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) THE NEW YOR
PUBLIC LIBRARY
ASTOR, LENOX,
TILDEN FU NDATIONS)
arene it
: o> Ww ie? call et cell
e: CONTENTS. Soon? pment
eee i td
* 5 ee ee 1)
ak = Prose i feet ——
Sa i 2 j i ia ae
—? as Ve ing AP agi —
Abbreviations and Symbols ~ - - = - = # © * © = = xib |
pis allem spt gga ce we! won te ee nl
Ceres, Ephemeris of - - - - - tee em = 8180 320.
te Ocoee oe e+ Shale BBlto S88:
Ceigaraticts of the Satelltes ofan: « = 10) -2 -— ute eile
Day of the Year + = = ta we) ve Se “= + = = XXIL.
Eclipses of Jupiter's Satellites - - + ta ma? E
the Sun and Moon = - == eet ee oe
Mqnation of Time - = = = -s)0= += = (0) == <n ld oe
the Equinoctial Points. = - - - ----- = = +
Equimectial Time =< © 2) o- = or => +> + =m 5 =e ining
ENN in == <= <= —= <> a
a of the Articles; &e. - = -- == = som = i+
Festivals and Anniversaries - - -- - - - - - - - -
Fraction of the Year - - = = -+ = = © wm eos =
Georgian, Ephemeris of the * = <= 4 = = = © =
Juno, Ephemeris of - © - ©-=---9- --- <=--"°-
—+—_—_ for Opposition- + - ------- 5+
Jupiter, Ephemeris of - --- + -- = -=-- = + --
oes)
iv CONTENTS.
Moon's Node, Mean Longitude of, « - eee
Obliquity of the Ecliptic - - - --
Observatories, Longitude and Latitude of the Principal -
Occultations, of Stars by the Moon, visible at Greenwich -
Elements for computing
——— of Jupiter's Satellites by Jupiter - -
Pallas, Ephemerisof - - - - - -
———_——_——— for Opposition - - - -
Parallaxes of the Planets - - - - - - -
Phenomena - - - - - 7
Pole Star, Tables to find the Latitude by - 2 es
Stars, Mean Places of, for 1838 - - - - -
—— Apparent Places of, for 1838 - - - -
—— Constants, for Reduction of - - -
— Logarithms of A, B, C, D, for Reduction of
—— Formule, for Reduction of - - - - -
— Correction of, for2€ - - - - - =
Saturn, Ephemerisof - - - - - - + -
Ringof- - - - - - - - - -
Sidereal Time at Mean Noon - - - - - -
Semidiameters of the Planets - - - - - -
Sun, Ephemeris of the - - - - - - - -
—Eclipseesofthe - - - - - - = =
— Aberration ofthe - - - - - - - -
—Parallaxofthe - - - - - - - =
Terms, Law and University - ee eee
Tides- - - - - ae Ta is Ga cio
Time Equivalents, Tables of
‘Transits of Jupiter's Satellites and their Shadows -
University Terms - - ede Be SB eee
Venus, Ephemerisof - - - - - - - =
Phasesof - - - - - - - += =
Vesta, Ephemerisof - - - - - - - =
for Opposition - - -
Pages
- 266
- 266
490 to 494
452 to 454
455 to 467
- XXI
313 to 315
316 to 317
359 to 361
468 to 476
483 to 485
362 to 364
368 to 407
366 to 367
- XXII
- 365
408 to 409
335 to 346
- 476
-- It
359 to 361
Ito III
468 to 471
- 266
- 266
- xii
478 to 481
486 to 489
- XXI
279 to 290
- 477
303 to 305
306 to 307
PREFACE.
Tux Navtican Aumanac and AstroxomicaL Ermemunis for the year 1838 has
deen constructed upon the same plan as those of the preceding years, commencing
with the year 1834,
‘Tne Sun’s Longitude from the Mean Equinox, the Latitude, and the Earth’s Radius
Vector have been deduced from the New Tubles appended to Kffemeridi Astronomiche
di Mitano per U Anno 1833, (Milano, 1832), using a difference of Meridians =36" 45".
‘The Perturbations of Longitude and Radius Vector produced by each of the Planets,
Venus, Mars, Jupiter, and Saturn, have been computed accurately from the Tables for
every 10th day of the year; the Sums then interpolated with second differences for
every 5th day and thence the daily perturbations by simple proportion. The other
parts of the calculations have been performed independently for every Mean Noon.
The Latitude of the Sun, depending on the attractions of the Moon, was computed
for every day, and that depending upon each of the Planets, Venus and Jupiter, was
obtuined for each tenth day and interpolated.
‘The Nutations of the Obliquity of the Ecliptic (A) and of Longitude (4 L), have
been derived from MS, Tables constructed according to the following formule :
Aw= = 92500 cos R— 0/0903 cos 2 & + 0/-0900 cos2 p + 05447 cos2O
AL=—17'2985 sin B + 02082 sin 2 B—O'"2074 sin 2 Y — 1/2550 sin2O
where & is the Mean Longitude of the Moon's ascending Node, ) the true Longitude
of the Moon, and © the true Longitude of the Sun. (Ast. Soc: Cat., pages xiv and xv.)
‘The Mean Obliquity of the Ecliptic has been taken=23° 27' 37/43, on January 1,
1838, and the Mean Annual diminution=0'"457. (Brsset’s Tab. Reg. page 9.)
‘The Sun's Right Ascension and Declination were computed independently for
¢ Earth’s Mean Distance, has
from the Transits of Venus,
“Gotha, 1824. page 108.)
vi PREFACE.
where f denotes, for the 19th century, the number of years from the preceding bis-
sextile year, Assuming Meridian of Greenwich to be 9° 21"5 West of that of
Paris, and altering the epoch to the Mean Noon of January 1 of the year 1800 + f,
the Sun's Mean Longitude (M) for the meridian of Greenwich is hence found equal to
280° 53/ 32'"75 +4. 27605844 + @, 0” 0001221805 — f. 14’ 47083,
SSA rah peer ir day (n) of the year 1800-+4,
‘Sidereal Time = 2 4, "56555348 + Nutation in RA, =
‘The Longitude of the Moon from the Mean Equinox, the Latitude, Horizontal
‘Parallax and Semidiameter have been derived froth Bunemannr’s Tables de la Dune
(Paris, 1812), using 9 difference of Meridians = 9" 21": They have been computed
independently and in daplicate for every Mean Noon ani Midnight of the Years and
second differences have been taken into account wherever the irregular variation of
‘the Equations rendered such # correetion appreciable, ‘The Longitude being reduced
to the True Equinex, each set of results has then been differenced to the fourth
order, compared and carefully examined, Wherdter the progression of the fourth
differences indicated a probable error of 0/7 or more, the original computations
‘have been examined,
hi Anode diel SD afisk have, Hews odipyated for each noon and
midnight, examined by means of differences to the fourth order, and interpolated
for every hour.
The Places of Mercury, Venus, and Mars, from the Mean Equinox, have been
derived from Lixpewav's Tables*, ussuming Greenwich to be 42" 56° West of
Seeberg; and those of Jupiter, Saturn, and the Georgian, from Boutann’s new
‘Tables,t with » difference of meridians = 9" 21"5,
For Mercury, the Perturbations, were obtained immediately from the Tables, for
,fach-alternate day and interpolated with first differences: the remainder of the calcu-
lations were performed independently for eyery day.
‘ For Venus, the Heliocentric Longitude from the Mean Equinox, Latitude and
Radius Vector were computed independently for every cighth day, then interpolated
with fourth differences for each day, and the Longitude reduced to the True Equenox.
‘The Geocentric places were computed for every fourth day, and the intermediate
values obtained by interpolating with fourth differences.
® Investigatio nova Orbit a Merowrio circa Sotem descripte, accedunt Tabula Pianeter ex Elemeutia
recens repertis cl Thooria Gravitatiy Must. De Laplace construct, ddictore Brwxuanno Dx Lax
vexAv. Goth, 1815. ato.
Tabu: Ferevix move ef correcta ew Theoria Gravitetis clarinimi De Laplace ef «x Observationiter
recentixsimis in sprenia Avtrenonion Serbergeasi habitis erufe, Auctore Beaxnanno De Lixommau.
Guthw, 1810, do,
Tabufe Martis nove et correet# ex Theoria Gravitatis clarissint De Laplace ef ex —
recentissimis erute, duciere Buamnsnog De Liswnnavs Kisenberg, 1511. Ato.
© F Tables Artronomigues publites par be Bureau dea Longitudes de France, contenant let ‘Table te
Jupiter, de Saturng ef df Uranas, constraifes Le sh Thdorie we te bee Seg
Bouvasicn Parts, 1821. Ato, . ve;
PREFACE. vii |
For Mars, the Heliocentric Longitude from the Mean Equinox, Latitude and
Radius Vector were obtained independently for every twelfth day, and interpolated
with fourth differences for each day, previously to the application of Nutation. The -
Geocentric places were computed’ for every fourth day, and interpolated with fourth
differences,
For Jupiter, Sater, adit the Gagan, che Hfliocentrls Lone fers Bt Seon
Equinox, Latitude and Railius Vector were computed direetly from the Tables at
intervals of thirty days; and interpolated, for each day, with second differences, pre-
viously to the application of Nutation. The Geocentrie places were obtained inde-
pendently for every sixth day, and interpolated for every day, using differences to the
fourth order.
The whole of the calculations relating to the Minor Planets have, for the firet time,
been performed at the Navricar Acmawac Office.
Adopting as 2 basis the Elements of the Orbits given at pages vii and viii of the
Navricar Atmawac for 1837, the Heliocentric Longituies have been first computed
and the periods of the next Oppositions ascertained approximately. The only Oppo-
sitions in 1838 are those of Vesta and Juno. For cach of these Planets the Variations
of the Elements, caused by Venus, the Earth, Mars, Jupiter, and Saturn, have been
computed for intervals of ight, days, for the whole period between the Oppositions,
agreeably to the method described in Professor Ainy’s paper, “ On the Calculation
of the Perturbations. of the Small Planets and the Comets of short period. —
(Arrexprx to Navrican Ataranac, 1837, page 149).
For the Perturbations, the following masses of the disturbing Planets have been
maa RESior 4 “entvae Da thd taeaellcs We Mle Moved oP WiDlbaers
Yenus ong Sotar Tables, &c.—Phil. Trans., 1828, page $0).
Earth avi (Systime dw Monde, 5th Edition, page 209).
Mars san) Cys camARo, Cony soe one, 198), eae 18) ‘
Jupiter aay (Arnx, Mem, Ast, Soc. vol. vi. page 97). P|
Satu hz (Systéme du Monde, Sth Edition, page 209),
‘The following are the resulting Elements :-—
IT. Vesta.
Epoch, 1838, Dec. 29°0 Boxe Diss ot ee
o 4 4 \ Pes
Mean Longitude of (3 - - - ¢ = - - LO |
Longitude of the @- = - 250)
Lon Tie af Ascending Nols aes
Inelinntion of the Orbit - - # =
Angle of Excentricity |
Mean daily Sidereal Motion. ne
8 1838, Deo, 89, 1"
~
viii PREFACE.
‘Th. Juno.
Epoch, 1838, June 17°0 Mean Time at Greenwich.
- 23h 38 231
Mean Longitude of f-- -- € - - ee
Thagtnds of to Pecan @--- 54 17 as | ea es a
Longitude of Ascending Node » = = 170 54 53°6 jane 175
Inclination of the Orbit - - i --- 13 237%
Angle of Excentricity- - - @ --- 14 52 3970
Mean daily Sidereal Motion on - - - 81432547
& 1838, June 17, 16" 2" 55" Mcan ‘Time at Greenwich.
With these Elements and their Variations for twenty days preceding and following
the days of Opposition, the Ephemerides for Opposition were obtained.
The Approximate Ephemeris for the year, of each of the Planets, Vesta, Pallas, and
Ceres, was deduced from the Elements for 1837: for Juno the Elements for 1837 were
used only to the period of opposition, and the new Elements for the remainder of the
year.
The Semidiameters of the Planets, for the Mean Distance of the Earth from the
Sun, have been adopted es follow: e
Mercury, Eq, Sem. 3°23 (Lindenau’s Tables of Mercury, page’S8)
Venus, Eq. Sem. 8°25 (Delambre’s Astronomy, vol. ii. page 620)
Mars, Eq. Sem, 4°435 (Littrow’s Astronomy, vol. ii. page 389)
Jupiter, Eq. Sem. 99°704 (Mem. Ast, Soc., vol. iii. page 301)
Saturn, Eq. Sem, $1 °*106 (Ast. Nach. N° 189)
Georgian, Eq. Sem. 37°25 (Delambre’s Astronomy, vol. ii. page 620)
‘The Eclipses of Jupiter's Satellites have been computed, in*duplicate, from De-
LamBae’s Tables Ecliptiques des Satellites de Jupiter, d'aprés la Théorie de M, te
Marquis Dx va Prace et la folalité des Observations faites depuis 1662 jusqu’a
Van 1802 (Paris, 1817), using the corrected Epochs given in the Navricat Aumanac
for the Year 1832, and a difference of Meridians = 9™ 21".
For the Configurations and Occultations of the Satellites, as well as the Transits
of the Satellites and their Shadows over the disc of the Planct, Mr, Wootnovse’s
Tables in the Arerxpix to the Navrtcat, Atmanac for 1835 have been used,
The Mean Places of the 100 Principal Fixed Stars for Jan. 1, 1838, together with
the Anoual Variations, have been deriyed from the fundamental Catalogue for 1930,
contained in the Second Edilion of the Nauricar Ausanac for 1834, pages 362 to
367, by means of the Formule at page xiv of the Parace to that Volume.
The Logarithms of A, B,C, D, at page XXII. of each Month, have been com~
puted agreeably to the Formule at page 365, omitting only in the Values of C and I
the terms — 0°004 sin 2 and — 0’"090 cos2 €; and for the only Stars that can be
sensibly affected by the omission, viz. the five Polar Stars, a Table of
given at pages 408 and 409. J
The Table of Constants for facilitating the Reduction of Stars generally, Tt
PREFACE. ~ ix
been computed from Busse1’s Formule, given at page $65, using the A, B,C, D, con-
tained in this volume.
The apparent places of 95 of the principal Stars have been deduced from the Mean
Places for January 1, 1838, using the Variables A, B,C, D in the present volume with
new constants computed for the year 1840, instead of the constants in the Astrono-
mical Society's Catalogue for 1830. For the five Polar Stara the constants have
been computed for 1838 and 1839, aud interpolated. The corrections were computed _
independently for every tenth day, with the exception of those for « and } Unsa
Mrxonrts, which were interpolated, with second differences, from computations made
for every third day of the year. 2
A further correction of the right ascension for daily aberration is necessary, where
extreme accuracy is required, and may be computed as follows: Let @ denote the
latitude of the place, and 3 the declination of the Star, then the correction (in time) _
for the upper transit is,
+ 0°°0206 cos p sec 3
— 00206 cos sec 3
The Lists of Moon-Culminating Stars and Occultations have been selected from
‘Mr. Francis Baity’s Catalogue of Zodincal Stars. (London, 1827.) _
The Mean Places of the Stars for both Lists were taken in order of preference,
1, From the Catalogue of the 100 Stars in this Work. _ 2. From Mr. Posp's printed
Catalogue of 1112 Stars. 3. From the Astronomical Society’s Catalogue. The
reduction of the Mean to the Apparent Places hus been performed by means of the
Astronomical Society's Constants; the corrections for each star on the contiguous days
being obtained by different computers for the Moon-Culminuting List, and those for
the Occultations by duplicate computations,
The calculations of the Elements of Occultations, the Occultations visible at Green-
wich, and the Solar and Lunar Eclipses, have been made in duplicate, and in the
manner described by Mr, Wootnovuse in the Appendix to the Naurican Arsrasac
for 1836.
The Elements at page 476, for determining the appearance of Suturn’s Ring, have
been calculated by means of the formule: at page viii of the Naurican Aumawac for
1836, adopting Brssex’s later determinations of the values of 8, ¢ anda’, viz, :—
% = 166° 53’ 89 4 46462 (¢— 1800)
i= 28 10 44°7— 0 350 ((—1800) pan Nach, Nov274; 9016167:
a! = 39308 (Ast. Nach., No. 275, col. 170),
the mean distance of the Planet from the Sun being taken = 9°54301, agreeably to
Bovyann’s Tables of Saturn, instead of 95421889, the value used by Brssus in the
reduction of his observations,
and for the /ower transit,
ble TH, given at page 401 of the
well as Table XV at page 412,
as been entirely reconstructed, by
i
x "PREFACE.
adapting the equations for each month to their proper argument, apparent tim > id
[EU E o Daaepieet ot
by means of M. Lunnocx’s Tables, XVI. and XIX.
Ties kas ey a clo st rps ¥y SliAhS cD tar!
(@ Uniee Minoris), at any hour of the day, are similar to those published annually by”
= a—peosk + ¥sin 1" (psin h)* tana
where 4 denotes the latitude
_ @ —— the true altitude of the Star ,
P —— -the apparent polar distance, expressed in seconds of are
hk ~—— the hour angle of the Star=S —a; S being the sidereal time of
observation, and « the right ascension of the Star. .
Table I contains the value at sg Saacarel sapmanKneon A) ot, the frat erect y
assuming, as mean values, p =93' 6”, and «= 15° 27’.
Table contains the value of the third term (4 sin 1” (p sin h)* tan a) or the
second correction, using the same mean quantities as in Table I. :
‘Table I, which is speciad for the year 1838, and depends upon the diffe
between the trac and assumed values of p and @, contains the (hired correetic
increased by 1’ for the purpose of rendering the quantities additive. “ta
A fourth term (— }sin‘1” (pcosA) (psinh)*) is omitted, its greatest value being”
only 0”°55. pert
_ Tn the construction of this Ephemeris generally, duplicate computations have be
made where necessary, and independent calculations performed to guard agai
errors in principle, and all results finally examined by means of differences.
W. S. STRATFORD, Lied Hey
Nautical Alwanae Somerset Houre, ‘Superintendent of the Nautical
ae re a
ae
Ss mal
Le eae
FIXED ano MOVEABLE FESTIVALS, ANNIVERSARIES,|
$e, Se. |
Epiphany - - ©: = - - Jan. 6'|{ Restoration of K. Charles TI) Miy 29 |
Martyrdom of KR, Charles I,- - - 30 |) Pentecost—Whit Sunday + June 3
| - = Feb, 11 | Trinity Sunday - - - =) - 9-10
Corpus Christi - -~ - + -)- M4
St. John Bapt—Midsm' Day - - 24
Birth of K.W.IV."- - = -~ ~/@1
Coronation of K.W.IV. - Sept, &
St. Michael—Michaelmas Day - - 29
Gunpowder Plot- - - - Noy, 5
St. Andrew
Ist Sunday in Advent
EXPLANATION OF
ASTRONOMICAL SYMBOLS AND ABBREVIATIONS.
© The Sun. |
€ The Moon,
% Mercury.
9 Venus.
Gord The Earth.
Conjunction, . 9 Aries. ~
Quadrature.
Opposition,
Ascending Node.
Descending Node.
North.
South,
Degrees.
Minutes of Are,
Seconds of Arc.
Hours.
Minutes of Time.
Seconds of Time.
~ceoMB@AeSnwaoa
LAW TERMS, 1838,
cap. 70, s. 6. (Passed July 23, 1830.)
prevecries by tahstel EWALD YY ie 3, 5.2, (Passed Dec. 23, 1830.)
Hinary Team - - - - Begins Jan. 11 Ends Jan, 31
- - May 10
- - June l4
~ Noy. 26
Begian. | Ends. Begins.
Jan. 15 | April 7 | Jan. 13
April 25 | June 2] April 25
dune 6| July 7] - - -
Oct. 10 | Dec. 17 | Oct, 10 Nov. 12, Midnight, | Dec, T
The Act, July 3. The Commencement, July 3.
EPHEMERIS
FOR THE YEAR
1838,
. FOR THE MERIDIAN
Or THE
ROYAL OBSERVATORY AT GREENWICH.
ey FEF EFS fer FRE SPF
JANUARY, 1838.
AT APPARENT NOON.
Sidereal | Rquation of
4 E THE SUN'S Time | Time,
= of the ole
a 2 2 A aa aided to
= peeerisg We Daten the | Apparent
a lel 5 hee 1 tour, [Meridiaa*] Times
” mes nm
1 is 46 36-78 139 s. 23 1 48" ioe | L 10°99] 3 50
2) 18 51 6} 1023} 22 56 9 *5] 1-03 | L 1094] 4 1884
3] 18 55 26°22) 1-006] 22 51 15-16 |1 10°89) 4 46°77
4] 18 59 50°37] tovgas | 22 44 590) 16-28 [1 10°S4) 5 14-29
5}19 4 14°08} 10-969 38 28s] azear | E 10°78] 5 41°37
6119 8 37°34] 1o-949] 22 31 30°5| 1852 | 1 10°72] 6 7°99
Z]19 13 Or12] 10%927] 22 24 GO} 19°62 | 1 10°66] 6 34-14
8]19 17 22°37] 1o-g05 | 22 16 15 °2) 20-71 | 1 10°59] 6 59%
9]}19 21 44°09] 1o-ass | 22 7 B83) 21-79 | 1 10°52] 7 24
10]19 26 5°25| 10-57} 21 59 15 "4) coene | 1O"44] 7 49
11] 19 30 25°83] jo-sa9 | 21 56 6°9) os-g: [1 10°36] 8 13°33
12/19 34 45°82] 107807 21 40 33-0) ga-ga | 1 10-28] 8 36°70
19.39 5°19] 1o7e1] 21 30 33
19 43 23°93] 10-753 | 21 20 10%
19 47 42-01] 10-726] 21 9 21-4) osroa [I 10°01] 9 43°03
———
une
16]19 51 59°S4| 10-097] 20 58 8°5) e9-0¢ |1 992110 3°85
17]19 56 16°18] 1070] 20 46 31° ‘ ‘
Thur} 18/20 0 32°23] 10%s9] 20 34 310] ator | 1 9°73] 10 4343
Frid.|19]20 4 47°58] 10¢10] 20 22 6-9
] Sat. |20]20 9 2°20) 10-580] 20 9 1977
Sun.|21/20 13 16°09] yos4s] 19 56 9
Mon.|22}20 17 29°22] 10515] 19 42 37°) aae7a [I 9°31] 11 54°00
S| 23}20 21 41°60] 1oss9] 19 28 43-4) a5-64 | 1 9°20)12 9°76
} Wed.) 24)20 25 5319] 10-449] 19 14 27°) 96-56 | 1 Qr0g]12 24
j Tes Thur. 25720 30 3-98) 10416 18 59 50°5| 71 [1 898/12 S8*O4
‘ag .|26}20 34 1396] to-sso] 18 44 52°) aa 26 8°R7] 12 52°32
Sat, |27}20 38 23°12] 10-007] 18 29 $473) sg-10 [1 8°76] 13 4789
} Sun. }28}20 42 31°45| 10-13] 18 13 55°9} 29-92 | 1 8°65] 13 16°64
| Mon.| a 20 46 38°95 | 10-278 17 57 57°9| 4o-72 | 1 8°54] 13 27°56
Tues, 30/20 50 45°61) 10-243] 17 41 407) ates |} 842) 13 3)
} We] 31/20 54 51°44/ 10-207] 17 25 4°6) ae-27 | 8°31] 13 4
| Thur.|32/20 58 56+41 S.17 8 10°11
2 Tn i Seite ig Ye fous by smibtracting 09 from the S
Day of the Month.
Cen Ave wee
JANUARY, 1838.
bh mes
18 46 3602
18 51 0°87
18 55 25°35
18 59 49 41
19 17 21710 |
19 21 42°75
19 34 44°27
19 39 3°58
19 43 22 25
19 47 40°27
19 51 57 64
19 56 14°33
20 0 30°33
20 4 45°63
20 9 020
20 13 1404
20 17 27°14
7
‘1
9
BSS
soe
aoe
ass
19 28 50°5
19 14 3570
Ce See SAD One Hew, |
22 82s
a6
S82 sk S25.
=)
ee 833 dfs 23
=e
© ean ZEa,
4 JANUARY, 1838,
| MEAN TIME. 3
9°9926613
99926663
99926706
9 9926771
99926862
9 9926978
99927122
9 “9927292
99927492
99927720
9 "9927976
9 ‘9928259
99928570
99928908
99929271
99929658
99930067
57 55°8
37 21°8
56 4971
56 184
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JANUARY, 1838.
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7 56 44°89 | 25 46 51-0] 63-25 | 19
7 58 57°00 | 25 40 27-9) 65-07 | 20
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CONFIGURATIONS OF THE SATELLITES OF
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‘This Table represents, at 145 after Mean Noon of each day of the month, the relative po
the images of Jupiter and his Satellites, as they would appear (disregarding their latitude
inverting telescope. Jupiter ix indicated by the white circles (O) in the centre of the p
Satellites by points. The numerals 1, 2, 3, and 4, annexed to the points, serve to di
‘the Satellites from each other ; and theit positions are such as to indicate the directions of }
lites’ motions, which are in all cases to be considered ax /owards the numeral, When a S
at its greatest elongation, the point is placed above or below the centre of the numeral,
cirele (O) at the Jeft or right hand of the denotes that the Satellite placed by the six
took disc of Jupiter, and @ black cirele te) that it is either dehind the disc, or in the at
j} Jupiter.
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APPROXIMATE SIDEREAL TIMES
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OCCULTATIONS OF JUPITER’S SATELLITES BY JUP
AND OF THR ~
TRANSITS OF THE SATELLITES AND THEIR SHADOWS
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MEAN TIME. ,
THE MOON’S RIGHT ASCENSION AND DECLINATION. —
Hows| Right Asceasion Declination, [Bz-Be tiow.| Right Ascension| Deetination.
