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THE QUARTERLY
JOURNAL OF SCIENCE.
CONDUCTED BY
Sir W. FAIRBAIRN, Barr, F.R.S.; WILLIAM CROOKES, F.RS.;
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OF THE MIDDLE TEMPLE, BARRISTER-AT-LAW,
EDITOR.
VOLUME VII.
dHith Allustrations ow Copper, Stone, and ddlood.
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THE QUARTERLY
JOURNAL OF SCIENCE.
JANUARY, 1870.
I. LIGHT AND SOUND:
AN EXAMINATION OF THEIR REPUTED ANALOGY.
By W. F. Barrerr, I.C.8., Natural Science Master at the
London International College, &c.
Lone before we knew anything of the origin either of sound or
light, the existence of an analogy between these forces had been
the subject of speculation by some philosophers. But the idea of
such an analogy did not originate in philosophy; it was not con-
fined to a few; it resulted in more than speculation. From the
earliest times we find among all nations a crude perception of a simi-
larity between sound and colour. This perception became rooted
in their languages. The same words, in many cases, were employed
to denote either light, or sound. A vivid impression received by
the eye was equivalent to a forcible shock received by the ear : thus,
the English “loud,” the French “ criard,” the German “ schreiend,”
are identical expressions, relating to sound, also applied to glaring
colours. FF aintness of vision and feebleness of voice were spoken of
as one. Our own words dim and dumb were probably cognate
terms in Anglo-Saxon.
It is easy to trace this correspondence in language much farther,
but that is not our present business. Let us inquire if this wide-
spread mental analogy between sound and colour rests upon a
physical basis. Is it true that light and sound are alike, and if so
in what way are they alike? How can the swift flash from a gun
be said to resemble the sluggish report that follows? Except
esthetically, where is the likeness between a painting by Raphael
and a theme by Beethoven ?
At the outset let us remark that no attempt will be made to
show the identity of light and sound: it is their resemblance, their
parallelism, and not, of course, their oneness we wish to establish.
A parallelism that probably is metaphysical as well as physical ; so
that the estimation of beauty of colouring and harmony of sound
may, hereafter, be found to resolve themselves into mental actions
VoL. VIL. B
2 Light and Sound. [Jan.,
essentially the same. Here, however, we have solely to deal with
the physical aspect of the question. In pursuit of our object it will
be necessary to compare the principal phenomena of light and
sound, and for this purpose it will be convenient to break up the
subject into sections. If the analogy be just, it will assuredly gather
strength as the comparison proceeds ; if it be false, then each section
cannot fail to force this fact upon the mind. In either case the
result ought to be profitable, if we simply seek the truth.
§ 1. Ortein oF Ligut anp Sounp.
Light and sound are both the products of vibratory motion.
But to evolve light the motion must be enormously swift, whilst to
produce sound the motion must be comparatively slow. In the
former case only impalpable molecules can be made to attain the
requisite swiftness—light is therefore a molecular motion of vibra-
tion. In the latter case visible masses of matter can be moved to
and fro with the necessary speed: sound is therefore usually the
product of a molar motion of vibration. Further, to continue the
light, or to sustain the sound, the to-and-fro motion must be per-
formed in equal times ; it must be zsochronous. If not isochronous
the light will be either intermittent or varying in colour, and the
sound will be either a noise or musical notes of varying pitch.
Now comes a remarkable point. Sound and even music are
usually produced by a disturbance very different from a vibratory
motion. If we hit a tuning-fork on our knee, strike the strings of
a piano, or pluck the strings of a harp, we produce music by rough
mechanical means ; so the noise of hammering, the roar of cataracts,
the whistling of the wind, or “the scream of a maddened beach,”
are all sounds, that is motions of vibration, produced by a rude
motion of translation. Light, also, can be evolved by similar
agency. ‘The rubbing of two pieces of quartz or sugar, the sparks
from a flint or steel, and the incandescence produced by the friction
of meteors against the air are familiar examples of light generated
by mechanical means.
How can we account for the transition from molar to molecular
motion, from an impulse, such as a blow, to a regular pendulum-like
swing? th of a
second apart. Similarly our ear cannot distinguish between a suc-
cession of similar sounds that follow each other at shorter intervals
than the ~;th of a second. Like the blending into one of the
colours on a spinning-top, the separate sounds link themselves
together and constitute a musical note.
Radiant sound and light being both wave-motions, many laws
are found common to both. When light falls upon a body it is
either transmitted, absorbed, reflected, refracted, or inflected. The
same phenomena can be observed when we substitute sound for light.
Let us briefly examine this remarkable series of analogies.
§ 4. Transmission or Light anp Sounp.
Through transparent bodies light is transmitted freely. But
if a series of transparent substances, each alternately differing in
density, be placed together, the progress of light is obstructed, and
may even be altogether stopped. Thus a perfectly transparent
block of glass, if reduced to powder, is perfectly opaque. Air, a
medium of different density, now intervenes between the particles
of glass, and the light echoed, as it were, from particle to particle
is so weakened that it cannot struggle through.
In the same way sound in its passage is enfeebled, or even
obliterated, if it pass through several media of alternately varying
* Savart: ‘ Annales de Chimie et de Physique.’
10 Light and Sound. | Jan.,
density. Wood transmits sound perfectly well, so does air, but
if the wood be reduced to sawdust, sound is no longer transmitted.
Thus cotton-wool deadens sound. Solid glass, salt, and ice, and
all transparent solids. transmit ight and sound; reduced to powder,
they are opaque both to sound and light. A glass of water trans-
mits both light and sound, so does carbonic acid gas; but if the
two be mixed, as in soda-water, a mixture nearly opaque to both
light and sound is the result. By tapping a glass of soda-water
during and after the effervescence the sound effect can readily be
heard. The bubbles of gas break up the continuity of the water
and render the sound emitted by the glass dull; when the bubbles
have escaped, the ringing note of the glass returns. The same
effect occurs in gaseous media. Humboldt, when journeying upon
the plains of the Orinoco, noticed that columns of alternately hot
and cold air enfeebled the passage of sound just as they lessened
the passage of light. In the same way through fog, sound, like
light, is propagated with extreme difficulty. The cause of this
arises from the particles of water that are then suspended in the
atmosphere, and by their presence produce variations of density.
It has too been generally noticed that a good hearing day pre-
cedes wet weather, and before a wet day we generally notice the
atmosphere becomes remarkably clear. This clearness has by an
eminent physicist * been attributed to the fact that on ordinary
days our atmosphere contains innumerable spores or germs floating
in the air. At the approach of wet weather the little germs absorb
the moisture, they become heavier and sink to the ground; thus
the atmosphere is cleared from these solid particles which at the
same time obstructed the free transmission of light, and interfered
with the free transmission of sound.
§ 5. Apsorption oF Licut anp Sounp.
A. black glass, or a black surface like velvet, absorbs the light
that falls upon it. The light, as already observed, becomes trans-
lated into heat in the absorbing body. Woollen textures, curtains,
and the like, are to sound what a dark glass is to light. Such
obstacles stop the progress of the sonorous pulses, and also convert
what was sound into heat. In the case of light there is further a
selective absorption of certain rays; this gives rise to the colour of
a body. Such selective absorption is a molecular act, probably due
to the synchronism between certain luminous waves and the oscilla-
tions of the particles in their path. Hence selective absorption can
only exist when there is a mixture of waves from which to select.
Transferring these ideas from particles to a body as a whole, a
corresponding selective absorption exists when there is a complex
* De La Rive.
1870. | Light and Sound. ii
source of sound. If a bundle of different tuning-forks be struck,
sonorous pulses of varying length will be emitted. Allowing this
composite pulsation to fall on a single quiescent fork, only that
pulse, which corresponds to the rate of vibration of the fork, will be
absorbed, and by this means the hitherto silent fork will be thrown
into vibration.
§ 6. Reriection or Lignt anp Sounp.
This is one of the best known, and at the same time one of the
closest analogies between light and radiant sound.
When a beam of light, 1, falls wpon a polished surface, m m, it
rebounds in the same plane, and at an equal angle on the other
side of an imaginary perpendicu- Re
lar, p, drawn from the surface of Ee,
the mirror. This is expressed by ; . i
saying the angle of reflexion is
equal to the angle of incidence. oe |
The same law is rigorously true .
for sound. It is easy to observe
this reflexion from the sides of a
cliff, a blank wall, or the roofs of ~
churches. Echo is due to this reflexion of sound. Standing be-
tween two parallel mirrors, successive and gradually fainter reflexions
of the body will be seen. The same is true with regard to sound, as
can be observed when speaking between two perpendicular walls,
sufficiently distant from each other.
Under certain conditions light is “internally or totally reflected,”
as it is termed ; that is, at a considerable obliquity of incidence light
cannot emerge from a dense medium into a rarer one: this may be
well observed when a glass rod is made red hot at one end, the
distant extremity glows by internal reflexion. In the same manner
sound can be internally reflected. When a sound made under
water strikes the surface of the water very obliquely, the greater
part of the sound is unable to escape into the air, owing to the total
reflexion occurring at the upper surface of the water.*
With curved reflectors sound is affected in the same way as
light. A sound-focus or a sound-image may be obtained by a con-
cave reflector. ‘The following lecture illustration of this fact was
shown by the writer two years ago at the Royal Society of Dublin.
Two parabolic mirrors ss were placed as in Fig. 3. At c, in the
focus of, s,a watch is suspended; in the conjugate focus c’ of
the other mirror, s, a sensitive flame was caused to burn. ‘The
flame moves at the slightest sound. The light rays rr from
y
ae A
N\
/
“YZ
TA
* This fact has been established by the experiments of Colladon and Sturm on
the Lake of Geneva.
12 Light and Sound. [Jan,
the flame are rendered parallel by s and converged upon the watch
by s, where a brilliant spot of ight is seen. Similarly the sound-
waves from the ticking of the watch follow the opposite course,
Fig. 3.
—,--§-----------------------—-----— —-—~---——- --——- —-- — — --— —- - ~~ -- - -- ----
SS en ee Se
and an acoustic focus is cast upon the flame. The flame throbs
in exact time with the beats of the watch. Moving the watch
or the flame nearer together places them out of the focus, and the
flame by its stillness announces the fact.
It is easy for any one to repeat this experiment with very
homely apparatus. Circular dish-covers of earthenware or metal
may be used as mirrors, and for the flame may be substituted a
little funnel with a short tube leading to the ear.
§ 7. Rerraction oF Ligor AnD Sounp.
Light on passing from a dense medium to a rare one, or vice
versa, 18 bent out of its original course. So also is sound. Light
may by refraction be converged and focussed by lenses. Sound-
lenses may also be made.* Filling a thin india-rubber balloon with
a dense gas, like carbonic acid, a double convex acoustic lens is
produced. By means of such an arrangement divergent sound
rays, from, for example, the ticking of a watch, can be converged
and focussed. Placing a sensitive flame in the focus, this refrac-
tion of sound may be rendered apparent to a large audience.
§ 8. Iyriection oF LigHt anp Sounp.
This is an effect produced upon divergent waves merely by the
presence of an obstacle in their path. When a sea-wave meets an
isolated rock it breaks, spreads itself around the rock, and clasps
itself again at a short distance behind. Thus only comparative rest
is found behind such a breakwater. Similarly a sonorous wave
meeting an obstacle, say a large pillar, girdles the pillar and thus
* As first demonstrated by Sondhauss.
1870. | Light and Sound. 13
partially destroys the sound-shadow which such a pillar would other-
wise throw. In former time it was urged that if light be a wave-
motion, there ought also to be inflection and only partial shade behind
an opaque object. The inflection of light has since been discovered ;
light does slightly encroach, in the form of fringes, upon the shadow
cast by an object. Nevertheless, owing to the rectilinear propaga-
tion of hight, shadow is a characteristic feature of light. Is there
an analogous sound-shadow? ‘There is, notwithstanding inflection.
If we pass close beside a church, the bells of which are ringing, we
shall notice that on coming beneath the tower we enter a region,
nearer the source of sound, yet where the sound is very perceptibly
less audible; and as we gradually emerge from this acoustic shadow
the sound grows louder. So also when listening to an approaching
train, as it is occasionally hidden from view, accompanying sound-
shadows flit across the ear. And in a more elastic medium than
air, such as water, sound-shadows would, necessarily, be more
intense and sharply defined.
§ 9. Harmony or Coztour anp Music.
It is in this division of our subject that we find a wide-spread
and tacit acceptance of the analogy of light and sound. We instinc-
tively criticize in like terms the works of a painter and a musician.
We speak of the harmonious blending cf colours in a picture, as we
do of the chords in a musical composition. We compare, apparently
without reason, the order of colours in a rainbow to the notes of the
gamut. Like Locke’s blind man who said scarlet was to him as
the deep sound of a trumpet, we think of red as a low note, of blue
as ahigh one. We find, as a rule, that good taste in art goes hand-
in-hand with good taste in music; hence a large number of eminent .
painters have been excellent musicians.* All this points to the
fact that pleasure given to the eye or ear evokes similar mental
impressions,
Now the question arises, Has all this esthetic oneness of colour
and music any physical foundation, over and above that general
analogy we have so far traced between light and sound? We believe
the following considerations will show not only that it has some
foundation, but that the analogy is far more wonderful than has
hitherto been suspected.
Let us take as our standard of colours the series given by the
disintegration of white light, the so-called spectrum. As our stand-
ard of musical notes let us take the natural or diatonic scale. We
may justly compare the two: for the former embraces all possible
gradations of simple colours, and the latter a similar gradation of
notes of varying pitch.
* Omitting many living painters, of whom this is true, it is sufficient to name
Tintorretto, Caracci, Salvator Rosa, Dominichino, Guido Reni, Leonardo da Vinci;
and Rubens also is said to have been passionately fond of music.
s
14 | Light and Sound. | Jan.,
Further, the succession of colours in the spectrum is perfectly
harmonious to the eye. Their invariable order is red, orange, yellow,
green, blue, indigo, violet. Any other arrangement of these colours
is less enjoyable. Likewise the succession of notes in the scale is
the most agreeable that can be found. The order is C, D, HK, F,
G, A, B.* Any attempt to ascend or descend the entire scale by
another order is disagreeable. The order of colours given in the
spectrum is exactly the order of luminous wave-lengths, decreasing
from red to violet. The order of notes in the scale is also exactly
the order of sonorous wave-lengths, decreasing from C to B.
The interval of wave-lengths embraced between the extreme
colours of the visible spectrum is ordinarily as the ratio of 1:0-57,
corresponding to the interval known as a seventh in music. But
the writer is well informed that by proper means further limits can
be seen, 222. from what is known as the solar line A to the solar
line L.t (See upper figure in Plate: L is not shown.) The wave-
length of A is 76, and of Lis 38 hundred-thousandths of a milli-
métre, or as the ratio of 1:0°50, corresponding to the interval of
an octave in music, or just the range of the scale.
Arbitrarily placing C under the colour at the solar line A, wiz.
a deep brownish red, then the octave higher of C would fall under
whatever colour is found at the solar line L, viz. a lavender grey.
Now comes this important question, Are the intermediate colowrs
of the spectrum produced by vibrations that bear a definite ratio to
the vibrations giving rise to the intermediate notes of the scale?
According to our knowledge up to this time, apparently not.
In an ingenious little work by Dr. Macdonald, before alluded to,
an attempt has been made to establish this analogy indirectly ; {
but if direct comparison fails, it is useless to push the matter
farther. Newton himself sought for this analogy between note
and colours, but he only found the relative spaces occupied by each
colour in the spectrum to be similar to the relative intervals of
musical notes. This is, obviously, a false analogy. We must
compare wave-lengths of light with wave-lengths of sound; not,
of course, their actual lengths, but the ratzo of one to the other.
Until very recently it has been impossible to do this accurately.
New maps of wave-lengths of the different parts of the spectrum
have, however, of late appeared.§ Let us reduce the newest and
best determinations of wave-lengths to a common ratio, and com-
* The fact that Newton saw seven colours in the spectrum, and there are seven
notes in the scale, is only an accident; the number of colours, or tints, entirely
depends on the judgment of the observer.
+ This is on the authority of Mr. Crookes, who has on favourable occasions seen
the spectrum extending this length, where a quartz train of lenses and prisms was
aie ie a pity this brochure of Dr. Macdonald’s is so disfigured by its typo-
graphy, it is also too speculative and dogmatic.
The most recent by Thalen. ‘Transactions of Royal Society of Upsala, 3rd
Series, vol. vi.; also ‘ Annales de Chimie et de Physique,’ Oct., 1869.
1870.] Light and Sound. 15
pare the result with the wave-lengths of the notes of the scale
reduced to the same ratio. Here are the limits of wave-lengths of
the different colours of the spectrum as most carefully determined by
Prof. Listing.* In the third column the writer has added the mean
wave-length of each colour, and in the fourth column the ratio of one
colour to another, taking the mean wave-length of red as 100.
TABLE OF WAVE-LENGTHS OF COLOURS IN THE SPECTRUM.
WAVE-LENGTHS: IN MILLIONTHS OF A MILLIMETRE.
ESE -
Name. Limit. Mean. Ratio.
FRG seh xe, hee 728. to G47. ae 685 fe 100
Orange .. .. 647 to 586 oe 616 aa 89
Vellow? "i209" so S66 to dad ae 560 zs 81
Green Yi 4s deo to 492 ie ala an 79
Bless oon 220 492) to 455 sis 473 sf 69
Indigo... .. 455 to 424 wn 439 “G 64
Violet 424 to 397 410 60
Here next is a table giving the middle notes of the scale, their
wave-lengths, and their reduction to a common ratio, taking C as 100.
TABLE OF WAVE-LENGTHS OF NOTES OF SCALE,
Wave-length
Name. in inches. Ratio.
Ops e 52 100
iD ue 461 89
Hi, 42 80
Beeps 39 79
Ge. 35 67
2s tal 31 60
Bis: 272 53
Cl: 26 50
Putting together the two ratios, the following remarkable cor-
respondence at once comes out :—
RATIO OF WAVE-LENGTHS OF NoTES COMPARED TO RATIO OF WAVE-LENGTHS
OF COLOURS.
Notes. Ratio. Colours, Ratio.
CH. . 100 bd sae UCI Skt eg ee LOO
Dis. 89 Baek icais Orange Sap ears.
io gargs 80 cae, ae Vellowis ae 9.2 SL
ig: 75 BaD cy Greene. Td
G.... 67 Beth pete Blue and mae 67
(mean) :
fee ee 60 LAacane Wiolete ke) a. se) GO
Lier 53 on Ae [Ultra violet .. 53]
GAs 50 EN (POpscnre.. wee. <> BO]
Assuming the note © to correspond to the colour red, then we
find D exactly corresponds to orange, E to yellow, and F to green.
Blue and indigo, being difficult to localize, or even distinguish in
the spectrum, they are put together: their mean exactly corre-
sponds to the note G. Violet would then exactly correspond to
* Poggendorff’s * Annalen,’ vol], cxxxi., p. 564.
16 Light and Sound. [Jan.,
the ratio given by the note A. The colours having now ceased,
the ideal position of B and the upper C in the spectrum are calculated
from the musical ratios. This coincidence, as unexpected as it is
perfect, is represented in the two upper figures on the Plate.*
Had space permitted, we should have ventured to trace out to
some extent this common harmony of colour and sound. All we
can do is to point out a few suggestions that occur at once.
Every one knows that the juxtaposition of two colours nearly
alike is bad, and it is well known that two adjacent notes of the
scale sounded together produce discord. Selecting and sounding
together two different notes we may produce either discord or
harmony; so with the juxtaposition of certain colours, either
pleasurable or painful effects are produced. Thus—the notes D and
E, together, are bad; so are orange and yellow when contrasted.
C and G harmonize perfectly, so do red and blue. C and F is an
excellent interval, so is the combination of red and green. Now,
on referring to the Plate, it will be seen that the foregoing notes
exactly underlie those very colours that we have named with them.
But, further, it is possible to obtain a real optical expression of
the musical intervals.t| By refiecting a beam of light from one
vibrating tuning fork to another placed at right angles, curves of
light are obtained, which vary according to the combination of forks
we select.: The most perfect harmony, viz. two notes in unison,
gives the simplest curve—a circle. The next most harmonious
interval, an octave and its fundamental note, gives the figure of 8;
the next, the interval of a fifth, gives a more complete figure, and
soon. The complexity augmenting as the ie lessens. Some
of these curves are shown on the lower figure in the Plate. By
the side of each curve is put the musical notes from which it was
derived, and for the sake of comparison the colours which would
correspond to each interval are also brought down. It will be
seen that harmony runs throughout.
A musical chord thus becomes both a representative picture,
and an acoustic painting, whilst the musical scale is literally a
rainbow of sound. It is hardly too much to say that we might
possibly translate into a musical melody a sunset, a flower, or a
painting by a Rubens or a Raphael.t
But here let us check our imagination. We have throughout
the foregoing article endeavoured to avoid overstating the analogy.
Let us now be careful lest we become victims of the “ zdola tribus,”
lest we strive to impose on nature a greater degree of simplicity
than her facts will justify.
* There will be noticed over the spectrum on the Plate ascale of actual wave-
lengths, by which the remarkable but natural crowding together of the colours at
the red end is well seen.
+ First accomplished by M. Lissajous.
+ On this subject an able article by Mr. C. Seth Smith, recently appeared in
the ‘ Builder.’
be wien
1870. | Ny ae
II. ON THE PRINCIPLES AND METHODS OF
SEWAGE IRRIGATION,
=A KWAGE utilization is perhaps one of
the most hotly-debated subjects of the
day, and frequent references to it have
from time to time appeared in the
pages of this Journal. These will be
found repeatedly in the Chronicles of
Science (Agriculture), and in two ar-
ticles, entitled respectively “Sewage
and Sewerage,”* and “On the appli-
cation of Sewage to the Soil,”} wherein
\| the progress made in the development
| of works for sewage irrigation purposes
has been recorded. Our present object
is to give a brief account of the best
means for carrying out irrigation works
| for the disposal of town sewage, and
of the laying out of lands preparatory
to the application of sewage, so far as they can be deduced from the
results of past experiments, and from works hitherto constructed
and brought into operation in different parts of the United King-
dom. We shall, however, preface our remarks on the above-named
subjects by a reference to one or two points in connection with
them, with the view to show that the present movement in favour
of utilizing our town sewage is but the revival of a practice of great
antiquity, which, owing to numerous causes, has, for many cen-
turies, been abandoned and perhaps forgotten.
The recognized power of earth to act as a disinfectant may first
be traced to the Mosaic lawgiver, but it is not improbable that it
was applied to that purpose before the departure of the Israelites
from Egypt, and that the injunction for it to be so used whilst they
were on their wanderings was but a law for the observance of a
then well-known sanitary precaution. The filth of Jerusalem was,
it is recorded, at one time burnt in an oven in the valley of Hinnom,
which also served for human sacrifices, and was called “tophet, :
from “toph,” a drum, used on such occasions to drown the cries of
the victims. Ata later period, however, when the Mosaic religion
was restored, the Temple purified and rebuilt, and the country began
to prosper under the protectorate of powerful neighbouring nations,
large sewers and aqueducts were constructed, which still exist,
owing to the fact of their being cut in the solid rock upon which
the city was built. Eusebius, who was a native of that country,
* * Quarterly Journal of Science,’ 1866, p. 180. + Ibid., 1867, p. 357.
