  arrows,  and 
the  follower  hold  6  arrows,  and  the  end  of  the  line  cut  off 
45  links  more,  the  whole  length  of  the  line  is  set  down  in 
links  thus,  3645. 

When  the  ground  is  not  level,  but  either  ascending  or  de- 
scending ;  at  every  chain  length,  lay  the  offset-staff,  or  link- 
staff,  down  in  the  slope  of  the  chain,  on  which  lay  the  small 
pocket  level,  to  show  now  many  links  or  parts  the  slope  line 
is  longer  than  the  true  level  one  ;  then  draw  the  chain  for- 
ward so  many  links  or  parts,  which  reduces  the  line  to  the 
horizontal  direction. 


problem  n. 
To  lake  Angles  and  Bearings. 

Let  b  and  c  be  two  objects,  or  two 
pickets  set  up  perpendicular ;  and  let 
it  be  required  to  take  their  bearings, 
or  the  angles  formed  between  them 
at  any  station  a. 


1.  With  the  Pimm  Table. 


The  table  being  covered  with  *  paper,  and  fixed  on  "ts 
ataod  ;  plant  it  at  the  station  a,  and  fix  a  fine  pin,  or  a  foot 
of  the  compasses,  in  a  proper  point  of  the  paper,  to  repre- 
sent the  place  a  ;  Close  by  ihe  side  of  this  pin  lay  the  fiducial 
edge  of  the  index,  and  turn  it  about,  still  touching  the  pin, 
till  one  object  b  can  be  seen  through  the  sights :  then  by  the 
fiducial  edge  of  the  index  draw  a  lute.  In  the  same  manner 
draw  another  line  in  the  direction  of  the  other  object  o» 
And  it  is  done. 

2.  With  the  Theodolite,  4*c 

Direct  the  fixed  sights  along  one  of  tho  lines,  as  ab,  by 
turning  the  instrument  about  till  the  mark  b  is  seen  through 
these  sights ;  and  there  screw  the  instrument  fast.  Then 
turn  the  moveable  index  round,  till  through  its  sights  the 
other  mark  c  is  seen.  Then  the  degrees  cut  by  the  index, 
on  the  graduated  limb  or  ring  of  the  instrument,  show  the 
quantity  of  the  angle. 

3.  With  the  Magnetic  Needle  and  Compass. 

Turn  the  instrument  or  compass  so,  that  the  north  end 
of  the  needle  point  to  the  flower-de-luce.  Then  direct  the 
sights  to  one  mark  ns  b,  and  note  the  degrees  cut  by  the 
needle.  Next  direct  the.  sights  to  the  other  mark  c,  and 
note  ngnin  the  degrees  cut  by  the  needle.  Then  their  sum 
or  difference,  as  the  case  may  be,  will  give  the  quantity  of 
the  angle  bac. 

4.  By  Measurement  with  the  Chain,  <fc. 

Measure  one  chain  length,  or  any  other  length,  along 
both  directions,  as  to  b  and  c.  Then  measure  the  distance 
6c,  and  it  is  done.— This  is  easily  transferred  to  paper,  by 
making  a  triangle  Abe  with  these  three  lengths,  and  then 
measuring  the  angle  a. 


0UBV12T1XO. 


417 


pboblbh  in. 


To  survey  a  Triangular  Field  abc. 
1.  By  the  Chain. 


ap  794 

AB  1321 

fc  826 


C 


Having  set  up  marks  at  the  come  ,  which  is  to  be  done 
in  all  cases  where  there  are  not  marks  naturally ;  measure 
with  the  chain  from  a  to  p,  where  a  perpendicular  would 
fall  from  the  angle  c,  and  set  up  a  mark  at  p,  noting  down 
the  distance  a  p.  Then  complete  the  distance  ab,  by  mea- 
suring from  p  to  b.  Having  set  down  this  measure,  return 
to  p,  and  measure  the  perpendicular  pc.  And  thus,  having 
the  base  and  perpendicular,  the  area  from  them  is  easily 
found.  Or  having  the  place  r  of  the  perpendicular,  the 
triangle  is  easily  constructed. 

Or,  measure  all  the  three  sides  with  the  chain,  and  note 
them  down.  From  which  the  content  is  easily  found,  or  the 
figure  is  constructed. 


Measure  two  sides  ab,  ac,  and  the  angle  a  between  them. 
Or  measure  one  side  ab,  and  the  two  adjacent  angles  a  and 
b.  From  either  of  these  ways  the  figure  is  easily  planned  ; 
then  by  measuring  the  perpendicular  cp  on  the  plan,  and 
multiplying  it  by  half  ab,  the  content  is  found. 

problem  IV. 

To  Measure  a  Four-sided  Field. 
1.  By  the  Chuin. 


Measure  along  one  of  the  diagonals,  as  ao  ;  and  eitfce 
the  two  perpendiculars  be,  bf,  as  in  the  last  prohWA  * 


2.  By  taking  some  of  the  Angles. 


4*8 


LAHP 


else  the  tides  ab,  bo,  cd,  da.  From  either  of  which  the 
figure  may  be  planned  and  computed  as  before  directed* 

Otherwise,  h  C\aU. 

Measure,  on  the  longest  side,  the  distances  at,  aq,  ab  ;  and 
the  perpendiculars  rc,  <u>. 

2.  J9y  tatoig  mne  ©ffAe  itagfat. 


ap  110  I  852  rc 
aq  745   505  qd 

AB  1110  I 


Measure  the  diagonal  ac  (see  the  last  fig.  but  one),  and 
the  angles  cab,  cad,  acb,  acd. — Or  measure  the  four  sides, 
and  any  one  of  the  angles,  as  bad. 


Thus. 
ac  501 
cab  37°  W 

CAD  41  15 

ub  72  25 
acd  54  40 


Or  thus. 
ab  486 
bc  304 
cd  410 
da  462 
bad  78"  35'. 


PROBLEM.  V, 


To  survey  any  Field  by  the  Chain  only. 

Having  set  up  marks  at  the  corners,  where  necessary,  of 
the  proposed  field  abcdefg,  walk  over  the  ground,  and  con* 
aider  how  it  can  best  be  divided  into  triangles  and  trapeziums ; 
and  measure  them  separately,  ns  in  the  last  two  problems. 
Thus,  the  following  figure  is  divided  into  the  two  trapeziums 
abco,  gdef,  and  the  triangle  ocn.  Then,  in  the  first  tra- 
pezium, beginning  at  a,  measure  the  diagonal  ac,  and  the 
two  perpendiculars  cm,  iro.  Then  the  base  gc  and  the 
perpendicular  vq.  Lastly,  the  diagonal  df,  and  the  two 
perpendiculars  pE,  og.  All  wbich  measures  write  against 
the  corresponding  parts  of  a  rough  figure  drawn  to  resemble 
the  figure  surveyed,  or  set  them  down  in  any  other  form  you 
choose. 


«0 


Thus. 


Am 

135 

130 

mo 

Aft 

410 

180 

TIB 

AC 

550 

cq 

152 

230 

q» 

CG 

440 

FO 

237 

120 

oo 

FP 

288 

80 

FD 

520 

Or  thus. 

Measure  all  the  sides  ab,  bc,  cd,  dk,  ef,  fg,  ga  ;  and  the 
diagonals  ac,  cg,  gd,  df. 

Otherwise. 

Many  pieces  of  land  may  be  very  well  surveyed,  by  mea- 
suring any  base  line,  either  within  or  without  them,  with  the 
perpendiculars  let  fall  on  it  from  every  corner.  For  they 
are  by  those  means  divided  into  several  triangles  and  trape- 
zoids,  all  whose  parallel  sides  are  perpendicular  to  the  base 
line ;  and  the  sum  of  these  triangles  and  trapeziums  will  be 
equal  to  the  figure  proposed  if  the  base  line  fall  within  it ;  if 
not,  the  sum  of  the  parts  which  are  without  being  taken  from 
the  sum  of  the  whole  which  are  both  within  and  without,  will 
leave  the  area  of  the  figure  proposed. 

In  pieces  that  are  not  very  large,  it  will  be  sufficiently 
exact  to  find  the  points,  in  the  base  line,  where  the  several 
perpendiculars  will  fall,  by  means  of  the  crass,  or  even  by 
judging  by  the  eye  only,  and  from  thence  measuring  to  the 
corners  for  the  lengths  of  the  perpendiculars. — And  it  will  be 
most  convenient  to  draw  the  line  so  as  that  all  the  perpen- 
diculars may  fall  within  the  figure. 

Thus,  in  the  following  figure,  beginning  at  a,  and  mea- 
suring along  the  line  ao,  the  distances  and  perpendiculars  on 
the  right  and  left  are  as  below. 


Ab 
AC 

xd 

AC 

A/ 
AO 


315 
440 
585 
610 
990 
1020 


350  6b 
70  cc 

320  dv 
50 

470 /f 
0 


4t» 


LA*B 


PBOBUm  TI. 


To 


ike  Of***. 


jjtitiwm  being  a  crooked  hedge,  or  brook,  dec.  Front 
a  measure  in  a  straight  direction  along  the  side  of  it  to  b. 
And  in  measuring  along  this  line  ab,  observe  when  you  m 
directly  opposite  any  bends  or  corners  of  the  boundary,  as  si 
c,  4,  e,  ic.;  and  from  these  measure  the  perpendicular 
offsets  dfc,  di,  fcc.  with  the  ofiset.staff,  if  they  are  not  very 
large,  otherwise  ,  with  the  chain  itself ;  and  the  work  is  done* 
'fhe  register,  or  field-book,  may  be  as  follows : 


Oft.  left. 

Baaa  line  am 

0 

0 

A 

c* 

62 

45 

AC 

di 

84 

220 

Ad 

ek 

70 

840 

Kt 

fl 

96 

510 

*f 

gm 

57 

034 

*g 

m 

91 

785 

AB 

Ac   d  e    J    9  3 


FROBLEV  VH. 

To  survey  any  PieUjeUh  the  Plain  Table. 
1.  Prom  one  Station. 


PtAirr  the  table  at  any  angle  as 
c,  from  which  all  the  other  angles, 
or  marks  set  up,  can  be  seen  ;  turn 
the  table  about  till  the  needle  point 
to  the  flower-de-luce ;  and  there 
screw  it  fast.  Make  a  point  for  c 
on  the  paper  on  the  table,  and  lay 

the  edge  of  the  index  to  c,  turning   

it  about  c  till  through  the  sights  '  A.  JB 
you  see  the  mark  d  :  and  by  the  edge  of  the  index  draw  a 
dry  or  obscure  line :  then  measure  the  distance  cd,  and  lsy 
that  distance  down  on  the  line  cd.  Then  turn  the  index 
about  the  point  c,  till  the  mark  £  be  seen  through  the  sights, 
by  which  draw  a  line  and  measure  the  distance  to  b,  layiag 
it  on  the  line  from  c  to  s.  In  like  manner  determine  the 
positions  of  ca  and  cb,  V*y  \wnxva£the  sights  auccossircly  to 


•UEVEYIXG. 


441 


a  and  b  ;  and  lay  the  length  of  those  lines  down.  Then 
connect  the  points,  hy  drawing  the  black  lines  cd,  de,  ka, 
ab,  bo,  for  the  boundaries  of  the  field. 

From  a  Station  within  the  Field. 


When  all  the  other  parts  cannot 
be  seen  from  one  angle,  choose  some 
place  O  within,  or  even  without,  if  v 
more  convenient,  from  which  the  other 
part 8  can  be  seen.    Plant  the  table 
at  O,  then  fix  it  with  the  needle 
north,  and  mark  the  point  O  on  it. 
Apply  the  index  successively  to  (), 
turning  it  round  with  the  sights  to 
each  angle,  a,  b,  c,  d,  e,  drawing  dry  lines  to  them  hy  the 
edge  of  the  index  ;  then  measuring  the  distances  oa,  or, 
and  laying  them  down  on  those  lines.    Lastly,  draw  the 
boundaries  ab,  bc,  cd,  de,  ea. 

3.  By  going  round  the  Figure. 

When  the  figure  is  a  wood,  or  water,  or  wlien  from  some 
other  obstruction  you  cannot  measure  lines  across  it ;  begin 
at  any  point  a,  and  measure  around  it,  either  within  or 
without  the  figure,  and  draw  the  directions  of  all  the  sides, 
thus:  Plant  the  table  at  a  ;  turn  it  with  the  needle  to  the 
north  or  flower-de-luce  ;  fix  it,  and  mark  the  point  a.  Apply 
the  index  to  a,  turning  it  till  you  can  see  the  point  k,  and 
there  draw  a  line  :  then  the  point  b,  and  there  draw  a  line  : 
then  measure  these  lines,  and  lay  them  down  from  a  to  Kund 
b.  Next  move  the  table  to  b,  lay  the  index  along  the  line 
ab,  and  turn  the  table  about  till  you  can  see  the  mark  a,  and 
screw  fast  the  table ;  in  which  position  also  the  needle  will 
again  point  to  the  flower-de-luce,  as  it  will  do  indeed  at  every 
station  when  the  table  is  in  the  right  position.  Here  turn 
the  index  about  b  till  through  the  sights  you  seek  the  mark  c ; 
there  draw  a  line,  measure  bc,  and  lay  the  distance  on  that 
line  after  you  have  set  down  the  table  at  c.  Turn  it  then 
again  into  its  proper  position,  and  in  like  manner  find  the 
next  line  cd.  And  so  on  quite  around  by  e,  to  a  again. 
Then  the  proof  of  the  work  will  be  the  joining  at  a  :  for  if 
the  work  be  all  right,  the  last  direction  ka  on  the  ground, 
will  pass  exactly  through  the  point  a  on  the  paper ;  and  the 
measured  distance  will  also  reach  exactly  to  a.  If  these  do 
not  coincide,  or  nearly  so,  some  error  has  been  committed, 
and  the  work  must  be  examined  over  again. 

Vol.  I.  57 


442 


LAND 


PllOBLEX  VIII. 

To  surrey  a  Field  xci'h  the  Theodolite,  «fc. 

I.  From  One  Point  or  Station* 

When  all  the  angles  can  be  seen  from  one  point,  as  the 
angle  c  first  fig.  to  lust  prob.),  place  the  instrument  at  c,  and 
turn  it  about,  till  through  the  fixed  sights  you  see  the  mark 
a,  and  there  fix  it.  Then  turn  the  moveable  index  about 
till  the  mark  a  be  seen  through  the  sights,  and  note  the  de- 
grees cut  on  the  instrument.  Next  turn  the  index  suc- 
cessively to  k  and  n,  noting  the  degrees  cut  off*  at  each ;  which 
gives  all  the  angles  h<;a,  bck,  bod.  Lastly,  measure  the 
lines  cb,  ca,  ce,  cd  ;  and  enter  the  measures  in  a  field-book, 
or  rather,  against  the  corresponding  parts  of  a  rough  figure 
drawn  by  guess  to  resemble  the  field. 

2.  From  a  Point  within  or  without. 

Plant  the  instrument  at  o  (last  fig.),  and  turn  it  about  till 
the  fixed  sights  point  to  any  object,  as  a  ;  and  there  screw  it 
fast.  Then  turn  the  moveable  index  round  till  the  sights 
point  successively  to  the  other  points  n,  c,  b,  no'ing  the 
degrees  cut  off  at  each  of  them  ;  which  gives  all  the  angles 
round  the  point  o.  Lastly,  measure  the  distances  oa,  ob,  oc, 
od,  oe,  noting  them  down  as  before,  and  the  work  is  done. 

3.  By  going  round  the  Field. 

By  measuring  round,  either  %  EL-- 
within  or  without  the  field,  pro. 
ceed  thus.  Having  set  up  marks 
at  b,  u,  &c.  near  the  corners  as 
usual,  plant  the  instrument  at 
any  point  a,  and  turn  it  till  the 
fixed  index  be  in  the  direction 
ab,  and  there  screw  it  fast  :  then 
turn  the  moveable  index  to  the  / 
direction  ac  ;  and  the  degrees  cut  off  will  be  the  angle  a. 
Measure  the  line  ab,  and  plant  the  instrument  at  b,  and! 
there  in  the  same  manner  observe  the  angle  a.  Then  mea- 
sure bc,  and  observe  the  angle  c.  Then  measure  the  dis- 
tance cd,  and  take  the  angle  d.  Then  measure  de,  and 
take  the  angle  e.  Then  measure  ef,  and  tak^  the  angle  r. 
And  lastly,  measure  the  distance  fa. 

To  prove  the  work  ;  add  all  the  inward  angles,  a,  b,  c, 
Ac.  together ;  for  when  the  work  is  right,  their  sum  will  be 
equal  to  twice  as  many  right  angles  as  the  figure  has  sides, 


SUtVIYJNG. 


443 


wanting  4  right  angles.    But  when  there  is  an  angle,  as  f, 
that  bends  inwards,  and  you  measure  the  external  angle, 
which  is  less  than  two  right  angles,  subtract  it  from  4  right 
angles,  or  360  degrees,  to  give  the  internal  angle  greater  than    ■  sfc-; 
a  semicircle  or  180  degrees. 

Otherwise.  < 

Instead  of  observing  the  internal  angles,  we  may  take  the 
external  angles,  formed  without  the  figure  by  procuring  the 
sides  farther  out.  And  in  this  case,  when  the  work  is  right, 
their  sum  altogether  will  be  equal  to  360  degrees.  But  when 
one  of  them,  as  f,  runs  inwards,  subtract  it  from  the  sum  of 
the  rest,  to  leave  360  degrees. 

problem  rx. 

To  survey  a  Field  with  crooked  Hedges,  4*c. 

With  any  of  the  instruments,  measure  the  lengths  and 
positions  of  imaginary  lines  running  as  near  the  sides  of  the 
field  as  you  can  ;  and.  in  going  along  them,  men  sure  the 
offsets  in  the  manner  before  taught ;  then  you  will  have  the 
plan  on  the  paper  in  using  the  plain  table,  drawing  the 
crooked  hedges  through  the  ends  of  the  offsets  ;  but  in  sur- 
veying with  the  theodolite,  or  other  instrument,  set  down 
the  measures  properly  in  a  field-book,  or  memorandum* 
book,  and  plan  them  after  returning  from  the  field,  by  lay. 
ing  down  all  the  lines  and  angles. 


So  in  surveying  the  piece  arcde,  set  up  marks,  a,  b.  r,  #2, 
dividing  it  so  as  to  have  as  few  sides  as  may  be.  Then  begin 
at  any  station,  a,  and  measure  the  lines  a//,  6c,  cd,  d>i>  taking 
their  positions,  or  the  angles,  a,  6,  c,  d  ;  and,  in  going  along 
the  lines,  measure  all  the  offsets,  as  at  m,  n,  o,  p,  &c.  along 
every  station. line. 

And  this  is  done  either  within  the  field,  or  without,  as 
may  be  most  convenient.   When  there  wc*  oV^rt^Mrai 


LAUD 


within,  as  wood,  water,  hills,  ozc.  then  measure  without,  t» 
in  the  next  following  figure. 


problem  x. 

7b  Survey  a  Field,  or  any  other  Thing,  by  ttco  Stations. 

This  is  performed  by  choosing  two  stations  from  which 
all  the  marks  and  objects  can  be  seen  ;  then  measuring  the 
distance  between  the  stations,  and  at  each  station,  taking 
the  angles  formed  by  every  object  fr<  m  the  station  line  or 
distance. 

The  two  stations  may  be  taken  either  within  the  hounds, 
or  in  one  of  the  sides,  or  in  the  direction  of  two  of  the  ob- 
jects, or  quite  at  a  distance  and  without  the  bounds  of  the 
objects  or  part  to  be  surveyed. 

In  this  manner,  not  only  grounds  may  be  surveyed,  with- 
out even  entering  them,  but  a  map  may  be  taken  of  t'.ie 
principal  parts  of  a  county,  or  the  chief  places  nf  a  town, 
or  any  part  of  a  river  or  coast  surveyed,  or  any  other  inac- 
cessible objects ;  by  taking  two  stations,  on  two  towers,  or 
two  hills,  or  such-like. 

B 


8T7HVEY1JG. 


445 


PRO B LEX  XI. 

To  survey  a  large  Estate. 

If  the  estate  be  very  large,  and  contain  a  great  number  of 
field*,  it  cannot  welt  be  done  by  surveying  all  the  fields 
singly,  and  then  putting  them  together ;  nor  can  it  be  done 
by  taking  all  the  angles  and  boundaries  that  enclose  it.  For 
in  these  cases,  any  small  errors  will  be  so  much  increased,  as 
to  render  it  very  much  distorted.    But  proceed  a*  below. 

1.  W  ilk  over  the  estate  two  or  three  times,  in  order  to 
get  a  perfect  idea  of  it,  or  till  you  can  keep  the  figure  of  it 
pretty  we  I  in  mind.  And  to  help  your  memory,  draw  an 
eye-draught  of  it  on  paper,  at  least  of  the  principal  parts 
of  it,  to  guide  you ;  setting  the  names  within  the  fields  in 
that  draught. 

2.  Choose  two  or  more  eminent  places  in  the  estate,  for 
station?*,  from  which  all  the  princip.il  parts  of  it  can  be  seen  : 
selecting  th'  se  stations  as  far  distant  from  one  another  as 
convenient. 

3.  Take  such  nng'es,  between  the  station*,  as  you  think 
necessary,  and  measure  the  distances  from  station  to  station, 
always  in  a  ri^ht  line  :  these  things  must  be  done,  till  you 
get  an  many  angles  and  lines  as  are  sufficient  for  determining 
all  the  points  of  station.  And  in  measuring  any  of  these 
station  distance*,  mark  accurately  where  these  lines  meet 
with  any  hedges,  ditches,  roads,  lanes,  paths,  rivulets,  dec.  ; 
and  where  any  remarkable  object  is  placed,  by  measuring 
its  distance  from  the  station- line  ;  and  where  a  perpendicular 
from  it  cuts  that  line.  And  thus  as  you  go  along  unv  mnin 
station. line,  take  offsets  to  the  ends  of  all  hedges,  am/ to  any 
pond,  house,  mill,  bridge,  6zc.  noting  every  thing  down  that 
is  remarkable. 

4  As  to  the  inner  parts  of  the  estate,  they  must  be  deter- 
mined, in  like  manner,  by  new  station  lines  ;  for,  after  the 
main  stations  are  determined,  and  every  thing  adjoining  to 
them,  then  the  estate  must  be  subdivided  into  two  or  three 
parts  by  new  station  lines  ;  taking  inner  stations  at  proper 
places,  where  you  can  have  the  best  view.  Measure  these 
Stat  ion- lines  as  you  d  d  tl  e  first,  and  all  their  intersections 
with  hedges,  and  offsets  to  such  objects  as  appear.  Then 
proceed  to  survey  the  adjoining  fields,  by  taking  the  angles 
that  the  sides  make  with  the  station. 'ine,  at  the  intersections, 
and  measuring  the  distances  to  each  corner,  from  the  inter, 
sections.  For  the  station. lines  will  be  the  bases  to  \\W  \V» 
future  operations ;  the  situation  of  aft  pun*  Ym&%  «D&t*Vi 


448 


LAKD 


dependent  on  them  ;  nnd  therefore  they  should  be  taken  of 
as  great  length  a*  possible  ;  and  it  is  best  for  them  to  run 
along  Home  of  the  hedges  or  boundaries  of  one  or  more  fields, 
or  to  pass  through  some  of  their  angles.  All  things  being 
determined  fur  these  stations,  you  must  take  more  inner 
stations,  and  continue  to  divide  and  subdivide  till  at  last  you 
come  to  single  fields  :  repeating  the  same  work  for  the  inner 
stations  as  for  the  outer  ones,  till  all  is  done  ;  and  close  the 
work  as  often  as  you  can,  and  in  as  few  lines  as  possible. 

5.  An  estate  nmy  be  so  situated  that  the  whole  cannot  be 
surveyed  together  ;  because  one  part  of  the  estate  cannot  be 
seen  from  another.  In  this  case,  you  may  divido  it  into 
three  or  four  parts,  and  survey  the  parts  separately,  as  if 
they  were  lands  belonging  to  different  persons  ;  and  at  last 
join  them  together. 

6.  As  it  is  necessary  to  protract  or  lay  down  the  work  as 
you  proceed  in  it,  you  must  have  a  scale  of  a  due  length  to 
do  it  by.  To  get  such  n  scale,  measure  the  whole  length  of 
the  estate  in  chains  ;  then  consider  how  many  inches  long 
the  map  is  to  he  ;  and  from  these  will  be  known  how  many 
chains  you  must  have  in  an  inch  ;  then  make  the  scale  ac- 
cordingly, or  choose  one  already  made. 


PROBLEM  XII. 

To  survey  a  County,  or  large  Trad  of  Land. 

1.  Choosk  two,  three,  or  four  eminent  places,  for  stations; 
such  as  the  tops  of  high  hills  or  mountains,  towers,  or  church 
steeples,  which  may  he  seen  from  one  another  ;  from  which 
most  of  the  towns  and  other  places  of  note  may  also  be  seen  ; 
and  so  as  to  be  as  far  dis  ant  from  one  another  as  possible. 
On  these  places  raise  beacons,  or  long  poles,  with  flags  of 
different  colours  flying  at  them,  so  as  to  be  visible  from  all 
the  other  stations. 

2.  At  all  the  places  which  you  would  set  down  in  the  map, 
plant  long  poles,  with  Hags  at  them  of  several  colours,  to 
distinguish  the  places  from  one  another  ;  fixing  them  on  the 
tops  of  church  steeples,  or  the  tops  of  houses  ;  or  in  the 
centres  of  smaller  towns  and  villages. 

These  marks  then  being  set  up  at  a  convenient  number  of 
places,  and  such  as  may  be  seen  from  both  stations  ;  go  to 
one  of  these  stations,  and,  with  an  instrument  to  take  angles, 
standing  at  that  station,  take  ail  the  angles  between  the  other 
station  nnd  each  of  these  marks.  Then  go  to  the  other 
station,  and  take  all  the  angles  between  the  first  station  and 


SURVEY:*©. 


447 


each  of  the  former  marks,  setting  them  down  with  the 
others,  each  against  its  fellow  with  the  same  colour.  You 
may,  if  convenient,  also  take  the  angles  at  some  third  station, 
which  may  serve  to  prove  the  work,  if  the  three  lines  inter* 
sect  in  that  point  where  any  mark  stands.  The  marks  must 
stand  till  the  observations  are  finished  al  both  stations  ;  and 
then  they  may  be  taken  down,  and  set  up  at  new  places. 
The  same  operations  must  be  performed  at  both  stations,  for 
these  new  places  ;  and  the  like  for  others.  The  instrument 
for  taking  angles  must  ba  an  exceeding  good  one,  made  on 
purpose  with  telescopic  sights,  and  of  a  good  length  of  ra- 
dius. 

3.  And  though  it  be  not  absolutely  necessary  to  measure 
any  distance,  because,  a  stationary  line  being  laid  down  from 
any  scale,  all  the  other  lines  will  be  proportional  to  it ;  yet 
it  is  better  to  measure  some  of  the  lines,  to  ascertain  the 

'  distances  of  places  in  miles,  and  to  know  how  many  geome- 
trical miles  there  are  in  any  length  ;  as  also  from  thence  to 
make  a  scale  to  measure  any  distance  in  miles.  In  measuring 
any  distance,  it  will  not  be  exact  enough  to  go  along  the 
high  roads  ;  which,  by  reason  of  their  turnings  and  windings, 
hardly  ever  lie  in  a  right  line  between  the  stations  ;  which 
must  cause  endless  reductions,  and  require  great  trouble  to 
make  it  a  right  line ;  for  which  reason  it  can  never  be  exact. 
But  a  better  way  is  to  measure  in  a  straight  line  with  a  chain, 
between  station  and  station,  over  hills  and  dales,  or  level 
fields  and  all  obstacles.  Only  in  case  of  water,  woods, 
towns,  rocks,  banks,  <kc.  where  we  cannot  pass,  such  parts 
of  the  line  must  be  measured  by  the  methods  of  inaccessible 
distances  ;  and  besides,  allowing  for  ascents  and  descents, 
when  they  are  met  with.  A  good  compass,  that  shows  the 
bearing  of  the  two  stations,  will  always  direct  us  to. go 
straight,  when  the  two  stations  cannot  be  seen  ;  and  in  the 
progress,  if  we  can  go  straight,  offsets  may  be  taken  to  any 
remarkable  places,  likewise  noting  the  intersection  of  the 
station. line  with  all  roads,  rivers,  dtc. 

4.  From  all  the  stations,  and  in  the  whole  progress,  we 
must  be  very  particular  in  observing  sea-coasts,  river-mouths, 
towns,  castles,  houses,  churches,  mills,  trees,  nicks,  sands, 
roads,  bridges,  fords,  ferries,  woods,  hills,  mountains,  rills, 
brooks,  parks,  beacons,  sluices,  floodgates,  locks,  &c,  and  in 
general  every  thing  that  is  remarkable. 

5.  After  we  have  done  with  the  first  and  main  station* 
lines,  wbich  command  the  whole  county  :  we  must  then 
take  inner  stations,  at  some  places  already  determined  ;  which 
will  divide  the  whole  into  several  partitions  :  and  from  these 
•tations  we  must  determine  the  places  of  as  traiw)  ^ga 


land 


remaining  towns  as  we  can.  And  if  any  remain  in  that 
party  we  must  take  nnre  stations,  at  Home  places  already 
determined  ;  from  which  we  may  determine  the  rent.  And 
thus  go  through  all  the  parts  of  *lho  county,  taking  atalkm 
after  station,  till  we  have  determined  the  whole.  And  in 
general  the  station  distances  must  always  pass  through  such 
remarkable  points  as  have  been  determined  before,  by  the 
former  stations. 


rKOBLEM  XIII. 

To  survey  a  Town  or  City. 

This  may  be  done  with  any  of  the  instruments  for  taking  ^ 
angles,  but  best  of  all  with  the  plain  table,  where  every 
minute  part  is  drawn  while  in  sight.  Instead  of  the  common 
surveying  or  Gunter's  chain,  it  will  he  best,  for  this  purpose, 
to  have  a  chain  50  feet  long,  divided  into  50  links  of  one 
foot  each,  and  an  offset- staff  «;f  10  feet  long. 

Begin  at  the  meeting  of  two  or  more  of  the  principal 
streets,  through  which  you  enn  have  the  longest  prospect?, 
to  get  the  longest  station  lines :  there  having  fixed  the  in* 
strument,  draw  lines  jf  direction  along  those  streets,  using 
two  men  as  marks,  or  poles  set  in  wooden  pedestals,  or  per- 
haps some  remarkable  places  in  the  houses  at  the  fan  her 
ends,  as  windows,  doors,  corners,  dtc.  Measure  those  lines 
with  the  chain,  taking  onsets  with  the  staff,  at  all  corners  of 
streets,  bendings,  or  windings,  and  to  all  remurkable  thing*, 
as  churches,  markets,  halls,  colleges,  eminent  houses,  &c. 
Then  remove  the  instrument  to  another  station,  nlon"r  one  of 
these  lines  ;  and  there  repeat  (he  same  process  as  before. 
And  so  on  till  the  whole  is  finished. 


SURVEYING* 


449 


Thus,  fix  the  instrument  at  a,  and  draw  lines  in  the 
direction  of  all  the  streets  meeting  there  ;  then  measure  ab, 
noting  the  street  on  the  left  at  m.  At  the  second  station  b, 
draw  the  directions  of  the  streets  meeting  there  ;  and  mea- 
sure from  b  to  c,  noting  the  places  of  the  streets  at  n  and  o 
as  you  pass  by  them.  At  the  third  station  cy  take  the  di- 
rection of  all  the  streets  meeting  there,  and  measure  cd.  At 
d  do  the  same,  and  measure  de,  noting  the  place  of  the 
cross  streets  at  p.  And  in  this  manner  go  through  all  the 
principal  streets.  This  clone,  proceed  to  the  smaller  and 
intermediate  streets ;  and  lastly  to  the  lanes,  alleys,  courts, 
yards,  and  every  part  that  it  may  be  thought  proper  to  re- 
present in  the  plan. 

THEOREM  XIV. 

To  lay  down  the  Plan  of  any  Survey. 

Ir  the  survey  was  taken  with  the  plain  table,  we  have  a 
rough  plan  of  it  already  on  the  paper  which  covered  the 
table.  But  if  the  survey  was  with  any  other  instrument,  a 
plan  of  it  is  to  be  drawn  from  the  measures  that  were  taken 
in  the  survey  ;  and  first  of  all  a  rough  plan  on  paper. 

To  do  this,  you  must  have  a  net  of  proper  instruments, 
for  laying  down  both  lines  and  angles,  &c.  ;  as  scales  of  va- 
rious sizes,  the  more  of  them,  and  the  more  accurate,  the 
better,  scales  of  chords,  protractors,  perpendicular  and  pa- 
rallel rulers,  <kc.  Diagonal  scales  are  best  for  the  lines, 
because  they  extend  to  three  figures,  or  chains,  and  links, 
which  are  100  parts  of  chains.  But  in  using  the  diagonal 
scale,  a  pair  of  compasses  must  be  employed,  to  take  on  the 
lengths  of  t!io  principal  lines  very  accurately.  But  a  scale 
with  a  thin  edge  divided,  is  much  readier  for  laying  down 
the  perpendicular  offsets  to  crooked  hedges,  and  for  marking 
the  places  of  those  offsets  on  the  station- line  ;  which  is  done 
at  only  one  application  of  the  cd«;e  the  scale  to  that  line, 
and  then  pricking  off  all  at  once  the  distances  along  it. 
Angles  are  to  be  laid  down,  either  with  a  good  scale  of 
chords,  which  is  perhaps  the  most  accurate  way,  or  with  a 
large  protractor,  which  is  much  readier  when  many  angles 
are  to  be  laid  down  at  one  point,  as  they  arc  pricked  off  all 
at  once  round  the  edge  of  the  protractor. 

In  general,  all  ILies  and  angles  must  be  laid  down  on  the 
plan  ii>  the  same  order  in  which  they  were  measured  in  the 
field,  and  in  which  they  are  written  in  the  field-book  ;  lay- 
ing down  first  the  angles  for  the  position  of  \vma,  wraX. 

Vol.  I.  58 


LAJCD 


lengths  of  the  lines,  with  the  places  of  the  offsets,  and  then 
the  lengths  of  the  offsets  themselve*,  all  with  dry  or  obscure 
lines;  then  a  black  line  drawn  through  the  extremities  of 
nil  the  offset*,  will  be  the  edge  or  bounding  line  of  the  field, 
ccc.  After  the  principal  bounds  and  lines  are  laid  down, 
and  made  to  fit  or  close  properly,  proceed  next  to  the  smaller 
objects,  till  you  have  entered  every  thing  that  ought  to  ap- 
pear in  the  plan,  as  houses,  brooks,  trees,  hills,  gates,  stiles, 
roads,  lanes,  mill*,  bridges,  woodlands,  Ac.  dec. 

The  north  side  of  a  map  or  plan  is  commonly  placed 
uppermost,  and  a  meridian  is  somewhere  drawn,  with  the 
compass  or  flower-de-luce  pointing  north.  Also,  in  a  vacant 
part,  a  scale  of  equal  parts  or  chains  is  drawn,  with  the  title 
of  the  map  in  conspicuous  characters,  and  embellished  with 
a  compartment.  Hills  are  shadowed,  to  distinguish  them  in 
the  map.  Colour  the  hedges  with  different  colours  ;  repre- 
sent hilly  grounds  by  broken  hills  and  valleys  ;  draw  single 
dotted  lines  for  foot-paths,  and  double  ones  for  horse  or  car- 
riage roads.  Write  the  name  of  each  field  and  remarkable 
place  within  it,  and,  if  you  choose,  its  contents  in  acres, 
roods,  and  perches. 

In  a  very  large  estate,  or  a  county,  draw  vertical  and  ho- 
rizontal lines  through  the  map,  denoting  the  spaces  between 
them  by  letters  placed  at  the  top,  and  bottom,  and  sides,  for 
readily  finding  any  field  or  other  object  mentioned  in  a 
table. 

In  mapping  counties,  and  estates  that  have  uneven  grounds 
of  hills  and  valleys,  reduce  all  oblique  lines,  measured  up* 
hill  and  down. hill,  to  horizontal  straight  lines,  if  that  was 
not  done  during  the  survey,  before  they  were  entered  in  the 
field-book,  by  making  a  proper  allowance  to  shorten  them. 
For  which  purpose  there  is  commonly  a  small  table  engraven 
on  some  of  the  instruments  for  surveying. 

THE  NEW  METHOD  OF  SURVEYING. 

PROBLEM  XV. 

To  survey  and  plan  bp  the  new  Method. 

Is  the  former  method  of  measuring  a  large  estate,  theac 
curacy  of  it  depends  both  on  the  correctness  of  the  instru- 
ments, and  on  the  care  in  taking  the  angles.  To  avoid  the 
errors  incident  to  such  a  multitude  of  angles,  other  methods 
hu\c  of  late  years  been  used  by  some  few  skilful  surveyors  : 
the  most  practical,  expeditious,  and  correct,  seems  to  be  the 


SURVEYING. 


451 


following,  which  is  performed,  without  taking  angles,  by 
measuring  with  the  chain  only. 

Choose  two  or  more  eminences,  as  grand  stations,  and 
measure  a  principal  base  line  from  one  station  to  another  ; 
noting  every  hedge,  brook,  or  other  remarkable  object,  as  you 
pass  by  it ;  measuring  also  such  short  perpendicular  lines  to 
the  bends  of  hedges  as  may  be  near  at  hand.  From  the  ex- 
tremities of  this  base  line,  or  from  any  convenient  parts  of 
the  same,  go  off  with  other  lines  to  some  remarkable  object 
situated  towards  the  sides  of  the  estate,  without  regarding 
the  angles  they  make  with  the  base  line  or  with  one  another  ; 
still  remembering  to  note  every  hedge,  brook,  or  other  ob- 
ject, that  you  pass  by.  These  lines,  when  laid  down  by  in- 
tersections, will,  with  the  base  line,  form  n  grand  triangle  on 
the  estate ;  several  of  which,  if  need  he,  being  thus  mea- 
sured and  laid  down,  you  may  proceed  to  form  other  smaller 
triangles  and  trapezoids  on  the  sides  of  the  former  :  and  so 
on  till  you  finish  with  the  enclosures  individually.  By  which 
means  a  kind  of  skeleton  of  the  estate  may  first  be  obtained, 
and  the  chief  lines  serve  as  the  bases  of  such  triangles  and 
trapezoids  as  are  necessary  to  fill  up  all  the  interior  parts. 

The  field-book  is  ruled  into  three  columns,  ns  usual.  In 
the  middle  one  are  set  down  the  distances  on  the  chain. line, 
at  which  any  mark,  offset,  or  other  observation,  is  made  ; 
and  in  the  right  and  left  hand  columns  are  entered  the  off- 
sets  and  observations  made  on  the  right  and  left  hand  re- 
spectively of  the  chain-line  ;  sketching  on  the  sides  the  shape 
or  resemblance  of  the  fences  or  boundaries. 

It  is  of  groat  advantage,  both  for  brevity  and  perspicuity, 
to  begin  at  the  bottom  of  the  leaf,  and  write  upwards  ;  de- 
noting the  crossing  of  fences,  by  lines  drawn  across  the  mid. 
die  column,  or  only  a  part  of  such  a  line  on  the  right  and 
left  opposite  the  figures,  to  avoid  confusion  ;  and  the  corners 
of  fields,  and  other  remarkable  turns  in  the  fences  where  off- 
sets are  taken  to,  by  lines  joining  in  the  manner  the  fences 
do  ;  as  will  be  best  seen  by  comparing  the  book  with  the 
plan  annexed  to  the  field-book  following,  p.  454. 

The  letter  in  the  left-hand  corner  at  the  beginning  of  every 
line,  is  the  mark  or  place  measured  from;  and  that  at  the 
right-hand  corner  at  the  end,  is  the  mark  measured  to  :  but 
when  it  is  not  convenient  to  go  exactly  from  a  mark,  the 
place  measured  from  is  described  such  a  distance  from  one 
mark  towards  another ;  and  where  a  former  mark  is  not  mea- 
sured to,  the  exact  place  is  ascertained  by  saying,  turn  to  the 
right  or  left  hand,  such  a  distance  to  such  a  mark,  it  being 
always  understood  that  those  distances  are  tuken  in  the 
chain  line* 


4» 


LAND 


The  characters  used  are,  f  for  turn  to  the  right  handf 
}  for  turn  to  the  left  hand,  and  placed  over  an  offset, 
to  show  that  it  is  not  taken  at  right  angles  with  the  chain- 
line,  but  in  the  direction  of  some  straight  fence  ;  being 
chiefly  used  when  crossing  their  directions  ;  which  is  a  better 
way  of  obtaining  their  true  places  than  by  offsets  at  right 
angles. 

When  a  line  is  measured  whose  position  is  determined, 
either  by  former  work  (as  in  the  case  of  producing  a  given 
line,  or  measuring  from  one  known  place  or  mark  to  another) 
or  by  itself  (as  in  the  third  side  of  the  triangle),  it  is  called 
a  fast  line,  and  a  double  tine  across  the  book  is  drawn  at  the 
conclusion  of  it ;  but  if  its  position  is  not  determined  'as  in 
the  second  side  of  the  triangle),  it  is  called  a  loose  line,  and  a 
single  line  is  drawn  across  the  book.  When  a  line  becomes 
determined  in  position,  and  is  afterwards  continued  farther, 
a  double  line  half  through  the  hook  is  drawn. 

When  a  loose  line  is  measured,  it  becomes  absolutely  ne- 
cessary to  measure  some  other  line  that  will  determine  its 
position.  Thus,  the  first  line  ah  or  bh,  being  the  base  of  a 
triangle,  is  always  determined  ;  but  the  position  of  the  second 
side  hj  does  not  become  determined,  till  the  third  side  jb  is 
measured  ;  then  the  position  of  both  is  determined,  and  the 
triangle  may  be  constructed. 

At  the  beginning  of  a  line,  to  fix  a  loose  line  to  the  mark 
or  place  measured  from,  the  sign  of  turning  to  the  right  or 
left  hand  must  be  added,  as  at  h  in  the  second,  and  j  in  the 
third  line ;  otherwise  a  stranger,  when  laving  down  the 
work,  may  as  easily  construct  the  triangle  hjb  on  the  wrong 
side  of  the  lino  ah,  us  on  the  right  one  :  hut  this  error  can- 
not be  fallen  into,  if  the  sign  above  named  be  carefully  ob- 
served. 

In  choosing  a  line  to  fix  n  loose  one,  care  must  be  taken 
that  it  does  not  make  a  very  acute  or  obtuse  angle  ;  as  in  the 
^  triangle  pur,  by  the  an«rle  at  b  being  very  obtuse,  a  small 
deviation  from  truth,  even  the  breadth  of  a  point  at  p  or  r, 
would  make  the  error  at  b,  when  constructed,  very  consi. 
derable  ;  but  by  constructing  the  triangle  pnq,  such  a  devia. 
tion  is  of  no  consequence. 

Where  the  words  leave  off  are  written  in  the  field* book,  it 
signifies  that  the  taking  of  offsets  is  from  thence  discominu. 
ed  ;  and  of  course  something  is  wanting  between  that  and 
the  next  offset,  to  be  afterwards  determined  by  measuring 
some  other  line. 

The  field. book  for  this  method,  and  the  plan  drawn  from 
it,  arc  contained  in  the  four  following  pages,  engraven  on 
copper  plates ;  answerable  to  which  the  pupil  is  to  draw  a 


  -  - 

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■UBVJBVIXG* 


458 


plan  from  the  measures  in  the  field-book,  of  a  larger  size, 
viz.  to  a  scale  of  a  double  size  will  be  convenient,  such  a 
scale  being  also  found  on  most  instruments.  In  doing  this, 
begin  at  the  commencement  of  the  field-book,  or  bottom  of 
the  first  page,  and  draw  the  first  line  ah  in  any  direction  at 
pleasure,  and  then  the  next  two  sides  of  the  first  triangle  bhj 
by  sweeping  intersected  arcs ;  and  so  all  the  triangles  in 
the  same  manner,  after  each  other  in  their  order ;  and  after- 
wards setting  the  perpendicular  and  other  offsets  at  their 
proper  places,  and  through  the  ends  of  them  drawing  the 
bounding  fences. 

Note.  That  the  field-book  begins  at  the  bottom  of  the  first 
page,  and  reads  up  to  the  top ;  hence  it  goes  to  the  bottom 
of  the  next  page,  and  to  the  top  ;  and  thence  it  passes  from 
the  bottom  of  the  third  page  to  the  top,  which  is  the  end  of 
the  field-book.  The  several  marks  measured  to  or  from, 
are  here  denoted  by  the  letters  of  the  alphabet,  first  the  small 
ones,  a,  b,  c,  dy  &c,  and  after  them  the  capitals  A,  B,  C,  D9 
dec.  But  instead  of  these  letters,  some  surveyors  use  the 
numbers  in  order,  1,  2,  3,  4,  dtc. 

OF  THE  OLD  KIND  OF  FIELD-BOOK. 

In  surveying  with  the  plain  table,  a  field-book  is  not  used, 
as  every  thing  is  drawn  on  the  table  immediately  when  it  is 
measured.  But  in  surveying  with  the  theodolite,  or  any 
other  instrument,  some  kind  of  a  field  book  must  be  used  to 
write  down  in  it  a  register  or  account  of  all  that  is  done  and 
occurs  relative  to  the  survey  in  hand. 