THURSDAY 1, SATURDAY 3.
hom s 2 ” w hom os ora
0} 225 8°19 IN.16 35 25°6) isa-72] 0 | 4 12 7°10 IN.25 7 42°) 7
1] 22717°64| 16 4847-9) 192-72) 1] 4 14 25-18] 25 15 13°°9) 7
2/229 27°64] 17 2 472)/191-70| 2) 4 16 43°31 | 25 22 36-6) 72)
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} 3 | 2 31 37°60 | 17:15 14°4) 3907] 3 | 4 19 1°64) 25 29 51 “1) Jor
4} 283.47°72| 17 28 18°4) 129-9] 4 | 4 21 20°12] 25 36 57 °0| 63:
5|235.57°99| 17 41 16°83) 128-60] 5 | 4 23 38°75 | 25 43 544) 6s)
6/2388 843] 1754 7°9\ 12753} 6] 4 25 57°52 | 25 50 43-2) 66
7| 240 19°03 | 18 6 53*1)126-43| 7 | 428 1642 | 25 57 23-4 68)
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g| 2 44 40°73 | 18 32 44]12093] 9 | 4 32 54°65 | 26 10 17-7] 62
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12| 251 14°55] 19 9 2°5| 121-02] 12 | 4 39 52-94 | 26 28 3378
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14} 255 37°97] 19.33 7°9\119-77| 14 | 444 32-41 | 26 40 075) bo
15 | 2 57-49°94 | 1945 075) 117-02] 15 | 4 46 52°30 | 26 45 30-6) 53)
16}3 0 2710] 19 56 4672) 116-43] 16 | 4 49 12°31 | 26 50 51°8
17} 3 214743] 20 8 25°1/ 115-30) 17 | 451 32°41 | 2656 4°21) 50
18] 3 4 26°94] 20 19 56°9| 114710] 18 | 453 52°61 | 27 1 7°5) a9)
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21/3 LL 5'57| 20 53 502] 110-Ss] 21] 5 0 53°76] 27 15 2470) 4
22/3 13 18°82 | 21 4.537] 109-38] 28) 5 3 1430] 27 19 51S
23.13 15 32°25 IN.21 15 50°0| 10817] 2315 5 34°92 IN.27 24 1070] 6
FRIDAY 2. SUNDAY 4.
0 | 3 17 45°86 IN.21 26 89 °D) 106-95] 0) 5 7 55°61 |N.27 28 19 *S) do
1} 3.19 59°66 | 21 37 20°7| 105-72] 1] 5 10 16°36| 27 32 19°9) a3
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13 | 3 46.59°66 | 23.35 50°3| 9023] 13 | 5 38 28"40 | 28 8% 35°7] a0
14 | 349 15 ‘84 | 23 44 52°0) 29-97] 14 | 5 40 49°50 | 28 10 87°7| a8
15 | 3 51 32-20] 23 53 45-8] 87-62] 15 | 5 43 10-58 | 28 12 305) 4
16 | 3 53 48°73 | 24 2 31°S| 86-27] 16 | 5 45 31°65 | 28 14 14°R) a5
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_ ERDBUABS: 1838.
MEAN TIME.
THE MOON'S RIGHT ASCENSION AND DECLINATION.
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URSDAY 8.
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WEDNE:
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FRIDAY 16.
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FEBRUARY, 1838.
SENURUAN Bs
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15 29 1s ‘4 s.22. 31
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19 44 23°19] 26 28 11°3) 70-50 2148 4-41) 17 31 34°68) 148-53
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173-72 | 18 | 2 86 29°55
173-29 | 14 | 2 38 44°56
172-70 | 15 | 2 40 59°73
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17i70s | 18 | 2 47 46°15
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: FEBRUARY, 1838. 3:
PHASES OF THE MOON.
) First Quarter ----------- 1 5 34°0
© FullMoon ------------ 9 1583
( Last Quarter ----------- 17 5 39°3
@ New Moon ------------ 24 0 8°0
ab ee
€ Apogee---------------- 10°19
© Perigee---------------- 241
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88 40 24|2866] 90 13 262883] 91
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MEAN TIME.
LUNAR DISTANCES.
33 Stare N BL » ee . |Pe
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| Spica my W.] $4 3 38/2741] 35 39 23)2725 af 15 30) 2710
a Aquile E. | 69 13 39)3727] 67 57 21/3734 41 10) 3748
| | Suw E. | 92 46 21/s104] 91 18 16) 3086] 89 49 49] s069] 88 21
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Satum W.] 11 54 18 sia1] 13 21 50/3002] 14 52 0} 2905
Sun E. | 80 51 33/2960) 79 20 30)29«1] 77 49 3) 2921
} 19| Supiter -W.] 96 32 29)2122| 98 15 32]2103] 99 59 2 2085
Spica m W.| 60 21 28)2462] 62 3 30/2433] 63 46 4| 2424
| |Saturn W.] 24 25 12/2995] 26 4 17/2360] 27 a4 7} 2530
| Antares W.| 14 27 22/2462] 16 9 20/2402] 17 52 4) e424
| Sun E. | 68 31 37)2802] 66 57 12)2783] 65 22 22) 2763
20| Jupiter W.]110 29 24)227a]112 16 2) 2256}114 3 6) 2237
} «| Spica my = -W.| 74 10 49 2218] 75 56 30| 2294] 77 42 38| 2276
| W.| 37 56 46/2976) 39 40 55/2353] 41 25 37/2092
| Antares W,] 28 16 54/2511] 30 2 37/2293] 31 48 47/2275
)} | Sox E.] 55 44 4/2643] Sa 6 8) 2624) 52 27 46) 2606
| 21 Spica ny W.] 88 28 38|2179] 90-17 462153 92 7 19|20
| Saturn = W.| 52 4 21/2214) 53 52 28)2197] 55 41 0/2179
Antares W.] 42 34 54/2172] 44 24 4/2156] 46 13 38] 2140
| Sun E. | 42 28 44/2499] 40 47 29) 2483] 89 5 52/2467
22|Saturn W.| 66 40 50\2090] 68 32 5)2077] 70 23 39] 2065
| Antares W.] 57 18 57/2057] 59 11 3)2045] 61 3 27/2034
25 | « Arictis E.| 46 7 32\2063] 44 15 36)2076] 42 24 0/2090
} | Aldebaran E. | 76 44 21) 2000] 74 51 55/2003) 72 59 43) 2061
| 26 | Sun W.| 28 14 22/2980] 29 58 23/2991] 31 42 10] 2409
| a Arietis HE. | 31 23 50 2222] 29 35 55\2255] 27 48 49| 2292
| Ald E. | 61 52 3)2ize] 60 1 55/2149] 58 12 13/2165
} «=| Pollux EE. J105- 14 21) 2053/1038 22 10 2066]101 30 18/2079
27| Sux -W,| 41 58 27/2488] 43 39 57)2505| 45 21 sl 20er
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Pollux E. | 90 26 28}2166] 88 37 9/2182] $6 48 14/2198
28 | Sun W. | 55 19 21/2620) 56 57 35] 2649] 58 35 24/2668
Aldebaran E. | 33 30 22) 2523] 31 49 41/2565] 30 9 58) 2610
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| CONFIGURATIONS OF THE SATELLITES OF JUPITER,
At is*, Mraw Tore,
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CONFIGURATIONS OF THE SATELLITES 0
At Li, Meaw Time,
at 11” after
at its greatest elongation, the point is placed above or below the centre of the nu
cirelo (O) ak the left or right hand of the page, denotes that the Satellite placed by
| eee: Girclo (@) that it is cithor behind the dise, oF
Busaa,
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——
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SSP SeSoSGoSESS5845,
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=-
210 69
18 13 24°5
731 1%
20 49 43°1
10 7 26°5
23 26 16°0
1244 0°7
2 2 55°2
15 20 47-3
6 18 42-4
10 16 566
14 14 43-2
18 12 23-9
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5 14 49°8
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18 33 16-2
APPROXIMATE SIDEREAL TIMES
OCCULTATIONS OF JUPITER'S SATELLITES BY
AND oF THR
TRANSITS OF THE SATELLITES AND THEIR SHADOWS
OVER THE DISC OF THE PLANET.
10 17
19 2 37 |inthe Shadow] 27% 8
—1 2470
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—1 2542
12563
1 2582
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T APPARENT NOON.
Sidereal tic
| 4 THE SUN’S Tine | tee
= ofthe fo be
| 2|3 Senitiam.| Stded te
1 sls pie. pig | Posing | moe rho)
RightAscension| for | Declination. for the | Apparent,
ale 1 hour, {nee Meridian.) Times
h * os @ ” moe ne \
} Sun. | 1] 0 41 37°69 4-28 -59°S] o7-77 [1 aMS} a AG |
| Mon.) 2] 0 45 15 97 452 6°0| s7-sa ]1 444) 3 43 2a
}) Tues.) 3] 0 48 54-36 515 770| 57-31 |t 446) 3 25-12
| Wed.) 4] 0 52 92°87 | 9-11 | 5 38 2°5) sp-06 ]1 449]3 712
Thur 5] 0 56 11°53 | g-118 6 0 518) 56-79 4°51] 2 49°
Frid.| 6] 0 59 50°35 | 9126 6 23 3479) 5652 454] 2 31
Sat. | 7] 1 3 29°36 | 9139] 6 46 11°3) 56-20 4°37 2 14-10
Sun.| 8]1 7 8°58 | 9149] J 8 40°8| 55792 4°60] 1 56-82
Mou} 9] 1 10 4802 | guse 7 31 2°9) 5561 464] 1 39°76
Tues) 10] 2 14 27°72 | 9166] 7 58 17°75) 55-28 4-68] 1 22-95
|) Wed.|t1] 1 18 7°70 | 9-178 8 15 24°2) 54-93 4°'72)1 6-42
Thur) 12] 1 21 47°97 | 9191 8 37 22°) S459 4°76] 0 50°18
| Frid.|13] 1 25 28°54 | 9-205] 8 59 12-7] sa22 ]1 a-s1] 0 34-25
Sat. |14] 1 29 946 | 9-220 9 20 53°9| Saas ]1 4°85] 0 18 °66—
Sun.|15] 1 32 50°74 | 9-235 9 42 26°0| sa44 11 4°90) 0 San
Mon.|16] 1.36 32°38 | 9-251] 10 3 4876) 53°03 ]1 4°96] 0 11-47 |
‘Tues 17] 1 40 1440 | 9-268 10 25 1°3) S261 Jl 501 cmaeey o*
Wed.) 18] 1 43 56°82 | 9-288] 1046 4°0| t248]1 507] 0 40 o
Thur) 19} 147 39°65 | 9302] 11 6 5672] s172]1 5°13 0 53°75 | o:
Frid. 20] 1 51 22°90 | g:so1 | 11 27 37°] 8128 ]1 S-19]1 Jos | o
Sat }21]1 55 6:59 | oxo | 1148 7-7) 50-77 1 5°25] 119-85
ma |
| Su. 22] 1 58 50-72 | gras | 12 8 263] sores |) 5131) 1 32728 | gs
jj Mon.}23] 2 2 35°31 | 9377] 12 28 33°0) 49°77 |] 1 5°38] 1 44°16 | om
} Tucs| 24] 2 6 20°36 | 9-397 | 12 48 27-4) 49°25 |1 5-45] 1 55-62 | o
| Wed. 2s 210 5789] 9419] 13 8 g°3| ae-71 [1 5752] 2 G63 | gs
Thur] 26] 2 13 51°92 | 9438 | 13 27 38°3| #818 |1 5°59] 2 1712 | oF
bes 27] 217 38°43 | g-4se | 13 46 54°0| 4752 1 5°66] 2 27-15 ”
Sat. |28] 2 21 25443 | 9479] 14 5 56-0| 470011 5°73] 2 3668 | oF
Sun. /29) 2 25 12-92 | gsor | 14 24 440) 4641] 5°81] 2 4572 | o
} Mon.|30] 2 29 0°93 | g-s22 | 14 43 17°8| 45-79 ]1 5°88] 2 54-25 | @
Tues| $1] 2 32 49 45 N15 1369 1 596)% 2-27 |
| * Mean ‘Time of the Semidiameter passing may be found by subtracting 0*'18 from the Siderew
APRIL, 1838.
"
N.0 20
0-22
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0°17
orld
0°01
$.0*10
O22
0°35
048
060
0-70
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0-78
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087
088
0°85
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0°70
0°59
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0-33
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5.005
0 07
org
026
032
034
O34
0°31
0 0001559
© 0002780
© 0004002
0 0005226
6 0006450
0 0007677
6 0008906
0 "0010136
6 0011370
0 0012605
0 0013841
0 0015077
0 0016313
0 0017547
0 0018777
0 G020001
0 0021219
0 0022426
0 "0023623
0 "0024809
0 0025983
0 0027142
0 "0025268
0 029420
0 -0030536
0 0031638
0 0032724
0 0033796
0 0034855
0 0035902
16 161
16 24'0
16 291
16 304
16274
16 203
16 97
15 56%
15 422
15279
15148
15 3%
Msg
PPP ore oF
1 40 29°0 |12°6] 10 381
6 2°5]13 6] 11 1
7
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7 27 17"
7°13 IN.27 22 41°5
MONDAY 2.
23°53 [N.27 17 5
39°61
=
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GAs bsnidas
ve
gdederusses
2
2
3
3
3
3
3
4
4
46
48
51
53
5
5
woeen Sh
h
6
6
6
6
6
6
6
6
6
6
6
6
6
7
7
7
7
7
i
7
7
7
7
7
7
i
7
7
7
7
7
7
7
7
i
7
7
7
i
7
8
8
8
8
8
8
8
8
8
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=
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geees
SESSSESSESSSESReEee
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USHKGUIASNHORALSHSBALHOERAENS
MEAN TIME.
THE MOON’S RIGHT ASCENSION AND DECLINATION.
ho om
22 26°78
24 1219
25 57°53
27 42°81
29 28°03
31 13°19
32 58°31
34 43°37
15 13 184 36 28 40
18 ck O: 38 13°38
14 48 38 6| 124° 39 58°34
14 36 13 °8| 124" 41 43°26
17 54°51) 14 23 45 °7) 125" 43 28°15
19 44°92] 14 11 14-4] 120° 45 13-02
21 35°13] 13 58 40°0 46 57°87
23 25°13] 1346 2:5 48 42°71
25 14'94] 13 33 21-9 50 27 ‘54
27 4°55] 13 20 38-4) 127% 52 12°36
28 53°97] 13 7 5178
30 43°20] 1255 2-4
32 32°25] 12 42 101
34. 21°13] 12 29 150
36 9°82] 12 16 17°71
37 58'35|N.12 3 166
FRIDAY 6.
39 46°70|N.11 50 133
41 34°89] 1137 7-4
43 22/92) 11 23 58°9
45 10°79] 11 10 47°9
46 58°51| 10 57 344
4846705) 10 44 18
50 33°50
52 20°78
54 7°93
55 54-94
57 41°82
59 28°58
115-21
3 1°73
4 48°13
6 34°43
8 20°62
10 6°71
11 52°69
13. 38°59
15 24°39
17 10°11
18 55°74
20 41°30
11 22 26°78 |N,
rs
SSSR SS aoGLSEEte
CRUSH eee Robe SGEeUnd
eSSHddd dK de Gsad
ee eo
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eEBGSTSS 2 eR Sl uSkS-as
-
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a
~
“4
1
“4
4
4
7 21 5735
0 23 42°77
3 25 28°25
4 27 13°81
“rl 12 28 59°45
8 12 30 4518
1 12 32 31-00
“4 12 34 1690
9 12 36 2°91
6 12 37 4901
5 12 39 35-22
ay 12 41 21°54
Gd
0
SaStisttssReeosee
SSSSSSCERLELLEE OS
Mei GG eS OE SGE DES dE ES
| BSSUESSeaSESSESS a
$e
—— — .
THE MOON'S RIGHT ASCENSION AND DECLINATIO
bhomios
14 15 43°63
14.17 41-22
14 19 89°07
14 21 37 25
14 23 35°74
14 25 34°57
14 27 33°72
14 29 33°20
14 31 33-02
14 33 33°17
14 35 33 66
14 87 34°50
14 39 85°69
14 41 37 22
14 43 39°11
14 45 41°35
14 47 43:95
14 49 46°91
14 SI 50°23
4
M4
ty
15 0 7°17] 2015 2)
28 1753/8. 10 2 15 2 12°34/8.20 26 &
TUESDAY 10. . THURSDAF 12,
30 8 '34/S.10 35 15
41 59°38 15
33 50 64 15
35 42°14
37 83°87
39 25°83
4L 18°05
43 10°51
45 322
46 56°18
~
0
1
2
8
a
5
6
7
8
9
10
i
1s
13
it
Ea
16
17
18
19
20
21
22
23
-_ -
wen
12 43°83
14 51°27
16 59°10
19 7°32
21 15°92
23 24°91
25 34°29
27 44°07
29 54°23
EnfS8
SdeGESuK
Cen anveewneos
=
soos
15 40 50°96
15 43 3-49
15 45 16°41
15 47 29°73
15 49 43-44
15 51 57°54
15 54 12°03
15 56 26°92/S
SRESESSSEses
Seaek
Li]
Cen Ks sews
wb
WONF UU WYVV PWR OC tone cwHs
FRIDAY 13.
homes 9. vi
15 56 26-92|S.24 80 2%
16 58 42°20) 24 38 23°0
16 0 57°87) 24 46 3671
16 3 13°94! 24 54 42°0
16 5 80°39) 25 2 40°3
16 7 47°23| 25 10 81°28
1610 445) 25 18 14°6
16 12 22°06) 25 25 50°3
16 14 40°05| 25 33 1872
16 16 58°41] 25 40 384
16 19 17°16) 25 47 507
16 2 86°28| 25 54 55°0
16 23 55°78| 26 1513
16 26 15°65| 26 8 39°5
16 28 85°39) 26 15 19°5
16 30 5649] 26 21 5173
16 33.1746) 2628 149
16 85 38°79] 26 84 29°8
16 38 0°47) 26 40 36°3
16 40 22°51) 26 46 34°3
16 42 44°90) 26 52 23°97
16 45 762) 2658 444
16 47: 30°70| 27 3 36%
16 49 54°11'5.27 8 59'S
SATURDAY 14.
16 52 17'°85/8.27 14 137
16 54.4192) 27 19 189
16 57 6°32) 27 24 15%
16 59 31°03} 2729 23
17 16606) 27 33 40-2
17 42140) 27 38 89
17 6 4774) 27 42 28:3)
17 9 12°98) 27 46 334
17 11 39°22] 27 50 8970
17 14 5°74] 27 54 3072
17 16 82°55] 27 58 11°8
17 18 59°63) 28 1 43°83
17 21 26°99| 28 5 6-2
17 23 54°61] 28 8 189
17 26 22449) 28 11 218
17 28 50°63] 28 14 149
17 31-19-01) 28 16 5871
17 33 4763) 28 19 314
17 86 1648] 28 21 54°8
17 88 45°56] 2824 871
17 41 14°86) 28 26 114
17 43. 44'37| 28 28 4%
17 46 1408] 28 29 47-6
17 48 44-00) 28 31 20°5
17 51 14710/S.28 32 437)
MEAN TIME.
THE MOON'S RIGHT ASCENSION AND DECLINATION.
aso} 0
eous | 1
sors | 2
79°72 8
jas 4
m3] S
m5 | 6
74°65 7
may] 8
jes | 9
jory2 | LO
6grsa | LI
63-03 | 12
66-67 | 13
65-30 | lt
bao | 1S
base | 16
6.08 | 17
59°67 | 18
sarza | 19
56-78 | 20
65-33 | 21
6378s | 22
bas7 | 23
50°37 0
4g-s8 | 1
476 | 2
46°32 8
aja | 4
43-23 5
airse | 6
410 | 7
38 5S 8
36-93 | 9
35-38 | 10
au-7a | 1
az-ig | 12
sous | 13
2e-8s | la
27-20 | 15
25-55 | 16
23°90 | 17
ae-ee | 18
20-55 | 19
18°87 | 20
a7-ip | 2a
1-49 | 22
13°77 | 23
ea
b me
17 SL 14710)8,
1] 53 44°39
SUNDAY 15.
o 1 WF
28 32 4371
28 33 55°5
17 56 14°85| 28 34 5775
17 58 45°48) 28 35 4973
18 1 16'27| 28 36 3076)
18 3 47°21) 2837 15
18 6 18°30) 28 37 22-0
18 $ 49°52) 28 37 $2°1
18 11 20°38| 28 37 316
18 13 52°35] 28 37 20°6
18 16 23°95] 25 36 590)
18 18 55°64) 28 36 26-9
18 21 27 44| 28 35 4472
18 23 59°33| 28 34 50'S
18 26 31-30| 28 33 46°9
18 29 3°34| 28 32 $272
18 $1 35'44| 2831 679
18 34 7°60) 28 29 31°0
18 36 3982) 28 27 44:3
18 39 12'07| 28 25 47°0
18 41 44°36) 28 23 38-9
18 44 16°67| 28 21 202
18 46 49°00| 28 18 5078
18 49 21°34 18.28 16 10°6
MONDAY 16.
18 51 53 '63/S,28 13 19'8
18 54 26°01| 28 10 183
18 56 58°33) 28 7 671
18 59 30°63| 28 3 43"
19 2 289|/ 28 0 9%
19 43512) 27 66 25°3
19 7 7°30] 27 52 30:3
19 9 8944| 27 48 24°7
19 12 1b°51] 27 44 85
19 14 43°51) 27 39 417
19.17 1544) 27 35542
19 19 47°29| 27 30 162
19 22 19°05] 27 25 17%
19 24 50°72] 2720 84
19 27 92°28] 27 14 48°8
19 29 53°73) 27 9 18%
19 32 25 07 Eis 3 38-0
19 34 56°28 57 46°9
19 37 27°37] 26 51 45°5
19 39 68°32) 26 45 33°7
19 42 29°13] 26 39 116
19 44 59°79 Beis
19 47 30°30| 26 25 56'5
19 50 0°65) 2619 3°6
19 52 30°83|8,26 12 06
76 APRIL, 1838.
MEAN TIME. an
i” THE MOON'S RIGHT ASCENSION AND DECLIN to?
11 10°31
13 26°72
2215 42°71
22 17 5849
22 20 14°05
22 22 29 40
22 24 4455
22 26 5949
22 29 14°23
22 31 28°78
22 33 43°13
WEDNESDAY 18.
© ;20 51 34 02/S,22 34 10° 0 /22 42 38°69/5.11 28 20
1} 20 53 58°72] 22 23 10 1/22 44.5213) 1La2
220 56 23°17] 2212 @ 2/9247 5°41
3 |20 58 47°37] 22 045 8/22 49 1852
4j2l 111-30] 21 49 19 4/22 51 31°47
5 |21 3 34°98] 21 37 46 5 |22 53 44°27
6|21 5 58-40] 2126 4 6 |22 55 56°91
7|21 8 21°56] 21 1414 7/22 58 9-40
8/21 10 4446] 21 215 8/23 0 21°75
9}21 13 7-10] 2050 9 9 {23 2 33°96
} 10 }21 15 2948] 20 37 54 10 }23 4 4604
IL |21 17 51°61) 20 25 32 11 |23 6 57-98
12/21 20 13°47] 20 13 12/23 9 9°80
1
13 |21 22 35°07] 20 0 93
14/21 24 56°42) 19 47 3)
15|21 27 17°50} 19 34 4
16/21 29 38°33} 19 21 44°
17 }21 31 58°90] 19 8 36°0
18 )21 34 19°21] 18 55 20°55
19 |21 $6 39°27] 18 41 57 °8) 155-98
|} 20 |21 38 59°07| 18 28 27°9) 13697
21/21 41 1862] 18 14 50°9) 197-32
22 }21 43. 37°92] 18 1 7 Olise-48
23 [21 45 56°96) 17 47 16°1)139-40
f) 24/21 48 15°76/8.17 33 18°5
13 |23 11 21°50
14 | 23 13 3308
15 |23 15 44°55
16 |23 17 55°91
17 |23. 20 718
18 |23 22 18°34
19 |23 24 29-41
20 | 23 26 40°39
21 | 23 28 51°29
22 /|28.31 2°11
23 |23 33 12°85
24 |23 35 23:53
SATURDAY 21.
h
23 35 23°53
23 37 34°14
9
0
0
9
0
0
0
0
0
°
0
0
fe ee et OC OOSSSSOSSSSSS
2148
oy
5.4 41 22°68
PHH Sco S OOOH eH DRE eu
N2
SUNDAY
32°00 |N.2
42°37
53°21
on ec)
VI
17700
176°83
17665
17643
17622
175°97
178-70
175-43
17512
174 "30
1747
RREESSESSRSSS I Se mu swnuweo
Ces ds4s4evwes
MONDAY 23,
‘
° 4 ”
. 9 20 38°7
9 37 28°38
9 £152
10 10 580
10 27 36°8
10 4¢ 11°8
It 0 426
117 9°38
1) 33 318
1 49 49 '8
12 6 33
12 22 12 ¢2
12 38 164
12 54 158
13 10 10-2
13 25 59°
13 4 43°8
13 37 22°7
14 12 56°3
14 28 244
14 43 468
1459 3°
15 14 14%
-15 29 19°7
TUESDAY 24.
24°75 (N15 44 18
6 42-98
145
2015
39 09
58°27
17°70
37°36
57°27
17 42
37°82
58 46
19°35
40 48
1°86
23:49
45°36
748
20°84
8 5245
oOuwuUekea ea SOwuwe wo
Se H-Sy Ses swsese
15.59 11
16 13 58°3
16 28 38°6'
16 43 125
16 57 39°9
17 12 0°6
17 26 146
17 40 218
17 54 2271
18 8 15°3
18 220155
18 35 40"4
18 49 12°0
19 2 36°3
1915 530
19 29 2°
19 42 3%
19 54 .57°3
20 7 43-2
20 20 210!
20 32 50°9
20 45 126!
20 57 2671
N21 9 31°3
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43) 107 83
22 51 51°3| 10630
2
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3 173) 10) Fo] 1
3
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21 44 56°3| 11598
21 56 27°4| 113-75
22 7 499) 112-28
22:19 36) 11080
22 30 84) 10932
er 9 si:
21 93 16°5| 116 63
22 41
25
7
73
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38
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S“g5ces2eogeee2
2522 Ss aaa
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FAM Bannan aAnnnann
22) 4 4 23°75
6 5732
THURSDAY 26.
9 26°04 (N25 14 50°1) 8299
SEERRERAPRRES ARSE S3RRESS
32 Zone sar arenca—70
22 s" RERSCRARS ASSAF
naeene teed sande seaeanse es
wWeoseVv servos vovovwowvvw~o~oo~o~y eee |
aaa
CHAM EHONMACH AMT SOM erseaans
80°70
3) 53°26
8) 5150
“4| 4800
9S) 44-48
6°7| 42-7 | 2
10) 70°97
27 32 2°4) «62s
27 27 14
27 36 3
27:17
27 6 17°2| 55-02
27 11 Ne
27 22 15 °8| 49°77
25 31 876) 79-03
25 39 2°8| 77:37
25 46 47°0| 7567
26 54 45°8| 5348
27 0 86°7| 8648
54°92
23°94
53°10
22°40
sakca
CHAM TOM DASH
UT. APRIL, 1838. 79
MEAN TIME.
THE MOON'S RIGHT ASCENSION AND DECLINATION.