VOL. VII. C
18 ; On the Principles and Methods | Jan.,
and died about the year 340, mentions Timocrates, the surveyor of
Syria, by whom the city was throughout provided with water. The
water used for flooding the court of the Temple, to wash away the
offal and blood of the sacrifices, drained into a pit, now called “ The
Fountain of the Virgin;” from whence, after mingling with the town
sewage, it was conducted to a second one, now called the Pool of
Siloam—but which, it is thought, is not the one formerly known by
that name— and thence to the king’s garden, for purposes of irriga-
tion. These pits served, no doubt, as settling-tanks to collect the
solid matter; and thus, in their general arrangement, we can per-
haps trace the earliest recorded attempts at utilizing sewage, and
one which, so far as our information goes, does not appear to have
differed materially from the most approved practice of the present
day.
"The difficulty in getting rid of night-soil and refuse im large
towns by any other method has necessitated the adoption of
sewers and water-carriage for that purpose, and with our present
knowledge on the subject it does not appear probable that sewers
will ever be superseded. “It matters not,” remarked Mr. Bailey
Denton in a recent letter to ‘The Times’* newspaper, “ whether the
earth-closet system of excretal sewerage gains ground in places
where advantageous circumstances suggest its adoption, sewers
must exist in every place where habitations are congregated toge-
ther, whether it be a city or a village, for the discharge of liquid
refuse from the chamber, the bath, and the kitchen, independently
of the excrements of the closet, which form in reality but a small
proportion of the entire refuse of the dwelling.” The introduction
of sewers in places has, as might naturally be expected, led to their
being used also as drains, and the result appears to have been satis-
factory, although the reports by the Medical Officer of the Privy
Council tend to show “that where a system of separating the sew-
age of dwellings from the water of the soil on which they stand has
been adopted, and the sewerage and drainage can be discharged by
different channels, the maximum of success may be achieved.” On
the other hand, Mr. Denton states that “wherever sewerage and
drainage—which have different sanitary effects, and ought to be
distinct operations—have not been carried out together, intention-
ally or accidentally, the operations have failed, more or less, in the
purposes for which they were designed.”
The mixture of water with sewage is looked upon by some
agriculturists as a great drawback to its application. Apart, how-
ever, from water-carriage being the cheapest, as well as the most
convenient form of removing the sewage of towns, it is of value in
distributing it, and enables the operation of spreading solid manure
over the face of the earth, which must otherwise take place, to be
* «Times, October 28, 1869.
1870. | of Sewage Irrigation. 19
dispensed with. By the process of irrigation, too, fertilizing matter
is distributed over the land with uniformity, and it is presented to
the plant in such a state that it is at once ready to be assimilated,
that is, it is at once food for the plant; the plant grows more ra-
pidly, the period of growth is greatly shortened, and, consequently,
we get a greater number of crops in a given period, under the
irrigation system, than could possibly be obtained under any pro-
cess of dry manuring. The quantity of water mixed with the solid
matters in the ordinary sewage of towns is very great, and it has
been estimated that, including rainfall, 350 parts of water are em-
ployed in removing one part of excrement; thus the sewage is
delivered to the land in a very diluted state, but, as has been
proved by results, by no means too weak for useful application.
The strength of pure sewage would be far too much for vegetation,
and, instead of improving it, would tend utterly to destroy it; but
thus diluted it is reduced to a state in which it appears to be most
readily absorbed by the earth, and thence taken up by plants as it
is required for their nourishment.
In order to meet the requirements of local circumstances, where
land is not available for purposes of irrigation, attempts have from
time to time been made to separate the solid particles from the
fluid, the former bemg made into a species of artificial manure,
whilst the latter is allowed to pass away into the most convenient
channel for its escape. The value of the manurial ingredients held
in solution, being to that contained in the solid portions as six to
one, the great fertilizer ammonia also being afloat in the liquid
portion, it is not to be wondered at that these experiments have
invariably failed, and the works erected for carrying out the
different processes have, almost without exception, been abandoned.
After filtration, the general plan has been to mix the solid residuum
with dry rubbish, town ashes, charcoal, or other bases for forming
a solid substance; the unwillingness, however, of farmers to pur-
chase this manure at a remunerative price to the manufacturers,.
and often their refusal to pay for it at all, necessarily led to the
early closing of all works constructed for the purpose of its manu-
facture. .
In order to counteract the loss of valuable manurial ingredients
which, under the above processes, passed off with the liquid por-
tions of the sewage, recourse was next had to the use of chemical
reagents with the view of causing a precipitation of those fertilizing
ingredients which are held in solution, and for this purpose use
has been made of lime, sulphate of alumina, soluble phosphate of
magnesia, perchloride of iron, &c.; but as none of these have been
successful in causing a precipitation of ammonia, or any other
manuring substance, it is needless to enter here into any further
details regarding these experiments. Suffice it to ei no
C
20 On the Principles and Methods | Jan.,
attempt hitherto made to extract a useful manure from sewage
which could be applied in a solid form has proved anything but a
failure.
The Commission appointed by the British Association to report
“On the Treatment and Utilization of Sewage,” states, with refer-
ence to the treatment of liquid sewage, that at fifteen of the places
which are sewered, wholly or partially, the liquid sewage is sub-
jected to treatment either by allowing it to remain for a time in
settling-tanks, from which the deposit is occasionally removed, as
at Burton-on-Trent, Birmingham, Epsom, Farnham, and Andover,
or by filtermg, as at Uxbridge and Ealing. In eight stances
deodorizing materials are added, such as lime and carbolic acid, as
at Carlisle and Harrow. Lime alone is used at Leicester; lime
and chloride of lime at Luton ; perchloride of iron at Cheltenham ;
perchloride of iron and lime at N orthampton ; ferruginous clay
wetted with sulphuric acid at Stroud ; and at Leamington the lime
treatment has lately been superseded by the A, B, Cc, method pro-
posed by Messrs. Sillar and Wigner. By this treatment the
sewage is clarified, and a deposit is separated which is sold as
manure.
In regard to the effects thus produced, it is stated that at
Leicester the sewage runs off as pure as ordinary rain-water; at
Ealing it is said to be free from smell, colourless, and harmless to
vegetable or animal life; at Stroud and Luton the effect is stated
to be satisfactory ; at Harrow the nuisance is said to be somewhat
mitigated ; and at Abergavenny the stench is said to be abated by
the treatment of the sewage; at Bury St. Edmunds upward filtra-
tion through charcoal and gypsum has been abandoned in fayour of
costly irrigation; at Banbury treatment of the sewage has failed ;
at Hereford, where it was proposed to be adopted, it has not been
tried on the score of expense; at Tunbridge it is about to be tried ;
and at Hastings and Cambridge experiments are being made. ;
With regard to the relative advantages of solid and liquid
manure, supposing even that all the fertilizing properties of sewage
could be retained in a solid form, we cannot perhaps do better than
to quote the following extract from the ‘ Minutes of the General
Board of Health relating to Drainage and Sewerage of Towns, &c.,
1852, by whom the question seems to have been satisfactorily set
at rest :—“ It is established by wide general experience that drained
land does not deteriorate, but increases in fertility, and maintains
its increased fertility from year to year, though washed through
and through by all heavy falls of rain carried away by the drains.
The rationale of this fact was displayed in the experiments prose-
cuted by Professor Way, which show that upon the application of
manures in the liquid form the fertilizmg elements do not escape
through the soil, but are retained by it chemically. On the other
1870. ] of Sewage Irrigation. 21
hand, where manures are applied as top-dressings in the solid form,
it is proved by experience that after heavy showers of rain the solid
manure is washed away, bodily as it were, into the ditches and
watercourses; so that whilst the outfalls from land top-dressed
and undrained are turbid with the matter carried away, and com-
plained of as a nuisance, the outfalls from drained land, richly
manured with the liquid, discharge pellucid streams.”
Liquid sewage has a special value distinct from the fertilizing
matter it contains, and also from the water that transports it; and
this is its temperature. The value of this peculiar property cannot
be over-estimated in a country similar to this, in which extreme
changes of atmospheric temperature often take place suddenly, and
injuriously affect both plants and animals, and this is more particu-
larly demonstrated in the depth of winter and during long and con-
tinuous frosts. “It is a rather remarkable circumstance,” observes
Mr. Baldwin Latham, “that when the greatest degree of tempera-
ture is required the sewage possesses it, that is, the temperature of
sewage has been found by the author to increase with the period
of duration of frost. This is probably owing to the stagnation of
surface-water, and also to the habits of the people, as much less
cold water is used in the depth of winter than at other times. So
great is the value of temperature, that a crop under sewage irriga-
tion may be seen growing eyen at the time of a severe frost.”
It does not appear that there exist any soils to which sewage
irrigation may not be beneficially applied. That portion of the
Craigentinny Meadows at Edinburgh known as Figgate Whinns,
consists of absolutely pure sand, whilst the soil of other parts is a
good loam passing into a strong clay; the former, which was
originally worthless, now produces grass crops which sell at
from 20/. to 287. per acre per annum, thus showing that no land
can be too poor for profitable cultivation where liquid sewage is
obtainable in sufficient quantity. A larger amount of sewage
is required for light than for heavy soils, particularly during the
first year of its application; and clay appears of all others to possess
the peculiar property of separating the manurial ingredients more
completely, and of retaining them better, than any other soil, and
it is consequently found that the crops grown are much heavier,
and that altogether clay soils produce a far better result than those
of a light, sandy nature. Gravelly soils require a certain time to
become thoroughly saturated with the sewage, and absorb it
greedily while the operation is in progress.
The value of a good system of drainage in all agricultural land
is sufficiently understood at the present day; but if it be beneficial
under ordinary circumstances, it is absolutely necessary where irri-
gation is adopted, especially in heavy soils. “I have no doubt,”
says Mr. Denton, in the letter above referred to, “that in cases of
22 On the Principles and Methods | Jan.,
sewage applied by way of irrigation to the surface of undrained
clay land, or to water-logged free soil lacking natural drainage, the
earth will become sodden, and liable to create a malaria; but with
a perfect system of under-drainage (designed with relation to surface
irrigation) at the first description of soil, and natural drainage in
the second, sewage-irrigated land may be rendered perfectly harm-
less.” From time to time complaints have been raised that land
irrigated with sewage-water was offensive to the surrounding
neighbourhood ; the observations of the British Association Com-
mission, however, tend to prove that in most cases the application
of the sewage for irrigation has not been attended with any apparent
change in the sanitary condition of the district, whilst in several —
instances there has been a marked improvement. Generally speak-
ing, too, no objection appears to have been made to the application
of sewage in this manner, and where such objections have been
made, on the ground that the application was offensive and in-
jurious, they do not appear to have been supported by medical
authorities, and in several instances they have ceased. .
The quantity of sewage that may be applied with advantage to
an irrigated area in the course of the year has been closely investi-
gated by Mr. Latham, and as the results of his calculations agree
entirely with the experience obtained at Croydon, and with the
experiments made by the Sewage Commission, we give them here
as being probably the closest approximation to exactness yet ob-
tained. Where it is considered desirable to apply as much sewage
as will be sufficient for the growth of a grass crop, without drawing
on the resources of the soil, 3645 tons of sewage per acre per
annum will be required to grow 30 tons of grass, 4860 tons of
sewage for a crop of 40 tons of grass, and 6075 tons for one of 50
_ tons of grass. If, however, the soil will provide half the potash
required, then, to grow 30 tons of grass per acre, there will be
required 1837 tons of sewage; to grow 40 tons of grass per acre,
2450 tons of sewage; and to grow 50 tons of grass per acre, 3062
tons of sewage. As 40 tons of grass per acre may be considered as
easy of production on a properly-regulated irrigated area, and as it
would not be desirable to exhaust the soil of any of its constituents,
Mr. Latham considers that 4860 tons per acre may be said to be
the right amount of sewage, and this closely assimilates with the
conclusions arrived at by the Sewage Commission, who reported
that 5000 tons of sewage per acre per annum was the right amount
to apply im order to get the greatest results.
The actual value of town sewage yet remains, to a certain
extent, an open question, but it may be accepted as a universal
rule, that only under the most exceptionally favourable circum-
stances can the sale of it afford any adequate return upon the cost
of constructing sewage works; so that, however profitable its use
1870. | of Sewage Irrigation. 23
may be to the farmer, it cannot be relied upon as a source of much
income to the town whence it is obtained. The theoretical value
of sewage has been calculated by some of our most eminent
chemists and others, and the results arrived at vary from ld. to
upwards of 2d. per ton. Practically, however, it has been found
that this is too high, and that its real value—that is to say, the
price which a farmer could afford to pay for it—does not exceed
from $d. to 1d. per ton, and in estimating the probable returns from
the sale of sewage it will always be safer to adopt the lower figure.
| The cost of the application of sewage for irrigating land appears
to be dependent on a number of local conditions, and, consequently,
to vary considerably. It would seem, from the data collected by
-the Commission appointed by the British Association, that in many
instances the outlay requisite for this purpose would exceed what a
farmer could be expected to incur, and that in such cases, at least,
it would be proper to regard this outlay as coming under two
distinct heads, wz. that which a town may reasonably be expected
to bear for the mere object of getting rid of its refuse, and that
which a landowner or farmer may be able to incur for the improve-
ment of his land. It is probable that when viewed in this light
the application of liquid sewage to land would become a source of
revenue to towns only under special favourable circumstances, but
that, in opposition to the opmions which have been somewhat
hastily formed in certain cases, it will more frequently entail some
amount of expenditure on the towns themselves. At the same
time the benefit to land and the improvement in the condition of
rivers to be realized by this mode of dealing with liquid sewage
can scarcely be matter of doubt or uncertainty any longer.
For carrying out a system of irrigation it is necessary, of
course, that the sewage should, in the first place, be brought by
channels or drains to the neighbourhood of the fields to be irrigated,
where the more solid parts are separated from the liquid by allow-
ing it to settle for a time, or, as is more generally the case, by a
coarse system of filtration. For the distribution of the liquid, four
different methods have been applied, wiz.: 1. That known as the
hose and jet system. 2. Sub-irrigation, or the distribution of
the fiuid below the surface of the ground. 3. By means of surface
channels. And, 4. By total submersion. In deciding, however,
which is the best system for distributing sewage, two things should
be kept in view: the first is that all arrangements for its distribu-
tion should be as simple and inexpensive as possible; and the
second, that owing to the constant quantity of sewage to be dealt
with, the arrangements must be capable of being worked at all
times and seasons. With these preliminary remarks we proceed
now to describe briefly the principles upon which the different
methods of distribution, above referred to, are carried out.
24 On the Principles and Methods | Jan.,
1. The Hose and Je& System.—The fatal objection to this
system is that it is not capable of application at all seasons. In
laying out works for the purpose, the sewage must, in the first
instance, be brought into the field by means of underground pipes,
which must also be laid in a sort of network over the whole grounds
to be manured, to which pipes with couplings or hydrants for
attaching a hose are fixed at certain points (see Vignette). In all cases
where the hose and jet system is applied, the sewage must be deli-
vered under pressure to enable it to be distributed over the field at a
considerable altitude above its surface, as well as to overcome the
friction in the pipes, and a head of from 10 to 12 feet is necessary
where the sewage is delivered by the force of gravitation. Where
a natural fall cannot be obtamed, pumping becomes necessary, and
this adds considerably to the cost. One great objection to the hose
and jet system is that sewage cannot be applied to crops by it
except at the earliest stages of their growth, owing to the necessity
for dragging long lengths of hose over the land; it is therefore
quite inadmissible when the crop has grown to any considerable
height. Besides, by this mode of application the sewage is sprinkled
over the crops, falling upon them as a shower, instead of being
applied to the roots, which, though it would be unimportant and ©
harmless were pure water only used, becomes actually injurious to
vegetation in the case of sewage irrigation, by leaving certain de-
posits upon the leaves and stems of plants, which clog their pores
and check growth. The system has enjoyed a partial success on
the farms of Mr. Alderman Mechi and Mr. Nelson, but at Rugby,
and other places, it has totally failed, and been abandoned. Mr.
Rawlinson has stated that it would cost more to distribute 500 tons
of sewage per acre by the hose and jet than it would to apply
5000 tons by surface channels.
2. Sub-Irrigation—Under this system porous pipes, or tubes
perforated with small holes, are laid under the ground at such a
depth as to be beyond the reach of the plough, through which the
sewage-water is forced. In some instances the pipes that are used
for drainage may be made use of for this purpose by merely stop-
ping up their outlets during the time that they may be required
for irrigation, by which means the water will be dammed back
until it reaches the upper stratum of the earth and the roots of
the plants. This system has been practised in Switzerland to a
limited extent; it is, however, expensive, and is open to the objec-
tion that it tends to raise the water in the land to the level of the
soil, and the earth thus becomes water-logged, in addition to which
it is attended with a great waste of fertilizing matter owing to the
depth at which the sewage is delivered below the surface, a part
of it gravitating still lower into the earth, and only a portion
reaching the roots of the plants.
1870. | of Sewage Irrigation. 25
3. Surface Channels.—For the purpose of distributing sewage
by means of open carriers, or surface channels, it may, if desirable,
be brought to the head of every field in a covered channel, or it
may be permitted to flow through open ditches, as may be most
convenient. This system, which is the simplest and most effectual,
may be carried out in various ways, according to the configuration
of the land. By it sewage can be at all times applied to the plant,
as it merely runs in a thin film over the surface of the ground at
its root ; but in all cases it is necessary that the land be specially
prepared for the sewage by careful levelling, and otherwise accord-
ing to its natural contour. This may be done in three ways, which
are respectively known as the pane and gutter system, the catch-
work system, and the bed system. The pane and gutter system is
the best, and is admissible in all fields having a gentle rate of
inclination. The land under this system is laid out, transversely
between the open carriers that distribute the sewage, quite level ;
the sewage is brought to the head of the field in an open or covered
main carrier running transversely across it, or in the direction of
its least fall; the carriers for distributing the sewage branch out
from the main carriers and run down the field in the direction of
its greatest fall; the sewage is distributed over the intervening
space between the distributing carriers by means of stops or sluices
(see Fig. 1) being placed in the carriers, which dam back the
@o
sewage and make it flow right and left over the ground in a
|
ve the ia passes from the main carriers into the secondary
Fia. 2.
Pane and Gutter.
carriers at a (Fig. 2), which being dammed up at certain points
are caused to overflow, the surplus water being carried away by the
26 : On the Principles and Methods : [ Jan.,
discharging drains B. A fair slope for this plan is from 1 in 100 to
1 in 120, or thereabouts.
The catchwork system is suitable in all cases where the ground
has a rapid rate of inclination, as, for instance, on the side of a hill.
lt consists of a series of carriers one above another, as illustrated in
Fig. 3. The sewage, flowing into the first and highest carrier, falls
over the intervening land between it and the next lower carrier,
which then takes up the water to distribute it in the same way on
the land below it, and so in turn the process goes on till the bottom
of the field is reached.
Fic. 3.
Catchwork.
The sewage is first received at a, and flows over the ground to
B, thence to c, and it is finally conveyed away by the trough or
cafrier D. ‘The carriers in this case may be cut at a distance from
each other of from 35 to 40 feet. As to the slope itself, 1 in 12
would be found a good limit, although 1 in 4 or 5 has not been
considered too steep.
The bed system is well adapted for level lands, or where there
is but a slight fall. On this plan the land is laid out im a series of
ridges and furrows ; the sewage is admitted into carriers which run
along the summit of each ridge, and falls over the incline into the
furrow below. This will be readily understood from the annexed
plan and description, Fig. 4.
A represents the ridge carriers which receive the sewage from
the main carriers, running at right angles to them at the head of
Fic. 4.
A
Ridge and Furrow.
the field, and B shows the carriers in the furrows which are con-
nected with the discharging drains. The sides of the slopes are
carefully levelled to an inclination of about 1 in 120, and the ridges
may be placed at an average distance of from 30 to 80 feet apart,
according to the crop put into the ground.
1870. | of Sewage Irrigation. 27
4, Total Submersion.—The method of carrying out this system
is by raising a bank round the field to be irrigated, and then turn-
ing the water into it, where it is left until absorbed or evaporated,
being from time to time replenished as may be necessary. It is
extensively carried out in Piedmont and Lombardy in the cultiva-
tion of rice, and, unlike any other, it 1s the only system of irrigation
that is considered likely to affect the health of the imhabitants in
the immediate neighbourhood of its operation, its special drawback
being that it converts every field where it is practised into a swamp
of the worst possible description.
In conclusion, we may give the following short particulars re-
garding the selection of crops to be cultivated by sewage; on this
point, however, more experience is required, as, owing to the greater
facility by which it can be applied to grass, but few experiments
have been made for its use with other crops. Fast growing, succu-
lent grasses appear to be the favourite crops, and especially Italian
rye-grass, of which crops varying from 30 to 50 tons to the acre
may be obtained annually ; and on one occasion as much as 61 tons
were obtained in the year at the Lodge Farm, Barking. At Rugby
some experiments have been made in the growth of oats, and the
results reported to be of a most satisfactory nature. At Barking
a couple of roods of land were ploughed up, irrigated with sewage,
and sown with wheat; whilst a similar quantity of land, not
irrigated, was also sown. ‘The yield of the sewaged land was
exactly 14 time that of the land which was not so treated. Mangold
wurzel has been grown with excellent results at Chelmsford, and at
Barking the average return has been 50 tons per acre, just double
that grown upon unsewaged soil. Winter greens, lucerne, beet,
flax, celery, and cabbages have all been grown upon the farm at
Barking, and have produced returns beyond all expectation, the
onion being the only plant that evinced any repugnance at being
treated with sewage. |
Experience has now shown us that town sewage is not a
refuse, and that allowimg it to fall into the nearest rivers, or into
the sea, is nothing more nor less than wilful waste, to such an
extent as to amount to a national loss, to say nothing of the con-
sequent diminution of food which ensues by the destruction of fish.
Few towns are so situated as not to be able to dispose of a portion,
at least, if not the whole of their sewage upon adjoining lands, and
where this is the case no more economical plan for getting rid of
it has yet been devised. Where such accommodation is wanting
it may be found necessary to have recourse to some one or other of
the artificial means of deodorization to which we have already
referred ; for although attempts to extract, by this means, a really
valuable solid manure have hitherto proved unsuccessful, it would
be unreasonable to draw the conclusion that means will not, sooner
28 The Solar Eclipse of August last. | Jan.,
or later, be discovered whereby all the fertilizing properties of town
sewage may be separated from the water, and made available for
disposal in the shape of solid manure.
The following is a list of the works referred to in the foregoing
article :—
1. Reports of the Commission appointed to inquire into the best
mode of distributing the Sewage of Towns, and applying tt
to beneficial and profitable uses, dated March, 1858, August,
1861, and March, 1865. Printed by Parliament.
2. Reports of the Commissioners appointed to inquire into the best
means of preventing the Pollution of Rivers, dated March,
1866, May and August, 1867. Printed by Parliament.
3. Lectures on Drainage, Sewage Irrigation, Water-supply, and
Water-works, delivered at the Royal Engineer Establishment,
Chatham, during the Autumn Session of 1867. By Baldwin
Latham, C.E.
4. The Sewage Question. By Frederick-Charles Krepp. London :
Longmans, Green, & Co., 1867.
. The Purification and Utilization of Sewage. By Baldwin
Latham, C.E. London: E. and F. N. Spon, 48, Charing
Cross, 1867.
6. Sewage, and its general Application to Grass, Cereal, and Root
Crops. By Thomas Cargill, C.E., &c. Robertson, Brooman,
and Co., 166, Fleet Street, London, 1869.