This  book  every  one  contrives  and  rules  as  he  thinks  fittest 
for  himself.  The  following  is  a  specimen  of  a  form  which 
has  been  formerly  used.  .  It  is  ruled  in  three  columns,  as  in 
the  next  page. 

Here  Q  1  is  the  first  station,  where  the  angle  or  bearing 
is  105°  25'.  On  the  left,  at  73  links  in  the  distance  or  prin- 
cipal line,  is  an  offset  of  92  ;  and  at  610  an  offset  of  24  to  a 
cross  hedge.  On  the  right,  at  0,  or  the  beginning,  an  offset 
25  to  the  corner  of  the  field  ;  at  248  Brown's  boundary 
hedge  commences  ;  at  610  an  offset  35  ;  and  at  954,  the  end 
of  the  first  line,  the  0  denotes  its  terminating  in  the  hedge. 
And  so  on  for  the  other  stations. 

A  line  is  drawn  under  the  work,  at  the  end  of  every  sta- 
tion line,  to  prevent  confusion. 


454 


LAKD 


Form  ofthU  FiM.Book. 


Offset*  and  Remarks 
on  the  left. 

Stations, 
Bearings, 

and 
Distances. 

Ofiveta  and  Remarks 
on  the  right. 

80 
OS 

a  cross  hedge  34 

0  1 
105°  25' 
00 
73 
248 
610 
054 

25  corner 

Brown's  hedge 

35 

00 

house  corner  51 
34 

0  2 
53*  10* 
25 
120 
764 

21 

20  a  tree 
40  a  stile 

a  brook  30 

foot-path  16 
cross  hedge  18 

0  3 
67*  20 
61 
248 
635) 
810 
973 

35 

16  a  spring 
20  a  pond 

Then  the  plan,  on  a  small  scale  drawn  from  the  above 
field- book,  will  be  a*  in  the  following  figure.  But  thn  pupil 
may  draw  a  plan  of  3  or  4  time*  the  size  on  his  paper  book. 
The  dotted  lines  denote  the  3  chain  or  measured  linea,  and 
the  bluck  lines  the  boundaries  on  the  right  and  left. 


But  some  skilful  surveyors  now  make  use  of  a  different 
method  for  the  field-book,  namely,  beginning  at  the  bottom 


455 


of  the  page  and  writing  upwards ;  sketching  also  a  neat 
boundary  on  either  hand,  resembling  the  parts  near  tho 
measured  lines  as  they  pas*  along ;  an  example  of  which  was 
given  in  the  new  method  of  surveying,  in  the  preceding 
pages. 

In  smaller  surveys  and  measurements,  a  good  way  of  set- 
ting  down  the  work,  is  to  draw  by  the  eye,  on  a  piece  of 
paper,  a  figure  resembling  that  which  id  to  be  measured  ; 
and  so  writing  the  dimensions,  as  they  are  found,  against 
the  corresponding  parts  of  the  figure.  And  this  method 
may  be  practised  to  a  considerable  extent,  even  in  the  larger 
surveys. 

SECTION  III. 


OF  COMPUTING  AND  DIVIDING. 

PROBLEM  XVI. 

To  compute  the  Contents  of  Fields. 

1.  Compute  the  contents  of  the  figures  as  divided  into 
triangles,  or  trapeziums,  by  the  proper  rules  for  these  figures 
laid  down  in  measuring ;  multiplying  the  perpendiculars  by 
the  diagonals  or  bases,  both  in  links,  and  divide  by  2 ,  the 
quotient  is  acres,  after  having  cut  off  five  figures  on  the  right 
for  decimals.  Then  bring  there  decimals  to  roods  and 
perches,  by  multiplying  first  by  4,  and  then  by  40.  An 
example  of  which  is  ghen  in  the  description  of  the  chain, 
pag.  480. 

2.  In  small  and  separate  pieces,  it  is  usual  to  compute  their 
contents  from  the  measures  of  the  lines  taken  in  surveying 
them,  without  making  a  correct  plan  of  them. 

3.  In  pieces  bounded  by  very  crooked  and  winding  hedges, 
measured  by  offsets,  all  the  parts  between  the  offsets  are  most 
accurately  measured  separately  as  small  trapezoids. 

4.  Sometimes  such  pieces  as  that  last  mentioned  are  com* 
puted  by  finding  a  mean  breadth,  by  adding  all  the  offsets 
together,  and  dividing  the  sum  by  the  number  of  them,  ac- 
counting that  for  one  of  them  where  the  boundary  meets 
the  station* line  (which  increases  the  number  of  them  by  I, 
for  the  divisor,  though  it  does  not  increase  the  sum  or  quan- 
tity t  >  be  divided) ;  then  multiply  the  length  by  that  mean 
breadth. 

5.  But  in  larger  pieces  and  whole  estate**  wmm£&%<& 


456 


LARD 


many  fields,  it  is  the  common  practice  to  make  a  rough  plan 
of  the  whole,  and  from  it  compute  the  contents,  quite  inde. 
pendent  of  the  measures  of  the  lines  and  angles  that  wort 
taken  in  surveying.  For  then  new  lines  are  drawn  in  the 
fields  on  the  plans,'  so  as  to  divide  them  into  trapeziums  and 
triangles,  the  bases  and  perpendiculars  of  which  are  measured 
on  the  plan  by  means  of  the  scale  from  which  it  was  drawn, 
and  so  multiplied  together  for  the  contents.  In  this  way, 
the  work  is  very  expeditiously  done,  and  sufficiently  correct; 
for  such  dimensions  are  taken  as  afford  the  most  easy  method 
of  calculation ;  and  among  a  number  of  parts,  thus  taken 
and  applied  to  a  scale,  though  it  be  likely  that  some  of  the 
parts  will  be  taken  a  small  matter  too  little,  and  others  too 
great,  yet  they  will,  on  the  whole,  in  all  probability,  very 
nearly  balance  one  another,  and  give  a  sufficiently  accurate 
result.  After  all  the  fields  and  particular  parts  are  thus 
computed  separately,  and  added  all  together  into  one  sum ; 
calculate  the  whole  estate  independent  of  the  fields,  by  di- 
viding it  into  large  and  arbitrary  triangles  and  trapeziums, 
and  add  these  also  together.  Then  if  this  sum  be  equal  to 
the  former,  or  nearly  so.  the  work  is  right ;  but  if  the  sums 
have  any  considerable  difference,  it  is  wrong,  and  they  must 
be  examined,  and  re-computed,  till  they  nearly  agree. 

6.  But  the  chief  art  in  computing,  consists  in  finding  the 
contents  of  pieces  bounded  by  curved  or  very  irregular  lines, 
or  in  reducing  such  crooked  sides  of  fields  or  boundaries  to 
straight  lines,  that  shall  enclose  the  same  or  equal  area  with 
those  crooked  sides,  and  so  obtain  the  area  of  the  curved 
figure  by  means  of  the  right-lined  one,  which  will  commonly 
be  a  trapezium.  Now  this  reducing  the  crooked  sides  to 
straight  ones,  is  very  easily  and  accurately  performed  in  this 
manner: — Apply  the  straight  edge  of  a  thin,  clear  piece  of 
lantern. horn  to  the  crooked  line,  which  is  to  be  reduced, 
in  such  a  manner,  that  the  small  parts  cut  off  from  the 
crooked  figure  by  it,  may  be  equal  to  those  which  are  taken 
in  :  which  equality  of  the  parts  included  and  excluded  you 
will  presently  be  able  to  judge  of  very  nicely  by  a  little  prac- 
tice :  then  with  a  pencil,  or  point  of  a  tracer,  draw  a  line  by 
the  straight  edge  of  the  horn.  Do  the  same  by  the  other 
sides  of  the  field  or  figure.  So  shall  you  have  a  straight- 
sided  figure  equal  to  the  curved  one  ;  the  content  of  which, 
being  computed  as  before  directed,  will  be  the  content  of  the 
crooked  figure  proposed. 

Or,  instead  of  the  straight  edge  of  the  horn,  a  horse-hair, 
or  fine  thread,  may  be  applied  across  the  crooked  sides  in 
the  same  manner ;  and  the  easiest  way  of  using  the  thread,  it 
to  string  a  amaVV  ateufat  how  with  it,  either  of  wire,  or  cane. 


IUKVJCYM6. 


457 


or  whale-bone,  or  such-like  slender  elastic  matter ;  for  the 
bow  keeping  it  always  stretched,  it  can  be  easily  and  neatly 
applied  with  one  hand,  while  the  other  is  at  liberty  to  make 
two  marks  by  the  side  of  it,  to  draw  the  straight  line  by. 

EXAMPLE. 

Thus,  let  it  be  required  to  find  thejeontents  of  the  same 
figure  as  in  Prob.  ix,  page  443,  to  a  scale  of  4  chains  to  an 
inch. 


Draw  the  4  dotted  straight  lines  ab,  bc,  cd,  da,  cutting 
off  equal  quantities  on  both  sides  of  them,  which  they  do  as 
near  as  the  eye  can  judge  :  so  is  the  crooked  figure  reduced 
to  an  equivalent  right-lined  one  of  4  sides,  abcd.  Then 
draw  the  diagonal  b»,  which,  by  applying  a  proper  scale 
to  it,  measures  suppose  1256;  Also  the  perpendicular,  or 
nearest  distance  from  a  to  this  diagonal,  measures  456 ;  and 
the  distance  of  c  from  it,  is  428. 

Then,  half  the  sum  of  456  and  428,  multiplied  by  the 
diagonal  1256,  gives  555152  square  links,  or  5  acres,  2  roods, 
8  perches,  the  content  of  the  trapezium,  or  of  the  irregular 
crooked  piece. 

As  a  general  example  of  this  practice,  let  the  contents  be 
computed  of  all  the  fields  separately  in  the  foregoing  plan 
facing  page  453,  and,  by  adding  the  contents  altogether,  the 
whole  sum  or  content  of  the  estate  will  be  found  nearly  equal 
to  103}  acres.  Then,  to  prove  the  work,  divide  the  whole 
plan  into  two  parts,  by  a  pencil  line  drawn  across  it  any  way 
near  the  middle,  as  from  the  corner  I  on  the  right,  to  the 
corner  near  s  on  the  loft ;  then,  by  computing  these  two 
large  parts  separately,  their  sum  must  be  nearly  equal  to  the 
former  sum,  when  the  work  is  all  right. 

Vol.  I.  59 


458 


LAND  SURVEYING. 


PROBLEM  XVII. 

To  Transfer  a  Plan  to  Another  Paper,  $c. 

After  the  rough  plan  is  completed,  and  a  fair  one  is 
wanted  ;  this  may  be  done  by  any  of  the  following  methods* 

First  Method.— Lay  the  rough  plan  on  the  clean  paper, 
keeping  them  always  pressed  flat  and  close  together,  by 
weights  laid  on  them?  Then  with  the  point  of  a  fine  pin 
or  pricker,  prick  through  all  the  corners  of  the  plan  to  be 
copied.  Take  them  asunder,  and  connect  the  pricked  points 
on  the  clean  paper,  with  lines  ;  and  it  is  done.  This  method 
is  only  to  he  practised  in  plans  of  such  figures  as  are  small 
and  tolerably  regular,  or  bounded  by  right  lines. 

Second  Method* — Rub  the  back  of  the  rough  plan  over 
win  black-lead  powder  ;  and  lay  this  blacked  part  on  the 
clean  paper  on  which  the  plan  is  to  be  copied,  and  in  the 
proper  position.  Then,  with  the  blunt  point  of  some  hard 
substance,  as  brass,  or  such-like,  trace  over  the  lines  of  the 
whole  plan  ;  pressing  the  tracer  so  much,  as  that  the  bJack 
lead  under  the  lines  may  be  transferred  to  the  clean  paper  : 
after  w  hich,  take  off  the  rough  plan,  and  trace  over  the  leaden 
marks  with  common  ink,  or  with  Indian  ink. — Or,  instead  of 
blacking  the  rough  plan,  we  may  keep  constantly  a  blacked 
paper  to  lay  between  the  plans. 

Third  Method. — Another  method  of  copying  plans,  is  by 
means  of  squares.  This  is  performed  by  dividing  both  ends 
and  sides  of  the  plan  which  is  to  be  copied  into  any  conve- 
nient number  of  equal  parts,  and  connecting  the  correspond- 
ing points  of  division  with  lines  ;  which  will  divide  the  plan 
into  a  number  of  small  squares.  Then  divide  the  paper,  on 
which  the  plan  is  to  be  copied,  into  the  same  number  of 
squares,  each  equal  to  the  former  when  the  plan  is  to  be 
copied  of  the  same  size,  but  greater  or  less  than  the  others, 
in  the  proportion  in  which  the  plan  is  to  be  increased  or 
diminished,  when  of  a  different  size.  Lastly,  copy  into  the 
clean  squares  the  parts  contained  in  the  corresponding  squares 
of  the  old  plan  ;  and  you  will  have  the  copy,  either  of  the 
same  size,  or  greater  or  less  in  any  proportion. 

Fourth  Method. — A  fourth  method  is  by  the  instrument 
called  a  pentagraph,  which  also  copies  the  plan  in  any  size 
required  :  for  this  purpose,  also,  Professor  Wallace's  eido* 
graph  may  be  advantageously  employed. 

Fifth  method. — A  very  neat  method,  at  least  in  copying 
from  u  fair  plan,  is  this.  Procure  a  copying  frame  or  glass, 
made  in  this  manner  :  namely,  a  large  square  of  the  best 


AlTOFfCBRS9  WORK. 


window  glass,  set  in  a  broad  frame  of  wood,  which  can  be 
raised  up  to  any  angle,  when  the  lower  side  of  it  rests  on  a 
table.  Set  this  frame  up  to  any  angle  before  you,  facing  a 
strong  light ;  fix  the  old  plan  and  clean  paper  together,  with 
several  pins  quite  around,  to  keep  them  together,  the  clean 
paper  being  laid  uppermost,  and  over  the  face  of  the  plan  to 
be  copied.  Lay  them,  with  the  back  of  the  old  plan,  on  the 
glass ;  namely,  that  part  which  you  intend  to  begin  at  to 
copy  first ;  and  by  means  of  the  light  shining  through  the 
papers,  you  will  very  distinctly  perceive  every -line  of  the  plan 
through  the  clean  paper.  In  this  state  then  trace  all  the 
lines  on  the  paper  with  a  pencil.  Having  drawn  that  part 
which  covers  the  glass,  slide  another  part  over  the  glass,  and 
copy  it  in  the  same  manner.  Then  another  part :  and  so 
on,  till  the  whole  is  copied.  Then  take  them  asunder,  and 
trace  all  the  pencil  lines  over  with  a  fine  pen  and  Indian  ink, 
or  with  common  ink.  And  thus  you  may  copy  the  finest 
plan,  without  injuring  it  in  the  least. 


OF  ARTIFICERS'  WORKS, 


AND 

TIMBER  MEASURING. 


1.  OF  THE  CARPENTER'S  OR  SLIDING  RULE. 

The  Carpenter's  or  Sliding  Rule,  is  an  instrument  much 
used  in  measuring  of  timber  and  artificers'  works,  both  for 
taking  the  dimensions,  and  computing  the  contents. 

The  instrument  consists  of  two  equal  pieces,  each  a  foot 
in  length,  which  are  connected  together  by  a  folding  joint. 

One  side  or  face  of  the  rule  is  divided  into  inches,  and 
eighths,  or  half-quartoM  On  the  same  fuce  also  are  several 
plane  scales  divided  mm  twelfth  parts  by  diagonal  lines; 
which  are  used  in  plannutg  dimensions  that  are  taken  in  feet 
and  inches.  The  edge  of  the  rule  is  commonly  divided 
decimally,  or  into  tenths  ;  namely,  each  foot  into 


400 


ARTIFICERS*  WORK. 


parts,  and  each  of  these  into  ten  parts  again  ;  so  that  by 
means  of  this  last  scale,  dimensions  are  taken  in  feet,  tenths, 
and  hundredths,  and  multiplied  as  common  decimal  numbers, 
which  is  the  best  way. 

On  the  one  part  of  the  other  face  are  four  lines,  marked 

b,  c,  d  ;  the  two  middle  ones  b  and  c  being  on  a  slider, 
which  runs  in  a  groove  made  in  the  stock.  The  same  num. 
berg  serve  for  both  these  two  middle  lines,  the  one  being 
above  the  numbers,  and  the  other  below. 

These  four  lines  are  logarithmic  ones,  and  the  three  a,  s, 
c,  which  are  all  equal  to  one  another,  are  double  lines,  as 
they  proceed  twice  over  from  1  to  10.  The  other  or  lowest 
line,  d,  is  a  single  one,  proceeding  from  4  to  40.  It  is  also 
called  the  girt  line,  from  its  use  in  computing  the  contents 
of  trees  and  timber ;  and  on  it  are  marked  wo  at  17*15,  and 
AO  at  18-05,  the  wine  and  ale  gage  points,  to  make  this  in- 
strument serve  the  purpose  of  a  gaging  rule. 

On  the  other  part  of  this  face,  there  is  a  table  of  the  value 
of  a  load,  or  50  cubic  feet  of  timber,  at  all  prices,  from  6 
pence  to  2  shillings  a  foot. 

When  1  at  the  beginning  of  any  line  is  accounted  1,  then 
the  1  in  the  middle  will  be  10,  and  the  10  at  the  end  100 ; 
but  when  1  at  the  beginning  is  counted  10,  then  the  1  in  the 
middle  is  100,  and  the  10  at  the  end  1000  ;  and  so  on.  And 
all  the  smaller  divisions  are  altered  proportionally. 


n.  ARTIFICERS'  WORK. 

Artificers  compute  the  contents  of  their  works  by  several 
different  measures.  As, 

Glazing  and  masonry,  by  the  foot ;  Painting,  plastering, 
paving,  6zc.  by  the  yard,  of  9  square  feet :  Flooring, 
partitioning,  roofing,  tiling,  6zc.  by  the  square  of  100 
square  feet : 

And  brickwork,  either  by  the  yard  of  9  square  feet,  or  by 
the  perch,  or  square  rod  or  pole,  containing  272}  square 
feet,  or  30}  square  yards,  being  the  square  of  the  rod  or 
pole  of  16}  feet  or  5}  yards  long. 
As  this  number  272}  is  troublesome  to  divide  by,  the  }  is 
often  omitted  in  practice,  and  the  content  in  feet  divided  only 
by  the  272. 

All  works,  whether  superficial  or  solid,  are  computed  by 
the  rules  proper  to  the  figure  of  them,  whether  it  be  a  tri- 
angle, ot  rectang\e,  &  ^axa\taV)^«d,  or  any  other  figure. 


mUCKLAYSBft'  WORK*  401 


III-  BRICKLAYERS'  WORK. 

Brickwork  is  estimated  at  the  rate  of  a  brick  and  a  half 
thick.  So  that  if  a  wall  be  more  or  less  than  this  standard 
thickness,  it  must  be  reduced  to  it,  as  follows : 

Multiply  the  superficial  content  of  the  wall  by  the  number 
of  half  bricks  in  the  thickness,  and  divide  the  product  by  3. 

The  dimensions  of  a  building  may  be  taken  by  measuring 
half  round  on  the  outside  and  half  round  on  tho  inside ;  the 
sum  of  these  two  gives  the  compass  of  the  wall,  to  be  multi- 
plied by  the  height,  for  the  content  of  the  materials. 

Chimneys  are  commonly  measured  as  if  they  were  solid, 
deducting  only  the  vacuity  from  the  hearth  to  the  mantle,  on 
account  of  the  trouble  of  them.  All  windows,  doors,  dec.  are 
to  be  deducted  out  of  the  contents  of  the  walls  in  which  they 
are  placed. 

The  dimensions  of  a  common  bare  brick  are,  8J  inches 
long,  4  inches  broad,  and  2\  thick ;  but  including  the  half 
inch  joint  of  mortar,  when  laid  in  brickwork,  every  dimen- 
sion is  to  be  counted  half  an  inch  more,  making  its  length 
9  inches,  its  breadth  4),  and  thickness  3  inches.  So  that 
every  4  courses  of  proper  brickwork  measures  just  1  foot  or 
12  inches  in  height. 

EXAXPLE8. 

Exam.  1.  How  many  yards  and  rods  of  standard  brick* 
work  are  in  a  wall  whose  length  or  compass  is  57  feet  3 
inches,  and  height  24  feet  6  inches ;  the  wall  being  2\  bricks 
or  5  half  bricks  thick  ?  Ans.  8  rods,  17}  yards. 

Exam.  2.  Required  the  content  of  a  wall  62  feet  6  inches 
long,  and  14  feet  8  inches  high,  and  2|  bricks  thick  ? 

Ans.  169-753  yards. 

Exam.  3.  A  triangular  gable  is  raised  17|  feet  high,  on 
an  end  wall  whose  length  is  24  feet  9  inches,  the  thickness 
being  2  bricks :  required  the  reduced  content  ? 

Ans.  32-08J  yards. 

Ex  ax.  4.  The  end  wall  of  a  house  is  28  feet  10  inches 
long,  and  55  feet  8  inches  high,  to  the  eaves ;  20  feet  high 
is  2£  bricks  thick,  other  20  feet  high  is  2  bricks  thick,  and 
the  remaining  15  feet  8  inches  is  l£  brick  thick ;  above  which 
is  a  triangular  gable,  of  1  brick  thick,  which  rises  42  courses 
of  bricks,  of  which  every  4  courses  make  a  foot.  What  is  the  - 
whole  content  in  standard  measure  ? 

&n&.  Y*x&&« 


402 


carpenters'  and  joiners'  work. 


IV.  MASONS'  WORK. 

To  Masonry  belong  all  sorts  of  stone  work  ;  and  the  mea- 
sure made  use  of  is  a  foot,  either  superficial  or  solid. 

Walls,  columns,  blocks  of  stone  or  marble,  &c.  are  mea- 
sured by  the  cubic  foot  ;  and  pavements,  slabs,  chimney- 
pieces,  &c.  by  the  superficial  or  square  foot. 

Cubic  or  solid  measure  is  used  for  the  materials,  and  square 
measure  for  the  workmanship. 

In  (he  solid  measure,  flic  true  length,  breadth,  and  thick, 
ness  arc  taken  and  multiplied  continually  together.  In  the 
superficial,  there  must  be  taken  the  length  and  breadth  of 
every  part  of  the  projection  which  is  seen  without  the  general 
upright  face  of  the  building. 

EXAMPLES* 

Exam.  1.  Required  the  solid  content  of  a  wall,  53  feet 
6  inches  long,  12  feet  3  inches  high,  and  2  feel  thick  ? 

Ans.  1310J  feet. 

Exam.  2.  What  is  the  solid  content  of  a  wall,  the  length 
being  21  feet  3  inches,  height  10  feet  9  inches,  and  2  feet 
thick  ?  Ans.  521-375  feet. 

Exam.  3.  Required  the  value  of  a  marble  slab,  at  8*.  per 
foot ;  the  length  being  5  feet  7  inches,  and  breadth  1  foot 
10  inches  ?  Ans.  1Z.  1*.  lOJd. 

Exam.  4.  In  a  chimney-piece,  suppose  the 
length  of  the  mantle  and  slab,  each  4  feet  6  inches 
breadth  of  both  together         -       3  2 
length  of  each  jamb  -.44 
breadth  of  both  together.  1  9 

Required  the  superficial  content  ?     Ans.  21  feet  10  inches. 


V.  CARPENTERS'  AND  JOINERS'  WORK. 

To  this  branch  belongs  all  the  wood-work  of  a  house, 
such  as  flooring,  partitioning,  roofing,  &c. 

Large  and  plain  articles  are  usually  measured  by  the 
square  foot  or  yard,  &c.  ;  but  enriched  mouldings,  and  some 
other  articles,  are  often  estimated  by  running  or  lineal  mea. 
sure  ;  and  some  things  are  rated  by  the  piece. 

In  measuring  of  Joists,  take  the  dimensions  of  one  joist, 


carpenters'  and  joiners'  work. 


463 


and  multiply  its  content  by  the  number  of  them  ;  consider- 
ing that  each  end  is  let  into  the  wall  about  &  of  the  thick- 
ness,  as  it  ought  to  be. 

Partitions  are  measured  from  wall  to  wall  for  one  dimen- 
sion, and  from  floor  to  floor,  as  far  as  they  extend,  for  the 
other. 

The  measure  of  Centering  for  Cellars  is  found  by  making 
a  string  pass  over  the  surface  of  the  arch  for  the  breadth, 
and  taking  the  length  of  the  cellar  for  the  length  :  but  in 
groin  centering,  it  is  usual  to  allow  double  measure,  on  ac- 
count of  their  extraordinary  trouble. 

In  Roofing,  the  dimensions,  as  to  length,  breadth,  and 
depth,  are  taken  as  in  flooring  joists,  and  the  contents  com- 
puted the  same  way. 

In  Floor -boarding,  take  the  length  of  the  room  for  one  di- 
mension, and  the  breadth  for  the  other,  to  multiply  together 
for  the  content. 

For  Stair-cases,  take  the  breadtii  of  all  the  steps,  by  mak- 
ing a  line  ply  close  over  ihem,  from  the  top  to  the  bottom,  and 
multiply  the  length  of  this  line  by  the  length  of  a  step,  for 
the  whole  area. — By  the  length  of  a  step  is  meant  the  length 
of  the  front  and  the  returns  nt  the  two  ends  ;  and  by  the 
breadth  is  to  be  understood  the  girts  of  its  two  oater  sur- 
faces, or  the  tread  and  riser. 

For  the  Balustrade,  take  the  whole  length  of  the  upper 
part  of  the  hand-rail,  and  girt  over  its  end  till  it  meet  the 
top  of  the  newel-post,  for  the  one  dimension  ;  and  twice  the 
length  of  the  baluster  on  the  landing,  with  the  girt  of  the 
hand-rail,  for  the  other  dimension. 

For  Wainscoting,  take  the  compass  of  the  room  for  the 
one  dimension  ;  and  the  height  from  the  floor  to  the  ceiling, 
making  the  string  ply  close  into  all  the  mouldings,  for  the 
other. 

For  Doors,  take  the  height  and  the  breadth,  to  multiply 
them  together  for  the  area. — If  the  door  be  panneled  on 
both  sides,  take  double  its  measure  for  the  workmanship  ; 
but  if  one  side  only  be  panneled,  take  the  area  and  its  half 
for  the  workmanship.  For  the  Surrounding  Architrave,  girt 
it  about  the  uppermost  part  for  its  length  ;  and  measure  over 
it,  as  far  as  it  can  be  seen  when  the  door  is  open,  for  the 
breadth. 

Window-shutters,  Bases,  &c.  are  measured  in  like  manner. 
In  measuring  of  Joiners'  work,  the  sttin^  \a  roa&fe  v&  ^ 


464 


SLATERS  AND  TILERS'  WOBK. 


close  into  all  mouldings,  and  to  every  part  of  the  work  over 
which  it  passes. 

EXAMPLES. 

Ex  ax.  1.  Required  the  content  of  a  floor,  48  feet  6  inches 
long,  and  24  feet  3  inches  broad?        An*.  11  sq.  76}  feet. 

Exam.  2.  A  floor  being  36  feet  3  inches  long,  and  16  feet 
6  inches  broad,  how  many  squares  are  in  it  ? 

Ans.  5  sq.  98}  feet. 

Exam.  3.  How  many  squares  are  there  in  173  feet  10 
inches  in  length,  and  10  feet  7  inches  height,  of  partitioning  ? 

Ans.  18*3973  squares. 

Exam.  4.  What  cost  the  roofing  of  a  house  at  10*.  6d. 
a  square  ;  the  length  within  the  walls  being  52  feet  8  inches, 
and  the  breadth  30  feet  6  inches  ;  reckoning  the  roof  £  of 
the  flat?  Ans.  121.  12s.  ll}d. 

Exam.  5.  To  how  much,  at  0*.  per  square  yard,  amounts 
the  wainscoting  of  a  room  ;  the  height,  taking  in  the  cornice 
and  mouldings,  being  12  feet  6  inches,  and  the  whole  com- 
pass  83  feet  8  inches ;  also  the  three  window-shutters  are 
each  7  feet  by  8  inches  by  3  feet  G  inches,  and  the  door  7  feet 
by  3  feet  0  inches ;  the  door  and  shutters,  being  worked  on 
both  sides,  arc  reckoned  work  and  half  work  ? 

Ans.  36/.  12*.  2*d. 


VI.  SLATERS'  AND  TILERS'  WORK. 

In  these  articles,  the  content  of  a  roof  is  found  by  mul- 
tiplying the  length  of  the  ridge  by  the  girt  over  from  eaves 
to  caves ;  making  allowance  in  this  girt  for  the  double  row 
of  slates  at  the  bottom,  or  for  how  much  one  row  of  slates  or 
tiles  is  laid  over  another. 

When  the  roof  is  of  a  true  pitch,  that  is,  forming  a  right 
angle  at  top;  then  the  breadth  of  the  building,  with  its  half 
added,  is  the  girt  added  over  both  sides  nearly. 

Iu  angles  formed  in  a  roof,  running  from  the  ridge  to  the 
eaves,  when  the  angle  bends  inwnnN.  it  is  called  a  valley  ; 
but  when  outwards,  it  is  onllcd  n  hip. 

Deductions  are  made  ibr  chimney  shafts  or  window  holes. 


PLASTERERS*  won. 


EXAMPLES. 

Exam.  1.  Required  the  content  of  a  slated  roof,  the 
length  being  45  feet  9  inches,  and  the  whole  girt  34  feet  3 
inches?  Ans.  174^  yank. 

Exam.  2.  To  how  much  amounts  the  tiling  of  a  house, 
at  25*.  6d.  per  square ;  the  length  being  43  feet  10  inches, 
and  the  breadth  on  the  fiat  27  feet  5  inches ;  also  the  caves 
projecting  16  inches  on  each  side,  and  the  roof  of  a  true 
pitch  ?  Ans.  241.  9s.  fyd. 


VH.  PLASTERERS'  WORK. 

Plasterers'  work  is  of  two  kinds ;  namely,  ceiling,  which 
is  plastering  on  laths ;  and  rendering,  which  is  plastering  on 
walls :  which  are  measured  separately. 

The  contents  are  estimated  either  by  the  foot  or  the  yard, 
or  the  square,  of  100  feet.  Enriched  mouldings,  dec.  are 
rated  by  running  or  lineal  measure. 

Deductions  are  made  for  chimneys,  doors,  windows,  &c. 

examples. 

Exam.  1.  How  many  yards  contains  the  ceiling  which  is 
43  feet  3  inches  long,  and  25  feet  6  inches  broad  ? 

Ans.  122}. 

Exam.  2.  To  how  much  amounts  the  ceiling  of  a  room, 
at  10J.  per  yard :  the  length  being  21  feet  8  inches,  and  the 
breadth  14  feet  10  inches  ?  Ans.  1/.  9s.  8Jrf. 

Exam.  3.  The  length  of  a  room  is  18  feet  6  inches,  the 
breadth  12  feet  3  inches,  and  height  10  feet  6  inches ;  to 
how  much  amounts  the  ceiling  and  rendering,  the  former  at 
Sd.  and  the  latter  at  3d  per  yard  :  allowing  for  the  door  of 
7  feet  by  3  feet  8,  and  a  fire-place  of  3  feet  square  ? 

Ans.  1Z.  13*.  3jd. 

Exam.  4.  Required  the  quantity  of  plastering  in  a  room, 
the  length  being  14  feet  5  inches,  breadth  13  feet  2  inches, 
and  height  9  feet  3  inches  to  the  under  side  of  the  cornice, 
which  girts  8}  inches,  and  projects  5  inches  from  the  wall 
on  the  upper  part  next  the  ceiling  ;  deducting  only  for  a  door 
7  feet  by  4? 

Ans.  53  yards  5  feet  3}  inches  of  rendering 
18         5       6  of  ceiling 

39      Of}  ofwrarcfe. 
Vol.  I.  60 


406 


CLAftflUtl'  WOfcX. 


VIII.  PAINTERS9  WORK. 

Painters'  work  is  computed  in  square  yards.  Every  part 
is  measured  where  the  colour  lies  ;  and  the  measuring  line  is 
forced  into  all  the  mouldings  and  corners. 

Windows  are  done  at  so  much  a  piece.  And  it  is  usual  to 
allow  double  measure  for  carved  mouldings,  dec. 

EXAMPLES. 

Exam.  1.  How  many  yards  of  painting  contains  the  room 
which  is  65  feet  6  inches  in  compass,  and  12  feet  4  inches 
high  ?  Ans.  89}£  yards. 

Exam.  2.  The  length  of  a  room  being  20  feet,  its  breadth 
14  feet  6  inches,  and  height  10  feet  4  niches  ;  how  many 
varus  of  painting  are  in  it,  deducting  a  fire-place  of  4  feet 
by  4  feet  4  inches,  and  two  windows  each  6  feet  by  S  feet 

2  inches  ?  Ans.  73^  yards. 
Exam.  3.  What  cost  the  painting  of  a  room,  at  6d.  per 

yard  ;  its  length  being  24  feet  6  inches,  its  breadth  16  feet 

3  inches,  and  height  12  feet  9  inches  ;  also  the  door  is  7  feet 
by  3  feet  6,  and  the  window-shutters  to  two  windows  each 
7  feet  9  by  3  feet  8 ;  but  the  breaks  of  the  windows  them- 
selves  are  8  feet  6  inches  high,  and  1  foot  3  inches  deep  ;  in- 
cluding also  the  window  cills  or  seats,  and  the  soffits  above, 
the  dimensions  of  which  are  known  from  the  other  dimen. 
sions  :  but  deducting  the  fire-place  of  5  feet  by  5  feet  6  ? 

Ans.  31  3*.  10}d. 


IX.  GLAZIERS'  WORK. 

Glaziers  take  their  dimensions,  either  in  feet,  inches,  and 
parts,  or  feet,  tenths,  and  hundredths.  And  they  compute 
their  work  in  square  feet. 

In  taking  the  length  and  breadth  of  a  window,  the  cross 
bars  between  the  squares  are  included.  Also  windows  of 
round  or  oval  forms  are  measured  as  square,  measuring  them 
to  their  greatest  length  and  breadth,  on  account  of  the  waste 
in  cutting  the  glass. 

examples. 

Exam.  1.  How  many  square  feet  contains  the  window 
which  is  4*25  feet  long,  and  2-75  feet  broad  ?        Ans.  llf 


PAVEIt'*  WORK. 


407 


Exam.  2.  What  will  the  glazing  a  triangular  sky-light 
tome  to,  at  lOd.  per  foot ;  the  base  being  12  feet  6  inches, 
and  the  perpendicular  height  6  feet  9  inches  ? 

Ans.  II.  15s.  \\d. 

Exam.  3.  There  is  a  house  with  three  tiers  of  windows, 
three  windows  in  each  tier,  their  common  breadth  3  feet  1 1 
inches  : 

now  the  height  of  the  first  tier,  is  7  feet  10  inches 
of  the  second      6  8 
of  the  third         5  4 
Required  the  expense  of  glazing  at  I4d  per  foot  ? 

Ans.  13*.  lis.  lO^d. 

Exam.  4.  Required  the  expense  of  glazing  the  windows 
of  a  house  at  13i.  a  foot ;  there  being  three  stories,  and  three 
windows  in  each  story  : 

the  height  of  the  lower  tier  is  7  feet  9  inches 
of  the  middle        6  6 
of  the  upper         5  3| 
and  of  an  oval  window  over  the  door  1  10} 
the  common  breadth  of  all  the  windows  being  3  feet  9 
inches  ?  Ans.  121.  5s.  6d. 


X.  PAVERS'  WORK. 

Pavers'  work  is  done  by  the  square  yard.  And  the  con* 
tent  is  found  by  multiplying  the  length  by  the  breadth. 


EXAMPLS8. 

Exam.  1.  What  cost  the  paving  a  foot-path,  at  Ss.  4d.  a 
yard  ;  the  length  being  35  feet  4  inches,  and  breadth  8  feet 
3  inches  ?  Ans.  51.  7s.  ll$d. 

Exam.  2.  What  cost  the  paving  a  court,  at  3*.  2d.  per 
yard  ;  the  length  being  27  feet  10  inches,  and  the  breadth 
14  feet  9  inches  ?  Ans.  71.  4s.  5}d. 

Exam.  3.  What  will  be  the  expense  of  paving  a  rectan. 
gular  court-yard,  whose  length  is  63  feet,  and  breadth  45 
feet ;  in  which  there  is  laid  a  foot-path  of  5  feet  3  inches 
broad,  running  the  whole  length,  with  broad  stones,  at  8*. 
a  yard  ;  the  rest  being  paved  with  pebbles  at  2s.  6d.  a  yard ; 

Ans.  401  5s.  10^1. 


XI.  PLUMBERS*  WORK. 


Pmnsfts'  work  is  rated  at  so  much  a  pound,  or  else  fey 
the  hundred  weight  of  113  pounds. 

J  Sheet  lead,  used  in  roofing,  guttering,  Ac  is  from  II  t» 
101b.  to  the  square  foot.  And  a  pipe  of  an  inch  bore  ia  cess* 
feoely  l&or  141b,  to  tbe  yard  in  length, 

jEgAJt*  1.  How  much  weighs  the  lead  which  is  80  feet 
C  inches  long,  and  3  feet  3  inches  broad,  at  8|lb.  to  the 
a^iarefeot?  P    Ana.  1091  ^  lb. 

Exam.  2.  What  cdst  the  covering  and  guttering*  reef 
With  lead,  at  18s.  the  cwU ;  the  length  of  the  roof  being  43 
feet,  and  breadth  or  girt  over  it  32  feet ;  the  guttering  57 
feet  long,  and  2  feet  wide  ;  the  former  9*831  lb.  and  the  latter 
7<37ftlb.  to  the  square  foot  ?  Ana,  1151.  9s.  ljd- 


XII.  TIMBER  MEASURING. 

PROBLEM  I. 

7b  find  the  Area,  or  Superficial  Content  of  a  Board  or 
Plank. 

Multiply  the  length  by  the  mean  breadth. 

Note.  When  the  board  is  tapering,  add  the  breadths  at 
the  two  ends  together,  and  take  half  the  sum  for  the  mean 
breadth.    0{  else  take  the  mean  breadth  in  the  middle. 

By  the  Sliding  Rule. 

Set  12  on  b  to  the  breadth  in  inches  on  a  ;  then  against  the 
length  in  feet  on  b,  is  the  content  on  a,  in  feet  and  fractional 
parts. 

bxaxflbs. 

£xax.  1.  What  is  the  value  of  a  plank,  at  lfd.  per  feet, 
whose  length  is  12  feet  6  inches,  and  mean  breadth  11 
iftfbes?  Ans.  ls.5d. 


^  TIMBU  MSA1UBIK9.  469 

Exam.  2.  Requred  the  content  of  a  board,  whose  length  is 
11  feet  2  inches,  and  breadth  1  foot  10  inches  ? 

Ans.  20  feet  5  inches  8*. 
Exam.  3.  What  is  the  value  of  a  plank,  which  is  12  feet 
9  inches  long,  and  1  foot  3  inches  broad,  at  2±d.  a  foot? 

Ans.  3* .  3|  A 

Exam.  4.  Required  the  value  of  5  oaken  planks  at  3d. 
per  foot,  each  of  them  being  17 1  feet  long  ;  and  their  several 
breadths  as  follows,  namely,  two  of  13£  inches  in  the  middle, 
one  of  14 J  inches  in  the  middle,  and  the  two  remaining 
ones,  each  18  inches  at  the  broader  end,  and  11 J  at  the  nar. 
rower  ?  Ans.  II.  5s.  9±d. 

PROBLEM  II. 

To  find  the  Solid  Content  of  Squared  or  Four-tided  Timber. 

Multiply  the  mean  breadth  by  the  mean  thickness,  and 
the  product  again  by  the  length,  for  the  content  nearly. 

By  the  Sliding  Rule. 

C  D  D  C 

As  length  :  12  or  10  :  :  quarter  girt :  solidity. 
That  is,  as  the  length  in  feet  on  c,  is  to  12  on  d,  when 
the  quarter  girt  is  in  inches,  or  to  10  on  d,  when  it  is  in 
tenths  of  feet ;  so  is  the  quarter  girt  on  d,  to  the  content 
on  c. 

Note  1.  If  the  tree  taper  regularly  from  the  one  end  to 
the  other ;  either  take  the  mean  breadth  and  thickness  in 
the  middle,  or  take  the  dimensions  at  the  two  ends,  and  half 
their  sum  will  be  the  mean  dimensions :  which  multiplied  as 
above,  will  give  the  content  nearly. 

2.  If  the  piece  do  not  taper  regularly,  but  be  unequally 
thick  in  some  parts  and  small  in  others ;  take  several  different 
dimensions,  add  them  all  together,  and  divide  their  sum  by 
the  number  of  them,  for  the  mean  dimensions. 

EXAMPLES. 

Exam.  1.  The  length  of  a  piece  of  timber  is  18  feet 
6  inches,  the  breadths  at  the  greater  and  less  end  1  foot 
6  inches  and  1  foot  3  inches,  and  the  thickness  at  the  greater 
and  less  end  1  foot  3  inches  and  1  foot ;  required  the  solid 
content?  Ans.  28  feet  7  inches. 


Exam.  2.  What  is  the  content  of  the  piece  of  MfhBef, 
whoee  length  is  24£  feet,  and  the  mean  breadth  and  thick* 
ness  each  1-04  feet  ?  Ana.  26}  feet. 

Exam.  3.  Required  the  content  of  a  piece  of  timber, 
whose  length  is  20-38  feet,  and  its  ends  unequal  squares,  the 
side  of  the  greater  being  19 J  inches,  and  the  side  of  the  less 
9}  inches  t  Ana.  29*7562  feet 

Exam.  4.  Required  the  content  of  the  piece  of  timber, 
whose  length  is  27*36  feet ;  at  the  greater  end  the  breadth 
Is  1*78,  and  thickness  1*23  ;  and  at  the  less  end  the  breadth 
is  1-04,  and  thickness  0*91  feet  ?  Ans.  41  -278  feet. 

PROBLEM  m. 

To  find  the  Solidity  of  Round  or  Unfavored  Timber. 

Multiply  the  square  of  the  quarter  girt,  or  of  J  of  the 
toean  circumference,  by  the  length,  for  the  content. 

By  the  Sliding  Rule. 

Ae  the  length  upon  c  :  12  or  10  upon  d  :: 
quarter  girt,  in  12ths,  or  lOths,  on  d  :  content  on  c. 

Note  1.  When  the  tree  is  tapering  take  the  mean  dimen- 
sions as  in  the  former  problems,  either  by  girting  it  in  the 
fciddle,  for  the  mean  girt,  or  at  the  two  ends,  and  taking  half 
the  sum  of  the  two  ;  or  by  girting  it  in  several  places,  then 
adding  all  the  girts  together,  and  dividing  the  sum  by  the 
number  of  them,  for  the  mean  girt.  But  when  the  tree  is 
very  irregular,  divide  it  into  several  lengths,  and  find  the 
content  of  each  part  separately. 

2.  This  rule,  which  is  commonly  used,  gives  the  answer 
about  i  less  than  the  true  quantity  in  the  tree,  or  nearly 
what  the  quantity  would  be,  after  the  tree  is  hewed  square 
in  the  usual  way :  so  that  it  seems  intended  to  make  an 
allowance  for  the  squaring  of  the  tree. 

On  this  subject,  however,  Hutton's  Mensuration,  part  v. 
sect.  4,  may  be  advantageously  consulted. 


EXAMPLES. 


Exam.  1.  A  piece  of  round  timber  being  9  feet  6  inches 
long,  and  its  mean  quarter  girt  42  inches  ;  what  is  the 
content  ?  Ans.  116$  feet 

Exam.  2.  The  length  of  a  tree  is  24  feet,  its  girt  at  the 
thicker  end  14  feet,  and  at  the  smaller  end  2  feet ;  required 
the  content  7  Ans.  96  feet 


T1XBXK  UASUBHIO.  471 

Exam.  3.  What  is  the  content  of  a  tree  whose  mean 
girt  is  3*15  feet,  and  length  14  feet  6  inches  ? 

Ans.  8-9922  feet. 

Exam.  4.  Required  the  content  of  a  tree,  whose  length 
is  IH  feet,  which  girts  in  five  different  places  as  follows, 
namely,  in  the  first  plaoe  9*43  feet,  in  the  second  7*92,  in 
the  third  6-15,  in  the  fourth  4*74,  and  in  the  fifth  3*16  ? 

Ans.  42-519525. 


[  472  J 


1 

• 


CONIC  SECTIONS. 


DEFINITIONS. 


1.  Conic  Sections  are  the  figures  made  by  a  plane  cut- 
ting a  cone. 

2.  According  to  the  different  positions  of  the  cutting 
plane  there  arise  five  different  figures  objections,  namely,  a 
triangle,  a  circle,  an  ellipsis,  an  hyperboK,  and  a  parabola : 
the  three  last  of  which  only  are  peculiarly  called  Conic  Sec- 
tions. 


3.  If  the  caning  plane  pass  through 
the  vertex  of  the,  cone,  and  any  part  of 
the  base,  the  section  will  evidently  be  a 
triangle  ;  as  vab. 