. ° b
0|7 7 98°62 |N.27 49 37°7 o}s
1}7 950-25] 27 45 47:3 1\8
2/712 11°34] 27 41 4841 2\8
3| 7 14 32°30] 27 37 403 3/8
4| 7 16 53°11] 27 33 238 4/8 11 18°39] 25 10 48°2
5| 719 13°38 | 27 28 589 5/8 1329°69| 25 3 19:2
6 | 7 21 33°30 24 255 6/8 15 40°60 | 2455 43°5
7| 7 23 52°87 | 27 19 436 7|317 5113] 2448 14
8| 726 12°09] 27 14 535 8/820 127] 2440 119
9| 7 28 30°95} 27 9 5541 9| 8 22 1102] 24 32 163
lo | 7 30 49°45 | 27 4 484 8 2420738 | 2424 141
(2 | 733 738 | 26 59 337 8 26.29°36| 2416 544
2/735 25°35 | 26 54 109 8 28 .37°95| 24 7 50°4
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PHASES OF THE MOON.
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ie APRIL, 1838. 85
"MEAN TIME. —
LUNAR DISTANCES.
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52 35 38/2870] 51 2 Aljcgs4
83 48 54) 2663] 82 11 24/2651
80 42 47) 2263] S2 29 41) 2252
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84 36 41/2177] 86 25 43) 2168
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124 27 Jl2105]126 17 5g) 2106
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| 78 32 15/2968 2) 81 34.17 2954 |
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13 35 39°12] 11 16 20°} 196 +60
13 37 31°57] 11 30 0°5| 136 25
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13 48 51°89
13 50 46°24
13 52 40°89
13 54 35°93
13 56 31°07
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MAY, 1838. 97
MEAN TIME.
HE MOON'S RIGHT ASCENSION AND DECLINATION.
:Aseension.| Declination, | Bisbee How | Right Ascension. Declination. | Pi-Dee.
SUNDAY 13. TUESDAY 15.
me or®# ” hme of * ”
\7 57 °51|8.28 20 21°0| 203 | 0/20 37 58°22/S.23 25 4°6]100+77 |
0 30°58] 28 18 151] 22°77 | 1/20 40 22-72| 23 15 0°0|102-20
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5 36°68] 28 13 31-1] 26-35 | 3/20 45 10°84) 22 54 25°1) 105-02
8 9°68) 28 10 53°0| 2313 | 4/20 47 34°46) 22 43 55°0|106~a2
0 42°64} 28 8 472) 29°93 | 5 |20 49 57°79| 22 33 16°5|107~73
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0 53°93] 27 55 1°7| 37+05 9 |20 $9 28°11) 21.49 21°0)11995
$ 26°56) 27 51 19°4) as-s2 | 10/21 1 49°95) 2138 2111447
5 59°11| 27 47 26°5| soo | 11 |21 4 11°48] 21 26 35°3/115-77
8 31°56] 27 43 22°9| 42-07 | 12/21 6 32°71] 2115 O-7}117 "03
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MONDAY 14. WEDNESDAY 16.
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THE MOON'S RIGHT ASCENSION AND DECLINATION.
our | Right Ascension. Declination. ] Dit, Dee toar| Right Ascension, ;
MONDAY 21.
ms ow Ww
53°37 °33 |N.13 26 40°7
he b
o}1 0} 3
1} 15550777] 13 42 0°9 1} 3.47 59°13 | 2354 1
2/158 445] 1357 162 2/3 50 26°03 | 24 3 83
3/2 0 18°39] 14 12 267 3| 3 52.53°17-} 24 12 5673):
4|2 2 82°58| 14 27 32°2 4/3 55 20°55 | 2422 96
5} 2 447703 | 14 42 32°6 5| 357 48'16| 24 31 13°5
6}e2 1*7a| 14 57 27°9 6} 4 015°99| 2440 870
7} 2 9 1671] 15 12 178 7/4 24405 | 24 48 52°9
8} 211 31°95] 1527 2:3 8/4 5 12°32 | 2457 2872
9| 2134745) 15 41 414 9| 4 7 40°81] 25 5 53°9
10} 216 3°23) 15 56 14°8 10} 410 9°51) 2514 9°8
11} 2.18 19°27] 16 10 42°5 11 | 4 12 3840] 25 22 1670
12} 220 35°59] 1625 4°5 12] 415 749] 25-30 123
13} 2 22 52°19 | 16 39 20°5 13| 4 17 36°78 | 25 37 58°7
14} 225 9°07 | 16 53 306 14} 420 6°25] 25 45 35°2
15} 2:27 26-22) 17 7 34° 15| 4 22 35°89 | 2553 1°7
16} 2 29 43°66] 17 21 32°3 16/425 5°71| %6 0182
17 | 232 1°39) 17 35 23°7 17|427.35'70| 26 7 246
18} 234 1940] 1749 8°8 18| 480 5°84] 26 14 20°9
19 | 2 36.37°69 | 18 2 47°3 19 | 4 32 36713 | 2621 70
20 | 2 38 56°27 | 18 16 19°3 20/435 6°57 | 26 27 42°68
21) 241 1514 | 18 29 446 21) 4373715 | 2634 B44
22/243 34°30} 18 43 341 22/440 7°86! 26 40 23°8
23 | 245 53°74 IN.18 56 14°7 ela IN.
TUESDAY 22.
248 1347 (N19 9 194 445 9°64 .N
250 33°49 | 19 22 17-0 447 40°70
2525381] 1935 74 4 50 11°86
255 14°41) 19 47 50°6 4 52 43411
257 35°30 | 20 0 264 455 14°45
259 56749 | 20 12 54°58 457 45°86
3 217796) 2025 15% 5 0 17734
3 4 39°72| 20 37 288 5 2 48°89
8 7 1°77) 20 49 34°3 5 5 20°49
3 9 24°10] 21 1 32-0 5 7 52713
311 46°73 | 21 13 21°7 5 10 23°81
$14 9°63} 2125 355 5 12 55°52
3 16 32°82) 21 36 372 515 27°25
318 56°30 | 2148 2-7 517 58°99 | 27 53 18°8
321 205} 21 59 20°0 5 27 56 45°9
323 44°09 | 22 10 28-9 5 280 2°3)
$26 8740) 22 21 294 5 28 3 671
3.28 32°98 | 22 32 21-4 5 2 6 32
$30 57°83 | 2243 4:8 5 28 ites
3.33 22°96 | 22 53 396 5 2611 21
3.35 48°34 | 23 4 5% 5 28 13 cic |
338 13°99| 28 14 go8 5 15 37
3 40 39°90 | 23 24 31°0 5 28 17 59°6
343 6°06) 23 34 30°3 5 28 19 511)
3 45 20 6) 5 Ne BWosa-n
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| homo Save &
| 0 | 5 45 46746 IN.28 21 32-0
| 1/5 48.17°66| 2823 2°3
2) 5 50 48°77 | 28 24 22°71
3|553.19°76| 28 25 31°4
4/555 50°64 | 28 26 30-2
S| 5 58 21°38 | 28 27.18 °6'
| 6) 6 0 51°99) 28 27 56's
|} 7} 6 3 22:46) 26.28 23-9
} 8/6 552777] 28 2841-0
916 8 22°93 | 28.28 47°s
10 | 6 10 52-91 | 2$ 28. 44°2
11 | 6 13 22-72. | 28 28 30°3
12 | 6 15 52°35 | 28.28 62
13 | 6 18.21°78 | 28 27 31°9)
14 | 6 20 5102) 28 26.4744
15} 623 20°04 | 28 25 52°7
16} 625 48°85 | 28 24 48°)
17, | 628 1743 | 28 23 33°38
18 | 6 30 45°78 | 28 22 8%
19 | 6 33-1390 | 28 20 340
20 | 635 41°76 | 28 18 4974
21/635 9'38| 28 16 55")
22/6 40 36-74 | 28 14 50-9
231643 3:82 N28 12.3771
SATURDAY 26.
0 | 6 45 30°64 (N.28 10 13'S
1] 64757718] 28 7 40-4
21650 e342] 28 45777
3] 652 49°38] 28 2 5°5
4|655 15°04] 2759 3°8
5. | 6 57 40°39 | 27 55 52°6
6]7 © 543] 27 52 32°5
7\7 2306] 2749 30
8] 7 4.54°37 |, 27.45 24°2
9]7 7 18°65] 27 41 3673
10] 7 94240] 27 37 39-4
11] 712 5°81] 27 33 33°5
12| 7 14 29°88 | 27 29 186
13] 7 16 51°60] 27 24 54'9
14] 7 19 13°98 | 27 20 22:4
15) 7 21 35°99) 27 15 412
16] 723 57°65 | 27 10 51:3
17] 726 18:95 | 27 5 52°9
18] 7 28 39°88] 27 0 46:0
19] 731 014] 26 55 30-7
20 | 733 20°62 | 2650 7-0
21/7 35 40°43 | 26 44 35-0
22] 7 37 59°86| 26 38 54°9
23.) 7 40 18°91] 2633 6%
|) 24 | 7 42 37°57 |N.26 27 10-3
WEESESEESEOSECOSLC RE SADE MDEDEORD
mR oe oe eISSN
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47 13°71
49 31°20} 26 8
5148°29| 26 2
54 4°98| 25 55
56 21°27 | 25 48
58 37°16 | 25 41
0 52°06] 25 34
3,7°74| 25.27
528-42] 25 20
7 36-70 | 25 13.
9 50°57] 25 5
12 4°03} 24 58
14.1709] 24 50
16 29°73 | 24 42
18 41°97 | 24 34
20 53°80 | 24 26
23 522) 24 18
25 16°23) 24 10
27 26°84 | 24 2
29 37°03 | 23 53
31 46°83 | 23 45
33 56°21 |N.23 36
MONDAY 28,
36 5°19 (N23 27 4475
38 13-76| 23 18 52
40 21°93 | 23 9 S34
42.29°70 | 23 0 48°9)
44.37°07 | 2251 38-4
46 44°03 | 22 42 22-2
48 50°60 | 2233 O71
50 56°78 | 22 23 324
53 2°56) 22 13 59-0
55 7°94) 22 42071
57 12°94 | 21 54 35°]
59 17°54 | 21 44 459
121°76| 21 34 50°7
3.25°59| 21 24 502
5 29°04 | 21 14 446)
7 32411] 21 4 338)
9 34°80} 20 54 17 9) 4
11 3712} 20 43 571
13 39°07 | 20 33 14 a
15 40°64 | 2023 0-9) x6
17-41-85 | 20 12 25
19 42°69 | 20 1 45
214318] 19 51 0
23 43°30 | 19 40 1170
25 43:07 |N.19 29 177
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14 35 1871
14 22 47°5
14 10 140
13 57 3775
13 44 58-2
13 32 1670
13 19 31*1
13 6 4374
12
12
12
12
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18 4844
20 33°92
22 19°30
24 4°60
25 49°81
27 34°95
29 20°02
31 5°02
32 49°96
34 34°84 7
36 19°66/N.4 20 1775
FRIDAY, JUNE 1.
1138 444|N4 6 169
wee we 4
SSUcSwackanan
Sea DADDONII Oo Ee
aes
SBwac
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) First Quarter
© FullMoon --- 9 4 57°5
© Last Quarter ~~ 16 9 419
@ New Moon - - - 23 4 23°0
> First Quarter - - 30 19 35-4
q
TV. MAY, 1838, 103
|. Star's Name Pil, % +a PL
3B ae i ii
z| Positi diffe
”
1| Sun Ww. | S42
Pollux w. 2046
Jupiter E, 4) 3053
Spica mE. soat |
Samm E. 3038 |
2} Sun w. 6 3445 |
Pollux Ww. Bi 3073
Spica m E.
Saturn E,
Antares E,
3) Sun Ww.
Pollux Ww.
Spica m E.
Satum = EL 75 27 38/3071] 73 58 53/3071
Antares E. 86 49 20/2073] 85 20 37) 2072] 83 51 53) 3071
4) Sun WwW. 3491 /129 55 58) 427/131 17 44) 5483
Pollux Ww. 64 42 44) a088
Regulus W-
Spica nm E.
Saturn E
Antares E. 74 58 37| 3054) 7.
5| Pollux Ww. 73 39 46) 3014
Regulus W. 37 2 11/4001
Jupiter W. 25 49 9) 5021
Saturn E. Si 42 90285
Antares E, 63 3 olin
6) Pollux = -W. 85 43 13) 2955
Regulus W. #9 3 22) 2966
Jupiter W. 37 51 42) 2959
Saturn = EL 39 41 58) 2986
Antares E. 50 59 24) 2904
7| Regulus W. 61 16 7) 2893
Jupiter W. 50 5 17] 2889
Saturn E. 27 36 10) 2972
Antares E, 38 44 55) 2884] 37
E. Ot 16 58} 3712] 90
Ww. 73 41 42) 2813] 75 2798 |
Ww. 62 31 21/2813] 64 39 56/2794
E. 26 17 58) 2808] 24 43 40) 2758 ‘ 2789 |
E. SL 0 43/3665] 79 48 19] 3663 3660 |}
86 20 49/2737] 87 56 40)2708 2718
75 10 42) 2737 2718}
32 17 47/2734
13 37 si) 12 hb
70 42 Vij abys
} 36 Bla6jel 99 13 2662100 50.
22 57 54
68 54 18)
2705] 38 42 45/2695] 40 19 32] 2685] 41 56
4| 2002] 88 15 48) 2894] 86 43
2560|109
26 iilesseftn1 6 4:
52) 2553| 66 35 52)2548] 68 16
100 19 56)
87 57 25
34.83 41
80 30 45
57 26 21
2611 5
21 18 12
67 14 24
68 33 9)
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2436] 60
2429] 47
2998} 38
2838] 60
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2754/17
2975) 73
2078] 61
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2321) 87
ae] 75
2636) 46
2638] 92
2276
2092
2590
3495
3050
2564
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29 55)2812/128. 55
9 53j2s28] 61 52 ee
10) Jupiter
| | Spica m W.] 43.33
BY) cos7/I17 1 10)2977|115 30 29) 2968
17 48]2596] 59 57
3 33/2683] 26 40
73 17 45]
39 51 21
27 23 33
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90 53 44)
53 20 13)
40 56 10)
36 33)
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35 46 50 58 7)2647
32 27] 96 54 51) 2651}
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27 26)
13 53
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| 90 37 17)3061
| 62 29 20/2903
. | 42 52 Sliz9a1
17 21 34/2869
« Aquile W.] 84 40 55) 3054
sae a 55 46 13 2002
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At 10", Mean Time,
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L 2 727520) 10 8 54°3
4 156 31°3| 4 44 32°3
5 |2025 8°5| 23 20 872
7 14 53.47°S | 17 55 45°78
9+ | 9 28 85-2] 12 81 22-3
11 351 50| 7 7 07
12 | 2219 42°9] 142 37°3
14 16 48 235 | 20 18 16°6
16+ | 1117 1°6| 14 53 53°4
18 545 41°8| 9 29 32°3
20 om206] 4 5 98
21 18 43 1°5 | 22 40 49°3
ss 13 11 40°3 | 17 16 26-8
25 7 40 21°5 | 11 52 6°7
27 29 0'3| 627 44:2
28 | 2037 41°99] 1 3 24-4
30 15 6209/19 39 2°1
L 4 425 55°0| 7 14 20°6
7 17 45 1°6| 20 47 28°
11 7 3 4°3| 10 19 31°6
14 | 20 22 7°0| 23 52 35-2
ise | 9 40 8°8| 13 24 37°8
21° | 29259116] 257 41°5
25% | 1217 112 | 16 29 41-8
29 1 36 10°1 2417
Il. 2+ | 10 51 17-7 | 13 32 53°5
S+ | 14 4 94 | 16 46 168
9 1450 115 | 18 0 24
9 18 225'0 | 21 12 47°5
16 18 4°1 | 22 27 10°1
16 22 9°0 | 139 1655
25 | 22 59
24 1 19
31 2 89
31 5 28
a 8+
8
25
25+
ov THE
OCCULTATIONS OF JUPITER'S SATELLITES BY
AND OF TRE
TRANSITS OF THE SATELLITES AND THEIR SHADOWS
OVER THE DISC OF THE PLANET.
For correcting the Places of the Fixed Stars. |
At Mean Midnight,
Togs ot
Day of the Month.
+9 °3731 |—0 "9563
1141s 9 3785
1°1350 9 3838
11281 Ft +9 "3892
Sen OFF BH
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94314
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94470
+9 4521
94571
9 4622
+9 4674
94725
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+9 4825 |—0 "9399
974875 | 09393
974925 | 079386
+9974 |—0 “9380
0 “9373
0 "9367
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2] 439 3526 | 22 10 32° | 15 4771 442 2°03
3] 443 41°17 | 2218 12° | 15 46°9 445 58°59
4) 4474744 | 2225 284 | 15 46-8 449 55°h
5] 451 64°05 | 22 32 21-3 | 15 46 453 51-70
6] 456 099 | 22.38 506 | 15 46 457 48°26
7) 5 0 $25 | 92 44 5672 | 15 465 5 1 4k32
8] 5 4 15°81 | 22 5037-9 | 15 46-4 5 5 41°38
9] 5 8 23°64 | 2255 55°7 | 15 4673 5 9 37°95)
0] 51231774 | 23 O49 | 15 46+2 5 13 34°51
p] 5 16 40-10 | 23 5 18-9 | 15 4671 5 17 31°07
2] 5 20 486s | 23 9 2471 | 15 4670 5 21 27°63
| 5245746 | 23 13 4°99 | 15 45°9 5 25 24419
| 529 6°44 | 23 1621-2 | 15 4578 § 29 20°75
53315758 | 23 19 13°0 | 15 45°7 5 33 1730
537 24°87 | 23 21 401 | 15 45°] 0.1102 | 5 37 19°55
541 34°29 | 23 23 4274 | 15 45°6 |] 0 23°83 | 5 41 10-41
545 43°81 | 23 25 2070 | 15 45°5 | 0 36°85 | 545 6°96 |
549 53-40 | 28 26 32-8 | 15 45-4] 0 49°88 | 549 3°52
554 3°05 | 23 27 20°83 | 15 454] 1 2°97 | 5 53 0-08
558 12°72 | 23 97 43-9 | 15 45-3] 1 16°07 | 5 56 56°65 |
6 222-35 | 23 27 42-2 | 15 45-3] 129717 | 6 O 53°2L
6 63200 | 2327 15-7 | 15 45-2] 1 4222 | 6 4 49°78
610 41°55 | 23 26 24°3 | 15 45-2] 1 55°21 | 6 8 4654
6145100 | 2325 S71 | 15 45¢2 10 | 6 12 42°90
619 0°32 | 23 23 e772 | 15 4571 86 | 6 16 39°46
623 gg | 23 212176 | 15 45" 48 | 6 20 36-01
627 1849 | 23 18 5173 | 15 45-1 6 24 32°37
| 27°29 | 23 15 56°75 | 15 45°1 6 28 29712
30] 635 35°86 | 23 12:37°2 | 15 45° 6 32 25
81] 639 44-20 N23 8 5375 6 36 222
Apparent Noon may be assumed the same as that for Mean Noon.
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17 44 26°85
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Sun,| 2) 10 44 8 019%
Mon.| 3/10 47 7 38 2270
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Wed,| 5/10 55 13 ‘84 654 bs
Thur) 6/10 58 80-45 6 31 468
Frid) 7/11 2 26°86) 9010 | 6 9 21%
Sat. | 8/11 6 3°09) 9r003 | & 46 50°
Sun.| 9)11 9 39°16| 8-997 | 5 24 128
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| 11] 11 16 50 ‘89| s-982 | 4 38 4)
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| "Thur 13]11 24 2°24) sge2] 8 52 505
Prid.| 4 ll 27 37:80) sso | 8 29 483
Sat. | 15] 11 31 13°31 3 6 423
Sun, | 16] 11 34 48 243 325
| Mon 17] 11 38 24 220196
‘Tues| 18} 11 41 59°74 157 38
Wed.| 19] 11 45 $5 ‘23 33 455
‘Thur 20 Hy 49 10°7 10 250
Frid,| 21] 11 52 46°31 47 2°7
Sat. |22]11 56 22-03 23139 0
Sun, |23]11 59 57 om 3
Mon,|24]12 3 33°65 23 112
Ties.) 25/12 7 9°65 46°36°9
Wed,| 86] 12 10 45°79 10° 2°7
Thur| 27] 12 14 22°11 33 281
eat 12 17 58°61 56 52°8
at. |29]12 21 35°31 20°16 3
| Sun, | 30) 12 25 12°25 248 3845
Mon.|31]12 28 49°43] | |S3 6589) — Ja 493
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| 5] 10 55 1404 $4 42 | 15 53°79] 1 20°94] 10 56 34°98
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| 15] 11 31 1492 3 637°7 562] 4 46°51
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m. | 17 | 11 38 25-08 220 14°3 56°7 | 5 28°55
es, | 18] 1142 0°61 1 56 58° 57°0 | 8 49°57
d. | 19] 11 45 3616] 1 33 39°5 373 §
ur. | 20] 1149 11°75] 1 10 18°6 57°53
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0 20°36 | 21 25 294 55 75
222-90] 2115 16°3 41 53°5
425709 | 21 4 S8°L 28 37°71
6 26°94 | 20 54 34-7 15 18°3
8284] 20 44 63 " 157°3
10 29°61 | 20 33 32°8 10 48 34°1
1230-43 | 20 22 54-4 ‘ 10 35 8°
14 30°92 | 20 12 111 10 21 412
16 31°08 N20 1 22°9)
CSSCECSESSSSSEZAHHEDDHHHEDED
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1b 18 54°87
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1124 9-70
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11 27 3912.N.
TUESDAY WU
1b 29 ae
1b 31 8-20
SERcEEGASESSuSHaCESES
BASEREESSe BSBSoSEEBZoSE_
Sdeehse i secsaudassdes
9
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SEPTEMBER, 1838.
i MEAN TIME.
THE MOON’S RIGHT ASCENSION AND DECLINATION.
frie anacin| netietinne| iene Ameen) etenieony
"
FRIDAY 21. SUNDAY 23,
homes ° homies
13 85 30-22 /S.12 8 15 7 47 46
13 37 1940 15 9 50°51
15 11 53"9h
-
BES
Pye
44384
46 28°50
48 18-98
50 9°70
52 0°65
53 51°85
53 43°28
57 34°96
59 26°89
1 1907
3 11°50
5 4°20
6 57°16
8 50°39
10 43 "89
12 37°66
14.31°71 3
16 26-04 54 19 34
18 20 °66|S.16 57 58'S 56 30°55 1S.
SATURDAY 22. .
20 15 °56)S.17
22 10°76
24 6-25
26 2°04
27 58°13
29 5452
31 51 22
33 48 23
$5 45°55
37 43-719
39 41-14
41 3942
43 38 02
129710
12865
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127 68
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17 14 27°83
17 16 51°24
17 19 14°95
17 21 38°94
17 24 3°21
17 26 27°76
17 28 52°57
17 31 17°65
17 33 42°99
17 36 8°58
17 38 34-42
17 41 0°50
17 43 26°82
17 45 53°36
17 48 20°13
17 53 14°32
17 55 41°73
17 58 9°34
18 0 37°14
18 3 5*12
18 5 33°28
18 8 1°61
18 10 30°11
9 |18 12 58°77
18 15 27°57
18 17 56°52
18 20 25°61
18 22 54783
18 25 24°17
18 27 53°63
18 30 23°19
18 32 52°85
18 35 22°61
18 37 52°46
18 40 22°39
18 42 52°39
18 45 2245
18 47 52°58
18 50 22°75/S
28 28 41°9/ 22-12
&
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WEDNESDAY 26.
17 50 47°12|8,28 42 504
28 43 35°9
28 44 114
28 44 369
28 44 52°5)
28 44 58°0
28 44 53-4
28 44 38°7
28 44 13°9
28°43 38-8
28 42 53°6
28 41 581
28 40 52°3
28 89 362
28 38 9°8
28 36 331
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1260
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SATURDAY 29.
me err
49 25°17/S.22 19 11°3
$1 50°49] 22 747'5
54.15°61| 21 5
56 40°53| 21 44 331
1 29°74
3 54°04) 2
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ll 5°70
13 29°16 10
15 5242 1L
18 1546 12
20 38°29 13
23 0°91 14
25.2832 15
27 45°52 16
30-7 "50 17
32 29°28) 18 32 lad
$4 50°84) 18 18 21°2 19
37 12°20) 18 4 2075 20
39 33°35) 17 50 12°3 21
41 54°29| 17 35 5678 22
44.1502) 17 21 34°0 23
46 35°55 /S.17 7 471
SUNDAY 30.
homes ° ul
21 46 35°55|S,17 7
21 48 55°88] 1
2151 16°00) 16 37 43°1)1
2153 35°93| 16 22 52°38
2155 55°66) 16 7 54°7
2158 15°19] 15 52 50°3
0 34°93} 15 37 394
2 53°67} 15 22 2271
5 12°62] 15 6 58"
7 31°39
9 49°9)
12 $3
14 26°57] 14 421°3
16 44°60) 13 48 2771
19 246) 13 82 2771
21 20°15] 13°16 2175
PHASES OF TH
E MOON,
© Full Moon = - -- ---
Last Quarter
@ New Moon - - - - - - -
doh
=e $18 17°5
- 1010 Ob
Str crete Is 8 448
LSU SEL: GELEERIELE [Ree
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46 10 41)26
1
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an
7 45
47 38.
90 6
59
1s
21 42
45
7
27 28°
7
255 825 =
"MEAN TIME.
LUNAR DISTANCES.
Aldebaran
Pollux
Mars
Venus
Sun
« Arietis
Aldebaran
Mars
Venus
Sun
e Arietis
Aldebaran
Venus
Son
« Arictis
Aldebaran
Pollux
Venus
Son
Aldebaran
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Mars
Sun
Aldebaran
Pollux
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Antares
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BH se2 hae4 hres
&
37\2729| 87 39
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=
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Saturn E.
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wW.
E.
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Fomalhaut E.
# Pegasi E.
Son Ww.
Saturn = W.
Fomalhaut E.
« Pegasi E,
Son w.
Saturn = W.
Antares W.
-Fomalhaut E.
a«Pegasi E.
Sux w.
”
34 2 46)3406
22 35 48) 3241
35 0 27/3035
88 37 58) 3893
45 2 59/3359
23 1 35/2992
78 44 30| 3265
104 38 51
56 11 33
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67 31 36
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2920
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66 38 sjex99] 68 21 44
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33 22 59/229] 31 57 22
54 25 18/2798] 52 50 48)
94 31 28)2977] 92 47 20
129 21 22i2510/131 2 21
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68 7 40\2205] 69 56 0
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ses1] 86 9
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sues] 59 0
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3145) 90 14
aigi] 70 24
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2979] 42 15
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aaoa] 30 33 605 |
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40 23 47/2969] 38 52 23 4/3076 |
78 39 8jee2a| 76 51 8 ajaisdy
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84 36 36] 2073] 86 28 16)2061] 88 20 15| 2050]
64 6 18/2116 |
94 55 is 92119}
ot
196 SEPTEMBER, 1838. ‘x
CONFIGURATIONS OF THE SATELLITES OF JUPITEF
Tuz SATELLITES or JUPITER
are not visible this Month,
JUPITER being too near to the SUN.