. A Short Account of the Modes of Sewage Disposal in some of
the Chief Towns in England. By Capt. T. I’. Dowden, R.E.,
1869.
8. Report on the Treatment and Utilization of Sewage by Com-
mission appointed by the British Association, 1869.
or
~]
Ill. THE TOTAL SOLAR ECLIPSE OF AUGUST LAST.
By Wiiu1am Crooxss, F.B.S., &e.
Tur important observations which were made last year with the
spectroscope, polariscope, and photographic camera caused the total
solar eclipse which took place on the 7th of August, and was visible
over the greater part of North America, to be regarded with more
than ordinary interest, as it was anticipated that the few minutes’
opportunity then afforded would enable several points left. doubtful
last year to be satisfactorily cleared up.
SPECTRUM OF THE PROTUBERANCES.
will a
We §
Yi EMS 2 &
SPECTRUM OF THE CORONA.
PROF® . YOUNG.
SPECTRUM OF THE AURORA BOREALIS
MR WINLOCK.
/
;>
17
!
THE TOTAL SOLAR ECLIPSE OF 1869.
1870.] The Solar Eclipse of August last. 29
Commencing at noon in Alaska, the line of totality ran through
British America, passing through the south-west corner of
Minnesota diagonally through lowa, crossing the Mississippi
near Burlington, thence through Illinois, West Virginia, and
North Carolina, and entering the Atlantic Ocean on the North
Carolina coast, near Beaufort. The path of the eclipse through
the more inhabited parts of the continent literally bristled with
telescopes ; the whole line being converted into one vast observatory.
Although the duration of totality was less than in India last year,
the circumstances were more favourable for observation, the heat
being less and the position of the sun more convenient for observa-
tion, instead of bemg almost vertical. The principal points which
had to be observed were the nature of the protuberances, examined
with the spectroscope and recorded photographically ; the nature
of the corona; and the detection, if possible, of any intra-Mercurial
planet. As might be expected from the easy accessibility of the
entire line of totality, this eclipse has been most thoroughly observed
by numerous parties, the report of whose work will in due time be
presented to the scientific world.
The most important observations were those recorded by the
Iowa expedition, towards the expenses of which 5000 dollars had
been voted by Congress. ‘The writer has to thank his friend, Dr.
Henry Morton, Professor of Chemistry in the University of Penn-
sylvania, who had the superintendence of this expedition, for full
details of the results obtained, together with some exquisite photo-
graphs of the phenomena of totality, &c. These pictures show, in
the first place, very fine definition in the telescope employed, as the
roughness or mountainous character of the moon’s edge is clearly
given in the pictures of partial phase, as well as the sun-spots and
surrounding facule.
The telescopes which were available for the purpose were two
fine Munich Equatorials, of 6 inches aperture, with clockwork, and
also an excellent Dolland, of 4 inches aperture, equatorially mounted,
but without clockwork. It was concluded that on account of the
risk of local clouds it would be desirable to take all these instru-
ments, and distribute them over some distance on or near the
central line, and it was also considered that at least five skilled
operators would be necessary to each instrument. The next
important point was the choice of the party, and it was soon
found that an excellent selection might be had from among those
whose position or engagements would allow them to volunteer
without other compensation than the moral one contingent on
success; and after a few changes, rendered necessary by sickness
or other inevitable cause, the party as finally constituted consisted,
besides Professor Morton, of Professor A. M. Mayer, Ph.D. ;
Professor C. F. Himes, Ph.D.; Messrs. J. Zentmayer, O. H. Willard,
4
30 The Solar Eclipse of August last. | Jan.,
EK. L. Wilson, H. C. Phillips, E. Moelling, J. C. Browne, W. J.
Baker, James Cremer, H. W. Clifford, O. H. Kendall, J. Mahoney,
and W. VY. Ranger.
It was a question of some moment to decide whether, for
obtaining the photographic records, they should follow the plan
adopted by the French and German expeditions of last year, and
take the photograph in the principal focus of the object-glass, thus
securing great intensity of light in a small image, or follow the
method employed by Dr. De la Rue in 1860, when he used an
ordinary Huygenian eye-piece so placed as to produce an enlarged
image of the first image from the object-glass. It was found by
experiment that with a clear sun it was necessary to reduce the
aperture of the telescope (which was 4 inches, and 50 inches focus)
to 14 inch, and to use a diaphragm slide of oth inch aperture,
in order to get a proper exposure when the solar image was
enlarged from °6 inch (its diameter at the principal focus of the
objective) to 24 inches on the ground glass. The same size of
aperture was adopted for the larger instruments during the partial
phases, the entire aperture, in all cases, of course being used
during totality.
The work of designing and constructing these lenses, and also
the different attachments to the cameras for securing exposures of
various degrees of rapidity, from a very small fraction of a second
to any desired length, was placed in the hands of Mr. Joseph
Zentmayer, whose extended scientific attainments, combined with
unrivalled skill in the construction of optical instruments, peculiarly
fitted him for such a task.
As the operation of the eye-piece, when employed to produce an
image on the screen or ground glass of a camera, is essentially
different from that which it performs in its usual office, it was
judged best by Mr. Zentmayer to make some alterations in its
form. Thus, in the first place, since in the present case the “ eye-
lens” of the eye-piece undoubtedly makes a secondary image of the
primary image formed within the eye-piece by the combined action
of the objective and the field-lens of the eye-piece, it is clearly
desirable to make this lens of a longer focus than usual, so that its
errors may be of less account. It was also essential to give the
new eye-plece a wide angle, so as to secure a sufficient field not only
for the solar disc, but also for the corona.
While therefore the ratio of focal lengths in the two lenses of
the ordinary eye-piece is usually 1:3, it was in this case as 1:2.
While the distance between the lenses is usually the sum of their
focal lengths divided by 2, it was here made equal to the sum of
the focal lengths divided by 2, plus *24 inch. This was to give
space for the introduction of the reticule of spider lines, which
would otherwise have been brought too near the field-lens, and also
=
1870. ] The Solar Eclipse of August last. a
to keep this lens beyond the conjugate focus of the eye-lens, as
otherwise particles of dust on the former would have been too
- faithfully portrayed by the latter.
The elements actually adopted were as follows :-—
Ft. In
Focal length of objective .. i a, 36
Radius of field-lens 0 1°375
eye-lens 0 0°687
Focus of field-lens Ke 0 2°6
Diameter of field-Iens (= R) 0 1°375
Focus of eye-lens . : Oris
Diameter of eye- -lens Ss R) 0 0:°687
Distance between lenses, 1° see 0° 5 Os) 22
Equivalent .. Or I" 7a
Distance of reticule from eye e-lens for 5- in. distance 0 1°62
of ground glass..
When the instruments were boxed and packed, it was found
that, with the various photographic appliances, they made no less
than five farniture-car loads of material.
In arranging the division of the party into three sections, with
the three telescopes, so that they might be distributed along the
line of totality, and thus diminish the chance of universal extinction
by local clouds, Professor Morton was chiefly guided by the desire
of securing in each section such a diversity of special ability as might
make each self-dependent and complete; also, to leave nothing
undone to secure content and harmony of feeling. He assigned to
himself the University telescope, which being of smaller size and
without clockwork movement, could not be expected to do as good
work as the others: though should they by chance be overclouded,
ats result would be invaluable.
The High School telescope, 6-inch aperture, 9 feet focal length,
was under the charge of Professor A. M. Mayer, Ph.D., and Mr.
O. H. Kendall. It was stationed at Burlington, 40° 48! Li Di;
Oh. 56m. 13s. West of Washington. By, ‘measurements of the
photographs taken by this party, Professor Mayer has shown a
change of shape in one of the larger spots during the eclipse,
amounting to a motion of 2000 miles, in its edges.
The Gettysburg telescope, 6- inch aperture, 84 feet focal length,
was in charge of Professor C. I’. Himes, Mr. a Zentmayer, and
Mr. E. Moelling. ‘This was stationed at Ottumwa, about 75 miles
nearly west of Burlington.
With the University telescopes were Mr. E. L. Wilson and
Professor Morton. ‘This section was placed at Mount Pleasant,
between the other stations.
It is almost needless to say that all officials connected with the
railways acted with the greatest liberality in transporting the appa-
ratus and observers to the selected sites.
The various parties having reached their destinations, arrange-
ments were at once made to get the instruments into position. In
32 The Solar Eclipse of August last. [Jan.,
the case of the Burlington party, all went smoothly, and the dark
weather alone prevented final adjustment until the night of the 6th,
or morning of the 7th, when this was secured by Professor Mayer,
who sat up all night for the purpose.
With the Ottumwa instrument it was, however, found that the
clockwork had become seriously deranged in carriage, so that Mr.
Zentmayer was obliged to take it entirely apart and refit it. The
final adjustment was only given to this instrument during the
morning of the 7th by Mr. Zentmayer, who had watched all night,
vainly, for a star.
The telescope at Mount Pleasant having no clockwork, and being
otherwise unfit for any fine adjustment, required no arrangement
except what could be given during the morning of the 7th.
The weather on the eventful day of the eclipse was at all sta-
tions perfect, thus rendering needless the policy of distribution, and
no less than 116 negatives were taken, including 13 during totality,
showing a large number of prominences, some massive and others
delicate as well as radiant brushes of a softer light, such as have
been before seen, but never as yet photographed. By another of
the sections of this large party, beside similar pictures to the above,
one was obtained showing the curious phenomena known as Baily’s
beads, being simply the last glimpse of the sun’s edge cut by the
peaks of lunar mountains into irregular spots. The time of expo-
sure determined by Professor Mayer for the partial-phase pictures
was the ;1,th of a second. Those taken during totality were
exposed from five to sixteen seconds.
The general character of the prominences will be seen by the
coloured illustration, which has been excellently copied from the
original photographs and micrometric measurements forwarded to
us by Professor Morton. The dotted circle inside the circumfe-
rence of the moon, shows the relative diameter and position of the
sun at the middle of the total eclipse. The accompanying woodcut
may be regarded as a key to the coloured picture, and will serve to
facilitate the following description of the phenomena :—
The line 4 B represents the direction of a parallel of declination.
cpa declination circle. FE is the moon’s path from first contact
at ¥. The prominences are here all shown at once; although, of
course, those on the sun’s eastern limb alone were seen at first, those
on the west side only at the end of the totality. Proceeding from
the north to the east, we first meet with a small prominence having
the position angle of about 56° 30’; it 1s of the shape of a rice
grain, with its base but slightly below the circumference of the
moon. In breadth it is 2°50', and im height 22”; ag 1' on the cir-
cumference of the sun equals 124 miles, and 1" of arc of the sun’s
distance on August 7th subtends 449 miles, it follows that its
actual dimensions are 21,000 miles long and 9900 miles high.
1870.] The Solar Eclipse of August last. 33
The next protuberance lies imbedded in the moon’s border, and has
in form the appearance of a short, deeply-articulated worm; its
mean position is 69° 17’; its length 46,700 miles, and its ereatest
height 9900; between that protuberance and the point oc on the
woodeut, are two flames in the midst of the glow previously de-
scribed. Midway the diffused light rises to an elevation of 60,500
miles. We now come to a curiously-formed protuberance. Some
have compared it to an ear of corn, but in the photographs it appears
like an eagle with outspread wings resting on the trunk of a tree
which leans towards the north. On one plate where the tree-stump
is cut off by the advancing moon, the resemblance to an eagle on
the wing is perfect. The form of this object indicates instability,
Fig: 1.
and impresses one with the idea that it is a great travelling whirl
of flame, the direction of whose rotation—as indicated by the posi-
tion of the wings and the projection of one on the other—is retro-
grade, or in the same direction as the motion of the hands of a
watch. Dr. Mayer, chief of the Burlington Section of the Phila-
delphia Photographic Expedition, has examined, with care, the
successive photographs of it, and he says that although at first he
thought that the last impression differed from those preceding in
that the wings had become longer and more in a line with each
other, yet on subsequent examination he could not really decide
that a perceptible motion had taken place during the time of totality.
The height of this object is 36,700 miles, and the spread of the
VOL. VII. D
34 The Solar Eclipse of August last. [Jan.,
wings 70,800 miles. The next protuberance extends to between E
and 1 on the woodcut; it is of very irregular outline, and shows
portions of its substance detached from the general mass and floating
freely above it. The most elevated and bright of these detached
flames floats at a height of at least 20,000 miles above the surface
of the sun. Beyond1a white nebulous cloud rises to the elevation
of 60,500 miles. Next follow two protuberances at x.
We now pass to the western limb of the sun, and meet with the
remarkably large and massive protuberance at @ on the woodcut.
It is shaped like a bird’s head, with the beak and under-side of the
head resting on the limb of the moon. Ona photograph taken at
Ottumwa, lowa, just before the sun came out, this protuberance had
the exact appearance of an albatross head with the beak open,
holding a rounded mass between the extremity of the jaws. ‘The
protuberance at F bears the most striking resemblance to a cater-
pillar. It extends through an angle of 11°, or 81,800 miles; its
maximum elevation, which is at the head of the caterpillar, is 23,000
miles. Out of the head issued two horns ; the one nearest the front
being the higher of the two, and terminated with a knob or ball
from which curves a broken line of light to the border of the moon.
The next prominence at has the shape of a grain of rice slightly
constricted in the middle. Between u and is another protuberance.
Professor Young, who examined these prominences during the
totality, has continued his spectroscopic notes of the prominences
since the eclipse, and on September the 13th he obtained a
view from which the accompanying woodcut is taken. He
describes it as a long, straggling range of protuberances—the sketch
giving a very fair idea of the number, form, and arrangement of
the immense cloudy mass. The points a and b were very bright.
On September 18th he noticed a remarkable phenomenon,
which, although not bearing directly on the eclipse phenomena, is
sufficiently rare to make it deserve recording in these pages.
Whilst examining the spectrum of a large group of spots near the
sun’s western limb, his attention was drawn to a peculiar knobbi-
ness of the F line (on the sun’s disc, not at the edge), represented
by the following cut a, at the point e. In a very few moments
a brilliant spot replaced the knobs; not merely interrupting and
1870.] The Solar Eclipse of August last. 35
reversing the dark line, but blazing like a star near the horizon,
only with blue instead of red light. It remained for about two
minutes, disappearing, unfortunately, whilst *
the observer was examining the sun’s image oti
upon the graduated sereen of the slit, in order ” & ¢ ¢ 1
to fix its position. It is not known, there-
fore, whether it disappeared instantaneously or
gradually. 6 gives an idea of this appearance.
On returning to the eye-piece, Professor Young
saw what is represented at ce. On the upper e
(more refrangible) edge of F there seemed to
hang a little black moat, making a barb, whose
point reached nearly to the faint iron line just
above F. As given on Angstrém’s atlas, the
wave-length of F is 486:07, while that of
the iron line referred to is 485-92 (the units being millionths of a
millimetre). This*shows an absolute change of 0:15 in the wave-
length, or a fraction of its whole amount, represented by the decimal
"00030, and would indicate an advancing velocity of about 55°5
miles per second in the mass of hydrogen whose absorption pro-
duced this barbed displacement. The barb continued visible for
about five minutes, gradually resolving itself into three small
lumps, one on the upper and two on the lower line, Fig. 1,d. In
about ten minutes more the F line resumed its usual appearance.
Whilst on the subject of the solar prominences it may not be
out of place to refer to some observations by Professor F. Zéllner,
who has succeeded in observing them without an eclipse with
great sharpness and clearness. From the nature ofthe method the
same protuberance was simultaneously observed in three different
colours corresponding to the three homogeneous lines of its spec-
trum. ‘There is, however, a material difference between the red
and blue image on the one hand, and the yellow on the other.
The latter is very intense only in close proximity to the edge of
the sun’s disc, and in this respect corresponds to the other images ;
while the more delicate details disappear at a greater distance.
This difference does not seem to be caused by the greater bright-
ness of the spectrum in that region, but appears to depend on one
of the two following hypotheses for an explanation :—either that the
rays which give rise to the yellow image emanate from a gas
having a greater specific gravity than hydrogen, and therefore
existing at a lower level, or that the greater intensities of tempera-
ture and pressure nearer the surface of the sun cause hydrogen to
emit these rays. 3
Professor Zéllner’s paper, which will appear in the next number
of the journal of the Franklin Institute (for early proofs of which
the writer has to thank Professor Morton, the editor), is ae
D
WIZ
/1\\N
36 The Solar Eclipse of August last. [ Jan.,
with beautifully coloured drawings showing the rapid changes
which sometimes occur in the forms of these prominences even in
the course of a few hours. Observing one of the most remarkable
formations, the Professor says, “I hardly believed my eyes when I
noticed in it the tongue-like motion of a flame. This motion was
slower, however, compared with the size of the flame than that of
high towering flames at great conflagrations. The time required
by such a wave in passing from the base to the apex was about
two or three seconds.”
In comparing the general impression of the protuberances with
terrestrial phenomena, the author states that the great majority
remind him of the different forms of our clouds and fog. The
cumulus type is completely developed in the cases here referred to.
Other formations remind us of masses of clouds and fogs floating
closely over lowlands and seas, whose upper parts are driven and
torn by currents of air, and which present the well-known, ever-
varying forms when viewed from the tops of high mountains.
Professor Zodllner hopes, by using larger prisms and a circular
sl't in the spectroscope, to be enabled to observe simultaneously all
the protuberances on the edge of the sun, in the different parts of
the spectrum, just as in a total solar eclipse of long duration.
Returning to the August eclipse, one of the most beautiful
observations was on the first contact by means of the spectroscope.
Professor Young has been giving much attention to this subject, and
had fitted up a very efficient instrument for the purpose. The instru-
ment consisted of a spectroscope with five prisms of 45° each, having
faces 24 by 3} inches ; the collimator and telescope had apertures of
24 inches, with a focal length of 17. These were connected with a
ecmet-seeker of 4 inches aperture and 30 inches focus, used with an
eye-piece, and giving an image of the sun 23 inches in diameter on
the slit of the spectroscope. A graduated screen at the slit determined
positions of points on the sun’s limb, and a wire micrometer measured
the positions of spectrum lines. The whole was mounted equatorially
with slow-motion screws. During the eclipse he was stationed at
Burlington, Iowa, and shortly before the first contact was due, he
found that there was a solar prominence located at the spot where
first contact must occur (see F in cut on page 33). He therefore
fixed his spectroscope with the slit radial to the solar edge at the
point, so getting a prominent spectrum whose width was determined
by the height of the prominence. Closely watching this, he pre-
sently found that it began to narrow steadily, and at the instant
that 1t became a mere line and disappeared he recorded first contact.
The moon’s approach was perceived full 30” before its actual ap-
pulse ; the observation was perfectly easy, and the time determined
is certainly to be relied on within half a second, and probably much
less. The presence of a prominence at the point of contact is not
1870. | The Solar Eclipse of August last. 37
essential to the success of the method, as there is everywhere on the
sun's limb sufficient depth of chromosphere to answer the purpose.
From the first photograph showing contact made by the Philadel-
phia party at the same place, Professor A. M. Mayer, who had
charge of that division, calculated the time of actual first contact,
and found that it came within two-tenths of a second of the record
made by Professor Young.
Professor Young proposes to apply the spectroscope in this
manner to observations both of the external and internal contacts at
the next transit of Venus.
The partial-phase pictures show the various sun-spots visible at
the time (about six in number) with admirable definition, the larger
ones being surrounded by a marked fringe of faculee. They all show
a beautiful gradation of shade from the border of the sun inwards.
This shading of the source of light is due to the absorption of the
peripheral rays which necessarily pass through a greater thickness
of the dense solar atmosphere than those which emanate from the
central portion of the disc; on a more searching examination of
the relative intensities of light of different portions of the solar
disc, there may be observed on all of these photographs, close to
the limb of the advancing or retreating moon, a bright glow like
that of early dawn, which extends from the moon to a distance of
about 15”. Unless this glow can be accounted for in node and in
measure by diffraction, it would appear as if it were due to a lunar
atmosphere, although Dr. Mayer, in suggesting this explanation,
confesses that he cannot understand how an atmosphere capable of
producing such marked effects when projected against the intensely
lighted dise of the sun, should have no appreciable refractive effect
on small stars when occulted by the moon. We should be more
inclined to account for this glow as being the effect of specular
reflexion from the surface of the moon grazed by the sun’s rays.
A party under Professor Pierce devoted themselves exclusively
to the recording of that strange phenomenon, the corona. ‘To
secure any impression from this object, which, notwithstanding its
apparent brightness, is remarkably deficient in photographic power,
it was necessary to make a very small image and to give a very
long exposure.
The telescope was therefore arranged to produce an image in
its principal focus simply, and during the totality an exposure of
forty seconds was given. By this means a picture was obtained
of which the cut on the next page is a very careful copy. From the
long exposure, the motion of the moon, and probably also of the ight
im the corona, there is little sharpness of definition, and the promi-
nences only appear as bright spots. The general shape of the
corona is, however, very well given, and the curious appearance of
curvature, in some parts, is very manifest. Professor Himes, who
38 The Solar Eclipse of August last. | Jan.,
was at Ottumwa, describes the corona as approaching much more
nearly in regularity the four-rayed form generally given, and which
eda had always seemed idealized or con-
fo ventional. The 8. W. ray was, however,
unequally subdivided with the smaller
part towards the north. The whole
seemed of a fibrous, slightly curled
or twisted character, somewhat like a
cirrus cloud, and of silvery whiteness.
The prominences, especially the large
one a little to the left of south, seemed
at the first instant of a dazzling
white, but after his attention had been
diverted for a few moments, it ap-
peared of a brilliant decided rose colour
bordering on crimson, and remained
~ of this colour to the close. To Mr.
Zentmayer, who was engaged at the camera and had used neither
telescope nor screen, it appeared white, with a slightly roseate hue.
To Mr. Moelling, under similar conditions, it appeared white
throughout. Messrs. Brown and Baker, who had a short glimpse
of it from the door of the dark room, rather incline to the opinion
that it was white. Professor Pickering, who was at Mount
Pleasant, Iowa, describes the corona as an irregular four-pointed
star with, of course, a black centre. ‘Two of the rays were nearly
vertical and two horizontal, the left-hand one pointing somewhat
downward, while between it and the iower ray was a fifth smaller
point. The colour was pure white, very different from the full
moon, but resembling a cumulus cloud. Its texture resembled
the ragged edge of a thundercloud, or the crest of a wave torn
by the wind. The striz were not radial but spiral, as if the sun
had been turned in such a way that the upper edge moved towards
the east.
During the totality Professor Young gave special attention to
observation of the corona with the spectroscope. He found that,
in place of a subdued solar spectrum, which would have been anti-
cipated from the reports of former observations, it yielded a spec-
trum of bright lines. These are represented in the coloured illus-
tration, and below the spectrum of the corona is given a copy of
the spectrum of an aurora borealis as observed by Professor Win-
lock on the evening of April 15th. From the close accordance
between the coronal lines and three of the auroral lines, Professor
Young considers it almost certain that the corona is simply ar
electric discharge, no doubt varying with great rapidity, as we see
in the case of the aurora; in fact, that the solar corona is a perma-
nent aurora. It is, however, right to state that in an article by
1870. ] The Solar Eclipse of August last. 39
Mr. J. N. Lockyer in ‘ Nature,’ for November 4th, he throws some
doubt on this conclusion, and hesitates tofregard the question as
settled, were the new hypothesis less startling than it is.