4.  If  the  plane  cut  the  cone  parallel  to 
the  base,  or  make  no  angle  with  it,  the 
section  will  be  a  circle  ;  as  abd. 


5.  The  section  dab  is  an  ellipse 
when  the  cone  is  cut  obliquely  through 
both  sides,  or  when  the  plane  is  inclin- 
ed to  the  base  in  a  less  angle  than  the 
side  of  the  cone  is. 


6.  The  section  is  a  parabola,  when 
the  cone  is  cut  by  a  plane  parallel  to 
the  side,  or  when  the  cutting  plane  and 
the  side  of  the  cone  make  equal  angles 
with  the  base. 


DHflNITlOm. 


473 


7.  The  section  is  an  hyperbola,  when 
the  cutting  plane  makes  a  greater  angle 
with  the  base  than  the  side  of  the  cone 
makes. 


8.  And  if  all  the  sides  of  the  cone  be 
continued  through  the  vertex,  forming 
an  opposite  equal  cone,  and  the  plane 
be  also  continued  to  cut  the  opposite 
cone,  this  latter  section  will  be  the  op- 
posite hyperbola  to  the  former ;  as  dac. 


9.  The  Vertices  of  any  section,  are  the  points  where  the 
cutting  plane  meets  the  sides  of  that  vertical  triangular  sec- 
tion which  is  perpendicular  to  it ;  as  a  and  b. 

Hence  the  ellipse  and  the  opposite  hyperbolas,  have  each 
two  vertices  ;  but  the  parabola  only  one  ;  unless  we  consider 
the  other  as  at  an  infinite  distance. 

10.  The  Axis,  or  Transverse  Diameter,  of  a  conic  section, 
is  the  line  or  distance  ab  between  the  vertices. 

Hence  the  axis  of  a  parabola  is  infinite  in  length,  \b  being 
only  a  part  of  it. 


Ellipse.  Hyperbolas.  Parabola. 


1 1 .  The  centre  c  is  the  middle  of  the  axis. 

Hence  the  centre  of  a  parabola  is  infinitely  distant  from 
the  vertex.  And  of  an  ellipse,  the  axis  and  centre  lie  within 
the  curve  ;  but  of  an  hyperbola,  without. 

12.  A  Diameter  is  any  right  line,  as  ab  or  db,  drawn 
through  the  centre,  and  terminated  on  each  side  by  the  curve ; 
and  the  extremities  of  the  diameter,  or  its  intersections  with 
the  curve,  are  its  vertices. 

Hence  all  the  diameters  of  a  parabola  are  parallel  to  the 
axis,  and  infinite  in  length.    Hence  also  evei^  ftassfttax  <& 
Vol.  I.  61 


474 


CONIC  SECTIONS, 


the  ellipse  and  hyperbola  has  two  vertices ;  but  of  the  pan. 
bola,  only  one  ;  unless  we  consider  the  other  as  at  an  infinite 
distance. 

13.  The  Conjugate  to  any  diameter,  is  the  line  drawn 
through  the  centre,  and  parallel  to  the  tangent  of  the  curve 
at  the  vertex  of  the  diameter.  So,  fo,  parallel  to  the  tangent 
at  i>,  is  the  conjugate  to  de  ;  and  111,  parallel  to  the  tangent 
at  a,"  is  the  conjugate  to  ab. 

Hence  the  conjugate  hi,  of  the  axis  ab,  is  perpendicular 
to  it. .. 

14.  An  Ordinate  to  any  diameter,  is  a  line  parallel  to  its 
conjugate,  or  to  the  tangent  at  its  vertex,  and  terminated  by 
the  diameter  and  curve.  So  dk,  el,  are  ordinates  to  the  axis 
ab  ;  and  mn,  xo,  ordinates  to  the  diameter  dk. 

Hence  the  ordinates  of  the  axis  are  perpendicular  to  it. 

15.  An  Absciss  is  a  part  of  auy  diameter  contained  between 
either  of  its  vertices  and  an  ordinate  to  it ;  as  ak  or  bk,  or 
dn  or  en. 

Hence,  in  the  ellipse  and  hyperbola,  ever}'  ordinate  has 
two  determinate  abscisses ;  but  in  the  parabola  only  one  ;  the 
other  vertex  of  the  diameter  being  infinitely  distant. 

1G.  The  Parameter  of  any  diameter,  is  a  third  proportional 
to  that  diameter  and  its  conjugate,  in  the  ellipse  and  hyper- 
bola, and  to  one  absciss  and  its  ordinate  in  the  parabola. 

17.  The  Focus  is  the  point  in  the  axis  where  the  ordinate 
is  equal  to  half  the  parameter.  As  k  and  l,  where  dk  or  el 
is  equal  to  the  semi -parameter.  The  name  focus  being  given 
to  this  point  from  the  peculiar  property  of  it  mentioned  in  the 
corol.  to  thcor.  5*  in  the  Ellipse  and  Hyperbola  following,  and 
to  theor.  0  in  the  Parabola. 

Hence,  the  ellipse  and  hyperbola  have  each  two  foci ;  but 
the  parabola  only  one. 


18.  If  t)al,  fhg,  be  two  opposite  hyperbolas,  having  as 
for  their  first  or  transverse  axis,  and  ab  for  their  second  or 
conjugate  axis.  And  if  dm,  fbg,  be  two  other  opposite  hy. 
pcrbolns  having  the  same  axes,  hut  in  the  contrary  order, 
namely,  ab  their  fatal  txxvs,  *iA  »  tat\t  n*»wA\  vWwvlvfiee 


DEFINXTIOXS* 


475 


two  latter  curves  d*e,  fbg,  are  called  the  conjugate  hyper- 
bolas to  the  two  former  dae,  pro  ;  and  each  pair  of  opposite 
curves  mutually  conjugate  to  the  other ;  being  all  for  con- 
venience of  investigation  referred  to  one  plane,  though  they 
are  only  posited  two  and  two  in  one  plane ;  as  will  appear 
more  evidently  from  the  demonstration  of  th.  2.  Hyperbola. 

19.  And  if  tangents  be  drawn  to  the  four  vertices  of  the 
^curves,  or  extremities  of  the  axes,  forming  the  inscribed 
rectangle  iiikl  ;  the  diagonals  hck,  icl,  of  this  rectangle, 
are  called  the  asymptotes  of  the  curves.  And  if  these  lfamp. 
totes  intersect  at  right  angles,  or  the  inscribed  rectangle  be 
a  square,  or  the  two  axes  ab  and  ab  be  equal,  then  the  hy- 
berbolas  are  said  to  be  right-angled,  or  equilateral. 


SCHOLIUM. 


The  rectangle  inscribed  between  the  four  conjugate  hy- 
perbolas, is  similar  to  a  rectangle  circumscribed  about  an 
ellipse,  by  drawing  tangents  in  like  manner,  to  the  four  ex. 
tremities  of  the  two  axes  ;  and  the  asymptotes  or  diagonals 
in  the  hyperbola,  arc  analogous  to  those  in  the  ellipse,  cut- 
ting this  curve  in  similar  points,  and  making  that  pair  of 
conjugate  diameters  which  arc  equal  to  each  other.  Also, 
the  whole  figure  formed  by  the  four  hyperbolas,  is  as  it 
were,  an  ellipse  turned  inside  out,  cut  open  at  the  extre. 
mi  tics,  d,  e,  f,  g,  of  the  said  equal  conjugate  diameters,  and 
those  four  points  drawn  out  to  an  infinite  distance  ;  the  cur. 
vature  being  turned  the  contrary  way,  but  the  axes,  and  the 
rectangle  passing  through  their  extremities,  continuing  fixed. 

And  further,  if  there  be  four  cones 
cscrf,  cop,  cmp,  cno,  having  all  the 
same  vertex  c,  and  all  their  axes  in  the 
same  plane,  and  their  sides  touching  or 
coinciding  in  the  common  intersecting 
lines  mco,  ncv  ;  then  if  these  four 
cones  be  all  cut  by  one  plane,  parallel 
to  the  common  plane  of  their  axes,  there 
will  be  formed  the  four  hyperbolas,  gqr, 
fst,  vkl,  win,  of  which  each  two  op- 
po8itesare  equal ;  and  each  pair  resembles 
the  conjugates  to  the  other  two,  as  here 
in  the  annexed  figure ;  but  they  are  not 
accurately  the  conjugates,  except  only 
when  the  four  cones  are  all  equal,  and 
then  the  four  hyperbolic  sections  are  all  equal  also. 


[  476  ] 


OF  THE  EIJJPSE. 

THEOREM  X. 

The  Squares  of  the  Ordinntes  of  the  Axis  are  to  each  other 
as  the  Rectangles  of  their  Abscisses. 

Let  avb  be  a  plane  passing  through 
the  apju  of  the  cone  ;  agiii  another 
section  of  the  cone  perpendicular  to 
the  plane  of  the  former  ;  ab  the  axis 
of  this  elliptic  section  ;  and  fg,  hi,  or- 
dimftes  perpendicular  to  it.  Then  it 
will  be,  as  fg3  :  hi3  : :  af  .  eb  :  ah  .  iib. 

For,  through  the  ordinates  fg,  hi, 
draw  the  circular  sections  xgl,  min, 
parallel^  to  the  base  of  the  cone,  having  kl,  mn,  for  their 
diameters,  to  which  fg,  hi,  are  ordinate,  as  will  as  to  the 
axis  of  the  ellipse. 

Now,  by  the  similar  trangles  afl,  ahn,  and  bfk,  bhh, 

it  is  AF  l  AH  *     FL  :  UN, 

and  fb  :  iib  : ;  kf  :  mu  ; 

hence,  taking  the  rectangles  of  the  corresponding  terms, 
it  is,  the  rect.  af  .  fb  :  ah  .  hb  : :  kf  .  fl  :  mu  .  iin. 

But,  by  the  circle,  kf  .  fl  =  f.;8,  and  mh  .  hn  =  hi9  ; 
Therefore  the  rect.  af  .  fb  :  ah  .  hb  : :  fg8  :  hi*,    q.  e.  d. 


^  THEOREM  II. 

As  the  Square  of  the  Transverse  Axis 
Is  to  the  Square  of  the  Conjugate  : 
So  is  the  Rectangle  of  the  Abscisses 
To  the  Square  of  their  Ordinate. 


ft 

For,  by  theor.  1,  ac  .  cb  :  ad  .  db  :  :  c«9  :  de*  ; 
But,  if  c  be  the  centre,  then  ac.cbs  ac1,  and  ca  is  the 
semi-conjugate. 


OF  TBS  SLUMS.  477 

Therefore  ac9  :  ad  •  db  : :  ac*  :  db9; 

or,  by  permutation,  ac9  :  ac9  :  :  ad  •  db  :  de9  ; 
or,  by  doubling,      abs  :  ab*  :  :  ad  .  db  :  db1.    a.  s.  d. 

Cord.  Or.  by  div.  ab  :  —  :  :  ad  .  db  or  ca9  —  cd9  :  db1. 

'  ab 

that  is,  ab  :  p  :  :  ad  .  db  or  ca9  —  CD9 :  db9  ; 

where  p  is  the  parameter^-,  by  the  definition  of  it. 

That  is,  As  the  transverse,  9 
Is  to  its  parameter, 
So  is  the  rectangle  of  the  abscisses, 
To  the  square  of  their  ordinate. 

THEOREM  III. 

As  the  Square  of  the  Conjugate  Axis 

Is  to  the  Square  of  the  Transverse  Axis, 

So  is  the  Rectangle  of  the  Abscisses  wf  the  Conjugate,  or 
the  difference  of  the  Squares  of  the  Semi-conjugate  and 
Distance  of  the  centre  from  any  Ordinate  of  that  Axis, 

To  the  Square  of  the  Ordinate. 


That  is, 
cb9  :  :  ad .  db  or  ca9—  cd1 : 


For,  draw  the  ordinate  ed  to  the  transversa  ab. 
Then,  by  theor.  1,  ca9  :  ca1  :  :  de1  :  ad  .*bb  or  ca1  —  cd*, 

or  ca9  :  ca9  :  :  cd*  :  ca9  —  cJe9, 

But  ca9  :  ca9  :  :  ca9 :  ca9, 

theref.  by  subtr.  ca9 :  ca9  : :  ca9  —  cd1  or  ad  .db  :  da9. 

Q.  E.  D. 

Carol.  1.  If  two  circles  be  described  on  the  two  axes  as 
diameters,  the  one  inscribed  within  the  ellipse,  and  the  other 
circumscribed  about  it ;  (hen  an  ordinate  in  the  circle  will 
be  to  the  corresponding  ordinate  in  the  ellipse,  as  the  axis  of 
this  ordinate,  is  to  the  other  axis. 

That  is,  ca  :  ca  :  :  dg  :  de, 
and  ca  :  ca     dg  :  dz. 
For,  by  the  nature  of  the  circle,  ad  •  db  =  dg*  ;  theref. 
by  the  nature  of  the  ellipse,  ca9  :  ca9 :  :  ad  •  db  or  do*  :  de9, 
or  ca  :  ca  ; :  iw  \  iv* 


conic  SBCTIOKt. 


In  like  manner      .       ca  :  ca  :  :  dg  :  o*e. 
Also,  by  equality    -       dg  :  de  or  <:d  :  :  o*e  or  tc  2  dg. 
Therefore  ego  is  a  continued  straight  line. 

Corel.  2.  Hence  also,  as  the  ellipse  and  circle  are  made  up 
of  the  same  number  of  corresponding  ordinates,  which  are 
all  in  the  same  proportion  of  the  two  axes,  it  follows  that 
the  areas  of  the  whole  circle  and  ellipse,  as  also  of  any  like 
parts  of  them,  are'  in  the  same  proportion  of  the  two  axes, 
or  as  tfcfe  square  of  the  diameter  to  the  rectangle  of  the  two 
axes ;  that  is,  the  areas  of  the  two  circles,  and  of  the  ellipse, 
are  as  the  square  of  each  axis  and  the  rectangle  of  the  two ; 
and  therefore  the  ellipse  is  a  mean  proportional  between  the 
two  circles. 

THEOREM  IV. 

The  Square  of  the  Distance  of  the  Focus  from  the  Centre, 
is  equal  to  the  Difference  of  the  Squares  of  the  Semi- 
axes. 

Or,  the  square  of  the  Distance  between  the  Foci,  is  equal  to 
the  Difference  of  the  Squares  of  the  two  Axes. 


That  is,  cf9  =  ca8  -  ca* 
or  f/j  =  ab1  —  a6J 

b 

For,  to  the  focus  f  draw  the  ordinate  fe  ;  which,  by  the 
definition,  will  be  the  semi  parameter.    Then,  by  the  nature 
of  the  curve       -        -       ca8  :  ca1 : :  ca2  -  of*  :  Ft* ; 
and  by  the  def.  of  the  para,  ca8  :  ca2  :  :  ca8  :  fk2  ; 
therefore  -       .       c/ia  =  ca2  -  cr2 ;  ♦ 

and  by  addit.  nnd  subtr.       cf2  =  ca2  —  ca'; 
or,  by  doubling,  •       rf2  =  ab3  —  ab*.    q.  e.  p. 

Carol.  1.  The  two  semi-axes,  nnd  the  focal  distance  from 
the  centre,  are  the  sides  of  a  right. angled  triangle  era  ;  and 
the  distance  Fa  from  the  focus  to  the  extremity  of  the  con- 
jugate axis,  is  =  ac  the  semi-transverse. 

Carol.  2.  The  conjugate  semi-axis  ca  is  a  mean  proper, 
ttonal  between  af,  fb,  or  between  a/*, /b,  the  distances  of 
either  focus  from  the  two  vertices. 

For  co"  =  ca?  —  cf*  =■  Vsfc-  "V  ^  •      — w \  =  af  .  fb. 


Or  THE  ELLIPSE. 


THEOREM  V. 


x  The  Sum  of  two  lines  drawn  from  the  two  Foci  to  meet  , 
at  any  Point  in  the  Curve,  is  equal  to  the  Transverse 
Axis. 


For,  draw  ag  parallel  and  equal  to  ca  the  semi-conjugate ; 
and  join  cg  meeting  the  ordinate  de  in  h  ;  also  take  ci  a 
4th  proportional  to  ca,  cf,  cd. 
Then  by  theor.  2,  ca8  :  ag2  :  :  ca3  —  cd3  :  de3; 
and,  by  sim.  tri.    ca2  :  ag3  :  :  ca3  —  cd3  :  ag8  —  dh*  ; 
consequently        de3  =  ag3  —  du2  =  ca3  —  dh3. 
Also,  fd  =  cf  ^  cd,  and  fd2  =  cf2  —  2of  .  cd  +  cd3  ; 
And,  by  right-angled  triangles,  fe3  =  fd3  +  de2  ; 
therefore  fe2  =  cf2  +  ca2  —  2cf  .  cd  +  cd2  —  dh3  ; 
But  by  theor.  4,  cf3  +  ca3  =  ca2,  % 
and  by  supposition,  2cf  .  cd  =  2ca  •  ci ; 
theref.  fe3  =  ca3  —  2ca  .  ci  +  cd3  —  dh3. 
Again,  by  supp.  ca3  :  cd3  :  :  cf3  or  ca3  —  ag3  :  cr ; 
and,  by  sim.  tri.  ca3  :  cd8  :  :  ca3  —  ag3  :  cd3  —  dh3  ; 
therefore    •     ci3  =  cd3 — dh8; 
consequently     fe2  =■=  ca3  —  2ca  .  ci  +  cr*. 
And  the  root  or  side  of  this  square  is  fe  =  ca  —  ci  =  ai. 
In  the  same  manner  it  is  found  that fz  =  ca  +  ci  =  bi. 
Conseq.  by  addit.  fe  +  ft  =  ai  +  bi  =  ab.    q.  k.  d. 

Cord.  1.  Hence  ci  or  ca  —  fe  is  a  4th  proportional  to 
ca,  cr,  CD. 

Coral.  2.  And  /e  — fe  =  2ci ;  that  is,  the  difference  be* 
tween  two  lines  drawn  from  the  foci,  to  any  point  in  the 
curve,  is  dquble  the  4th  proportional  to  ca,  cf,  cd. 

CoroL  3.  Hence  is  derived  the  common  method  of  de- 
scribing this  curve  mechanically  by  points,  or  with  a  thread, 
thus: 


480 


come  accnoxi. 


In  the  transverse  take  the  foci  f,/, 
mod  any  point  i.  Then  with  the  radii 
ai,  bi,  and  centres  r,/,  describe  arcs 
intersecting  in  b,  which  will  be  a 
point  in  the  curve.  In  like  manner, 
assuming  other  points  i,  as  many 
other  points  will  be  found  in  the 
curve.  Then  with  a  steady  hand, 
the  curve  line  may  be  drawn  through  all  the  points  of  inter- 
section E. 

Or,  take  a  thread  of  the  length  ab  of  the  transverse  axis, 
and  fix  its  two  ends  in  the  foci  f,  /,  by  two  pins.  Then 
carry  a  pen  or  pencil  round  by  the  thread,  keeping  it  always 
stretched,  and  its  point  will  trace  out  the  curve  line. 


THEOREM  VI. 

If  from  any  Point  i  in  the  Axis  produced,  a  Line  il  be 
drawn  touching  the  Curve  in  one  Point  l  ;  and  the  Or- 
dinate lh  be  drawn ;  and  if  c  be  the  Centre  or  Middle 
of  ab  :  Then  shall  cm  be  to  ci  as  the  Square  of  am  to  the 
Square  of  ai. 


cm  : 


For,  from  the  point  i  draw  any  other  line  if.h  to  cut  the 
curve  in  two  points  is  and  h  ;  from  which  let  fall  the  perpen- 
diculars ed  and  hg  ;  and  bisect  do  in  k. 

Then,  by  theor.  1,  ad  .  db  :  ag  .  gb  :  :  de2  :  gh9, 
and  by  sim.  triangles,  id*  :  ig3  :  :  de9  :  gh9  ; 
there f.  by  equality,  ad  .  db  :  ag  .  gb  :  :  id*  :  ig*. 

But  DB  =  CB  +  CD  =  AC  +  I'D  —  AG  +  DC  CG  =  2cE  +  AG, 

and  GB  =  CB  CG  =  AC  CG  =  AD+  DC  —  CG  =  2cK  +  AD  5 

theref.  ad  .  2ck  +  ad  .  ag  :  ag  .  2c k  +  ad  .  ag  :  :  id*  : 
and,  by  div.  dg  .  2ck  :  ig8  —  id2  or  dg  .  2ik  :  :  ad  .  2ck  + 

AD  .  AG  :  IDa, 

or       2ck  :  2ik  :  :  ad  .  2ck  +  ad  .  ag  :  id', 
or  ad  .  2ck  :  ad  .  2ik  :  :  ad  .  2ck  +  ad  .  ag  :  id9  ; 
theref.  by  div.  ck  :  ik  :  :  ad  •  ag  :  id'  —  ad  .  2ik, 
and,  by  corop.  ck  :  ic  :  :  ad  .  ag  :  id9  —  ad  .  id  +  ia9 
or        -        ck  :  ci  :  :  ad  .  ag  :  ai9. 


OF  THE  ELLIPSE. 


481 


But,  when  the  line  ih,  by  revolving  about  the  point  i, 
comes  into  the  position  of  the  tangent  il,  then  the  points  e 
and  ii  meet  in  the  point  l,  and  the  points  d,  k,  g,  coincide 
with  the  point  m  ;  and  then  the  last  proportion  becomes 
cm  :  ci :  :  am3  :  ais.    q.  e.  d. 

THEOREM  VII. 

If  a  Tangent  and  Ordinate  be  drawn  from  any  Point  in  the 
Curve,  meeting  the  Transverse  Axis  ;  the  Semi -transverse 
will  be  a  Mean  Proportional  between  the  Distances  of  the 
said  two  Intersections  from  the  Centre. 

That  is, 

ca  is  a  mean  proportional 
between  cd  and  or  ; 

or  cd,  ca,  cr,  are  con- 
tinued proportionals. 


For.  by  tlieor.  G,  cd  :  ct  :  :  ad9  :  at2 
that  is,  cd  :  ct  :  :  (ca  —  co)a :  (ct  —  ca)3, 
or   -    cd  :  ct  :  :  cd3  +  CAa  :  ca9  +  ct1, 
and  -    cd  :  dt  :  :  cd3  +  ca9  :  ct9  —  cd9, 
or    -    cd  :  dt  :  :  cd!  +  ca2  :  (ct  +  cd)dt, 
or   -    cd9:  cd  .  dt  :  :  cd*  +  ca2 :  (cd  .  dt)  -f-  (ct  .  dt), 
hence  cd2:  ca9  :  :  cd  .  dt  :  ct  .  dt, 
and  -    cd':  caj  :  :  cd  :  ct. 

therefore  (t^.  78,  Geora.)  cd  :  ca  :  :  ca  :  ct.    q.  e.  d. 

Cord.  1.  Since  cr  is  always  a  third  proportional  to  cd, 
ca  ;  if  the  points  d,  a,  remain  constant,  then  will  the.  point 
T  be  constant  also  ;  nnd  therefore  all  the  tangents  will  meet 
in  this  point  t,  which  are  drawn  from  the  point  e,  of  every 
ellipse  described  on  the  same  axis  ar,  where  they  are  cut  by 
the  common  ordinate  def  drawn  from  the  point  d. 

Cord.  2.  When  the  outer  ellipse,  by  enlarging,  becomes 
a  circle,  as  at  the  upper  figure  at  e,  then  by  drawing  et 
perp.  to  ce,  and  joining  t  to  the  lower  e,  the  tangent  to  the 
point  e  at  the  ellipse  is  obtained. 

theorem  viii. 

If  there  be  any  Tangent  meeting  four  Perpendiculars  to  the 
Axis  drawn  from  these  four  Points,  namely,  the  Centre,  the 
two  Extremities  of  the  Axis,  and  the  Point  of  Contact ; 
those  four  Perpendiculars  will  be  Proportions. 
Vol.  I.  62 


488 


COKIC  SKCTIOM* 


That  is, 
AO  :  de  :  :  ch  :  bi. 


For,  by  theor.  7,  tc  :  ac  :  :  ac  :  dc, 
theref.  by  div.       ta  :  ad  :  :  tc  :  ac  or  cb, 
and  by  comp.        ta  :  td  :  :  tc  :  th, 
and  by  sim.  tri.      ao  :  de  :  :  cn  :  hi.    q.  E.  D. 

Cord.  1.  Hence  ta,  td,  tc,  tb  )  ^  .  , 

and       TG,  TB,  TH,  TI  \  *">  P~pOrtM»^ 

Fur  these  are  as  ao,  dr,  ch,  bi,  by  similar  triangles. 

Corel.  2.  Draw  ai  to  bisect  de  in  p  ;  then  since 
ta  :  te  :  :  tc  :  ti,  the  triangles  tab,  tci  are  similar,  as  well 
as  the  triangles  aed,  cbi,  and  adp,  abi. 
Hence    -    ad  :  dk  :  :  cb  :  bi 
and        -    ad  :  dp  :  :  ab  :  bi 

.\  de  :  dp  :  :  ab  :  cb  :  :  2  :  1  ;  which  sug- 
gests another  simple  practical  method  of  drawing  a  tangent 
to  an  ellipse. 


theorem  ix. 


If  there  be  any  Tangent,  and  two  Lines  drawn  from  the 
Foci  to  the  Point  of  Contact ;  these  two  lines  will  make 
equal  Angles  with  the  Tangent. 


That  is, 
the  JL  vet  =  L  fve. 


For,  draw  the  ordinate  dk  and /a  parallel  to  fe. 
By  cor.  1 ,  theor.  5,  ca  :  cd  :  :  cf  :  ca  —  fk, 
and  by  theor.  7,      ca  :  cd  :  :  ct  :  ca  ; 
therefore  ct  :  cf  :  :  ca  :  ca  —  fe  ; 

and  by  add.  and  sub.TF  :  rf :  :  fe  :  2ca— fe  or /e  by  th.  5. 
But  by  sim.  tri.       tf  :  rf :  :  re  :fe  ; 
therefore      ft:  —  fe>  and  conseq.         =  /.foe. 
But  because  fe  is  parallel  to  fe,  the      k  ^fet  ; 
therefore       ^.fet  =  Lfot.    q.  e.  d. 


Or  TUB  ILLIP8X 


488 


Cord.  As  opticians  find  that  the  angle  of  incidence  is  equal 
to  the  angle  of  reflection,  it  appears  from  this  theorem,  that 
rays  of  Tight  issuing  from  the  one  focus,  and  meeting  the 
curve  in  every  point,  will  be  reflected  into  lines  drawn  from 
those  points  to  the  other  focus.  So  the  ray  fn  is  reflected 
into  fe.  And  this  is  the  reuson  why  the  points  f,/,  ure  call- 
ed the  foci,  or  burning  points. 

theorex  x. 

All  the  Parallelograms  circumscribed  about  an  Ellipse  are 
equal  to  one  another,  and  each  equal  to  the  Reclaugle  of 
the  two  Axes. 


That  is, 
the  parallelogram  pqrs 
the  rectangle  ab  •  ab. 


S 

Let' kg,  egy  be  two  conjugate  diameters  parallel  to  the 
aides  of  the  parallelogram,  and  dividing  it  into  four  less  and 
equal  parallelograms.  Also,  draw  the  ordinate*  i>k,  de,  and 
ck  perpendicular  to  pq;  and  let  the  axis  c.\  produced  meet 
the  sides  of  the  parallelogram,  produced  if  uecessury,  in  t 
and  t. 

Then,  by  theor.  7,     ct  :  ca  : :  ca  :  cd, 

and       -        -        c/  :  ca  : :  ca  :  erf ; 

theref.  by  equality,    err  :  ct  : :  cd  :  cd  ; 

but,  by  sim.  triangles,  ct  :  ct  : :  td  :  cd, 

theref.  by  equality,    td  :  cd  : :  cd  :  cd, 

and  the  rectangle      td  .  dc  =  is  the  square  cd\ 

Again,  by  theor.  7,    cd  :  ca  : :  ca  :  ct, 

or,  by  division,  cd  :  ca  : :  da  :  at, 

and  by  composition,  cd  :  db  : :  ad  :  dt  ; 

conseq.  the  rectangle  cd  .  dt  =  cd9  =*  ad  .  dh*. 

But,  by  theor.  1,       ca*:  ca*::  (ad  .  db  or)  cd* :  de?, 

therefore       -         ca  :  ca  . :  cd  :  dk  ; 

or       -       -       -    ca  i  dk  : :  ca  :  cd ; 

By  th.  7,        -        ct  :  ca  :  :  ca  :  ca\ 


*  Cord.  Bet-nil <«  cd1  =  ad  .  ns  —  ca^  —  «d", 

therefore  ca*  =  cd1  ~f-  cH* . 
In  like  manner,  c«J  =  ss'-f  *V. 


484 


oohic  tactions 


by  equality 
by  sim.  tri. 
theref.  by  equality, 
But,  by  trim.  tri. 
theref.  by  equality, 
and  the  rectangle 
But  the  reet. 
theref.  the  rect. 
conseq.  the  rect. 


ct  :  ca  :  :  ca  :  db, 

ct  :  ct  :  :  de  :  de, 

ct  :  ca  :  ;  ca  :  de. 

ct :  ck  :  :  ce  :  de; 

cr  :  ca  :  :  ca  :  ce, 

ck  •  ce  ~  ca  .  ca. 

ck  .  ce  =  the  parallelogram  cbp*, 

ca  •  c<i  —  the  parnllelograra  cbic, 

ab  •  ab  ~  the  parallelogram  pqrb-  q.e*d. 


THEOREM  XX. 


The  Sum  of  the  Squares  of  every  Pair  of  Conjugate  Diame- 
ters, is  equal  to  the  same  constant  Quantity,  namely,  the 
Sum  of  the  Squares  of  the  two  Axes. 


That  is, 
ab*  +  a&*  =  eo8  +  eg9 ; 
where  eo,  eg,  are  any  pair  of  con- 
jugate  diameters. 


For,  draw  the  ordinates  ed,  edy 
Then,  by  cor.  to  Theor.  10,  ca3  =  cir  +  cd\ 
and        -        -        -        co9  =  de'  4-  de1 ; 
therefore  the  sum       ca8  +  va1  =  cd2  +  dk*  +  cd?  +  de*. 
But,  by  right-angled  as,     ce51  =  cna  4-  de', 
and  ce2  =  cd3  +  de1 ; 

therefore  the  sum        t  e2  4-  cc2  =  cn2  +  de2  +  cd1  +  de1. 
consequently      -        ca2  +  ca2     ce2  +  ce* ; 
or,  by  doubling,  ab2  +  ab2  =  kg5  +  eg9.       q.  b.  d. 


THEOREM  XII, 


The  difference  between  the  semi -transverse  and  a  line  drawn 
from  the. focus  to  any  point  in  the  curve,  is  equal  to  a 
fourth  proportional  to  the  semi -transverse,  the  dixtnnce 
from  the  centre  to  the  focus,  and  the  distance  from  the 
centre  to  the  ordinate  belonging  to  that  point  of  the 
curve. 


OF  trs  uunii 


485 


That  is, 
ac  —  fe  =■  ci,  or  fe  =  ai  ; 
and/is  —  ac     ci,  or /k  =  bi. 
Where  ca  :  cf  :  :  cd  :  ci  the  4th 
proportional  to  ca,  cf,  cd. 


For,  draw  ao  parallel  and  equal  to  ca  the  semi-conjugate  ; 
and  join  co  meeting  the  ordinate  de  in  h. 
Then,  by  theor.  2,  ca2  :  ah2  : :  ca"  -  cd2  :  dr2: 
and,  by  sim.  tri.  ca9  :  ao*  :  :  ca*  —  cd2  :  ^oa  —  dh"  ; 
consequently    dk2»aoj-dh*=oi*— dh*. 
Also   -   fd=cf^-cd,  end  fd^cf2— 2cf  .  cd+cd2  ; 
but  by  right-angled  triangles,  fd'+dk^fk2  ; 
therefore    -    FK^ci^+ca2— 2cf  .  cd+cd2— du1. 
But  by  theor.  4,  ca,+CFa=CA*; 
and,  by  supposition,  2cf  .  cd=2ca  .  ci ; 
therefore    -      -       fb2=ca2— 2c a  .  ci+cd2— do1. 
But  by  supposition,  ca2  :  cd'  : :  cf8  or  ca2— ag2  :  cta. 
and,  by  sim.  tri.      ca2  :  cna  : 
therefore    -     -    ci^cd2  —  nna ; 
consequently     -    fe9«»ca2  —  2ca  .  ci  +  cr2. 
And  the  root  or  side  of  this  square  is  fe  =-=  ca  —  ci  =  ax. 
In  the  same  manner  is  found /e=  ca+ci=bi.       q.  v.  d. 

Carol.  1.    Hence  ci  or  ca  —  fe  is  a  4th  proportional  to 

CA,  CF,  CD. 

Carol.  2.  And  fp.  —  fe  =■  2ci  ;  that  is,  the  diffi  rence 
between  two  lines  draw  from  the  foci,  to  any  point  in  the 
curve,  is  double  the  4th  proportional  to  ca,  cf,  cd. 


:  ca2— ao2  :  cd2— dh2; 


THEOREM  XIII. 


If  a  line  be  drawn  from  either  focus,  perpendicular  to  a  tan- 
gent to  any  point  of  the  curve ;  the  distance  of  their  inter- 
sections  from  the  centre  will  be  equal  to  the  semi-transverse 
axis. 


That  is,  if  fp, 
fp,  be  perpendi- 
cular to  the  tan- 
gent T17?,  then 
shall  cp  and  cp 
be  each  equal  to 
ca  or  CB. 


486 


come  SECTIONS. 


For  through  the  point  of  contact  e  draw  rs,  and  /* 
meeting  fp  produced  in  o.  Then  the  L  gkp  =  ^  pep, 
being  each  equal  to  the  L  f&pt  and  the  angles  at  p  being 
right,  and  the  side  pk  being  common,  the  two  triangles  gep, 
fep  are  equal  in  all  respects,  and  woe  =  fe,  and  gp  =  fp. 
Therefore,  since  fp  =  £fg,  and  fc  =  \rf,  and  the  angle  at 
f  common,  the  side  cp  will  be  -=  £/b  or  J  ab,  that  is  cp  =  ca 
*©r  cb.    And  in  the  same  manner  cp  =  cx  or  cb.      o>  e.  v. 

Card.  1.  A  circle  described  on  the  transverse  axis,  as  a 
diameter,  will  pasc  through  the  points  p,  p  ;  because  all  the 
lines  ca,  cp,  cp9  cb,  being  equal,  will  be  radii  of  the  circle. 

Cord.  2.   cp  is  parallel  to /e,  and  cp  parallel  to  fb. 

Cord.  8.  If  at  the  intersections  of  any  tangent,  with  the 
circumscribed  circle,  perpendiculars  to  the  tangent  be  drawn, 
they  will  meet  the  transverse  axis  in  the  two  foci.  That  is, 
the  perpendiculars  pf,  pf  give  the  foci  ryf, 

THEOREU  XIV. 

The  equal  ordi nates,  or  the  ordi nates  at  equal  distances 
from  the  centre,  on  the  opposite  sides  and  ends  of  aa 
ellipse,  have  their  extremities  connected  by  one  right  line 
passing  through  the  centre,  and  thut  line  is  bisected  by 
the  centre. 

That  is,  if  cd  =  r«,  or  the  ordinate  de  =  gii  ; 
then  shall  cr  =  ch,  and  k<;ii  will  be  a  right  line. 


For  when  cd  =  cg,  then  also  is  de  =  on  by  cor.  2,  th.  1. 
But  the  L  d  =r  ^  «,  being  both  right  angles  ; 
therefore  the  third  side  ce  =  en,  and  the  /  dce  =  ^.gcb, 
and  consequently  ech  is  a  right  line. 

Coroh  1.  And,  conversely,  if  ecu  be  a  right  line  passing 
through  the  centre  ;  then  shall  it  he  bisected  by  the  centre, 
or  have  ce  —  ch  ;  also  de  will  be  =  oh,  and  cd  =  co. 


OF  TU  SLUMS.  487 

Carol.  2.  Hence  also,  if  two  tangents  be  drawn  to  the  two 
ends  b,  h  of  any  diameter  eh  ;  they  will  be  parallel  to  each  > 
other,  and  will  cut  the  axis  at  equal  angles,  and  at  equal 
distances  from  the  centre.  For,  the  two  cd,  ca  being  equal 
to  the  two  co,  cb,  the  third  proportionals  <t,  cs  will  be 
equal  also  ;  then  the  two  sides  ce,  ct  being  equal  to  the  two 
ch,  cs,  and  the  included  angle  ect  equal  to  the  included 
angle  bcs,  all  the  other  corresponding  parts  are  equal :  and^ 
so  the  L  t  =  L  s,  and  te  parallel  to  ns. 

Carol.  3.  And  hence  the  four  tangents,  at  the  four  extre- 
mities of  any  two  conjugate  diameters,  form  a  parallelogram 
circumscribing  the  ellipse,  and  the  pairs  of  opposite  sides  are 
each  equal  to  the  corresponding  parallel  conjugate  diameters. 
For,  if  the  diameter  eh  be  drawn  parallel  to  the  tangent  ts 
or  hs,  it  will  be  the  conjugate  to  eh  by  the  definition  ;  and 
the  tangents  to  e,  k  will  be  parallel  to  each  other,  and  to  the 
diameter  eh  for  the  same  reason. 


THEOREX  XV. 

If  two  ordinates  ed,  ed  be  drawn  from  the  extremities  e,  e, 
of  two  conjugate  diameters,  and  tangents  be  drawn  to 
the  same  extremities,  and  meeting  the  axis  produced  in 
t  and  r; 

Then  shall  cd  be  a  mean  proportional  between  cd,  da,  and 
cd  a  mean  proportional  between  cd,  dt. 


For,  by  theor.  7,  cd  :  ca  : 

and  by  the  same,  cd  :  ca  i 

theref.  by  equality,  cd  :  cd  : 

But,  by  sim.  tri.  dt  :  cd 

theref.  by  equality,  cd  :  cd 

In  like  manner,  cd :  cd  : 

Corel.  1.  Hence  cd  :  cd  : :  cs  :  ct. 


:  ca  :  ct, 
:  <:a  :  cn  ; 
:  cr  :  ct, 
:  ct  :  cb; 
:  cd :  dt. 
:  cd  :  da.  a. 


s.  p. 


488 


come  lECTiom. 


«   Carol.  2.  Hence  also  cd  :  erf  :  :  de  :  de. 

And  the  rectangle  cd.de  =  erf  .  rff ,  or  A  cdb  =  a  ede. 

Corof.  8.  Also  WJ  =  cd  .  dt, 
and  cd*  ■=  cd  .  rfa, 

Or  erf  a  mean  proportional  between  cd,  dt  ; 
and  cd  a  mean  proportional  between  cdy  da. 

P  THEOREM  XVI. 

TTie  name  figure  being  constructed  as  in  the  last  theorem, 
each  ordinate  will  divide  the  axis,  and  the  semi-axis  added 
to  the  external  part,  in  the  same  ratio. 

[See  the  last  fig.] 

That  if»,  da  :  dt  :  :  dc  :  db, 
and  dx  :  rfa  :  :  dc  :  rfn. 
For,  by  Theor.  7,  cd  :  ca  :  :  ca  :  ct, 
and  by  div.  en  :  ca  :  :  ad  :  at, 
and  by  com  p.  cd  :  db  :  :  ad  :  dt, 
or,  -  -  -  da  :  dt  :  :  dc  :  db. 
In  like  manner,    o*a  :  rfa  :  :  rfc  :  ds. 


a.  e.  D. 


Corol.  \.  Hence,  and  from  cor.  3  to  the  last,  it  is, 


cd1  =  CD  . 
cd3  =  cd 


DT  =  AD 
rf*R  =  Ad  , 


DB  =  CAa  —  CD*. 


ds  =  CA8 


crf\ 


Corol.  2.  Hence  also,  ca2  =  cd2  +  cd2, 
and  ca3  =  de*  +  de*. 

Corol.  3.  Further,  because  ca2  :  ca1  :  :  ad  .  db  or  erf2 :  de*, 
therefore  ca  :  ca  :  :  erf  :  de, 
likewise  ca  :  ca  :  :  cd  :  rfe. 

THEOREM  XVII. 


If  from  any  point  in  the  curve  there  be  drawn  an  ordinate, 
and  a  perpendicular  to  the  curve,  or  to  the  tangent  at  that 
point :  then,  the 

Dist.  on  the  trans,  between  the  centre  and  ordinate,  cd, 
Will  be  to  the  dist.  pd,  ™  "> 

As  sq.  of  the  trans,  axis 
To  sq.  of  the  conjugate. 


EL 


ca"  :  ca' 


That  is, 
:  :  dc  :  dp. 


D  P  C 


For,  by  theor.  %  ca?  ;  ccr  *.   kt>  *  to 


• 


OF  THE  ELLIPSE. 


489 


But,  by  rt.  angled  As,  the  rect.  td  .  dp-=pes  ;  V 
and,  by  cor.  1,  theor.  16,  cd  •  dt=ad  .  db  ; 

therefore    -    -    -  ca2  :  ca' :  :  td  .  dc  :  td  .  dp, 
or    -    -    -    -    -  ac2  :  ca3  :  :  dc        :  dp.    q.  e.  d. 


THEOREM.  XVIII. 


If  there  be  two  tangents  drawn,  the  one  to  the  extremity**- 

of  the  transverse,  and  the  other  to  the  extremity  of  any^^ 
other  diameter,  each  meeting  the  other's  diameter  pro- 
duced ;  the  two  tangential  triangles  so  formed,  will  be 
equal. 


For,  draw  the  ordinate  de.    Then  # 
By  sim.  triangles,  cd  :  ca  :  :  ce  :  cn  ; 
but,  by  theor.  7,    cd  :  ca  :  :  ca  :  ct  ; 
the  re  f.  by  equal,  ca  :  ct  :  :  ce  :  ex. 

The  two  triangles  crt,  can,  have  then  the  angle  c  common, 
and  the  sides  about  that  angle  reciprocally  proportional ;  those 
triangles  are  therefore  equal,  namely,  the  a  cet  =  a  can. 
Cord.  1.  From  each  of  the  equal  tri.  cet,  can, 
take  the  common  space  cape, 
and  there  remains  the  external  A  pat  =  apne. 
Corel.  2.  Also  from  the  equal  triangles  cet,  can, 
take  the  common  triangle  ced, 
and  there  remains  the  A  ted  =  trapez.  aned. 


The  same  being  supposed  as  in  the  last  proposition  ;  then  any 
lines  kq,  qg,  drawn  parallel  to  the  two  tangents,  shall 
also  cut  off  equal  spaces.    That  is, 


That  is, 
the  triangle  cET=the 
triangle  can. 


theorem  xix. 


Vol.  I. 


68 


For,  draw  the  ordinate   pb.  Then 
the  three  aim.  triangles  can,  cde,  cgh, 
are  to  each  other  as       ca*,  cd1,  cgs  ; 
th.  by  div.  the  trap,  aned  :  trap,  anhg  : :  ca2— cd*  :  caj— ce*. 
But,  by  theor.  1,       de8  :  oq9  : :  cas— cd*  :  ca2— cc1. 

theref.  by  equ.  trap,  aned  :  trap,  anhg  :  :  de*        :  oq*. 
But,  by8im.  As,  tri.  ted  :  tri.    kqo    : :  de*        :  gq\ 
theref  by  equality,  ankp  :        ted    : :  anho     :  kqc. 
But,  by  cor.  2,  theor.  18,  the  trap,  aned  =  A  ted; 
and  therefore  the  trap,    anho  ="  A  kqg. 
In  like  manner  the  trap.  anA#=  AKgg.    o.  e.  d. 
Carol.  1.  The  three  spaces  anhg,  tehg,  kqg,  are  aW  equal. 
Carol.  2.  From  the  equals  anhg,  kqg, 
take  the  equals  anA^,  Kqg, 
and  there  remains  ghuo  =»  gqoa. 
Corol.  3.  And  from  the  equals  #Ahg,  gqao9 
take  the  common  space  £?lkg, 
and  there  remains  the  Alqh  =  At?  A. 
Corol.  4.  Again,  from  the  equals  kqo,  ttshg, 
take  the  common  space  klhg, 
and  there  remains  tclk  =  -A Left. 

Corol.  5.  And  when 
by  the  lines  kq,  gh, 
moving  with  a  parallel 
motion,  kq  comes  into 
the  position  ie,  where  ^ 
cr  is  the  conjugate  to  T 
ca;  then 


the  triangle     kqg  becomes  the  triangle  ntc, 
and  the  space  anhg  becomes  the  triangle  anc  ; 
and  therefore  the  Airc  =  A  anc  =  tec. 
Corol.  6.    Also  when  the  lines  kq  and  hq,  by  moviag 
with  a  parallel  motion,  come  into  the  position  cef  me, 


OP  THE  ELLIPSE. 


tke  triangle     lqh  becomes  the  triangle  cent, 
and  the  space  telk  becomes  the  triangle  tec  ; 
and  theref.  the  Ac  cm  =  A  tec  =  Aanc  =  &uic. 


theorem  xx. 


Any  diameter  bisects  all  its  double  ordinotes,  or  the  lines 
drawn  parallel  to  the  tangent  at  its  vertex,  or  to  its  con- 
jugate diameter. 