SEPTEMBER, 1838. 197
ECLIPSES OF THE SATELLITES OF JUPITER.
Tus ECLIPSES or tuz SATELLITES or JUPITER
are not visible this Month,
JUPITER being too near to the SUN.
198 SEPTEMBER, 1838. x
APPROXIMATE SIDEREAL TIMES
ov THE
OCCULTATIONS OF JUPITER’S SATELLITES BY JUPITER,
AND OF THE
TRANSITS OF THE SATELLITES AND THEIR SHADOWS
OVER THE DISC OF THE PLANET.
Tur SATELLITES or JUPITER
are not visible this Month,
JUPITER being too near to the SUN.
Day of the Month,
Won OF we
XII.
For correcting the Places of the Fixed Stars.
At Mean Midnight,
A
41-2416
12443
12469
412494
1°2517
1°2539
+1 2560
12579
12597
41 °2614
1 2629
12643
+1 °2656
1 2667
12677
+1 2686
12694
12700
412705
12709
12712
+1 2713
1°2713
12712
+1 2709
|
|—0 "623
0 "8126
08219
—9 ‘7999
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0 0862
99405
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+9 9893
00857
01949
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03545
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+9 "8142
98158
98174
+9°8190
9 8205
9 8221
+9 $236
9 ‘8251
9 3266
+9 8280
9 8295
98309
+9 8324
9 °6338
98352
+9 °3366
9 °8380
9°8394
+9 8408
9 “8422
9 8436
+9 "8449
9 8463
98476
+9°8490
98503
9 °8517
4-9 '8530
9 8544
98557
D
| 2
09789
09795
09801
—0"9806
0°9811
09816
—0 ‘9821
0 ‘9825
0 “9829
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0°9837
9 "9840
—0 "9843
0 °9846
0 -ys49
—0 9851
0 9853
0 -°9855
—0 9856
09857
0-9858
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0 °9859
0°9859
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0°9858
09857
—0'9856
09854
09853
+9 8570 |—0 985)
1317 avs
13 13 4°39
13.9 8449
13 5 12°59
13. 1 1668
12 57 20°78
12 53 24°88
12 49 28°9
12 45 33 "0
12 41 37°15
12 37 41°23
12 33 4532
12 29 49 “41
12 25 53°50
12 21 57°39
12 18 17°63
1214 5°78
12 10 9°87
1g 6 13°97
12 2 18°07
IL 58 22-17
11 54 26°26
11 50 30°35
1 46 34°44
IL 42 38°53
11 38 42°62
IL 34 46-70
11 30 50°79
11 26 54°88
11 22 58°97
1b 19 3°07
home ‘
12 28. 49°43) 9-061
12 32 26°89] 9074
12.36 4°66) 9-087
www,
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12 39 42°75] 9-102
12 43 21°19) 99117
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12 54 18°86) 9*170
12 57 58°94] 9-189
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13° 5 20°50) 9-230
18 Y 2°02) 9-252
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13 12 44°06] 9-274
18 16 26°61) 9297
13 20 9°77| 97321
13 23 53°47| 9-345
13 27 37°76! 9370 |
13 31 22°04) 9:age |
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13 38 54°25) 9-449
13 42 4102} 9-476
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13 46 28°44) 9:503
13 50 16°52) 9531
13 54 5°27) 9-560
13 57 54°71] 9°390
Id 1 44°86) 9-619
14 & 35°71) 9-649
14 9 27°28] 9620
14 13 19°59} 9-7at
14 17 12°65) 9-743
14 21 649) 9°776
1425 1*1L
* Acon Time of the Semidiameter passing may be found by subtracting 0*18 from th
|
Right Ascension, Declination, | Semidiam*] 71°" | Sidereal Time,
moe homo
10 14°40 | 12 39 538
m, | 1] 12 26 50°98 s, 7 8's | 16 0%
es | 2] 12 s2 2649 330 27°5 | 16 0O°9] 10 33°44] 1243 1493
ed. | 3] 1236 6°30 353.43°8 | 16 1°1 | 10 52-18 | 12 46 58 46
ure] 4/12 89 dad | £1657°3 | 16 14] 11 10°59] 12 50 55 05
id. | 5] 1243 22°93 | 440 7°68 | 16 1°7] 11 28°65] 12 54 51-56
6/1247 1°79| 5 314°9 | 16 2-0] 11 46°34 | 12 58 48-13
m | 7) 12 504106) 5261s |16 22] 12 863] 13 2 4469
m | 8/32 5420-75) 549 17°38 | 16 2-5] 12 20-50] 13 6 41-25
jes. | 9] 12 58 0°87 612 128 | 16 2°8] 12 36°94] 13 10 37-81
td.) 10]13 14145! 635 3° | 16 30] 12 52-92] 13 14 34°37
ur] ID] 13 5 22°52) 6574871 | 16 3:3] 13 8-40
ld. | 12 ]13 9 4-09 7 202777 | 16 3°] 13 23°39
b | 13]13 124617) 743 14 | 16 3°S] 13 37°36
n, | 14] 13 16 2677 8 528°8 | 16 4*1 | 13 51-79
m. | 15] 13 20 11 $2749" | 16 4:4] 14 5718
es. | 16] 13 23 5569 850 3° | 16 4°74) 14 17-99
od. [17] 13 27 4002) giz 90 | 16 49] 14 30-21
vr,|18]13 31 2a'94| 9 34 72 | 16 5B] 14 41-84
id, | 19] 13 35 106 | 955570 | 16 5S] id 52-88] 13 50 3-34
| 201713 38 56°62) 1017379 | 16 5°7] 15 3-27] 13 53 59-89
nm | 21/713 42 43°42 | 1039 9°8 | 16 6°] 15 13°03] 13 57 56-45
mm, | 22] 13 46 30°87) 11 03241 | 16 63] 15 22°13] 14 1 53-00 |
es.| 23] 13 50 18°98 | 11 21 444 | 16 66] 15 30°58] 14 5 49°56
fd. | 24113 54 7°76) 11 42 462 | 16 68] 15 38°37] 14 9 4613
ur.) 25) 13 57 57°23) 12 337°3 | 16 741] 15 4546] 14 13 42-69
@ | 26) 14 1 47-40) 12 261771 | 16 73] 15 51-84] 14 17 39-24
t | 27] 14 5 38°27) 12 44 45°3 | 16 7:6] 15 57°53 | 14 21 35-80
28] 14 9 29°86) 13 5 14 | 16 78
2g] i413 2219 | 1325 St | 16 8-0
30] 1417 15°27 | 13 44 560 | 16 83
=
oe
31] i421 912) 14 433°8 | 16
32] 14 25 3°76 S14 23 580 | 16 88
i BEEF
* The Semidiameter for 4pparent Noon may be assumed the
et
187 51 16'9
19247 13
193 46 16°7
194 45 g4-4
195 44 54‘
196 44 16'S
197 43 412
198 43 8 *1
199 42 87°3
200 42 87
201 41 424
202 41 18 "2
208 39 365
209 39 26:2
210 39 176
211 39 10°6
212 39 53
214 38 59'S.
215 38 53'8
216 38 59 ‘8
217 39 2%
0)
NO-12
oe
0-38
Ov5L
0°63
0°73
0°82
0°87
0-90
0°90
0°87
Oo-81
0-72
0 ai
0-48
O'34
ol
|N.0 “08
‘8.003
O13
1'5/8.0"
00001516
0 0000255
99998999
99997749
9 9996504
99995266
99994033
99992804
9°9991581
979990364
99989148
99987935
9 9986723
9 °9985511
99984299
99983086
9°9981873
99980637
9 "9979441
99978224
99977007
9 9975794
9 9974582
9°9973374
2 Bik
) 3909789
9 9968612
99967447
9 9966296
9 "9965161
9 "9964040
15 19°3
15 772
la 574
14 50°1
Id 452
14 424
15 36°7
15 49°0
16 17
16 13°9
16 24°
16 324
16 36'2
16 354
2 S255
ea Raa B28 Gab GRE Gea Sze
1838,
OCTOBER,
hur] 11}120 6 12-3) 126
13] 144 26 47 °5/ 150
14] 156 20 51°5| 162 1
fed.| 10/107 31 40) 113
Hid. | 12] 132 23 19 °5 | 138
a
ow
?
=
=
=
fur] 32] 31 24 45°6) 38
MEAN TIME,
ASCENSION AND |
home °
22 41 52°05|S.10 4
3
=
—
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2 on
Cees hse eve co
SYERESABSH
Srssceeeeseens
geeress_s
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ne
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10
9
9
9
9
8
8
8
7
7
6
6
5
5
5
4
4
4
19 15 "34
21 32°85 |
mre rere errooocoocoesccooscs]
23 33 35 K0/S. 4
TUESDAY
23 35 49 ‘85)S. 3
23 38 3°87
23 40 17 86
23 42 31-82
23 44 45°76
46 59 68
49 1339
51 27°50
53 41 "40
55 55°30
58 9°21
0 23°13
2 37°07 |S.
4 51°03
7 502
9 19 04
11 33°09
13 47°19
16 1°33
18 15752
20 29°77
22 44-08
24 5846
27 12°91
29 27°43 |N. 3 35
38° 3°13
$5 21
37 40
39 59°64
42 18°88
44 38°34
46 58°00
49 17°88
51 37°97
53 58-28
56 18781
58 39°57
1 05
3 21°76
5 43-21
8 4°88
10 26°79
12 48°93
15 11731
17 33°93
19 56°79
WRHUBK HK SSDS Se OHHH wD wes
WWWKKWKK RYE Re eee eR RR ee Ree
|] cooscooeocosesss
OCTOBER, 1838. 205
‘MBEAN TIME. _ 4
THE MOON’S RIGHT ASCENSION AND DECLINATION.
thtAsceusion,| Declination,
PRIDAY 5. SUNDAY 7,
moe or ” homes OR ’
19 56°79 IN.17 7 46°0| 14750] 0 | 4 18 41 ‘84 |N.26 12 59-0] 7a-sa
22:19°89 | 17 22 31‘0/ 186-30] 1) 4 21 14°72] 26 20 190] 7-55
24 43°23 | 17 37 8°8) 1457] 2) 4 23 47°70 | 26 27 28°3| 69-73
27 6°82 | 17 SL 39°2/ 14352] 3 | 4 26 20°77] 26 34 26°7) 67-93
29 3065 | 18 6 21) is235] 4 | 4 28 53°93] 26 41 14°3| 66-13
$1 54°72 | 18 20 174) sates] 5 | 431 27°17) 26 47 51°!) base
34 19°04 | 18 34 2571) 1a0-00] 6 | 4 34 O49] 26 54 17-0! G20
36 43°60 | 18 48 25°1| 138767] 7 | 4 36 33°87 | 27 0 32°0! 60-67
39 S41] 19 2 17°)/ 13738] 8] 439 7°30] 27 6 360) se-es
41/3345 | 19°16 12) 136-00] 9 | 4 41 40°60 | 27 12 29°21) 57-02
43-58°75 | 19 29 37°2] 13465] 10 | 4 44 14°33 | 27 18 112) 5520
46 24°29 19 43° SI) 13397] 11 | 4 46 47°91 27 23 42°) 53°37
48 50°07 | 19 56 24°7/1s0-ss] 12 | 4.49 21°51 | 27 29 2°6| cis
51 1609 | 20 9 36°0 13 | 4.51 55°14] 27 34 11°8| 49770
53°42°36 | 20 92 38°58 14] 4 54 23°78] 27 39 10°0| a7-5
36 8°86 | 20 35 3371 15 | 457 2°43) 27 43 57°1| 46-03
58 35-60 | “20 48°18°7 16 | 459 36°07 | 27 49 33°3| sais
1 2:58| 21 0 55°7 1j|5 2 42°85
3 29-80 | 21 13 2378) i}s 4 40°52
5 57°25) 21 25 43°0 19/5 7 abba
8 24°94] 21 37 53°3 2015.9 a6 “85
10 52°85 | 21 49 54°5 21 | 512 35°00
13 21°00 | 22 1 46°6 22/5 14 ag13
15 49°37 IN22 13 294 231517 313s
SATURDAY 6.
18 17°96 N22 25 2°9) 114-02 Oo 4°
20 46°78 | 22 36 2770) 112-45 2 37°46
23°15°81 | 22 47 41°7| 11085
25 22 58 46-8! 109-25
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OCTOBER, 1838. 209
MEAN TIME.
THE MOON'S RIGHT ASCENSION AND DECLINATION, ]
Right Ascension.| Declination. | Bie Bee Hour} Right ion.| Declination.
SUNDAY 21. TUESDAY 23,
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The SATELLITES are not visible until the 18th day of this Month,
JUPITER being too near to the SUN.
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the Satellites hy points. The numerals 1, 2, 3, and 4, annexed to the points, serve to
the Satellites from each other ; and their positions are such as to indicate the directions
which arg in all cases to be considered as fomards (he numerals, When
in areal sloageton the point is placed above or below the centre of the
left or right hand of the page, denotes that oe Sn
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hom & bh
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20 | 21 32 19-9] 11 Im. !
22 116 04755] 6 Im. i
24 | 1029 18°6| 0 Tm, * |
26 4 a 45°2 | 19 Im. |
27 «| 23 26 161 | 13 Im. !
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* The Satellites are“ not visible until the 18th day of this Month,
Jupiter being too near to the Sun,
220 OCTOBER, 1838.
= ;
| APPROXIMATE SIDEREAL TIMES
or TER
| OCCULTATIONS OF JUPITER'S SATELLITES BY JUPITER,
|| AND OY "THe " sea
TRANSITS OF THE SATELLITES AND THEIR SHADOWS
|| OVER THE DISC OF THE PLANET® |
Occourations,
Satellite] Immersion. Emersion.
i. LD 21 9 37
Shatew, [28 12 50
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| * The Satellites are not visible until the 18th day of this Mouth,
Jupiter being too near to the Sun, |
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14 32 52°76
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38 10°69 | 18 56 31°8 5 3 37 30°40 | 23 43 46 3).o1-1s
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42 59°41 | 19 23 258 7342 35°07) 24 3 50°2
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47 49°59 | 19 49 50°5 9| 347 42°77| 2423 146
50 15°23 | 20 2 51'S 10 | 3.50 16°63 | 24 32 41/8
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MEAN TIME.
LUNAR DISTANCES.
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17 16 51-60
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17 25 41°80
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17 34 33°19
17 38 59°24
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PALLAS. 817
EPHEMERIS OF PALLAS FOR THE OPPOSITION.
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SATURN.
NOVEMBER, 1838.
MEAN TIME.
1810 49°1
18 12 23°9) -0385597| 0
18 13 58°5) 0387616) 0
18 15 33°0| 70389537) 0
1817 7'4) *0391360| 0
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18 20 15°
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THE GEORGIAN. 347
JANUARY, 1838, |
MEAN TIME, |
mes orw bm
30 35°44/S, 10 10 51°7\1'3143067) 8 47'S
30 44°17) 5) *3146035) 3 43°5
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THE GEORGIAN. 349
MARCH, 1838.
MEAN TIME.
&
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"322970323 14°5]339 37 49°9
'3228874 [23 10°8]338 38 28°
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THE GEORGIAN.
JULY, 1838;
SOR San Boe
Ses
S58 B86
MEAN TIME,
Right
Scension,
Noon
me | oO 8 mn ° oon w
56 18°08S,7 38 57-2 |1-2922249/16 17°2]3 046.25
56 15°53] 7 89 15°2 | -2918959/16 13°3]539 48 38°] 0 46 25°
56 12°86} 7 39 34°1 | °2915697/16 9°3]339-49 L7°3| 0 46 25°.
56 9°99) 739 541 | “2912463 0 46 25°
56 6:96, 7 40 1571 | “2909258 046 25"
56 3°76) 7 40 37°1 | “2906083 0 46.25"
56 0°39) 7 41 071 | '2902939/15 53°3]339 51 S22} 0 46 25"
5556786, 7 41 24°1 | -2899827/15 49°3]339 52 30°9| 0 46 25"
55.53°17| 7 41 49°1 | '2896749/15 45°3]339 53 9°6) 0 46 25"
55.49°31| 7 42 15-1 | °2893704/15 41-3]339 53 48'3| 0 46 25°7
55 45°30) 7 42 42-0 | -2890694/15 37°3|339 54 26°9| 0 46 25°
554112) 743 99 | 28%7720/15 33°3]339 55 5:4) 0 462577
55.36°79| 7.43 38°7 | °2884783/15 29°3}339 55 440] 0 46 25°8
55 32°31] 744 8°4| “2881883/15-25°3/339 56 22'5| 0 46 25°83,
5527767) 7 44.39°1 | “287902215 21°3]339 57 Lal 0 46 25:8
55 22°88) 7 45 10-6 | 287620115 17°3]339 57 39°8| 0 46 25:
5517793, 7 45 43°0 | °2873421|15 13°3]339 58 1875| 0 46 25
55 12°84] 7 46 16°3 | *2870682/15 9°3]339 58 57°28] 0 46.25
55 7°61) 7.46.50°5 | °2867986/15 5°3]339.59 35'9) 0 46 26:0
55 2°23) 747 25°S | 2865334/15 1°2)340 0 1477) 0 46 2670
54.56°7) 4 48 L'4 | °2862797/14 57°2/340 0 53'4| 0 46 26:0
S45i-o4) 7 I4 53°2]340 1 3271] 0 46 26°0
b 10 210°], 0 462671
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THE GEORGIAN. 855
SEPTEMBER, 1838.
MEAN TIME.
5 SSS.
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233 S85 SEE eee.
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THE GEORGIAN. 357
NOVEMBER, 1838.
MEAN TIME,
Geoceutric, Heliocentric.
°
3:
2
=
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» MEAN PLACES OF 100 PRINCIPAL FIXED STARS,
FOR JANUARY 1, 1838,
a Star's Name, Mag.) Right Ascension. | Annual Var.
5
€ hom
\F Anu ----+- 2 |10 8 47°790|4 2/3034 fs
‘Uns Masonis - -|1,2] 10 53 40°365 3 °8069
Lronis - - - = - 3B JIL 5 28-946
* Hydow et Crateris -|$,4]11 11 La ‘se2
Lxonts +--+ - 2.3/1 40 47°570|+
‘Unse Masonis- -| 2 [11 45 16°554
t# Chamileontis- - -|'5 |12 9 0°227
is-- - + = -| 1 12 17 38°772
BCorvi - --- - - 2.3/12 85 53°437|4
}Canum Venaticorum| 2.3] 12 48 26 628
Vincints (Spica)| 1 |13 16 40 058
ns# Masogis - -|2.3]13 41 8 “800
13 46 58425 |4 IN.19 12 49-15
13 52 27 623 5.59 35 12°51
ld 8 16-498
14 28 39 "825
see 14 87 54°753)4
eS eS Id 41 55 “826 |4
14 51 15 "220
aie ee eh 15 8 17°979|4
Cornon® Boreaus 15 27 49 °S11/4 2°527)
@ SERPENTIS ~ - - - 15 36 17°557|4 2°938
© Urse Minoris - - - 15 49 59 825 273687
p ji ---- - 34730
SOprnrvcar - - - - 16 5 SI°757\|4- 3°1375
@Sconri (Antares) 16 19 297165 36626
Draconis - - - - - 16 21 48 499 0'7944
16 31 35°055}4- 6 °2511
17 2 49°356
1] 7 15832
4 $51
26
FORMULE OF REDUCTION,
ACCORDING TO PROFESSOR BRSSEL.
— Adopting the Notation and Coefficients employed by Mr, Baily, in his Intro~
duction to the New Tables of the Astronomical Society of London.
=cosa seed ©
b = sin « sec 3
c= 46:0206 + 20°0426 sin @ tan >
d=cosa tan
a’ = tan w cos }—sina sind
c= the annual proper motion in Right Ascension, in arc.
Ac’= the annual proper motion in Declination.
ere ¢ denotes the time from the beginning of the year, expressed in fractional
rts of 1 year, © the Sun's and © the Moon’s true longitude, % the mean lon-
tude of the Moon's node, and w the obliquity of the Ecliptic, each for the time ¢:
SS
FIXED STARS, 1838. 367
CONSTANTS vox FACILITATING raz REDUCTION or STARS.
by of the At Greenwich Mean Midnight.
= | f @ h H if
w ” Citi u of 0) i
uly 5| +21°63 | +12°74 | 317 41 | +2027 | 167 39 | + 1789 |
lo} 2249 13°05 | 318 37 20°20 | 163 14 2°53
15 | 23°33 13°38 | 319 27 20°11 158 46 316 |
20] 24°15 13°70 | 320 11 2001 154 16 3°77 |
]
25] 424°95 | +14°02 | 32049 | +19°89 | 149 42 | + 4°36
30] 25-972 14°33 | 321 23 19°76 | 145 4 4-9l
dug. 4 26°45 14-64 321 53 19°62 140 22 S44
9 27°16 14°95 322 19 19 48 135 36 592
14] +27°83 | +1524 | 322 42 | +19 ‘34 130 46 | + 6°36
| 19 28°47 15°51 323 4 19°21 125 50 6°75
2h] 2908 15°77 | 323 24 198 | 120 50 7‘l0 |
eg | 29°66 1602 | 323 43 1896 | 115 45 7-41 |
fept. 3] +3022 | 416-26 324 2 | 418 "86 110 36 | + 7°66 |
i s| 30°76 1648 | 324 22 18°78 | 105 23 7°86
® 9 | si*29 1669 | 324 42 1s'72 | 100 7 800
18} 31°80 16-89 | 325 4 184 94 49 8-08
23 | +32°30 | 417708 | 325 28 | +18 °68 s9 28 | + sll
28] 32°81 17°25 | 325 54 18°69 84 6 8°07
Det. 3] 33°32 1743 | 326 22 18 ‘73 78 46 7°98
e 8] ss-s4 1760 | 326 53 18°30 73 26 782
«AS | 484°38 | 17°77 | 327 26 | +18"89 68 s | + 7°61
1] 34°9t 17°94 | 328 2 18°99 62 52 734
| 23] 35°53 Ig‘12 | 328 40 19 "11 57 39 ol
es] 36715 18 '30
Nov. 2] +36°80 | +1850 +19°39 47 Mh | + 6°20
37 48 1871 42 22 5-72
38°20 18°94 37 23 519
38°96 1919 32 9
APPARENT PLACES or « axp 3 URS MINORIS,
FOR THE UPPER TRANSIT AT GREENWICH,
URSH MINOR, Da;
.
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Bes
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APPARENT PLACES or a Axo 2 URSE MINORIS,
FOR THE UPPER TRANSIT AT GREENWICH.
JULY.
@ URS MINOR,
Polaris
Sen ver woe
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FIXED STARS, 1838.
APPARENT PLACES OF THE PRINCIPAL FIXED STARS, 1]
FOR TiiE UPPER TRANSIT AT GREENWICH.
Dec. North. |
3 27 23 36
" ” seit
ine fe
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35 60 on
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20 43.0%
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} 5228 ° 79) 95-4 9%
o'20 2
* | 52-65 977) 362%
pepe eta
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i
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22:3 07
FIXED STARS, 1838, 379
APPARENT PLACES OF THE PRINCIPAL FIXED STARS,
FOR THE UPPER TRANSIT AT GREENWICH.
=Po
233
i a3 ys
21 25°5 0
$1 26°3
b. 10 27-0 ee
el
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| FIXED STARS, 1838. 381
APPARENT PLACES OF THE PRINCIPAL FIXED STARS,
FOR THE UPPER TRANSIT AT GREENWICH,
@ On10Nts, # Geminorum.
a. Bas i
Go8S sees
FIXED STARS, 1838. 385
| APPARENT PLACES OF THE PRINCIPAL FIXED STARS,
FOR THE UPPER TRANSIT AT GREENWICH.
—- we
wesos
x=
iS ahaa’ fase soee
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= Gar
FIXED STARS, 1838. 887
APPARENT PLACES OF THE PRINCIPAL FIXED STARS, |
FOR THE UPPER TRANSIT AT GREENWICH. |
}
my. y Argus. « Unss Masonis. 3 Leonts. |
baal RA. | Dees Souk | B.A. | Dees Northe| BA. | Doce Nori.
| | 1 as" | ss a9'| ad sd" | oF 36
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20
30
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=
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APPARENT PRINCIPAL FIXED STARS, |
FOR THE UPPER TRANSIT AT GREENWICH.
i
2 B Unsa Mixonts, & Libre, a Cononat Borrants. |
SSSe FSF
Ssose Soe
60°6
60-2
59°8
594
FIXED STARS, 1838. 397
APPARENT PLACES OF THE PRINCIPAL FIXED STARS,
FOR THE UPPER TRANSIT AT GREENWICIL
15 57-0
16 00
se
CSS exe
Seus Suis
S525 e288
GG aad Sdee
ea
RENT PLACES OF THE PRINCIPAL FIXED STARS,
FOR THE UPPER TRANSIT AT GREENWICH.
FIXED STARS, 1338)
APPARENT PLACES OF THE PRINCIPAL FIXED STARS,
FOR THE UPPER TRANSIT AT GREENWICH. |
woe
ST
85
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25
0 il
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.
SETS,
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8B S852
fad
APPARENT PLACES OF THE PRINCIPAL FIXED STARS
FOR THE UPPER TRANSIT AT GREENWICH.
MOON-CULMINATING STARS. 411
At Greenwich Transit.
« Aurige - - -
¢ Geminorum = -
© Aurige - - -
« Geminorum =~
Moon I.
Moon I.
« Geminorum
» Geminorum =
« Geminorum -
» Geminorum -
Moon If. _u,c|
NX Caneri- - + -
» Cancri- - - -
® Caneri- - - -
y Cancri- - = -
134°89
130757
CCSCeem Sersmis IAA SOOCOUt,
9
9
9
9
9
9
9
2
118-25 | 63 88 |
114°89 | 62-92 |
"
~ MOON-CULMINATING STARS. 413
21 4 28°84
21 35 56°33
22 6 17°24
22 35 34°62
131°57 |
133-°01
1
1
I
2
2
2
2
2
2
3
Moon I. wie.
B Virginis - -
b Virgie - -*
8 Virginis ---
irginis = - *
Moon Il, Le,
Moon I. we.
7Virginis ~ ~ -
Virginis - - -
Vinnie = -
eae
Moon I. be!
ae Ih vel
‘irginis -
mn Virgiuie .
© Virgins -
» Virginis ~
Moon ff.
——oe
sas.
10 22°03
4 16°50
10 22-06
1 51-97
50 45°95
16 46°05
15 30 43 ‘22
50 46‘01
22
2 pen
107°87 | 60°96
109 ‘22 | 61°38
MOON-CULMINATING STARS. 417
hom a
4 37 53°04
4 32 31-92
4 53 2542
32 31-91
Moon I.