The most complete series of spectroscopic observations were
those taken of the prominences. During totality nine bright lines
were observed by Professor Young in the spectrum of one of the
protuberances, wz. c dazzling in brilliancy; 1017°5 (near p, the
numbers refer to Kirchhoff’s scale) very bright, but not equal to c;
1250 + 20, very faint, position only estimated; 1350 + 20, like
preceding ; 1474 (a little below E), conspicuous, but not more than
half as bright as 1017°5; F next to cin brightness; 2602 + 2, a
little famter than 1474, position determined by micrometrical refer-
ence to the next; 2796, a little below a; the well-known H y line
in brightness between 1017°5 and 1474; and finally h, or H6é,
somewhat brighter than 1474. 6 it is supposed was not seen; on
account of a mistake in carrying that portion of the spectrum
through the field, there was no prominence on the slit. The lines
marked # in the coloured illustration are hydrogen lines.
The opportunity which was afforded by the total obscuration
of the sun’s light was taken advantage of to search for planetary
bodies between Mercury and the sun, but without success, although
Mercury, Venus, Mars, Saturn, Regulus, and Arcturus were plainly
visible. The horizon all around was lighted up by a sort of dim
twilight for four or five degrees in breadth, and above this rim of
light hung a leaden canopy, increasing in depth towards the zenith.
At the Ottumwa station a curious appearance was noticed by
Mr. Zentmayer. During the time that the pictures of the partial
phase were being taken at long intervals, the ground-glass plate
was put in the camera to note any irregularities in the clock move-
ment, should they occur. About twenty-five minutes before the
totality, Mr. Zentmayer observed some bright objects on the ground-
glass, crossing from one cusp to the other of the solar crescent.
Each object occupied about two seconds in passing, and they all
moved in right lines, nearly parallel, and in the same direction.
These points were well defined, and conveyed to the mind of Mr.
Zentmayer, who is accustomed to the use of the camera for photo-
graphic purposes, the strong impression of being images of objects,
and not points of light merely. It is, moreover, certain that the
objects, whatever they might be, must (in order to have produced
such sharply-defined images on the ground-glass) have been several
miles distant from the telescope, as even a point of light at a less
see would have produced an enlarged image, with a hazy
order.
The most complete account of the photographic operations is
recorded in the report to Professor Morton by Dr. Mayer, who was
the chief of the Burlington party. They arrived at their destination
40 The Solar Eclipse of August last. [Jan.,
on August 4th, and up to the morning of the 7th they were occupied
in putting together the base and frame of the telescope, mounting the
bed-plate, the polar and declination axis and circles, the cradle
holding the telescope, fitting-in the tube and optical part, adjusting
the verniers and bringing the instrument into altitude and azimuth
adjustment. The whole of Friday, August 6th, there was a driving
rain, an east wind, and a dull murky atmosphere, foreboding the
worst results on the morrow—after haying spent previous weeks in
preparation, and having travelled over a thousand miles, in the hope
of carrying back with them permanent photographic records of the
long-thought-of eclipse.
As they retired to rest there appeared signs of the clouds
breaking. They had barely fallen asleep when the clerk, according
to previous arrangement, woke them with the agreeable news that
there were plenty of stars. ‘They were soon dressed, and were
charmed by the sight of a cloudless sky ; and Professor Coffin, Drs.
Gould and Mayer were up all night putting their own special
instruments in adjustment. When all was finished, the sun was
rising, and the air as pure and serene as one could wish. On
Saturday morning the chronograph was mounted, and electric
wires were led to the camera, to Professor Young’s spectroscope,
and to the station of Dr. Gould outside the building. The two
threads of the reticule of the camera were placed one parallel and
the other at right angles to the celestial equator, and experiments
were now begun by Mr. Willard to ascertain the chemical focus.
This was obtained after the tube had been following the sun for an
hour or more, and after the focus was fixed the clockwork was kept
going, so that no change in focus should supervene from a change
in temperature in the lenses and tube. The clockwork adjustment
had been regulated with such accuracy that it drove the telescope so
that a star would remain closely bisected for twenty minutes. By
3 p.m. all was in readiness, and each one at his allotted post of duty,
ready for work.
The image of the sun was 2°04 inches in diameter, and was
taken on a 44 x 54 inch plate. Mr. Zentmayer had so constructed
the camera eye-piece, that the image of a reticule of two spider-
threads at right angles to each other was formed on the plate with
the image of the sun, and these threads were so mounted that they
could be adjusted respectively parallel and at right angles to the
celestial equator, and thus fix on the photographs the positions of
the sun and moon, and give the position angles of points on the
surface and periphery of the sun.
The tube carrying the camera lenses screwed into a plate in
which, immediately in front of the anterior lens, was a guide, in
which a thin plate having a horizontal slot of ‘0224 inch in width
was caused to descend by the action of a spring. This was used
1870. | The Solar Eclipse of August last. 41
for the partial phases. During totality the full aperture of the
object-glass was employed, and a slide plate was used, having a
circular opening which allowed the full beam to pass. This plate
had two falls instead of one. On setting the plate free by the top
trigger it fell, and the collodion plate was exposed to the entire
beam ; after the desired exposure a lower trigger was relieved, and
the plate made a second fall, and the lens being covered by the top
of the plate, the exposure ceased. ‘These triggers were connected
with a Morse register having a paper fillet running through it; at
every second the clock for an instant opened the electric circuit,
and there was a very short break made in the line marked by the
pen on the fillet; thus the seconds of t¢me were stepped off in space
on the paper ribbon. The triggers were so connected with this
chronograph that an additional break was made during the time
the photographic plate was being exposed. By measuring this
break on the paper ribbon and comparing its length with the
length of the second in which it occurs, the exact fraction of the
second during which the plate was exposed will be given.
Dr. Mayer arranged for his own duty to keep the telescope
in adjustment, and to manipulate the apparatus of exposure and
chronographic registration, while Mr. Willard placed the plate in
the camera and gave the several times of exposure he desired during
totality. Mr. Phillips coated the plates and handed them to Mr.
Montford, who carried them to Mr. Willard, and thence, after
exposure, to Mr. Mahoney, who developed them, assisted by Mr.
Leisenring.
The wall of the dark room adjoining where the telescope stood
was fitted with two dark valves, or dumb waiters, by which the
plate-holders could be passed in and out without the admission of
light or the necessity of any of the operators moving from their
places. Seven negative baths were used, standing in a trough of
water to keep them cool, four plate-holders, and a large wooden
trough with grooved sides, similar to a negative-rack; this was
filled with a weak solution of hyposulphite of soda. In the dark
room the first operator’s duty was to coat plates and- put them into
the baths ; the second took them out, put them into the plate-holders,
and passed them out of the room by means of one of the dumb
waiters. After exposure, the holders were returned to the dark
room by the second dumb waiter, when the third operator took the
plate from the holder, developed, washed, and then dropped it into
one of the grooves in the large fixing trough. There the plates
remained slowly fixing till after the eclipse was over, when they
were taken out in the same order in which they were put in,
washed, and numbered with a diamond.
At the telescope Mr. Rock was detailed to attend to the very
important duty of calling out the seconds of the chronograph-fillet ;
42 The Solar Eclipse of August last. [Jan.,
Mr. Kendall called out the minutes at each 60-seconds call of Mr.
Rock, and wrote it on the fillet. He also had charge of the chrono-
graph, and started it when Dr. Mayer called “clock,” while, at the
same signal, Mr. Rock began the registration of seconds.
Dr. Mayer had laid out the following programme of work :—First
to take in rapid succession, beginning 10 seconds before the computed
time of first contact, a series of five photographs. Secondly, one just
before second contact, one just after second contact, as many as pos-.
sible during totality, one just before the end of totality, and another
just after the sun reappeared. Thirdly, to take again a series in
rapid succession about the end of the eclipse. Fourthly, during
partial phase, to take a picture every four or five minutes.
When the chronometer marked 12 h. 48 m., Mr. Rock began to
count and register the times on the fillet. Every one was at his
post, the lanterns lighted, and nothing could be heard but the count
and tap of the chronograph. At 12h. 49m. 45s, the first photograph
was taken, and following at intervals of from 10 to 12 seconds five
perfect pictures were secured. The contact is first visible on the
third. Photographs were now leisurely taken at intervals of about
four minutes, until twelve plates in all were taken.
About five minutes before totality, Mr. Willard removed the
diaphragm of two inches aperture, which was used during partial
phase, and exposed the full aperture of the object-glass, whilst Dr.
Mayer changed the slide with -0224-inch slot for the one which
admitted the whole beam at once on the plate in the camera.
The order was given to prepare the plates. ‘The first plate was
taken at 13 h. 51m. 39°15 s., or 7 seconds before the time of second
contact as observed by Professor Coffin. ‘The slide was soon reset
for another exposure, and as Mr. Willard desired the first plate of
totality to be exposed five seconds, Dr. Mayer kept on counting
zero, zero, zero, with the taps of the chronograph, until striking the
upper trigger at zero, he counted one, two, three, four, five, when
the lower trigger was struck and the plate removed.
Counting the first plate, taken seven seconds before second con-
tact, six photographs were taken in 2m. 3s. After the sixth was
removed there still remained 50 s. of total phase. There was a delay
in the plate. The observer grew impatient; he called plate! plate!!
but, alas, it was found impossible to manipulate more than six
plates in two minutes and three seconds. The store had been used
up too rapidly, and so they did not succeed in getting an impression
just before the sun came forth. The next plate was taken 29-2
seconds after third contact, and is a valuable photograph of a thin
crescent, with the cusps sharply cut.
Dr. Mayer describes the appearances during totality i in the fol-
lowing words :—“ About 15 minutes before totality it became so
cool that I was obliged to put on my coat. A minute or two before
— 7!
1870.| Instruction in Science for Women. 43
totality, the sky grew ashen, or rather leaden in hue, and as, with
face turned towards the sun, I kept the count from the chronometer
for the first exposure, Venus and Mercury came out shining beau-
tifully on a ground of bluish grey. I thought I saw a flashing,
twirling motion in the corona, or in the last rays of the sun; but of
this I will not be positive, for my attention was not, at the time,
specially directed to minute observation. Moths and insects in
profusion passed between me and the sun, while a flock of birds
with troubled irregular flight seemed seeking cover from the un-
natural gloom which surrounded them.
waste ; but since the transport of this waste liquid is too costly (it
may be very usefully applied where it can be had with ease), the
author describes a method of making hypophosphoric acid by the
slow combustion of phosphorus. According to his experiments, 2
grammes of this acid dissolved in 10 or 12 litres of water, is a strong
poison for all kinds of insects, and not only does not hurt plants,
but actually does good by increasing the soluble phosphates in the
soil.
The solution of oxide of copper in ammonia acts as an energetic
solvent upon cellulose ; this property is made use of by A. Jouglet to
waterproof paper in the following manner :—A tank is made to con-
tain the solution just alluded to, and the paper is rapidly passed just
over and in contact with the surface of the liquid, by means of pro-
perly-placed rollers moving with speed. The paper, on leaving, is
pressed between two cylinders, and next dried by means of so-called
drying cylinders, similar to those in use in paper-mills. The short
contact of the felty paper-tissue with the liquid gives rise to just
sufficient solution of cellulose to form an impermeable varnish.
A process for the preservation of butchers’ meat, invented by
M. Georges, is now in use on the large scale at Monte Video. The
meat, in pieces weighing from 2 to 50 kilos., is placed in a mixture
of water, hydrochloric acid, glycerine, and bisulphite of soda. After
haying been steeped for some time, the pieces are taken out and
dusted over with finely-powdered dry bisulphite of soda, and then
packed in air-tight boxes, filled as full as possible. In this state
the meat keeps fresh any length of time, and becomes perfectly fit
for use—equal to fresh butchers’ meat—by steeping for a short
time in water to which vinegar has been added, and afterwards ex-
posure to air; the price of the preserved meat, of which it would be
easy to supply to London and to Paris daily over 10 tons, is from
50 to 60 centimes per kilo. :
Hydrate of chloral, the new anesthetic and sedative, is daily
increasing in importance, and many processes have been given for
VoL. VII. T
262 Chronicles of Science. [ April,
its preparation: the best is probably that of MM. Miller and
Paul. Their process consists in passing a current of dry and pure
chlorine gas into pure and absolute alcohol, until the contents of the
flask are, after about seventy hours, converted into a white and
crystalline mass; when this operation is properly conducted, a large
quantity of hydrate of chloral is obtained. Hydrate of chloral is
readily sublimed, and may be thus obtained as a dry, snow-white,
neutral crystalline powder. It does not exhibit any smell at the
ordinary temperature of the air; it volatilizes slowly, without
absorbing much moisture, unless it be placed in a very damp place ;
it fuses at 56°, boils at 145°, is completely soluble in a small quan-
tity of water, and also soluble in alcohol, ether, chloroform, sulphide
of carbon, benzol, and fatty substances. Its aqueous solution ought
to be neutral to test-paper, and should not become turbid by a solution
of nitrate of silver.
It is now proposed to make the reflecting surfaces of looking-
glasses of platinum instead of tin amalgam or silver. M. Jouglet
prepares the platinizing compound in the following manner :— Very
thin platinum foil is dissolved in aqua regia, the solution carefully
evaporated to dryness,the solid chloride next placed on a triturating
marble, and gradually mixed with essential oil of lavender. When
incorporated with the chloride, the mixture is placed in a porce-
lain capsule, and left standing for several days; the fluid is decanted
from any sediment, and filtered. As flux for 100 grains of platinum
the following ingredients are used:—25 grains of litharge and
25 grains of borate of lead, mixed and triturated together with
about 10 grains of essence of lavender; this is next mixed with the
platinizing fiuid. After a layer of platinum has been formed upon
the glass, it is fixed by burning it in by placing the glass in pecu-
harly-constructed mufiles.
From a series of observations made at Monaco, on the shores of
the Mediterranean, Dr. Gillebert d’Hercourt concludes that there is
always on the sea-shore an atmosphere impregnated with saline
particles ; this layer of air has, at the above-named place, some 500
metres horizontal and 60 metres vertical extent. This impregna-
tion of salt is due to what the author terms “ pulverization” of the
sea-water by the breaking up of the surf, and is not directly in-
fluenced either by barometric pressure, hygrometric state of the
atmosphere, or temperature. This hydro-mineral dust, as it is
called by the author, is, unless there happen to exist near the coast
physical obstacles in the shape of high mountains, carried far away
inland, and is not to be confounded with what is of more coarse
nature, and termed “spray,” which is only quite local and produced
when a gale of wind blows. The author states that, even on calm
days in winter, the atmosphere near Monaco is up to a height of 70
1870. | Chenustry. 263
metres, and some few miles inland, impregnated with this hydro-
mineral dust.
As a proof of the greatly-improved mode of manufacture of
sulphide of carbon and its very extensive use, M. Contet states that
in 1840 the kilo. of rectified sulphide of carbon cost 50 franes (2/.).
In 1848 M. Deiss manufactured it, and sold it at 8 francs per kilo. ;
and now it may be had wholesale at 50 centimes the same quantity.
As regards the purification, M. Sidot first re-distils the raw product,
then shakes the distillate up with mercury until the latter becomes
black, and this operation is so long repeated as the metal is affected _
by the fluid, or rather by any sulphur dissolved in it. Sulphide
of carbon thus purified is freed from the foetid odour it generally
has, and exhibits a smell of ether. M. Cloeg renders commercial
sulphide of carbon inodorous by leaving it for twenty-four hours in
contact with half per cent. of its weight of finely-powdered corro-
sive sublimate, care being taken to shake or stir up this mixture.
The mercurial compound combines with the substances which are
the cause of the foetid odour of this substance, and an insoluble
compound is deposited. The liquid is carefully decanted, and after
a little pure inodorous fat has been added, the sulphide is re-distilled
by the heat of a water-bath. The sulphide thus obtained exhibits
an ethereal odour, and is eminently suitable for the extraction of
oils, fats, &c., from various substances, since on evaporation of the
purified sulphide these matters are obtained in as fresh and pure a
state as if the oils had been obtained by pressure.
M. Coupier has succeeded in obtaining fuchsine without the use
of arsenic by the action of hydrochloric acid and iron, in small
quantities, upon pure aniline and nitro-toluol, taking care to apply
a suitable temperature. Commercial aniline and commercial nitro-
benzol also yield the same result; and M. Schtitzenberger states
that having been requested to test the results of this reaction, he
has found that the aniline red obtained is identical with that ordi-
narily made, and declared it to be a salt of rosaniline. The yield
is very fair, and somewhat larger than when arsenic is used.
A lengthy memoir on various processes for preserving timber
has been published by Dr. Ott. From it we learn that the opinion
that carbolic acid and substances containing it are effectual in pre-
serving timber is erroneous. The real preservative action of the
tar-oils is due, according to this author, to a greenish fluorescent
oil that comes over at the last stage of the distillation. Direct trials
with pyren and paranaphthaline do not yield successful results. The
question whether tar (coal-tar) contains a sufficient quantity of
the fluorescent greenish oil just alluded to, to justify the use of coal-
tar for preservative purposes, is answered in the negative. The
decay of timber, or peculiar transformation which makes it unfit for
© 2
264 Chronicles of Science. [ April,
practical purposes, seems to be, in most instances, produced by the
attack of fungi and lichens. The mouldering of wood is distinct
from decay, it being merely a chemical process caused by the action
of water with small access of air. None of the processes invented
to preserve timber by chemicals are perfect. The most simple and
practical method is the old, but, unfortunately, far too slow plan of
properly subjecting timber to the action of air and water, as prac-
tised in ship-building yards. A propos of the method of preserving
wood by impregnation with sulphate of copper, it may be interest-
ing to know that by an order recently issued by M. le Maire de
Douai, the bakers of that town have been prohibited from using
the wood of old railway sleepers as fuel for their ovens, since many
of these sleepers have been impregnated with sulphate of copper,
and there is danger that sonie compound of copper might poison
the bread.
Professor Morton has described the works at New York where
oxygen gas 1s manufactured on the large scale. The works consist
of retort-houses, engine-rooms, store-house, pumps for compressing
gas in cylinders, and a gas-holder of 26,000 cubic feet capacity.
The process is carried on as follows :— About 700 lbs. of manganate
of soda are placed in the retort, and heated to the requisite degree ;
superheated steam from a boiler is then admitted for about ten
minutes. Two equivalents of the manganate of soda and two of water
react upon each other, the water combines with the soda of the
manganate to forma hydrate of soda, the manganic acid is converted
into sesquioxide of manganese, containing only half the proportion of
oxygen, and the other half of the oxygen passes off in the free state.
At the conclusion of this part of the process the steam is shut off,
and the superheated air is admitted for about fifteen minutes, where-
upon the sesquioxide combines with more oxygen from the air, and
is re-conyerted into manganic acid, which again combines with soda.
The retorts in each furnace are charged with 700 Ibs. of permanga-
nate of soda, and by the consumption of 2 chaldrons of coke, and
with the labour of three men, 25,000 cubic feet of oxygen are made
per day. Itis now sold at 23d. per cubic foot, compressed in reser-
voirs up to a pressure of 250 Ibs. to the square inch. The gas is
of excellent quality, and very pure.
1870. | Engineering—Civil and Mechanical. 265
6. ENGINEERING—CIVIL AND MECHANICAL.
Light Railways.—The great question of the day amongst engi-
neers, at the present time, is the construction of light, or narrow-
gauge railways. The enormous expense which has attended the
laying-down of existing lmes upon what is styled the “standard”
gauge, and their comparative unremunerativeness, have naturally
led to the consideration of how the existing want of increased
facilities of communication can best be supplied so as to recommend
new projects for railway extension to the confidence of capitalists
and the public generally. The subject has also obtained increased
prominence in consequence of the arrival of a Russian Commission
to investigate the means of communication in this country, and who,
together with many other foreigners of distinction, and leading
English engineers and others, paid a visit last February to the little
Festiniog Railway in North Wales. As this line has the narrowest
gauge of any existing railway worked by locomotive power, some
description of it here may not be inappropriate.
Festiniog Railway.—This line, which is 134 miles in length,
extends from Portmadoc to the slate quarries in the neighbourhood
of Festiniog. It is slightly under 2 feet in width of gauge, and
was originally constructed for horse traction, by which power it
was worked until 1863, when the increased traffic necessitated the
employment of steam power for that purpose. ‘The line was
strengthened and improved, diminutive locomotives were con-
structed expressly for it, and since 1865 passenger carriages have
been attached to each train. ‘The difference in level between the
two termini is 700 feet, and the average gradient is 1 in 92. The
steepest gradient on the portion now used for passengers is 1 in 79 ° 82,
and the steepest on which locomotive engines are employed, 1 in 60.
Some of the curves are exceedingly sharp, having radii varying from
2 chains to 4 chains. As the line is a continuous incline from
Portmadoce to Festiniog, the locomotive is employed only to draw
the trams in one direction; it then returns by itself, and the
loaded trains run by gravitation down to Portmadoc—their speed
being regulated by breaks. The original capital of the company
was 36,0007. Since that outlay was incurred the line has been
almost reconstructed ; workshops have been erected and rolling
stock manufactured out of revenue, bringing up the total cost of
the line to about 86,0007. The net profits have amounted to
upwards of 30 per cent. on the original capital, and they exceed
123 per cent. on the total outlay of the undertaking.
New Tunnel under the Thames.—The past quarter has wit-
nessed the completion of a tunnel under the river Thames between
Tower Hill and Vine Street, Tooley Street. The noticeable feature
266 Chronicles of Science. [ April,
of this work is the extreme rapidity, and comparatively trifling cost
at which it has been constructed, the time occupied being only one
year, and the total expense less than 20,000/., whereas the old
Thames Tunnel occupied eighteen years in construction, and cost
over half-a-million sterling. This new tunnel consists of a circular
driftway, 7 feet 3 inches in diameter, having an inclination from either
side towards the centre of the river of 1 in 30. It is approached on
each bank by a perpendicular shaft, that on the Middlesex side
being 56 feet deep, and that on the Surrey side 52 feet. The hit
at either end consists of an iron chamber, to the roof of which a
chain is attached, which passes over a pulley at the head of the
shaft, and at the other end is fixed to a balance weight, capable of
adjustment according to the number of passengers in the lift. The
bottom of each shaft communicates with a waiting-room, having
seats along the sides. Along the tunnel is laid a railway of 2 feet
6 inches gauge, on which a small omnibus runs, capable of accom-
modating fourteen passengers at one time. Under the level of the
tunnel at the bottom of each shaft there is an engine-room contain-
ing a 4-horse power engine for raising and lowering the lifts, and
that on the Surrey side is also employed for hauling the omnibus,
which is driven by means of an endless steel cord passing round a
vertical pulley-wheel at the Surrey end of the tunnel, and a horizon-
tal pulley-wheel placed between the rails at the Middlesex end.
PROCEEDINGS OF SOCIETIES.
Institution of Civil Engineers—The session of 1870 was in-
augurated on the 11th January by an address from the newly-
elected President, Mr. Charles Blacker Vignoles, F.R.S. It would
be impossible briefly to summarize Mr. Vignoles’ speech, which for
interest and importance has never been surpassed, and rarely
equalled. In reading over this important paper, it appears that no
branch of the profession has escaped notice from the time when “in
the earlier stages of the human race their first want must have been,
as it is now, a supply of water for men and beasts of tribes, whether
nomadic or stationary, when no longer within reach of the natu-
ral streams or springs; and assuredly,” said Mr. Vignoles, “the
individual who first dug a well in the desert, and raised water to
the surface, by the simple contrivance of pole and bucket, was the
first mechanic—the first pre-historic engineer, whose rude invention
has nevertheless been followed in all subsequent ages,” down to the
completion of the Suez Canal, “by cutting across the sandy ligament
which has hitherto united Asia and Africa, by which a water com-
munication has been opened, which will never again be closed so
long as mercantile prosperity lasts or civilization exists.”