That  is,  if  oq  be  pa- 
rallel to  the  tangent  te, 
or  to  ce,  thenehall  La  = 

Mr- 


For,  draw  qh,  qh  perpendicular  to  the  transverse. 
Then  by  cor.  3,  theor.  19,  the  A  lqh  ="=  vqh ; 
but  these  triangles  are  also  equiangular ; 
consequently  their  like  sides  are  equal,  or  La  =  14. 

Cord*  Any  diameter  divides  the  ellipse  into  two  equal 
parts. 

For,  the  ordinates  on  each  aide  being  equal  to  each  other, 
aud  equal  in  number ;  all  the  ordinates,  or  the  area,  on  one 
side  of  the  diameter,  is  equal  to  all  the  ordinates,  or  the  areu, 
on  the  other  side  of  iU 


TBEOKEX  XXI. 


As  the  square  of  any  diameter 
Is  to  the  square  of  its  conjugate,  • 
So  is  the  rectangle  of  any  two  abscisses 
To  the  square  of  their  ordinate. 

That  is,  ce8  :  ce9 ::  el  •  lo  or  ce3  —  cl2  :  lq*. 


For,  draw  the  tangent 
te,  and  produce  the  or- 
dinate ul  to  the  trans- 
verse at  k.  Also  draw 
<w»  ex  perpendicular  to 
the  transverse,  and  meet. 
ingEG  in  n  and  x. 

Then,  similar  triangles 


r 


\ 


403  come  iBcnoKt. 

being  as  the  squares  of  their  like  sides,  it  is, 

by  sim.  triangles,  Acet  :  A  cut  : :  ce*  :  cl8; 

or,  by  division,    Ackt  :  trap,  tklk  :  :  ck*:  ce1 —  cxa. 

Again,  by  sim.  tri.  A      :  A  t<m  : :  cc* :  l<*'. 
But,  by  cor.  5thcor.  19,  the  Ac*m  =  acet, 
and,  by  cor.  4  theor.  10,  the  Ai<w  =  trap,  tslk  ; 
theref.  by  equality,  ce  :  ce1 : :  en*  —  cl*  :  m*, 
*  or        -        •        ce3  :  ce* :  :  el  .  lg  :  i.qs.  q.  b.  d. 

Cord.  1.  The  squares  of  the  ordi nates  to  any  diameter, 
are  to  one  another  as  the  rectangles  of  their  respective 
abscisses,  or  as  the  difference  of  the  squares  of  the  semi- 
diameter  and  of  the  distance  between  the  ordinate  and  centre. 
For  they  are  all  in  the  same  ratio  of  ce2  to  ce\ 

Corel.  2.  The  above  being  a  similar  property  to  that  be* 
longing  to  the  two  axes,  all  the  other  properties  before  laid 
down,  for  the  axes,  may  be  understood  of  any  two  conjugate 
diameters  whatever,  using  only  the  oblique  ordinates  of  these 
diameters,  instead  of  the  perpendicular  ordinates  of  (he  axes  ; 
namely,  all  the  properties  in  theorens  6,  7,  8, 14,  15,  16,  18, 
and  )9. 


THEOREM  XXII. 


If  any  two  lines,  that  any  where  intersect  each  other,  meet 
the  curve  each  in  two  points  ;  then 
the  rectangle  of  the  segments  of  the  one 
is  to  the  rectangle  of  the  segments  of  the  other, 
as  the  square  of  the  diam.  parallel  to  the  former 
to  the  square  of  the  diam.  parallel  to  the  latter. 


That  is,  if  cr  and  cr  be  y' 
parallel  to  any  two  lines  ^ 


phq,  pnq 


then  shall 
ph  .  hq  :  pn 


For,  d  raw  the  diameter  che,  and  the  tangent  te,  and  its 
parallels  pk,  hi,  mii,  meeting  the  conjugate  of  the  diameter 
cr  in  the  points  t,  k,  i,  m.  Then,  because  similar  triangles 
are  as  the  squares  of  their  like  sides,  it  is, 

by  sim.  triangles  cua :  up2  :  :  acri  :  £gpk, 

and     .    -    -    .  v:uA  \  uiv1  %  \  kvaiw  ^hk  ; 

t!*eref.  by  division,  en?  *.  o#  —  ^v?  *.  *.      \  *x-vnu 


OF  THE  ELLIPSE. 


Again,  by  aim.  tri.  ce3:  cn9 :  :  acts  :  Ackh; 

and  by  division,    cr1  :  cr*  —  cu9  :  :  Acte  :  tehm. 
But,  by  cor.  5  theor.  19,  the  Acte  =  A  cm, 
and  by  cor.  1  theor.  19,  tf.hg      kphg,  or  tehm  =  kpbm  ; 
the  re  1*.  by  equ.  ce9  :  ce3  —  ch9  : :  cr*  :  gp9—-  gh9  or  ph  .  HQ. 
In  like  manner  ck*  :  ce*  —  ch9  :  :  cr9 :  pu  .  uq. 
Theref.  by  equ.  cr3  :  cr3  :  :  ph  .  na  :  pH.  Hq.  q.  e.  d. 

Carol.  1.  In  like  manner,  if  any  other  line  p'n'q,  parallel 
to  cr  or  to  pq,  meet  phq  ;  since  the  rectangles  ph'q,  p'n'q' 
are  al*o  in  the  same  ratio  of  cr9  to  cr9 ;  therefore  reel. 
phq,  :  pnq  :  :  pii'q  :  pu'q'. 

Also,  if  another  line  p  ho?  be  drawn  parallel  to  pq  or  cr  ;  * 
because  the  rectangles,  p  Aq',  p  hq  are  still  in  the  same  ratio, 
therefore,  in  general,  the  rect.  phq  :  puq  : :  p  ha  :  p  hq'. 

That  is,  the  rectangles  of  the  pans  of  two  parallel  lines, 
are  to  one  another,  as  the  rectangles  of  the  parts  of  two  other 
parallel  linen,  any  where  intersecting  the  former. 

Cord.  2.  And  when  any  of  the  lines  only  touch  the  curte, 
instead  of  cutting  it,  the  rectangles  of  such  become  squares, 
and  the  general  property  still  attends  them. 


Corel.  3.  And  hence  «  :  re  : :  If  :  /e. 


[484] 
OF  THE  HYPERBOLA. 


THEOREM  I. 


The  Squares  of  the  Ordinate*  of  the  Axis  are  to  each  other 
as  the  Rectangles  of  their  Abscisses. 

Let  avb  be  a  plane  passing 
through  the  vertex  and  axis  of 
the  opposite  cones;  agih  an- 
other section  of  them  perpendi- 
cular to  the  plane  of  the  former ; 
ab  the  axis  of  the  hyperbolic 
sections;  and  fo,  hi.  ordinatcs 
perpendicular  to  it.  Then  it  will 
be,  as  fg2  :  hi3  : :  af  .  fb  :  ah  .  hb. 

For,  through  the  ordinates 
fg,  hi,  draw  the  circular  sections 
kgl,  min,  parallel  to  the  base  of 
the  cone,  having  ki.,  m\,  for  their  diameters,  to  which  fg, 
hi,  are  ordinates,  as  well  as  to  the  cxis  of  the  hyperbola. 

Now,  by  the  similar  triangles  afl,  ahn,  and  bfk,  bhm, 
it  is  af  :  ah  :  :  fl  :  hn, 
and  fh  :  hr  : :  kf  :  mh  ; 

hence,  taking  the  rectangles  of  the  corresponding  terms, 

it  is,  the  rect.  af  .  fb  :  ah  .  iiu  :  :  kf  .  fl  :  mh  .  hn. 
But,  by  the  circle,  kf  .  fl  ■»  fg3,  and  mh  .  hn  =  hi3  ; 
Therefore  the  rect.  af  .  fb  :  ah  .  hb  :  :  kg9  :  hi2. 

q.  e.  D. 


THEOREM  II. 


As  the  Square  of  the  Transverse  Axis 
Is  to  the  Square  of  the  Conjugate  : 
So  is  the  Rectangle  of  the  Abscisses 
To  the  Square  of  their  Ordinate. 


That  is,  ab3 

ac3  :  ac?  : ;  - 


OF  TflS  RTPSRBOLA. 


For,  by  theor.  1 ,  ca  .  cb  :  ad  .  db  : :  ca*  :  dr*  ; 
But,  if  c  be  the  centre,  then  ac  .  cb  =  ac1,  and  ca  is  the 

setni.conj. 

Therefore  .  ac1  :  ad  .  db  : :  cc*  :  de*  ; 
or,  by  permutation,  ac9  :  oc9  : :  ad  .  db  :  dk*  ; 
or,  by  doubling,      ab'  :  a&9 : :  ad  .  db  :  db1.  <l.  e.  d. 

ab9 

Cord.  Or,  by  div.  ab  :  —  : :  ad  •  db  or  cd*— ca1  :  de*, 

J  AB 

that  is,  ab  i  p  1 1  ad  •  db  or  cd* — ca*  :  de*  ; 
ab3 

where  p  is  the  parameter  —  by  the  definition  of  it. 

That  is,  As  the  transverse, 
Is  to  its  parameter, 
So  is  the  rectangle  of  the  abscisses, 
To  the  square  of  their  ordinate. 


Otherwise,  thus ; 


Let  a  continued  plane,  cut 
from  the  two  opposite  cones,  the 
two  mutually  connected  oppo- 
site hyperbolas  hag,  hag,  whose 
vertices  arc  a,  a,  and  bases  u<», 
hgy  parallel  to  each  other,  fall, 
ing  in  the  planes  of  the  two  pa- 
rallel circlet* lgk,  Jgk.  Through 
c,  the  middle  point  of  ah,  let  a 
plane  be  drawn  parallel  to  that 
of  lok,  it  will  cut  in  the  cone 
lvk  a  circular  section  whose  di- 
ameter is  mn  ;  to  which  circu- 
lar section,  let  d  be  a  tangent  at  t. 

Then,  by  sim.  tri. 
Acm,  AFL 
and,  by  sim.  tri. 
acn,  an 


ac  :  cm 


AF  :  I*L  ! 


ac  :  cn  : :  of  :  fk. 


/,  ac  •  ca  i  cm  •  eft  1 1  af  •  Fa  :  lf 
or,  ac*  :  c£*  : :  af  .  ra  :  fg*. 


FK, 


In  like  manner,  for  the  opposite  hyperbola 
ac*  \cP  n  hf  .fa  :fg*. 

Hens  ct  is  what.ic  usually  denominated  the  semMSonjvgsje 
to  the  opposite  hyperbolas  hak,  hak :  but  it  is  evidently  «sf 
in  the  same  plane  whh  them. 


406 


OOXIC  SKCTIOXS. 


THEOREM  III. 

As  the  Square  of  the  Conjugate  Axis 

In  to  the  Square  of  the  Transverse  Axis, 

So  is  the  Sum  of  the  Squares  of  the  Semi  •conjugate,  and 

distance  of  the  Centre  from  any  Ordinate  of  the  Axis, 
To  the  Square  of  the  Ordinate. 

m 


ca9 


That  i*, 
ca1  : :  ca1  +  cd9 


dm9. 


For,  draw  the  ordinate  ed  to  the  transverse,  ab. 


ca9 

CA9 

ca9 

CA9 


Then,  by  theor.  1,  ca9 
or      -       -  ca* 
B^ut     -  ca3 
tfieref.  by  compos,  ca9 
In  like  manner,      ca9  :  ca9  : : 
Corol.  By  the  last  theor.  ca9 
and  by  this  theor.  ca9  : 
therefore     -  de* 
In  like  manner, 


de9 
ca2 

CA9 

ca9 
ca9 

I*9 
Df9  .  dE* 


AD  .  DB  Or  CD1   —  CA9, 
C*E9   —  CA9. 
.  CA9. 

+  erf9  <*e9. 

+  CD'  :  DC9.        Q..  E.  D. 

: :  cd9 — ca9  :  de9 9 


:cd9+ca9 

: CD9  —  CA9 

:  cd9— ca1 


:d*3, 
:  cd9 


4-  CA9 

cd9  +  ca9 


THEOREM  IV. 


The  Square  of  the  Distance  of  the  Focus  from  the  Centre,  is 
equal  to  the  Sum  of  the  Squares  of  the  Semi-axes. 

Or,  the  Square  of  the  Distance  between  the  Foci,  is  equal  to 
the  Sum  of  the  Squares  of  the  two  Axes. 

That  is,  f . 

cf9  =  ca9  +  ca9,  or  Hrt 
pfi      ab9  +  ab*. 


For,  to  the  focus  f  draw  the  ordinate  fe  ;  which,  by  the 
definition,  will  be  the  semi- parameter.  Then,  by  the  nature 
of  the  curve  .  ca9  :  ca9  : :  cf9  —  ca9  :  fe1  ; 

and  by  the  def.  of  the  para,  ca9  :  ca9  ; :       ca9      :  fe9  ; 
therefore        -        -       ca2  =  cf9  —  ca9  ; 
and  by  addition        •       cf2  =  ca9  +  ca9  ; 
or,  by  doubling,  —       -V  afc* *         4.  *•  D. 


Or  THE  HYPERBOLA. 


497 


Corol.  1 .  The  two  semi-axes,  and  the  fncal-distance  from 
the  centre,  are  the  sides  of  a  right-angled  triangle  c\a  ;  and 
the  distance  \a  is  =  cf  the  focal  distance. 

Corol.  2.  The  conjugate  semi-axis  ca  is  a  mean  propor- 
tional between  af,  fb,  or  between  a/*,/b,  the  distances  of 
either  focus  from  the  two  vertices. 

For  ca*  =  cf3  —  ca2  =  (cf  +  ca)  .  (cf  —  ca)  =  af  .  fb, 

THEOREM  V. 

The  Difference  of  two  Lines  drawn  from  the  two  Foci  to 
meet  at  any  Point  in  the  Curve,  is  equal  to  the  Transverse 
Axis. 


For,  draw  ag  parallel  and  equal  to  ca  the  semi. conjugate  ; 
and  join  cg,  meeting  the  ordinate  de  produced  in  h  ;  also 
take  ci  a  4th  proportional  toe  a,  cf,  cd. 

Then,  by  th.  2,  ca   :  ag   : :  cd3  —  ca3  :  de1  ; 
and,  by  sin.    As,  ca2  :  ag3  : :  CDi  —  ca3  :  dh3  —  ag'  ; 
consequently        de3  =  dh3  —  ag3  =  dh3  —  ci?. 
Also,  fd  =  cf    cd,  and  fdj  =  cf3  —  2cf  .  cd  -f •  cd3  ; 
and,  by  right. angled  triangles,  fe3  =  fd2  +  de3. 
therefore  fe3  =  cf3  —  caJ  —  2cf  .  cd  +  cd2  +  dh 
But,  by  theor.  4,     cf3  -r~  ca3  =  cas, 
and,  by  supposition,  2c f  .  cd  =  2c a  .  ci ; 
theref.  fe3  =  ca3  —  2ca  .  ci  +  cd3  +  dh"  ; 
Again,  by  suppos.    ca2  :  cd2  : :  cf*  or  ca2  +  ag3  :  cr  ; 
and,  by  sim.  tri.       ca3  :  cd3  : ;  ca3  +  ag3  :  cd3  +  dh1  ; 
therefore       -        ci3  =  cd3  +  dh3  ■=  en3  ; 
consequently  fe3  =  ca3  —  2ca  .  cr  +ci3. 

And  the  root  or  side  of  this  square  is  fe  =  ci  —  ca  =  ai. 
In  the  same  manner,  it  is  found  that/k  =  ci  +  ca  =  bi. 
Conseq.  by  subtract.  f%  —  fe  =  bi  —  ai  =  ab.        q.  b.  d, 

Corol.  1.  Hence  ch  =  ci  is  a  4th  proportional  to  ca,  cf, 
cd. 

Corol.  2.  And /e  +  fe  =  2ch  or  2ci ;  or  fe,  ch,  fk9  are 
in  continued  arithmetical  progression,  the  common  difference 
being  ca  the  semi-transverse. 

Vol.  I.  64 


4fe8  COKIC  SECTIONS. 

\  CoroL  8.  Hence  is  derived  the  common  method  of  deecrib- 
*irtg  this  curve  mechanically  by  points,  thus: 

In  the  transverse  ab,  produced,  take  the  foci  f,/,  nnd  anj 
point  i.  Then  with  the  radii  ai,  bi,  and  centres  f,/„  describe 
arcs  intersecting  in  e,  which  will  be  a  point  in  the  curve.  Id 
like  manner,  assuming  other  points  i,  as  many  other  points 
will  he  found  in  the  curve. 

Then,  with  a  siendy  hand,  the  curve  line  may  be  drawn 
through  all  the  points  of  intersection  r. 

In  the  same  manner  are  constructed  the  other  two  or  con- 
jugate hyperbolas,  using  the  axis  ab  instead  of  ab. 


THEOREM  VI. 

If  from  any  Point  i  in  the  Axis,  a  Line  il  be  drawn  touching 
the  Curve  in  one  Point  l  ;  and  the  Ordinate  lm  be  drawn ; 

:  and  if  c  be  the  Centre  or  the  Middle  of  ab  :  Then  shall  cm 
be  to  ci  as  the  Square  of  am  to  the  Square  of  ai. 

**>- 

That  is, 
cm  ;  ci  : :  am2  :  Aia. 


For,  from  the  point  i  draw  any  line  irh  to  cut  the  curve 
in  two  points  e  and  11 :  from  which  let  fall  the  perps.  ed,  hg  ; 
and  bisect  no  in  k. 

Then,  by  theor.  1,       \d  .  db  :  ac  .  gb  : :  de3  :  gh9, 
and  by  sim.  triangles,         ur*     :     iGa      :  :  de3  :  gh*; 
theref.  by  equality,  ad  .  db  :  ag  .  gb  : :  id9  :  ig*. 

But  DB  =  CH  +  CD  =  CA  +  CD  =  CG  +  CD  —  AG  =  2cK  AG, 

and  tut  =  cn  +  ct:  =  c\  +  cc  =  cg  +  cd — ad  =  2ck— ad  ; 
thcrcf.  a i) .  2c k  —  ad  .  ag  :  ag  .  2ck  —  ad  .  ag  : :  id3  :  ig3, 
and.  by  div.  »g  .  2ck  :  ig3  —  id2  or  dg  .  2ik  : :  ad  .  2c B 

—  ad  .  ag  :  id2  ; 
or    -    2c  k  :  2ik  :  :  ad  .  2ck  —  ad  .  ag  :  id3  ; 
or    ad  .  2c k  :  ad  .  2ik  :  :  ad  .  2c k — ad  .  ag  :  id3; 
theref.  by  div.  ck  :  ik  : :  ad  .  ag  :  ad  .  2ik  —  id8, 
and,  by  div.     ck  :  ci  : :  ad  .  ag  :  id2  — •  ad  .  (id  +  ia), 
or       -  ck  :  ci  :  :  ad  .  ag  :  ai2. 

But,  when  the  line  in,  by  revolving  about  the  point  i,  comes 
into  the  position  of  the  tangent  il,  then  the  points  e  and  h  meet 
in  the  point  l,  nnd  the  points  d,  k,  g,  coincide  with  the  point 
>i  ;  and  then  the  last  proportion  becomes  cm  :  ci  ; :  am3  :  ai3. 

E.  D. 


.»  / 

OF  THE  HTPBfiBOLA. 


THEOREM  VII. 

If  a  Tangent  and  Ordinate  be  drawn  from  any  Point  in  the 
Curve,  meeting  the  Iransverse  Axis ;  the  Semi- 1 runs vewc 
will  he  a  Mean  Proportional  between  the  Distances  of  the 
said  Two  Intersections  from  the  Centre. 

That  is, 

ca  is  a  mean  proportional  between 
cd  and  ct  ;  or  cd,  ca,  it,  are  con- 
tinued proportionals. 

For,  by  th.  6,  cd  :  ct  : :  ad*  :  at3, 
that  is,       -      cd  :  ct  : :  (cn  —  ca)s  :  (ca  —  ct)1, 
or      -       -      cd  :  ct  : :  cd'  +  ua3  :  ca2  +  cr3, 
and    -       -      cd  :  or  : :  cd3  4-  ca1  :  cd2  —  ct3, 
or     -       -      cd  :  dt  ; :  cd*1  +  ca9  :  (cd  +  ct)  dt,  & 
or       cd*  :  cd  .  dt  : :  cd8  +  ca3  :  cd  .  dt  +  ct  .  td  ; 
hence  cd2  :  ca3  : :  cn  .  dt  :  ct  .  td, 
and     coa  :  ca3  ; :  cd  :  ct, 

theref.  (th.  78,  Geom.)  cd  :  ca  : .  ca  :  ct.  q.  e.  d. 

Carol.  Since  ct  is  always  a  third  proportional  to  cn,  ca  ; 
if  the  points  d,  a,  remain  constant,  then  will  the  point  r  be 
constant  also  ;  and  therefore  all  the  tangents  will  meet  in  this 
point  t,  which  are  drawn  from  the  point  e,  of  every  hyperbo- 
la described  on  the  same  axis  ar,  where  they  are  cut  by  the 
common  ordinate  deb  drawn  from  the  point  d. 

THEOREM  VIII. 

If  there  be  any  Tnngent  meeting  four  Perpendiculars  to  the 
Axis  drawn  from  these  four  Points,  namely,  the  Centre, 
the  two  Extremities  of  the  Axis,  and  the  Point  of  Contact ; 
those  four  Perpendiculars  will  be  Proportionals. 


That  is, 
ao  :  de  : :  en  :  bi. 


ac  :  nc, 

tc  :  ac  or  cd, 

TC  '  TB, 

cu  :  HI. 


499 

■  I 


For,  by  thcor.  7,  tc  :  ac  : . 
theref.  by  div.  ta  :  ai>  : : 
and  by  com  p.  ta  :  td  : : 
mad  by  sim.  tri.      ao  :  de  : : 


600 


CONIC  1X011091. 


Cord.  Hence  ta,  td,  tc,  tb  )  | 

and  TO,  TE,  Til,  ti  \ 

For  these  are  as  ag,  de,  cii,  bi,  by  similar  triangles. 


ore  also  proportionals. 


THEOREM.  IX. 

If  thore  be  any  Tangent,  and  two  Lines  drawn  from  the  Foci 
to  the  Point  of  Contact ;  these  two  Lines  will  make  equal 
Angles  with  the  Tungent. 

That  is,  1  l^n^^FD 

the  JL  fbt  =  L  foe. 


For,  draw  the  ordinate  pe,  and  fe  parallel  to  fe. 
By, cor.  1,  theor.  5,  ca  :  cn  :  :  cf  :  ca  +  fe, 

cd  : :  cr  :  ca  ; 
cf  :  :  ca  :  ca  +  fe  ; 
rf  :  :  fe  :  2ca  +  fe  or /e  by  th.  5. 

if  ::  fe  :/k; 

-fey  and  conseq.    Le  =  &f$e. 
fe  is  parallel  to  fe,  the  Le  =  Z.fkt  ; 

Z.  FKT  =  £fEC.  Q.  K.  D. 


and  by  th.  7,  ca 
therefore  -  ct 
and  by  add.  and  sub.  tf 
But  by  sini.  tri.  i  f 
therefore  -  fv. 
But,  because 
therefore  the 

Corol.  As  opticians  find  that  the  angle  of  incidence  is  equal 
to  the  angle  of  reflection,  it  appears,  from  this  proposition, 
that  rays  of  light  issuing  from  the  one  focus,  and  meeting  the 
curve  in  every  point,  will  be  reflected  into  lines  drawn  from 
the  other  focus.  So  the  ray  ft:  is  reflected  into  fe.  And 
this  is  the  reason  why  the  points  f,  /,  are  called  foci,  or 
burning  points. 


THEOREM  X. 


All  the  Parallelograms  inscribed  between  the  four  Conjugate 
Hyperbolas  are  equal  to  one  another,  and  each  equal  to 
the  Rectangle  of  the  two  Axes. 


That  is, 
the  parallelogram  pqrs 
the  rectangle  ab  .  ab. 


4 


OF  THE  HYPEBBOLA. 


Ml 


Let  eg,  eg,  be  two  conjugate  diameters  parallel  to  the  i 
of  the  parallelogram,  and  dividing  it  into  four  less  and  equal 
parallelograms.  Also,  draw  the  ordi nates  dk,  de,  andec 
perpendicular  to  pq  ;  and  let  the  axis  produced  meet  the  sides 
of  the  parallelograms,  produced,  if  necessary,  in  T  and  t. 

Then,  by  theor.  7,  ct  :  ca  : :  ca  :  cd, 
and  -  •  cl  :  ca  : :  ca  :  cd ; 
theref.  hy  equality,  ct  :  cl  : :  cd  :  cd  ; 
but,  by  sim.  triangles,  ct  :  ct  : :  td  :  cd, 
theref.  by  equality,  td  :  cd  : :  cd  :  cd, 
and  the  rectangle  td  •  dc  is  '=  the  square  cd?. 
Again,  hy  theor.  7,  cd  :  ca  : :  ca  :  ct, 
or,  by  division,  cd  :  ca  : :  da  :  at, 

and,  by  composition,   cd  :  db  : :  da  :  dt  ; 
conseq.  the  rectangle  cd  .  dt  : :  cd2  =  ad  •  db*. 


But,  by  theor.  X*'  okr 

therefore        -  ca 

or  .  ca 

By  theor.  7,    .  ca 

By  equality     -  ct 

By  sim.  tri.     -  ct 

theref.  by  equality,  ct 

But,  by  sim.  tri.  ct 

theref.  by  equality,  ck 

and  the  rectangle  ck  , 

But  the  rect.  ck 

theref.  the  rect.  ca 

conseq.  the  rect.  ab 


co8 : :  (ad  .  db  or)  aP  ; 


ca 

de  : 
ct 

CA 

CT  ; 
ca  : 
ck  : 
ca  : 


cd 

:  ca 
cd 

:  ca 
de 

:  ca 
;  ce  : 
ca  : 


Ct  =  CA 


DE, 
id. 
CA. 
DE. 

DE  ; 

de. 
de ; 
ce. 
ca. 


ce  =  the  parallelogram  cepc, 
ce  =  the  parallelogram  cere, 
ab  =  the  paral.  pqrs.      q.  e.  d. 


THEOREM  XI. 


The  Difference  of  the  Squares  of  every  Pair  of  Conjugate 
Diameters,  is  equal  to  the  same  constant  Quantity,  namely, 
the  Difference  of  the  Squares  of  the  two  Axes. 


That  is. 
ab" —  ab2  —  kg*  —  eg ; 
where  eg,  eg  are  any  conjugate 
diameters. 


•  Corol.  Becnu*e  erf1  =  ai>  .  dk  =  cd*  —  ca9. 

therefore  ca9  =  cd1  —  cd2. 
la  Lice  manner    ejff  =  «V*  —  d*9. 


Mt 


come  SECTIOXS. 


For,  draw  the  ordirmtcs  kd,  rd. 
Then,  by  cor.  to  theor.  10,  ca3  =  cd3  —  cd*9 
and       -       -       -       -    ca1  =  de2  —  dk3  ; 


theref.  the  difference  ca3  — 

ca3 

=  t'i)s 

+  DK3  — 

cd*—de*. 

Bui,  by  right-angled  As, 

CE7 

s=  CD* 

+  DK3, 

and  - 

ce1 

=  cd* 

+  de2  ; 

theref.  the  difference  ce3  — 

ce2 

—  CD3 

+  DK3  — 

cd*  —de9, 

consequently     .     ca3  — 

Ctl2 

=  CK3 

—  ck3  ; 

or,  by  doubling,       ab3  — 

ab2 

=  EG3 

-eg2. 

a,  e.  d. 

THEOREM  XII. 

All  the  Parallelograms  are  equal  which  are  formed  between 
the  Asymptotes  and  Curve,  by  Lines  drawn  Parallel  to 
the  Asymptotes. 


That  is  the  lines  gk,  f.k,  ap,  aq, 
being  parallel  to  the  asymptotes  <;ii,  <7 ; 
then  the  para  I.  igek  =  pural.  cpaq. 


For,  let  a  be  the  vortex  of  the  curve,  or  extremity  of  the 
semi-transverse  axis  a<\  perp.  to  which  draw  al  or  a/,  which 
will  be  equal  to  the  semi-conjugate,  by  definition  19.  Also, 
draw  hkdi/i  parallel  to  l/, 

Then,  by  theor.  k2,  v\s  :  al=  :  :  co3  —  ca3  :  de3, 
and,  by  parallels,       ia2  :  al2  :  :  (  n3  :  mi  -  ; 
theref.  by  subtract.    ca2  :  al3  :  :  <\\3  :  dii*  —  dk3  or 

rect.  ii  k  .  v.h  ; 
conseq.  the  square  al2  =  the  rect.  in:  .  f7i. 

But,  by  sim.  tri.  i  a  :  al  :  :  gk  ;  eh, 
and,  by  the  same,  a  a  :  a/  :  :  kk  :  v.h  ; 
theref.  by  comp.  pa  .  \q  .  al3  .  :  gk  .  f.k  :  iik  .  v.h  ; 
and  because         al3  =  iik  .  k/i,  theref.  pa  .  aq  =  <;e  .  ek. 

But  the  parallelograms  cgk.k,  cpaq,  being  equiangular, 
are  as  the  rectangles  gk  .  kk  and  pa .  aq. 

Therefore  the  parallelogram  gk  ~  the  paral.  pq. 

That  is,  all  the  inscribed  parallelograms  are  equal  to  one 
another.  q.  e.  d. 

CoroL  1.  Because  the  rectangle  gkk  or  cgk  is  constant, 
therefore  ok  is  reciprocally  as  cg,  or  cg  :  cp  :  :  pa  :  gk. 
And  hence  the  asvmnUiU'.  continually  approaches  towards 
the  curve,  bul  i\g\*:t  vw^^X^  \\  .      vvt  w^ywaUy 


C  K  Q     £  h 


OF  THE  OYPEBBOLA. 


as  co  increases  ;  and  it  is  always  of  some  magnitude,  except 
when  co  is  supposed  to  be  infinitely  great,  for  then  gk  is 
infinitely  small,  or  nothing.  So  that  the  asymptote  co  may 
be  considered  us  a  tangent  to  the  curve  at  a  point  infinitely 
distant  from  c. 

Carol.  2.  If  the  abscisses  cd, 
cv,  cg,  &c.  taken  on  the  one 
asymptote,  be  in  geometrical  pro- 
gression increasing  ;  then  shall  the 
ordi nates  uh,  ki,  ok,  &c.  parallel 
to  the  other  asymptote,  be  a  de- 
creasing geometrical  progression,  £r 
having  the  same  ratio.  For,  all 
the  rectangles  cdh,  cei,  cor,  &c.  being  equal,  the  ordinates 
dh,  ki,  gk,  dec,  are  reciprocally  as  the  abscisses  cd,  ck,  cg, 
die.  which  are  geometricals.  And  the  reciprocals  of  geome- 
trical are  also  geometricals,  and  in  the  same  ratio,  but  de- 
creasing, or  in  converse  order. 


THEOREM  XIII. 

The  three  following  Spaces  between  the  Asymptotes  and  the 
Curve,  arc  equal  ;  namely,  the  Sector  or  Trilinear  Space 
contained  by  an  Arc  of  the  Curve  and  two  Radii,  or  Lines 
drawn  from  its  Extremities  to  the  Centre  ;  and  each  of 
the  two  Quadrilaterals,  contained  by  the  said  Arc,  and 
two  Lines  drawn  from  its  Extremities  parallel  to  one 
Asymptote,  and  the  intercepted  Part  of  the  other  Asymp- 
tote. 


That  is, 

The  sector  cae  =  paeg  =  qaek, 
all  standing  on  the  same  arc  ae. 


For,  bytheor.  12,  cpaq  =  cgkk  ; 
subtract  the  common  space  cgiq, 
there  remains  the  paral.  pi  =  the  par.  ik  ; 
To  each  add  the  trilineal  iae,  then 
the  sum  is  the  quadr.  pa  kg  =  qakk. 

Again,  from  the  quadrilateral  caek 
take  the  equal  triangles,  caq,  cek, 
and  there  remains  the  sector  cak  =  qaek. 
Therefore  cae  =  qaek  =  faeg.  q.  e.  d. 


MM 


cosiic  lEcnoifi. 


SCHOLIUM. 


In  the  figure  to  theorem  12,  cor.  2,  if  c  d  =  1,  and  ce,  ca, 
&c.  be  any  numbers,  the  hyperbolic  Bpaces  hdei,  iegk,  &c. 
are  analogous  to  the  logarithms  of  those  numbers.  For, 
whilst  the  numbers  cd,  ce,  cg,  6zc.  proceed  in  geometries! 
progression,  the  correspondent  spaces  proceed  in  arithmetical 
progression ;  and  therefore,  from  the  nature  of  logarithms 
are  respectively  proportional  to  the  logarithms  of  those  num. 
hers.  If  the  angle  c  were  a  right  angle,  and  cn  =  dh  =1 ; 
then  if  ce  were  "=  10,  the  space  deih  would  be  2*30258509, 
&c. ;  if  co  were  =  100,  then  the  space  dgkh  would  be 
4-60517018  :  these  being  the  Napierean  logarithms  to  10  and 
100  respectively.  Intermediate  a  re  are  corresponding  to  in- 
termediate abscissae  would  be  the  appropriate  logarithms. 
These  are  usually  called  Hyperbolic  logarithms ;  but  I  he 
term  is  improper :  for  by  drawing  other  hyperbolic  curves 
between  hik  and  its  asymptotes,  other  systems  of  logarithms 
would  be  obtained.  Or,  by  changing  the  angle  between  the 
asymptotes,  the  same  thing  may  he  effected.  Thus,  when 
the  angle  c  is  a  right  angle,  or  has  it:,  sine  =  1.  the  hyperbo- 
lic spaces  indicate  the  Napierean  logarithms;  hut  when  the 
angle  is  25  44'  27}",  whose  sine  is  =  -43420148,  A:c.  the 
modulus  to  the  common,  or  ttriggs's,  logaiithms,  the  spaces 
deih,  &c.  measure  those  logarithms.  I*)  both  eases,  if  spaces 
to  the  right  of  dh  are  regarded  as  posit  ice,  those  Jo  the  left 
will  be  negative;  whence  it  follows  that  the  logarithms  of 
numbers  less  than  1  arc  negative  also. 


The  sum  or  difference  of  the  semi -transverse  and  a  line  drawn 
from  the  focus  to  any  point  in  the  curve  W  equal  to  a  fourth 
proportional  to  the  semi. transverse,  the  distance  from  the 
centre  to  the  focus,  and  the  distance  from  the  centre  to  the 
ordinate  belonging  to  that  point  of  the  curve. 


THZOREM  XIV. 


fe+ac=xi,  or  FK=AI  ; 
and  fit —  ac=ci,  or  fK—m. 
•Where  c\  : cf  :  :  cn  :  ci  the 
4th  propor.  to  ca,  cf,  cd. 


That  is, 


OF  TUB  HYPERBOLA.  fiM 

For,  draw  ao  parallel  and  equal  to  ea  the  semi. conjugate  { 
and  join  co  meeting  the  ordinate  de  produced  in  h. 

Then,  by  theor.  2,  CAa  :  ao*  : :  cd2— ca2  :  de2; 
and,  by  aim.  As,  ca2  :  ao2  : :  coa— ca8  :  dh3 — AGa; 
consequently  db2s5sdh2 — ag2=dh2— ca*. 

Also  fd=cf^cd,  and  fd3=cf3 — 2cf  .  cd+cd2; 
but,  by  right-angled  triangles,  fd2+de2=-fr2; 
therefore  fe^cf3—  ca7 — 2cf  •  cD+cDa+DHi. 

But  by  theor.  4,      cf2— ca'=x'Aa, 
and,  by  supposition,  2cf  .  cd=2ca  .  ci  ; 
tlieref.  fe2=ca2— 2ca  .  ci+cd2+dh2. 

But,  by  supposition,  ca2  :  cd2  : :  of2  or  ca2+ag2  :  ci1? 
and,  by  sim.  as,     ca2  :  cd2  : :  ca2+ao2  :  cd2+dh2  ;    c  c- 
therefore       -  ci^cdM-dh^ch2; 
consequently    -    fb^ca2— 2ca  .  ci+ci3. 

And  the  root  or  aide  of  this  square  is  fe=ci — ca=ai. 

In  the  same  manner  is  found  /e— ci+ca=bi.  a.  e.  b. 

Coral.  1.  Hence  ch=ci  is  a  4th  propor.  to  ca,  cf,  cd. 

Cord.  2.  And  /e+fe=2ch  or  2ci ;  or  fk,  ch, /e  are  in 
continued  arithmetical  progression,  the  commr*  difference 
being  ca  the  semi- transverse.  \ 

Corol.  3.  From  the  demonstration  it  appears,  that  de2  = 
dh2  —  ao2  =  dm2  —  ca\  Consequently  dh  is  every  where 
greater  than  de  ;  and  so  the  asymptote  cgh  never  meets  the 
curve,  though  they  be  ever  so  far  produced  :  but  dh  and  de 
approach  nearer  and  nearer  to  a  ratio  of  equality  as  tlfey 
recede  farther  from  the  vertex,  tity  at  an  infinite  distance  they 
become  equal,  and  the  asymptote  is  a  tangent  to  the  curve  at 
an  infinite  distance  from  the  vertex. 


theorem  xv. 

If  a  line  be  drawn  from  either  focus,  perpendicular  to  a  tan- 
gent to  any  point  of  the  curve;  the  distance  of  their  in- 
tersection from  the  centre  will  be  equal  to  the  semi-trans- 
verse axis. 


Vol.  I. 


65 


•  That  is,  if  ff,  fp  be  per- 
pendicular to  the  tangent 
Trp,  then  ahall  cp  ami  cp  be 
each  equal  to  ca  or  ca. 


For,  through  the  point  of  contact  ■  draw  n,  aad  /a,  nenV 
ing  fp  produced  in  e.  Then,  the  £obp«  £*bp,  being  each 
equal  to  the  l/ap,  and  the  anglee  at  f  being  n^at,  and  the 
aide  pb  being  common,  the  two  trangtes,  obf,  i»  emeaaal 
in  all  respects,  and  ae  «■  »  ra,  and*  or  ■*  fp.  Thotufae, 
aince  re^po,  and  re=^rfp  and  the  eagle,  at  f  cxNaaaocvthe 
aide  cr  will  be  =4/e  or  4ab,  that  ia  cp«*ca  sccb. 

And  in  the  same  manner  op«CA  or  ca.  e>  sfeBt 

Corn/.  1.  A  circle  deecribed  on  the  transverse  axis,  as' a' 

diameter,  will  pass  through  the  points  r,  p;  because  all  the 
lines  ca,  cp,  en,  being  equal,  will  be  radii  of  the  circle. 

Carol.  2.  cr  is  parallel  to  /a,  and  cp  parallel  to  Fa. 

Coral.  3.  If  at  the  intersections  of  any  tangent  with  the 
circumscribed  circle  perpendiculars  to  the  tangent  be  drawn, 
-they  will  meet  the  transverse  axis  in  the  two  loci.  That  is, 
the  perpendiculars  ff,  pf  give  the  foci  f, /. 


THSOBBM  XVI. 


The  equal  ordinates,  or  the  ordinatea  at  equal 

from  the  centre,  on  the  opposite  sides  and  ends  of  aa 
hyperbola,  have  their  extremities  connected  by  one  right 
line  passing  through  the  centre,  and  that  line  is 
by  the  centre. 


That  is,  if  en  £3  co,  or  the 
ordinate  dk  =  oh  ;  then  shall 
cb  =  cr,  and  ech  will  be  a 
right  line. 


For,  when  cd  =  co,  then  also  is  ra  =  on  by  cor.  9  theor.  1. 
But  the  L  d  =  L  o,  being  both  right  anglee ; 
therefore  the  third  aide  ca  =■=  cw,  and  the  L  MB  «  L  oca, 
and  conaequetrtty  ttt^ottafe* 


Carol.  1.  And,  conversely,  if  ech  be  a  right  line  pairing 
through  the  centre  ;  then  shall  it  be  bisected  by  the  centre; 
or  have  cr  «  ch,  also  de  will  be  =  on,  and-cn  =  c«. 

Carol,  2.  Hence  also,  if  two  tangents  be  drawn  to  the  two 
ends  e,  H  of  any  diumeier  eh  ;  they  will  be  parallel  to  each 
other,  and  will  cut  the  axis  at  equal  tingles,  and  at  equal  dis- 
tances from  the  centre.  For,  the  two  cd,  ca  being  equal  to 
the  two  co,  cr,  the  third  proportionals  or,  <:»  will  be  equal 
also  ;  then  the  two  sides  ce,  ct  being  equal  to  the  two  1.11, 
<  a,  and  the  included  angle  ect  equal  to  the  included  angle 
Res,  all  the  other  corresponding  parts  are  equal :  and  so  the 
L  t  =  JL  s,  and  te  parallel  to  ns. 

Carol.  3.  And  hence  the  four  tangents,  at  the  lour  ex- 
tremities of  any  two  conjugate  diameters,  form  a  parallelogram 
inscribed  between  the  hyperbolas,  and  the  pairs  of  opposite 
sides  are  each  equal  to  the  corresponding  parallel  conjugate 
diameters. — For,  if  the  diameter  eh  be  drawn  parallel  to  the 
tangent  te  or  hs,  it  will  be  the  conjugate  to  eh  by  the  defini- 
tion ;  and  the  tangents  to  e,  A  will  be  parallel  to  each  other, 
add  to  the  diameter  eh,  for  the  same  reason. 

theobem  xvir. 

If  two  ordinates  edv  ed  be  drawn  from  the  extremities  f,  e, 
of  two  conjugate  diameters,  and  tangents  be  drawn  to 
the  same  extremities,  and  meeting  the  axb  produced  in 
t  and  r  ; 

Then  shall  cd  be  a  mean  proportional  between  cd,  da, 
and  cd  a  mean  proportional  between   cd,  dt. 


For,  by  theor.  7,      cd  :  ca  :  :  ca  :  -ct,  , 

and  by  the  same,      cd  2  ca  : ;  ca  :  cr  ; 

thtref.  by  equality,    cd  :  cd  :  2  ca  :  ct. 

But  by  sim.  tri.       #nr  :  cd  :  :  ct  :  cr  ; 

theref.  by  equality,   (So  :  cd  :  :  cd  :  dt. 

In  like  manner,        cd  2  cd  :  :  cd  :  d*.        a.  e.  d. 
Coral.  1.    Hence  cd  :  cd  : :  cr  :  cr.  % 
Carol.  2.    Hence  also  cn  :  cd  :  vdt :  de. 
Aad the rect.  cd.  djs  =  cd.de,  or  A  cde  ~  &c<fe. 


JjffiM-S.  Akocf~oD.»r,telcaP«e«.dta. 
7        Or  cd  a  mean  proportional  between  ca»  vr  % 
and  cd  a  mean  proportional  between  cd,  dsu 

The  mm  igvro  befog  constructed  aetata*  lael  awea»oeitj»B> 
pmch  ordinate  will  divide  tbe  axis,  and  the  ■■—  a  madded 

to  the  external  partem  the  tame  ratio. 

[See  the  last  fig.] 
That  is,  da  :  dt  : :  dc  ;  m, 
and  dx  :da  :  :4c:  da. 
For,  by  theor.  7,  cd  :  ca  8 :  ca  :  cr, 
and  by  dir.  -  cd  :  oa  : :  ad  t  at£ 
and  by  eomp.  ■  cd  :  db  t :  ad  :  dt, 
or  •  •  da  :  or  : :  dc  :  db. 
In  like  manner,  4a  :  da  : :  dc  :  dm.  q.  b»  d. 

Carol.  1.    Hence,  and  from  cor.  9  to  the  last  prop*  it  is 

Cd2  —  CD  •  DT  =  AD  •  DB  =  CD5    CA*, 

and  cd*  =  cd .  da  =  Ad  .  da  =  ca"  =  cd* . 
Carol.  2.  Hence  also  cas=cds  — cd',  and  ca*=de*—  db*. 
Corel.  3.  Farther,  because  ca9 :  ca2: :  ad  .  dbotcJ'  :  db*« 
therefore  ca  :  ca  : :  cd  :  db. 
likewise  ca  :  ca  : :  cd  :  de. 

THEOBEM  XIX. 

If  from  any  point  in  the  curve  there  be  drawn  an  ordinate, 
and  a  perpendicular  to  the  curve,  or  to  the  tangent  at  that 
point :  then  the 

Dirt,  on  the  trans,  between  the  centre  and  ordinate,  cd, 
Will  be  to  the  dist.  pd, 
As  square  of  trans,  axis 
To  square  of  the  conjugate. 


That  is, 
cas  :  co2  : :  dc  :  dp. 


For,  by  theor.  2,  ca*  :  cd*  : :  ad  .  db  :  db1, 
But,  by  it.  angled  as,  the  reel,  td  .  dp  =  de1, 
and,  by  cor.  1  theor.  16,         cd  .  dt  =  ad  .  db; 
therefore  •    -  ca*  :  co9 : :  td  .  dc  :  td  •  dp, 

or  %    •    •    •  CA?  \  OQ>  % \ TO  4»S*B> 


OF  TBS  BYMMOLA* 


an 


THBOftJBK  XX. 