Moon 1.
e Geminorum
£ Geminoram
« Geminorum
¢ Geminoram
Moon I,
Moon I.
@ Geminorum
« Geminorum
« Geminorum
* Geminorum
Uc,
134°56
190 46
OREM SIND D SOOO Bane es
cc
a ad Sew ww
.
wu
Sa8S28
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OABAR
MOON-CULMINATING STARS.
«@ Scorpii -
Moon Il, ke 16 21 1°27
Moon Il. vu. “7)| 16 50 25-39
§ Ophiuchi = rf 17 12 4°5
3 Sagittarii - 17 87 22"
8 Ophiuchi- - 17 12 4°60
3 Sagittarii - 17 37 22°49
Moon Il, & 17 20 50°76
Moon II. te. 17 52 8-28
2 Sagittarii- -4 | 18 10 37°81
Sagittarii- ; 18 35 32°34
2 Sagittarii- 18 10 37°85
Sagittarii « a 18 35 32°37
Moon ll, Le, 18 24 4°94
Moon I. 18 56 24°72
4*Sagittarii 19 26 50°75
59 Sagittarii- 19 46 59°92
A Sagittarii- 19 26 50°78
59 Sagittarii 19 46 59°95
Moon It. 19 28 50°29
Moon II. 1-C 20 1 4°90
Sf Capricorni 6 | 2020 0°33
Capricorni ‘ 20 36 29°58
Moon II, . 20 32 54°34
Moon IL, w.c.) 21 4 8°18
Moon If, | 21 34 40°41
Moon II, wv, 22 4 29°35
Moon IT. J 22 33 37°20
Moon II, v.c. 23 2 904
Moon 1. 29
Moon I,
Moon T,
vee.) (3°7)
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© Leonis ~
v Leonis-
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» Virginis
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9 Virginis
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Moon I,
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Moon II, wel
(192)
18°20
45°70
38°01
27°21
30°27
41°01
30 26
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36°37
40°67
38°83
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38-84
11-98
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43:42
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16 19 30°79
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130°75
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17 12 543
17 5 25°30
17 12 546
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17 32 32°13
17 55 25°78
18 10 38°75
17 55 25 "82
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19 26 51°65
18 56 So 62
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Moon I. P 2 13 28°80 143-18
Moon I. . 4) 2 42 26°19 146 42
Moon I. +C. 300 5 14970
Moon I. Lo, 152 68
Moon I. at 5 155 ‘04
Moon I, 5 156 "46
Moon T. -C i 156 A
Moonl, ie] “ 155 ‘65
C Tauri - - - - 5 :
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Moonl. te tt 149 "85
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| MOON-CULMINATING STARS. 427
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14 41 58°01
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7 24 23-32
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17 54 8 '12
17 55 27°69
18 10 40°76
17 55 27°70
18 10 40°77
18 26 59°53
18 45 1643
18 56 52°82
18 45 1644
18 56 52°S4
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19 35
19 52
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21 17 2749
28 3°14
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57 43-64
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22 36 47°06
23 5 58°24
23 5 58°27
23 4 0°63
23 30 88°18
23 53 3348
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MOON-CULMINATING STARS. 433
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MoonK, lac, 10 7 18°47
Moon I. ne. 10 30 18°22
Moon I. | 10 52 41°51
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Moon If. v.c}(17°9)] 127 13°13) 10 58 | 139) 69)
| y'Arietis- - - -| 4.5 1 44 42°09 18 30
§'Arietis - = + - 6 2 910'99| Na9 9
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@'Arietis - + - - 6 2 9 10%! 19 9
Moon II, Lol - = | 155 21°60 | 14 18) T4975 | JO
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Moon II, vw.c|(20")] 3 22 43°01 22 38} 14g 63 | 727
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Moon Il. Lol - + | 8 5253746 | 24 48} ISBOd | 73!
Moon If. vic} (210)] 4 23 29 60 26 22 | 15386 | 73°
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Toori----| 2@ | 516 582} 28 28
Moon II. Le} - + | 4 54 22°56] 27 35 | 154°8O |
Moon II. ue.) (22°1)] 5 25 20-60 28 22 | 15468 | 73
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« Aurige - - + 4 6 5 5°62 29 33
Moon ll, hej - = | 5561089} 28 43 | 153°40 | 73°
Moon II. wv.c|(23'1)] 6 26 37°72] 28 37 | 150°99 | 72!
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20 38 52°13
20 36 33°28
20 55 1412
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20 55 1411
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Moon II. v.c, a 1205
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Moon II, Loy “i . 109 65
Moon If, v.c, 4 . 107 “93
Moon Tl, he. “ K 106 "88"
Moon II. wc, ‘ 3 106 50
Moon ll. hel - - 106”
Moon II. t-e,| (28 6) “ 107 °7)
Moontl. hel - - . 109 28
Moon HI. w.c,| (29 6) 1b 48
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Moon I. .e, y 125 °63
Moon I, | ‘ 5 130 "21
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11 12 49 00
11 28 41721
11 12 49°03
11 28 4124
11 21 53'3
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2 47 28 42
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18 3°97
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MOON-CULMINATING STARS. 447
At Greenwich Transit.
3 Zen mM
Ar eous wv,
Suebsss fF
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v' Tauri -
r Tauri - -
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Moon If,
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11 26 8°06
11 42 18°35
11 51 41°57
11 42 18°38
11 51 41°60
11 47 37°30
12 8 58°67
12 33 29°53
12 45 58°57
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Mag-
Name, Apparent
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tn Time,
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¥ Virginis - + -| 5.6 | 12 45 58°60) 5S. 8 39
Moon It. tc] - - | 12 30 2147 3 53.| 107 22
Moon If, v.c.| (24 ‘0) | 12 51 54°87 6 44.| 108 "48
A9Virginis - - -| 5.6 | 12 59 27°35 9 52
a Virginis - - - 1 13 16 42°22 | 5.10 19
49Virginis - - -| 5.6 | 12 59 97°38 | S. 9 52
aVirginis ---| % | 13 164225] 10 19
MoonIt. lel - + | 13 18 47°85 9 33 | 110 ‘48
Moon II, v.c| (25 '0)| 13 36 9°26 12 16} 113 21
NVirginis - - -| 4 | 14 10 23°48 | S.12 37
Moon If. 13 59 7°69 | S.14 55 | 116 64
Moon II. 1492 51°18 | 17 25 | 120-71
Moon IT. 14 47 26°96 | S.19 46 | 12534 |
Moon IT, 15 13 1700] 21 55 | 130°39 |
Moon IT, 15 39 37°30 | $.23 50 | 135 68
Moon If, 16 7.1726] 25 28 | 140795 |
Moon It. 16 35 58°69 | S.26 47 | 14588
Moon II, 17 5 35°68 27 45 | 150714
Moon If. 17 35 57°98 | 5.28 19 | 15338 1
Moon I, 18 4 24°84 | S.28 27 | 155/29 H
Moon 1. 18 35 3346] 28 9] 155 ‘89
Moon I. 19 6 40°66 | S.27 24 | 155 08
Moon 1. 19 37 30°36 | 26 13 | 15301
Moon I. v.c} (26) | 20 7 49°07
MoonI. te} - - | 20 37 27°22
Momf. v.c) (96) ] 21 6 19°56
Moon I. | 21 34 25-12
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22 28 2880] 1
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22 22 68
22 44 129
22 54 40
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# Geminoruam = -
Moon II, v.c,
San anaceuna
MOONKQULMINATING SFARS. 451
At Greenwich Transit.
? Geminorum
3 Geminorum
-
7 Geminorum
$Geminorum -
Moonll, le} - -
Moon II. v.t] (15 6)
\ Cancri- - - - 6
4 Cancri- - - - 6
@ mms ar
@owrnco So,
Ryereg wa
es
toed
3 Arietis- - -
C Tauri - - -|
47 Geminorum
ec Geminorum
40 Arietis - - -
C Tauri - - -/4.
¢ Geminorum
A Caneri - - -
37 Leonis - - -
4 Leonis - -
X Cancri - -
@ Leonis ~ -
A*Scorpii- -
(237) Scorpii- -
47 Geminorum
2
14
3
7| B Virginis - -/3.
x Libre - - -/5.
« Capricorni -
Mencury- -
¢ Geminorum
37 Leonis - - ~
(84) Sagittarii -
33 Capricorni
« Leonis- -
A* Scorpii -
6 |(237) Scorpii -
7' Sagittarii -
aw Aquarii
x Leonis
Jurrren -
S88 #22 8 B28 Ss
« Cupricorni
t Piscium = -
t' Piscium -
(CCULTATIONS OF PLANETS AND FIXED STARS BY THE MOON,
70 Aquarii
n Piscium -
w Arietis - -
¢ Arietis - -
t' Arietis - -
9 Tauri - - -
d Pleiadum-
x Tauri - -
e Geminorum
x Leonis - -
¢ Arietis - -
x Tauri - -
C Touri - -
47 Gem
(is9yPtachans
‘
‘3
VISIBLE AT GREENWICH.”
aa Hon wn
ow
454 OCCULTATIONS, 1838,'
OCCULTATIONS OF PLANETS AND FIXED STARS BY THE MOO
VISIBLE AT GREENWICH,
Star’s Name,
Piscium -
y Arietis - -
9 Tauri - -
d Pleiadum-
» Tauri - - -
Ff Pleiadum-
h Pleiadum-
C Tauri - -
ec Geminorum
* Star setting, } Star below the horizon,
§ Star rising. + A near approach,
456 _ OCCUPATIONS, 1 B38)
ELEMENTS
for facilitating the Computation of Occultations of certain Stars by the Mos
At Greenwich Mean Time of 6
Star's Name.
d Pleiadum
9 Touri - ~
f Pleiadum
B Tauri - -
C Tauri - -/4.
« Geminor. | 4
v Geminor, | 5
c Geminor. | 6
1 oo or
6/s, 8
7:34 :14°89|N.26 9 59°0)1 Perr
18|N.27 10 49°8|S.45 23] 4
X Cancri - 8] 24 31 40°6|N,33 25] 88
1 Leonis -3.
|
| 9? Geminor. é
|
37Leonis ~ 6
6
4
i Leonis ~
Jurirer 639 05) 65 23/90N.
o Leonis ~ 1112 48°33] 6.54533) 46 18} 90N_.
B Virginis -|3.4 11 42 16°88|N. 2 40 35°3\N.67 50] 90N_
n Virginis -'3.4 15 38 56 13 5674 8.23 19] 22N._
a Scorpii -/'4 | 18 23 22 11 52°8|S. 141)25N._
a Scorpii -| 1/2151 2 4 28\N,2429)49N.
A Ophiuchi |4.5) 16 41 50 21 316 S,69 58} 518.)
3 Sagittarii| 5 | 515 4 % 52785 aaBeae 1} 88.
7 Sagittarii| 5 [11 54 5 " IN.68 26) 60N.
(359)Sagitt.| 5 13 6 9| “1IN, 026) 16N..
@ Sagittarii |4.5) 3 19 25 “8/8, 72 10) 568.
r Sagittarii | 4/1116 3 S. 617)13N,_
« Piscium -| 4 |14 47 54 8.62 43] 11S,
Mar. 1] 3 Arietis -| 4 | 0 25 53 -7|N.75 49) 90.N.
£ Arietis 5 | 15048 “80 |N. "3 /N.12 47) 57 N. ¢
4 Pleiadum /4.5/14 44 52 E 4 °3|S.36 2] 10N. +
e Pleiadum | 5 |14 5257 "| 56 of 12S. 5
c Pleiadum| 5 (15 9 2 E "7| 4737] 2S.)
d Pleiadum | 5 |15 22 35 “LLIN. 1/S.20 9) 25N.)
1] y Tauri - -}| 3 )15 52 12 : " °9|S.24 354] 21N.
1] f Pleiadum | 5 |16 35 32] 3 : 9) 15 1/30N.
3] A Tauri - -| 2 | 93015 2 "2/8.34.56] 9N.
3) C Tauri - -/4.5)20 53 48 9°52IN.2 *5|N49 14] 90N.
ELEMENTS
for facilitating the Computation of Occultations of certain Stars by the Moon.
Greenwich
At Greenwich Mean Time of 3
Day 3
ofthe | Star's Name. | 2 | ‘ppa Diff. of
Month, 2 eof
( and #.
Mar. 4] © Aurige -| 4
q 5] « Geminor. | 4 28 6563) 3227) 11N, 548.
5] v Geminor. | 5 2715 71 041) 44N.
| 6] @ Geminor. | 5 127 10 5148.37 45
| 6] Xcancti -) 6 |18 40 2
i 8] » Leonis -|3.4/19 15 25] 9 58 31°40
Whe is -| 4 |12 8 16)11 12 48°65
| 11] AVirginis -/3.4) 456 g]11 42 17-28|N. 2 40 32-9
11] y Virginis -|3.4 21 45 51]12 11 38°66|N. 0 13 53°6|S.
16] A'Scorpii -) § |12 47 33]15 43 55°00|S.24 50 20
A®Scorpii =| 6 |13 15 55]15 44.57°59| 24.45 316
16](237) Scorpii) 6 |17 8 37]15 53 34°83/S.25 24 32°3
4
1
5
5
ES
17} & Scorpi
17] @ Scorpii -
18] 3 Sagittarii
1 0 5/16 11 22°13/S.25 11 55°6)8.
43153
12 43 50
16 19 30°02
17 37 22°48
26 4 S\N.
27 45 45°3/8.37
40°93/S.29 34 50°1
7 Sagittarii | 5 |19 35 9}1
7
(359) Sagitt. 7
8
1
1
49'91/S.28 28 43.8.
49'64| 2754 2°3/8.13 22
59°83] 20 11 20°8|N.39 57
35°86/S.19 36 7°2\N.36 6)
r Sagittarii
¢ Copricorni
« Copricorni
Mans ~ -|
Mencuny| - | 2
Arietis -) 5 |11
Pleiadum |4.5) 23 5:
34°66/S. 1 32 59'3
20°49)S. 131 314 5
35°48|N.20 26 27 2N.
15°34|N.23 36 1'8)S. $0 49] 16N.
C Tauri - -|4.5)
«Auriga -| 4
7
Seasin
Apr. 1] 47 Geminor.
« Geminor,
v Geminor.
Geminor.
=BS5
| asasres Shwe weew weow
27 34 10°62)
271
26 10
5
5
5
5 8'29/N.29 33 15"
23744] 516 3°06] 2828 06
15/N.97 10 5:
4) 328 45) 7 15 39'92/N.28
753 14] 7 25 5641
5/15 34.38] 7 43 35°
5
7 3] 9 58 S0°93/N.1
1350 3/10 8 0°00
140 36]11 12 48'49
+418 29 7]11 42:17°26,N.
8
7S.
8.4)11 17 10} 12 11 38°7:
Libre - -/5.6)12 28 16/1
~| 5/18 23 36]1
Rsscorpii
13] @ Seorpii -) 4
13] @ Scorpii -| 1.}10 5 54] 1
14] 8 Sagittarii
15] 7'Sagittarii
7 Sagittarii | 4
18] «© Capricorni) 5 |1
18] « Capricorni) 5 |i
Mexcury| -
25] ¢ Pleindum | 5 |10 1
25] ¢ Pleiadum | 5 |10 2:
25] d Pleisdum | 5 }10 4
25) y Tawi - -| 3.)11 1
15 |(359) Sugitt.
12
12
16
23:
2
au
=
=
a
Zz
=
a
”
a
-m
"a
2
a
3
=
=
ry
i
me
~
1
a
27] © Tauri ~ -/4.5)13 26 45) 543 8°65
27| « Aurigw +) 4 |22 15 22] 6
27| 8 Touri - -| 2
Geminor.
29] v Geminor.
29] ¢ Geminor. | 6 |11 28 50] 7 34 13°84
29] Geminor.
May 2] 7 Leonis
2g] «
-/3.4) 84
4] ¢Leonis -
4] B Virginis
2/37Leonis -| 6
=| 5 | 0 43 53) 15 43 56'2'
Scorpii -) 4 )12 44 6/16 11 23°50
10] @Seorpit -) 1 )16 12 45}16 19 3143
5] 9 Virginis
10] A*Scorpii
10} o@
460
} Day
| of the
| J] Month,
aoaun
Wass wows
ee
OCCULTATIONS, 1838.
ELEMENTS |
for facilitating the Computation of Oceultations of certain Stars by the Moo
At Greenwich Mean Time of 6
Star's Name.
«€ Piscium -
« Arictis
Arietis
Pleiadum
¢ Pleiadum
¢ Pleiadum
d Pleiadum
» Tauri - -
f Pleiadum
@ Geminor.
x Leonis
Dig UPITER ~
3 Sagittarii
7‘ Sagittarii
(359) Sagitt.
@ Sagittarii
7 Sagittari
9 Capricorni
¢ Capricorni|
+y Cupricorni)
« Capricorni
3 Capricorni
« Aquarii -'
Aquarii
t Piscium
« Piscium
¢'Piscium
¢ Avietis
¢ Arictis
a
ll
dae
PIC
a
ae
wo
& gees
“=
=
Sawn wong
Oe
2
Ssu0k
aS
wweow
uo
ew weoe
ee
oe
«e
3.2847
16 17 57
17 30 25
5 22 56
B45 42
16 410
2244 14
23 56 37
14 16 57
22 20 29
20 21 59
9 55 18
11 13 38
12 16 52
1410 51
223511
5 1224
14.47 25
8 40 50
13.47 18
M4 121
20 5415
xr
and 4.
11 12 48°00
11 42 16°80
12 11 38°36
13 16 41°65
15 43 56°61
16 11 23°98
16 19 31°96
17 37 25°13
17 54.43°77
17 57 52°75
18 35 35°39
18 56 52°82
20 55 13°75
2128 3°16
2131 935
21 33 39°18
2138 8°28
2157 43°64
23 5 58°26
017 7°46
0 54 34°23,
1 5 18°06
2 49 58°75
3 537°16
ate ay 19°97}!
235
23°26 ies
N.23 36 29/8
23. 33 15°9/8
27 10 5274/8
8 12 36°1|N.61
N. 7.54 1°91N.69 11] 90N..
IN. 6 54 56°1\N.14 59] GON.
240 36°2|N.35 14] 86N.
IN. 0 13 56°3|S.56 18] 11S.
5.10 19 0°2'N.61 23] 50 N.
S.24 50 27721N.63 53] 65 N.
25.12 1°7/S.12 36] 15 N.
26 4 11°5/N.14 36] 38 Ne
S,27 45 4779|8.29 2} 9S.
S,29 84 52°4/N.70 34] 60.N.
2828 SQN. 258) 17N.
27 9 Vals 6089 438.
S.27 53 59°2/N, 3
8.20 29 18°1)S.79
2011 5°0\N,
17 23 129 S.
8.19 35 5171
8.16 5
S. 6 5:
ee2e Suze
eff. S880
Urge sue &
Zon znam zy
-225 SS58
Bees teese
ESke
w ar
SSSR Sahu,
Ss »
seus S28
-
aon
2715 49/8.12 2
IN.27 10 49'4 ier
6545
3.58 5215/5. 1a 3
IN, 240 38°L NUE .
Te ae lee
"O1) 2450
99 ot se dou is.
5/825 12 18/834 57 “os
3
“4
"43/5.26° 4 1178/8, 7 26 sl oN.
82] 27 45-49°6|S. 45. 258.
"53| 2934 54°7/N.54
359) Sagitt.) 7 52°51/S.28 28 7'9/S.12 8
+ Sagittarii 56 52°85|S.2754 1°5/S. 7 87] 13d
» Capricorni 55 14°32) 20 29 17°6|S. 79 50] 54
# Capricorni 26 3°88) 2011 4:0/N75. Tom
7o
e
4
40
57
35°
4
16
16"
@ Virginie -| 1 | 7 22 59
A'Scorpii =| 5/10 39 89
3
5
5
5
3
2
4
@
6
3
9
1
7 Capricorn 31 10°06/S.17 23 Lo"9|S. 74
50)
43
1 33 39°92/S. 19 85 49'7|N.72 &
2138 9°03} 1651 16:08. 65 81]
on 7]21 57 44°47| 14.38 53'5|S. 75 89) 3
12 13 53/22 40 @-42|S,1124 g:2i\N.e4
al
2835 46/23 5 59°33/S, 654 55°0|S. #
14 34 29]23 39 39°68/S, 3.39 16°5\N.
0 18 41] 0 54 35°68IN. 7 1 21°5|S. 4
¥ Atictis. -| 6/1455 20] © 21 58°45|N.16 59 25°3|N,19
OCCULTATIONS, 1838. 463
| ELEMENTS
for facilitating the Computation of Occultations of certain Stars by the Moon,
At Greenwich Mean Time of 6
a} bom
39] 250
10] 3 5
: 13] 335
5 57| 335
5 ae] 336
5 20] 3.36
3 ai] 337
5 11} 3.39
6 4i2 25 14 41°6|N.89 19
2 516 28 28 0°6/S.15 15] 29
zi 543
« Aurige =| 4 6 5.
# Geminor. | 4 |1610 31] 71
5 |20 3641] 7 2
5 | 42039] 74)
6 |16.37 47] 61
15.17 58
1333 4
15 58 22
17 12 28
ou:
w Scorpii -|a.4/19 85 49
a@ Seorpii -| 4 | 5 43.37
a Scorpii =| 1) 921 9
3 Sugittarii | 5 |18 31 11
7 Sagittarii
conne
SREB weeS
secu &
=
mow
4
1
5
5
5
4
5
4
5
« Capricorni
b Capricornis 4
« Aquarii -/4,5)
50 Aquatii -) 6
Aquarii -| 5
x Aquarii 6
¢ Piscium
ome
-—ow oer
se
wash
ao _
att
=———
Day
Star's Name, | =
Cer AACS agus
eeo0
B Virginis -
Juriren -
A'Seorpii -
eee
=Sau
S55>
y' Sagittarii
359) Sagitt.
v Sagittarii
a Sagittaril
y Capricorni|
© Capricorni!
y Capricorni)
® Capricocni
$ Capricorni
3.4
5
3.4
4
1
5
5
ELEMENTS
for facilitating the Computation of Occultations of certain Stars by |
At Greenwich Mean Time of 3
SSa4u sous wesese wow,
-_ = _)
eG5h Guba G4RR FSu8,
11 42 16°89
12 17 50°65 |
15 43 55°36
1549 5°31
11 22 34/16 11 22°71
15 025/16 19
0 23 58]17 37 23°93
7 34 36/17 54 42°60
852 3517 57 51°59
9 2AQTIS 56 51°95
630 26/19 49 7°40
10 19 33]20 55 13°72
2128 3°38
2131 9°59
2133 39°45
2138 8758
2157 44°19|S.
7]22 40 2°24
2038 5/23 5 59°29
12 6 54]23 39 39°79
M
Laas
Sebe.
Ske
BS 288
é
Sees
Less o8F2 8
het
za
ow oat S882 S885 Ses,
See-
Le
$3
5G
24 50 239)
'S.25 38 37°5IN
‘3.25 11 59°3/S,36 18] 8S.
8.2828 777/S.1235] SN)
2754 28|S. 651 ere
26 37 40'7|N.32 59]56.N.
$.20 29 20'4/S.77 37155, |
S.2011 7'2|N.77 4a]7ON. |
17 23 13'6|S.72 241358,
19 35 53°0/N. Ne
gael 18°7 8.62 5 ne |
IS. 72 55]33S,
N. 66N.
4
OCCULTATIONS, 1838.
abi Bind voiaia
3 S885 S194"s sss¢
2 ZEAA 4 AALR Bae
3 S578 CECE RES
= ars Esse” eats
tis RACR 2 $253 2327
2 ZAGE i we ZAZA
SI 9 Shear Vere
a B32s Se SEE
| 2 mass 24nR ©2732
3/4 SaR2 gare aFar
2 Z ee
3 i $235 BRAS BSRR BB33
i Ba2e ghar BEES
3 = sone 2en8
a a neue, Ssam
3/32 =a>a —
- wees ae
ii ssa haldinsd= he teh
8 oon ied wine |
a j ae fe oad SEES
a ssf s1i5 Ae
3 3 feed aad ae |
wee CUR, RO oa nes 2
& 2 Soy PSan 2222 |
3
-
i
if
a
i
of
Apparent
owk.A.
ce
=
ie
ofthe ] Star's Name,
Month.
x Leonis -/4.5)
o Leonig -) 4/1
0°62
7:06) 3
$'37|N. ;
225/810 19 25/1
4/21 57 43°50
8/22 22 6°86
21) ¢ Aquarii -
21} @ Aquarii -| 5/1
Cena ee?
token -
‘Tauri - -
é Pleiadum
é Pleisdum
c¢ Pleiadum
d Pleiadum
a Tauri - -
T Pleiadum
A Pleiadum
B Tauri - -
© Tauri = -
«Auriga -
4 Geminor.
v Geminor.
¢ Geminor.
Geminor.
4.5)12 46 11
5
5
5
3
5
2
4,5)14.30 6
a
4
5
6
5
5.6) 14 29 58
for facilitating the Computation of Occultations of certain Stars by the Moon.
1253 45
13 8 50
13 21 31
13 49 14
14 29 47
4914
2253 33
234 0
643 47
10 7 22
13 59 31
UCOULTATIONS, 1838. 467,
ELEMENTS
At Greenwich Meay Time of 6
5
~
F.
Bb
ie
S22e.
BES VWHUAS CISH Sere cH
Sek
P POVD nny nnnm
Sy
£eas
ZAZZZ
ewe
1641
Pr ae
Be whee ©
ZZZZ
2 22 8
wm
ewe www we
SERS
27 34.115 \N,
1.29 33 12°6)5.
BSas anon =
2352
‘92IN.28 6 16°6
; 27 14 56°
26 9 49°
per 10 39°35 |S.
MMM OUMe wees weEwe Krol
en
ae Dw
Sees
ehBS
L—A Tolal Eclipse of the SUN, March 25, 1838, invisible at Greenwich.
Begins on the Earth generally March 25" 7* 338, Mean Time at Greenwich,
Longitude 161° 9’ E. of Greenwich. Latitude 58° 25'S.
Central and Total Eclipse begins generally - - March 25* §* 44-2
Longitude 149° 12’ E, of Greenwich, Latitude 77° 45’ 8.
Central and Total Eclipse at Noon - - March 25 Q* g™1. |
Longitude 135° 46’ W. of Greenwich. Latitude 57° 38° 5.
Central and Total Eclipse ends generally - - Mareh 234 11" om).
Longitude 74° 11’ W. of Greenwich. Latitude 19° 56'S. |
Ends on the Earth generally - - - - March 25° 12" 10™5, |
Longitude 91° 6' W. of Greenwich, Latitude 0° 20° S.