1870. | Engineering—Civil and Mechanical. 267
“On the Statistics of Railway Expenditure and Income, and
their Bearing on Future Railway Policy and Management.” A
paper on this subject was read before the Institution on 1st Fe-
bruary last, by Mr. John Thornhill Harrison. After referring to
the income from passengers and goods on the principal lines in the
kingdom, the question of the further extension of railways was con-
sidered, and it was urged that many lines might be constructed at
a cost of from 30002. to 50002. per mile, provided the landowners
would sell their land for the purpose at the ordinary market value ;
that the Board of Trade would allow level crossings, and that gra-
dients as steep as 1 in 20 or 1 in 80 were adopted. The subject of
expenditure for working the line was next dwelt upon in some
detail, and the percentage of net revenue on the total capital
expended. ‘Two large funds for investment of capital were also
considered : the National Debt, which amounted to 750 millions
sterling, and gave a return of 264 millions per annum, or 34 per
cent., which was a burden on the industry and capital of the country ;
and the capital expended on railways, which amounted to 500 mil-
lions sterling, giving a return of 20 millions, or 4 per cent. per
annum ; whilst a sum nearly equal to the interest on the National
Debt was annually expended in labour and materials.
Society of Engineers—On 7th February Mr. William Adams,
the newly-elected President, inaugurated the session of 1870-71 by
an address. After reviewing the progress of the Society, and advert-
ing to the several papers read during the preceding session, he pro-
ceeded to make some remarks upon locomotive engineering and the
rolling stock of railways, detailing the several improvements that
have of late years been introduced, and especially with reference to
the application of break-power for bringing trains to a standstill,
the two most important improvements for that purpose being the
steam-break of M. Le Chatelier, and the friction-wheel break of Mr.
John Clark.
South Wales Institute of Engimeers.—An important paper has
recently been read by Mr. Brogden, before the South Wales In-
stitute of Engineers, “On the Comparative Merits of Large and
Small Trams or Wagons for Colliery use.” In the course of the
discussion that followed it transpired that at a colliery in the Aber-
dare Valley there had been effected by the introduction of small
trams a saving of ls, 3d. per ton. In getting out 150 tons a day
with a large tram fourteen horses were employed at a cost of
41. 12s. 8d., whilst with small trams the same amount of work was
done for 1/. 11s. 8d., showing a saving of nearly 6d. a ton on that
item alone; besides which there was a difference in the price of
driving headways, in the cost of rails, sleepers, &c. By the use of
small trams there was also a considerable saving in the men called
“dusters,” and by reducing the headway a saving in “ gobbers.”
268 Chronicles of Science. [ April,
Men, it was also said, could earn more by the use of the small
tram, which is therefore advantageous to them as well as to the
masters.
Civil and Mechanical Engineers’ Society—On 8th December
last Mr. R. M. Bancroft read a paper before this Society “On the
Renewal of King’s Cross Station Roof.” When this station was
opened in 1852 its roof created some little sensation, as it was the
largest span-roof of the laminated type constructed in this country.
After a period of eighteen years’ existence it was found that the
timber which formed the ribs was in a state of rapid decay, and it be-
came necessary to replace them with something more durable. The
wrought-iron main ribs were formed and accurately curved so as to
fit in exactly between the old cast-iron shoes built in the walls on
each side, the cast-iron spandril fillings of the old roof bemg cut
shorter to suit the new wrought-iron ribs. The scaffold for the
construction of the roof was designed so as not to interfere with the
traffic constantly passing beneath it, and the large wrought-iron
plate-girders forming it were constructed of such section that they
might hereafter be used in bridges down the line.
Institution of Engineers in Seotland._—Professor W. J. Mac-
quorn Rankine read a very interesting paper before this Society,
upon bemg called upon to fill the presidential chair until the next
election. This paper partook of the nature of a presidential address,
and consisted of a review of the present state of engimeering progress
in its various and numerous branches; but it is on the subject of
“ Engineering Education” that Professor Rankine’s paper dwelt
with most force. In alluding to common errors under existing
systems of education, the Professor stated: “One is led to expect
results from the scientific branch of education which it is not really
capable of accomplishing. The purely practical parts of engmeering,
such as the use of tools and the superintendence of works, cannot
be soundly and thoroughly learned except through experience in
real business; and it is a mistake to endeavour to teach them
during a university course. The true laboratory for students of
engineering science is to be found in the workshops of such cities
as Glasgow, and amongst the earthwork, masonry, carpentry, and
ironwork of engineering structures in progress.”
Institution of Mechanical Engineers.—At the anniversary meet-
ing of this Institution on the 27th January last, a paper “On Le
Chatelier’s Plan of using Counter-pressure Steam as a Brake im
Locomotive Engines,” by Mr. C. W. Siemens, came under discus-
sion ; and a paper was read by Mr. C. Cochrane, of Dudley, “On
the further Economy of Fuel in Blast Furnaces, derivable from
the High Temperature of Blast obtained with Cowper’s Improved
Regenerative Stoves at Ormesby, and from increased Capacity of
Furnace, &c.” M. Le Chatelier’s plan for counter-pressure working
1 ee eee ———————e a _— e
1870.| Geology and Paleontology. 269
consists in introducing a small jet of hot water from the boiler into
the base of the blast-pipe or the exhaust part of the cylinder:
this jet being discharged at boiler pressure into the atmospheric
pressure of the exhaust passages, the greater portion of the water
instantly flashes into steam at atmospheric pressure, and instead
of the heated gases from the smoke-box, a moist vapour or fog is
now drawn into the cylinder behind the piston, upon the engine
being reversed.
LITERATURE.
“Our Iron-clad Ships; their Qualities, Performances, and Cost ;
with Chapters on Turret Ships, Iron-clad Rams, &.” By EH. J.
Reed, C.B., Chief Constructor of the Navy, &c.* Space will not
admit of such a review here as this work deserves. ‘The fact of
its coming from the pen of one so experienced in the subject will
at once commend it as an authority upon the matter of which ib
treats. Its title will convey a fair idea of the contents of the 320
pages of which this book consists; and we can only here state that
whilst this treatise on Iron-clad Ships evinces a masterly know-
ledge of the subject on the part of its author, the style in which
it is written is perfect, approaching at times to eloquence.
7. GEOLOGY AND PALAONTOLOGY.
(Including the Proceedings of the Geological Society and Notices
of recent Geological Works.)
Monographs of the Palzontographical Society, Vol. XXIII—The
success attending combined efforts was never more happily illus-
trated than in the case of the Palzeontographical Society, which was
formed twenty-three years ago for the purpose of describing and
figuring British Fossils. It has published the works of twenty-six
palzontologists, embracing in their monographs every division of
the animal kingdom found fossil in this country. Nor ig it merely
the letter-press descriptions of fossils which it effects (though these
now amount to 6405 pages 4to), but it is the superior means of
illustration it furnishes which gives such value to the volumes of
this Society. The plates now number 1006, and contain 18,991
figures. ‘The volume before us contains 43 plates, some of which
are double size. These plates, with descriptive text, are distributed
to subscribers for 1/. 1s. per annum.
The volumes of the Paleeontographical always contain a diverse
series of monographs; thus we have in this year’s-issue,— Fossil
* John Murray. London: 1869.
270 Chronicles of Science. 7 — [April,
Corals, Cretaceous Echinoderms, Oxford Clay Belemnites, Old Red
Sandstone Fishes, Lias Pterodactyles, and Crag Cetacea. Such a
“bill of fare” was never before presented at so modest a price.
Dr. Duncan’s part contains six species of Corals from the
Greensand of Haldon, thirteen species from the Gault, and six
from the Lower Greensand. ‘To this part is appended a complete
list of British Cretaceous Corals, fifty-eight in all.
Dr. Duncan remarks, “The Coral-fauna of the British area was
by no means well-developed or rich in genera during the long period
in which the Cretaceous sediments were being deposited. The
Coral tracts of the early part of the period were on the areas now
occupied by the Alpme Neocomian strata, and those of the middle
portion of the period were where the Lower Chalk is developed at
Gosau, Uchaux, and Martigues.”
“There are no traces of any Coral-reefs or atolls in the British
Cretaceous area, and its corals were of a kind whose representatives
for the most part live at a depth of from 5 to 600 fathoms.”*
In Professor Phillips’s monograph on the Oxford Clay Belem-
nites, the author notices a singular hiatus between the Inferior
~Oolite and the Oxfordian stage. It must, however, be borne in
mind that pelagic and freely-wandering animals (such as the
Belemnitide must have been, judging from their modern repre-
sentatives, the Squids, Calamaries, and Cuttle-fishes) form a less
sure basis for generalization than do the Brachiopoda and other
sedentary forms of Mollusca and the Corals.
Free swimming Cephalopoda might forsake a large area for
ages, if conditions were unfavourable, returning again at a later
epoch, and again becoming plentiful as fossil remains in the mud
of the period.
It 1s interesting to observe that Professor Phillips, who is per-
haps the most careful observer living, and the last man to be
carried away by an idea, has adopted the doctrine of descent with
modifications, as may be gathered from the following extract; 7}
speaking of Belemmnites explanatus, sp. nov., from the Kimmeridge
Clay, Professor Phillips observes, “On many accounts this form
of Belemnite is of interest in the study of the series to which
it belongs. On the one hand its resemblance to the older type
of B. abbreviatus (excentricus) of the Oxford Clay and Oolite,
and on the other to that of Speeton, in Yorkshire (L. lateralis), is
such as to offer a most instructive example for study, in relation to
the derivation of successive specific forms by hereditary transmis-
sion with modification.”
Some interesting modern types of Loricarian fishes illustrate
Mr. Ray Lankester’s monograph on the Cephalaspide of the Old
Red Sandstone.
+ eG, ft P. 128.
1870. | Geology and Palxontology. 271
These curious buckler-headed fishes are certainly among the
most interesting as they are undoubtedly the very earliest forms of
the vertebrate type with which we are acquainted.
One head-shield figured measures more than 6 inches across
and above 7 inches in length. | |
Mr. Fielding has most successfully rendered the fine and deli-
cate striae on the plates of Péeraspis in plates vi. and vu. The
histology of these fish-plates is carefully worked out and most beau-
tifully illustrated by Tuffen West.
Professor Owen’s monograph on the Lias Pterosawria deserves
more than a passing notice.
For the first time we see before us an entire British Pterodac-
tyle in his Dimorphodon macronyx, not restored at random, but
carefully put together bone by bone from the three specimens in
the British Museum. Démorphodon, as we thus know it, has a
long and slender tail firmly set and imbedded in ossified tendons,
rendering it apparently an inflexible rudder; the hind limbs are
well developed, as also are the claws and the wing-fingers. The
head is very large, with beautiful contrivances for lightening it by
means of large vacuities; the jaws are armed with larger laniary
teeth, and rows of more regular minute and pointed teeth. There
is no evidence that this species had a beak or horny termination to
its jaws as Von Meyer believes to have been the case in Rham-
phorhynchus from the Solenkofen beds.
Upon the affinities of the Pterosawria Professor Owen is at issue
with Professor Huxley, the former arguing against their Ornithic
and in favour of their Reptilian affinities, the latter placing them
in the same group with the Dinosauria, the Crocodilia, and the
Anomodontia (called by Professor Huxley the Ornithoscelida),
the most bird-like of the Reptilia.
Professor Owen argues that the possession of feathers and warm
blood are essentially bird-like attributes, whilst the absence of
feathers in the Pterosawria proves them to have been cold-blooded
reptiles. The Cockchafer 1s cited by Professor Owen to prove
that powerful flight may co-exist with cold blood; but if we could
compare the bulk of the insect with that of the Pterodactyle, there
seems little doubt that the temperature would algo increase with
the size of the animal, and in proportion to the increased muscular
work required to be accomplished. :
We deprecate the tone adopted by the author in his critical
review of Professor Huxley’s observations,* and earnestly hope it
may not be found in any future monographs.
The concluding Monograph, also by Professor Owen, treats of
the Cetacean remains, occurring in the Red Crag, belonging to the
genus Ziphius of Cuvier. These curious rostra are found in tole-
* BOTA.
272 Chronicles of Science. [ April,
rable abundance in the Coprolite-workings in the Red Crag of Suffolk,
and are usually much water-worn and eroded, as if the bed in which
they were originally deposited had undergone subsequent denuda-
tion on some later Tertiary sea-beach. ‘They often appear to have
been bored into by Pholades.
Twenty-three articles appear in the last three numbers of the
‘Geological Magazine.’ Of these the most important are: “On the
Sequence of the Glacial Beds,” by Searles V. Wood, jun.; “On
Lithodomous Perforations,” by J. Rofe, F.G.S.; “The Millstone
Grit of the North Wales Border,” by D. C. Davies ; “The Character
of Lavas,” by G. Poulett Scrope, F.R.S.; “On Faults in Strata,”
by W. T. Blanford and by G. H. Kinahan ; “ New Zealand Plesio-
saurs,” by Professor Owen; “ Boulder-Clay,” by Mr. James Geikie ;
“ Banded and Brecciated Concretions,’ by Dr. Ruskin. If Mr.
Searles Wood, jun., can only induce the Geological Survey to adopt
his classification for the later deposits of our island, much of our
misery and uncertainty about the Contorted Drift and Boulder-Clay
ends, and we may find a place for every pebble-bed and drift-deposit
which we meet with, and can colour it at once.
But the Geological Survey are not converted, although they will,
doubtless, gladly adopt much of Mr. 8. V. Wood, jun.’s, admirable
work on East Anglian surface-geology, when they come to Norfolk,
Suffolk, and Essex.
Mr. Scrope continues his favourite theme, the character of Lavas.
We hear, by-the-by, that he is arranging with Mr. Archibald Geikie
a descent upon the Lipari Islands and Stromboli this summer, so we
may look for a new view of modern volcanoes from a leading man of
the day in Geology.
PROCEEDINGS OF THE GEOLOGICAL Society oF Lonpon.
The present number of the ‘Quarterly Journal’ of this Society
deals in Australian Geology and Paleontology. On Dinosaurian
Reptiles and their affinity with Birds. The evidence afforded by
corals as to the physical geography of Western Europe in Secondary
and Tertiary times. The Brachiopoda of the Budleigh-Salterton
pebble-bed. A comparison of the Boulder-clay of the North of
England with that of the South. On the Graphite of the Lauren-
tian of Canada. On the Geology of the country around the Gulf
of Cambay. On the Rodents of the Somersetshire Caves.
With rocks of Secondary age in Australia we have been hitherto
unacquainted, and there seemed good reason to believe that this
remarkable country held its head above water through the Mesozoic
eriod. ©
: Mr. Charles Moore has, however, brought before us evidence of
1870. | Geology and Paleontology. 273
the occurrence of fossils in erratic blocks from Western Australia,
from the centre of the Continent, on Stuart’s route, and from
Queensland. These remains, although fragmentary, suffice to in-
dicate fossils of Liassic, Oolitic, and Neocomian age.
The propriety, however, of applying the European paleonto-
logical standard to the geology of the Antipodes is exceedingly
doubtful, and we are more than ever impressed with the value of
the late Edward Forbes’s observation, that the occurrence of similar
fossils in formations of widely-separated continents was rather a
proof of the diversity of their age than of their synchronous cha-
racter. That marine faunas extend over a far wider geographical
area than land animals must be admitted, but Mr. Seeley’s obser-
vation, that natural groups of corresponding value exist in different
areas of the globe, deserves consideration.
Professor Huxley contributes three papers, all bearing upon the
Dinosauria and their affinity with Birds.
The skeleton of a young Iguanodon from the Wealden of the
Isle of Wight (described long since by Professor Owen) proves,
upon further examination, to be a new genus of Herbivorous Dino-
saur (Hypsilophodon Foxit), and assists largely to increase the
evidence in favour of the affinity between Dinosaurian Reptiles and .
Birds. A head of Hypszlophodon (obtained by the Rev. W. Fox),
and referred to the same species, seems to have had its preemaxilla-
ries produced downwards and forwards into a short edentulous beak-
like process, the outer surface of which is rugose and pitted. The
peculiar form of the lower jaw of Iguanodon would seem to indicate
that its emargination was destined to receive this beak-like process.
of the premaxillaries. The pelvic bones are singularly avian in
their structure.
Professor Huxley reviews in his second paper the evidence
already cited by himself and others (especially by Professor H. D.
Cope, of Philadelphia), in favour of the ornithic affinities presented
by the Dinosauria, and discusses at length the recently ascertained
facts which bear upon this question. He compared the different
elements of the pelvic arch and hind limbs in the Crocodile, the
Dinosaur, and the Emu, and maintained that the structure of the
pelvic bones (especially the form and position of the ischium and
pubis), the relation between the distal end of the tibia and the
astragalus (which is perfectly ornithic), and the strong enemial
crest of the tibia, &c., furnish additional and important evidence
of the affinities between the Dinosauria and Birds.
In Professor Huxley’s third paper he referred to the biblio-
graphy of the Dinosauria, which, as a distinct group, were first
recognized by Hermann von Meyer in 1830. He then indicated
the families, into which he proposed to divide the group, viz.:
1. The Megalosauridx, with the genera Teratosawrus, Palxo-
274 Chronicles of Science. [April,
saurus, Megalosaurus, Potkilopleuron, Lelaps, and probably Eus-
kelosaurus.
2. The Scelidosauride, with the genera Thecodontosaurus,
Hylzosaurus, Pholacanthus, and Acanthopholis. (The omission
of Scelidosawrus is of course accidental, as the family is founded on
that genus.)
3. The Iguanodontide, with the genera Ceteosaurus, Iguanodon,
Hypsilophodon, Hadrosawrus, and probably Stenopelys.
Although Compsognathus had many points of affinity with the
Dinosauria, as in the ornithic character of its hindlimbs, yet it
differed from them in several important particulars. Professor
Huxley therefore makes a separate group for it, the Compsognatha
forming, with the Dinosauria, an order, the Ornithoscelida.
After treating of the Ornithoscelida in relation to other reptiles,
he concludes to place them in that great division of the Reptilia
which he calls Suchospondylia, in which the thoracic vertebre have
distinct capitular and tubercular processes. The Suchospondylia
embraces the Crocodilia, the Dicynodontia, the Pterosauria, and
the Ornithoscelida.
With regard to the relation of the Ornithoscelida to birds,
Professor Huxley stated that he knew of no character by which
the structure of birds, as a class, differs from that of reptiles, which
is not foreshadowed in the Ornithoscelida.
Dr. Duncan’s paper “On the Geography of Western Europe
during the Mesozoic and Cainozoic periods,’ elucidated by their
Coral-faunas, would seem to have been intended to create a discus-
sion for the purpose of bringing out the younger Agassiz, who is
over for a visit in Europe. Considerable misconception exists in
the minds of even advanced naturalists, as to the species of corals
peculiar to the deep sea, as contrasted with the reef, lagoon, and
shallow-water species. Dr. Duncan contrasted the fauna existing
in our seas with the extinct coral-fauna of the Secondary and Ter-
tiary epochs, and pomted out that a correspondence of physical
conditions in the deposition of certain strata was marked by the
presence of similar organic remains; thus the presence of compound
coenenchymal species of coral indicated reefs, and their absence in
places where simple or non-ccenenchymal Madreporaria are found,
is characteristic of deep-sea areas remote from land.
Professor Alexander Agassiz thought the depth at which true
reef-building corals are said to exist would be considerably ex-
tended. A reef is in the course of formation at the present time
off the coast of Florida.
Mr. Davidson has determined nearly forty species of Brachio-
poda from the pebble-bed at Budleigh-Salterton, near Exmouth,
Devon, and has figured them with his usual accuracy and artistic
skill in three beautiful plates. It is to be feared that, with certain
1870. | Meteorology. 275
paleontologists, a difference in horizon is sufficient to constitute a
difference in species; hence the zones of Ammonites, each marked
by a different species, which is said never to occur above or below
a certain narrow bed or horizon.
Professor Huxley would like to see the rise of a new race of
paleontologists, relying simply on zoological characteristics, and not
upon geological position. A considerable reduction in the number
of species would, he thinks, undoubtedly result.
Although the term species is too often used where variety would
be more appropriate, yet these distinctions —when kept within due
bounds—have been found of great value in tracing out, by their
characteristic fossils, the horizon of beds over widely-extended areas.
Mr. Searles V. Wood, jun., continues his researches on the
Boulder-drift. He finds the Yorkshire Glacial clays are of two
kinds; the lower containing chalk-debris abundantly, the upper
containing chalk sparingly in its lower part, and gradually losing
it upwards. The Boulders of Shap Fell Granite only occur in the
Boulder-clay, without chalk. Mr. Wood ascribes their dispersion
to the agency of floating ice during the submergence of the district.
The great chalky clay derived its chalk from the extrusion of a
great sheet of land-ice over the sea, the chalk-mud being due to the
abrading action of the ice.
The anniversary of the Geological Society of London was held
on the 18th February, when the President announced that the
Wollaston Gold Medal had been awarded to M. Deshayes, as an
expression of the estimation in which his services to Paleontology
and Geology (especially in regard to the classification of the Tertiary
formation and its Molluscan fauna) are held by geologists of this
country.
The balance of the Wollaston Donation-fund was presented to
M. Marie Rouault, of the Geological Museum of Rennes, in aid of
his researches upon the paleontology of the Devonian and Silurian
rocks of Brittany.
Neither of the gentlemen was present, but both sent letters of
thanks.
8. METEOROLOGY.
THe subject which has secured to itself the most important papers
published lately has been the wind-systems of the globe, a question
which had been left at comparative rest for some time.
Mr. Buchan’s paper “ On the Mean Pressure of the Atmosphere,
and the prevailing Winds over the Globe,” appears in vol. xxv. of
the ‘ Transactions of the Royal Society of Edinburgh,’ and has been
most carefully worked out. The mean monthly conditions of atmo-
276 Chronicles of Science. | April,
spherical pressure at the sea level are first discussed, on the basis of
all trustworthy observations which were accessible, and then the
prevailing winds are similarly treated, but with reference only to
direction, not to force. The results obtained are entered on charts
for each month and for the year. The broad facts arrived at are
that the wind flows in accordance with Buys Ballot’s Law around
the areas of barometrical depression and elevation, the motion being
retrograde in the first case, direct in the other, and that it does not
flow as a constant anti-trade at the earth’s surface in high latitudes,
as supposed by Maury. The ‘position of the respective areas of
barometrical disturbance varies very considerably from month to
month, and is mainly determined by the thermal conditions of the
globe at the respective seasons.
It will be seen that the ideas of Mr. Buchan are somewhat at
variance with Dove’s theory of the paramount importance of the
Polar and Equatorial currents (as N.E. and 8.W. winds) in regu-
lating climates. He has, however, submitted this theory to a special
test, as on calculating the directions of the prevailing winds at each
station he finds that almost always there are two maximum directions
shown, but that in only 30 per cent. of the stations do these direc-
tions belong to either of the above-named winds; so that it cannot
be maintained that there is a general flow of the winds of the North
Temperate Zone towards and from the Polar regions.
In the theoretical explanation of air-motion, given by Mr. Buchan,
the chain of reasoning is not perfectly conclusive. He argues in this
way: if motion in the lower strata of the atmosphere be in a definite
direction, a compensating movement must exist at an upper level.