If  there  be  two  tangents  drawn,  the  one  to  the  extremity  of 
the  transverse,  and  the  other  to  the  extremity  of  any  other 
diameter,  each  meeting  the  other's  diameter  produced:  the 
two  tangential  triangles  so  formed,  will  be  equal. 


For,  draw  the  ordinate  ox.  Then 
By  aim.  triangles,  cd  :  ca  : :  cb  :  cir ; 
but,  by  theor.  7,    cd  :  ca  : :  ca  :  ct  ; 
theref.  by  equal,  ca  :  cb  : :  cb  :  ext. 

The  two  triangles  cet,  can  have  then  the  angle  c  com- 
mon, and  the  sides  about  that  angle  reciprocally  proportional ; 
those  triangles  are  therefore  equal,  viz.  the  Acet  =  A  can. 

q.  B.  D. 

CoroL  1.  Take  each  of  the  equal  triangles  cbt,  can, 
from  the  common  space  cape, 
and  there  remains  the  external  A  pat  =  A  pub. 

Cord.  8.  Also  take  the  equal  triangles  cbt,  can, 
from  the  common  triangle  cbd, 
and  there  remains  the  A  ted  =  trapez.  anbd. 


The  same  being  supposed  as  in  the  last  proposition ;  then  any 
lines  kq,  go,  drawn  parallel  to  the  two  tangents,  shall  also 
cut  off  equal  spaces. 


That  is, 
the  triangle  cbt  = 
the  triangle  can* 


THEOREM  XXI. 


That  is,  * 
the  akqg  =  trapez.  anho. 
and  AKf£  =  trapez*  ana£. 


F$  draw  the  ordinate  Djk  Then 
The  three  mm.  trinngl^VAW,  cdb,  oob9 
are  to  each  other  as      ca%  gd%  oe* ; 
th.  by  di? .  the  trap,  anbd  :  trap,  akho  : :  cd*~ca*  :  co*— CA*. 
Bor,  by  thear.  1,  ob*      t  «Qf : :  cb*— ca*,:  og&— 

theref.  by  equ.  trap.  axbb  :  trap,  akhq  : :  db"  :  oq\ 
Bat,  by  aim.  As,  tri.  tkd  :  tri*  kqg  i  :  bb*  :  ao? ; 
theref.  by  equal*  aned  tbd  : :  a»bg     :  boo. 

Bot|  by  cor.  3  theor.  20,  the  trap,  aitkd  .=  A  tbd  ; 

jind  therefore  the  trap,  anho  =  A  kqo. 
Ill  like  manner  the  trap.  A*hg  —  Aiff.    q.  b.  b. 

Carat.  1.  The  threo  apacea  abhg,  tkbg,  kqo  are  aD 
equal. 

ConL  3.   From  the  equals  akbg,  kqg, 
*       take  the  equ*la  anA^,  Kqg, 

'  and  there  remaina  gkua  =»  gfQG. 

Carol.  8.    And  from  the  equals  £Ahg,  £?qg, 
take  the  common  space  ^i.ho, 
and  there  remains  the  Alqh  =  A 14*. 

Cord.  4.    Again,  from  the  equals  kqg,  tbhg,  « 
take  the  common  space  klho, 
and  there  remaina  tklk  =  alqh.  • 


CoroZ.  5.  And  when  by 
the  lines  kq,  gh,  moving 
with  a  parallel  motion,  kq 
comes  into  the  position  ir, 
where  ca  is  the  conjugato 
to  Ca  ;  then 


the  triangle   kqg  becomes  the  triangle  ikc, 
and  the  space  ax  kg  becomes  the  triangle  axc  ; 
and  therefore  the  Ainc  -  aanc~  Atcc. 

Corol.  6.  Also  when  the  lines  kq  nnd  no,  by  moving  with 
a  parallel  motion,  come  into  the  position  re,  i*ef 
the  triangle     lqh  becomes  the  triangle  cm, 
i  nd  th  '  spac/;  tklk  l>ec<  mes  thi  triangle  tkc  ; 
and  theref.  the  acix  a  atkc  =  A  axc  »  Aibc. 

THKOKEX  XXn. 

Any  diameter  bisects  nil  its  double  ordinate*,  or  the  lines 
drawn  parallel  to  the  tangent  at  its  vertex,  or  to  its  'coojo- 
gate  diameter. 


or  TBI  HYtSUOLA. 


611 


That  is,  if  oq  be  paral- 
lel to  the  tangent  te,  or 
to  c* ,  then  shall  lq  =  Lq* 


For,  draw  qii.  qh  perpendicular  to  the  transverse. 
Then  by  cor.  3  theor.  21,  the  a  lqh  =?=  &Lqh  ; 
but  these  triangles  are  also  equimigiilar; 
conseq.  their  like  sides  are  oqual,  or  ui  =  Lq. 
Corel.*  1.    Any  diameter  divides  the  hyperbola  into  two 
equaj^parts. 

For,  the  ordinates  on  each  side  being  equal  to  each  other, 
and  equal  in  number;  all  the  ordinates,  or  the  urea,  oa  one 
side  of  the  diameter,  is  equal  to  all  the  ordinates,  or  the  area, 
on  the  other  side  of  it. 

Cord.  2.  In  like  manner,  if  the  ordinate  he  produced  to 
the  conjugate  hyperbolas  at  q',  q\  it  may  be  proved  that 
lq'  =  tq .  Or  if  the  tangent  te  be  produced,  then  kv  =ew. 
Also  the  diameter  gckh  bisects  all  lines 'drawn  parallel  to  tk 
or  oq,  and  limited  either  by  one  hyperbola,  or  by  its  two  con* 
jugate  hyperbolas. 

THBOREX  XXin. 

As  the  square  of  any  diameter 
Is  to  the  square  of  its  conjugate, 
So  is  the  rectangle  of  any  two  abscisses 
To  the  square  of  their  ordinate. 
That  is,  ce*  :  cc*  : :  el  .  lg  or  cxa  —  cb*  :  lq*. 
For,  draw  the  tangent 

te,  and  produce  the  ordi- 
nate ql  to  the  transverse 

at  k.    Also  draw  qh,  ex 

perpendicular  to  the  trans* . 

verse,  and  meeting  eg  in 

h  and  m.    Then,  similar 

triangles  being  as  the 

squares  of  their  like  sides, 

it  is, 

by  sim.  triangles,      £cet  :  A  cut : :  ce*  :  cl*  ; 

i 


aftay  division,        AflfT  :  tap.  tub  : :  on*  :  €»•  —  .«■'. 

Again,  by  sim.  tri.   |fli :  alqb  : :  cea;LQ9.  ^ 

Bat,  by  oor.  5  theor.  81,  the  Aoex  «*  a  err, 

and,  by  cor.  4  theor.  31,  the  Alqji    trap,  raw ; 

theref.  by  equality,  ©a8  :  or*  : :  cl8     en*  :  aa*, 

or •     •     •     os*  :  oe*  : :  bl  •  lo  :  141.  .     o»  a*  ft. 

Gorrf.  1.  The  squares  of  the  ordinatee  to  any  diaiajntar, 
are  to  one  another  aa  the  rectangles  of  their  respective  ab» 
actssee,  or  aa  the  difference  of  the  squares  of  the  eeau- dia- 
meter and  of  the  distance  between  the  ordinate  and  centre. 
For  they  ate  all  in  the  same  ratio  of  caf  to  ce". 

Carol.  8.  The  above  being  a  similar  property  lo  that  Be- 
longing to  the  two  axes,  all  the  other  properties  before  laid 
down,  for  the  axes,  may  be  understood  of  any  two  ronisyfe 
diameters  whatever!  using  only  the  oblique  onlinatee  af  these 
diameters  instead  of  the  perpendicular  ordinatee  of  the  exes ; 
namely,  all  the  properties  in  theorems  6, 7,  8, 16,  17,  SO,  SI. 

Carol.  8.  Likewise,  when  the  ordinates  are  continued  to 
the  conjugate  hyperbolas  at  a',  g\  the  same  properties  Ml 
obtain,  substituting  only  the  sum  for  the  difference  of  the 
squares  of  ce  and  cl,  ../ 
That  is,  cBf  :  ce*  : :  cl1  +  cb*  :  Wa.  1 
And  so  lq*  :  LQ*  : :  cl*—  cb*  :  cl1 -r 

Carol.  4.   When/  by  the  motion  of  La'  parallel  to  haal( 
that  line  coincides  with  ev,  the  last  corollary  becomes 
cb1.:  ce*  :  :  2c  K*  2  Bv*f 
or  ce*  :  bv*  :  :    1   :  2, 
or  ce  :  bv  2  1 
or  as  the  side  of  a  square  to  its  diagonal. 
That  is,  in  all  conjugate  hyperbolas,  and  all  their  dia- 
meters, any  diameter  is  to  its  parallel  tangent,  in  the  constant 
ratio  of  the  aide  of  a  square  to  ita  diagonal. 

THBOBEM  XXIV. 

If  any  two  lines,  that  any  where  intersect  each  other,  mast 
the  curve  each  in  two  points ;  then 

The  rectangle  of  the  segments  of  the  one  ^ 
Is  to  the  rectangle  of  the  segments  of  the  other, 
As  the  square  of  the  diam.  parallel  to  the  former 
To  the  square  of  the  diam.  parallel  to  the  latter. 


Or  THX  HYPRRB3LA. 


51S 


That  is,  if  cr  and 
cr  be  parallel  to  nny 
two  lines  phq,  pnq  ; 
then  shall  cr8  :  cr* : : 
fh  •  hq  :  pu  •  H£. 


For,  draw  the  diameter  ens,  and  the  tangent  tr,  and  its 
parallels  pk,  ri,  hii,  meeting  the  conjugate  of  the  diameter 
cr  in  the  points  t,  k,  i,  m.  Then,  because  similar  triangles 
are  as  the  squares  of  their  like  side*,  it  is, 

by  sim.  triangles,    cr3  :  of*  : :  Acai  :  Agpk, 

and        -       -       cr*  :  oh9  : :  Acri  :  A  cum  ; 

tlicref.  by  division,  cr*  :  op3  —  on' : :  cki  :  kpuh. 

Again,  by  sim.  tri.   ck*  :  ciia : :  Actk  :  A  cam  ; 

and  by  division,       cr1  :  c»3  —  ckj  : :  Acre  :  teiix. 
But,  by  cor.  5  theor.  21,  the  Acte  =  Acir, 
an  J  by  cor.  1  theor.  21,  tkiio  =  kph  j,  or  tehm  =  kphm  ; 
tlieref.  by  equ.  C*1 :  ch'-ck*  : :  rRJ  :  gp1  —  oh1  or  ph  .  hq. 
In  like  m  inner  ce!  :  chj-ck1  : :  cr1 :  pa  .  Hq. 
Tberef.  byeq'i.  cuJ :  cr1 : :  ph  .  hh  :  pH  .  Hfl.  q.  r.  d. 

Coral.  1.  In  like  minner,  if  any  other  line  p'fTf',  parallel 
to  cr  or  to  pq%  meet  phq  ;  since  th  >  rectangles  ph  q.  p  %iq' 
are  also  in  the  same  ratio  of  crj  to  crJ ;  therefore  the  rect. 
phq  :  pnq  :  :  pii'q  :  pn'q. 

Also,  if  another  line  p  Aq'  be  drawn  parallel  to  pq  or  cr  ; 
because  the  rectangles  p  Aq  ,  phq  are  still  in  the  same  ratio, 
therefore,  in  general,  the  rectangle  phq  :  pnq  : :  p'Aq'  :  phq'. 
That  id,  the  rectangles  of  the  p  irts  of  two  parallel  lines,  are 
to  one  another,  as  the  rectangles  of  the  parts  of  two  other 
parallel  lines,  any  where  intersecting  the  former. 

Cord.  2.  And  when  any  of  the  lines  only  touch  the  curve, 
instead  of  cutting  it,  the  rectangles  of  audi  become  squares, 
and  the  general  property  still  attends  them. 


Vol.  L 


66 


914 


Carol.  3.    And  hence  tb  :  re  : :  Is :  ft. 


THEOREM  XXV. 

If  a  line  be  drawn  through  any  point  of  the  curves,  parallel 
to  either  of  the  axes,  and  terminated  at  the  asymptotes ; 
the  rectangle  of  its  segments,  measured  from  that  point, 
will  1>e  equal  to  the  square  of  the  serai-axis  to  which  it  is 

parallel. 


That  is, 
the  rect.  iiek  or  n*K  =  ca\ 
and  reel,  hsk  or  hek  ca8. 


e 


For,  draw  al  parallel  to  ca,  and  «x  to  ca.  Then 
hy  the  parallels.     ca8  :  ca'or  al*  : :  cd8  :  dh*  ; 
and,  by  tlicor.  2,    ca8  :  c«*  : :  cd"— ca*  :  v*.9  ; 
theref.  by  subtr.     ca2  :  ca* : :  c%" :  dh8  —  de*  or  HEX* 
But  the  antecedents       ca3,  ca8  are  equal, 
theref,  the  consequents  ca2,  hex  must  also  be  equal* 

In  like  manner  it  is  again, 
by  the  parallels,  ca3  :  ca2  or  al3  : :  cdj  :  dh>  ; 
and  by  theor.  3,  ca3  :  ca3  : :  cd3  +  cas  :  ne*  ; 
there!,  by  subtr.  ca3  :  ca3  : :  ca3  :  ne3  —  dh3  or  hjk. 

But  the  antecedents  ca3,  ca3  are  the  same, 

theref  the  conseq.  ca3,  hck  must  be  equal. 

In  like  manner,  by  changing  the  axes,  is  hsk  or  hek  =  ca** 

Corol.  1.  Because  the  rect.  hek  =  the  rect.  h«k. 
therefore  eh  :  en  :  :  en  :  ek. 
Aud  cxma&^iftaxYy     \&*ta*Y*J  greater  than  He. 


OF  THE  ltVF*XBOLA. 


MS 


CSdro/.  ft.  the  rectangle  Ark     (he  rect.  hb*, 
for,  by  aim.  tri.  feA  :  6k  : :  e& :  EX. 

8CHOLIUM. 

ft  is  evident  that  thii  proposition  is  general  for  any  line 
oblique  to  the  axis  aha,  namely,  that  the  rectangle  (if  the 
seg  n  mta  of  any  line,  cut  by  ttoe  curve,  and  t  originated  by  the 
asymptotes,  is  e.p*l  to  tfhe  squ  ire  of  the  semi-diamHter  to 
which  the  line  is  parallel.  Since  the  demonstration  is  drawn 
from  properties  that  are  common  to  art  diameters. 

THEOREM  zxvi. 

All  the  rectangles  are  eqiml  which  are  made  of  the  seg. 
mints  of  any  parallel  lines  cut  by  the  curve,  and  limited 
by  the  asymptotes. 


For,  each  of  the  rectangles  hex  or  hsk  is  equal  to  the 
squire  of  the  parallel  semi-diamater  c? ;  and  each  of  the  rect- 
angles huh  or  hek  is  oqu  il  to  the  sqi  ire  of  the  p.inllel  semi* 
diameter  oi.  and  therefore  the  rectangles  of  the  segments 
of  all  parallel  4ines  are  equal  to  one  another.  q.  k.  d. 

C)rol.  1.  The  rectangle  hrk  being  constantly  the  same, 
whether  the  point  R  is  taken  on  the  one  side  or  the  other  of 
the  point  of  contact  i  of  the  tangent  parallel  to  iik,  it  follows 
that  the  parts  uk,  kk,  of  any  such  line  hk,  are  equal. 

And  because  the  rectangle  HtK  is  constant,  whether  the 
point  e  is  taken  in  the  one  or  the  other  of  the  opposite  hy- 
perbolas, it  follows,  that  the  parte  He,  k«,  are  also  equal. 

Ctr&L  2.  And  when  hx  crimes  into  the  position  of  the 
tangent  mi,  the  last  corollary  becotftds  il  =  id,  arid  lit  —  in, 
and  lm  =  dn. 

Hence  also  the  diameter  cm  bisect*  all  the  parallels  to  dl 
which  are  terminate  J  by  the  asymprto,  a&outj  yav  — 


Carol.  8.  From  the  proposition,  and  the  bet  corollary,  it 
follows  that  the  constant  rectangle  hkk  or  khk  hi  *=  il*.  And 
the  equal  constant  rect.  ueK  or  me  =  mut  or  ix9  —  uP. 

Coral.  4.  And  hence  il  =  the  parallel  setni-diameter  cs- 
For,  the  rect.KHE  =  il*, 
and  the  equal  rect.  ees  =  in"  —  il*, 
theref.  il*  =«"  —  iL*f  or  n>  =  2iLa  ; 
but,  by  cor.  4  tbeor.  23,  is*  ■=  2cs>  9 
and  therefore     •  il   =  c*. 

And  an  the  asymptotes  pass  through  the  opposite  angles  of 
all  the  inscribed  parallelograms. 

THEOBB3I  XXVn. 

The  rectangle  of  any  two  lines  drawn  from  any  point  ia 
the  curve,  parallel  to  two  given  lines,  and  limned  by 

the  asymptotes,  is  a  constant  quuntity. 

That  i«,  if  ap,  eg,  pi  be  parallels, 
as  also      AQi  kk,  dm  p;irallelf, 
then  shall  the  rect.  pap.  =  rect.  gek  =  red.  ira. 


For,  produce  ke,  md  to  the  other  asymptote  at  u»,  l. 

Then,  by  the  parallels,  me  :  <;e  : :  ld  :  id  ; 

but       -       -       -     ek  :  ek  : :  dm  :  dm  ; 

theref.  the  fectangle  hkk  :  gek  :  :ldm  :  idm. 

But,  by  the  last  thwr.  the  rect.  hkk  =  ldm  ; 

and  therefore  the  rect.    gek  =  idm  =  paq.         q.  a.  a. 

THEOREM  XXVIII. 

Every  inscribed  triangle,  formed  by  any  tangent  and  the 
two  inter*  epted  parts  of  the  asymptotes  is  equal  lo  a 
constant  quantity  ;  namely,  double  the  inscribed  paral- 
lelogram. 

Thai  \s,  lYte  \x\*Ng&  ct%  —  % 


or  «m  nraaou. 


•17 


For,  since  the  tangent  ts  is 
bisected  by  the  point  of  contact 
e,  (th.  26,  cor.  2),  nnd  kk  is 
parallel  to  tc,  and  ge  to  ck  ; 
therefore  ck,  hs,  ge,  are  all 

equal,  as  are  also  co,  gt,  kk.   ^ — ,   

Consequently  the  triangle  urB      C  JC  g 

=  the  triangle  kes,  and  each  equal  to  half  the  constant  in- 
scribed parallelogram  gk.  And  therefore  the  whole  triangle 
CT8,  which  is  composed  of  the  two  smaller  triangles  and  the 
parallelogram,  is  equal  to  double  the  constant  inscribed  paral. 
lelogram  gk.  q.  e.  d. 

TnEOREJf  XXIX. 

If  from  tho  point  of  contact  of  any  tangent,  and  the  two  in- 
tersections  of  the  curve  with  a  line  parallel  to  the  tangent, 
three  parallel  linen  be  drawn  m  any  direction,  and  ter- 
minated by  either  asymptote  ;  those  three  lines  shall  be 
in  continued  proportion. 

That  is*  if  hkm  and  the 
tangent  1 1*  be  parallel,  then 
are  the  parallels  dh,  ei, 
ok  in  continued  propor- 
tion. 

C  D    E  L 
For,  by  the  parallels,  ei  :  il  : :  dh  :  nx ; 
and,  by  the  same,      ei  :  il  : :  gk  :  m  ; 
thoref.  by  compos,   ei9  :  il9  : :  dh  .  gk  :  hxx  ; 
but,  by  theor.  26,  the  rect.  hxr  =  il*  ; 
and  theref.  the  rect.    dh  .  ok  s  ei1, 
or       -       •  dh  :  ei  : :  ei  :  gk.         q.  e.  d. 

theorem  xxx. 

Dr.iw  the  semi-diameters  ch,  cix,  ck  ; 
Tneu  shall  the  sector  chi  ^  the  sector  cik. 


For,  because  hk  and  all  its  parallels  are  bisected  by  cis, 
therefore  the  triangle   c.\h  =  tri.  cxk% 


■If 


and  the  segment        wm  »  aeg,  nm  f 
consequently  the  sector  ao  =  sec.  cik. 

Carol.  If  the  geometrical  proportional*  hh,  mm9  w  be 
parallel  to  the  other  asymptote,  the  spaces  drib,  biko  wiB 
be  equal ;  for  they  are  equal  to  the  equal  sectors  chi,  cik. 

So  that  by  taking  any  geometrical  proportionuU  cd,  cm, 
go*  4tc.  and  drawing  dm,  bi,  «k,  &c.  parallel  to  the  other 
asymptote,  as  also  the  radii  uh.  ci,  ck  ; 

then  the  sectors  chi,  cut,  dec 

or  the  space*  dhik,  eiku,  dec.  1 

will  be  all  equal  among  themselves. 

Or  the  sectors  chi,  chx,  &c. 

or  the  spaces  dhir,  dhko,  dtc. 

will  be  in  nrithmeticaj  progression. 
And  therefore  these  sectors,  or  space*,  wilt  be  analogous  to 
the  logarithms  of  the  lines  or  bases  cd,  ck,  cu,  dsc*  }  namely, 
cm  or  dbib  the  log.  of  the  ratio  of 

co  to  ck,  or  of  cs  to  cg,  dec. ;  or  of  ei  to  dii,  or  of  gk  to  si,  Ac  ; 
and  chk  or  phk«;  the  log.  of  the  ratio  of  cd  to  co,  die. 
or  of  ok  to  dh,  Sic. 


OF  THE  PARABOLA. 


THEOREM  I. 

The  Abscisses  are  proportional  to  the  Squares  of  their 
Ordinates. 

Let  avm  be  a  section  through 
the  axis  of  the  cone,  and  agih  a 
parabolic  section  by  n  plane  per. 
pendicular  to  the  former,  and 
parallel  to  the  side  vm  of  the 
cone  ;  also  let  afh  be  the  com. 
mon  intersection  of  the  two 
planes,  or  the  axis  of  the  para- 
bola,  and  fg,  hi  ordinates  per- 
pendicular  to  it. 

Then  it  will  be,  as  ap  :  ah  : :  fg*  :  Hif. 
For,  through  the  ordinates  fg,  hi,  draw  the  circular  sec- 
tions, kgl,  min,  parallel  to  the  base  of  the  cone,  having  kl, 
MR  for  their  diamctera,  \o         yg^  hi  ace  ordinates,  as  well 
as  to  the  axis  of  \ta  ^itoVhA*. 


OF  THJB  PAJUBALA.  619 

Then,  by  similar  triangles,  af  :  ah  : :  fl  :  hn  ; 
but,  because  of  the  parallels,  kf  =  mh  ; 

therefore      -       -       -       af  :  ah  : :  kf  .  fl  :  mh  .  hn. 
But,  by  the  circle,  kf  .  fl  =  FG2/and  mh  .  hn  —  hi1  ; 
Therefore    -       -       -       af  :  ah  : :  fg9  :  hi9  .  o,.  E.  d. 

PqS  hi' 

Carol.  Hence  the  third  proportional  —  or  —  is  a  con* 

r    r  AF  AH 

stant  quantity,  and  is  equal  to  the  parameter  of  the  axis,  by 
defin.  16. 
Or  af  :  fg  : :  fo  :  f  the  parameter. 
Or  tho  rectangle  p  .  af  =  fg9. 


THEOREM  II. 


As  the  Parameter  of  the  Axis  : 
Is  to  the  Sum  of  any  Two  Ordinates  : : 
So  is  the  Difference  of  those  Ordinates  : 
To  the  Difference  of  their  Abscisses. 

That  is, 
f  :  gh  +  db  : :  gii  —  de  :  dg, 
Or,  p  :  ki  : :  ih  :  ie. 


For,  by  cor.  theor.  1,  p  .  ag  gh9, 
and       -       •       -      p  .  ad  -=  de9  ; 
theref.  by  subtraction,    p  .  dg  =  gh9  —  db9. 
Or,      -       -       •      p  .  dg  =  ki  .  ih, 
therefore       -       -      p  :  Kt  :  :  ih  :  dg  or  ei.        q.  e.  d. 

Cord.  Hence, because  p  .  ei  =  ki  .  ih* 
and,  by  cor.  theor.  1,     p  .  ag  —  gh9, 
therefore       -       -      ag  :  ei  : :  gh9  :  ki  •  ih. 

So  that  any  diameter  ei  is  as  the  rectangle  of  the  segments 
ki,  ih  of  the  double  ordinate  kh. 


theorem  hi. 


The  Distance  from  the  Vertex  to  the  Focus  is  equal  to  J  of 
the  Parameter,  or  to  Half  the  Ordinate  at  the  Focus. 


That  is, 
af  -  Jfe  =  {r, 
where  f  is  the  focus. 


590  O0XIC  tKCTIOXfl* 

For,  the  genera!  property  is  af  :  fb  : :  rmi  f. 

But,  by  definition  17,     -     fe  *  \r  ; 

therefore  also      -  at  =  Jfe  =  Jr.        q.  b*  d» 


TBKORBM  IV. 


A  Line  drawn  from  the  Focus  to  any  Point  in  the  Curve,  is 
equal  to  the  Sum  of  the  Focal  Distance  and  the  Absciss 
of  the  Ordinate  to  that  Point.  . 

6 

That  is, 

FE  =  FA  +  AD  =  GD, 

taking  ao  ~  af. 


For,  since  fd  =  ad  ^  af, 


theref.  by  squaring, 
But,  by  cor.  theor.  1, 
theref.  by  addition, 
But,  by  right-ang.  tri. 
therefore 

and  the  root  or  side  is 
or  - 


FD'  •=»  AF8  -  2AF  .  Ad  +  AD*, 
DEa  =  P  .  AD  -  4AF  .  AD  ; 
FD5  +  DK3  =  AF1  +  2AP  .  AD  +  AD*. 
FDfl  +  DEa  =  FE*  J 
FE2  =  AFa  +  2\F  .  AD  +  AD*, 
FE   =  AF  +  Al>, 

fk  =t  gd,  by  taking  ag  =  af. 

u.  E.  D. 

Carol  1.  If,  through  the  point  g,  the  HHH  G»  HHH 
line  on  be  drawn  perpendicular  to  the 
axis,  it  in  called  the  directrix  of  the 
parabola.*  The  property  of  which, 
from  this  theorem,  it  appears,  in  this  : 
That  drawing  any  lines  he  parallel  to 
the  axis,  he  is  always  equal  to  fe  the 
distance  of  the  forus  from  the  point  e. 

Corol.  2.  Hence  also  the  curve  is  easily  described  by  peinls. 
Namely,  in  the  axis  produced  take  ag  =  af  the  focal  dis- 
tance, and  draw  a  number  of  lines  ee  perpendicular  to  the 
axis  ad;  then  with  the  distances  gd,  gd,  gd,  dec.  as. radii, 
and  the  centre  f,  draw  arcs  crossing  the  parallel  ordi nates 
in  e,  e,  f.,  ©zc.  Then  draw  the  curve  through  all  the  points 
E,  s,  K. 


l  5 — ! 


*  Rach  of  the  other  conic  sections  has  n  directrix  ;  hut  the  conside- 
ration of  it  dotttnoA  nccwT  \\\  v\w  tftttfatat«<tm^taY?«dof  tavetUgstinf 
the  general  properties  ©A  \\\«  cwv«*. 


Of  TBI  PAJUIOLA. 


«1 


THEOREM  V. 


If  a  Tangent  be  drawn  to  any  Point  of  the  Parabola,  meet- 
ing the  Axis  produced;  and  if  an  Ordinate  to  the, Axis 
be  drawn  from  the  point  of  Contact;  then  the  Absciss  of 
that  Ordinate  will  he  equal  to  the  external  Part  of  the 
Axis,  measured  from  the  Vertex. 


That  is, 
if  tc  touch  the  curve 
at  the  point  c, 
then  is  at  =  ah. 


Let  cc,  an  indefinitely  small  portion  of  a  parabolic  curve, 
be  produced  to  meet  the  prolongation  of  the  axis  in  t  ;  and 
let  cm  be  drawn  parallel  to  ex,  and  cs  parallel  to  ag  the 
axis.    Let,  also,  p  =  parameter  of  the  parabola. 

Then,  by  aim.  tri.  cs  :  sc  : :  cm  :  ma  -f-  at  =  mt, 

MT  •  CS 

.\  cs  =  . 

CM 

Also,  th.  1.  cor.  p  .  Am  =  mc*  =  ms*  +  2ms  .  sc  +  sc*, 

=  mc*  -f  2mc  .  sc  +  sc1, 
and  p  .  am  =  mc'. 

Consequently,  omitting  sc1  as  indefinitely  small,  and  sub* 
trading  the  latter  equa.  from  the  former,  we  have 
p  .  (aju  —  am)  ="  p  .  cs  =  2cs  .  mc  : 
or,  substituting  for  cs  its  value  above, 


mt  .  cs 


=  2cs .  mc  ; 


or  p  .  MT  =  2mc*  : 
Consequently,  mt  • 


CM 

:2p  .  AM  (th.  1.) 

=  2am,  and  ma  =  at. 


Q.  E.  D. 


THEOREM  VI. 


If  a  Tangent  to  the  Curve  meet  the  Axis  produced  ;  then 
the  Line  drawn  from  the  Focus  to  the  Point  of  Contact, 
will  be  equal  to  the  Distance  of  the  Focus  from  the  Inter- 
section of  the  Tangent  and  Axis. 
Vol.  I.  07 


east 


coanc  sBcnsjs** 


That  i*, 
tv  ss.  rr. 


K  <* 

For,  draw  the  ordinate  vc  to  the  point  of  contact  c 

Then,  hy  theor.  5,  .\r  =  ad  ; 
therefore        •        ft  ~  af  +  ad. 
Kut,  by  theor.  4.      fc  =  af  +  ad  ; 

thcref.  by  equality,    fc  —  ft.  Q-  b.  d. 

Corol.  1.  If  ro  be  drawn  perpendicular  to  th*  curve,  or  to 
the  tangent,  at  c  ;  then  Khali  kg  =  fc  =  FT. 

For,  draw  rii  perpendicular  t )  tc,  which  will  also  bisect 
tc,  because  ft  =  fc  ;  and  therefore,  hy  the  nature  of  the 
pantile!*,  fii  ulso  bisects  tg  in  f.  And  consequently  fg  = 
ft  —  fc. 

So  tli  it  f  is  the  centre  of  a  cire'e  passing  through  t,  c,  g. 

Corol.  2.  The  subnormal  dg  is  a  constant  quantity,  and 
equal  to  half  the  parameter,  or  to  2af,  double  the  focal 
distance.    For,  since  ice;  is  a  right  angle, 
therefore  1 1>  or  <Jad  :  dc  :  :  dc  :  dg  ; 
but  by  the  def    ad  :  dc  : :  dc  :  parameter  ; 
therefore  do  =  half  the  parameter  =  2 aw 

Corel.  3.  The  tangent  at  the  vertex  an,  is  a  mean  propor- 
tional between  AFand  ad. 
For,  because  fiit  is  a  right  angle, 
therefore     -     ah  is  a  mean  between  af,  at, 
or  I  etween  -     af,  ad,  because  ad  =  at. 
Likewise,    -    fii  is  a  mean  between  fa,  ft, 
or  between  fa,  tc. 

Corol.  4.  The  tangent  tc  makes  equal  angles  with  fc  and 
the  axis  ft  ;  as  well  as  with  fc  and  ci. 
For,  because  ft  =  fc, 
Therefore  the  L  fct  =  L  ftc. 
Also,  the  angle  c.cf  -=  the  angle  gck, 
drawing  ick  parallel  to  the  axis  ag. 

Corol.  5.  And  because  the  angle  of  incidence  gck  is  =* 
the  angle  of  reflection  gcf  ;  therefore  a  ray  of  light  falling 
on  the  curve  in  the  direction  kc,  will  be  reflected  to  the  focus 
f.  That  is,  all  rays  parallel  to  the  axis,  are  reflected  totbs 
focus,  or  burning  uuuvx* 


Or  THE  PAS  ABOLA. 


62* 


THEOREM  VII. 

If  there  be  any  Tangent,  and  a  Do'ihle  Ordinate  c'riwn 
from  the  Point  of  Contact,  and  also  any  Line  parallel  to 
the  Axis,  limited  by  the  Tangent  and  Double  Ordinate  : 
Then  ahull  the  Curve  divide  that  Line  in  the  sum;  Ratio 
as  the  Line  divides  the  Double  Ordinate. 


That  is. 
ie  :  ek  :  ;  ck  :  kl. 


For,  by  sim.  triangles,  cx  :  ki  : :  cd  :  dt  or  2da  ; 
but,  by  the  def.  the  paratn.  p  :  cl  : :  <  o  :  2da  ; 
therefore,  by  equality,        p  :  ck  : :  «x  :  ki. 
•  But,  by  theor.  2,  v  :  ck  ::kl:rr; 

therefore,  by  equality,       cl  :  kl  :  :  ki  .  kb  ; 
and,  by  division,       •      ck  :  kl  :  ;  ie  :  ek.  q.  e.  d. 

THEOREM  VIII. 

The  same  being  supposed  as  in  theor.  7  ;  then  shall  the 
External  Part  of  the  Line  between  the  Curve  and  Tun- 
gen*,  be  proportioual  to  the  Square  of  the  intercepted  Part 
of  the  Tangent,  or  to  the  Square  of  the  intercepted  Part 
of  the  Double  Ordinate. 


That  is,  ie  is  as  ci*  or  as  ck', 

and    IK,    TA,    ON,   PL,  C2C. 

are  as  ci3,  ct',  co*,'cf3,  die. 
or  as  ck3,  cd9,  cm3,  cl*,  &c. 


For,  by  theor.  7,  ie  :  ek  : :  ck  :  kl, 
or,  by  equality,       ie  :  kk  : :  ck2  :  ck  .  kl. 
But,  by  cor.  th.  2,  ek  isai  the  rect.  ck  .  kl, 
therefore       -       ik  id  as  ck3,  or  as  ci3.    Q.  e.  d. 

Cord.  As  this  property  is  common  to  every  position  of 
the  tangent,  if  the  lines  ie,  ta,  o\,  due.  be  appended  on  the 
points  i,  r,  o,  dtc.  and  moveable  about  ihetn,  and  of  such 
lengths  as  that  their  extremities  k,  a,  n,  &c.  be  in  the  curve 
of  a  pa  rub  da  in  some  one  position  of  the  tangent ;  Ineu 
making  the  tangent  revolve  about  the  point  c,  u  ui»v«u.i* 


694 


CONIC  SBCTKKCS* 


that  the  extremities  e,  a,  h,  dee.  will  always  fern  the  cum 
of  some  parabola,  in  every  position  of  the  tangent. 


THXORXH  u. 

,  The  Abscisses  of  any  Diameter,  are  as  the  Squares  of  their 
Ordinates. 


That  is,  cq,  cr,  csg&c. 
are  as  qr1,  ra*,  sn*,  &c. 
Or     cq,  :  cr  : :  qjb1  :  ras, 
&c. 


For,  draw  the  tangent  ct,  and  the  externals,  si,  at,  it o, 
die.  parallel  to  the  axis,  or  to  the  diameter,  cs. 

Then,  because  the  ordinates,  qe,  ka,  sn,  6lc.  are  parallel 
to  the  tangent  ct,  by  the  definition  of  them,  therefore  all 
the  figures  iq,  tk,  os,  dtc.  are  parallelograms,  whose  op- 
posite sides  arc  equal ; 

namely,       -       •      ^k,  ta,  on,  dec. 

are  equal  to         -       cq,  cr,  cs,  dtc. 

Therefore,  by  theor.  8,  cq,  cr,  cs,  &c. 

are  as         -       -  \    ci3,  ct2,  coa,  die. 

or  as  their  equals  -       qk2,  ha*,  sn%  &c.  q.  k.  d* 

Cord,  Here,  like  as  in  theor.  2,  life  difference  of  the  ah* 
scisses  is  as  the  difference  of  the  squares  of  their  ordinates, 
or  as  the  rectangles  under  the  sum  and  difference  of  the 
ordinates,  the  rectangle  of  the  sum  and  difference  of  the 
ord mutes  being  equal  to  the  rectangle  under  the  difference 
of  the  abscisses  and  the  parameter  of  that  diameter,  or  a# 
third  proportional  to  any  absciss  and  its  ordinate. 


THEOREM  X. 

If  a  Line  be  drawn  parallel  to  any  Tangent,  and  cut  the 
Curve  in  two  Points ;  then,  if  two  Ordinates  be  drawn  to 
the  Intersections,  and  a  third  to  the  Point  of  Contact, 
those  three  Ordinates  will  be  in  Arithmetical  Progression, 
or  the  Sum  of  the  Extremes  will  be  equal  to  Double  the 
Mean. 


Or  Till  FABABA&A.  888 


That  is, 

BO  +  HI  =•  2CD. 


For,  draw  bk  parallel  to  the  axis,  and  produce  hi  to  &• 
Then,  by  aim.  triangles,  kk  :  hk  : :  tb  or  2ap  :  cd  ; 
but,  bu  theor.  2,      -     bk  :  hk  : :  kl  :  r  the  param. 
thereu  by  equality,      2ad  :  kl  : :  cd  :  p. 
But,  by  the  defin.        2ad  f  2cd  : :  cd  :  t» ; 
theref.  the  2d  terms  are  equal,  kl  =  2cd, 
that  is,       .       .       bo  +  hi  =  2cd.   q.  b.  d. 

Carol.  When  the  point  b  is  on  the  other  side  of  ai  ;  then 
hi  —  ob  =  2cd. 


THEOREM  XI. 

Any  diameter  bisects  all  its  Double  Ordinates,  or  lines 
parallel  to  the  Tangent  at  its  Vertex. 


• 

That  is, 


T 

H  X 
jj  X 

For,  to  the  axis  ai  draw  the  ordinates  eg,  cd,  hi,  and  M5 
parallel  to  them,  which  is  equal  to  cd.  ♦ 
Then,  by  theor.  10,  2mn  or  2cd  =  eg  +  hi, 
therefore  m  is  the  middle  of  eh. 

* 

And,  for  the  same  reason,  all  its  parallels  are  bisected. 

Q.  b.  D. 

Schol.  Hence,  ns  the  abscisses  of  any  diameter  and  their 
ordinates  huve  the  same  relations  as  those  of  the  axis,  namely, 
that  the  ordinates  nre  bisected  by  the  diameter,  and  their 
squares  proportional  to  the  abscisses  ;  ho  all  the  other  pro- 
perties of  the  axis  and  ||s  ordinates  and  abscisses,  before  da* 
monst  rated,  will  likewise  hold  good  for  any  diameter  and  its 
ordinates  and  abscisses.   And  also  those  of  the  parameters^ 


cone  ascnoss. 


understanding  the  parameter  of  any  diameter,  as  a  third  pio- 
portional  to  uny  absciss  and  its  ordinate.  Some  of  the  most 
materia]  of  which  are  demonstrated  in  the  tour  following 
theorems. 

TUEORXTl  III. 


The  Parameter  of  any  Diameter  is  equal  to  four  Times  the 
Line  drawn  from  the  »  ocus  to  the  Vertex  of  that  Diane* 
ter. 


M  N 


For.  draw  the  ordinate  m  i  parallel  to  the  tangent  ct  :  also 
cd,  perpendicular  to  the  axis  a.n,  and  fh  perpendicular  to 
the  tangent  ct. 

Then  the  abscisses  ad,  cm  or  at,  being  equal,  by  theor.  5, 
the  parameters  will  be  as  the.  squares  of  the  ordinate;?  co,  xa 
or  ct,  by  the  definition  ; 

that  is,       .       -     !•:/)..  cds  .  ct*, 

But  by  sim.  tri.  -  fii  :  ft  :  :  co   :  ct  ; 

therofore    -       .  v  :  p   :  :  fii*  .  ft*. 

But,  by  cor.  3,  th.  6,  fii3  =-  fa  .  ft  ; 

therefore    -       •  i»  :  p  : :  fa  .  ft  :  ft*  ; 

or,  by  equality,   -  v  :  p  : :  i  a  :  ft  or  fc 

Bui.  by  theor.  3,  p  =  4 fa, 

and  therefore     -  p  ~  4ft  or  4fc.         q.  e.  d. 

Cord.  Hence  the  parameter  p  of  the  diameter  cm  is  equal 
to  4fa  +  4ad,  or  to  p  +  4ad,  that  is,  the  parameter  of  the 
axis  added  to  4a o. 


THEOREM  XIII. 

If  an  Ordinate  to  any  Di:i meter  pass  through  the  Focun,  it 
will  be  equal  to  Half  Us  Parameter  ;  and  its  Absciss  equal 
to  One  Fourth  ot  vYv&  torm*  Vaxvuc&vwu 


OF  TUX  PARABOLA. 


an 


That  is,  cm  =  lp, 
and    me  =  \p. 


For,  join  fc,  and  draw  the  tangent  ct 
By  (he  parallels,    cm  =  ft  ; 
and,  hy  theor.  6,    fc  =  ft; 
also,  by  theor.  12,  fc  =  }p ; 
therefore    -   -     cm  =  Jp. 
Again,  by  the  defin.  cm  or  jp 


MF. 


MR 


£.  D. 


and  consequently     me  =  jp  =  2cm. 

Corel.  1.  Hence,  of  any  diameter,  the  double  ordinate 
which  passes  through  the  focus,  is  equal  to  the  parameter,  or 
to  quadruple  its  absciss. 

C  rol.  2.  flence,  and  from  cor  1, 
to  theor.  4,  and  theor.  6  and  12,  it 
appears,  that  if  the  directrix  on  be 
drawn,  and  any  lines  he,  he,  paral- 
lel to  the  axis ;  then  every  parallel 
he  will  he  equal  to  ef,  or  \  of  the  pa- 
rameter  of  the  diameter  to  the  point  e. 


THEOBKM  XIV. 


If  there  be  a  Tangent,  and  any  Line  drawn  from  the  Point 
of  Contact  and  meeting  the  Curve  in  some  other  Point,  as 
also  another  Line  parallel  to  the  Axis,  and  limited  by  the 
First  Line  and  the  Tangent :  then  shall  the  Curve  divide 
this  Second  Line  in  the  same  Ratio  as  the  Second  Line 
divides  the  First  Lino. 


That  is, 
ie  :  ek  :  :  ck  :  KL. 


For,  draw  lp  parallel  to  ik,  or  to  the  axis. 

Then  by  theor.  8,  ne  :  fl  :  :  ci*  :  cf% 

or,  by  sini.  tri.    -  ib  :  fl  : :  ck(  :  cl\ 

Also,  by  sim.  tri*  ik  :  fl  : :  ck  :  cl, 

or      -      -      -  ik  ;  fl  : :  ck*  :  ck  •  cl  ; 


9 


638  como  octioni.  * 

therefore  by  equality,  ir  :  ik  : :  ck  .  cl  :  cl"  ; 
or      -  -     ie  :  ik  :  :  ck  :  cl  ; 

and,  by  division,        ie  :  bk  : :  ck  :  kl.    a.  r.  d% 
Cord.  When  ck  =  kl,  then  ie  =  bk  =  Jik. 

TneoBBX  xv. 

If  from  any  Point  of  the  Curve  there  be  drawn  a  Tangent, 
and  also  Two  Right  Line*  to  cut  the  Curve  ;  and  Dia- 
meters be  drawn  through  the  Points  of  Intersection  b  and 
i.t  meeting  those  Two  Right  Lines  in  two  other  Prints  o 
and  k  :  then  will  the  Line  kg  joining  these  last  Twe 
Points  be  parallel  to  the  Tangent. 


For,  by  theor.  14,  ck  :  kl  ::  ei  :  kk  ; 
and  by  composition,  ck  :  ci.  ::  ki  :  ki  ; 
and  by  the  paiallels  ck  :  cl  ::  oh  :  lh. 
Hut,  by  aim.  tri.  -  ck  :  cl  : ;  ki  :  lh  ; 
theref.  by  equal.  -  ki  :  lh  : :  gu  :  lh  : 
consequently        -    ki  =  oh, 

and  therefore       -    kg  is  parallel  and  equal  to  t h.    q*  b.  b. 

TIIKOREM  xvi. 

If  an  ordinate  be  drawn  to  the  point  of  contact  of  any  tan- 
gent, and  another  ordinate  produced  to  cut  the  tangent ; 
it  will  be,  as  the  difference  of  the  ordinates 

Is  to  the  difference  added  to  the  external  part, 

So  is  double  the  first  ordinate 

To  the  sum  of  the  ordinates. 

That  is,  kh  :  ki  :  :  kl  :  KG. 


For,  by  cor.  \,  faew.  \,  *  \  xvc  -» *.  dc  :  da. 


OF  THE  PARABOLA. 


529 


and      -       .      -      p  :  2dc  : :  dc  :  dt  or  2da. 

Hut,  by  aim.  triangles,  ki  :  kc  : :  dc  :  dt  ; 

therefore,  by  equality,    j»  :  2dc  : :  ki  :  kc, 

or,       -       .       -        p  :  ki  : :  kl  :  kc. 

Again,  by  theor.  2,        p  :  kh  : :  kg  :  kc  ; 

1  he  re  fore  by  equality,   kh  :  ki  : :  kl  :  kg.  q.  e.  d. 