TRACK OF THE MOON'S SHADOW AND PENUMBRA UPON THE
SURFACE OF THE EARTH, DURING THE SOLAR ECLIPSE
OF MARCH 25, 1838,
iene eee ase
i
|
|
|
|
—
sOUTHERN
OcEAN,
ia
IL—A Partial Eclipse of the MOON, April 9, 1838, visible at Groenwich,
b
First contact with Penumbra, at - - 11 108
contact with dark Shadow - - - 12 32°1
ies reas tee Mean Time at
Lost contact with dark Shadow - - - 15 2571 | Greenwich,
Last contact with Penumbra - - - - 16 464 |
Magnitude of the Eclipse (Moon's diameter =1) 0°603, on the Northern limb.
At these times respectively the Moon will be in the Zenith of the places whose |
positions are,
, o ’
Longitude 11 14 E, Latitude
8 32 w.|
29 34 of Greenwich,
50 35 j
jo 21 W.
‘first contact with Shadow 76°, towards the East,
Inst contact with Shadow 20°, towards the West,
Angle from North Pote of {
T1I.—An Annular Ectipe of the SUN, Sept, 18, 1838, invisible al Groemvich.
Begins on the Eorth generally Sept, 18" 6° 21™8, Mean Time at Greenwich.
Longitude 169° 24’ E. of Greenwich. Latitude 63° 40’ N. |
Central and Annular Eclipee begins generully =" = Sept. 18¢ @* 1™1,
Longitade 38° 32/ E, of Greenwich. Latitada= 87° 2
Cantidad Annalee Eclipes ends gealisees eau
Longitude 57° 39’ W. of Greenwich.
Ends on the Earth generally -
Longitude 83° $1 W. of
TRACK OF THE MOON'S PENUMBRA UPON
OF THE EARTH DURING THE ;
OF § ER 18, 1838.
ft
J
j
IVA Partial Eclipse of the MOON, Oct, 3, 1888, &utdible @t Greomtoiele
= et *
First contact with Penumbra, at - - Py ny
First contact with dark Shadow- - - 1 10°2
Middle of Eclipse
Last contact with dark Shadow- - - 4 1271
Last contact with Penumbra - - - - 5 11-2
Magnitude of the Eclipse (Moon's diameter =1) 0°928, on the Sou
positions are,
Longitude 192°
158
136
ll¢
100
first contact with Shadow 98°, towaitls the Bast,
Sele fame Rene Bole of { last. contéct with Shadow 149°, tawardls the West,
ELEMENTS OF THE ECLIPSES OF THE SUN.
nA 4nd : peeereyee +t
'
ee
wea anBuabe dia,
GEASS RGA GW
mm
9
CF
1
54
33
2
18
0
61
16
16
*s "True Semidiameter ~~
O's True Semidiameter = -
"
wOVrqvorver ov
Seer scree oof
PMH AS & we
PHENOMENA, 1838,
Rew Ge tae
el oe
a
eee a,
=
eat
ae
RSsBeeaan
AKKCOFOKAT
DONA we ee
Os ot x 40 SH Oy Os HO He LK st
OOF
HOZARAOA
$$ --- ¥321N,
96 XAquari * 1 188.
ud€ --- % 1128.
Mad sPiscium * 0 31 N,
3 in Inf dO
hd€ --- k 536N,
% greatest Hel, Lat. N,
dC --- ¥ 838N,
3d¥Serpentis * 0 25S,
$6C€ --- $336N,
HdC --- H24iN,
& greatest Hel, Lat, 8,
Q9dC --- 26 ON.
@ at greatest brilliancy,
§ Stationary.
2
we
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8
5
1
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3
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FON HO He Otc a StH Hee BE SI O90 0 Ke tee
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FEBRUARY,
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hd Libre 2 1 25'N,
$6 oCeti * 0 48N,
? Stationary.
ud clLeonis * 0 19N.
ud€ --- %! 5S.
2 in Perihelion,
% greatest clong. 26 10 W.
+ & o Serpentis * 0 57S.
Sind
oF
é6€@ --- $034N.
eclip., inyis. at Greenwich.
6€ --- §$o2s.
é$Eridani * 1 475.
in Sup, d ©
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°
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t
%
“HOC --- %1385S,
€ eclipsed, vis. at Greenwich.
% in Perihelion.
Q at greatest brilliancy.
hd 6Libre * 1 13N.
msy --- 661858
¢ 6 oEridani * 1 125.
hé@ --- hk 616N.
$CTauri *0 2S.
ou
3¢
Sa
en-we8sua
FOr HOC HD HOCK te Oy +0 HOC ET +01
HHEK™ HYVHO
wreonrR RK
toh om
13 16 39
1610 6
1616 0
16 20 37
17 310
17 12 29
19 18 45
20 715
21°19 59
22 547
22 914
22.15 55
2320 3
2419 2
27 22 47
29 7 53
30 19 12
31 6 50
31 18 12
Sind
k8O
hdqLibe * 1 45N.|
td nOrionis *1 08
¥% inInf dO
oa
Lal
'
'
‘
HOR RHO [Kt 0 pe Ore 1
an0on,00F 000K a0
-
BR xk mx¥O XO
- = = ecoscvo-w
& wB oBSeotSn
4 2 PR PARMAMKRY
*%
°
&
2 in Aphelion.
€ d+ Geminor * 0
hd€ -+-+ kb
——————————
=o wemon enepes
ers
REKEEDE HR took amok ee
ne OL He
BF RENMYMOND LAO YY eH Te UUs
DomvoeDAwe veo ssn 0p bo
Bt Fo 70+ 90] ab G+ +201 FO OF = Fo OF 1] 201 201 OF at 201 FO
PSshoSeaeeoa ras sssesenee
“2m ART Oe RomonrIaaMsoH- ome
+] > 2
WaeGaeneases lie |'re re Seeecke sivas
HH ore oro. or orton
i te a ete
=
Sanaananoon
Aaa
BAS
2K OR RRS 3
3 14Ous 2
x EESERI Cries ones
al ‘Estee (gtr ee (1384
= Sas z Be eee
ig Se~nth we wm moe ~ SOuvee
Evv0Zov0vtvve, hove v Vv.
Wh LD NO.OF 204 OF Ot E94 204 Ce DL] #0 OF 204 +++ HOM] OF OF
ye@
| SPRPSSSLSSSCRERSTESSLS5
EP OM ACH SSAD OO” MOS a or
—— = ceelien | oe oom
= | sceeesed
| DECEMBER.
4b of
lo2stl4 ¥dC --- RON,
11 219 Qin’
12 1634 $d eSagitt. * 1178S.
142345 kRd@d --- k 623N,
11612 0 9d --- 2 446N
17 9 4 ¥& greatest elong. 20 10 BE.
18 215 QinSupdO
18 3 6 ¥dCq --- ¥3I6N.
201019 6m --- Glo ON.
fo)
ahs
2123 9 Hd -
23 342 469
2420 4 ¥Y Stationary.
23 446 SinQ-
26 326 Wd dAquarii * 0 25
27 0 0 @ greatest
27 10 39 bd y Ophiuchi * 0 1
29 138 48&oO -
2918 13 % in Perihelion,
sini
2 © in Perigee. ]
|
|
SATURN'S RING,
ELEMENTS FOR DETERMINING THE GEOCENTRIC POSITION,
MAGNITUDE, AND APPEARANCE OF SATURN'S RING.
————_ ———— -
1838. 5 ” ” ot oF
Jon. 1 |+231°9 35°38 414°37 | 423 57°99 | +23 58°0
Feb. 10 2 55'3 3746 15°47 24 234 2423-5)
Mar. 22 2587 4000 16°49 24 20°97 24206
May 1 2 42°5 41°74 16°93 23 55°] 23 as |
June 10 21911 41749 16-49 23 24°9 23 24-7
July 20 2 60 89°47 15 ‘56 23130 23 130
Aug. 29 212°9 36°95 14°77 23.33°8 | 23 33-7
Oct. 8 2 38°1 35°01 1441 24186 2418-7)
Noy, 17 3142 34°17 14°51 23 80 25 80
Dec. 27 8 51°3 34°61 1503 25 44°6 25 44°7
— 31 |+3 547 34°72 | 415711 | +25 47°2 | +25 473
p denotes the inclination of the Northern semi-minor axis of the Ring to the
circle of Declination; + East, — West.
a the major axis of the Ring.
b the minor axis; + North surface visible,
| — South surface visible.
tthe elevation of the Earth above the plane of the Ring, a8 seen from
Saturn; -+ North, — South. é
V the elevation of the Sun above the plane of the Ring, as seen from Saturn;
+ North, — South,
| Suowixe tae Mean Tive or tHe orearest Lisnation or raz Moon's
Arrarext Disc,
‘The Moon's Libration is here supposed to
take place in the plane of her Orbit:—and by
the time of the greatest Libration of her Ap-
parent Dise is to be understood the instant at
which, to an observer at the centre of the
Eurth, the variation of the Dise from its mean
state has attained its maximum.
Nahangn<
‘The right-hand column indicates the qua-
drant of the Moon's Dise in which the Li-
bration takes place, and in which the greatest
change of the Moon's surface will become
visible,
8.
Ss.
8.
Ss.
8.
8.
Ss.
8.
8.
8.
N.
8.
5.
8.
Ss.
8,
8.
5.
8.
N.
N.
N.
N.
N.
N.
N.
N.
Shen an ansnansnsnan=
TABLE,
Suowine vax Itcumsarep pontion or THe Discs or Vexus anp Mans.
|
]
rs
SSe saw
‘eo 220 Deo
33] 6 33)
a3
9
4zfio
1g}it
Ad} o
a
31/13 51 H
2 36/14 4¢
3 ets 16|
3 80/15 45
ell 4 1161
1 437/16
28/17 5 15|17 3
5918 19 17] 6 ajis 29]
40/19 2) | 6 e7h9 af
2719 56 87) 8 1721 2
35/21 20 36] 9 4922 33
g)22 55 as}ll 4
40) — 47, — fied 13
17112 48 0 3713 0 M4
18 12213 44 i
11)l4 33 2 Sid 26 ib
sats 16] 1 aging 21} 2 age. 9 I
37 32|14 52] 3 2615 \
18 1215 32] 4 716 28) ui
56 351/16 11] 4 497 a1 518
-|- 4 30/16 49 ee
-|- 5 917 80) 6 19118 44
-l- 5 S218 14)- -]- -
Tf the time of High Water be required, according to the civil mode 6
1, For the Morning Tide:—With the day of the month
take the time opposite thereto from the 2nd column of the month,
12 hours.
i
2, For the Afternoon Tide :—With the given date, take the inert
from the Ist column of the month.
ob,
480 TIDES.
‘TIME or HIGH WATER, ox raz FULL anv CHA
AT THE UNDERMENTIONED Ponts axp Praces.
Beachy (on Shore) England-
| Beachy (Offing) England-
Beaumari: Wales -
| hom
Aberdeen Bar ote = L 12
Aberdovy - = - 7 30
| Abe: - Wales = = i 30
Achill Head - Treland - = 0
Agnes (St.) = Scilly Isles - 410
Air Point- - Isleof Man- -10 30)
Aldborough - a = -10 45
Al Pier English Channel 6 45
Alne River - England - - 2 45
| Amlwick Port Ang - -10 30
Antwerp = Netherlands- 4 25|Cuckold’s Point
ArranIsle- - Scotland- = 1 15\Cuxhaven =~
Arundel Bar = England- = - 11 15|,.
Balla- - - Shetland 3 0/Deal
Baltimore- - Ireland - 3
Banff - + + — Scotland- 1
Bantry Bay - Ireland - 3
Barmouth- - Wales - 7
|
|
| Belfast. - - Ireland =
ae ie a Ce mi le) a
Cancale Bay - France - - - 6 0/Galloway
|) Berwick - - England- H - lay
Blakeney Harbour England- - Lights- NorthSea -
Blythe - - England- - 2 45| Dun! <2 con -
Bolt Head - England- - 5 55|Du Head §
Boston - - England- - 7 15|Dundalk Bay- - Ireland - —
Boulogne - - France - -10 50|Dundee - - - Scotland- ~
Brassa Sound- = ShetJand- -10 0)Dungarvon + + Ireland - =
Bree Bank - North Sea - - 3 30) Dun - + England- ~
os Bell) (ieee: a ee
| Bris ater ~ mg - - 45 a
Bridlington - ae + = 0) eoaraiones ae es
r Exmouth Bar- = =
Brid, > + England- - 6 Evemouth i
Brighton - - England- - -19 5) semouuh = = tae
Brielle - - Netherlands- - 3 0)Falmouth- - - England- —
Bristol - - England- - - 6 45|Flamboro' Head- England ~
Brouwershaven Netherlands- - 2 0|Flatholm- - = England =
Buchan Ness - Scotland- - -12 0) Flats (Kentish) - wland ~
Burnt Island - Scotland- - - 2 30|/Flushing- - = Ne -
Cairston - - Orkneys- - - 9 0 reve ae Pocaed 2 i
Calais- -_- France - - -11 30 Fowey - - - England- =
Caldy Island - W.C.of England 6 0 y
| Canela + St. Geo. Channel 10 30/Galloper - = =
ft
vee
i
&
i
[
7a
ie
&
i
Q\Grevelmes- = =
i
EB or HIGH WATER, ox tus FULL ano CHANGE or 11x MOON,
AT THE UNDERMENTIONED Ponts ann Pxacks.
h h
esend - - England - - 130|Plymouth Dock Yard England- - 5 33]
nock - - W,C,of Scotland 11 45) Portland Race- - England- - 9 15
‘nsey Pier - English Channel 6 30) Portland Road~ - England- - 6 15
fleet - - River Thames -12 ©|Port Patrick - - Scotland- -11 0
ae Eland — g 4g {Portsmouth Dock Ya. England- 11 40
vich ~~ - -11 30
RathlinI.,ChurchBay N.C, of Irel. 9
. Beans ey a 719 36) Ramsiate Harbour Peaciaai -11 46
aren ee - - 10 80) Rye Harbour - - England- -10 40)
n’s (St) - ane -11 0
>: rman an-11 0
evoetsluis - Holland- - - 2 0 [see cs gh a Eacad © i inte
ees aes = =) = 16 Oe Scilly Islands - - England- - 4 10
‘Point - Jutland - -12 Olccd - - - Enmpland- -10 15
th Harbour Treland = > =11 8 \Selsea Harbour - England = -11 15
oe od > = © °/Shannon Mouth - Ireland - = $ 45
ther River- England - - 5 30/SheernessDock Yard England- - 0 39
ich - - England - -12 ©/Shields- - - - England- - 3 0
de Bas- - France - - + 3 17|Skerries - - - Ireland - - 4 45
ty(St.Aubin's) English Channel 6 10 a Bay- - - Srelaod - - 645
ai bay - - - England- -10 30
fo ebatae Mice eee LAY Southampto - - England- -1) 40
lish Knock River Thames - 11 30 Spithead - - - England- - 9 30
fs Road - BristolChannel- 6 45 Spurn Point - - England- - 5 20
ale Harbour Ireland - - “wa leigh ae England- - 4 30
cudbright - Scotland - -11 is\erMra, | 2 2 Brae 2 268
YsEnd - England - - 4 30/Stromness- - - Orkneys - -10 30
h Pier - - Scotland - - 2 20|Sunderland - - England- - 3 0
tick Harbour Shetland - ~- 9 45|Swansea Bay - - Wales - - 5 56
is Islands - Scotland - - 6 0|Swin - - - - RiverThamesiz 0
rpool Dock England - -11 2 |
ton Bridge- River Thames - 2 7|Tay Bar - - - - 145
ghCarlingford Ireland - - -11 Terschelling 7, a - 3 30
Pier - England - -11 sree + aa
WaWareakouWaee > 2. 6 boomy ged a -9 |
trose - - Scotland - - 1 Bish ‘eam
laix- - - N.C.of France 5 345
nts Bay - England = + 4 2 50
les Point - Isle of Wight - 9
castle - - England - - 4
pot - - Wales - - - 6
port - - France ~ - -11
+ Light - River Thames - 1
tdness- - England - -10
eae - Scotland - -10
> - > Flanders - - 0
broke Dock Yd. Wales - - - 6
Jand Frith- Scotland
'
-
i}
4
om
Om BHAT
nos BROOD
Toman -=4o BEN
fona sae Sonn |
[fo~a wwe secs |
18|18
19}19
19) 19
18) 18
17)17
17)18)
15}16)16)17)17
16
17
17
SECOND DIFFERENCES,
In finding the Greenwich ‘Time corresponding to a reduced Lunar
4
5
6
6
j14|15)
15)15
'
The Correction given in this Table is to be added to the approximate Gre
Time when the Proportional Logarithms in the Ephemeris are d
| subtracted when they are éncreaving,
2 © /13)13/14)1
1 50 14
1 30 [14)15)16
1 40 [14
8
g
:
=)
o
2
=
BB
S
F
°
a
0
10
30
a
4d
1
1
#ogoRo R= ROR ORORO ROA sogog0 “guseenneossae
“a 22 2s 52 2 3 a e ™ x Serer sit eon oe |
_ =
Te Osaka eeassesanas?*
“sesesossesoscesesesescoesces
5
SE“SaRseesee2
"“SSrmrmnmenssoss
Smmonm moron oe mse reseeeanié
AAMT cd ——_
“eceesesesoossseoesssoessoosso
peRseasaaegaecnagcansesso*
“sesecsccoscsoosesososoossoossosososco
Fae code n othe Sorerse seston
SH Ora cet
“sseoesossossssosssososessesos
Fasesmomrmomanaesssaranmsrnns
ee Seees
“seocoosooscecsoosesssosescossosescs
Fa SoSSHuataemaocnamandnonmenan
BSASSAASe
TABLE IIL. (for 1838.)
Containing the Third Correction, (always to be added.)
“seseccoceesssoseesessoocecsece|es
Arguments :-—Sidereal Time and Date.
FosoocoonmaratmoooRnooKn sana sS
"esseoeosesesseessesessessoess
Secsccosocecosseoescceosscesesses
j
j
|
:
Arguments :—Sidereal Time and Approximate Latitude.
“eoessoossoosssossssoesosessoso
‘
SB BBO RO ROR BORIS
*o =
TABLE WU.
Approximate Latitude
s -
og | BPOMERRRAS~SaRsSRlPsa-sas
“a eo + » S&S & ~
s'S 22 = =
.
bcd
n+oPRenee os
“ssoossosoneat
WFSSSSSSSSCHHKARKRAANRAAAM KM SSS
3
AHSRSHAHAH MAA AAMBOHMSTED
amt aoe = aw oe
“SOSSSSSOH HH HMARARAHM KM SSSS
°8
=
wHoummegrsmRasesssaarssas®
TSOSSCOOCOSOK RAR MRAM OSOSS
=
oo aan Co 2 eensewrte tS
STORRS SSTSARSRAC asa
WSSSSSSOSS SSM MR MOOS SSS
Am OR MR OEE OO TOTO TIME ee ATA
—— ohm Conte! 2m Salad
ecesssoseseseSo ose ew swanmmooooscoso
TABLE III. (for 1888.)
Me ORF OHM RM OMTIAAMMOMBDoaroSH
amare ANTIK ae
"essescsoessossoeoseonennseseseseo
Containing the Second Correction, (always to be added.)
Arguments :—Sidereal Time and Approximate Latitude,
“8
Fosoessoeceoessseseosesssses
i
|" 2:2
Fae CoM RB DOMae aang onosrm
ser
SK HARSHER OR TH
Containing the Third Correction, (always to be added.)
Arguments :—Sidereal Time and Date.
“eooscoscoscosooooesoossseoesose
fo nm uwreenvworereaces28
24 3 56°5554
8S S8h 2
TABLE
For converting Ixreavars of Mzas Souan Time into Equivalent Ixrenvars
FRACTIONS OF SECONDS.
viz. January 2 = - -- --- 18 46 42-1]
m
2 01971
aes
She
»
223 dic
i
=
‘The Sum is the Sidercal Time required, 21 9 31412
@ da¢
0
0
0
o
o
o
0
o
o
o
o
0
o
o
o
BS
12 57 52°2157|
13 57 42°3862
14 57 32°5566
15 57 22-7270
16 57 12°8975
17 57 3°0679
18 56 53°2384
19 56. 43°4088)
20 56 33°5792
21 56 23°7497
22 56 13°9201
23.56 40906
12 57'8703
13 57°7064
89 53-4470
40 53°2831
41 5371193
42 529555
49 51°8087
50 516449
57 50°4981
For converting Inrenvars of Sipenear Time into Equivalent Intervars of
Mean Soran Time.
FRACTIONS OF SECONDS,
000997 0"33907 0-66817
001995 | 0~ 0*34904 0 67814
0 02992 | 0° 0 °35902 0 68812
003989 0 *36899 0 69809
0 04986 | 0-38 | 0737896 0°70806
005984 | 0°39 | 0°38894 | 0-72 | 071803
006981 | 0-40 | 0 "39891 | 0-73 | 0 "72801
007978 0740888 | 0-74 | 0 73798
»| 008975 | 0-42 | 041885 0°74795
009973 0 42883 0 °75793
0°10970 | 0~ 0 43880 0 -76790
0*11967 044877 | 0°78 | 0°77787
tho Equivalent
Sn Intervals, |
0712965 | 0-46 | 045874 | 0°79 | 0°78784
0 *13962 | 0- 046872 | 0° 0 °79782
0714959 0 -47869 | 0°81 | 0°80779
0 15956 | 0 0 “48866 0 °81776
016954 | 0°50 | 049864
0717951 | 0° 0 *50861
0 °18948 0 ‘51858
O'1994S 052855
020943 053853
22s
} aie
Mean
ling Sidereal Noon, viz. = - « - + Je
O12 fi
‘The Sum is the Mean Time required, Jan. 2 2 22 25-62
ro
9
3
the
peal Hierro
0 22937 | o- 05584
0 23934 [0°57 | 0 Sésa4
024932 0 57842
6 °25929 IM! 0 58839
0 -26926 0 59836
027924 0 60833
0 “28921 0 61831
o-29918 | 07
0 *30915
O-S1913
0 -32910
= Mean Time at the preceding Sidereal Noon + the Equivalent to the given Sidereal Time.
convert 21 9 31*12 Sidereal Time st Greenwich, Jan. 2, 1838, into Mean Time.
=|
Thi ‘Tante is nseful for the conversion of Sroxnx1. into Mzax Soran Time.
eee ¥ée S82
LATITUDES AND LONGITUDES OF ‘THE PRINCIPAT.
OBSERVATORIES.
‘The Longitudes are reckoned from the Meridian of Greenwich.
North Latitudes and #¥est Longitudes are indicated by the sign +
South Latitudes and Kast Longitudes by the sign —.
Asausem'---- > (fatal Cologa “e
Long. + 0° Bebop fst Alok, wo x. page 211,
Ano - - - = + Lat. + 60° 26'57" Argolaniler’s ;
aid vi gen
Long. 1° 29" 8''8 . Nach. vol. ix. page
Acrona - = = + (Prof. Schumacher.) rv @
Lat. 53° ar a pa ae
Long. — 0 Seas Sta Need a vol. viii. page 1 #
Lat. + 54° 21' 12°] |Communicated by the
Tionkack ped f Robinson. te
Anmacn = =
Beprorp - - = (Capt. Smyth, RN.)
Lat, +e 3° 276
Donkoaoe® i 5( 97 [lem Ast, Soe. vol, ¥. page 3
Bextun - - = = Lat. + 52° 31' 135 Berliner Astron. Jalirbuch
Long. — 0" 53™35°'5 1833, page 249,
(Mr. Maclear.)
Lat. 4 52° 5/ 25!
Long. 0” 1" 315 } atom. Ast, Soe. vol. v. page 3}
(Dr. Olbers.)
Lat. + 53° 4’ 36” — Ast, Nach, vol.i, 240,
Long. 0” 35"15°-9 This is the mean of the r
given in Ast, Nach. vol. i. page 2404 vol. iy,
392; vol. v. page 247; vol. viii. pases 1BL apg
BicGieswapr- =
S
z=
&
=
I
z
‘
’
‘
Bupa - = - = ; Cosa ; "2 Zeitschrift
at. + 47° 29° 12""2 its deine
page 70; and Mem. Ast. ei page 2
Long, — " 16" 127 Zach's
page 2685 and Zetischrift fiir Astronomie,
page 507. : :
(Colonel Beaufoy.)
Lat. + 51° 37 443 rok.
Long. £0» te 30's Mem. Ast, Sr, vol. i page 1
Busoey Hearn
LATITUDES AND LONGITUDES OF THE PRINCIPAL
OBSERVATORIES.
> > Lat. + 52° 12’ 50-7 Airy's Observations, vol.i. 87. |}
Lag eh ghee tee Goat Pan ae ieee |
(Airy on the Long, of the Cambridge Observatory.) |
are or Goov Hore - Lat. = 33° 56’ 3”
RISTIANA
OPENHAGEN
kacow =
fonrat -
Bun +
LORENCE ~
‘RNEVYA =
Long. — 1" 13"55*-0
> Lat. + 59° 5a’ 5”
Long. — 0° 42" sg" 8
- (University)
+ 55° 40’ 53”
Long. — 0" 50" 19**8
= Lat. + 50° 9° 497
Long. — 1" 19" 59° 745
- Lat, -+ 58° @2’ 47”
Long. — 1" 46"55*
+ Lat. + 53° 23’ 13”
Long. + 0° 25" 22"
- Lat. + 55° 57’ 20”
Long. + 0° 12" 43" 6
~ (St. Giovanni.)
Lat. + 43° 46" 4a" 4 eon
45" 3° 6
Long, — 0°
- Lat, + 46° 11 sg"4 2
be
ey
Mem. Roy. Ast. Soc, vol. vir
page 130.
Communicated by Mr. Henderson. |}
Ast. Nach. vol. vi. page 148.
Ast. Nach. vol. v. page 382.
Ast, Nach. vol. v. page 366.
Ast. Nach. vol. ix. page 164.
Ast, Nach, vol, viii. 176
and vol, x. oe <
Ast. Nach, vol. x. page 232.
Struve's Astronom. Observations,
_ vol. vis
page 2.
Jase. Nach, vol. x. page 274.
} atom. ‘Ast, Soe. vol. iv. page 568,
Correspondance Astrono-
vol. i. pages 1 to 14, |
ir une nourelle déter- |
LATITUDES AND LONGITUDES OF THE PRINCIPAL
OBSERVATORIES.
Kensinctos - ~ ~- (Sir James South.)
Lat. + 51° 30’ 127°7 : ,
Long. + 0° 0™46" J, | atem. Adt, So, vol. v. page 8
K - - = =, =-Lat. 4 51° 28 37” Boil’ Aton. Tales an
oa Long.e+ 0” 1" 3 } mmulce, page 128. (London,|
Lat. 4 54° 42’ 50” Introduction to Bessel's Asi
Observations for 1821,
Long, — 1 22" O'S Bessel’s Tab. Reg. page 2.