The lower currents are determined by the course of the isobaric
lines, therefore the upper currents may be inferred from these same
lines “ taken reversely together with the isothermal lines taken
directly.” He assumes that if, over any area, temperature near the
ground be low, it must necessarily follow that pressure at a great
height over the same area must be much reduced. This may perhaps
be true, but it is far from being as yet proved, in the utter absence
of the possibility of any experimental confirmation of the statement,
as we know nothing of the vertical distribution of pressure.
Taking the paper as a whole, it is one of the most valuable con-
tributions to the science which has appeared of late years, and the
least that can be said of it is that the results are fully commensu-
rate with the labour bestowed on the discussion.
The other paper to which we have referred is one by Dr. Julius
Hann, “ On the Winds of the Northern Hemisphere and their In-
fluence on Climate,” read before the Vienna Academy. In the first
part of this discussion the wind-systems are explained on the hypo-
thesis of Dove’s two currents ; the Equatorial, flowing over the sea ;
and the Polar over the land: but the variations in their respective
1870. | Meteorology. 277
directions from true 8. W. and N.E. are explained by the relations of
pressure. ‘That these variations do exist is shown by the fact that
in the great continent, the coldest point of the windrose shifts
through 108°, from N. 62° E. over the North Sea, to W. 44° N. in
Eastern Asia. The warmest point shifts similarly through 61°.
Corresponding changes are noticeable in the baric windrose, so that,
as Buchan shows, the main directions of the wind are not 8.W. and
N.E. As to the effect on rain, it is found that the sea winds are
always the rain bringers, and the land winds the contrary. Our
driest wind is N.E.; that for Pekin as well as for Toronto is N.W.
Part LI. is a special application of the results contained in the tables
to the peculiarities of climate of the respective stations.
The quarter has on the whole been rather barren of meteorolo-
gical papers both here and on the Continent, but this deficiency has
been more than supplied by some works of a general nature. Mr.
Keith Johnston, jun., has just brought out a ‘ Handbook of Physical
Geography,’ as a companion to the ‘ Physical Atlas.’ The chapters,
three in number, relating to Meteorology are very compact and
comprehensive. Much of what he says on winds has been adapted
from Mr. Buchan’s paper just noticed; but as regards climate, the
account of the Range Lines is a reproduction of a very good paper
by the author, which appears im vol. vi. of the ‘ Proceedings of the
Royal Society of Edinburgh.’ In this paper he has discussed the
range of temperature from January to July all over the globe. This
map is an entirely new idea, and a most useful one, as in the ques-
tion of Range all the differences between insular and continental
climates are involved. ‘Thus in these islands the range is about 20°.
At Yakutsk it is 106°. No part of the open ocean has a range
above 40°, while the curves above 60° are confined to the great
continents.
On the whole, Mr. Johnston finds, as a practical result, that in
the Temperate Zone the West coasts of continents have 15° less
range than the East coasts, and a similar contrast is noticed between
the opposite coasts of inland seas and lakes. ‘Thus the coasts of the
Mediterranean, which face Hast, have 10° more range than those
which face West. The same fact is noticed on the shores of Lake
Superior.
Dove has at last published Part Il. of his ‘ Klimatologische
Beitrage, twelve years after its predecessor. In this he furnishes
the text and tables to the ‘ Atlas of Monthly and Yearly Isotherms,’
which appeared in 1864. The first fifty pages are devoted to a
brief discussion of the climate of Western Europe, which is very
interesting, but hardly worthy of the author’s reputation. If we
test it by what he says of these islands, it is evident that the sources
of information are old and not quite accurate, while the statements
themselves bear signs of haste and carelessness. Thus we are told
VoL. VII. U
278 Chronicles of Science. [ April,
that the hemispherical cup anemometer was invented by Osler,
and improved by Dr. Robinson. Dove assumes that observations
in London, Liverpool, and Dublin, represent our climate fairly,
while the instances cited to prove the mildness of our climate fall
far below the real facts of the case, especially in the vegetable world.
This paper is followed by some remarks on the climate of the Polar
regions, but the bulk of the work is taken up with Temperature
Tables. These are most valuable, containing, as they do, for about
1200 stations the yearly, monthly, and seasonal means, with the
extreme range of climate, as well as that from summer to winter.
To these tables are appended others of the non-periodic variations,
giving for more than 400 places the monthly means derived from
several years’ observation, and the deviations from those means
observed in every year from 1856 to 1868. Remarks on the ave-
rage and absolute variability of temperature follow, and the volume
is concluded with a notice of some of the most remarkable exceptional
seasons which have been recorded, such as severe winters, e. g. 1838,
1850, both of which, though cold in Europe, were warm in America ;
famous vintages, e.g. the Comet Year, 1811, and various other
notabilia as regards climate. Many of these particulars have been
already described by Dove in his ‘ Five-day Means of Temperature,’
and in his papers read before the Berlin Academy ; but the thanks
of all meteorologists are due to him for having condensed such a
mass of information into a work of 300 pages.
Professor Wild has followed up the publication of the ‘ Annales’
for 1865 for the Russian stations by the announcement of the issue
of a new serial, ‘ Repertorium fiir Meteorologie.’ Formerly, a period-
ical under this title was published by the Geographical Society, at
the suggestion of Kamtz, who was himself the author of most of
the papers in it. The new ‘Repertorium’ is to appear under the
auspices of the Academy, and to contain special discussions of the
’ observations which are given in full in the ‘Annales, as well as
independent papers on the Meteorology of Russia. The first part
has already come out, and we find in it the instructions for the
reorganization of the meteorological stations throughout Russia,
with the tables for the reduction of observations on the basis of
centigrade and metrical scales, which are to be substituted for the
former tables drawn up by Kupffer. There is also an ‘ Essay on
the Wind and Rain of Taurida and the Crimea, by W. Koeppen.
It is impossible to do more than allude to this paper, which is of the
ereatest value, being a discussion of a large accumulation of trust-
worthy observations.
It is curious that at the very time that Sir E. Sabine was dis-
cussing the climate of Barnaoul and Nertschinsk, as described in our
last number, Lieutenant Rikatcheff was investigating the same sub-
ject, and he has published his results in a paper “On the Diurnal
1870. | - Meteorology. — 279
March of Temperature” at the two stations in question, deduced
from a series of twenty years’ hourly observations. This paper forms
part of No. II. of the ‘Repertorium.’ The results on the whole
agree very well with Sir E. Sabine’s. The climate of Nertschinsk
is more truly continental than that of Barnaoul, but this difference
is not exhibited to its fullest extent, owing to the difference in ele-
vation between the two stations, the former being situated 2200
feet above the sea, as compared with 400 feet, the elevation of the
latter.
The second report of the ‘ Norddeutsche Seewarte,’ that for the
year 1869, has just appeared. The main points brought forward —
by Herr von Freeden in this report have a special reference to
Sailing Directions and to the practical pecuniary value of the office
to the shipowners and traders of Hamburg. Accordingly, hitherto
he has not been able to devote his attention to the general subject
of ocean meteorology. However, the North German Parliament
has now adopted the office, and several of the seaport towns of
Prussia, such as Memel and Dantzic, have affiliated themselves to
it as branch stations for the issue of instruments and registers.
The Report also contains interesting information relating to the
Telegraphic Intelligence of Storms, sent to Hamburg by the Me-
teorological Office in- London. From this it appears that the storm
only preceded the warning on four occasions, three of which were
accounted ior by the intervention of Sundays, and that no intelli-
gence at all of two other storms was received, owing in one case to.
a break-down on the telegraph line. Accordingly it will be seen that
the storms which are felt on the Elbe almost invariably pass over
these Islands. The instances in which the weather at Hamburg
was undisturbed, subsequent to a warning, are all proved to have
been accounted for by the fact that the storm died out before crossing
the North Sea.
Tn conclusion, we have to notice the very important changes as
regards meteorology which are in progress in France. M. Le-
verrier has been superseded, and his successor at the ‘Observatoire
Impérial’ is M. Charles Delaunay. It is understood that for the
future meteorology will form no part of the duties of the astro-
nomical staff, and we hope that ere long this special science will
receive in France a development worthy of its daily increasing
importance.
280 Chronicles of Science. | April,
9. MINERALOGY.
From the days when Montezuma presented Cortez with four Chal-
chihuitls, on his landing at San Juan de Ulua, it has been matter
of dispute among mineralogists what was the true nature of the
ornamental stone designated by this Mexican name. That it was
held in the highest esteem is well known from many passages in the
old chroniclers. It appears to have been worn only by the chiefs,
and on the death of a great dignitary a chalchihuit] was placed in
the mouth of the corpse. Indeed, the name of the stone became
synonymous with all that was most valued; and according to one
tradition, Quetzalcoatl—the law-giver, priest, and instructor of the
Mexicans—was begotten by one of these stones, which the goddess,
Chimalma had placed in her bosom. In recently laying before the
Lyceum of Natural History of New York a fine collection of carved
chalchihuitls, Mr. Squier took occasion to bring forward a body of
evidence tending to identify the stone.* Molina, in 1571, defines
the word as signifying esmeralda baja—an inferior emerald. Saha-
gun describes it as “a jasper of very green colour, or a common
emerald.” Montolina, in 1555, in enumerating the riches of Mexico,
after speaking of gold, silver, and all metals and stones, refers to the
chalchihuitls, and concludes by saying, “ Las finas de estas son esme-
raldas.” Professor Blake has sought to identify it with the turquoise,
but the author considers this not to be the true stone of the Mexi-
cans and Central Americans. “The weight of evidence, in my opi-
nion,” says Mr. Squier, “ goes to show that the stone, properly called
chalchihuitl, is that which Molina defines to be ‘ baja esmeralda,’
or possibly nephrite, ‘a jasper of very green colour,’ as Sahagun,
already quoted, avers.”
Two Indian meteorites have been subjected to an exhaustive
examination by Professor Nevil Story Maskelyne, the Keeper of the
Collection of Minerals in the British Museum—a collection which
vies with Vienna and Calcutta in the number and variety of its me-
teoric specimens. One of the stones fell at Busti, between Goruck-
poor and Fyzabad, on the 2nd Dee., 1852; and the other fell at
Manegaum, in Khandeish, on the 26th July, 1843.7 The Busti
meteorite consists for the most part of enstatite, a silicate of mag-
nesia, in which are imbedded small spherules of Oldhamite. This
mineral is composed mainly of sulphide of calcium ; and the presence
of such a compound would seem to indicate that the conditions under
which the ingredients of the meteorite were formed must have been
very different from those met with on the surface of our globe.
* ‘Observations on the Chalchihuitl of Mexico and Central America.’ By
E. G. Squier, M.A. New York, 1869.
+ ‘ Proceedings of the Royal Society,’ Jan. 13, 1870, p. 146.
1870. ] Mineralogy. 281
Not only does it bespeak the absence of water and of oxygen; but
having regard to the conditions needful for the production of this
particular compound, the author thinks himself justified in pointing
to the presence of some reducing agent, which operated during the
formation of the constituents of the stone—such an agent as would
be furnished by Graham’s meteoric hydrogen.
Oldhamite forms spherules of a chestnut-brown colour, having a
specific gravity of 2°58, and presenting. a cubic cleavage. In some
of these spherules there are minute gold-coloured octohedral crystals,
which contain calcium, sulphur, and a rare metal—probably tita-
nium. As a befitting compliment to the gentleman who forwarded —
the Busti meteorite to this country, Maskelyne describes this second
mineral under the name of Osbornite.
Dr. Giovanni Striiver’s studies in Italian mineralogy have lately .
been directed to the examination of the iron-pyrites of Piedmont
and of Elba.* In the collection of the Engineering School of
Turin, and of the University Museum in the same city, nearly 6000
specimens of Italian pyrites are to be found. The author has thus
had ample materials for study, and that he has made good use of
his opportunities is clear from his exhaustive monograph on the
subject. He describes the various simple forms and combinations
in which the Italian mineral occurs, including many newly-observed
forms. It is notable that in 5603 specimens only three distinct
simple forms were found. The memoir is illustrated by a series of
fourteen plates.
Some few years ago, Herr Stein described a mineral under the
name of Staffelite. It had the extraordinary composition of a hydrous
phosphate and carbonate of lime, with a fluoride of calcium and
traces of iodine. It occurred usually as a greenish incrustation, but
was said to be also found in rhombohedral crystals. A similar sub-
stance has been met with in certain phosphorite workings near
Offheim, in Nassau ; and upon this crust of so-called staffelite were
some fine clear crystals of apatite. Dr. Kosmann publishes an
analysis of this apatite,t and assigns to it the formula: 5 (3 CaO.
~PO;)+2CaFl. It is notable for contaiming as large a percent-
age as 4:52 of fluorine, and for the presence of magnesia. The
author believes that staffelite is nothing more than an impure
form of apatite rapidly deposited and contaminated with the salts
of the mother-liquor from which it was evaporated. Dr. Kosmann
also describes a new mineral under the name of Lime Wavellite, the
composition of which is sufficiently indicated by its name.
In the Bergmannstroost mine at Altenberg in Silesia certain
needle-like crystals are found penetrating brown-spar. Under the
* “Studii sulla Mineralogia Italiana. Pirite del Piemonte e dell’ Elba.’
Torino, 1869.
+ ‘ Zeitschrift d. deutschen geolog. Gesellschaft,’ Bd. xxi., Heft 4, p. 795.
282 Chronicles of Scvence. [ April,
microscope they appear as strongly-striated rhombic prisms, with
indistinct octohedral terminations. Formerly they were taken for
antimony-glance, but when it was found that they contained lead,
they were referred to either the species Jamesonite or Boulangerite.
Dr. Websky has, however, recently shown that this mineral con-
stitutes a new ore, which he proposes to designate as Epiboulange-
rite. It is a sulphide of antimony and lead, which may be thus
formulated: (Sb,, P b;) §,;.*
Professor Wohler announces the discovery of minute crystals of
diamond, with the native platinum of the Oregon; and diamonds
are also reported from Bohemia.t}
Ramelsberg has been led to compare the relation of gadolinite
with several other species, and finds that datolite, euclase, and
gadolinite form an isomorphous group.t
10. MINING AND METALLURGY.
Mintne.
THE mining interests of the country are promised rather more than
the usual amount of attention from the British Legislature during
the present sitting of Parliament.
The Secretary for the Home Department has introduced his
“ Mines Regulation and Inspection Bill,’ which was read for the
second time on the 21st of February.
Lord Kinnaird, on Thursday, the 17th of February, introduced
a Bill to the House of Lords, which is an attempt to apply the
“Mines Regulation Act of 1870” to the metalliferous mines of the
country.
The President of the Poor Law Board has intimated his inten-
tion of bringing again, before the House of Commons, the considera-
tion of the question of rating metalliferous mines for the support
of the poor.
The Government Mines Regulation Bill, introduced by the
Home Secretary, professes, in its broader features, to fix definitely
the responsibility in connection with the workings of all collieries,
to secure increased safety in the mine, and to promote the better
education of the mining population.
Last year the Mining Association of Great Britain, and the
Colliery Inspectors, representing the Home Secretary, agreed to the
following provision :—‘“ That in every coal and ironstone mine an
amount of ventilation shall be constantly produced, adequate to
* ¢ Zeitschrift d. deutschen geolog. Gesellschaft, Bd. xxi., Heft 4, p. 747.
+ ‘Comptes Rendus,’ 24 Jan., 1870, p. 140.
t ‘ Zeitschr. d. d. geol. Gesell.,’ Bd. xxi., Heft 4, p. 807.
1870. | Mining. 283
dilute and render harmless noxious gases, to such an extent, that
the working places of the pit’s levels and workings, and the travel-
ling roads to and from the working places, shall be in a fit state for
working and passing therein, but that no owner, agent, or other
person shall be held to have contravened this regulation, wnless tt
shall be shown that all reasonable precautions have not been taken.”
This saving clause has been altered in the present Bill to :—“ Pro-
vided that no owner, agent, or other person shall be held to have
acted in contravention of this regulation, if it is shown that all
reasonable precautions have been taken by the owner, agent, or
person who is so charged.” |
This proposition is regarded as the turning-point of Mr. Bruce’s
Bill, and already loud is the cry amongst colliery owners and agents
against it. “It cannot be supposed for a moment,” says the ‘ Colliery
Guardian,’ “that they (the coal-owners) can take any other course
than that of opposing it to the utmost, nor will they find any diff-
culty in showing that English legislation contains no precedent for
an enactment which assumes that every person charged is guilty,
and may be punished as such, unless he can prove himself innocent.”
The question of responsibility ig the one over which the battle
will be fought. Every one is, of course, desirous of relieving him-
self from this burthen; and it is, indeed, a heavy one in some of our
collieries, where the lives of hundreds of men are dependent entirely
on the unceasing attention of a single mind. If the colliery owners
and agents can relieve themselves of this by any pressure which
they can bring upon our legislators, they will most certainly exert
themselves to the utmost to secure the necessary force. We cannot
ourselves sée any alternative. The responsibility of securing the
most perfect appliances, in every division of the workings of a
colliery, must rest somewhere, and it cannot be allowed to be capa-
ble of being shifted from one individual to another. In every
colliery some head-man must be made responsible, and the Bill does
not appear unjust on this point, for if this responsible head can
show, after an accident has occurred, that every proper precaution
had been taken, he will be held to be guiltless of any blame.
The employment of women and children, the payment of wages,
the special rules and provisions as to arbitration, are all carefully
dealt with in this Bill. The clauses which relate to inspection do
not appear to us to be entirely satisfactory. Much has been said of
the inability of twelve inspectors to visit, within the year, the 3000
collieries in the United Kingdom. It does not appear to us to be
desirable that they should do so, but an earnest and intelligent man
may make himself perfectly familiar with his district, without sub-
jecting himself to the labour, or the coal-owner to the annoyance, of
prying into the details of the subterranean workings. Lord Elcho
remarked,—“ The name of ‘Inspector’ was a misnomer, for the in-
284 Chronicles of Science. [ April,
spectors did not profess to go into the mines, they merely held an
inquiry when an accident had occurred. Accordingly they might
with more truth be called ‘ Accident Inquirers.” We fear a good
and sufficient reply cannot be given on this point to Lord Elcho.
Mr. Bruce, anticipating, as he could well do, from the discussions of
last year, on the same subject, attempted to answer this, but all that
he said, cannot be regarded as other than ingenious special pleading.
Mr. Lancaster referred to many of the causes leading to our
present imperfect system of working for coal. To these we can
only direct attention. His concluding remarks are of too much
value not to be quoted :—“ While many of the managers of mines
were men of first-class education, and also of great practical ex-
perience, it was necessary that the younger men should receive a
technical as well as a practical trainmg. He hoped that as to
some of these questions, the Home Secretary would adopt a much
bolder course than that which he had yet taken, and would not
hesitate to carry out the full recommendations which had been
made.”
Lord Kinnaird’s Bill provides for the establishment of General
Rules and Special Rules for Metalliferous Mines as nearly similar
as possible to those proposed for collieries. It is evident from this
that the different conditions of the two systems of mining cannot be
correctly understood by his Lordship. The Bill provides for the
effective ventilation of the metal mines, the depositing of plans
with the Secretary of State (there never has been any objection to
furnishing plans, as the large collection already in the hands of the
Government in the Mining Record Office proves), and for. such
arrangements as are thought to be conducive to the health of the
miners.
“Our Future Coal Supply” has claimed the attention of the
South Staffordshire and East Worcestershire Institute of Mining
Engineers, Mr. Richard Latham and Mr. George Spruce contri-
buting two papers containing much important matter relative to the
future workings of the thick coal of Staffordshire, and the probable
extension of the Staffordshire field towards the coal-field of Shrop-
shire.
Mr. Walter Ness, of Pelsall, also read a paper “On part of the
Coal-field of Fife, N.B.,” in which he proved, probably beyond much
doubt, a large extension of this coal-field beyond the present work-
ings. From this he adventures farther from the shore, and says:—
“Tf we take the total area of the Forth, where we have reason to
believe those Coal-measures exist in their entirety, we have about
180 square miles in their entirety . . . and we get 12,672,000,000
tons. Taking the other parts of the nation (sea-bed ?) in like manner
available, opposite Northumberland, Durham, and Yorkshire, and
under the German Ocean, also opposite Ayrshire, Cumberland, Lan-
1870.] Physics. 285
cashire, and the Bristol Channel, on the west coast, as jointly capable
of yielding a similar quantity of coal to that of the Firth of Forth, we
shall then have 25,344,000,000.” These are large figures—of their
value we can only judge by the exactness of other statements made
in this paper. “The investigation of the Royal Commission happily
assures us that there is coal enough in store for several generations
to come.” Such is the opening paragraph of Mr. Walter Ness’s
paper. The fact bemg that the Royal Commission has not given
one word of assurance in any form—and, we can state upon autho-
rity, that they are not yet in a position to do so.
METALLURGY.
There does not appear to be any novelty worthy of notice. The
arrangements made upon the termination of one of the Bessemer
Patents have led to considerable activity in the manufacture of
Bessemer steel, and probably the result will be that, ere long, steel
rails will almost entirely have superseded the iron ones, to which
we have been so long accustomed.
A few interesting experiments are in progress, but none of the
results yet obtained are sufficiently reliable to warrant our placing
them on record.
i -PENYSICS.
Licut.—It is a well-known fact that M. Schroetter proved that
the action of sunlight converts ordinary phosphorus into red
amorphous phosphorus. Sulphur, according to M. Lallemand, is
similarly affected by the direct action of sunlight, masmuch as the
sulphur previously soluble in sulphide of carbon, and crystallizable,
is converted into an amorphous modification insoluble in sulphide
of carbon. The author placed a concentrated solution of sulphur
in sulphide of carbon in a sealed tube, and exposed that tube some
time to the action of the sun’s rays, concentrated by a lens; this
causes a copious precipitation of sulphur as an amorphous insoluble
matter.
_ Mr. Burt has examined the action of coloured light upon the
Minwsa pudica. The plants are placed under glass jars constructed
of variously-coloured glass. The chief fact observed in respect of
these very sensitive plants is that by being covered with a green-
coloured glass jar, the plant rapidly becomes insensible, and dies in
a very short time.
The Rev. Father Secchi, after referring briefly to his former
observations of the spectrum exhibited by Uranus, states that the
286° Chronicles of Science. | April,
spectrum of Neptune consists chiefly of three lines, or bands, placed
near the green, and that its light is entirely devoid of red; this ig
confirmed by the colour exhibited by the planet when seen through
a telescope, which is a sea-green.
M. Feil has exhibited before the French Academy samples of
perfectly homogeneous heavy flint-glass for optical purposes free
from any bubbles or defects, and in masses weighing from 25 to
35 kilos. The process whereby this is obtained is not explained ;
but the statement is made that the crucibles having been protected
from the effects of the lead, a heavier glass even than Faraday’s
can be made. ‘The maker sent also a set of samples of beautifully-
made artificial precious stones, not mere specks, but of good size.
The aluminates of lime, of baryta and lime, of lead and of bismuth,
are proposed for flint-glass; and the aluminates of magnesia and
the silicates of magnesia and alumina for crown-glass.