Carol.  1.    Hence,  by  composition  and  division, 
it  is,  kh  :  ki  : :  gk  :  gi, 
and  hi  :  hk  : :  hk  :  kl, 
also  ih  :  ik  :  :  ik  :  ig  ; 

that  is,  ik  is  a  mean  proportional  between  ig  and  ih. 

Carol.  2.  And  from  this  last  property  a  tangent  cun  easily 
be  drawn  to  the  curve  from  any  given  point  i.  Namely, 
draw  ihg  perpendicular  to  the  axis,  and  take  ik  a  mean  pro- 
portional between  ih,  ig  ;  then  dmw  kc  parallel  to  the  axis, 
and  c  will  be  tbe  point  of  contact,  through  which  and  the 
given  point  i  the  tangent  ic  is  to  be  drawn. 

THEOREM  XVII. 

If  a  tangent  cut  any  diameter  produced,  and  if  an  ordinate 
to  that  diameter  be  drawn  from  the  point  of  contact ; 
then  the  distance  in  the  diameter  produced,  between  the 
vertex  and  the  intersection  of  the  tangent,  will  be  equal 
to  the  absciss  of  that  ordinate. 

That  is,  ie  =  ek. 
For,  by  the  last  th.  is :  ek  : :  ck  :  kl. 
But,  by  theor.  11,  ck  =  kl, 
and  therefore        ie  —  ek. 


Coral.  1.  The  two  tangents  ci,  li,  at  the  extremities  of 
any  double  ordinate  cl,  meet  in  the  same  point  of  the  dia- 
meter of  that  double  ordinate  produced.  And  the  diameter 
drawn  through  the  intersection  of  two  tangents,  bisects  the 
line  connecting  the  points  of  contact. 

CoroL  2.  Hence  we  have  another  method  of  drawing  a 
tangent  from  any  given  point  i  without  the  curve.  Namely, 
from  i  draw  the  diameter  ik,  in  which  take  ek  =  ei,  and 
through  k  draw  cl  parallel  to  the  tangent  at  e  ;  then  c  and  L 
are  the  points  to  which  the  tangents  must  be  drawn  from  i. 

THEOREM  XVIII. 

If  a  line  be  drawn  from  the  vertex  of  any  diameter,  to  cut 
the  curve  in  some  other  point,  and  an  ot$voaX«  >taoX 
Vox.  /.  68 


580 


conic  tKcnoirt. 


diameter  be  drawn  to  that  point,  as  also  another  ordinate 
any  where  cutting  the  line,  both  produced  if  necessary : 
'i  he  three  will  be  continual  proportionals,  namely,  the  two- 
ord. nates  and  the  part  of  the  latter  limited  by  the  said  line 
drawn  from  the  vertex. 

That  is,  de,  6H,  01  are 
crntinual  proportionals,  or 
de  :  gh  :  :  gh  :  gi. 


For,  by  thcor.  9,  -  -  .  de8  :  gh*  : :  ad  :  ao  ; 
i  ml,  by  sim.  tri.  -  -  -  de  :  oi  : :  ad  :  ag  ; 
theref.  by  equality,  -  -  de  :  gi  : :  hk*  :  gh9, 
that  is,  of  the  three  de,  gh,  ci,  1st :  3d  : :  1st*  :  2d*, 

therefore  1st :  2d   : :  2d  :  3d,   \  7  y 

that  is,  de  :  Grr  : :  gh  :  gi.      q.  e.  d. 

Cbrol.  1.  Or  their  equals  gk,  gh,  gi,  are  proportionals  ; 
where  ek  is  parallel  to  the  diameter  ad. 

CoroL  2.    Hence  it  is  de  :  ag  : :  p  :  gi,  where  p  is 
the  parameter,  or         ag  :  gi  :  :  de  :  p. 
For,  by  the  dcfiu.        ag  :  gh  :  :  gh  :  p. 
Cord.  3.    Hence  also  the  three  mn,  mi,  mo,  are  propor- 
tionals, where  mo  is  parallel  to  the  diameter,  and  am  parallel 
to  il.e  ordinatcs. 

For,  by  theor.  9,  -  mn,  mi,  mo, 
or  their  equals  -  ap,  ag,  ad, 
are  as  the  squares  of  pn,  gh,  de, 
or  of  their  equals  gi,  gh,  gk, 
which  are  proportionals  by  cor.  1. 

theorem  xix. 

If  a  diameter  cut  any  parallel  lines  terminated  by  the  curve  ; 
the  segments  of  the  diameter  will  be  as  the  rectangle  of 
the  segments  of  those  lines. 

That  is,  ek  :  em  :  :  ck  .  kl  :  nm  .  mo. 
Or,  ek  is  as  the  rectangle  ck  .  kl. 

For,  draw  the  diameter 
rs  to  which  the  parallels 
cl,  no  are  ordinatcs,  and 
the  ordinate  eq  parallel  to 
them. 

Then  ck  i»  \V\e  toffet- 
cnce,  and  kx  \Y\e  sum  of 
the  ordinatcs      cb  \  oVso 


OF  TBS  PARABOLA. 


531 


ttx  the  difference,  and  no  the  sum  of  the  ordinate*  eq,  ns. 
And  the  differences,  of  the  abscisses,  are  or,  as,  or  kk,  km. 

Then  by  cor.  theor.  9,  an  :  qs  : :  ck  •  kl  :  nm  .  mo, 
that  in       •       •       kk  :  km  :  :  ck  .  kl  :  nm  .  mo. 

Carol  1.  The  rect.  cl  .  kl  =  rect,  ek  and  the  pa  mm.  of  i>s. 
For  the  rect.  ck  .  kl  =  rect.  u«  and  the  param  of  rs. 

Carol.  2.  If  any  line  cl  be  cut  by  two  di « meters,  kk,  csii  ; 
the  rectangles  of  the  parts  of  the  line,  are  as  the  segments 
of  the  diameters. 

For  kk  is  as  the  rectangle  cz  •  kl, 
and  ch  is  as  the  rectangle  cii.iil; 
therefore  kk  :  oh  : :  ck  .  kl  :  cu  .  .hl. 

Carol.  3.  If  two  parallels,  cl,  no,  he  cut  by  two  diame- 
ters, km,  gi  ;  the  rectangles  of  the  parts  of  the  parallel*  will 
be  as  the  segments  of  the  respective  diameters. 

For    -    -    -     ek  :  km  : :  ck  .  kl  :  nm  .  no,  „ 
and    .    .    .     ek  .:  gh  : :  ck  •  kl  :  ch  .  hl, 
theref.  by  equal,  km  :  on  :  :  nm  .  mo  :  ch  .  hl. 

Carol.  4.  When  the  parallels  come  info  the  position  of 
the  tangent  at  p,  their  two  extremities,  or  points  in  the  curve, 
unite  in  rhe  point  of  contact  p  ;  and  the  rectangle  of  the  parts 
becomes  the  square  of  the  tangent,  and  the  same  properties 
still  follow  them. 

So  that,  ev  :  pv  :  :  pv  : 
•      ow  :  pw  : :  pw  : 


ev 

ev  ; 


gw  : 
gh  : 


:  pv 
pva 


:  p  the  param. 

:  PW», 

;  cn.  ii  l. 


theorem  xx. 'I 

If  two  parallels  intersect  any  other  two  parallels  ;  the  rect. 
angles  of  the  segments  will  be  respectively  proportional. 
That  is,  ck  .  kl  :  "m- 

E 


.  10. 


For,  by  cor.  3  theor.  $3,  pk  :  at  : :  ck  .  kl  :  gi  •  in 
And  by  the  same,      '     pk  :  ut  : :  dk  •  KB :  ni  •  io  ; 
therefc  byoquaL<iK.KL:  ox.  «     ax  .  w  ;si.io. 


CoroL  When  one  of  the  pain  of  intersecting  lines  comes 
k.  into  the  position  of  their  parallel  tangents,  meeting  and  limit* 
ing  oach  other,  the  rectangles  of  their  segments  become  ihe 
squares  of  their  respective  tangents.  So  that  the  constant 
ratio  of  the  rectangles,  is  that  of  the  square  of  their  parallel 
tangents,  namely, 

ce  •  kl:  dk  •  sis : :  tang9,  parallel  to  cl  :  tang9,  parallel  to  ac 

THEOBJE*  XXI. 

If  there  be  three  tangents  intersecting  each  other  ;  seek 
segments  will  be  in  the  same  proportion. 
That  is,  gi  :  in  :  cu  :  gd  : :  dh 
For,  through  the  points 
q,  i,  d,  h,  draw  the  diame- 
ters ok,  il,  dm,  iin  ;  ns 
also  the  lines  ci,  ei,  which 
are  double  ordinates  to  the 
diameters  ok,  iin,  by  cor.  1 
theor.  16  ;  therefore 
the  diameters  gk,  dm,  iin, 
bisect  the  lines  cl,  ce,  le  ; 
hence  km  =  cm  —  ck  =  Jce  —  {cl  =  )us  *e  Lx  0r  ne, 
and  mn  *  me  —  ne  =  !ce  —  £le  =  Jcl  «  ck  or  KL, 
But,  by  parallels,  gi  :  in  : :  kl  :  ln, 
and       -       .    cg  :  cd  : :  ck  :  km, 
also      -       -    dh  :  he  : :  mn  :  ne. 
But  the  3d  terms      kl,  ck,  mn  are  all  equal  ; 
as  also  the  4th  terms  ln,  km  ne. 
Therefore  the  first  and  second  terms,  in  all  the  lines,  are 
proportional,  namely,  gi  :  m  :  :  cc  :  gd  :  .  dii  :  he.    q.  e.  d» 


THEOREM  XXII. 

The  Area  or  Space  of  a  Parabola,  is  equal  to  Two-Thirds  of 
its  Circumscribing  Parallelogram. 

*Lct  acb  he  a  semi.pnrubola,  cb  ihe  axis,  f  the  focus,  ed 
the  directrix  ;  then  if  the  line  af 
be  supposed  to  revolve  about  f 
as  a  centre,  while  the  line  ae 
moves  along  the  directrix  per- 
pendicularly to  it,  the  nrea  gene- 
rated by  the  motion  of  ae,  will 
always  be  equal  to  double  the 
area  genera  ted  hy  fa  ;  and  con- 
sequently the  whole  external  area  aegd  =  double  the  area 


or  raft  PARABOLA- 


Ml 


For  draw  a  k  parallel,  and  indefinitely  near,  to  ab  ;  and 
draw  the  diagonals  ak'  and  a'k  ;  then  by  th.  6,  cor.  4,  the 
angles  b'a'a  and  ka'a  are  equal,  aa'  being  considered  as  part 
of  the  tangent  at  a'  ;  and  in  the  same  manner,  the  angles 
baa'  and  faa  are  also  equal  to  each  other  ;  and  since  ba  = 
af,  and  b'a'  —  a'f  ;  the  triangles  ea a'  and  b'a'a  are  each  equal 
to  the  triangle  a  a'f  ;  hut  the  triangle  baa'  =■  the  triangle 
bb'a,  being  on  the  same  base  and  between  the  same  parallels ; 
therefore  the  sum  of  the  two  triangles  bb'a  and  baa,  or  the 
quadrilateral  space  eaa'b'  is  double  the  trilateral  space  aa'f  ; 
and  as  this  is  the  case  in  every  position  of  fa',  b'a',  it  fol- 
lows that  the  whole  external  area  baco  =  double  the  inter- 
nal area  afc. 

Hence,  Take  do  =  fb,  and  complete  the  parallelogram 
do  he,  which  is  double  the  triangle  abf  ;  therefore  the  area 
abc  =  J  the  area  haco,  or  7  of  the  rectangle  aegh,  or  |  of 
the  rectangle  abci,  because  bc  =  |bo  ;  that  is,  the  area  of 
a  parabola  =  Jof  the  circumscribing  rectangle.     q.  b.  d.* 


THBOREM  XXIII. 

The  Solid  Content  of  a  Paraboloid  (or  Solid  generated  by 
the  Rotation  of  a  Parabola  about  its  Axis),  is  equal  to  Half 
its  Circumscribing  Cylinder. 

Let  ghdd  be  a  cylinder, 
in  which  two  equal  para  bo. 
loids  are  inscribed ;  one  bad 
having  its  base  bcd  equal  to 
the  lower  extremity  of  the 
cylinder ;  the  other  gch  in- 
verted with  respect  to  the 
former,  but  of  equal  base 
and  altitude.    Let  the  plane 
lr  parallel  to  each  end  of  the  cylinder,  cut  all  the  three  so. 
lids,  while  a  vertical  plane  may  be  supposed  to  cut  them  so 
as  to  define  the  parabolas  shown  in  the  ngure. 
Then,  in  the  semi-parabola  acb,  p  .  ap  =  pm1, 
also,  in  the  semi-parabola    aco,  p  .  cv  =  pit*, 
consequently,  by  addition,  p .  (ap  +  cp)=p  .  ac  «  pm*  +  fb*. 
But,  p  .  ac  =  cb*  =  PL*. 
Therefore  pl3  =  pm3  +  ph*  : 

That  is,  since  circles  are  as  the  squares  of  their  radii,  the 


p  y 

"  e  

*  This  Jem  »n  it  ration  whs  given  by  Lieut.  Drummond  of  the  Roynl 
Engineers,  *  hen  be  wai  a  gentleman  Cadet  at  the  Royal  Military  Acs- 


lo  a  Ctinder  »^#«e  Hei»j-  i«  pr.  ud  ft*  ft**e  li*lf  ike 
to  of  the  two  CirtoUr  Kmc*  ea.  sc. 


Let  *  -  3  1410  : 


B  D  C 


Th*n,  by  th*  l**t  theor.  %*pe  Y  Air  =  the  ». I  id  arc, 

and,  by  the  wifnc  \jc  X  Ar1  =  the  solid  aec, 

tl§#?r^f.  the  difT.  £pc  X  'ai*1—  *f  ;=the  fiust.  begc. 

Rut  kit1  —  ai"  =  ur  X  ' hi*  -r  ir% 

Iheref.        Jf*  X  di    X  'ad  4-  kt)  =  the  fro*  begc. 

But,  by  th.  I,  p  X  sit  —  ih.j,  and/>  X  ir  =  fg?: 

the  re  f.      X  dj  X  (in/1  +  fg*,  =  the  frost,  begc. 

q.  e.  d. 

fhoblems,  &c  for  exercise  in  comc  sections. 

1.  Demonstrate  flint  if  a  cylinder  be  cut  obliquely  the  sec- 
tion will  In;  an  ellipse. 

2.  Show  how  to  draw  a  tangent  to  an  ellipse  whose  foci  are 
r,  f}  from  a  given  point  i*. 

3.  Show  how  to  draw  a  tangent  to  a  given  parabola  from 
ii  given  point  v. 

4.  The  diameters  of  an  ellipse  are  16  and  12.  Required 
the  parameter  and  the  area. 

5.  The  bane  and  altitude  of  a  parabola  are  12  and  0.  Re* 
quired  the  parameter,  and  the  semi-ordinates  corresponding 
to  the  abscissa*  2,  .'1,  and  4. 

(I.  In  the  actual  formation  of  arches,  the  voussoirs  or  arch, 
gtoauft  arc  *j  cuV  a&  \o  >»tai«3%  ^on^adiaUar 


CONIC  SBCTI09CS. 


5S5 


to  the  respective  points  of  the  curve  upon  which  they  stand. 
By  what  const  ruction*  may  this  be  effected  for  the  parabola 
and  the  ellipse  ? 

7.  Construct  accurately  on  paper,  a  parabol.i  whose  base 
shall  be  12  and  altitude  9. 

8.  A  cone,  the  diameter  of  whose  base  is  10  inches,  and 
*hose  altitude  is  12,  is  cut  obliquely  by  a  plane,  which  enters 
at  3  inches  from  the  vertex  on  one  slant  slide,  and  comes  out 
at  3  inches  from  the  base  on  the  opposite  slant  side*  Requir- 
ed the  dimensions  of  the  section  ? 

9.  Suppose  the  same  cone  to  be  cut  by  a  plane  parallel  to 
one  of  the  slant  sides,  entering  the  other  slant  side  at  4 
inches  from  the  vertex,  what  will  be  the  dimensions  of  the 
section  ? 

10.  Let  any  straight  line  efb  be  drawn  through  f,  one 
of  the  foci,  of  an  ellipse,  and  terminated  by  the  curve  in  b 
and  r  ;  then  it  is  to  be  demonstrated  that  kf  .  fr  =  eb.{  pa- 
rameter. 

11.  Demonstrate  that,  in  any  conic  section,  a  straight  line 
drawn  from  a  focus  to  the  intersection  of  two  tangents  makes 
equal  angles  with  straight  lines  drawn  from  the  same  focus  to 
the  points  of  contact. 

12.  In  every  conic  section  the  radius  of  curvature  at  any- 
point  is  to  half  the  parameter,  in  the  triplicate  ratio  of  the 
distance  of  the  focus  from  that  point  to  its  distance  from  the 
tangent. 

Also,  in  every  conic  section  the  radius  of  curvature  is  pro- 
portional to  the  cube  of  the  normal. 

Also;  let  fc  be  the  radius  of  curvature  at  any  point,  p,  in> 
an  ellipse  or  hyperbola  whose  tranverse  axis  is  ab,  conju- 

fpF  .  rf)i 

gate  ab,  and  foci  f  and  /:  then  is  pc  =  ~  -^-t-. 

°  '  Jab  .  ab 

Required  demonstrations  of  these  properties* 


OH  Til  COMIC  NLCTBOH!  *S  WMW  **  AMMftMl  *0*A- 
TIOHC  CALLED  THS  BQ0ATIO]*  if  Tl|  W*TB.  • 


*  1.  Fortke  gltipm. 

Let  I  denote  ab,  the  transverse,  or  any  diameter; 

*  sb|h  its  conjugate ; 

*  =  ak,  any  absciss,  from  the  extremity  of  the  diam. 

y  =  ok.  the  correspondent  ordinate :  the  two  being  jointly 
denominated  co-ordinates. 
Then,  theor.  2,  ab*  :  hi*  : :  ak  .  kb  :  dk3, 
that  is,  1* :  e\ : :  x(f  —  x)  :  y*,  hence  iy  «  c"(<Jr  —  ar*), 

or  y  =  -y-  y/(tx  —  x9),  the  equation  of  the  curve. 

And  from  these  equations,  any  one  of  the  four  letters  or 
quantities,  f,  c,  x,  y,  may  easily  be  found,  by  the  reduction  of 
equations,  when  the  other  three  are  given. 

Or,  if  p  denote  the  parameter,  =  c1     1  by  its  definition  ; 

then,  by  cor.  th.  2, f.:  p  : :  *'v*-x)  :  y\  or  y*=  -y-  (fx— x*), 
which  is  another  form  of  the  equation  of  the  curve. 
Otherwise. 

If  f  =  ac  the  semiaxis ;  e  «=  cr  the  semiconjugate  ;  then 
p  =;  c*  -r  t  the  semi  parameter  ;  x  =  ck  the  absciss  counted 
from  the  centre ;  and  y  =  dk  the  ordinate  as  before. 
Then  is  ak  =  f— x,  and  kb  =  t  +  x,  and  ak  .  kb  =  {t  — x)  X 
(H-*)***8  —  Xs. 

Then,  by  th.  2,    :  c* : :  fi— x*  :  y',  and  <y  =  c*(f*  — x»), 

or  y  =  -j-  ^/(<* — Xs),  the  equation  of  the  curve. 

Or,  tip::  <■— x1  :  y\  and  y«  =     (C  — x*),  another  form 

of  the  equation  to  \\ie  cwrc*\  Vrom  ^\v\tVv  <me  of  the 
quantities  may  be  found,  HiYawi  vVv^  rax 


ZQUATIONS  OF  THJB  CVBVS. 


697 


2.  For  tJie  Hyperbola. 

Because  the  general  property  of  the  opposite  hyperbolas, 
with  respect  to  their  abscisses  and  ordinatcs,  is  the  same  as 
that  of  the  ellipse,  therefore  the  process  here  is  the  very  same 
as  in  the  former  cade  for  the  ellipse  ;  and  the  equation  to  the 
curve  must  come  out  the  same  also,  with  sometimes  only  the 
change  of  the  sign  of  a  letter  or  term,  from  +  to  — ,  or  from 
—  to  +,  because  here  the  abscisses  lie  beyond  or  without 
the  transverse  diameter,  whereas  they  lie  between  or  upon 
them  in  the  ellipse.  Thus,  making  the  same  notation  for  the 
whole  diameter,  conjugate,  absciss,  and  ordinate,  as  at  first  in 
the  ellipse  ;  then,  the  one  absciss  ak  being  x,  the  olher  bk 
will  be  t  +  x,  which  in  the  ellipse  was  t  —  r  ;  so  the  sign  of 
x  must  be  changed  in  the  general  property  and  equation, 
by  which  it  becomes  f3 :  c*  :  :  x[t  +  x)  :  y8 ;  hence  ftp  = 

c*  (tx  +  x*)  and  y  =  -j-  y/  (tx  +  jc2),  the  equation  of  the 

curve. 

Or  using  p  the  parameter,  as  before,  it  \s,t  :  p  : :  x(t+x)  : 
y*  or  y*  =  -j-  {tx  +  x*  ),  another  form  of  the  equation  to  the 
curve. 

Otherwise,  by  using  the  same  letters  f,  c,  p,  for  the  halves 
of  the  diameters  and  parameter,  and  x  for  the  absciss  ck 
counted  from  the  centre  ;  then  is  ak  =  x — t,  and  bk  =  x+t, 
and  the  property  P  :  c*  : :  (<  —  t)  X  (x+ 1)  :  y\  gives  *V=r 

€*  (x*  —  f)9  or  y  =  T  ✓(x*—  /a),  where  the  signs  of  t*  and  x% 

are  changed  from  what  they  were  in  the  ellipse. 

Or  again,  using  the  semi  parameter,  tip::  x* — £  :  y3,  and 

y*  =  -j-  (x3 —  f)  the  equation  of  the  curve. 

But  for  the  conjugate  hyperbola,  as  in  the  figure  to  theo- 
rem 3,  the  signs  of  both  x'J  and  t%  will  be  positive ;  for  the 
property  in  that  theorem  being  ca3  :  ca2 : :  cd*  +  ca"  :  ne3, 
it  is  f3  :  c*  : :  x*  +  f3  :  y>  =  D«a,  or  <ays=  c3(xa  +  <>),  and  y  =* 

\  y/(*?  +  0> tne  equation  to  the  conjugate  hyperbola. 

Or,  as  t :  p  : :  x*  +  c*  :  y8,  and  y3  =  (x3  +  f3)  also  the 
equation  to  the  same  curve. 


Vol.  I. 


69 


a*  x  *  y*rrvML  <r*.  jdt  imn.  vtraa;  ».  wmi 
as,  >i  a9,  sa  4r?inacei  pan£ei  to 
aansmou*.         a/  «  ir  =«,cisz. 
Mil  a*  =  «-  T"i*&-  sr  tM«r.  2&l  at  .  iv 
as  t«  .  ».  *>p    =  rj,  :a*  to  tie 

*/p*rV*a,  n«a  *.v*  1  Triton  sjs4  csm- 
aac**      take*  parauet  to  the  asvwaassBflL 
If  lite  a;>*r»*4a  fc*  arx  rectangular  ar  .  sr.  am.  r  vfi  be 
tquai  to  &  vfiare. 

3.  Fir  U*  P  mrmhoU- 

if  x  tenrtoi  any  ataciss  beginning  mt  the  vertex,  and  y 

ordinate:  alvi  />  tne  :*ararnei*r.  Then,  oy  oor.  theorem  1, 
ak  Mi*  k  f#  p.  <jt  1  y  y  p  :  hence  yz  =  jf  'is  the  equa- 
tion f/i  t.v;  \,htwa'+.    Or,  if  6i  =  abscissa  and  6  the  corre*- 

fforidiri^  ^rriiordiriat'.-,  ilien  ~  j  =  y%  is  the  equation. 

1.  For  the  Circle. 

H':raui«:  the  circle  is  only  a  species  of  the  ellipse,  in  which 
two  fixoH  an;  equal  to  each  other ;  therefore,  m«bmg  the 
(wo  fli'irnctorH  /  and  r  equal  each  to  d  in  the  foregoing  equa* 
Iioiih  to  thf!  ellip.se,  they  become  ya  =  cir — -r1,  when  the 
nhnciMH  t  h<;giriH  at  the  vertex  of  the  diameter :  and  ya  = 
|da  x*,  when  the  absciss  begins  at  the  centre.  Or  y  = 
(iJr  4  -  .■!■*),  and  y=  ^/(r2 — s2),  respectively,  when  r  is  the 
ruiliiiM. 

Scholium. 

lu  vvcry  onu  of  theso  equations,  we  perceive  that  they  rise 
to  tlm  *Jd  or  quadratic  degree,  or  to  two  dimensions  ;  which 
in  hImu  the  number  of  points  in  which  any  one  of  these  curves 
nut)  l»<i  nit  by  a  right  lino.  Hence  also  it  is  that  these  four 
eurvoM  are  niihI  to  he  linos  of  the  2d  order.  And  these  four 
urn  nil  the.  lines  that  aro  of  that  order,  every  other  curve  hav- 
ing muim  higher  equation,  or  may  be  cut  in  more  points  by  a 
right  lino. 

Wo  nun  heir  add  an  important  observation  with  regard 
to  all  eurves  o\y  rwwed  by  equations :  viz.  that  the  origin  of 


iukbxts  of  noraiMBTKY.  58t 

when  aU  the  terms  ef  its  equation  are  affected  by  one  of  the 
variable  quantities  x  or  y;  and  when,  on  the  contrary, 
there  is  in  the  equation  one  terra  entirely  known,  then  the 
origin  of  the  co-ordinates  cannot  be  on  a  point  of  the  curve* 
In  proof  of  this,  let  the  general  equation  of  a  curve  be  asf* 
+  bx*yi  =0 ;  then,  it  is  evident  that  if  we  take  »=  0, 
we  shall  likewise  haveiy*  =  0,  ory  =0;  and  consequently 
the  origin  of  the  co-ordinates  is  a  point  in  the  curve.  So 
again,  if,  in  the  same  equation,  we  take  y  =  0,  it  will  result 
thai  ax  =  0,  and  *  =0,  which  brings  us  to  the  same  thing  as 
before.  Bat,  if  the  equation  of  the  curve  include  one  known 
term,  as,  for  example,  aw*  +  fc'y*  +  cy* — =  0 ;  then 

taking  x  =  a,  we  shall  have  cy  —    =*=  0,  or  y  = '/ 

which  proves  that  the  corresponding  point  p,  of  die  curve, 

is  distant  from  the  origin  of  the  z'a  by  the  quantity  V 

A  simitar  troth  will  flow  from  making  y  =  0,  when  the  same 

equation  will  give  *  « 


ELEMENTS  OF  ISOPERIMETRY. 

Dtf.  1.  When  a  variable  quantity  has  it*  rimtations  re- 
jpdated  by  a  certain  law,  or  confined  within  certain  limits,  it 
is  called  a  maximum  when  it  has  reached  the  greatest  mag- 
nitude it  can  possibly  attain  ;  and,  on  the  contrary,  when  k 
has  arrived  at  the  least  possible  magnitude,  it  is  called  a  mi- 

Isepcrimetors>  or  fmpeiimeti  icai  Figures,  me  those 
which  have  equal  perimeters. 

Def.  3.  The  Locus  of  any  point,  or  intersection,  dec.  is 
the  right  line  or  curve  in  which  these  are  always  situated. 

The  problem  in  which  it  is  required  to  find,  among  figures 
of  the  same  or  of  different  kinds,  those  which,  within  equal 
perimeters,  shall  comprehend  the  greatest  surfaces,  has  long 
engaged  the  attention  of  mathematicians.  Since  the  admir- 
able  invention  of  the  method  of  Fluxions,  this  problem  has 
been  elegantly  treated  by  some  of  the  writers  on  that  branch 
of  analysis ;  especially  by  Haclaqrin  and  Simpson*   k  wud*> 


640 


ELEXKm  Or  fSOPBUMXTKT. 


more  extensive  problem  was  investigated  at  the  time  of 
"  the  war  of  problems,"  between  the  two  brothers  John  and 
James  Bernoulli :  namely,  "  To  find,  among  all  the  isoperi- 
metrical  curves  between  given  limits,  such  a  curve,  that,  con- 
structing a  second  curve,  the  ordinates  of  which  shall  be 
functions  of  the  ordinates  or  arcs  of  the  former,  the  area  of 
the  second  curve  shall  be  a  maximum  or  a  minimum."  While, 
however,  the  attention  of  mathematicians  was  drawn  to  the 
most  abstruse  inquiries  connected  with  isoperiraetry,  the  cfe- 
menls  of  the  subject  were  lost  sight  of.  Simpson  was  the  first 
who  called  them  back  to  this  interesting  branch  of  research, 
by  giving  in  his  neat  little  book  of  Geometry  a  chapter  on  the 
maxima  and  minima  of  geometrical  quantities,  and  some  of  w 
the  simplest  problems  concerning  isoperi meters.  The  next 
who  treated  this  subject  in  an  elementary  manner  was  Simon 
Lhuillier,  of  Geneva,  who,  in  1782,  published  his  treatise 
De  Relatione  mulua  Capacitatis  el  Terminorvm  Figurarum, 
die.  His  principal  object  in  the  composition  of  that  work 
was  to  supply  the  deficiency  in  this  respect  which  he  found  in 
most  of  the  Elementary  Courses ;  and  to  determine,  with  re- 
garb?  to  both  the  most  usual  surfaces  and  solids,  those  which 
possessed  the  minimum  of  contour  with  the  same  capacity ; 
and,  reciprocally,  the  maximum  of  capacity  with  the  same 
boundary.  M.  Legend  re  has  also  considered  the  same  sub- 
ject, in  a  manner  somewhat  different  from  either  Simpson  or 
Lhuillier,  in  his  EUments  dc  Geomttrie.  An  elegant  geo- 
metrical tract,  on  the  same  subject,  was  also  given  by  Dr. 
Horsley,  in  the  Philos.  Trans,  vol.  75,  for  1775 ;  contained 
also  in  the  New  Abridgement,  vol.  13,  page  653*.  The  chief 
propositions  deduced  by  these  four  geometers,  together  with 
a  few  additional  propositions,  are  reduced  into  one  system  in 
the  following  theorems. 


"  Another  work  on  the  same  general  subject,  containing  mnny  valua- 
ble theorems,  has  been  published  since  the  first  edition  of  this  volume, 
by  Dr.  CrtsucU  of  Trinny  College,  Cambridge. 


{541  ] 


SECTION  I. 


SURFACES. 


THEORXM  I. 

Of  all  triangles  of  the  same  base,  and  whose  vertices  fall 
in  a  right  Tine  given  in  position,  the  one  whose  perimeter 
is  a  minimum  is  that  whose  sides  are  equally  inclined  to 
that  line. 

Let  ab  be  the  common  base  of  a  series  of  triangles  abc\ 
abc,  &c.  whose  vertices  c',  c,  fall  in  the  right  line  lm,  jpven 
in  position,  then  is  the  triangle  of  least 
perimeter  that  whose  sides  ac,  bc,  are 
inclined  to  the  line  lm  in  equal  angles. 

For,  let  bm  be  drawn  from  b,  per. 
pendicularly  to  lm,  and  produced  till 
dm  =  bm  :  join  ad,  and  from  the  point 
c  where  ad  cuts  lm  draw  bc  :  also,  from 
any  other  point  c',  assumed  in  lm,  draw  c'a,  c'b,  cd.  Then 
the  triangles  dmc,  bmc,  having  the  angle  dcm  =  angle  acl 
(th.  7  Geom.)  =  mcb  (by  hyp.),  dmc  =■  bmc,  and  dm  =  bm, 
and  mc  common  to  both,  have  also  dc  =  bc  (th.  1  Geom.). 

So  also,  we  have  c'i>  =  c'b.  Hence  ac  +  cb  =  ac  +  cd 
~  ad,  is  less  than  ac'  +  c'p  (theor.  10  Geom.),  or  than  its 
equal  ac'  +  c'b.  And  consequently,  ab  +  bc  +  ac  is  less 
than  ab  +  bc'  +  ac'.    q.  e.  d. 

Cor.  1.  Of  all  triangles  of  the  same  base  and  the  same  al- 
titude, or  of  all  equal  triungles  of  the  same  base,  the  isosceles 
triangle  has  the  smallest  perimeter. 

For,  the  locus  of  the  vertices  of  all  triangles  of  the  same 
altitude  will  be  a  right  line  lm  parallel  to  the  base ;  and 
when  lm  in  the  above  figure  becomes  parallel  to  ab,  since 
mcb  =  acl,  mcb  =?  cba  (th.  12  Geom.),  acl  =  cab  ;  it 
follows  that  cab  =  cba,  and  consequently  ac  =  cb  (th.  4 
Geom.) 

Cor.  2.  Of  all  triangles  of  the  same  surface,  that  which 
has  the  minimum  perimeter  is  equilateral. 

For  the  triangle  of  the  smallest  perimeter,  with  the  same 
surface,  must  be  isosceles,  whichever  of  the  sides  be  con- 
sidered as  base :  therefore,  the  triaogU  of  ra^i^^\TMtfust 


542 


ELEMENTS  OF  ISOFEllIMETBT. 


has  each  two  or  each  pair  of  its  sides  equal,  and  consequently 
it  is  equilateral. 

Cor.  3.  Of  all  rectilinear  figures,  with  a  given  magnitude 
and  a  given  number  of  sides,  that  which  has  the  smallest 
perimeter  is  equilateral. 

For  so  long  as  any  two  adjacent  sides  are  not  equal,  we 
may  draw  a  diagonal  to  become  a  base  to  those  two  sides,  and 
then  draw  an  isosceles  triangle  equal  lo  the  triangle  so  cut 
off,  but  of  less  perimeter :  whence  the  corollary  is  manifest 

Sc?iolium. 

?■■ 

To  illustrate  the  second  corollary  above,  the  student  may 
proceed  thus  :  assuming  an  isosceles  triangle  whoso  base  is 
not  equal  to  either  of  the  two  sides,  and  then,  taking  for  anew 
base  one  of  those  sides  of  that  triangle,  he  may  construct  an- 
other isosceles  triangle  equal  to  it,  but  of  a  smaller  perimeter. 
Afterwards,  if  the  base  and  sides  of  this  second  isosceles  tri- 
angle are  not  respectively  equal,  he  may  construct  a  third 
isosceles  triangle  equal  to  it,  but  of  a  still  smaller  perimeter  ; 
and  so  on.  In  performing  these  successive  operations,  he 
will  find  that  the  new  triangles  will  approach  nearer  and 
nearer  to  an  equilateral  triangle. 

THEOREM  II. 

Of  all  triangles  of  the  same  base,  and  of  equal  perimeters, 
the  isosceles  triangle  has  the  greatest  surface. 

Let  abc,  abo,  be  two  triangles  of  the  same 
base  ab  and  with  equal  perimeters,  of  which 
the  one  auc  is  isosceles,  the  other  is  not : 
then  the  triangle  aim-  has  a  surface  (or  an 
altitude)  greater  than  the  surface  (or  than 
the  altitude)  of  the  triangle  \bd. 

Draw  c'd  through  o,  parallel  to  ab,  to 
cut  ve  (drawn  perpendicular  to  ab)  in  c  :  then  it  is  to  be 
demonstrated  that  ce  is  greater  than  c'k. 

The  triangles  ac'b,  adb,  are  equal  both  in  base  and  alti- 
tude ;  but  the  triangle  Ac'n  is  isosceles,  while  adb  is  scalene : 
therefore  the  triangle  ac'b  has  a  smaller  perimeter  than  the 
triangle  adb  (th.  1  cor.  1),  or  than  acb  (by  hyp.).  Conse- 
quently ac  <  ac  ;  and  in  the  right-angled  triangles  aec, 
aec,  having  ae  common,  we  have  c'e  <  ce  *.    q.  e.  d. 


♦  When  two  mathtma\\tB\  qpwfl&>»%  <&wx»kXm\  <^ 


SURFACES. 


548 


Cor.  Of  all  isoperimetrical  figures,  of  which  the  number 
of  sides  is  given,  that  which  is  the  greatest  has  all  its  sides 
equal.  And  in  particular,  of  all  isoperimetrical  triangles, 
that  whose  surface  is  a  maximum,  is  equilateral. 

For,  so  long  as  any  two  adjacent  sides  are  not  equal,  the 
surface  may  be  augmented  without  increasing  the  perimeter. 

Remark.  Nearly  as  in  this  theorem  may  it  be  proved 
that,  of  all  triangles  of  equal  heights,  and  of  which  the  sum 
of  the  two  sides  is  equal,  that  which  is  isosceles  has  the 
greatest  base.  And,  of  all  triangles  standing  on  the  same 
base  and  having  equal  vertical  angles,  the  isosceles  one  is 
the  greatest. 

# 

THEOREM  in. 

Of  all  right  lines  that  can  be  drawn  through  a  given  pointy 
between  two  right  lines  given  in  position,  that  which  is 
bisected  by  the  given  point  forms  with  the  other  two  lines 
the  least  triangle. 

Of  all  right  lines  on,  ab,  cd,  that 
can  be  drawn  through  a  given  point 
p  to  cut  the  right  lines  ca,  cd,  given 
in  position,  that,  ab,  wnich  is  bi- 
sected by  the  given  point  r,  forms 
with  ca,  co,  the  least  triangle,  abc 

For,  let  ee  be  drawn  through  a 
parallel  to  cd,  meeting  dg  (produced  if  necessary)  in  e  ; 
then  the  triangles  p  jo,  pae,  are  manifestly  equiangular ;  and, 
since  the  corresponding  sides  pb,  pa  are  equal,  the  triangles 
are  equal  also.  Hence  pbd  will  be  less  or  greater  than  pag, 
according  as  cg  is  greater  or  less  than  ca.  In  the  former 
case,  let  pacd,  which  is  common,  be  added  to  both  ;  then 
will  bac  be  less  than  dgc  (ax.  4  Geona.).  In  the  latter  case, 
if  pgcb  bo  added,  dco  will  be  greater  than  bac  ;  and  conse- 
quently in  this  case  also  bac  is  less  than  dco.    q.  e.  d. 

Cor.  If  ph  and  pn  be  drawn  parallel  to  cb  and  ca  re- 
spectively,  the  two  triangles  pam,  pbn,  will  be  equal,  and 
these  two  taken  together  (since  am  =  pn  a  mc)  will  be 
equal  to  the  parallelogram  pmcn  :  and  consequently  the 
parallelogram  pmcn  is  equal  to  half  abc,  but  less  than  half 
doc.  From  which  it  follows  (consistently  with  both  the  al- 
gebraical and  geometrical  solution  of  prob.  8,  Application  of 


it  denotes  that  the  preceding  quantity  is  less  than  the  succeeding  one : 
when,  on  the  contrary,  the  separating  character  is  > ,  it  denotes  that  the 
preceding  quantity  is  greater  th*n  the  succeeding  one. 


544 


KLXMEXTI  OF  UOPIUiaTBT. 


Algebra  to  Geometry),  that  a  parallelogram  is  always  lew 
than  half  a  triangle  in  which  it  is  inscribed,  except  when  the 
base  of  the  one  is  half  the  base  of  the  other,  or  the  height 
of  the  former  half  the  height  of  the  latter ;  in  which  case  the 
parallelogram  is  just  half  the  triangle :  this  being  the  maxi- 
mum parallelogram  inscribed  in  the  triangle. 

Scho*  urn. 

From  the  preceding  corollary  it  might  easily  be  shown, 
that  the  least  triangle  which  can  possibly  be  described  about, 
and  the  greatest  parallelogram  which  can  be  inscribed  in,  any 
curve  concave  to  its  axis,  will  be  whenjL  subtangent  is  equal 
to  half  the  base  of  the  triangle,  or  to  »  whole  base  of  the 
%  parallelogram  :  and  tliat  the  two  figures  will  be  in  the  ratio 
of  2  to  1.    But  this  is  foreign  to  the  present  inquiry. 

THEOREM  IV. 

Of  all  triangles  in  which  two  side*  are  given  in  magnitude, 
the  greatest  is  that  in  which  the  two  given  sides  are 
perpendicular  to  each  other. 

For,  assuming  for  base  one  of  the  given  sides,  the  surface 
is  proportional  to  the  perpendicular  let  fall  upon  that  side 
from  the  opposite  extremity  of  the  other  given  side  :  there- 
fore, the  surface  is  the  greatest,  when  that  perpendicular  is 
the  greatest ;  that  is  to  say,  when  the  other  side  is  not  in- 
clined to  that  perpendicular,  but  coincides  with  it  :  hence 
the  surface  is  a  maximum  when  the  two  given  sides  are  per- 
pendicular to  each  other. 

Otherwise.  Since  the  surface  of  a  triangle,  in  which  two 
sides  are  given,  is  proportional  to  the  sine  of  the  angle  in- 
cluded between  those  two  sides  ;  it  follows,  that  the  triangle 
is  the  greatest  when  that  sine  is  the  greatest :  but  the  greatest 
sine  is  the  sine  total,  or  the  sine  of  a  quadrant ;  therefore  the 
two  sides  given  make  a  quadrantal  angle,  or  are  perpendicular 
to  each  other*   q.  e.  d. 

THEOREM  V. 

Of  all  rectilinear  figures  in  which  all  the  sides  except  one  are 
known,  the  greatest  is  that  which  may  be  inscribed  in  a 
semicircle  whose  diameter  is  that  unknown  side. 

For,  if  you  suppose  the  contrary  to  be  the  case,  then  when- 
ever  the  figure  made  with  the  sides  given,  and  the  side  un- 
known, is  not  inscribable  in  a  semicircle  of  which  this  latter 


SURFACES. 


545 


i  the  diameter,  viz.  wtmever  any  one  of  the  angles,  formed 
by  lines  drawn  from  the  extremities  of  the  unknown  side  to 
one  of  the  summits  of  the  figure,  is  not  u  right  angle  ;  we 
may  make  a  figure  greater  than  it,  in  which  that  angle  shall 
be  right,  and  which  shall  only  differ  from  it  in  that  respect  : 
therefore,  whenever  all  the  angles,  formed  by  right  lines 
drawn  from  the  several  vertices  of  the  figure  to  the  extre- 
mities of  the  unknown  line,  are  not  right  angles,  or  do  not 
fall  in  the  circumference  of  a  semicircle,  the  figure  is  not  in 
its  maximum  state,    q.  e.  d. 

.  THEOREM  VI. 

I  Of  all  figures  made  £th  sides  given  in  number  and  mag. 
'    nitude,  that  which  may  be  inscribed  in  a  circle  is  the 
greatest. 

Let  abcdefg  be 
the  polygon  inscrib- 
ed, and  abcdefg  a 
polygon  with  equal 
sides,  but  not  inscri- 
bable  in  a  circle  ;  so 
that  ab  =  <i6,  bc  = 
be,  die.  ;  it  is  affirm, 
ed  that  the  polygon 
abcdbfg  is  greater  than  the  polygon  abedefg. 

Draw  the  diameter  bp  ;  join  ai\  ph  ;  upon  ab  =  ab  ma'ce 
the  triangle  abp,  equal  in  all  respects  to  abp  ;  and  join  ep. 
Then,  ofthe  two  figures  edebp,  pag  fe>  one  at  least  is  not  (by 
hyp.)  inscribable,  in  the  semicircle  of  which  ep  is  the  diame- 
ter. Consequently,  one  at  least  of  these  two  figures  is  smaller 
than  the  corresponding  part  of  the  figure  apbcdrfg  (th.  6). 
Therefore  the  figure  aprcdrfo  is  greater  than  the  figure 
apbc  'efg  :  and.  if  from  these  there  be  taken  away  the  re- 
spective triangles  apb,  apb,  which  are  equal  by  construction, 
there  will  remain  (ax.  5  Geom.)  the  polygon  abcdefg  greater 
than  the  polygon  abcdefg.    q,.  e.  d. 


THEOREM  VII. 

The  magnitude  of  the  greatest  polygon  which  can  be  con- 
tained under  any  number  of  unequal  sides,  does  not  at  all 
depend  on  the  order  in  which  those  lines  are  connected 
with  each  other. 

For,  since  the  polygon  is  a  maximum  under  given  side*,  it 
is  inscribable  in  a  circle  (th.  6).  And  this  inscribed  polygon 
is  constituted  of  as  many  isosceles  triangles  as  it  has  sides, 
those  sides  forming  the  bases  of  the  respective  triangles,  the 

Vol.  I.  70 


646 


ELEMENTS  OF  ISOmRIMJCTRY. 


other  rides  of  all  the  triangle*  being  radii  of  the  circle,  and 
their  common  summit  the  centre  of  the  circle.  ConJu»quenujr 
the  magnitude  of  tho  polygon,  tbmt  is,  of  the  asscmbliige  of 
these  triangles,  does  not  at  all  depend  on  their  disposition, 
or  arrangement  around  tho  common  centre,    a-  k.  d. 

THEOREM  VIU. 

If  n  polygon  inscribed  in  a  circle  have  all  its  sides  equal,  all 
its  angles  are  likewise  equal,  or  it  is  a  regular  polygon. 