Kosicsperc -
es ccta sara - + Lat, + 48° 3/29” Ast, Nach. vol. vi. page 67.
Long. — 0° 56"32'*3 Ast, Nach. vol. iii, page 121,
Pome ga ae gale ae
Long.— 3° 21" 3° “77 | pages 94.& 95. (Madras, 1)
(Sir T. M. Brisbane.)
Lat. + 55° 34’ 45”
Long. + 0” 10" 4°°0
Mannem - - - - Lat. +4 49° 29’ 14” Zach's Corvecponianes Ast
yol. 1, page 193,
Long. — 0° 33" 51°-4 As Rack, ‘ach, vol. ii. page 398.
Lat. + 43° 17’ 501 pose fp aise
Maxxastoun
hace. Nack, vol. x. page 214.
Manrsemirs - -
nae ae
Long. — 0” 21" 29*°0 Ane} vol. iv, page 36,
es rite ah ° "Zach's Correspondance
it. 4 45° 28° 7 "s Ast;
mique, vol. y. page 300.
Long. — 0" 36"47°°2 Ast. Nach. vol. ix. page 312,
Mopexa = - = = Lat. + 44° 38’ 53” emery te 1
Long. — 0° 43" 432 pages 94 and 60.
Monica - - = + (Bogenhausen.)
Lat. + 48° 8! 45" Ast. Nach. vol. i. 221,
Long.— 0° 46"26°°5 Ast. Nach. vol. vili. page 148
(Capo di Monte.)
Lat. +4 40° 51’ 466 Ast, Nach, vol. v, 294,
Long. — 0" 57" 0°'3 Communicated M.Caccia
to Captain B. RN.
Lat. + 46° 58’ 206 Ast, Nach, vol. vii. page 261,
Long.— 2" 7"55**1 Ast. Nach, vol. vii. page 306,
(Rey. W. R. Dawes.)
Lat. + 53° 34’ 18”
Long. + 0” 11™36"
Narirs = - =
Niconerr- - -
Onwserrk- - ~
}aten. Aut. Soc. vol, ¥. page 3
LATITUDES AND LONGITUDES OF THE PRINCIPAL
OBSERVATORIES.
Yxworp - - - - Ent. 519 45’ 40" |Requisite Tables, 3rd edit. (from
Long. + 0" 5™ 15 Trig. Survey.)
fapua- = = + + Lat. 445° 24’ 2” Ast. Nach. vol. v. page 411.
i Long. — 0” 47729°"2 Ast, Nach, vol, iv. page 347,
‘atrruo ~ = - = Lat. + 38° 6 44” Cacciatore, in Books 7 und 8 of |
Palermo Observations.
Long. — 6” 53"25"°6 Communicated by M. Cacciatore
to Captain B, Hall, RN.
‘amamatra - - ~ Lat, — 33° 48' 49/8 | Phil. Trans. for 1829, Part ili.
Long. — 10" 4™ 6°25 f pages 16 and 29.
- Lat. + 48° 50’ 13” tepae Tems for 1835, page
356,
Long. — 0° g™2it'S Phil. Trans. for 1827. (Hender-
sonon the of Green~
wich and Paris.)
‘ererspuncH- = + Lat. + 59° 56’ 31” ars des Tems for 1836, page |
=
J
a
.
'
,
‘
Long.— 2° 1" 15°°8 an Nach, vol, viii, page 360,
fonrsmouTa - - - Lat. + 50° 48’ 3” } Rie Susvey a 3rd edit, (from
Long. + 0° 4™23"'9
- Lat. + 50° 5’ 185 Saeoeed page 198.
Long. — 0° 57" 41°°9 Ast. Nach. vol. iii. page 264.
tome - - = = = (Roman College.)
Lat. + 41° 53/52” Conn, des Tems for 1822, page |}
313,
Long. — 0° 49"54"*7 Ast, Nach, vol, viii, page 88,
t. Fenxanno, neat | Lat, +4 36° 27! 45 Zack's Corespandance Astron |
Capiz - - at} brs sigs, Ths ae
Ase Nach, vol
‘RAGUE = =
Long, + 0" 24" 49° *1
t. Hetena = - = Lat. — 15° 58! 26”
Long. + 0" 22"50"
wouen = - = = (SirJd. PF. w. a
Lat. + 51°
Long, + 0° ee)
ourm Kinworra ~ (Rey, W. Pearson.)
Lat. + 52° 25° 51” A
Long. + 0° 4™ 2670 §-
veven = - = = Lat, + 49° 18’ 55"2 §
494.
TABLES.
LATITUDES AND LONGITUDES OF THE PRINCIPAL
OBSERVATORIES.
Torin - - - lew Observatory.)
x + 45° 4" 6” Communicated by M. Ph
Long. — 0° 30" 48" *4 Captain B. Hall, R.N.
VERONA - - - (Lyceum.)
Lat. + 45° 26/ (Approximate.)
Long. — 0" 44" 0°) Effem, Astron. di Milano fo
page 60.
Vienna - - + Lat. + 48° 1235” = Littrow’s Astron. Obsenr
Part viii. page 124.
Long,— 1" 5"81°'9 Ast. Nach. vol. iii. page 6
Vivizrs - - > (M. Flaugergues.)
Lat. + 44° 29 11” Zach's Correspondance 4
» Vol. ii, page 138,
Long. — 0° 18"44°°8 Ast, ‘ach, vol. v. page 25
Witna + - = Lat. +4 54°41’ 0” Ast. Nach. vol. iv. page 5
Long. — 1° 41™11°'9
Ast, Nach, vol. viii. page
EXPLANATION OF THE ARTICLES
CONTAINED 5M
E NAUTICAL ALMANAC AND ASTRONOMICAL EPHEMERIS
FOR THE YEAR 1838,
Axt the articles of the Ephemeris have been computed for Greenwich MEAN solar
time; and where they are expressed for apparent solar or sidereal time, it has been
chiefly for the convenience of astronomers. A day is the interval of time between the
departure of any meridian from a heavenly body and its succeeding return to it, and
derives its name from the body with which the motion of the meridian iscompared. The
interval between the departure and return of a meridian to the Sun is called a solar
day ; in the case of the Moon, the interval is called a /unar day; and in that of a Star,
a sidereal day, The revolution of the Earth on its axis is always performed in the
same time; and if the heavenly bodies preserved the same positions with respect to
each other, the intervals between the departure and return of a meridian to ¢ach would
be the same, and all days, consequently, of equal length. The San, (or, more strictly,
the Earth in its orbit,) the Moon, and the Planets are, however, in continual motion 5
and with velocities not only different from cach other, but varying in each partictilar
body: the length of a day, as determined by any of these bodies, is therefore a variable
quantity.
| Astronomers, with the view of obtaining a convenient and uniform measure of
| time, have recourse to a mean solar day, the length of which is equal to the mean or
average of all the apparent solar days in 9 year, An imaginary Sun, called the mean
Sun, is conceived to move uniformly in the Equator with the real Sun’s mean motion
in Right Ascension, and the interval between the departure of any meridian from the
mean Sun and its succeeding return to it is the duration of thé mean solar day.
Clocks and Chronometers are adjusted to mean solar time; so that a complete revolution
(throngh 4 Thotre) of ti Nout xi (GF iE SRAS sepeanas ates ees
exactly the same interval as the revolution of the Barth on its axix with respect to the
mean Sun, If the mean Sun could be observed on the mor
the hour hand returned to the same position.
tions of the frue Sun is called frue or
vailen of thee bo tie a
distance in time between the mean
‘496 EXPLANATION.
time"; hence it appears that the corresponding mean tim
the mean Sun had passed the meridian previously to the tr
the instant of observation the mean time clock or chronometer
this time,
A mere inspection of the columns of the Ephemeris is, of itself, suffic
that the quantities are continually varying, and that some reduction i
prlines nts are sfo tn gained ah By GS ee
quantities are registered. Take, for instance, the Sun’s Right A
of the month of January; on January 1, it is 18" 46" 36025 on.
is 18" 51" 0" 87; in the course of 24 mean hours it has therefore —
a" 24°85. If, then, the Right Ascension were required for any time
Mean Noons of January 1 and 2, as at 6” from Mean Noon of January 1,
necessary to increase the Right Ascension on January 1, by the proportional
the daily increase due for the 6", viz. by one-fourth part, or 1" 6°21. TI
in all cases be required, even under the meridian of Greenwich, for which t]
have been specially computed. Let a person be now supposed to be under
15° West of Greenwich, The positions of the heavenly bodies, as referred to #
of the Earth, are it of meridians, and are the same for all p
same absolute instant; but the relative times at Greenwich and the assumed n
would be different. If it were 1” from mean noon at the one place, it could
from mean noon at the other; for when we speak of time, we mean, as Tega
visible phenomenon, the distance of the Sun westward from a given meridian,
the same absolute moment of time the Sun cannot be at the same distance (r:
westward) from two meridians which are 15° distant from each other. Before we
make use of the Ephemeris, it is therefore necessary to ascertain, in every insta
distance of the Sun (in time) from the meridian of Greenwich, or what is con
under the assumed meridian, increased or diminished by the difference (in time)
two meridians, according as the assumed meridian is to the Weshoard or East
Greenwich, In a mean Solar day, or 24 mean Solar hours, the Earth, by its rotati
from West to East, has caused every meridian in succession from East to West to pass
the mean Sun; and since the motion is uniform, all the meridians distant from each
other 15° will have passed the mean Sun, at intervals of one mean hour; the meridian to
the Eastward passing first, or being, as compared with the Sun, alwayseue mean hour
in advance of the’ Westerly meridian. When it is 6" from mean noon place 15°
‘West of Greenwich, it is therefore 7° from mean noon at Greenwich; and it is for this
Greenwich time that we must deduce the quantities required from the
Ifa chronometer adjusted to Greenwich mean time be at hand, the Greenwich time
may be immediately obtained by applying a correction, deduced from the daily rate
and interval elapsed, and this will be preferable in all cases for obtaining La id
data from the Ephemeris.
The day adopted in this Ephemeris is supposed to begin at mean acoenfeatiahthe
instant when a clock or chronometer shows 0" 0" 0", Greenwich mean time, and is
continued through the 24 hours, to the following mean noon, when another day begias.
It may therefore be called the Mean Astronomical Day, although, in practice, astrono~
mere begin the day at the moment the true Sun’s centre is on their
In the civil, or common, method of reckoning, the day is supposed to commence at
the preceding midnight, and to be counted only to 12 hours or noon, when the 12 hours
are reckoned over again to the next midnight. ‘The civil reckoning is therefore always
i ace ax the civil time corresponding
EXPLANATION. 497
given astronomical time is hence readily found by adding. 12” to the latter:
if to Jan, 1" 7" 49", astronomical time, be added 12", the sum will be
1* 19 49", or Jan. 1¢ 7” 49" P.M. civil time. Again, to Jan. 1‘ 15" 35",
ical time, add 12%; the sum will be Jan. 2! 3" 35" A.M. civil time. It
‘appears that, from noon to midnight, the day of the month and the hour of the
the same in both methods; but from midnight to noon they differ; for at mid~
Satis biel eheaeegine ribcarrapee fast es 12” of its
Eaesyieiciver cirildnaetadkcevsn boclanco is on the contrary performed by démi-
ing the former by 12". Thus, January 2* 3 35" A.M. civil time, diminished by
", leaves January 1" 15" 35", for the corresponding astronomical time. j
To cach month there are devoted twenty-two pages, distinguished by the Roman
merals I. to XXII.
Forconyenience of interpolation, the quantities that follow next in order of suc-
ion have been added at the bottom of each page. Thus the quantities opposite
February 1 will be found inserted also opposite to January 32, the number of the
in cach month having been intentionally increased for such purpose.
Page I. of each Month.
The contents of this page are adapted to Apparent Noon, or the instant when the
’s centre is on the meridian of Greenwich. The Sun’s Right Ascension, here given,
Sore with Aberration, and reckoned from the true Equinox; it is therefore the
Time at Apparent Noon, or the time which ought to be chown by a Sidereal
Clock, at that instant. The Sun's Declination, at Apparent Noon, is the apparent
@ngular distance of the Sun from the Equator, measured on the meridian,
‘The columns entitled “Diff. for 1 hour” are intended to facilitate the reduction of
‘the quantities from the meridian of Greenwich to any other meridian, The values of
these quantities for any proposed mean time will, however, be more accurutely ascertained
‘by means of the numbers on page II., from which, indeed, they have been derived.
The Stdereal Time of the Sun's Semiidiameter passing the Meridian is useful for
reducing a transit observation of cither limb of the Sun, when one only has been
observed, to the transit of the centre.
The Equation of Time is the difference between Apparent and Mean Time, and
therefore serves for the conversion of either time into the other. The numbers here
given, show, for Greenwich Apparent Noon, the distance of the mean Sun from the
meridian, or the portion of time to be added fo, or subtracted from, (according to the
precept at the head of the column,) Greenwich a Noon to obtain the corre-
sponding Mean Time at the same m which ought to be shown by
the Mean Time Clock. It differs fi
the equation itself varies in the i
498 EXPLANATION.
15th and 16th days of the month; but after that
tracted from Apparent to obtain Mean Time.
‘Where time is dedaced from observations of the
apparent time; to convert it into mean time, the
and it is to be applied to apparent time, according to
column.
‘Thus, suppose the apparent time deduced from an ion
January 16, 1838, in longitude 45° or 3" cast ples be
required to convert it into mean time : C
Prmearidrinaniegrarirsiteamt bee) oo i
Greenwich, The difference of the equation for L hour is 0"839, 1
3, gives 2"517 for the variation in 3 hours, and this being
tion is increasing) to 10" 385, the equation of time at ap
10” 6°37, to be added (according to the
given apparent time 6", whence we obtain
clock, or chronaweter, indicates 0° 0 0", Gr whesi the hour angle or °:
equal to the equation of time. ‘
To find the Right Ascension and Declination for any other mean ti
at 9" 20" A.M, March 2, 1838, in longitude 98°, or 6° 32", West of G
astronomical time, corresponding to 9” 20" A.M. March 2, is
of March 1, or March 1* 21" 20",
March 2* 3" 52", is the corresponding Greenwich mean time, for
‘Ascension and Declination are to be found. The difference between
sions on March 2 and March 3 is 3" 43"93, that is, in the 24 hi
the Mean Noon of March 2, the Right Ascension has increased
it will, therefore, have received a proportional part of the increase in
amount is readily obtained by this proportion, 24": 3" 43°93 z2
which, being added to 22" 51" 46°13, the Right Ascension at Mean
gives 22" 52” 22°21, for the Right Ascension at the time
Ina similar manner the Declinations indicate a decrease 36"2
hours; therefore 24" ; 29/ 56’-2 :; 3" 52" ; 3’ 41/7, the ”
decrease for 3" 52", which, subtracted from S.7° 15’ 21""3, leaves S. 7° 11
the Declination required. }
The Semidiameter of the Sun. The numbers in this column express the
the centre of the carth subtended by the Sun's Semidiameter, and are
reducing observations of the limb to the centre, as in the instance of
tude of the Sun's upper or lower limb, or the distance of the Moon: e
Equation of Time. a Noam, and Oametee cove mest pera
at the instant of Mean Noon, and therefore serve more particularly to
into Apparent Time: for which purpose we have only to apply the equation according
to the precept at the head of the columm, ‘Thos, i Som meu noon of April 1, or
=a
, from the denomination given, to that required ; ani
Sell os esta ores
Interval in sidereal time from mean noon - = = = =
Retardation of mean on sidereal time for the interval -
Mean solar time required - - - = - - - = = :
which is the interval elapsed since mean noon, expressed in mean ti
fore the time which ought to be shown by a mean time clock.
Vice versd, to convert 2° 22™ 17°55 mean solar time, January 2, 1
sidereal time for the same meridian.
Mean interval from mean noon, January2 = = = =
Acceleration of sidereal on mean time for the interval
Sidereal interval from mean noon = - - = = = =
Sidereal time af mean noon, January 2 = = = = =
Sidereal time required - - - - - - = -~ = ~ @
which ought to be the time shown by the sidereal clock at the instant
If the place of observation be not on the meridian of Greenwich, the
must be corrected by the addition of 9''8565 for each hour (and prop
for the minutes and seconds) of longitude, if the place be to the west of Greer
but by its subtraction, if to the cast. Thus, in 9" map en e si
time at mean noon, January 2, instead of being, as in the foregoing
18" 46" 42° *11, must be corrected by adding 1™ 30° *37, thus giving 18" 45"
for the time to be uscd, instead of that act down in the
The conversion of mean solar to sidereal time, and vice basa may,
performed, and with perhaps less liability to error, by means of this and of the :
entitled Mean Time of Transit of the meh gate
month, using the Tables of Time Equivalents, inserted at pages 486 to 489.
To convert mean solar into sidereal time: To the sidereal time at
mean noon add the siderea) interval corresponding to the given mean |
will be the sidercal time required. (See Example at page 487.)
To convert sidereal into mean solar time: To the mean time at the
sidereal noon, add the zitan interval corresponding to the given sidereal time:
sum will be the mean solar time required, (See Example at page 489.)
In this mode of reduction there is not, as in the former, by means ‘of the Tables
of Acceleration and Retardation, any distinction of cases, all the atin en)
additive, a
The Tables of Time. Equivalents differ from the Tables of Acceleration »
tardation, in containing the values of intervele of each wyecien of Hime,
502 EXPLANATION.
correction of the registered value preceding the given
for midnight, or 12", of the 16th, is 14” 48"°8, and for the
is 44' 51/"8; the difference 30 is the variation in 12 hours,
12": 8/0125": 3,
which, added (because the quantities are increasing) to 14!
for the Moon’s Semidinmeter ut the time
Parallax at midnight of the 16th is 547216; and at the
54’ 32”°5; the difference 109 is the variation in the 12
given time; therefore, 12: 109 >; 5": 4'"54, or 4’%5,
the quantities are increasing) to 54’ 21/6 gives 54’ 26"1
Parallax required, If greater accuracy be desired, & further
applied to the values just obtained, on account of second differen
the error by supposing the first differences uniform.
error in the semidiameter which can arive by this supposition fs about
second: in i ,
from the
first and
The mean of the second differences is 0” 65, and 4 of thie, which is th
is 0” 08,
A similar operation performed on the Patallaxes will show the error, that would
arise on the supposition of uniform or equal first differences, to be n |
second ; it can never be more than about seven-tenths,
Page IV. of each Month, -_—
The Moon's Longitude and Latitude at Mean Noon and Mid
position of the Moon at these respective times, referred to the
true Equinox, as it would be seen from the centre of the earth.
results deduced immediately from the Lunar Tables, and are the foun
subsequent calculations in which the Moon is concerned. These quai
little use to the seaman, as the position of the Moon, with respect
is given for every hour in the succeeding pages; but the Moon's Long
in the formule for nutation, and is therefore necessary for its deter on.
finding the Moon’s Longitude and Latitude for any other times than those
Noon and Midnight, it is necessary to apply the equation of second, and somet
even of third and fourth differences, on account of the irregular variation of her my
The Moon's Age xt Mean Noon is the Mean Time elapsed since the Moon's ecliptic
conjunction with the Sun, or since the Sun and Moon had the same Longitude. The
numbers in this column represent her age at Greenwich, and are expressed indays, and
decimal parts of a day, :
‘The Moon’s Meridian Passage.—This column contains the Greenwich Mean ‘Time,
to the nearest tenth of a minute, at which the Moon’s centre is on the upper Meridian
EXPLANATION. 503
f£ Greenwich, and is useful to indicate when the Latitude may be obtained from an
4 meridian altitude of the Moon; also, in conjunction with a Table of Semi-
pal Arcs, to determine the times of the rising and setting of the Moon: it is likewise
useful in finding the time of High Water.
Pian the eymbul (:¢ ) Denoting’ conjunction ccciey, es tm Jesvuary 25, we are 19
understand that the Moon does not pass the upper meridian on that day at Greenwich.
‘his is the case once in every lunation, and arises from the circumstance of the Lunar
mie being greater than the Mean Solar day, and including it within its limits. In the
esent instance, the excess is 1" 1™'9, or the lmar day is equal to 25" Mean
Solar time; the Moon passes the meridian on the 24th at 23" 424, or 1
- bly 10 the noon of the 5th, and docs not return to fhe samo meridian wae) O* 449
after the noon of the 26th. For the same reason there is also one day in every luna-
f= fion on which the Moon does not transit the fower meridian, and this happens about
Pn sotecin, cx nh eSBs st eagle ten eee
180°, In the list of Moon-culminating Stars, at pages 410 to 451, the days on whieh
© only one transit occurs are readily seen. On April 23rd (page 423), for instance, it
f{ appears that the Moon transits the Jower meridian only, while on May the 9th
Gpage 424), the only transit is that at the upper meridian.
To find the Mean Time of Transit under any other Meridian, suppose 45° or 8" west
of Greenwich, on January 15, 1838. The Meridian being to the west of Greenwich,
the Transit will take place after the Greenwich time of ‘I'ransit on the 15th; there-
fore take the difference between the Meridian Passages on the 15th and 16th, which
is 397-0. Then, 24"; 0° 39°-0:: 3": 4-9, which added to the Greenwich Mean
‘Time of Transit gives 16" 6"'5 for the Mean Time of Transit at the given Meridian,
Had the assumed Meridian been 3° to the east of Greenwich, the Transit would
have taken place before the Transit at Greenwich, and the proportional part of the
difference between the 14th and 15th, must in this case have been subtracted, The
‘times thus deduced are only approximate; but they are sufficiently accurate for the
purposes usually required.
Pages V. to XII. of each Month,
The Moon's Right Ascension and Declination for every hour of the day, with the
Difference of Declination for 10 minutes. By means of the quantities here given, thé
Latitude, Time, Azimuth, Moon’s rising and setting, &c., may be deduced, with
nearly as little labour as is required in the case of the Sun, ‘The numbers
the position of the Moon, as it would appear from the centre of the Earth, with respect
to the Equator and the true Equinox: and they are given for every hour, with
the view of rendering any correction for second differences unnecessary, except where
extreme precision is required. ‘The Right Ascension for any time is readily obtained
simply adding the Lapsed iptentey Be ee nth bn tel
since the preceding hour, Thus, suppose the Right Ascension of mn
required at 8° 45"mean time of January 8, in |
wich. The given time, 8* 43", diminished by ®, g
time 4 45", ‘The Right Ascension at 4 ig 5
5"52; Kad» alge a Fh)
60": 2 22623: : 45": 1" 46°67, which
gives 8" 32" 29°96 for the Right
proposed.
0a EXPLANATION.
Seriaids to any hour ta of oe dilereace oh
_ hour. We ‘therefore say, 10": eee
ndded (because the Declinations are ij
nation at 4”, pies N07 A0'49°7, fu Gos oceaNA
The Phases of the Moon. ‘These are given at page XT
0° at the New Moon,
90° at the First Quarter,
180° at the Pull Moon,
270° at the Last Quarter,
‘The Moon's Apogee and Perigee. The numbers here given indicate, to the m
hour, the Greenwich Mean Time at which theMoon is opetely a her gre
Jeast distance from the Earth.
Pages XIII, to XVII. of each Month,
Lunar Distances.—These pages contain, for every third hour of Greenwich Man
‘Time, the angular distances between the centres of the Moon and certain heavenly
bodies, such as they would appear to an observer at the centre of the Earth. Whens
Lunar Distance has been observed on the surface of the Earth, apace!
centre, by clearing it of the effects of parallax and refraction, the
pages enable us to ascertain the exact Greenwich mean time at which the:
have the same distance, They are arranged, from awest to east,
day with the object which is at the greatest distance wesltvard of the
precise order in which they appear in the heavens; W. indicating that
west, and E, east, of the Moon. Thus we haye at cae view, hy epi
the date, all the lunar distances which are available for the
Longitude, .
‘The columns headed * P. 1. of Diff. contain the Proportional Logarithms of the
Differences of the distances at intervals of three hours, which are used in
Greenwich time corresponding to a given distance, according to te Wiorie aes
For the given day, seck in the Ephemeris for the nearest distance preceding, in
of time, the given distance, and take the difference between it and epi gie nd
from the proportional logarithm of this difference subtract the proportional siesta |
standing opposite to the said nearest distance in the Ephemeris; the
be the proportional logarithm of a portion of time to be ndded to the hour answering
to the nearest distance, to obtain the approximate Greenwich mean time corresponding
to the given distance.
If the distance between the Moon and a Star increased or decreased uniformly,
the Greenwich time corresponding to a given distance, as found by the above rule,
would be strictly correct; but an inspection of the columns of the Proportional
Logarithms in the re chaneie will show that this is not the case; and as the know-
ledge of the exact Greenwich time is desirable, a correction must be applied to the
time so found for the variation of the differences of the distances. ‘This correction
may be obtained by means of the Table at page 482 of the present volume, in the
following manner:
1. Find the Approximate interval, by the preceding rule.
EXPLANATION. - 505
2. Take the difference between the proportional logarithms standing opposite to the
in the Ephemeris which include the given distance,
3. With the approximate interval and this difference, as arguments, take out the
‘correction from the table.
i. 4. If the Proportional Logarithms are decreasing, add the correction to the
‘approximate time; ye ooong clam the result will be the accurate
Greenwich mean time.
Example 1.—Suppose it were required to find the Greenwich Mean Time, at which
the true distance between the Moon and « Pegasi would be 42° 25’ 12” on May 15,
1838. It appears, by inspecting the distances, that the time must be between XY"
and XVIII": the nearest distance preceding, in order of time, the given distance is
therefore the
Distance at XV" - - 431153, and PLL. - = 3081
True Distance - - - 42 25 12
Difference - - - 04641 - - PL. + - 5861
Approximate Interval - 1" 34" 54° - - PLL, = = 2780
The difference between the Proportional Logarithms in the Ephemeris, at XY"
and XVIII", is 46. Opposite to 1° 35” (or the quantity nearest to it, 1 30"), and
under 46, in the Table, we have for the correction 14", which, subtracted from. the
Approximate Interval, 1" 34” 54", because the Proportional Logarithms are increasing,
gives 1" 34" 40°, for the true interval from XV": and hence the Greenwich Mean
Time is 16" 34" 40",
‘We see that, in the preceding Example, the omission of this correction would only
produce an error of 3/5 in the Longitude. Cases may however occur, in which it
would be
Tt will sometimes happen, that the difference of the Proportional Logarithms will
excced 88, the limit of the Table of Correction ; in this case the Table may be entered
with one-half or any fraction of the difference of the Proportional Logarithms and the
Approximate Interval, and the corresponding correction increased in like proportion,
Example 11.—Suppose it were required to find the Greenwich Mean Time, at
which the true distance between the Moon and Aldebaran would be 17° 36" 16” on
November 2nd, 1838. By inspecting the distances, it appears that the time must
be between IX" and Midnight; therefore take the
Distance at IX* = - 18 1038 and PLL. - - $033
True Distance - - 17 361
Difference - - 03422 - - PL, - - 191
Approximate Interval - 1" gv 6 = = PLT. = )
‘The difference between the
Midnight, is 235, one-third of which is, say, 78;
opposite that nearest the Approximate Interval, is
ferred which has the least Proportional Logarithm opposite to j
dagen vino wher sry irletiaet preg |
‘on an observation of the distance; and it is
decrease as their natural numbers increase:
fore, indicates a greater velocity of the Moon, or a greater variati
interval, upon which the value of the observation depends. —
1838, between Noon and IIJ*, Jupiter is the most eligible
portional Logarithm, 2775, is less than that of any other,
columns of Proportional Logarithms, it will appear to deserve
the end of February 9, after which it is discontinued. ,
On the 15th day of February, between XV" and XVIIT*, the
of pease fe indieniah. Oy the Pope ees i
Regulus, Spica my, Saturn, Sun, and « Aquile; between
Spica my and Regulus are equally good, because the
difference is the same for each, the order of the others remains the
Saturn, which is discontinued.