M. Bontemps, the managing director of the celebrated glass
works at Choisy-le-Roi, has arrived at the followmg results in con-
nection with the coloration of glass under the influence of direct
sunlight :—Within three months after having been exposed to sun-
light, the best and whitest glass made at St. Gobain is turned very
distinctly yellow ; extra white glass (of-a peculiar mode of manu-
facture) has become even more yellow, and gradually assumes a
colour known as pelwre d’oignon; glass containing 5 per cent. of
litharge was also affected, but far less perceptibly; crystal glass,
made with carbonate of potassa (the other varieties referred to
contain carbonate of soda), litharge and silica, was not at all affected ;
English plate-glass, made by the British Plate-Glass Company,
and exhibiting a distinctly azure-blue tinge, remained also un-
affected. The author attributes the coloration, which begins with
yellow and gradually turns to violet, passing through red pelure
@oignon, to the oxidizing effects of the sun’s rays upon the pro-
toxides of iron and manganese contained in glass.
M. Schinz states that platinum brought to bright white heat
by means of the ignition of a mixture of hydrogen and carbonic
oxide gases, yields a light which, in relation to good coal-gas, is as
1°24 to 1:0.
Professor B. Silliman has examined, in a lengthy series of ex-
periments, the relation between the intensity of light produced from
the combustion of illuminating gas and the volume of gas consumed.
His experiments prove, among other matters, this theorem—that
the intensity of gas-flames (7. e. illuminating power) increases,
within the ordinary limits of consumption, as the square of the
volume of the gas consumed. The chief point of interest, for the
consumer of gas, to be deduced from the data here presented is, that
where it is important to obtain a maximum of economical effect —
1870.] Physies. 287
from the consumption of a given volume of illuminating gas, this
result is best obtained by the use of burners of ample flow.
Hrat.—According to MM. Troost and Hautefeuille, carbon
when combining with oxygen, only gives out 8000 caloric units;
boron, under the same conditions, yields 14,400 caloric units ; while,
when boron combines with three equivalents of chlorine, 104,000
caloric units represent the heat set free.
The heat disengaged by the combination of 1 grm. of amor-
phous silicium with oxygen is 7830 units, with chlorine 5030.
When 1 grm. of chloride of silicium reacts upon 140 times its
weight of water, it is 2915; the heat disengaged when 1 grm. of
amorphous silictum is converted into crystallized silicium is 290
units of heat.
Dr. St. Claire-Deville states that the oxygen dissolved during
the fusion of platinum causes this metal to present the same pheno-
menon as molten silver—viz. scintillation and spirting while in the
molten state. :
In a paper “On the Heat given off by the Moon’s Rays,”
M. Zantedeschi states that, as far back as the years 1685 and 1781,
the Italian savants Geminiano, Montanari and Paolo Frisi proved
the existence of rays of heat emitted by the moon, by means of
lenses and ordinary thermometers. The author refers to his
observations made some twenty years ago, when he applied thermo-
electric apparatus, as well as spirit thermometers and lenses, and
obtained results fully confirming those made and recorded by the
Tialian savants just alluded to. |
In Germany the doors of the steam-boiler furnaces are now very
generally provided with square pieces of mica, properly fastened, by
means of which the fireman is enabled to observe the fires without
the necessity of opening the furnace-doors too frequent!y, which is
injurious, on account of interfering with the draught and proper
course of combustion of the fuel, by reason of the access of irregular
currents of cold air. Mica withstands avery high temperature ; and
the accidental breakage of the squares of this substance is guarded
against by a properly-constructed iron-wire guard outside.
Dr. Ziurek states that gas from the brown coal from Fursten-
wald, five miles from Berlin, will shortly be made on the spot, and
collected in Berlin in twelve gas-holders, each of a capacity of
750,000 cubic feet. The gas will be carried, as usual, in under-
ground mains, and chiefly applied for heating purposes. 3000 cubic
feet of this gas have a heating power of one-third of a ton of best
coals, and are equal to 1 ton of best Prussian brown coal. 1000
cubic feet of this gas will cost about 5d. in Berlin; and the equi-
valent value of the heating power of this gas as compared with a
288 Chronicles of Science. [ April,
ton of coals will be 4s. 6d. The works have been made to supply
950,000,000 cubic feet of gas annually, or at the rate of 22 millions
of cubic feet daily.
Execrriciry.—A thermo-electrical apparatus, with galena and
iron, has been made by MM. Mure, Clamond, and Gaiffe. Ac-
cording to the results of their experiments, this apparatus deserves
the attention of all who require galvanic batteries, since regularity
and steadiness of action are here combined with economy and the
absence of inconvenient vapours.
For telegraphic work or domestic purposes, where a constant
galvanic current is required with little trouble (electric bells, fire and
thief detectors), the writer has found the new battery known as the
Leclanché cell to be most perfect in action. ‘The main feature is
that peroxide of manganese is used with zinc (not amalgamated) and
an aqueous solution of an alkaline salt, chloride of ammonium being
preferred. The cells are of three sizes: the smallest, with a porous
pot 4°3 inches high, can accomplish an annual electric work which
may be represented by 620 grains of copper reduced in the voltameter ;
the medium size, with a 6-inch porous pot, can reduce from 950 to
1000 grains; while the large size gives a work equal to 1500 or
2000 grains.
F. Zaliwski has described a galvanic element with three fluids.
This contrivance consists of two porous cells placed one inside the
other, and surrounded by another suitable vessel. The inner vessel
contains nitric acid and a piece of carbon, the intermediate vessel
contains sulphuricacid, and the outer vessel a solution of sal-ammoniac
in water and a piece of zinc. This author states that this arrange-
ment is superior to a Bunsen cell.
The phenomena of atmospheric electricity at the island of Haiti,
or St. Domingo, as it is also called, are of a very striking character.
According to Mr. Ackermann, who has during a series of five years
made meteorological observations at Port-au-Prince, there have, on ©
an average, been 129 days of each year either severe thunderstorms
or other very marked electrical phenomena, especially during the
months of May, July, August, and September. Severe thunder-
storms more frequently occur during day than night-time. The
year 1868 was especially remarkable for severe thunderstorms ;
during one of these, lasting for forty-five minutes, 400 lightning
flashes were distinctly seen.
A company has been formed in America with the view of cover-
ing other metals, by galvano-plastic means, with a more or less thick
coating of pure nickel. Since that metal is very hard, it resists,
even in thin layers, rather rough usage ; it is not oxidized, even in
contact with water, at the ordinary temperature, and the metal as-
1870.] Physics. 289
sumes a brilliant polish if required. The method employed for the
deposition of nickel was treated of at a meeting of the French Aca-
demy. The company alluded to have established a branch manu-
factory at Paris, under the management of M. Gaiffe.
M. Gaiffe calls attention to the fact that the presence of even the
smallest quantity of potassa, or soda, or alkaline earths in the bath
containing the nickelizing preparation is injurious to effect a pro-
perly-adhesive coating of the metal. The use of perfectly pure
double chloride of nickel and ammonium, or of perfectly pure sul-
phate of nickel and ammonium, and, moreover, of pure nickel as
one of the electrodes, is required. By these means the nickel is made |
to adhere regularly and strongly, and only requires polishing after
the metal, coated over, is taken from the bath. On the other hand,
M. Becquerel now states that he has purposely repeated some of
his former experiments, with the express view of ascertaining whether
the statement made by M. Gaiffe, concerning the injurious action of
the presence of potassa, be correct or not. The result of experi-
ments is that the presence of potassa is not at all injurious to, and in
no wise affects, the deposition of nickel, since the double sulphate of
nickel and potassa can be applied, as well as the double sulphate of
nickel and ammonia; but if the positive electrode is not made of
nickel, it is necessary to add free ammonia, in order to saturate the
sulphuric acid, which is set free.
M. Scoutetten states that the accidental striking of lightning on
the house of a vineyard proprietor caused the rupture of several
large hogsheads containing wine, which found its way into a cavity
existing in the cellar of the house. ‘The owner imagined his wine
lost and spoiled, but found, to his astonishment, that the wine, in-
stead of having been deteriorated, had become better than it was
before. This accidental occurrence having come to the knowledge of
General Marey-Mouge, caused M. Scoutetien to be consulted, and a
series of experiments instituted with various kinds of wine, of inferior
as well as medium quality. A series of experiments, made on the
large scale, and with various sources of electricity, led to the result
that electricity, under whatever form applied (whether as a regular
current, or a succession of discharges accompanied by sparks), im-
prove wine, rendering it mellow and mature. As to the mode of
action of this agent, the author thinks that the bitartrate of potassa
present in wine is decomposed, the potassa set free saturates the acids
of the wine, and the free tartaric acid, reacting upon the fatty matters
present, favours the formation of the ethers which constitute the
bouquet of the wine. Moreover a small quantity of water is decom-
posed, and the oxygen thereof reacts upon some of the constituents
of the wine, thereby forming new compounds which are peculiar to
old wines.
. 290 Chronicles of Science. [ April,
12. ZOOLOGY—ANIMAL PHYSIOLOGY AND
MORPHOLOGY.
PHysIoLoGy.
ftesearches on the Relation of Heat to Work in the Human Body.—
Professor Pettenkoffer, of Munich, has undertaken an investigation
into the amount of heat produced by the human body when at rest
and when at work, which promises to give highly important results.
The wonderful experimental chamber which King Max had con-
structed for Pettenkoffer’s work is to be made use of. The chamber,
which is about 10 feet square, is fitted with an iron tube through
which the air is regularly drawn by means of an aspirator worked
by a steam-engine, the air being accurately measured in a gas
meter. Smaller aspirators brmg measured quantities of the air
through analysis-tubes in which the quantities of carbonic acid, water,
hydrogen and carburetted hydrogens (the last two by combustion
with spongy platinum) are determined in the air both before and
after it enters the chamber. The small aspirators, bringing a small
but constant fraction of the whole air passed into the chamber
through the analysis apparatus, the quantities of carbonic acid gas,
water and hydrogen in the whole can be readily calculated. It is
now intended to take the temperature of the air before and after it
traverses the chamber, and in this manner to ascertain the actual
amount of heat produced by the human body when at rest and when
at work, and in relaticn to the amounts of the various excretions.
For this purpose a smaller chamber has been constructed within the
first made, and arrangements adapted by means of non-conductors,
&c., to prevent, as far as possible, the loss of heat. It is found that
there is a constant loss of about 40 per cent. of the total heat with
two candles burnt in the chamber ; of about 50 per cent. with four.
The heating effect upon the air passed through the apparatus is deter-
’ mined before each experiment with stearine candles of known weight,
and thus when a man is placed in the chamber instead of the candles,
you get his heating effect in terms of stearine candles, and this is,
of course, at once convertible into units of heat. The preliminary
experiments with candles promise very accurate and satisfactory
results from this method. As an apparatus for chemical analysis
the chamber is perfect ; so perfect that the percentage composition
of a candle can be determined as accurately by burning it in the
chamber, and the fractional analysis, as by the most complete direct
combustions. The determination of the heat produced is a matter
of more difficulty on account of the fluctuations of external tem-
perature and the delicacy of the thermometers which must be used ;
but Professor Pettenkoffer has used every precaution, and succeeded
in rendering the apparatus efficient. The experiments are now in
1870. } Zoology. 291
progress ; a man is to be kept in the chamber for six to eight hours,
and the work done is in the form of crank-turning.
The Absence of Currents in Uninjured Inactive Muscle.—Pro-
fessor Hermann states that if the gastrocnemius muscle of the frog
be so prepared for investigation that no contact between the cuta-
neous secretion and the surface of the muscle takes place, then, with
an exceedingly delicate galvanometer, only the very smallest deflec-
tion of the needle is obtained. He concludes, therefore, that by still
ereater care muscles can be obtained perfectly free from currents,
and regards previous observations of muscular currents as having a
very different significance to what has been supposed, being really |
artificial phenomena due to certain accidents of manipulation.
Pasteur’s Views on Fermentation.—Professor Liebig disputes
Pasteur’s theory that the decomposition of sugar in fermentation
depends on the development and multiplication of yeast-cells, and
that fermentation is only a phenomenon accompanying the vital
processes of the yeast. lLiebig considers that Pasteur’s researches
have not explained fermentation, but have only made known another
phenomenon—the development of yeast—which equally requires
explanation.
Physiology of Sepia.—A series of interesting experiments have
been made by M. Bert on this subject. He finds that the excision
of the large supra-cesophageal ganglion-mass causes no pain or
inconvenience to the animal, but simply deprives it of voluntary
motion. He hence infers it to be equivalent to the vertebrate cere-
brum. The contents of the salivary glands, as also of the liver and
pancreas (so-called), are acid. The peritoneal cceca excrete uric
acid. Strychnia and curare have the same effect on this animal as
on vertebrates.
MorpHoLoay.
Commensalism.—Professor Van Beneden, in an interesting ad-
dress to the Belgian Academy of Sciences, proposes this word to
distinguish a group of animals hitherto confused with what he would
term veritable parasites. _Commensal parasites, or commensals, do
not feed on the animal with which they are found, but by it: they
are not destructive or injurious to their hosts, but often are of ser-
vice, if we may judge from the constancy of association and the satis-
faction which both parties seem to enjoy. Professor Van Beneden
distinguishes fixed and free commensals. Among the fixed we may
mention the various barnacles which are attached to whales and sea-
turtles ; the Anemone parasitica, which invariably is fixed to a shell
inhabited by a particular species of Hermit-crab, said to exhibit great
affection for the polyp it bears on its back; many Polyzoa and Hy-
drozoa, which attach themselves to the carapaces of crustacea, espe-
cially the hairy-looking Dromia of our southern coasts.
292 Chronicles of Science. [ April,
Free commensals are the most numerous. Little fish live inside
jelly fishes, without incommoding their host, or being incommoded ;
a whole troop of a particular species may be thus sometimes seen.
Similarly a fish called Fierasfer lives inside a Holothurian, and in a
large species of Anemone the same observation has been made.
Dr. Semper has described, in addition to the little fish inhabiting
Holothurie, several molluscs, which also live in this way; whilst
Miller made known Entoconchon, from the Synapta; and Sty-
lifer lives on Hchinus. The Remora is a remarkable instance of
commensalism. This strange fish, by means of the sucker on the
back of its head, attaches itself to other fish and to whales, some-
times to ships, and is thus carried along through rich feeding-grounds.
The inhabitants of Mozambique use this fish as a means of captur-
ing others, tying a string to it and letting it out ito the sea, when
it attaches itself to some unsuspecting inhabitant of the ocean, which,
together with the Remora, is speedily dragged to shore. The little
crustacean (Pinnotheres), which lives inside the shell of the common
edible mussel, has long been known, and various species in this and
other countries have excited speculation and fable. There is no
doubt a most cordial understanding between the little crab and its
host ; and though we cannot go so far as to believe that the crusta-
-cean acts as a watchman for the Mytilus, warning it when to close
its shell, it 1s yet very evident that there is a close relationship of
reciprocal advantage existing between the two. Chztogaster, the
little worm which crawls about on Lymnezus and Planorbis—the
common water-snails of our ponds—is a good example of a com-
mensal, sticking very close to his friend, feeding on the Cercariz
(true parasites) and other matters which accumulate on the snail’s
body. Many tubicolous Annelids have a commensal, or messmate,
~ who shares their residence; such are many scale-bearmg Annelids
—the Polyndina, which ensconce themselves in the tubes of Che-
topterus insignis, of Terebella nebulosa, and others. One Polynde
was many years since described by Professor Huxley as living on
the common Cross-star, and hence named P. astericola.
The distinction between commensal and parasite is this, that
the parasite uses his host for food; whilst the animals which are men-
tioned above, and many others enumerated by Professor Van Bene-
den, though often termed parasitic, do not feed upon the tissues
of the animal with which they live, and hence have a very different
relation to them. ‘Their food consists often of what is rejected by,
or is even hurtful to, their hosts; and though the line between them
and true parasites may not be easy to draw sharply, it is yet useful
to recognize them under a distinct name, as proposed by Professor
Van Beneden.
A New Genus of Cervide.—Mr. R. Swinhoe, who, as consul at
Formosa and various stations on the Chinese coast, has done most
1870. | Zoology. 293
active and important work in the investigation of the fauna of that
part of Asia, described recently to the Zoological Society of London,
a new form of deer, common on the islands at the lower part of the
river Yangtse-Kiang, near Ching-Kuang, into the markets of which
city it is often brought, though it appears hitherto to have escaped
the observation of naturalists. This deer is distinguished by the
long canines and the total absence of horns in both sexes. Mr.
Swinhoe proposes to form a new genus for the reception of this
remarkable form, and gives it the name Hydropotes imermis.
Animals presenting two distinct Sexual Forms.— From the
time when the so-called alternation of generations became known
to zoologists, they have been familiar with various species of lower
animals which reproduce sexually under one form, and a-sexually
under a totally different form, the form presenting agamic repro-
duction being often so different from that in which sexual maturity
is ultimately attained, that at one time the two phases of the species
have been referred even to different classes of the animal kingdom.
The a-sexual Aphides, whose offsprmg become male and female
adults ; the Cecidomyia larvee, producing a-sexually larvee like them-
selves, which become eventually sexually mature flies; the various
Entozoa and the Annelids of the family Syllide, which reproduce
rapidly by fission, whilst at certain times individuals endowed with
sexual organs, and differing most markedly in their sete and other
characteristics are produced,—are familiar instances. Lately, by the
researches of Leuckart, Mecznikow, and Schneider, we have been
made acquainted with a nematoid worm parasitic in the frog, which
presents the remarkable condition, previously unparalleled in science,
of two sexual forms: the first, in which there are distinct males and
females, is a free living form; the second, to which the eggs of this
bisexual generation give rise, is hermaphrodite, but at the same
time truly sexual in its reproduction, according to M. Schneider, in
which it differs from all previously recorded cases of alternation of
generations. M. Claus asserts the same of the Nematoid, Leptodera
appendiculata; and the Acaleph Carmarzina has since been described
as presenting the same condition of things. M. Claparede, of Geneva,
amongst his other discoveries in the Bay of Naples, has brought to
hight a most interesting case among the highest Annelids of an
animal presenting two distinct sexual generations. The Nereis
Dumerilii is the worm to which these observations refer. For some
time this species has been a puzzle to zoologists, and M. Malmgren
had already detected its relation to Heteronereis; but the problem
has been fully investigated by M. Claparede. He finds that there
are absolutely two forms of sexually mature HHeteronereis (each
having its own males and females, as im nearly all Polychetous
Annelids): one small and very agile, swimming on the surface of
the sea, and thus widely dispersing its reproductive elements; the
VOL. VII. x
294 Chronicles of Scrence. [ April,
other much larger, but less agile, which never leaves the sea-bottom,
and fitted rather to reproduce the species in a fixed locality. The
egos of the two forms of Heteronereis are not at all similar; but the
zoosperms are identical in the two. This, however, is not the most
remarkable part of the case; for it appears that these two forms of
Heteronereis are neither more nor less than developed forms of the
Nereis Dumeriliz, which has also a sexual condition (consisting of
both males and females) as a Nereis. We have in the Nereis
Dumeriluv, according to M. Claparede, a worm which is adult both
as Nereis and Heteronereis, and has probably two Heteronereidan
forms. An important question is whether a worm which has arrived
at sexual maturity as a Nerezs can lose ugain its sexual characters,
and become a Heteronereis; or whether we must consider that a
worm once arrived at maturity as a Nereis can never itself become a
Heteronereid, but only the worms which it produces are destined for
this condition. The question is one of importance, which must be
solved by study of worms kept in the aquarium. Undoubtedly we
have here one of the most astonishing cases of protean diversity of
specific form ever brought before naturalists—of a kind, indeed, totally
unexpected. The history of the Axolotl (chronicled by us some time
since) presents a sort of parallel to this case ; but it may prove that
the resemblance is not so close as we might at present suppose.
M. Dumeril has shown that the Amphibian Axolotl of Mexico
reproduces when in its larval condition with perennial gills, as known
in the tropical region of Central America; and also that in colder
regions losing these gills, it assumes the more perfect Salamandroid
form, and is reproductively active in that condition. The perenni-
branchiate condition may be compared to the Nereis-form, the Sala-
mandroid to the Heteronereis; but it is to be observed that the dif
ferences are much greater in the case of the two forms of the worm
than in the Amphibian: also we have no parallel to the second He-
teronereis form of the Nereis Dumerili, which, by the way, is well
named @ propos of the distinguished herpetologist who has made
known the sexual peculiarities of Szvedon.
Miscellaneous.—The eminent comparative anatomist Professor
Keferstein, of Gottingen, has died at the early age of thirty-seven.
He was an active worker, from whom much in bibliological science
had been already gained, and from whom much was to be expected.
The Sars Fund.—A subscription has been started for the family
ot the eminent Scandinavian zoologist, Michael Sars, whose death
occurred last year. Whoever knows anything of marine zoology
knows of the work of Sars and of his eminent son, G. O. Sars. In
France and Germany the subscription is progressing, and in this
country Mr. J. Gwyn Jefireys has undertaken to receive contribu-
tions. We shall be glad to hear that the appeal to English savans
has been successful.
Quarterly List of Publications receibed for Webtetw.
1, On Comparative Longevity in Man and the Lower Animals. By
RK. Ray Lankester, B.A. Macmillun & Co.
2. Reports on the Progress of Practical and Scientific Medicine in
different parts of the World. Edited by Horace Dobell, M.D.,
Senior Physician to the Royal Hospital for Diseases of the
Chest. Longmans, Green, & Co.
8. Geology and Revelation; or, The Ancient History of the Earth
considered in the Light of Geological Facts and Revealed
Religion. By the Rev. Gerald Molloy, D.D., Professor of Theo-
logy in the Royal College of St. Patrick, Maynooth.
5 Longmans, Green, & Co.
4, Our Domestic Fire-places. New Edition, entirely re-written and
enlarged. By Frederick Edwards, jun. Longmans, Green, & Co.
5. Discussion of the Meteorological and Magnetical Observations
made at the Flagstaff Observatory, Melbourne, during the years
1858-1863. By George Neumayer, Ph.D., late Director of the
Flagstaff Observatory, &e. Mannheim: J. Schneider.
6. Education and Training, considered as a subject for State Legis-
lation. By a Physician. J. Churchill & Sons.
7. Reliquiz Aquitanice ; being Contributions to the Archeology and
Paleontology of Périgord, &c. By H. Lartet and H. Christie.
HKdited by T. Rupert Jones, &., &e. H. Bailliere.
8. Statistics of New Zealand for 1868. Printed by order of the New
Zealand Government. Wellington: G. Didsbury.
9. The Philosophy of the Bath, with a History of Hydro-therapeutics
and of the Hot-air Bath from the Harliest Ages. By Durham
Dunlop, M.R.LA. Dublin: Moffat & Co.
10. Christianum Organum ; or, the Inductive Method in Scripture and
Science. By Joseph Miller, M.A. Introduction by J. H.
Gladstone, Ph.D., F.R.S. Longmans, Green, & Co.
11. Choice and Chance. By Rev. W. A. Whitworth, M.A., Fellow of
St. John’s College, Cambridge.
Cambridge : Deighton, Bell, & Co.
12. Preliminary Field Report of the U.S. Geological Survey of
Colorado and New Mexico. By F. V. Hayden, U.S. Geologist.
Washington: Government Printing Office.
13. Geological Report of the Exploration of the Yellowstone and
Missouri Rivers. By the same Author.
VOR. VIE Y
296 List of Publications [ April,
_ 14. The Book of Nature and the Book of Man. By Charles O. G.
Napier, of Merchiston, F.G.S., &c. Illustrated with photo-
graphs and numerous woodcuts. J. Camden Hotten.
PAMPHLETS AND PERIODICALS.
Memoirs of the Geological Survey of India, published under the
Direction of Thomas Oldham, LL.D., &e. Calcutta.