For,  if  lines  be  drawn  from  the  several  angles  of  the  poly, 
gon,  to  the  centre  of  the  circumscribing  circle,  they  will 
divide  the  polygon  into  as  many  iuuawles  triangles  as  it  has! 
sides  ;  nnd  each  of  these  isosceles  triangles  will  be  equal  to™ 
either  of  the  others  in  all  respects,  and  of  course  they: will 
have  the  angles  at  their  bases  all  equal :  consequently,  .the 
angles  of  the  polygon,  which  are  each  made  up  of  two  angles 
at  the  bases  of  two  contiguous  isosceles  triangles,  will  be  equal 
to  one  another,    a.  k.  d. 

THEOREM  IX. 

Of  all  figures  having  the  same  number  of  sides  and  sequel 
perimeters,  the  greatest  is  regular. 

For,  the  greatest  figure  under  the  given  conditions  has 
all  its  sides  equal  (tli.  2.  cor.).  But  since  the  sum  of  the 
sides  and  the  number  of  them  are  given,  each  of  them  is 
given  :  therefore  (th.  6\  the  figure  is  inscribable  in  a  circle: 
nnd  consequently  (th.  6)  all  its  angles  ore  equal  ;  that  is,  it 
is  regular,    a.  e.  i>. 

Cor.  Hence  we  see  that  regular  polygons  possess  the  pro- 
perty of  a  maximum  of  surface,  when  compared  with  any 
okher  figures  of  the  same  name  and  with  equal  perimeters. 

THEOREM  X. 

A  regular  polygon  has  a  smaller  perimeter  than  an  irregular 
one  equal  to  it  in  surface,  and  having  the  same  number 
cf  sides. 

This  is  the  converse  of  the  preceding  theorem,  and  may 
be  demonstrated  thus  :  Let  r  and  I  be  two  figures  equal  in 
surface,  and  having  the  same  number  of  sides,  of  which**  is 
regular,  i  irregular  :  let  also  h'  be  a  regular  figure  similar  to 
r,  and  having  a  perimeter  equal  to  that  of  i.  Then  (th.  9) 
r'  >  i ;  but  \  =•  a;  vYu&tetac*  ^  >  ^  wuijt  are  si- 


947 


stoHar ;  ooajaoqaenfly,  perimeter,  of  b'  >  perimeter  of  a ;  while 
per.  a'  as  per.  1  (by  hyp.).  Hence,  per.  i  >  per.  a.  q.  b.  d. 

THBORKW  XI* 

The  surfaces  of  polygons,  circumscribed  about  the  same  or 
equal  circles,  are  respectively  as  their  perimeters*. 

D 

Let  the  polygon  abcd  hi!  circumscribed 
about  theeircte  vfoh  ;  and  let  this  polygon 
be  divided  into  triangles,  by  lines  drawn 
pfrom  its  several  angles  to  the  centre  o  of 
the  circle.  Then,  since  each  of  the  tan- 
gents ab,  nc,  dec.  is  perpendicular  to  its  -A. 
eomspondtnf  radius,  or,  op,  &c,  drawn  to  the  point  of  con- 
tact (th.  46Geom.) ;  and  since  the  area  of  a  triangle  is  equal 
lb  the  rectangle  of  the  perpendicular  and  half  the  base  (Mens, 
•f  Surface*,  pr.  3);  it  follows,  that  the  area  of  each  of  the 
triangles  abo,  bco,  Sic.  is  equal  to  the  rectangle  of  the  radius 
of  the  Circle  and  half  the  corresponding  side  ab,  bc,  &c.  ;  and 
consequently,  the  area  of  the  polygon  abcd,  circumscribing 
the  circle,  will  he  equal  to  the  rectangle  of  the  radius  of  the 
circle  and  half  the  perimeter  of  the  polygon.  But,  the  sur- 
face of  the  circle  is  equal  to  the  rectangle  of  the  radius  and 
half  the  circumference  (th.  04  Geom.).  Therefore,  the  sur- 
face of  the  circle,  is  to  that  of  the  polygon,  as  half  the  cir- 
cumference of  the  former,  to  half  the  perimeter  of  the  latter ; 
or,  as  the  circumference  of  the  former,  to  the  perimeter  of 
the  latter.  Now,  let  p  and  p'  be  any  two  polygons  circum- 
scribing a  circle  c  :  then,  by  the  foregoing,  we  htive 

surf,  c  :  surf,  p  : :  circum.  c  :  perim.  p. 

surf,  c  :  surf,  p'  :;  circum.  c  :  perim.  p\ 
But,  since  the  antecedents  of  the  ratios  in  both  these  proper- 
tions,  are  equal,  the  conaequents  are  proportional :  that  is, 
aurf.  p  :  surf,  p' : :  perim.  p  :  perim.  p'«     4.  k.  d. 

Cor.  1.  Any  one  of  the  triangular  portions  abo,  of  a  po- 
lygon circumscribing  a  circle,  is  to  the  corresponding  circular 
sector,  as  the  side  ab  of  the  polygon,  to  the  arc  of  the  circle 
included  between  ao  and  bo. 


•This  theorem,  together  with  tho  analogous  onei  re«prcling  hodips 
ctaaoiferihMg  cylinders  nnd  spheres,  were  piveu  by  Eme.-son  in  his 
tfrometry,  and  their  u*e4n  tan  theory  of  lso|M»rimetm  was  just  suggest- 
ed:  but  the  full  *ppKc*Uua  ef  them  te  that  theory  is  due  to  Siioee 
Uuillier. 


548 


xunanm  of  hokeikbtet. 


Car.  2.  Every  circular  arc  is  greater  than  Ha  chord,  aad 
leas  than  the  sum  of  the  two  tangents  drawn  from  its  extremi 
ties  and  produced  till  they  meet. 

The  first  part  of  this  corollary  is  evident,  because  a  r  bt 
line  is  the  shortest  distance  between  two  given  points.  T  <e 
second  part  follows  at  once  from  this  proposition  :  for  ea  f 
ah  being  to  the  arch  kih,  as  the  quadrangle  a  boh  to  the  c  r 
cular  sector  hieo  ;  and  the  quadrangle  being  greater  than  the 
sector,  because  it  contains  it ;  it  follows  that  ea  +  ah  if 
greater  than  the  arch  kih*. 

Cor.  8.  Hence  also,  any  single  tangent  sa,  is  greater  than 
its  corresponding  arc  ki.  ^ 

THEOREM  XII. 

If  a  circle  and  a  polygon,  circumscribahle  about  another 

circle,  are  isoperimeterc,  the  surface  of  the  circle  is  a 
geometrical  mean  proportional  between  that  polygon  and 
a  similar  polygon  (regular  or  irregular)  circumscribed 
about  that  circle. 

Let  c  be  a  circle,  p  a  polygon  isoperimetrical  to  that  circle, 
and  circumscribahle  about  some  other  circle,  and  p'  a  polygon 
similar  to  p  and  circumscribahle  about  the  circle  c :  it  is 
affirmed  that  p  :  c  :  :  c  :  p'. 

For,  p  :  p'  :  :  peri  nr.  p  :  perima.  p'  : :  circum*.  c  :  perim*.  t 

by  tli.  89,  geom.  and  the  hypothesis. 
But  (th.  1 1)  p ' :  c  : :  per.  p' :  cir.  c  ; :  per3,  p'  :  per.  p'  x  cir.c 
Therefore    p  :  c  : :     ....     c-ir9.  c  :  per.  P  x  cir.  c. 
:  :  cir.  c  :  per.  p'  :  :  c  :  p'.    Q.  e.  ». 

THEOREM  XIII. 

If  a  circle  and  a  polygon,  circumscribahle  about  another 
circle,  are  equal  in  surface,  the  perimeter  of  that  figure 
is  a  geometrical  mean  proportional  between  the  circum- 
ference of  the  tiret  circle  and  the  perimeter  of  a  similar 
polygon  circumscribed  about  it. 

Let  c  =  p,  and  let  p'  be  circumscribed  about  c  and  similar 
to  c  :  then  it  is  affirmed  that  cir.  c  :  per.  p  :  :  per.  p  :  per.  p'. 


*  This  second  enrol  In  r  v  is  introduced,  not  l>ecfui«*  (if  its  immrdiftle 
connexion  with  the  subject  nndr  discission,  but  because,  nottrith- 
standing  its  timpVuAly,  *v\\Wr%  V\wv«  employed  whole  pegetia 
attempting  Us  demoi\&Vt*V\w\, 


SURFACES* 


For  cir.  c  :  per.  p'  : :  c  :  p'  : :  p  :  p'  : :  per*,  p  :  per1.  p'. 
A  Up,  per.  p' :  per.  p      -  : :  per*,  p'  :  per.  p  X  per.  p'. 

Tbi  reforo,  cir.  c  :  per.  p  : :  per",  p  :  per.  p  x  per  p'. 

: :  per.  p  : :  per.  p.    q,.  b.  d.  ' 

THEOREM  XIV. 

The  circle  is  greater  than  any  rectilinear  figure  of  the  same 
perimeter :  and  it  has  a  perimeter  smaller  tha »  ai»y  recti- 
linear figure  of  the  same  surface. 

For,  in  the  proportion,  p  :  c  ::  c  :  p  (th.  12), since  c  <  p', 

therefore  p  <  c. 
And,  in  the  propor.  cir.  c  .  per.  p  : :  per.  p  :  per.  p'  (th*  13), 
or,  cir.  c  :  per.  p'  : :  cir3.  c  :  per*,  p, 
and  cir.  c  <  per.  p'  : 
therefore,  cir*.  c  <  per1,  p,  or  cir.  c  <  per.  p.    q.  e.  d. 

Cor.  1.  It  follows  at  once,  from  this  and  the  two  pre- 
ceding theorems,  that  rectilinear  figures  which  are  isoperi* 
metera,  and  each  circumscribable  about  a  circle,  are  re- 
spectively  in  the  inverse  ratio  of  the  perimeters,  or  of  the 
surfaces,  of  figures  similar  to  them,  and  both  circumscribed 
about  one  and  the  same  circle.  And  that  the  perimeters  of 
equal  rectilineal  figures,  each  circumscribable  about  a  circle, 
are  respectively  in  the  subduplicate  ratio  of  the  perimeters, 
or  of  the  surfaces,  of  figures  similar  to  them,  ana  both  cir- 
cumscribed about  one  and  the  same  circle. 

Cor.  2.  Therefore,  the  comparison  of  the  perimeters  of 
equal  regular  figures,  having  different  numbers  of  sides,  and 
that  of  the  surfaces  of  regular  isoperimetrical  figures,  is  re- 
duced to  the  comparison  of  the  perimeters,  or  of  the  surfaces 
of  regular  figures  respectively  similar  to  them,  and  circum- 
scribable about  one  and  the  same  circle. 

Lemma  1. 

If  an  acu*o  anglo  of  a  right-angled  triangle  be  divided 
into  any  number  of  equal  parts,  the  side  of  the  triangle 
opposite  to  that  acute  angle  is  divided  into  unequal  parts, 
which  are  greater  as  they  are  more  remote  from  the  right 
angles. 

Let  the  acute  angle  c,  of  the  right-  Cfev 
angled  triangle  acp,  be  divided  into  equal  V\^V 
parts,  by  the  lines  rc,  cd,  ce,  drawn  from  \\N\ 
that  angle  to  the  opposite  side;  then  shall        \  \ 
the  parts  ab,  bd,  &c.  intercepted  by  the   A  B  J>  E  7 


650 


ELEMENTS  OF  nOPEBJXETRY. 


lines  drawn  from  c,  be  successively  longer  us  they  are  more 
lemofe  from  the  right  angle  a. 

For,  the  tingles  acd,  bce.  &c.  being  bisected  by  c»,  CD, 
d&c.  iherefure  by  thcor.  83  Geom.  ac  :  cd  : :  ab  :  bd,  and 
rc  :  ce  :  :  bu  :  de,  and  dc  :  cf  :  :  de  :  ef.  And  by  th.  21 
Geom.  cd  >  ca,  ce  >  cb,  cf  >  cc,  and  so  on  :  whence  it 
follows,  that  db  >  ab,  de  >  db,  and  soon.    u.  e.  d. 

Cor.  Hence  it  is  ohviius  that,  if  the  part  the  most  remote 
from  the  right  angle  a,  be  repeated  a  number  of  times  equal 
to  that  into  which  the  acute  angle  is  divided,  there  will  re. 
suit  a  quantity  greater  than  the  side  opposi  e  to  the  divided 
angle. 

THEOREM  XV. 

If  two  reg  liar  figures,  circumscribed  about  the  same  circle, 
differ  in  their  number  of  sides*  by  unity,  that  which  has 
the  greatest  number  of  sides  shall  have  the  smallest  peri- 
meter. 

Let  ca  be  the  radius  of  a  circle,  and  ab,  ad,  the  haff  sides 
of  two  regular  polygons  circumscribed  about  thai  circle.,  of 
which  the.  number  of  sides  differ  by  unity,  being  C 
respectively  n  +  1  und  n.    The  angles  acb,  acd, 

therefore  arc  respectively  the  ~^  and  the  ^  th 

part  of  two  right  angles  :  consequently  these  <A-  I^D 
angles  ar*  as  n  and  n  +  1  :  and  hence,  the  angle  may  be 
conceived  divided  into  n  +  1  equal  purls,  of  which  bcd  is 
one.  Consequently,  (cor.  to  the  lemma)  (n  -f  1)  no  >  ad. 
Taking,  then,  unequal  quantities  from  equal  quantities,  we 
shall  have 

(n  +  1}  ad  -  (n  +  1)  bd  <  (n  +  1)  ad  -  ad, 
or(n  t!)ab<  n  .  ad. 
That  is,  the  scmiperimeter  of  the  polygon  whose  half  side  is 
ab,  is  smaller  than  the  scmiperimeter  of  the  polygon  whose 
half  side  is  ad  :  whence  the  proposition  is  manifest. 

Cor.  Hence,  augmenting  successively  by  unity  the  num. 
ber  of  sides,  it  follows  generally,  that  the  perimeters  of 
polygons  circumscribed  about  any  proposed  circle,  become 
smaller  as  the  number  of  their  sides  become  greater. 


THEOREM  XVI. 

The  surfaces  ef  regular  isoperimetrical  figures  are  grAriter 
as  the  number  of  their  sides  is  greater  :  and  the  peri- 
meters  of  equal  ve^ulur  figures  are  smaller  as  the  number 
of  their  sides  is  gtuutet. 


SOLIDS.  r,$| 

For,  1st.  Regular  isoperimetrical  figures  are  (cor.  1.  th. 
14)  in  the  inverse  ratio  of  figures  similar  to  tliem  circum- 
scribed about  the  same  circle.  And  (th.  15)  these  latter  ara 
smnller  when  their  .number  of  sides  is  greater  :  therefore,  on 
the  contrary,  the  foifaer  become  greater  as  they  have  more 
sides. 

2dly.  The  perimeters  of  equal  regular  figures  are  (cor.  1 
th.  14;  in  the  subduplicute  ratio  of  the  perimeters  of  similar 
figures  otptamscrib$d  .about  the  same  circle  :  and  (th.  15) 
these  latter  are  smaller  as  they  have  more  side's:  therefore 
the  perimtffsrs  of  the  former  also  arc  smaller  when  the  num- 
ber of  then*  sides  is  greater,    a.  e.  d. 


SECTION  II. 
4  SOLIDS. 

THEOREM  XV1T. 

Of  all  prisms  of  the  same  altitude,  whose  base  is  given  in 
magnitude  and  species,  or  figure,  or  shape,  the  right 
prism  has  the  smallest  surface. 

For,  the  area  of  each  face  of  the  prism  is  proportional  to 
its  height  ;  therefore  the  area  of  each  face  is  the  smallest 
when  its  height  is  the  smallest,  that  is  to  say,  when  it  is  equal 
to  the  altitude  of  the  prism  itself:  and  iu  that  case  the  prism 
is  evidently  a  right  prism,    q.  k.  d. 

TIIEOREM  xviii. 

Of  all  prisms  whose  base  is  given  in  magnitude  and  species, 
and  whose  lateral  surface  is  the  same,  tho  right  prism  has 
the  greatest  altitude,  or  the  greatest  capacity. 

This  is  the  converse  of  the  preceding  theorem,  and  may 
readily  be  proved  after  the  manner  of  theorem  2. 

TIIEOREM  XW. 

Of  all  right  prisms  of  the  same  altitude,  whose  liases  are4 
given  in  magnitude  and  of  a  given  number  of  sides,  that 
whose  base  is  a  regular  figure  has  the  smallest  surface. 

For,  the  surface  of  a  right  prism  of  given  altitude,  and 
base  giveu  in  magnitude,  is  evidently  proportional  to  the 
perimeter  of  its  base.  But  (th.  10)  the  base  being  given  in 
magnitude,  and  having  a  given  nnmber  of  sides,  its  netu 


f 

552  elements  or  nornuf  cm. 

meter  ■  smallest  when  it  is  regular  :  whence,  the  truth  of 
the  pr  position  is  manifest. 

THEOREM  XX. 

Of  two  right  prisms  of  the  same  altitude,  and  with  ir.*egu!ar 
bases  equal  in  surface,  that  whose  base  has  the  ^-eatest 
number  of  sides  has  the  smallest  surface  ;  aj^,  in  par- 
ticular, the  right  cylinder  has  a  smaller  surface  than  any 
prixm  of  the  same  altitude  and  the  same  capacity. 

The  demonstration  is  analogous  to  that  of  the  preceding 
theorem,  being  at  once  deduciblc  from  theorems  16  and  14. 

THEOREM  XXI. 

Of  all  right  prisms  whose  altitudes  and  whose  whole  sur- 
faces are  equal,  and  whose  bases  have  a  given  number 
of  sides  ;  that  whose  base  is  a  regular  figure  is  the 
greatest. 

Let  i',  p\  be  two  right  prisms  of  the  same  name,  equa\  in 
altitude,  and  equal  whole  surface,  the  first  of  these  having  a 
regular,  the  second  an  irregular  bnse ;  then  is  the  base  of 
the  prism  p',  less  than  the  base  of  the  prism  p. 

For,  let  p"  he  a  prism  of  equal  altitude,  and  whose  base 
is  equal  to  that  of  the  prism  p'  and  similar  to  that  of  the 
prism  p.  Then,  the  lateral  surface  of  the  prism  p"  is  smaller 
than  the  lateral  surface  of  the  prism  p'  (th.  It))  :  hence,  the 
total  surface  of  p"  is  smaller  than  the  total  surface  of  p',  and 
therefore  (by  hyp.)  smaller  than  the  whole  surface  of  p.  But 
the  prisms  p"  and  v  have  equal  altitudes,  and  similar  bases  ; 
therefore  the  dimensions  of  the  base  of  v"  are  smaller  than 
the  dimensions  of  the  base  of  p.  Consequently  the  base  of 
p%  or  that  of  p',  is  less  than  the  base  of  v  ;  or  the  base  of  r 
greater  than  that  of  p'.    q.  k.  d. 

THEOREM  XXII. 

Of  two  right  prisms,  having  equal  altitudes,  equal  total 
surfaces,  and  regular  bases,  that  whose  base  has  the 
greatest  number  of  sides,  has  the  greatest  capacity.  And, 
in  particular,  a  right  cylinder  is  greater  than  any  right 
prism  of  equal  altitude  and  equal  total  surface. 

The  demonstration  of  this  is  similar  to  that  of  the  pre- 
ceding theorem,  and  flows  from  th.  20. 


tOLIB*. 


THEOREM  XXm. 

The  greatest  parallelopiped  which  can  be  contained  under 
the  three  parts  of  a  given  line,  any  way  taken,  will  he 
that  constituted  of  equal  length,  breadth,  and  depth. 

For,  let  ab  be  the  given  line,  and, 
if  possible,  let  two  parts  ae,  kd,  be  1  |  \ 

unequal.  Bisect  ad  and  c,  then  will  A  C  B  D  B 
the  rectangle  under  ab  (=  ac+ce) 

and  ed  (=  ac  —  ce),  be  less  than  ac3,  or  than  ac  .  cd,  by 
the  square  of  ce  (th.  33  Geom.).  Consequently,  the  solid 
ab  .  ed  .  db,  will  be  less  than  the  solid  ac  .  cd  .  db  4  which 
is  repugnant  to  the  hypothesis. 

Cor.  Hence,  of  all  the  rectangular  parallelopipeds,  having 
the  sum  of  their  three  dimensions  the  same,  the  cube  is  the 
greatest. 

THSOBEM  XXIV. 

The  greatest  parallelopiped  thai  can  possibly  be  contained 
under  the  square  of  one  part  of  a  given  line,  and  the 
other  part,  any  way  taken,  will  be  when  the  former  pari 
is  the  double  of  the  latter. 

Let  ab  be  a  given  line,  and   t  t       t  , 

ac  =  2cb,  then  is  ac*  .  cb  the    "        I J  LI 
greatest  possible.  D  D     CTC  B 

For,  .let  ac  and  cb  be  any  other  parts  into  which  the 
given  line  ab  may  be  divided  ;  and  let  ac,  ac  be  bisected 
in  dd',  respectively.  Then  shall  ac9  .  cb  =  4ai>  •  dc  •  cb 
(cor.  to  theor.  31  Geom.  )  >  4ad'  .  dc  .  cb,  or  greater  than 
its  equal  c'a9  .  c  b,  by  the  preceding  theorem. 

THEOREM  XXV. 

Of  all  right  parallelopipeds  given  in  magnitude,  that  which 
has  the  smallest  surface  has  all  its  faces  squares,  or  is  a 
cube.  And  reciprocally,  of  all  parallelopipeds  of  equal 
surface,  the  greatest  is  a  cube. 

For,  by  theorems  19  and  21,  the  right  parallelopiped 
having  the  smallest  surface  with  the  same  capacity,  or  the 
greatest  capacity  with  the  same  surface,  has  a  square  for  its 
base.  But,  any  face  whatever  may  be  taken  for  base  :  there- 
fore, in  the  parallelopiped  whose  surface  is  the  smallest  with 
the  same  capacity,  or  whose  capacity  is  the  greatest  with  the 
same  surface,  any  two  opposite  faces  whatever  axe  squares  ; 
consequently,  this  parallelopiped  is  a  cube. 

Vol.  I.  71 


5M 


BLtMBffTs  of  uorxxmraT. 


THEOREM  XXVI. 

The  capacities;  of  prisms  circumscribing  the  same  right 
cylinder,  are  respectively  as  their  surfaces,  whether  total 
or  lateral. 

For,  the  capacities  are  respectively  as  the  bases  of  the 
prisms;  that  is  to  say  (th.  11),  as  the  perimeters  of  their 
bases  ;  and  these  arc  manifestly  as  the  lateral  surfaces : 
whence  the  proposition  is  evident. 

Cor.  The  surface  of  a  right  prism  circumscribing  a 
cylinder,  is  to  the  surface  of  that  cylinder,  as  the  capacity  of 
the  former,  to  the  capacity  of  the  latter. 

Def.  The  Archimedean  cylinder  is  that  which  circum- 
scribes a  sphere,  or  whose  altitude  is  equal  to  the  diameter 
of  its  base. 

THEOREM  XXVII. 

The  Archimedean  cylinder  has  a  smaller  surface  than  any 
other  right  cylinder  of  equal  capacity  ;  and  it  is  greater 
than  any  other  right  cylinder  of  equal  surface. 

Let  v  and  c  denote  two  right  cylinders,  of  which  the  first 
is  Archimedean,  the  other  not :  then, 

1st,    If .  .  .  r  =  c',  surf.  c<surf.  c' : 
«Mly,  if  surf,  c  =  surf,  c',  c>c'. 

For,  having  circumscribed  about  the  cylinders  c,  c',  the 
right  prisms  i\  p',  with  square  bases,  the  former  will  be  a 
cube,  the  second  not :  and  the  following  series  of  equal  ra- 
tios will  obtain,  viz.  c  :  v  :  :  surf,  c  :  surf,  p  :  :  base  c  :  base 
v  :  :  base  c'  :  base  v  :  :  r'  :  p'  :  :  surf,  c'  :  surf.  r'. 

Then,  1st :  when  c  =  c'.  Since  c  :  r  : :  c'  :  r',  it  follows 
that  p  =  r'  ;  and  therefore  (th.  25)  surf.  r<surf.  r'.  But, 
surf,  c  :  surf,  p  :  :  surf,  c'  :  surf,  r' ;  consequently  surf.  c< 
surf.  c'.    a.  r..  Id. 

2dlv  :  when  surf,  c  =-  surf.  c/.  Then,  since  surf,  c  :  surf, 
p  : :  surf,  c'  :  surf,  p',  it  follows  that  surf,  p  =  surf,  p' ;  and 
therefore  (th.  25)  p  >  p'.  But  c  :  r  : :  c'  :  r' ;  consequently 
c>c'.    a.  i:.  2i>. 

THEOREM  XXVIII. 

Of  all  right  prisms  whose  bases  are  circumscribable  about 
circles,  and  given  in  soecies,  that  whose  altitude  is  double 
the  radius  of  \n©  cwta  \nBttrta«&  v& 


SOLIDS. 


555 


smallest  surface  with  the  some  capacity,  and  the  greatest 
capacity  with  the  same  surface. 

This  may  be  demonstrated  exactly  as  the  preceding  theo- 
rem, by  supposing  cylinders  inscribed  in  the  prisms. 

Scholium, 

If  the  base  cannot  be  circumscribed  about  a  circle,  the 
right  prism  which  has  the  minimum  surface,  or  the  maximum 
capacity,  is  that  whose  lateral  surface  is  quadruple  of  the 
surface  of  one  end,  or  that  whose  lateral  surface  is  two  thirds 
of  the  total  surface.  This  is  manifestly  the  case  with  the 
Archimedean  cylinder ;  and  the  extension  of  the  property 
depends  solely  on  the  mutual  connexion  subsisting  between 
the  properties  of  the  cylinder,  and  those  of  circumscribing 
prisms* 

THEOSEX  XXIX. 

The  surfaces  of  right  cones  circumscribed  about  a  sphere, 
are  as  their  solidities. 

For,  it  may  bo  demonstrated,  in  a  manner  analogous  to  the 
demonstrations  of  theorems  11  and*26,  that  these  cones  are 
equal  to  right  cones  whose  altitude  is  equal  to  the  radius  of 
the  inscribed  sphere,  and  whose  bases  are  equal  to  the  total 
surfaces  of  the  cones :  therefore  the  surfaces  ai\d  solidities 
are  proportional. 

THEOREM  XXX. 

The  surface  or  the  solidity  of  a  right  cone  circumscribed 
about  a  sphere  is  directly  as  the  square  of  the  cone's 
altitude,  and  inversely  as  the  excess  of  that  altitude  over 
the  diameter  of  the  sphere. 

Let  vat  be  a  right-angled  triangle  which, 
by  its  rotation  upon  va  as  an  axis,  generates  a 
right  cone  ;  and  bda  the  semicircle  which  by 
a  like  rotation  upon  va  forms  the  inscribed 
sphere :  then,  the  surface  or  the  solidity  of 

the  cone  vanes  as  — . 

VB 

For,  draw  the  radius  cd  to  the  point  of  contact  of  the 
semicircle  and  vt.    Then,  because  the  triangles  vat,  vdc, 
are  similar,  it  is  at  :  vr  :  :  cd  :  vc. 
And,  by  compos,  at  :  at  +  vt  :  :  cd  :  cd  +  cv  =  va  ; 


556  ELEMENTS  OF  nOPEHlMSTIT. 

Therefore  at*  :  (at  +  vt)  at  : :  cd  :  va,  by  multiply* 

ing  the  terms  of  the  first  ratio  by  at. 

But,  because  vb,  vd,  va,  are  continued  proportionals, 

it  is  vb  :  va  :  :  vn3  :  va'  :  :  cd3  :  at3  by  aim.  triangles. 

But  cd  :  va  s  :  at3  :  (at  +  vt)  at  by  the  last :  and  thest 

mult,  give  cd  .  vb  :  va3  : ;  cd3  :  (at  +  vt)  at, 

or  v»  :  cd  : :  va3  :  (at  +  vt)  at  =  cd  .  — . 

But  the  surface  of  the  cone,  which  is  denoted  by  «r .  at*  + 
* .  at  .  vt*,  is  manifestly  proportional  to  the  first  member 
of  this  equation,  is  also  proportional  to  the  second  member, 

or,  since  cd  is  constant,  it  is  proportional  to  i^,  or  to  a  third 

proportional  to  bv  and  av.  And,  since  the  capacities  of  these 
circumscribing  cones  are  as  their  surfaces  (th.  29),  the  troth 
of  the  whole  proposition  is  evident. 

Lemma  2. 

The  difference  of  two  right  lines  being  given,  the  third 
proportional  to  the  less  and  the  greater  of  them  is  a  minimum 
when  the  greater  of  those  lines  is  double  the  other. 

Let  av  and  bv  he  two  right 

lines,  whose  difference  ab  is   x  ,  

given,  and  let  ap  be  a  third  7  i  _L  p 
proportional  to  bv  and  av  ;  ^  * 

then  is  ap  a  minimum  when  av  =  2bv. 

For,  since    ap  :  av  : :  av  :  bv  ; 

By  division  ap  :  ap  —  av  :  :  av  :  av  —  bv  ; 

That  is,       ap  :  vp  :  :  av  :  ab. 

Hence,  vp  .  av=ap  .  ab. 
But  vp  .  av  is  cither  =  or  <  Jap2  (cor.  to  th.  31  Geooi. 
and  th.  23  of  this  chapter). 

Therefore  ap  .  ab  <  {ap3  :  whence  4ab  <~  ap,  or  ap  >  4ab. 
Consequently  the  minimum  value  of  a p  is  the  quadruple  of 
ab  ;  and  in  that  case  rv  .=  va  ~  2ab.    q.  e.  of. 


•  w  being  rr-  3  141593.    See  Vol.  i.  p.  422. 

t  Though  the  evidence  of  n  single  demonstration,  conducted  on  sound 
mathematical  principles,  is  really  irresistible,  and  then-fore  needs  no 
corroboration  ;  yet  it  is  frequently  conducive  as  well  I  omen'al  improve- 
ment, as  to  mental  delight,  to  obtain  like  results  from  different  processes. 
In  this  view  it  will  be  advantageous  to  the  student,  to  confirm  the  truth 
of  several  i»{  \\\e  pro\io*\\\wia\ii  \\\\%  Ocv*\»Vt*\\^  w\*tvw.^  ^  fluxions  I 
Mialyth.   Let  the  Vn&vb  «nwvrcw*X»&  \^TOft^feaH«\KVN&%\A  v&wotVst'vt. 


■OUDfe 


THEOREM  XXXI. 

Of  all  right  cones  circumscribed  about  the  same  sphere,  the 
smallest  is  that  whose  altitude  is  double  the  diameter  of 
tho  sphere. 

For,  by  th.  30,  the  solidity  varies  as      (see  the  fig.  to 

that  theorem) :  and,  by  lemma  2,  since  va  —  vb  is  given,  the 
va" 

third  proportional  —  is  a  minimum  when  va  =  Sab.  q.  k.  d* 

Cor.  1.  Hence,  the  distanco  from  the  centre  of  the  sphere 
to  the  vertex  of  the  least  circumscribing  cone,  is  triple  the 
radius  of  the  sphere* 

Cor.  2.  Hence  also,  the  side  of  such  cone  is  triple  the 
radius  of  its  base. 

THEOREM  XXXII. 

The  whole  surface  of  a  right  cone  being  given,  the  inscribed 
sphere  is  the  greatest  when  the  slant  side  of  the  cone  is 
triple  the  radius  of  its  base. 

*  For,  let  c  and  c'  be  two  right  cones  of  equal  whole  sun 
face,  the  radii  of  their  respective  inscribod  spheres  being 
denoted  by  r  and  r'  ;  let  the  side  of  the  cone  c  be  triple  the 
radius  of  its  base,  the  same  ratio  not  obtaining  in  c ;  and 
let  c"  be  a  cone  similar  to  c,  and  circumscribed  about  the 
same  sphere  with  c.  Then,  (by  th.  31)  surf,  c"  <  surf,  c' ; 
therefore  surf,  c"  <  surf.  c.  But  c"  and  c  are  similar,  therefore 
all  the  dimensions  of  c"  are  less  than  the  corresponding 
dimensions  of  c  :  and  consequently  the  radius  r'  of  the  sphere 
inscribed  in  c"  or  in  c',  is  less  than  the  radius  s  of  the  sphere 
inscribed  in  c,  or  r  >  a',    q.  e.  d. 

Cor.  The  capacity  of  a  right  cone  being  given,  the  in- 
scribed sphere  is  the  greatest  when  the  side  of  the  cone  is 
triple  the  radius  of  its  base. 


example ;  and  let  ab  be  denoted  by  a,  av  by  x,  bv  by  x — a.  Then  we 
shall  have  x  —  a :  x :  t  x :  the  third  proportional ;  which  is  to  be  a 
minimum.  Hence,  the  fluxion  of  this  frnctfon  will  he  equal  to  sero 
(Flux.  art.  57).  That  is,  (Flui.arts.  19  and  35),  XJ^~L  =0.  Cost 
sequently  **— 8oz=0,  and  x-2«,  or  av=2ab,  at  above. 


558 


ELEMENTS  OP  ISOFESIXETRY. 


For  the  capacities  of  such  cones  vary  as  their  surfaces 
(th.  29). 


THEOREM  XXXIII. 

Of  all  right  cones  of  equal  whole  surface,  the  greatest  is  that 
whose  side  is  triple  the  radius  of  its  base  :  and  recipro- 
cally, of  all  right  cones  of  equal  capacity,  that  whose  side 
is  triple  the  radius  of  its  base  has  the  least  surface. 

For,  by  th.  20,  the  capacity  of  a  right  cone  is  in  the  com- 
pound ratio  of  its  whole  surface  and  the  radius  of  its  in- 
scribed sphere.  Therefore,  the  whole  surface  being  given, 
the  capacity  is  proportional  to  the  radius  of  the  inscribed 
sphere :  and  consequently  is  a  maximum  when  the  radius  of 
the  inscribed  sphere  is  such  ;  that  is,  (th.  32)  when  the  side 
of  the  cone  is  triple  the  radius  of  the  base*. 

Again,  reciprocally,  the  capacity  being  given,  the  surface 
is  in  the  inverse  ratio  of  the  sphere  inscribed  :  therefore,  it 


•  Here  again  a  similar  result  mny  easily  be  deduced  from  the  method 
of  fluxion*.  Let  the  radius  of  the  Iirsc  he  denoted  hy  x,  the  slant  side 
of  the  cone  hy  its  whole  surface  hy  a\ and  3*14159$  hy  r.  Then  the 
circumference  of  the  cone's  base  will  be  2*7,  iU  area  rx-\  and  the  con- 
vex surface  ?n:.    The  whole  surface  is,  therefore,  —  ir*1  -f-  *z= :  and 

this  being  —  a\  we  have  s  — —  T-    But  the  altitude  of  the  cone  b 

equal  to  the  square  root  of  the  difference  of  ti  c  squares  of  the  side  and 

of  the  radius  of  the  base  ;  that  is,  it  is  .-_  v(~  — ).    And  this  mnl- 

tiplied  into  \  of  the  area  of  the  base,  viz.  by  \vi\  gives  \tx2  V{—  — — \ 

for  the  capacity  of  the  cone.    Now,  this  being  a  maximum,  its  square 

must  be  so  likewise  (Flux.  art.  58),  that  h,  ^JLZ^**'*1,  or  rejecting  the 

denominator,  as  constant,  ah:- —  2t«7x'  must  be  a  maximum.  This,  in 
fluiions,  is  2a*xi  —  ti*a"i<x     0;  whence  wc  have  an-  —  4rJ3     0,  and 

consequently  x  ._  \  —  ;  and  a?  -  AvzK    Substituting  this  value  of  «* 

for  it,  in  the  value  of  z  above  given,  there  results  z  —  —  —  x  =  4*J* 

■—z  -  Ax  —  x  -  Therefore,  the  side  of  the  cone  is  triple  the  ra- 
dius of  its  base.  Or,  the  squan*  of  the  altitude  is  to  the  square  of  the 
radius  of  the  base,  hs  ft  \o  A  .  \u  vV&  v^&ax^  &&so&t&c  of  the  bast, 
as  2  to  1. 


SOLUM. 


MO 


is  the  smallest  when  that  radius  is  the  greatest;  that  is  (th. 
32)  when  the  side  of  the  cone  is  triple  the  radius  of  its  base. 

Q.  E.  D. 

THEOREM  XXXIV. 

The  surfaces,  whether  total  or  lateral,  of  pyramids  circum- 
scribed about  the  same  right  cone,  are  respectively  as  their 
solidities.  And,  in  particular,  the  surface  of  a  pyramid 
circumscribed  about  a  cone,  is  to  the  surface  of  that  cone, 
as  the  solidity  of  the  pyramid  is  to  the  solidity  of  the  cone  ; 
and  these  ratios  are  equal  to  those  of  the  surfaces  or  the 
perimeters  of  the  bases. 

For,  the  capacities  of  the  several  solids  are  respectively  as 
their  bases  ;  and  their  surfaces  are  as  the  perimeters  of  those 
bases  :  so  that  the  proposition  may  manifestly  be  demonstrat- 
ed by  a  chain  of  reasoning  exactly  like  that  adopted  in  theo- 
rem 11. 

THEOREM  XXXV. 

The  base  of  a  right  pyramid  being  given  in  species,  the  capa- 
city of  that  pyramid  is  a  maximum  with  the  same  surface, 
and,  on  the  contrary,  the  surface  is  a  minimum  with  the 
same  capacity,  when  the  height  of  one  face  is  triple  the 
radius  of  the  circle  inscribed  in  the  base. 

Let  f  and  p'  be  two  right  pyramids  with  similar  bases,  the 
height  of  one  lateral  face  of  p  being  triple  the  radius  of  the 
circle  inscribed  in  the  base,  but  this  proportion  not  obtaining 
with  regard  to  p' :  then 

1st.    If  surf,  p  =  surf,  p',  p  >  p'. 

2dly.  If  .    .  p  =  .    .  p',  surf,  p  <  surf.  p'. 

For,  let  c  and  c'  be  right  comes  inscribed  within  the  pyra- 
mids p  and  p' :  then,  in  the  cone  c,  the  slant  side  is  triple  the 
radius  of  its  base,  while  this  is  not  the  case  with  respect  to 
the  cone  c'.  Therefore,  if  c  =  c',  surf,  c  <  surf,  c' ;  and,  if 
surf,  c  =  surf,  c',  c  >  c  (th.  33). 

But,  1st.  surf,  p  :•  surf,  c  : :  surf,  p'  :  surf,  c  ; 
whence,  if  surf,  p  =  surf,  p',  surf,  c  =  surf,  c  ; 
therefore  c  >  c\    But  p  :  c  : :  p'  :  c'.    Therefore  p  >  p'. 

2dly.  p:c::p':c'.  Theref.  if  p=p,  c=c'  :  consequently 
surf,  c  <  surf,  c .  But  surf,  p  :  surf,  c  •  :  surf,  p' :  surf.  c\ 
Whence,  surf,  p  <  surf.  p. 

Cor.  The  regular  tetraedron  possesses  the  property  of  the 
minimum  surface  with  the  same  capacity,  and  of  tha  toAai* 


MO 


ELEMENTS  OF  ISOFEIUXETEY. 


mum  capacity  with  the  same  surface,  relatively  to  all  right 
pyramids  with  equilateral  triangular  bases,  and,  a  fortiori, 
relatively  to  every  other  triangular  pyramid. 

THEOREM  XXXVI. 

A  sphere  is  to  any  circumscribing  solid,  bounded  by  plane 
surfaces,  as  the  surface  of  the  sphere  to  that  of  the  cir- 
cumscribing solid. 

For,  since  all  the  planes  touch  the  sphere,  the  radius  drawn 
to  each  point  of  contact  will  be  perpendicular  to  each  re- 
spective plane.  So  that,  if  planes  be  drawn  through  the  cen- 
tre of  the  sphere  and  through  all  the  edges  of  the  body,  the 
body  will  be  divided  into  pyramids  whose  bases  are  the  re- 
spective planes,  and  their  common  altitude  the  radius  of  the 
sphere.  Hence,  the  sum  of  all  these  pyramids,  or  the  whole 
circumscribing  solid,  is  equal  to  a  pyramid  or  a  cone  whose 
base  is  equal  to  the  whole  surface  of  that  solid,  and  altitude 
equal  to  the  radius  of  the  sphere.  But  the  capacity  of  the 
sphere  is  equal  to  that  of  a  cone  whose  base  is  equal  to  the 
surface  of  the  sphere,  and  altitude  equal  to  its  radius.  Con- 
sequently, the  capacity  of  the  sphere,  is  to  that  of  the  circum- 
scribing solid,  as  the  surface  of  the  former  to  the  surface  of 
the  hitter :  both  having,  in  this  mode  of  considering  them,  a 
common  altitude,    q.  k.  p. 

Cor.  1.  All  circumscribing  cylinders,  cones,  &c.  are  to 
the  sphere  they  circumscribe,  as  their  respective  surfaces. 

For  the  same  proportion  will  subsist  between  their  inde- 
finitely small  corresponding  segments,  and  therefore  between 
their  wholes. 

Cor.  2.  All  bodies  circumscribing  the  same  sphere,  are 
respectively  as  their  surfaces. 

THEOREM  XXXVII. 

The  sphere  is  greater  than  any  polyedron  of  equal  surface. 

For,  first  it  may  be  demonstrated,  by  a  process  similar  to 
that  adopted  in  theorem  9,  that  a  regular  polyedron  has  a 
greater  capacity  than  any  other  polyedron  of  equal  surface. 
Let  p,  therefore,  be  a  regular  polyedron  of  equal  surface  to 
a  sphere  s.  Then  r  must  either  circumscribe  s,  or  fall  partly 
within  it  and  partly  without  it,  or  fall  entirely  within  it.  The 
first  of  these  sud^siVvoti*  \a  cxrotaurg  \^vV,  V\^<*thesis  of  the 
proposition,  because  m  c*s^<v\fc 


SOLIDS. 


Ml 


be  equal  to  that  of  s.  Either  the  2d  or  3d  supposition  there, 
fore  must  obtain  ;  and  then  each  plane  of  the  surface  of  p 
roust  fall  either  partly  or  wholly  within  the  sphere  s  :  which- 
ever of  these  be  the  case,  the  perpendiculars  demitted  from 
the  centre  of  s  upon  the  planes,  will  be  each  less  than  the 
radius  of  that  sphere  :  and  consequently  the  polyedron  r 
must  be  less  than  the  sphere  s,  because  it  has  an  equal  base, 
but  a  less  altitude,    q.  e.  d. 

Cor.  If  a  prism,  a  cylinder,  a  pyramid,  or  a  cone,  be  equal 
to  a  sphere  either  in  capacity,  or  in  surface ;  in  the  first  case, 
the  surface  of  the  sphere  is  less*  than  the  surface  of  any  of 
those  solids ;  in  the  second,  the  capacity  of  the  sphere  is 
greater  than  that  of  either  of  those  solids. 

The  theorems  in  this  chapter  will  suggest  a  variety  of 
practical  examples  to  exercise  the  student  in  computation. 
A  few  such  are  given  below. 

EXERCISES. 

Ex.  1.  Find  the  areas  of  an  equilateral  triangle,  a  square, 
a  hexagon,  a  dodecadoo,  and  a  circle,  the  perimeter  of  each 
being  30. 

Ex.  2.  Find  the  difference  between  the  area  of  a  triangle 
whose  sides  are  3,  4,  and  5,  and  of  an  equilateral  triangle  of 
equal  perimeter. 

Er.  3.  What  is  the  area  of  the  greatest  triangle  which 
can  be  constituted  with  two  given  sides  8  and  11  ;  and  what 
will  be  the  length  of  its  third  side  ? 

Ex.  4.  The  circumference  of  a  circle  is  12,  and  the  pe- 
rimeter of  an  irregular  polygon  which  circumscribes  it  is  15 : 
what  are  their  respective  areas  ? 

Ex.  5.  Required  the  surface  and  the  atiMfty  of  the 
greatest  parallelopiped,  whose  length,  breadth;  and  depth, 
together  make  18? 

Ex.  6.  The  surface  of  a  square  prism  is  546 :  what  is  its 
solidity  when  a  maximum  ? 

Ex.1.  The  content  of  a  cylinder  is  169-645068:  what 
is  its  surface  when  a  minimum  ? 

Ex.  8.  The  whole  surface  of  a  right  cone  is  201  -061952 : 
what  is  its  solidity  when  a  maximum  ? 

Ex.  9.  The  surface  of  a  triangular  pyramid  is  43*30127: 
what  is  its  capacity  when  a  maximum  ? 

Ex.  10.   The  radius  of  a  sphere  is  10.   Required  the  so- 

Vol.  I.  72 


663 

• 


questions  in 


lidities  of  this  sphere,  of  its  circumscribed  equilateral  cone, 
and  of  its  circumscribed  cylinder. 

Ex.  11.  "the  surface  of  a  sphere  is  28*274887,  and  of  an 
irregular  polycdron  circumscribed  about  it  85 :  what  are  their 
respective  solidities  ? 

Ex.  12.  The  solidity  of  a  sphere,  equilateral  cone,  sad 
Archimedean  cylinder,  are  each  500 :  what  are  the  surfaces 
and  respective  dimensions  of  each  ? 

Ex.  13.  If  the  surface  of  a  sphere  be  represented  by  the 
number  4,  the  circumscribed  cylinder's  eonvex  surface  and 
whole  surface  will  be  4  and  0,  and  the  circumscribed  equila- 
teral cone's  convex  and  whole  surface,  6  and  0  respectively. 
Show  how  these  numbers  are  deduced. 