Tt is by no means to be inferred from these remarks that obeervations:
distances are to be neglected ; on Sp wernt ee registered
riably be observed when an opportunity offers. ith however, on a
results, a considerable difference shoulil be discovered the
will indiente the stare which are least Tinble to be affected by
therefore deserving of a greater degree of confidence as to the
obtained from them.
Page XIX. of each Month,
Configurations of the Satellites of Jupiter, ;
In addition to the explanation given at the foot of the page, it may
that when two Satellites are in or near conjunction, instead of the usual s
it has been thought better to place one above the other, without regard t
latitudes, but merely to distinguish them in their relation of upper and lor
‘The Satellites arc'in the superior parts of their orbits, or have Jup
them and the Earth, when they are moving from West to East, or
hand of the page; but they are in the inferior parts of their
Earth and Jupiter, when they are moving from East to West, or
in the former case Eclipses and Occultations occur, and in the latter
Satellites and their Shadows,
If an inverting telescope be directed towards Jupiter on March"17, 1
Mean Time, the Satellites will appear to an observer at Greenwich in the pos
laid down in the Table. The Ist Satellite, which is really to the
will appear to the right of it; and the 2nd, Srd, and 4th, which are really to e right,
will appear to be to the left, ye. 4g
West and East, at the head of the page, are inserted to show the
of the Satellites with respect to Jupiter, as they would appear in a telescope #
EXPLANATION, 507
‘invert, Jupitér being always to the South of the zenith of Greenwich, the Satellites
are here laid down on the left of Jupiter would appear to the West, and those on
eed i tn Fatt a Hen.
‘As regards their positions to the east or west, the page viewed direetly, exhi-
Dits the Satellites in an inverted order; but if the leaf be turned over, and the page
‘Yiewed from the other side, they will appear in their real positions. The simplest
mode of changing the position of a Satellite from apparent to real, and nice vers,
is to draw a line from the Satellite through Jupiter’s centre, and to place the Satellite
this line at the same distance from the centre as before, only on the opposite
‘side. If this operation be performed upon the Contigurations as laid down in this
volume, the Satellites will be reduced to their real positions.
As the Configurations are given for Mean Astronomical time, which agrees with
Civil time only from 0" to 12", or from noon to midnight, when the time exceeds 12”
the excess will indicate the Civil time of the succeeding day of the month.
Thus in November, 1838, the Configurations are given for 17° 30" mean time, but
the 17th hour from noon is the same as the 5th hour from the following midnight,
when a new Civil day has commenced. The appearances, therefore, relate to 5* 30"
A.M. of the day following, according to the common mode of reckoning time; that is,
the Configurations at 17" 30" on November the 26th relate to 5" 30" A.M. on
November the 27th.
‘The Configurations enable an observer to distinguish the Satellites from each other,
and from Stars in the vicinity of Jupiter.
Page XX. of each Month,
Eclipses of the Satellites of’ Jupiter.
On this page are given the Mean and Sidereal Times of the Eclipses of the Satellites,
together with diagrams exhibiting the position of each Satellite with respect to the
disc of the Planet at the moment of Immersion or Emersion, as it will appear in an
inverting telescope. ‘These diagrams have been laid down from calculations made for
the eclipse nearest to the middle of cach month; but they will serve very well for the
whole of the month, except near opposition, the change in the position of Jupiter and
his Shadow in the interval being too small to be appreciable by the eye, as is
evident by comparing the Phases for any two successive months. All the Eclipses
which happen when Jupiter is 8° above, and the Sun 8° below the horizon of Green-
wich, are marked with an asterisk to indicate that they are visible at that place;
and some which are even within these limits have been also marked, as, under favour-
able circumstances, they may sometimes be o
The Tempero ee u
To find the time at which the Immersion or BE
add the difference of longitude (in time) to the time of #)
wich, if the meridian be east of Greenwich, or to si
sum or difference will be the time required. ‘But thi determines
the occurrence of the phenomenon: Jupiter may be’
or he may be above it, and the intensity of sun-light, 0
mnay be such as to render the Satellites invisible. To
se has generally been -coneldcoed thst dhe Sesishovlastas sede
and Jupiter not less than 8° above it at the same time. Adop
means of a celestial globe, or near enough for the purpose, by
rising and setting of the objects, with the assistance of a table of |
readiest means of determining the longitude ; Selene b
appene tha Lmmaralonof Fapitr’a feat SaslSsl ta hw Gaaanan ES
at Paris at 21" 9" 77 Mean Time at that place; by reference to
appears that the Immersion will take place at Greenwich at 20° 59" 6
Mean Time difference, 9” 21*'5, is the difference of
wich and Paris; and, because the Paris time-is greater than that at Greenwich, we
infer that Paris is to the east of Greenwich,
Independent of defects in the tables, there are difficulties
vation of these phenomena which unfit Uys for accurate determinations of
to those corresponding observations which have been made under circumsti
most similar, and | particularly with telescopes of the same quality and po
extreme accuracy is not required, the Eclipses of the Satellites will
good approximation towards the difference of meridians, and observations
should on no account be neglected, especially when the f{mmersion and Eme
the same Satellite are both visible,
Page XX. of ench Month,
Approximate Sidereal Times of the Occultations of Jupiter’s Sle by Soeleniaas
of the Transits of the Satellites and their Shadonws over the Dise of te
These phenomena are inserted in order to apprise Astronomers when
about to happen, as observations of them may tend to improve the Tables of the
Satellites, The instruments required to observe them with any thing like precision
will preclude the possibility of their ever becoming available at sea. "The times are
given in days, hours, and minutes; the day being supposed to commence at mean
noon, and the hours and minutes representing sidereal time, such will be shown
by a sidereal clock on that day.
‘The Phenomena for cach Satellite are arranged under three distinct heads, eid emats
in the order of the days of the month, so that an inspection of the columns opposite
to each Satellite is necessary to determine what phenomena will happen on a given day,
Where an asterisk is annexed to the day of the month, it signifies that the pheno=
EXPLANATION. 509
on is visible at Greenwich, the limits of visibility being the same as those'adopted
e eclipses.
In the month of May, 1838, under the general heading “ Occultetions"”
te to Satellite 1, and under Immersion, the first quantity recorded is 2* 6" 45",
lich signifies that at 6° 45" sidereal time on May the 2nd an Immersion of the
Satellite takes place, but that it is invisible at Greenwich. Under Emersion we
for the whole of the month, ‘In the shadow,” which signifies that the Emersion
the Satellite cannot be seen; because, although it ceases to be oceulted by the body
‘of the Planet, it is still involved in its shadow, from which it docs not indeed escape
f= until 10" 8" 54°°3 sidereal time. (See Eclipses of the Satellites of Jupiter on the
ee iss een of the mooth.) Again, in the column of Occultations opposite to
= ite LI, it mppears that the 3rd Satellite is occulted on the 9th day of the
= month; that it disappears behind the disc of the Planet at 13" 2", reappears at
fe 16° 32", Sidereal time; and that both the Immersion and Emersion are visible at
= wich,
» In the column headed Transits of Satellites, the first transit of Satellite I.
|
|
at Greenwich appears to be on -the lat day, when the Ingress takes place at
‘9° 30", and the egress at 11" 49", Sidereal time; that is, it comes into contact with
Jupiter's disc at 9" 30", remains on the dise 2” 19", and quits it again at 11" 49",
| sidereal time; the egress only is visible at Greenwich.
Tho Transits of Shadows are to be interpreted in a similar manner.
Page XXII, of each Month.
1, Logarithms of A, B, C, D, for correcting the Places of the Fixed Stars.
Tn the formule which express the relation of the apparent place of a Star to its
mean place, and reciprocally, there are certain factors which are independent altogether
of the Star's place, and are therefore common to all Stars. These factors depend
upon the longitudes of the Sun, Moon, and Moon's ascending Node.
The Logarithms here given are the logarithms of these independent factors, conve-
niently arranged for incorporation with other terms depending upon each particular
Star, according to the method recommended by Professor Bessel. ‘They have been
computed for Mean Midnight at Greenwich, according to the formule exhibited at
page 365, omitting in C and D the terms depending on 2 € .
I the Aotreental Seestsl, eRe neki aslo eeraeaa ae
with the Astronomical Society’s Tables,* which contain the
yemaining factors depending on the Star’s place; and for th
in that Catalogue, they appear to afford every facility that ¢
Paisdpal Fed Dass topetat o ‘
wr ine Rapeave and Gate tha DUSeiui Rea
an Introduction, explanatory of their C
1827, dto.
2, Mean Time of’ Transit of the First Point of Aries.
‘The time in this column shows the distance of the mean Sun from the meridian,
the instant when the (rue point of intersection of the ecliptic and equator (called
- the first point of Aries) is on the meridian of Greenwich ; and as the distance of the
GRRL geil of Asste frtex the vaeridlins,-a( dhe tualant the ined Guise tw Gaiiiicadaaas
‘is denominated Sidereal Time at Mean Noon, this may, by analogy, be termed the
Mean Time at Sidereal Noon. It is the time which ought to be shown by & mean
‘time clock adjusted to the Greenwich meridian, at the moment that a clock, adjusted
to sidereal time, indicates exactly 0' 6” 0°. The use of this column is to facilitate the
reduction of sideresl to mean solar time, with the help of the Table of Time Equiva-
dents, given at pages 488 and 489, of this volume, as has been already explained at
page 500.
3. Mean Equinoctial Time.
Mean Equinoctial Time signifies the Mean Time elapsed since the inetant of the
Mean Vernal Equinox. The numbers in this column represent this time, at every
Mean Noon, in Mean Solar days and fractional parts of a day; it is reckoned from
the Mean Vernal Equinox of 1837, between Jannary 1‘ and March 227463822, but
after March 22%-463822 from the Vernal Equinox of 1838; for the Equinoctial Year
has been assumed, according to Bessel, (Conn. des Tems, 1831, Additions, page 154)
equal to 365°242218 Mean Solar days; and as the Equinoctial Time corresponding to
the Mean Noon of March 22, 1838, is 364°778395, it is evident that the
Year of 1837-8 was completed, and that a new year commenced, at "463822 after
Mean Noon of the 22nd,
‘The fraction of the day at the head of the column is common to all the days of the
Equinoctial Year. Thus, at Mean Noon of January 19, 1838, the Equinoctial Time
is 302°-778395, and on January 20 it is 303/+779395, and so on until March
224 463822, when the year terminates, and the fractional part of the day
At Mean Noon of March 23, 1838, the Equinoctial Time is 0"*536178, and this
fraction is to be annexed to all the numbers in the column of days, from the period
of the change until the equinox of 1839.
At the instant the Mean Sun arrives at the Mean Vernal Equinox, it must also be on
some meridian, and this meridian will then have its Equinoctial time corresponding
with its Mean Solar time, each of which will be 0° 0" 0°, and they will continue to
correspond throughout the Equinoctial Year. At the end of the Equinoctial Year,
the Sun will have passed this méridian 365 times, and have performed, besides, a
certain portion of its 366th diurnal revolution, viz. 0* 242218 ; it will, therefore, have
arrived at some other meridian, which will now, in its turn, reckon the Mean Equi-
noctial and Mean Solar time from the same point, and remain constant for the year.
Thus the meridian, from which the time is reckoned, is shifting its position at the
end of every year by 0° 242218, or 5" 48™ 47°64, to the Westward. Between the
Vernal Equinoxes of 1838 and 1839, this itinerant meridian corresponds to Longitude
0° 536178 or 12° 52 5* 78 East of Greenwich,
This species of time was first introduced in the Supplement to the Nautical Almanac
for 1928, with very full explanation of its nature and use. It there appears, that
the use of Equinoetinl Time is to afford an uniform date, which shall be mdependent
of the different meridians, and of all inequalities in the Sun’s motion, and shall thus
save the necessity, when speaking of the time of any event's happening, of mentioning
512
at the same time the place where it was observed or
thing to say that a comet passed its
Mean Time at Greenwich; at 5° 56" 21°, Mean Time
wich and Paris enter as elements of the expression ;
period elapsed since an ¢poch common to all the
ently of all ‘localities. By this means. all ambiguities i
before alluded to, Paris being 9" 21"°5 East of Greenwich, ubtr
time and we get 5" 47" 0"0 for the Greenwich
288*-778395, or 288! 18" 40" 53°33, the Mean Equinoctial Time at
Noon of January 5, and the sum will represent the Mean Eq
Comet’s passage of its perihelion, viz. 289" 0° 27" 53°33, from |
the year 1837.
4. Day of the Fear.
The numbers in this column indicate the complete days st mean no
elapsed since mean noon of January 1, Mean noon of January h
0, and 1 is found opposite to that of January 2, because at that instant
day has elapsed. oul
5. Fraction of the Year. ¢
These fractions are the quotients found by dividing the numbers in the
column by 365°25. The day and fraction of the year are useful in many Astro-
nomical calculations,
Obliquity of the Ecliptic. (Page 266.)
‘The apparent inclination of the plane of the Ecliptic to that of the Equator is here
given for every LOth day of the year, and continued to January 6 of the fol
ing year, marked December 37 for the sake of convenience. This
is ever varying, as well from the effect of its mean diminution, as of the nu-
tation of the carth’s axis: it is an important clement in ‘positions
of the heavenly bodies, with reference to cither of the planes, when we know
their positions with respect to the other; as, for instance, in
Ascensions and Declinations from Longitudes and Latitudes, and vice versa, eA the
apparent Obliquity be required for any date not to be found in the
be obtained by simply taking the proportional Fi: of the eects of te
corresponding to the interval which comprises the given date. Thus, the apparent
Obliquity on August 18, 1988, is 23° 27’ 46"-41, For the variation of the Obli-
quity in the ten days between Angust the 9th and the 19th, is 0"*10, or 001 for
one day, and this being multiplied by 4, the number of days between the 9th and the
13th, gives 004, to be added to the Obliquity of August the 9th. For most purposes,
EXPLANATION. 513
however, the Obliquity corresponding to the date in the Table nearest to the given
date ix eullicient, asin crident from an inspection of the quantition
Sun’s Horizontal Parallax. (Page 266.)
‘The Sun's Horizontal Parallax is the greatest angle under which the equatorial
emidiameter of the earth would appear at the Sun’s centre. It varies inversely
as the distance, and the numbers in this column show the values for every tenth day
of the year,
‘The Parallax serves for reducing a Solar observation made at the surface of the
earth to what it would have been if made at the centre.
Sun's Aberration, (Page 266.)
The progressive motion of light, combined with the motion of the Earth in ite orbit,
‘causes the Sum to appear in a different position from that which he occupies,
the true position being always in advance of the apparent. The numbers in this
column indicate, for every 10th day of the year, the amount of Aberration, or the
quantity to be applied to the true longitude of the Sun to obtain the apparent
longitude. The longitudes derived from the Solar Tables include Aberration, and are
therefore apparent longitudes, such as are contained in this Ephemeris. If the trae
longitude of the Sun be wanted, as is the case in finding the longitude of the Earth
for the calculation of the Geocentric place of a body, the aberration must be applied
with a contrary sign, Thus, on June 9, 1838, at Mean Noon, by adding 20°05,
the amount of aberration, to 78° 8° 11, the apparent longitude of the Sun, we
obtain 78° 8’ 21/15 for the true longitude.
Equation of the Equinores. (Page 266.)
‘The Solar and Planetary Tubles furnish us with the places of the Heavenly Bodies
referred to the Mean Equinox; but the true place of the Equinox at any time differs
from its mean place, by a quantity which is termed the Equation of the ;
and the numbers here given show the value of the Equation for every 10th day of
the year. They are to be applied, with their proper signs, to the Longitudes reckoned
from the Mean Equinox, to obtain the values with respect to the True Equinox.
Tf the Longitude of a hae fap ey ayicere atte Sante Tala bs taily
apphving it with the comasyintans that
from the Mean Equinox on that day.
EXPLANATION: 515,
ler ein tn tnt ren time not given in the Ephemeris, and under
any lag ele sor id iy fy bake og by interpolation in the
Pt an
Jupiter's passage over this meridian on the same day. The difference of longitude 2
eee et in wy to the given time, gives 8" for the corresponding Greenwich
1. “For the Right Asconsion ‘The Right Ascension dn a hanna
and on January 16 it is 11" 19" 5094; the differetiee 8-37 is the variation of the
Right Ascension in 24 icin hours; therefore, 94" ; 937 2: 8" + 279, ee
Proportional part of the varintiol anawering to &*Y and thié
atl Ce he ih uci re cei) ft 0g 1 igh
Ascension at mean noon on January 15, gives 11" 19" 56%52 for the Right
required.
2. For the Declination. ‘The Declination ot Samiliry 15 ik N. 5° 43/564, and
on the 16th it is N. 8° 45' 7-3, the difference, 1” 10’, ss eshte fh al iho
and the proportional part of this variation fet 8" d 23""6, which, added to the
Declirtation at noon ob the 15th, gives N. 5°44 S0"4 for the Declination required.
3. For the Meridian Passage, ‘Take the difference of the times of two consecutive
transits; and considering this difference as an neceleration or retardation of the Meri-
dian Passage while the planet has passed over 24" of geographical longitude, take the
Proportional part of it, due to the difference of meridians, for a correetion to be applied
to the Meridian at Greenwich, ing in mind that in east longitudes the
snge precedes eee Nea when Fanta aceelerated, and follows it, when te
are retarded; and the contrary in hog pg te In the present case Jupiter
the meridian of Greenwich on January 15 at 15 ree peek 1b at oe 5m a
the difference ix 4""1, therefore 24" : 4-1 :: 2": 0°, the proportional part to be
tracted from 15" 39"=4, (because the passages are retarded, te pe oy
Greenwich, ) which gives 15"39™1, mean time at the given place, for the Meridian Pas-
sage. Where great accuracy is not required, as in predicting the time of passage, in
order to be prepared for observing the altitude of the planet on the meridian, for the
determination of the latitude, this method will suffice,
Parallaces and Semidiameters, (Pages 359 to 861.)
These are given for the noon of every Sth day of the year, and may be interpolated,
if required for any intermediate day.
516
In pages 362 to 364 are given the mean Right As
principal fixed Stars for Jan. 1, 1888, together with their
‘The stendard Stare ar distinguished by expt a
Example \. Required the Mean Right Ascension and. )
Aldebaran on May 31, 1838. The Annual Variation of the
- 34265; the Fraction of the year corresponding to May
of May); the product of these numbers (1"408) is the
annual variation due to the period elapsed since January
the sign is +, to the Mean Right Ascension on Jan. 1,
4 26" 39"326, for the Mean Right Ascension on May 31,
of the Declination is + 7’°944, which multiplied by “411 as 1
duct (3""27) added, beewuse the sign is + and the peer
Declination on Jan. 1, 1838, viz. N. 16° 10° 40'-92, gives N. 16°
Mean Declination required:
Example 2. Required the Mean Right Ascension and Declination |
Miworts on June 2, 1838. Here the Annual Variation of Right A: J
and the fraction of the Year “416 (page XXII. of June); the
therefore being subtracted, because the sign of the Annual Vi
14" 51” 15" 220, the Right Ascension on Jan. 1, gives 14" 51" 1510;
Ascension on June 2, 1838,
For the Declination, we have the Annus) Variation =— "713,
plied by “416, gives 6’-12. The Declination being North,
Variation —, this product must be subtracted from N, 74° 49' 3°61, «
is N. 74° 48 57’ 49.
Example 3. Required the Mean Declination of « Sconru or Antares on
1838. The Annual Variation is — 8'°514, and the fraction of the Y
product of these numbers (3'"50) being added, because the 00 he
the sign of the Variation —, to the Declination on Jan. 1, wis. 5, 26° 35568
sum, S. 26° 3’ 59°59 is the Declination on May 31, 1838,
Next (page 365) follow Besecl’s Formule: of Reduction? and (pages 366 and 367)
a Table for the Reduction of Stars, independently of iene ey om
stants, an example of which is given at page 510. ‘ es
‘The apparent places of « ii pt ae Se oo of the
year, and those of the remaining 98 Stars for every tenth day. They
position which ought to be shown by perfect instruments at the time of the oe
transit over the meridian of Greenwich; and, therefore, supposing th
mean places to be correct, they serve to detect any errors of the
The hours and minutes of Right Ascension, and the degrees and niotiace
Declination, are placed at the heads of the columns as constants, and belong
equally to all the numbers below them, ‘This arrangement has rendered it necessary,
EXPLANATION. 517
in numerous instances, to continue the seconds beyond 60, as the width of the page
would not permit of otherwise indicating any change in the minutes. Thus, the ap-
parent Ascension of « Ontonts, at page 380, on December 17, 1838, is registered.
5" 27"64"05, and is to be read 5°28" 4°05, Again, the Declination of « Canis
Majoris (page 382), on the same day, is registered S. 28° 44’ 74-1, which
Brailes S. 287 45! 14-1,
‘The small figures on the right hand of the vertical columns of seconds represent the
differences of the quantities above and below them on the left, or the variation of
Right Ascension ond Declination in 10 daye, and serve to find, by interpolation, the
values for any intermediate day. As in the case of the Planets before explained, a
Star will sometimes arrive at the meridian twice in one Mean Solar day. Wherever
this occurs, an asterisk is placed opposite to the interval, and it signifies that the Star
has passed the meridian 11 times in the 10 Mean Solar days, and consequently that
the Right Ascension or Declination on any intermediate day is to be determined in
these particular instances by taking ,';th part, instead of y'yth, for the daily variation in
the interval. Thus, at page $85, we find in the instance of « Argus, an asterisk
opposite the interval between August J and 19, and a difference of 0°08 opposite to the
interval between the seconds belonging to those dates; we therefore infer that 11 transite
have taken place, and that the daily variation of the Right Ascension is 0*:007,
When extreme accuracy is required, the apparent places of the 5 Polar Stars demand
a further correction, depending on the terms which involye2¢. The apparent places
do not include these corrections, on account of the rapid variation of the argument,
viz. about 26° in a day, but they are given in a Table at pages 408, 409, for every
degree of the Moon’s Longitude, and may he readily applied, agreeably to the precept
at the foot of that Table.
Formule for correcting for daily aberration are given in the Preface.
Moon-Culminating Stars, (Pages 410 to 451.)
‘Those Stars are denominated Moon-Culminating Stars, which being near the
Moon’s parallel of Declination, and not differing much from her in Right Ascension,
are proper to be observed with the Moon, in order to determine differences of meri-
dians. ‘This is effected by comparing the differences of the observed Right Ascensions
of such a Star and the Moon's bright limb at any two meridians. If the Moon had no
mation, the diference of her Right Ascenslon from that of the Stax woul le eonetant at
all meridians ; but in the interval of her transit over two n
Ascension will hare, vanes, aul Ee betwee
comes up with the Moon; hence, and
"Porth daeenioaion of St
In the present List, however, the
ht ocr eee
wlll be onkl eel, 5
renee sae 5 snags reser
his mage cntsne emo Table, the fit showing
of the Moon's Aj feos ac eal ae
Discs of Venus and “apres belies a
‘ eee
Tides. (Pages 478 to 481.)
~ ‘The Mean Times of High Water at London Bridge are me seers
the year, on the assumption that the time of high water on
| the Establishment of the Port, is 7%. The first high tide
_ after Mean Noon of any day ir deer Sa the Let ‘eohanay eat Yn ect Sad
2nd column. Where a line (—) is inserted, it indicates that there is only one high
tide on that day. Thus on February 5 there is only ates \ Pale sea
11" 28", but the succeeding high tide does not take place 8" after mean
of February 6.
ripe ob penny nace Poomp edie tg tet A
481, are reckoned from represent the Establishments of the
Porls, pingrgeigiiwe ge ne eta ig aurea
dian at the same time as the Sun; or the intervals between the times of Transit
of the Moon and the-times of High Water on full ancl days. They serve
to determine the time of high water on any other day at places in the usual
manner. The time of high water, however, at any of the places contained in this
table, may be deduced for every day from the time of high water at) London Bridge,
by taking the difference between the establishment of the port at each of these places,
and the establishment of the port at London Bridge, viz. 2" 7", and considering this
a a constant quantity, representing the difference of the tides between London Bridge
and the place, to be added to, or subtracted from, London, Bridge tides, according as
the establishment'of ‘the port ef the piace, {a Jaler, or earlier thaw et at Laniion
Bridge. Thus the establishment Oe 12", and at Loudon
Bridge 2" 7" ; the difference is 0" 55", and the Aberdeen. tide precedes that at Lendoni:
therefore, by subtracting 0* 55" from the London Bridge tides, we obtain the Aberdeen
tides in mean time. On February 19, 1838, the first high water at London Bridge
occurs at 8" 35", which being diminished by 0" 55", gives 7" 40™ for the correspond
ing tide at Aberdeen, and so for other places.
Table showing the Co
BRPLANATION, =a
ERRATA.
(Continued from page 526 of the Nautical Almanac for 1837, London, 1835.)
I.—NAUTICAL ALMANAC FOR THE YEAR 1835,
First & Second Editions, (London, 1833 and 1835.)
Nye Sa Boer Dec. 25, ¥, for —0°9608 read —0-9008
APPENDIX.
Page 14, line 3, for (G) 619 read (G) 61°9 a
— —%— (G—0) — (G)-9o
Second Edition. (London, 1835.)
Page ix, line 21, omit with the Moon.
II.—NAUTICAL ALMANAC FOR THE YEAR 1836,
(London, 1834.)
Page vii, line 7, for 75°185 read 75 225
I1L—NAUTICAL ALMANAC FOR THE YEAR 1837.
(London, 1835.) :
Poge vii, line 10, for interpolated read
xii, University Terms, Cambridgy
29, Wednesday, Feb. 8, Right Ascensi
for 0% 0" 18°7L re
244, Dec, $2, Sidereal Time .
for wu
247, Dec, 24, Meridian Passnge
396, © Urew Minoris, R.A,
LONDON:
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