Ex.  14.  The  solidity  of  a  sphere,  circumscribed  cylinder, 
and  circumscribed  equilateral  cone,  are  as  the  numbers  4, 6, 
and  0.    Required  the  proof. 


PRACTICAL  EXERCISES  IN  MENSURATION. 

Quest.  1.  Wiiat  difference  is  there  between  a  floor  28 
feet  long  by  20  broad,  and  two  others,  each  of  half  the 
dimensions  ;  and  what  do  all  three  come  to  at  45*.  per 
square,  or  100  square  feet  ? 

Ans.  dif.  280  sq.  feet.    Amount  18  guineas. 

Quest.  2.  An  elm  plank  is  14  feet  3  inches  long,  and  I 
would  have  just  a  square  yard  slit  off  it ;  at  what  distance 
from  the  edge  must  the  line  be  struck  ?       Ana.  7f|  inches. 

Quest.  3.  A  ceiling  contains  114  yards  6  feet  of  plaster, 
ing,  and  the  room  is  28  feet  broad  ;  what  is  the  length  of  itf 

Ana.  36$  feet. 

Quest.  4.  A  common  joist  is  7  inches  deep,  and  2J 
thick  ;  but  I  want  a  scantling  just  as  big  again,  that  shall 
be  3  inches  thick  ;  what  will  the  other  dimension  be  ? 

Ans.  11}  inches. 

Quest.  5.  A  wooden  trough  cost  me  3*.  2d.  painting 
within,  at  6d.  per  yard  ;  the  length  of  it  was  102  inches, 
and  the  depth  21  inches  ;  what  was  the  width  ? 

Ans.  27}  inches. 

Quest.  6.  If  my  court-yard  be  47  feet  9  inches  square, 
and  I  have  laid  a' foot-path  with  Purbeck-stone,  of  4  feet 
*ide,  along  one  side  of  it ;  what  will  paving  the  rest  with 
flints  come  to,  at  6d.  per  square  yard  ?      Ans.  bl.  16#.  0\<L 

Quest.  7.  lL  ladder,  36  feet  long,  may  be  so  planted. 


XSKSUSATIOX. 


568 


that  it  shall  reach  a  window  30*7  feet  from  the  ground  on 
one  side  of  the  street ;  and,  by  only  turning  it  over,  without 
moving  the  foot  out  of  its  place,  it  will  do  the  same  by  a 
window  18-9  feet  high  on  the  other  side  :  what  is  the  breadth 
of  the  street  ?  Ans.  50  084  feet. 

Qubst.  8.  The  paving  of  a  triangular  court,  at  18d.  per 
foot,  came  to  1007. ;  the  longest  of  the  three  sides  was 
88  feet ;  required  the  sum  of  the  other  two  equal  sides  ? 

Ans.  10-085 /eet. 

Quest.  9.  The  perambulator,  or  surveying  wheel,  is  so 
contrived,  as  to  turn  just  twice  in  the  length  of  a  pole,  or 
16^  feet ;  required  the  diameter  ?  Ans.  2*626  feet. 

Quest.  10.  In  turning  a  one- horse  chuise  within  a  ring  of 
a  certain  diameter,  it  was  observed,  that  the  outer  wheel 
made  two  turns,  while  the  inner  made  but  one  :  the  wheels 
were  both  4  feet  high ;  and,  supposing  them  fixed  at  the 
statutable  distance  of  5  feet  asunder  on  the  axle-tree,  what 
was  the  circumference  of  the  track  described  by  the  outer 
wheel  ?  Ans.  62-832  feet. 

Quest.  11.  What  is  the  side  of  that  equilateral  triangle, 
whose  area  cost  as  much  paving  at  8d.  a  foot,  as  the  palli. 
sading  the  three  sides  did  at  a  guinea  a  yard  ? 

Ans.  72-746  feet. 

Quest.  12.  A  roof,  which  is  24  feet  8  inches  by  14  feet 
6  inches,  is  to  be  covered  with  lead  at  81b.  per  square  foot : 
what  will  it  come  to  at  18*.  per  cwt.  ?    Ans.  22/.  19*.  10><i. 

Quest.  13.  Having  a  rectangular  marble  slab,  58  inches 
by  27,  I  would  have  a  square  foot  cut  off  parallel  to  the 
snorter  edge ;  I  would  then  have  the  like  quantity  divided 
from  the  remainder  parallel  to  the  longer  side  ;  and  this 
alternately  repeated,  till  there  shall  not  be  the  quantity  of 
a  foot  left :  what  will  be  the  dimensions  of  the  remaining 
piece?  Ans.  20*7  inches  by  6-086. 

N.  B.  This  question  may  be  solved  neatly  by  an  alge- 
braical process,  as  may  be  seen  in  the  Ladies'  Diary  for  18V 3. 

Quest.  14.  Given  two  sides  of  an  obtuse -angled  triangle, 
which  are  20  and  40  poles  ;  required  the  third  side,  that  the 
triangle  may  contain  just  an  acre  of  land  ? 

Ans.  58-876 or  23  099. 

Quest.  15.  How  many  bricks  will  it  take  to  build  a  wall, 
10  feet  high,  and  500  feet  long,  of  a  brick  and  half  thick  ; 
reckoning  the  brick  10  inches  long,  and  4  courses  to  the 
foot  in  height  ?  Ans.  72000. 

Quest.  16.  How  many  bricks  will  build  a  square  pyramid 
of  100  feet  on  each  side  at  the  base,  and  also  100  feet  per- 


:ttodfinsnsisnsnf.a 

\  inches  bog,  6  inch**  broad,  and  8  inches  thick? 


Qmr.  17.  IT,  from  a  right-angled  triangle, 
-is  1%  and  perpendicular  16  feet,  a  line  be  drawn  parallel  le 
Jar, 


ttii^off  a  triai^W  whose  araak  M 
required  the  aides of  this  triangle?  - 

Ana.  6,  8,  and  10. 

'  Qraev.  18.  If  a  round  pillar,  7  inches  acroee*  bare  4  feet 
«f  Hon*  in  it;  of  what  diameter  ia  the  column,  of  equal 


tenth,  that  conlaint  10  tinea  as  nmeh  f  .jb,  • 

Quest.  19.  A  circular  fishpond  ie  to  be  made  inn  gar* 
den,  that  shall  take  up  just  half  an  acre  ;  what  innat  be  the 
length  of  the  cord  that  striken  the  circle  T  s  Ans*  SYf^prda. 

QrasT.  20.  When  a  roof  is  of  a  tree  pitch,'  the  rafters 
are  f  of  the  breadth  of  the  building :  now  supposing  the 
eaves-board*  to  project  10  inches  on  a  side,  what  will  the 
new  ripping  a  house  cost,  that  measures  32  feet  9  inches 
long,  by  22  feet  9  inches  broad  on  the  flat,  at  15s.  per 
square  f  Ans.  81.  15s.  *\<L 

Quest.  21.  A  cable,  which  is  3  feet  long,  and  0  inches 
in  compass,  weighs  221b. ;  what  will  a  fathom  of  that  cable 
weigh,  which  measures  a  foot  round  ?  Ans.  78jlb. 

Quest.  22.  A  plumber  has  put  281b.  per  square  foot 
into  a  cistern,  74  inches  and  twice  the  thickness  of  the  lead 
long,  26  inches  broad,  and  40  deep ;  he  has  also  put  three 
stays  across  it  within,  16  inches  deep,  of  the  same  strength, 
and  reckons  22s.  per  cwt.  for  work  and  materials.  A  mason 
has  in  return  paved  him  a  workshop,  22  feet  10  inches  broad, 
with  Purbeck  stone,  at  Id.  per  foot ;  and  upon  the  balance 
finds  there  is  3*.  6d.  due  to  the  plumber ;  what  was  the 
length  of  the  workshop,  supposing  sheet  lead  Tvv  of  an  inch 
thick  to  weigh  5-809lbs.  per  foot  ?  Ans.  32-2825  feet 

Qckst.  23.  The  distance  of  the  centres  of  two  circles, 
whose  diameters  are  each  50,  being  given,  equal  to  30;  what 
is  the  area  of  the  space  inclosed  by  their  circumferences ! 

Ans.  559*119. 

Quest.  24.  If  20  feet  of  iron  railing  weigh  half  a  ton, 
when  the  bars  are  an  inch  and  quarter  square ;  what  will  50 
feet  come  to  at  3} d.  per  lb.,  the  bars  being  but J  of  an  inch 
square  1  Ans.  20Z.  Of.  2d. 

Quest.  25.  It  is  required  to  find  the  thickness  of  the 
lead  in  a  pipe,  of  ttu  vm&  ami  piaster  bore,  which  weighs 


I 


MElfSUEJ^TIOlt. 


565 


141b.  per  yard  in  length  ;  the  cubic  foot  of  lead  weighing 
11925  ounces  ?  Ans.  -20737  inches. 


Quest.  26.  Supposing  the  expense  of  paving  a  semicir- 
cular plot,  at  2#.  4d.  per  foot,  come  to  102. ;  what  is  the 
diameter  of  it  ?  Ans.  14*7737  feet. 

Quest.  27.  What  is  the  length  of  a  chord  which  cuts  off 
£  of  the  area  from  a  circle  whose  diameter  is  280  ? 


Quest.  28.  My  plumber  has  set  me  up  a  cistern,  hit 
shop-book  being  burnt,  he  has  no  means  of  bringing  in  the 
charge,  and  I  do  not  choose  to  take  it  down  to  have  it 
weighed  ;  but  by  measure  he  finds  it  contains  Mf\  square 
feet,  and  that  it  is  precisely  |  of  an  inch  in  thickness.  Lead 
was  then  wrought  at  2/.  per  fother  of  19}  cwt.  It  is 
required  from  these  items  to  make  out  the  bill,  allowing 
6J  oz.  for  the  weight  of  a  cubic  inch  of  lead  ? 

Ans.  4/.  \U.2d. 

Quest.  20.  What  will  iho  diameter  of  a  globe  be,  when 
the  solidity  and  superficial  content  are  expressed  by  the 


Quest.  30.  A  sack,  that  would  hold  3  bushels  of  corn, 
is  22^  inches  broad  when  empty ;  what  will  another  sack 
contain,  which,  being  of  the  same  length,  has  twice  its 
breadth  or  circumference  ?  Ans.  12  bushels. 

Quest.  31.  A  carpenter  is  to  put  an  oaken  curb  to  a 
round  well,  at  84.  per  foot  square  :  the  breadth  of  the  curb 
is  to  be  8  inches,  and  the  diameter  within  3}  feet :  what 
will  be  the  expense  ?  Ans.  61.  6|<f. 

Quest.  32.  A  gentleman  has  a  garden  100  feet  long,  and 
80  feet  broad  ;  and  a  gravel  walk  is  to  be  made  of  an  equal 
width  half  round  it :  what  must  the  breadth  of  the  walk  be, 
to  take  up  just  half  the  ground  ?  Ans.  25*068  feet. 

Quest.  33.  The  top  of  a  may-pole,  being  broken  off  by 
a  blast  of  wind,  struck  the  ground  at  15  feet  distance  from 
the  foot  of  the  pole  ;  what  was  the  height  of  the  whole  may- 
pole, supposing  the  length  of  the  broken  piece  to  be  39 
feet  ?  Ans.  75  feet. 

Quest.  34.    Seven  men  bought  a  grinding-stone  of  60 
inches  diameter,  each  paying  |  part  of  the  expenxe  ;  what 
part  of  the  diameter  must  each  grind  down  for  his  share  ? 
Ans.  the  1st  4-4508, 2d,  4-8400,  3d  5-3535,  4th  6  0705, 
5th  7-2079,  6th  9-3935,  7th  22-6778  inches. 

Quest.  35.  A  maltster  has  a  kiln,  that  is  16  feet  6  inches 
square  :  but  he  wants  to  pull  it  down,  and  build  a  new  one, 


Ans.  278-6716. 


Ans.  6. 


 /aVytWeatawasasnehati 

what  onnt  te  the  length  of  its  side  T 
Ovist.  90.  How  assay  8  inch  < 
12  inch  cohe  T 

Qukst*  91*  How  long  must  tho  tether  of  a  home  he,  Hist 
will  allow  him  to  grase,  quite  aroaaat,  just  an  mere  sf 
ground?  An*.  30*  jar*. 

QvasT.  38.   What  will  the  painting  of  a  conical  sane 


to  at  84  per  yard  ;  supposing  the  height  to  ha  118 
feet,  and  the  circumference  of  the  base  64  feet  7 

Ana.  112.  On  SjdL 

Quest.  89.  The  diameter  of  a  standard  corn  baahal  it 
18}  inches,  and  its-depth  8  inches;  then  what  aanat  the 
diameter  of  that  bushel  be,  whoso  depth  is  7}  inches! 

Ana.  19-1087  inches. 

Qukst.  40.  Suppose  the  ball  on  the  top  of  St.  ftwTi 
church  is  0  feet  in  diameter ;  what  did  the  gilding  of  h  coat 
at  8}  per  square  inch  ?  Ans.  2871.  10s.  Id. 

Qukst.  41.  What  will  a  frustum  of  a  marble  cone  come 
to  at  12*.  per  solid  foot ;  tho  diameter  of  the  greater  end 
being  4  feet,  lhat  of  the  less  end  1  j,  and  the  length  of  the 
slant  side  8  feet  ?  Ans.  801.  It.  lOjd. 

Quest.  42.  To  divide  a  cone  into  three  equal  parts  by 
sections  parallel  to  the  base,  and  to  find  the  altitudes  of  the 
three  parts,  the  height  of  the  whole  cone  being  20  inches? 

An*  the  upper  part  18-867 
the  middle  part  3*61)5 
the  lower  part  2-528 

Quest.  48.  A  gentleman  has  a  bowling-green,  880  feet 
long,  and  200  feet  broad,  which  he  would  raise  I  foot  higher, 
by  means  of  the  earth  to  be  dug  out  of  a  ditch  that  goes 
round  it  :  to  what  depth  must  the  ditch  be  dug,  supposing 
its  breadth  to  be  every  where  8  feet  ?  Ans.  7f  f  feet. 

Quest.  44.  How  high  above  tho  earth  must  a  person  be 
raised,  thut  he  may  see  J  of  its  surface  ? 

Ans.  to  the  height  of  the  earth's  diameter. 

Quest.  45.  A  cubic  foot  of  brass  is  to  be  drawn  into  wire 
of  of an  inch  in  diameter ;  what  will  the  length  of  the 
wire  be,  allowing  no  loss  in  the  metal  ? 

Ans.  97784-707  yards,  or  55  miles  084*707  yards. 

Qukst.  46.  Of  what  diameter  must  the  bore  of  a  cannon 
be,  which  is  cast  for  a  ball  of  241b.  weight,  so  that  the  dia- 
meter of  the  bore  may  be  T!ff  of  un  inch  more  than  that  of 
the  ball  1  Ans.  5*047  inches. 


XKSSUJUTIOff. 


567 


Quest.  47?  {Supposing  the  diameter  of  an  iron  91b,  ball  to 
be  4  inches,  as  it  is  very  nearly ;  it  is  required  to  find  the. 
diameters  of  the  several  balls  weighing  1,  2,  3,  4,  6,  12, 
18,  24,  32,  36,  and  421b.  and  the  calibre  of  their  guns, 
allowing  f1,  of  the  calibre,  or  T'ff  of  the  ball's  diameter,  for 
windage. 

Answer. 


Wt. 

Diameter 

Calibre 

ball. 

ball. 

gun. 

1 

1*9230 

1-9622 

2 

2-4228 

2-4#23 

3 

2  7784 

2-8301 

4 

30526 

31149 

6 

3-4943 

3-5656 

9 

4-0000 

4  0816 

12 

4-4026 

4-4924 

18 

5-0397 

5-1425 

24 

5-5469 

5*6601 

32 

6-1051 

6-2297 

36 

6-3496 

6  4792 

42 

6-6844 

6-8208 

Quest.  48.  Supposing  the  windage  of  all  mortars  to  be 
v\r  of  the  calibre,  and  the  diameter  of  the  hollow  part  of  the 
shell  to  be  fs  of  the  calibre  of  the  mortar  :  it  is  required  to 
determine  the  diameter  and  weight  of  the  shell,  and  the 
quantity  or  weight  of  powder  requisite  to  fill  it,  for  each  of 
the  several  sorts  of  mortars,  namely,  the  13,  10,  8,  5*8,  and 
4*6  inch  mortar. 

Answer. 


Calib. 

Diameter 

Wt.  shell 

Wt.  of 

Wt.  shell 

mort. 

ball. 

empty. 

powder. 

filled. 

46 

4-523 

7-320 

0-583 

8-903 

5-8 

5-703 

16-677 

1*168 

17-845 

8 

7-867 

43-734 

3  065 

46-829 

10 

9  833 

85-476 

5-986 

91-462 

13 

12-783 

187-791 

13151 

200-942 

Quest.  49.  If  a  heavy  sphere,  whose  diameter  is  4  inches, 
be  let  fall  into  a  conical  glass,  full  of  water,  whose  diameter 


*********  *******  Mraqoimi  to  del  warn  hew 
mMtfsr  «tt  ran  over  ? 
iM  95*979  ensie  inches,  or  near  }*  parte  of  a  pint 
QeenY.  60.  Tbe  dbmW  of  a  sphere  and  com  baa* 
she  ohm  as  in  tbe  last  opeetion,  aadfctbe  cone  only  J  Mi 
voter;  reqpired  whet  pert  of  tbe  ant  of  the  sphere  .ie  m 
Banned  in  the  water  T  Ana.  -546 -parts  of  em  mk 

Quest.  51.  Tbe  cooe being  stiB  the  etaee,  and  ±  Me! 


water  ;  required  tbe  diameter  ofaaphere  which  ahall  be  jet 
eJI  covered  by  the  water  T  Ins.  2*443096  inches. 

Quest.  68.  If  a  person,  with  -aa  air  balloon,  ascend  ve> 
tteally  from  London,  to  each  height  that  ha  can  j« 
Oxford  appear  ia  the  horisoa ;  it  ie  leqoired  to  <  ~ 


bia  height  above  the  earth,  supposing  its  circumference 
be  96000  mile*,  aad  the  distance  between  London  and 
Ox*fd49*tttt3mi)s*T 

Ana.  yVVi  of*  milo,  or  647  yards  I  loot 
Quest.  58.  In  a  garriaon  there  are  three  remarkable  ob- 
jects, a,  b,  c,  the  distances  of  which  from  one  to  another 
are  known  to  be,  as  213,  ac  434,  and  ac  962  yards ;  I 
am  desirous  of  knowing  my  position  and  distance  at  a  place 
.  or  station  s,  from  whence  I  observed  the  angle  ass  18*  90', 
and  tbe  angle  can  20°  5C,  both  by  geometry  and  trigo- 
nometry. 

Answer. 

At      005-7122,  A  c 

na      429-0814,  "  " 

cs  5242805. 


Qubst.  54.  Required  the  same  as  in  tbe  last  question,, 
when  the  point  b  ia  on  the  other  aide  of  ac,  supposing  ab  9, 
ac  12,  and  nc  6  furlongs ;  also  the  angle  asb  38°  45',  and 
the  angle  bsc  22°  30\ 

Answer. 
as  1004, 
bs  1504, 
os  14-01. 


Quest.  55.  It  is  required  to  determine  the  magnitude  of 
a  cube  of  gold,  of  the  standard  fineness,  which  shall  bs 
equal  to  a  sum  of 900  millions  pounds  sterling  ;  supposing  a 
guinea  to  weigh  5  dwts  9$  grains.  Ans.  23*549  feet 

Quest.  56.  Tta  &\\&Yi  <A  *  fot^^ss&vi  1000  feet  long, 


MENSURATION. 


569 


9  feet  deep,  29  feet  broad  at  bottom;  and  22  at  top ;  how 
much  water  will  fill  the  ditch  ? 

Ans.  1158127  gallons  nearly. 
Quf.8t.  57.  If  the  diameter  of  the  earth  bo  793011)1168, 
and  that  of  the  moon  2160  miles :  required  the  ratio  of  their 
surfaces,  and  also  of  their  solidities  :  supposing  them  both  to 
be  globular,  as  they  are  very  nearly  ? 

Ans.  the  surfaces  are  as  13|  to  1  nearly ; 
and  the  solidities  as  49}  to  1  nearly. 

B 


Quest.  58.  Let  abc  be  the  profile,  or  perpendicular  sec- 
tion of  a  breast. work,  and  ep  that  of  a  ditch.  Now,  sup- 
pose the  area  of  the  section  abc  is  88  feet,  the  depth  of  the 
ditch  rd  6  feet,  er  =  so  =  3  feet ;  what  is  the  breadth  of 
the  ditch  at  top  when  the  sections  of  the  ditch  and  the 
breast- work  are  equal  ;  that  is,  when  the  earth  thrown  out  of 
the  ditch  is  sufficient  to  make  the  breast-work"? 


Vot.  I 


571 


LOGARITHMS 

or  THE 

NUMBERS 

/ 

FROM 

1  to  1000, 


-    — ' 

N. 

Log. 

N. 

Log. 

N. 

Log. 

N. 

Log. 

1 

0.000000 

26 

1-414973 

ai 

1-707570 

76 

1.880814 

2 

0*301030 

27 

1-431364 

52 

1-716003 

77 

1*886491 

3 

0-477121 

28 

1-447158 

53 

1-724276 

78 

1-892095 

4 

0*602060 

29 

1-462398 

54 

1-732394 

79 

1-897627 

.  5 

0-698970 

30 

1-477121 

55 

1-740363 

80 

1-903090 

6 

0-778151 

31 

1-491362 

56 

1-748188 

81 

1  >908485 

7 

0*845098 

32 

1-505150 

57 

1-755875 

82 

L913814 

8 

O'9O3O90 

33 

1-518514 

58 

1-7(33428 

83 

1-919078 

.  9 

0*954243 

34 

1-531479 

59 

1-770852 

84 

1-924279 

10 

roooooo 

35 

1-544068 

60 

1-778151 

85 

1-929419 

H 

1-041393 

36 

1-556303 

61 

1-785330 

86 

1-934498 

1* 

1*079181 

37 

1.568202 

62 

1-792392 

87 

1-939519 

13 

1*113943 

38 

1-579784 

63 

1-799341 

88 

1-944483 

14 

1*146128 

39 

1.591065 

64 

1-806180 

89 

1-949390 

15 

I* 176091 

40 

1.602060 

65 

1-812913 

90 

1*954243 

.  16 

1-20412C 

41 

1.612784 

66 

1-819544 

91 

1-959041 

17 

1-230449 

42 

1.623249 

67 

1-826075 

92 

1-963788 

18 

1-255273 

43 

1.633468 

68 

1-832509 

93 

1*968483 

19 

1-278754 

44 

1.643453 

69 

1-838849 

94 

1*973128 

20 

1-301030 

45 

1.653213 

70 

1-845098 

95 

1-977724 

21 

1-322219 

46 

1.662758 

71 

1.851258 

96 

1-982271 

22 

1-342425 

47. 

1.672098 

72 

1.857333 

97 

1-986772 

23 

1-361728 

48 

1.681241 

73 

1.863323 

98 

1-991226 

24 

1-380211 

49 

1.690196 

74 

1.869232 

99 

1-995635 

25 

1-397940 

50 

1- 698970 

75 

1*875961 

100 

2-00000Q 

tf.  B.  In  the  following  table,  in  the  last  nine  columns  of  each  page, 
where  the  first  or  leading  figures  change  from  9's  to  O's,  points  or  dots  . 
are  now  introduced  instead  of  the  O's  through  the  rest  of  the  line,  to 
catch  the  eye,  and  to  indicate  that  from  thence  the  corresponding 
natural  number  in  the  first  column  stands  in  the  next  lower  line,  and 
it*  annexed  fira£  two  figures  of  the  Logarithm  in  the  second  column, 


301  1566 

30*4*0007 


N 


500  4771*1  7266  74 1 1  7555  7700(7844  7983  8  1 33 


M  ,139 
49  1 562 1 1502, 1642 


1566  §7 1  I  8855  3999  9143  9287 
IOO07OI5I  029  4  043&  0582  0725 
1443  1586  1729  1872 
J874  3016  3159  3302 
43004442  45854727 
5863  6005  6147 


20162159 
3445  3587 
4869  50M 


7280  7431  7563  7704 
86928833  8974  " 


580 
1783 

276o]29Gg|3O40|3179 
415sU294|4433  4572 
5544  J€83  5S32j5960 
6930  7068  7206  7344 
831 J  [8448  85 S  6  8724 
9687  9824,9962]  .  .99 
317|50IGS9  1196.1333, 147t> 


Jt8 
319 

320 

322 
32 


2427 
3791 
5150 
6505 
7856 
9203 


328 

329 
330 
331 


333  521138 
3444 
3746 


333 
334 
335 
33$ 
337 
338 
339 
340 
34 
342 
343 
344 
345 
346' 
347 


5874 
7196  7328 


8S14 


9328  9959 


256412700:2837 
3927j4065|4l99 
52865421  5557 
5640  6776  6911 
79918126  8260  _ 
93379471  9606  9740 


324510545  0679  08130947 

325  1883  2017  2151  22B* 

326  32183351- 

327  4548  4681 
6006 


8646 


1269 
2575 


3484  3617 


4946 
6271 
7592 


2B3S  29663096 
876:4006141 36  4266  4396 
5045  5  174  5304  5  434  5563  5693 
6339  6469  659816727  6ft56  6985 
7630  775&I7888  8016  814&8274 
89 1  719045  9 1 74  9302  9  43t>,9  559 


6289  6430  6572  67  I  4  6855  6997 


3750 
5079 
6403 
7724 


8909  9040 
353 
1661 


943] 

0869 
330? 
3730 

5153  5*95 


79  ae 

9396 
801 
2201 
3597 
4969 

7759 
9137 
,511 


9677 
I  OS  i 
2481 

3876 
5367 
65  1  5,6653 
7697S035 


9275|94 1*9550 


,648 


1081 

24182551 
3883 
5211 
6535 
7855 
9171 
484 
1792 


530200 
1479 
2754 
4026 
5294 
6558 
1819 


0323O456IO584 
I607i  1734!  1862 
288213009  3136 
4153  4230:4407 
5421  5547,5674 
66S5]68llj6937 
794518071  8197 


0712 
1990 
3264 
4534 
5800 
7065 
■139 


0340 
2117 


6664  8799 
9-1*3 
349  1432 


3226  3356 
*&«6 
5822 
7114 
8402 
9687 


6932 
3251 


95669697 
,876  1007 
2183*314 
3*36  3616 
4656*765  4915 
5951  6081  6i  10 
72*3  7372  7501 
8531  8  6608 


5741 
7064 
8  3  S3 


785  922 

17441 1  SflojSOl  7|  2 1 54(229 
3 1 09  3246i5382  3  J I  shsSS 
447 1  4607147 4mg78  50/  4 
5826,5964  6099  6 « 34^6370 
73l6;745l|7586.772l 
169349068 
.277  .411 

1616  mo 

2951  3084 
4332<*415 
5609 


9815 
1096 


0968 

224512372 
3391  3518  3645 
4661  4787  4914 
5927  6053  6  1  80 


7189)7315 
0448  0574 


7441 
8699 


907  &ta*0M  %<n  awfe  vi  %i^aw*  m*>  J 


788 
9945  7 
122  5  1351 

3772  389? 
5041  5167 
6306  6432 
7567  7693 
8tf25  Fn 


OP  NUMBER*.  G7S 


IN. 

0 

1 

2 

3 

4 

5 

6 

7 

6 

9 

ji50 

176091 

6381 

6670 

6959 

7248 

7536 

7825 

8113 

8401 

8689 

151 

8977 

9264 

9552 

9839 

.126 

.413 

.699 

.986 

1272 

1558 

|l62 

181844 

2129 

2415 

2700 

2985 

3270 

3555 

3839 

4123 

4407 

153 

4691 

4975 

5259 

5542 

5825 

6108 

6391 

6674 

6956 

7239 

154 

7521 

7803 

8084 

8366 

8647 

8928 

9209 

9490 

9771 

.  .51 

155 

190332 

0612 

0892 

1171 

1451 

1730 

2010 

2289 

2567 

2846 

156 

3125 

3403 

3681 

3959 

4237 

4514 

4792 

5069 

5346 

5623 

157 

5899 

6176 

6453 

6729 

7005 

7281 

7556 

7832 

8107 

8382 

158 

8657 

8932 

9206 

9481 

9755 

..29 

.303 

.577 

.850 

1124 

159 

201397 

1670 

1943 

2216 

2488 

2761 

3053 

3305 

3577 

3848 

160 

4120 

4391 

4663 

4934 

5204 

5475 

5746 

6016 

6286 

6556 

f61 

6826 

7096 

7365 

7634 

7904 

8173 

8441 

8710 

8979 

9247 

162 

9515 

9783 

.  .51 

.319 

.586 

.853 

1121 

1388 

1654 

1921 

163 

212188 

2454 

2720 

2986 

3252 

3518 

3783 

4049 

4314 

4579 

164 

4844 

5109 

5373 

5628 

5902 

6166 

6430 

6694 

6957 

7221 

165 

7484 

7747 

8010 

8273 

8536 

8798 

9060 

9323 

9585 

9846 

166 

220108 

0S70 

0631 

0892 

1153 

1414 

1675 

1936 

2196 

2456 

167 

2716 

2976 

3236 

3496 

3755 

4015 

4274 

4533 

47*2 

5051 

168 

5309 

5568 

5826 

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11.418792':  8.744556.  9.999529:  8.745207 

11.415486.  8.746802;  9.9993-2-2!  8.747479 


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0,019235 
9.02043s 


L  mint  >  L  Tuiii 


9.997614  9,02  1 620r  1 0,  1*7  S3*u 

9,99 rm  |  9.022534,  i 0,977 i  66 ! 


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9.038048 


9,397547  9.02/6*5 


9,026455 


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9.02756? 
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sjorisoj  9.033009 

9,9974661  9.034791 


MUM 


Column. 


IV*. 


9.US5894, 

MSfpgs 


LOJ723U 


9,S9743»j  9  035969 


ia9fl99il 
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1 0,96  o  75 
10.966391 
10.9  G3  209 


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9.99742J  ao.iSiilfi  UKfjuit^i 
9,9974ltj  9.039485  <0.96G515 
9,097397  9,040551 
9,039197 1  9,997383  9,04 (3  1 3 
9,0tfU42  U  .9  97369  9.04-2973 


9.041485  9.997355  9,044130 


9.042625!  9-997341 
9,043763  9.9:/7327 


I  9.O40O36  9.997399 
9.047154  9,997235 


10.959340 
10.958187 

10.9570a; 

10.955870 
J  0*95471 6 


9  046434  10.953566 


9.044895  9.997313  9,0475*2  10.05-U i* 


9.049  860 


9,048277*  i,ijrg|  9-05 IGOS 
9. 049400]  9,997257  9.052144 


36  9.06O460  9,9971(2  9.063348  10.9366^ 


9.0505  k  9 
9,031635 
9,052749 
9.055859 

9,054966 
9,056071 
9.0J7172 
9,058271 
9.0553ft7 


9.06(551 

9.062659  9.1197083 
9.063724 
9.09  4806 
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9.997242 
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9.997214 
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9.9971  ■ 
9,997170 
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9.397141 
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9,053277 
9,054407 
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9.05778* 

9.0581*0" 


10,964031 
10.962*56 


10.951273 
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10.9489921 
10.947836 
10.946723 
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9,061130  ID  931^70 
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9.065556  10934444 
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9.997053  9.O67754  I0.934248 
9,997039  0  ,06  Hti46  10-9  3 1 1 5  4 
9,99702i!  9.0C9938  10.930062 


9.094047 
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9,097065 
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9,099065 
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9.103037 
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9,105992 
9,  L 00973 
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9,108*27 
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9,110873 
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9,113809 
9.1(4774 
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9.116656 
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9.99675  J 
9.9907551 
9.9967211 
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9.936688 
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9,093037  9.996641 


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9  090187  10,9098 
9.091228  '10.9017 72 
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10,902578 
10,90(554 


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9,100487  IU893SI3 


9.109559, 
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9.906384  9,11-2543 


9.121417 


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9,9963.35 
9,996318 
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9.996285: 
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9.130404  ia879596 


9.1 13533 

9.I14HI 
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9.116491 
9.U7472 
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9.12&I69  9.99ft  1 85 


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9.070176  99969791  9,07319710.9^6803 
9.071342  9,99696 1!  9.074278  10,925722 
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4a  9,073366  9,996934  9,076432  10,923563 

49  9,074^24  9.996919!  9  077505  10-922495  Q.U3551 

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51 1  9.076  53  ,J  9-996889  9.079644  j  0,0^0350  9.135387 

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9.079676  9J196843  9,082833||0,9J7l(V7  9.138128 

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9.123306  9.9961J4 
9,124248  9.9961 1 7 
9.125187[  9.9961 10 
9.126(25,  9.996083 
9,1 2706 SI  9,996066 

9,lJ7993l  9.996049 

9.128925,  fxmm* 

9,129854'  9,996015, 
9,13078 1  j  9.995998 

9.i3i706j  9,  lasna 

9. 1-J2630  9.905063 


9,126211 


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122348  10,877652 


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9.1'242S4|ii.J!ir5rifi 
9.1252  W  10,874751 


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9,1271 7sfi  10,87282* 


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9,1VJ087 
9,130041 
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9-131 944Jio«g|OS8| 


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9.135736]  10.8*4274  13 


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9.9959 16 
9.99592  8 
9.99591 1  9  139476 


9,995*7*1 


9.137603 
9.(38542 


9.995894  9,f404Q9  (0.839591 
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9,905850  9.lHJ_r,LJ  1 0,85^731  I 
9.995841 


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10,862395 
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9,441658;  9.9W33'  9  458025  10.541075 
y.-H-jiV.n;  9  ;*S-696  9,459400  10440600 
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1,9834771  9,4C^42  10. 53775 B  9.470046 


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9,93^^93 
9.933*17 
9  933141 
9.9.1.^66 


Hum, 


9.77734* 
9.7776*8 
9777915 
9778*01 
9778488 
9778774 


10^2658 
10***37* 
10!fi*i>85 
221799; 


9  721978  9.9*0286 
97**181  9.929*07 
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9  7*279 1.  9  9*8972 
9  7229L14!  9  9U8853 

9723197  9.9*8815 


10  910698: 
10.210415 
10.910132 
10*09849 


1  97876a* 
1  97  87 886 
;  9788170 
1  9788453 

9788736 

9789019 

9  789302 
9  789585 
9  7S9B6S 
9  790151 
9  790434 
9  790716 

9.790999 
9  7*11281 
9791563 
9  791846 
9,7921*9 
979*410 

9  79*60*  10  207308 
9  792974  (0,207006 
9  793*56!io206?44 
9  7035^8,10,20646* 
9  793819 j  |0  «06|81 
9  794101  10.205899 

979438*10  205617 
9  794664  10  205.I06 


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10.9090OI 
10.208719  16 
10.208437 
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10,20787* 
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9  7^4^46, 10905054 
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10 


9  72340i  l  9  9*8736 
9  72360.1  9  92865! 
9  723805  9-928578 


603 


LOG.  8IKKS,  TANGENTS,  &C. 


34  Ut-A- 


33  Peg. 


7 
8 
V 
IU 
II 
W 

IS 

u 

IS 
16 
17 
18 

IV 
41 

as 
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45 

46 

47 
48 
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11 

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43 

145 

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151 
54 
53 
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£ 
57 
58 
59 
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9.744414 
9  794614 
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9.745017 
9.745419 
9  745440 

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9.746044 
9.746445 


9.746446 1  9.9475481  9-798877  10.4OJ  143 


9.746636 

9.796827 
9.747-.J47 
9.747448 
9747448 
9.747648 
9.747848 

9.7*8027 

9.748447 

9.7484, 

9.748040 

9.748845 

9.749141 


Co»i  ie.  :    V*n-i     I  Co  fang 
9.928440:  9^97789 \\0.&ni\V 
9.948)44'  9.7MJ7ttl0.4(U.UO; 


10.41! 


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9.928183  9.79G6J4|l0.4a3368; 


9.948461  9.793151 


9.9481(4  9.79<i9l3  10  40308 

9.948025  9.7971  4  10.404836 

9.947946  9.7974741 10.40  4546 1 

9  927867'  9.797755  10.402445 

9.947787  9.7980.16  10.40196  i 

9.947708  9.798J  1 6  1 0.4U !  68  4 

9.947649  9  798596(0.40140) 


1 0.4008 13 
I0.40r>563 


9.947470'  9*799157 

9.947390  9  799437 

9.947.110  9.799717  10.40048! 

9.9  J 7431  9.799997 

9.947151  9.8(Kh>77 


4.947071 
9.946991 

9.94691  I 
9. 9  46  S3 1 
9*'.' 267 5 1 
9-946671 
9.946591 
9.94651 1 


9.800357 


S.iie.    ,  CJo^in-.. 

9  736109!  QShUtol 
9.716.KU|  9.94.1509 
9.736498'  9.9414  27 
9.7366D4j  9  941145 
9  736886;  9.941461 
9.737080|  9.943181 
9  7374741  9.941098 


9.814517 
9.813794 


9.tfl307ujl(M869W.5h 


9.811147 
9.813641 
9.813899 


11U87U3IO 
10I  874U6;S9 


10  186653157 
i(M86177i56 
IOI86l0li55 


9.814176  IU-I85844-54 


9.737467  9.'32.V)I  6i  9  814454  10.I85548,51 
9  737661  9.1)44913,  9  8 1 4748  IO.I8j47*!S« 
9  737855'  9.944851'  0.8 1500 ••10.184996,5 1 
9.718018  9.944768:  lJ.8i54*MU.I8i7*0;5U 
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9  7184141  9.944601)  9.815811  i  10.1841 69,48 

9.738647'  9.934540'  9.816107*,  10.183893,47 
9  71884o|  9  9444.48:  9.816184.10  181618,46 
9.739013:  9.9-44155.  9.816658  10.181.144  45 
9  739406!  9.944474'  9.816911!  10  1*3067  44 
9.73.1398:  9.9441 89  9.8174JJI  I0-I8479i  U 
9.71J59oj  9.924106  9.81 738*  1 0-1 84516  44 

9.739783j  9.924043  9.8 1 7759- » 0.1 84441  41 

lo.  j  9860 1  j  9.739  »75  994194"  9.8l &i!S '1O181905  40 
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9.804513]  10.197  iH7  j  9.74n744  9'94l6o7-  'JAW  115  IU.1  SO  865' 561 


IM.4O0OO3 
10.199743 
10.199443 


9.8008  i6lO.I99l64 

9.8011 16  10.198884 

9.8. 0396 


9.945949  9.S..»4l6iiI|0.195534,j  9  742080  9.941023  9  841057  '0.17894^4 9; 
9  94iS68  9.804745|  10.195455  ■  9.7444: 1  j  9.940959  9.841334  10  l?b6ob,*5| 


9  744 16  >'  9  94085 6  9  841 60G  I U. » 7819 4>  4"! 


9.749243  9.9464.51  9.804794- I0.I9740S  ;  9.740931.  9.921544  9.811410  10.180 WJ  55 
9.749444  9.946151  V;>3074||0.196948,.  9.741 145!  99*1441  9  813684  IO.I8OII6  J4: 
9.749641!  9.946470  9.8  ».»33l ; 1 0.1906 49  9  74l3iG  9.941357  981935J  IU.18uo4j  53| 
9  749840;  9  946190  9.8.1363./;  10.196370  9.741308'  9.9*41474  9  8 2*  1434  10.179766  34' 
9-730:)l8|  9.946110  9.803909!  10.U»6o9i  .  9.741699  9  94||90  9-84O50S  10.179494  51} 
9.730417  9.946049  9  Soil  87;  10.195815"  9  741889-  9.941  u»7  9.84078.>  !U.l794l7  30] 

9.730  U  5 

9.S3U6I8  -        ...  ...... 

9.730811  9.945788  9.8.i3023;lo.|9l9«"7  j  9  74416    9  940856  9  84 

9.7  31009;  9.945707  9.805304!  10.1946  »8  '  9.7  446 ?4  9.94  )774  9.84 1 880  10.1781 40! 46 

9.731406,  9.9456-46  9.803580  1O.I9444O:  9.742*44  9.94o688  9.^42154  I0.l77&4o|45! 

9.75l40il  9.945545  9.805859  10.194141  :  9.743033  9.94ofi0i  9  844449  10.177571  j44; 

9.73lC04i  9.92546..  9.So6|37  10-I93S63   9.743423  9  940540  9.84470!' LO.I77497.43I 

9  731799!  9.945384  9.806il5jlO.I93585-!  9.74.1413,  9.9404.16  9.844977  -10.1 77u43!44| 

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9.945 4  >4  9.80697 1 1  hi. 1 93049  !  9.74379 9.940468 

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9.945060  9.807547  10.194473  9.744171  9  940099  9  844074  10.175948  18; 

9  944979  9  So780j'ia  194195  9.74 1361  9.940015  9.844345  IO.l756Ss!l7! 
9-944897  9.8tisOS!ial91.H7  ■  9  744550,  9.919911.  9.8446 19  10.175381  :t6i 


9-734193 
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9.733569 
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j 4  9. 84345 1  1 0.1 76749  (41 
18  9  84*544  10.176476 131, 


9.944816  9.808361  ■10.191659  j  9  744739  9.91:'846  9.844893  I0.175IU7  l5| 

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9.944654  9.S0S9I6,1 10.191 084  '  «<.745117  9.919677  9  8454  >9  tO.174561 ,13; 

9.944574  9.8091 93 >| 0.1 90807  '  9.745306  9.919593  9.8457 13'  10,174487  W' 


9.73S96I'  9.944491  9.8(»9 471  |().l 90529 

9.7341 5 7i  9.9444o/  9.8()'.-74s  (O.I904S4 
9-734353 
9.7345-19 


9.711744 
9.734939 

9.735135 


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9.944348  9  8|oo45,  IO.IS9975  1 
9.944446  9  8 1 0302, 10.1 89698  . 
9.944 1 64  9"  8 1  ( )5  8» ».  1 0. 1 89441 M 
9.9440S3  9  810837  10.189143 


9  745494  9.91950S  9.S43986  10.174O14  H' 

9.745683  9  919445  9.846459,  i0.1 71741  ilO 

9.745871  9  91933;.:  9.846514, 10.1 75468)  9' 

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9.7-16448  9.919169  9.847078: 10. 1 74944>  7: 

9  746436  9.91 9o55  9.847351  I0.17ii649j  6, 


9.74662i  9.919(hKi  9.8^7624'  10.1 74!7C!  * 
9.746814  9.91S  M5  9.84." 897.  0.174105'  ** 


9.94 iOO I  9.81 1 1 34  10.1 8S86G 
9.73533- »;  9.9439 1 9  9.8 11 4 10  10. is S.VJi » 

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>7  lifir. 


LOO.  SINES.  TANGENTS,  <fec. 


607 


34  1^ 


35  lit*  * 


Sine. 
9.747584 
9  7*7740 
9.747-»36 
9  748143 
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9  74S497 
9.748683 

9.748870 
9.749O50 
9.749213 
9.749449 
9.749615 
9  749801 

13  9.749987 

14  9.750174 
9.750338 
9.750543 
9.750749 
9  750914 


15 
10 
17 
18 

19 
AO 
21 
« 

43 
44 


45 

27 
48 


0.751099 
9.751494 
9.751469 
9.7516U 
9.7518.19 
9.754043 

9.754408 
9.754394 
9.754576 
9.754760 
09  9.754944 
30  9.753148 


31 
34 
53 
34 
35 
36 

37 
38 
39 
40 
41 
44 

43 
44 
45 
46 
47 
48 

49 
50 
51 
54 
53 
54 

55 
56 
57 
58 
59 
60 


9.753314 
9.753495 
9.753679 
9.753864 
9.754046 
9.754449 

9.754414 
9.754595 
9-754778 
9*754960 
9-755143 
9-755346 

9.755508 
9.755690 
9.755874 
9.756054 
9.756436 
9756418 

9.756600 
9.756784 
9.75696.) 
9.757144 
9.757346 
9  757507 

9.757C88 
9.757869 
9.758050 
9  758430 
9  758411 
...  9.738591, 
/  Cosine.  I 


Kj>t*t  It*. 

9.918374 
9.91*489 
9.918404 
9.91  831 8 
9.91443) 
9.918147 
9  918064 

9.917976 
9.91*891 
9.91 780* 
9.917719 
9917634 
9.917548 

9.917466 
0.917376 
9.9I74JO 
9.917401 
9917118 
9  917034 

9.916946 
9.916859 
9.916773 
9.916687 
9  916600 
9.91651  i 

9.91644: 
9.916341 
9.916454 
9.016 167 
9.9160b) 
9-915934 

9.915907 
9.915840 
9.915733 
9.915646 
9.915559 
9-915474 

9.915385 
9.915497 
9.915410 
9.91514S 
9.915035 
9.914948 

9.914960 
9.91477. 
9.914685 
9.91459% 
9.914510 
9.914444 

9.914334 
9.914446 
9.914158 
9.9140701 
9.913984 
9.9l3894j 

9.913806! 
991371 8[ 
9-913630- 
9.91 3541 1 
9-9 1 34531 
A.91 33651 


Tany.  | 

9.848987 
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9.849534 
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9  830077 
9.810 I 19 


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