Report on the Filtration of the Water of the Hooghly. By David
Waldie, F.C.S.
Analysis of the Khettree Meteorite, with an Account of its Fall.
Same Author.
Reports of the Mining Surveyors and Registrars of Victoria.
Melbourne: John Ferres.
On the Geographical Distribution and Physical Characteristics of
the Coal-fields of the North Pacific Coast. By Robert Brown,
F.R.G.S., Commander and Government Agent of the first Van-
couver Exploring Expedition, &c., &e. Edinburgh: Neill & Co.
Observations on the Chalchihuitl of Mexico and Central America.
By E. G. Squier, M.A., &e., &e. New York.
Dr. Walter’s Doctrines of Life. Reply to London ‘Lancet.’ (From
‘St. Louis Medical and Surgical Journal.’)
A Physical Theory of Animal Life. A Review by Julian.
On the Identity of the Vital and Cosmical Principle. By R. Lewins,
M.D.
The Nature of Man Identical with that of other Animals. By Julian.
On Colour Tests as Aids to Diagnosis. By John Day, M.D. From
the ‘ Australian Medical Journal
Report of the Committee for the Purpose of Investigating the Rate of
Increase of Underground Temperature Downwards, in various
Localities, of Dry Land and under Water. Professor Everett,
D.C.L., F.R.S.E., Secretary. _
An Investigation into some previously undescribed Tetanic Symptoms
produced by Atropia in Cold-blooded Animals, with a Comparison
of the Action of Atropia on Cold-blooded Animals and Mammalia.
By T. R. Fraser, M.D. Edinburgh: Neill & Co.
Midland Steam-Boiler Inspection and Insurance Co.’s Report.
Annual Report of the Secretary of the Interior for 1869.
Washington.
Notes on Books (Quarterly List and Analysis). Longmans.
Microscopic Objects Figured and Described. No. 1, January, 1870.
By J. H. Martin, Seowlary, Maidstone and Mid. Kent Natural
History Society. Van Voorst,
1870.] received for Review. 297
The Food Journal; a Review of Social and Sanitary Economy and
Monthly Records of Food and Public Health.
London: J. M. Johnson & Sons, 3, Castle Court, Holborn.
Revue Bibliographique Universelle. Paris: 77, Rue de Bac.
The American Naturalist. Peabody Academy of Science. Salem, Mass.
Scientific Opinion.
The Geological Magazine.
The Photographer’s Annual and Almanac for 1870.
J. W. Green, 54, Paternoster Row.
PROCEEDINGS OF LEARNED SOCIETIES, &c.
Proceedings and Papers of the Kilkenny and South-East of Ireland
Archeological Society. Dublin: McGlashan & Gull.
Transactions of the Edinburgh Geological Society.
Edinburgh: Neill & Co,
Proceedings of the Literary and Philosophical Society of Liverpool.
(1868-9.) London: Longmans.
Proceedings of the Manchester Literary and Philosophical Society.
( Extract.)
Proceedings of the Royal Institution of Great Britain.
» Royal Society.
Monthly Notices of the Royal Astronomical Society.
NOTICE TO AUTHORS.
* * Authors of OrtainaL Paprrs wishing Reprints for private
circulation may have them on application to the Printers of the
Journal, Messrs. W. Crowszs & Sons, 14,.Caarine Cross, 8.W.,
at a fixed charge of 30s. per sheet per 100 copies, including a
CoLoureD Wrapper and Tirtz Paasz, but such Reprints will
not be delivered to Contributors till ONE Montu after publication
of the Number containing their Paper, and the Reprints must be
ordered before the expiration of that period.
ek
‘~ he
‘JueLy,-mo-u0ojIng ‘Aromerg smog » ddostly ‘sassepy ye Arouuny,
PiLaTE. —QUARTERLY JOURNAL OF SCIENCE, No. xxvii.
SS
THE QUARTERLY
JOURNAL OF SCIENCE.
JULY, 1870.
I. BEER, SCIENTIFICALLY AND SOCIALLY
CONSIDERED.
By James Samuetson, Editor.
Dourine a visit which I paid last year to Germany, the Tyrol, and
Switzerland, I was greatly struck with the fact that in countries
where beer is the national beverage, the humbler classes are com-
paratively sober; whilst in those parts where wine, even the thin
wine of the country, and ardent spirits usurp the place of the milder
beverage, there is a nearer approximation to the habits of our own
people—in other words, there is a large amount of drunkenness.
In publishing elsewhere a short account of my observations,* I
ventured to express the opinion that the man who should succeed
in introducing into Britain and bringing into general consumption
a mild, brisk, sparkling beverage such as one gets abroad, would be
a greater benefactor to his people than the most self-denying devoted
advocate of teetotalism, and some of the most influential organs in
the country, and notably three, have more or less emphatically
endorsed this view in their criticisms. What is still more satisfac-
tory, I have received inquiries concerning the difference between
the processes of manufacture of the English and German beer, from
persons who haye the will and ability to carry out my suggestion,
whilst German beer is daily more sought after, and in our large
towns, such as London, Manchester, and Liverpool, it may readily
be procured, though the cost is rather high owing to the limited
consumption. Instead, therefore, of having over-estimated the im-
portance of the beer question, I find that it is far more deserving of
consideration than I had imagined, and after having directed my
attention to it, and inquired further into its scientific and social
aspects, I have arrived at the conclusion that there are few subjects
of greater national importance to us as Englishmen, |
One of the journals to which reference has been made,t has gone
so far as to say that “wholesome beer and wholesome recreation
* ‘The German Working Man.’ Longmans.
+ ‘The Illustrated London News,’ January 1; ‘The Pall Mall Gazette,’
January 8; ‘ The Gardener’s Chronicle,’ March 19.
{ ‘The Pall Mall Gazette.’
WOOL. “Vek. x
300 Beer, Scientifically and Socially Considered. [July,
are, for the most part, beyond the reach of our working men ;” and
although much of the blame rests with the operatives themselves,
who prefer to give 6d. per quart for bad beer at a public-house,
rather than the same price for the finest Burton ale, which they
could easily procure by combination, yet it is perfectly true that a
large proportion of the beer now sold to the masses is totally unfit
for consumption. If any of my readers are disposed to doubt this,
let them read the following paragraph which I have extracted from
the proceedings of the Liverpool Select Vestry, as reported in the
Liverpool ‘ Daily Post’ of January last :—
“POISONOUS BEER AND LUNACY: A BREWERS TESTIMONY.”
“A conversation as to the cost of pauper lunatics arose, and
Mr. Glover, addressing the committee, said he thought that, with
regard to lunacy, they began at the wrong end. He had visited
the lunatic asylums in Lancashire within the last three or four
months, and he had asked the masters of the institutions what was
the cause of the increase in pauper lunatics? The answer was
drunkenness, and he (Mr. Glover) believed that that was the case.
He thought the health committee ought to be asked to appoint
some sort of an inspector to look after the quality of the drink sold.
They appointed inspectors of meat and fish, and they condemned
bad fruit, but bad drink was ten times worse than all of them.
There was a law which, if put in force, punished people for using
poisonous ingredients in the making of beer—preventing them from
using grains of paradise, nux-vomica, oil of vitriol, ammonia, and
other things that were used in making beer. ‘That was in addition
to malt and hops, but if only malt and hops were used there would
be no lunatics from drink. His impression was that all a working
man could spend in honestly brewed beer would not kill him or
- drive him mad, if the beer were good. There were some dishonest
publicans as well as dishonest brewers; and there were some pub-
licans who rode handsome chargers, and their wives were driven
about in splendid equipages, and they were doing great injury to
people and filling the workhouses. He believed the drink they
sold was not honest drink, but contained some of the things he had
described. When a brewer had beer that would not keep long, he
said to his customer, when it got a little sour, that he would change
it. It was taken back to the brewery when sour, and then the dis-
honest publican bought it for 10s. or 1/. a barrel. He then
went to the druggist’s shop, and got something that neutralized
the acid; and, was not the poor creature who afterwards drank
the beer likely to go mad? Ifa man had a pint or two of good
honest beer, he would never go mad. The health committee ought
to attend to the matter, and see that good beer was given to the
people.”
1870. ] Beer, Scientifically and Socially Considered. 301
We shall presently have an opportunity to consider scientifically
the character of those precious ingredients, grains of paradise,
cocculus indicus, and other substances not mentioned by the candid
brewer whose remarks I have just quoted, with which the poor
man’s beer is drugged; but before doing so, I propose to give a
short account of the materials which ought to be used in the
production of wholesome beer, of the scientific principles involved
in the art of brewing, and of the most approved methods adopted
at respectable breweries at home and abroad.
It would oceupy too much space to enter fully into the history |
of beer, but it may interest some of my readers to know that its use
is well authenticated in the days of ancient Rome, and according to
Tacitus, the old Teutons had already acquired that taste for “ Lager,”
which has been transmitted to their descendants in our time, for
that author mentions it as their common drink. Pliny, too, states
that it was consumed in Spain and Gaul, and that it was made from
various kinds of grain, whilst a recent writer on the history of
Burton-on-Trent,* tells us that the brewing of ale in that town is
unquestionably coeval with the Abbey, it being a beverage of much
repute with the Saxons, so that there can be little doubt of its
having been drunk all over Europe in very early times. Mr. Moly-
neux, the author referred to, tells us, however, that the brewing
trade of Burton-on-Trent is comparatively recent, and the credit of
haying originated it is accorded to one Benjamin Printon who lived
in the early part of the last century, whilst at the close of that
century there seem to have been only nine brewers in Burton,
amongst whom appear the names of Bass and Worthington, but
not yet that of Allsopp, whose ancestor, Mr. Benjamin Wilson, was
however doing a large business in 1748. Such of my readers as
are curious on these matters, will do well to peruse Mr. Molyneux’s -
interesting little treatise, where they will also find a variety of in-
formation concerning the geology, &c., of the Burton district: but
we must now proceed to consider the materials which enter into the
manufacture of beer.
Those are, or should be, water, malt (barley), hops, and yeast,
and these substances possess not only a practical value for the
brewer, but many special points of interest for the chemist and the
student of botany. There has long been, to the uninitiated, a
mystery connected with the water of Burton-on-Trent, the prevalent
notion being that it is the river water which possesses some special
virtue for brewing purposes. The fact is, however, that it is the
spring-water of the district which is so well adapted for the manu-
facture of beer, and, although the effect is not yet clearly understood,
* “Burton-on-Trent ; its History, its Waters, and its Breweries.’ By William
Molyneux, F.G.S. Triibner and Co,
+ ‘Burton and its Bitter Beer.” By Dr. Bushnan. W. 8. Orr and Co.
a 2
302 Beer, Scientifically and Socially Considered. [ July,
the cause has long been well known to chemists. It arises from the
presence in the water of “earthy sulphates and carbonates,’ and
the absence of organic matter which is fatal to the brewing process.
Analysis has shown the Burton water to contain nearly 19 grains
of sulphate and 15 grains of carbonate of lime to the imperial
gallon (besides sulphates of potassa and magnesia), and the theory is
that these alkalies combine with the acid of the malt extract, and,
in the form of insoluble salts, are precipitated and carry down with
them the nitrogenous substances which it is desirable to get rid of
in the brewing process; so, for the same reason that the presence of
salts of lime and potash in the Burton water is advantageous, that
of organic matter would be injurious, and the freedom of the water
from the latter is therefore very advantageous to the brewer.
Should any of my readers desire further information on this subject
for practical purposes, they may obtain it in the able article on
“ Beer,” in Dr. Muspratt’s ‘ Dictionary of Chemistry,’ or in those on
the same subject in Ure’s ‘ Dictionary of Arts,’ and Watts’s ‘ Dic-
tionary of Chemistry ;’ while Mr. Molyneux’s work, already named,
also contains an excellent chapter on the “ Waters of Burton,” and
the effect upon them of the strata through which they percolate.
Malt, as every one knows, is barley steeped and dried. There
are various kinds of malt, known as pale, amber, brown, and black,
of which the first-named is employed in brewing pale ale, and the
last (which is roasted like coffee) is used for colouring porter.
Barley undergoes two kinds of change during its conversion into
malt, the one morphological, that is to say, in its plant life, the
other chemical. In order to effect the conversion it is steeped for
two or three days in water, then spread out upon a floor to germi-
nate, and when it has sprouted to a certain
length it is taken to the kiln to dry, and in the
subsequent handling “the radicles” which have
shot forth during germination, are broken off
and the grain assumes to a great extent its
original appearance. The annexed woodcuts
will render the morphological change appa-
rent to the eye; Fig. 1 being a grain of barley
with the husk removed to show the embryo;
Figs. 2 and 3 the same after germination.*
But a chemical change, not so easily understood, also takes
place in the malting process, and I will endeavour in a few sentences
to make it as clear as possible. For our purposes, the barley may
* These woodcuts, and some others in this article, have been copied, with the
permission of the publishers, from the plates in a beautiful and interesting volume
‘On Strong Drink and Tobacco Smoke, by the late H. P. Prescott, F.L.S., just
published by Messrs. Macmillan and Co. Frequent references will be made to this
work. Mr. Prescott died recently of consumption, and his book has been passed
through the press, and edited, with much good feeling, by Professor Huxley.
1870. | Beer, Scientifically and Socially Considered. 303
be said to be composed of two main constituents, albumen and starch,
and during the germinating process the albumen is converted into
a new substance, diastase, so called from its property of being able
to split up the other constituent of the grain, starch, into dextrin
or gum, and sugar. The object of this chemical change in nature
is to supply the embryo of the plant with a soluble pabulum or
nutriment; but as in malting the germination is arrested at an
early stage, the starch is converted into soluble gum and sugar,
merely to be extracted in the mashing process which follows at the
brewery. The result of this extraction is to produce the “ worts,”
or “ wort,” the stock, so to speak, of the beer.
The morphological changes which take place in the growth of
the barley, either during germination or subsequently, are deeply
interesting, and an illustrated account of them will be found in
Mr. Prescott’s work referred to, whilst a detailed description of
the chemical changes to which the grain is subject is contained in
the various articles on “ Beer” (more especially Dr. Muspratt’s) in
the Dictionaries already quoted. ‘These are, however, beside our
purpose, and we must now pass on to the other materials used in
brewing, namely, hops and yeast, both of which are as interesting
as malt to the chemist and botanist.
The hop-plant belongs to the same botanical group as the stinging
nettle (Urticacez) and is cultivated chiefly in the counties of Kent,
Sussex, Surrey, Worcester, and Hereford, and also imported from
the Continent. The bitter principle which it contains, and which is
extracted in the boiling process of the brewer, is called “ lwpulzte,”
and it is found in the fruit, which is so well known as hardly to need
description. or the guidance of my readers, however, I will extract
a short account of it from Mr. Prescott’s work, accompanied by such
of the figures as seem essential :—
“The fruit of the plant,” he says on p. 40, “(technically called
strobilz), which is so largely used in brewing, consists of a series of
delicate green, semi-transparent bracts, attached to a common stalk
(Fig. 4) and overlapping at their edges in a very elegant manner.
The seeds are minute, flattened, conical berries of a light-brown
colour; they are attached to the bases of the bracts (Fig. 5) which
fold over at their lower edges to afford them additional support,
and each inner seed-containing bract is covered by another exter-
nally. Attached to the outer seed-coat is a beautiful transparent
membrane, and on this lie, in countless numbers, minute golden-
coloured oval bodies which are the lupulite so valuable to the
brewer (Fig. 6). These granules are abundant on the bracts, espe-
eially at their bases, where the seed is lodged ; they are also present.
in large quantities on the leaves of the plant. When one of these
granules is placed in water under the microscope, and a drop of
sulphuric or nitric acid is added, it immediately bursts, and the
304 Beer, Scientifically and Socially Considered. (July,
coloured matter discharged is seen to consist of excessively minute,
somewhat spherical, particles of an oily nature, that move freely and
Fie. 4. Fic. 6. Pic. 5.
with great rapidity amongst each other with a tremulous motion.
This peculiar motion may at times be observed in the contents of the
granules before they are broken.” *** “A common practice
amongst hop-buyers is to take a small quantity of the dried hop-
fruit, place it m the palm of one hand, and with three or four
knuckles of the other, to chafe and bruise it. The value of the
sample is judged of by the aroma it emits and the sticky almost
resinous stains left upon the hand. This is a rough but effective
way of judging both of the number and produce of the lupulite
granules by crushing them. Good sound hops will yield about
one-sixth part of their weight of these grains. Analyzed by the
chemist they are found to contain, besides a volatile oil, no fewer
than thirteen substances, more or less in combination with each
other. But it would appear that to the volatile oil, soluble in water
and alcohol, and the bitter principle, /wpulite, the most valuable
properties of the fruit are due.”
T have made this somewhat lengthy extract from Mr. Prescott’s
book for a twofold reason ; first, because it conveys in brief and clear
terms all that is interesting to us, in this portion of the subject, and
secondly, because I consider that his powers of observation and his
practical researches deserve to be prominently noticed. In another
part of his book he tells us that he examined the spent hops of
breweries and found that not more than one-half their lupulite is
made available, a circumstance which shows how necessary it is to
call into requisition, more largely, the services of scientific men, even
in our most commonplace manufacturing processes. =
1870. | Beer, Scientifically and Socially Considered. 305
Yeast is a lowly unicellar plant called Torula cerevisiw. The
growth of its cells (which on examination with the microscope are
found to contain minute nuclei) has been ably described * by an
eminent botanist (Dr. Henfry), who obtained some fresh wort in
which fermentation had commenced and placed a drop of the liquid
under the microscope. At first, he says, these globules enlarged
until they attained a certain size, and then they remained unchanged
for a time. Next, a little point-like bud was seen to project from
one portion of the cell-wall, and this grew until it attamed the same
size as the parent cell. This occupied about three hours, and by a
repetition of the process sixteen cells were developed from a single ~
one. After a time the growth slackened and at length it ceased, the
observer believed, “ undoubtedly because all was removed from the
liquid which could serve for
their growth.” The following Fig. 7.
woodeuts represent the micro-
scopical appearance of the cells
of the yeast fungus, Fig.7 being ,
. that found at the bottom, and
Fig. 8 a “white mealy sub-
stance,’ at the top of the liquid ;
the growing globules will be seen in the former, from which my
microscopical readers will perceive that the plant multiplies by the
well-known but incomplete process of fission.
These, then, are the materials which should be employed in the
brewing of good ale. Water, free from organic matter and con-
taining sulphate and carbonate of lime ; barley, in the form of malt ;
hops, and yeast ; and although the reader will have gathered from
the preceding short account of these substances, what leading prin-
ciples are involved in their use and treatment, I propose briefly to
recapitulate the changes which occur in the brewing process, before
attempting to describe the practical operation. In the malting or
germination of the barley the albumen in the grain becomes con-
verted into diastase, the property of which is to change the starch
(also constituent in the barley) into soluble dextrin or gum, and
sugar, and consequently the malt possesses a sweet taste which is
not present in the grain previous to malting. In the mashing
process, this sweet substance is washed out of the malt, and with
the water employed for the purpose goes to form the “wort,” or
stock of the beer. This “wort” is subsequently boiled with hops,
which contain a bitter principle, /wpulite, and an essential oil, of
which the effect is to impart a bitter aromatic flavour to the beer,
at the same time as the chief organic constituents of the wort are
removed. And finally through the introduction of yeast, a minute
* «Micrographic Dictionary’ (article “ Yeast-Plant”), from which, with the
publisher’s permission, the woodcuts are copied.
306 Beer, Scientifically and Socially Considered. [ July,
plant, the cells of which multiply with incredible rapidity, fermen-
tation 1s set up, the chemical effect of which is to convert the sugar
contained in the “ wort,” into carbonic acid and alcohol. ,
The brewer takes care, however, to stop the fermentation at a
certain stage, so that a portion of the sugar may remain uncon-
verted, and the chemical change is then completed in the cask or
bottle, the carbonic acid being held in solution until the beer is drawn
or otherwise exposed to atmospheric action. This gives to good beer
its brisk sparkling appearance and puts a head upon it: in no case
is the effect so conspicuous as in the bottled German beer and Eng-
lish and Scotch pale ales, which continue to effervesce and sparkle
like champagne, long after the liquid is poured into a tumbler.
Passing now from the theory to the practice of brewing, I pro-
pose to conduct my readers through some portions of the magnifi-
cent establishment of Messrs. Allsopp and Sons, of Burton-on-Trent,
where all that science and skill can accomplish has been done to
perfect the process. Let us commence with the malting; and the
reader must imagine himself m a large chamber (one of several
devoted to this purpose), one end of which is partitioned off for the
steeping process. ‘This side of the room, which forms an elongated
trough, is divided into squares, and partly floored with a number
of perforated tiles, which serve to drain off the water; and when
the barley is sufficiently steeped, it is turned out upon the chamber
floor, close to the trough. Here it is kept within certain limits, by
means of a removable partition consisting of boards, which can be
fixed between the columns that run across the chamber parallel to
the steeping-trough, or removed at pleasure; and the barley is then
said to be in the “couch,” where it is gauged by the Excise. After
gauging, the partitions are removed and the steeped barley is spread
evenly over the chamber floor to germinate: the germination haying
reached the proper stage (as already described), it is conveyed to
the kiln to dry. But at Allsopps’ the transfer of the barley from
the germinating floor to the kiln is only the passage from one chamber
to another immediately adjoining ; and unless his attention is directed
to the floor, the uninitiated visitor would observe nothing in this second
chamber to denote its function. The floor is paved with perforated
tiles, and in the kiln pit underneath, which is the same size as the
upper chamber, there stand a series of open furnaces, or gigantic
braziers, in which coke fires are lighted when the kiln isin use. Over
the fires there is a contrivance called a disperser, by which the heat
rising from these furnaces is equalized over the whole surface; and
when the spectator looks up at this disperser, he percetves plainly
the perforations in the tiles of the kiln floor above, and which
allow the heat to penetrate to the malt. After kiln-drying, the
barley, or as it is then called, malt, is subjected to one more process,
namely, screening. This consists in allowing it to run over an ob-
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lique screen, and during its passage the malt dust and radicles are
removed. ‘These make an excellent food for cattle, varying in value
from 51. to 7/. per ton, according to the requirements of the season.
This completes the malting process; and now we pass on to the
brewing, which commences with the grinding of the malt. By
means of a “Jacob’s ladder,” it is conveyed to an upper story, and
there allowed to fall into a hopper, which feeds a pair of smooth
rollers, very similar to those used im an oil mill for rolling linseed.
Being thus split, and partially ground, it is carried along the chamber
floor by means of an Archimedian screw, and passed through a hole
in the floor into a large hopper in the story below. This hopper is
fixed above the “mash-tun,” or ‘ mash-tub,” where the ground malt
is mixed with water at a temperature of 170° to 180°, and undergoes
the mashing process. The room in which we are now supposed to
stand contains eight such tubs, each capable of treating fifty quarters
of malt, and two of them are shown in Plate II., the one closed and
the other open. I was, unfortunately, unable to obtain a sketch,
which would fully illustrate the mashing process, but will endeavour
to make it as clear as possible with the means at my command.*
The mash-tun has a false bottom, composed of radiating sections,
the object of this being to take them out to clean after each mashing.
Then there revolve in the tub two kinds of apparatus, the one for
“mashing,” the other for “sparging,” to be explained presently.
An upright spindle revolves in the centre of the tun; and rotating
with it, is a strong horizontal wooden pole, having one end affixed
to the central spindle, and the other end, to which a cog-wheel is at-
tached, resting upon rack-work that runs completely round the inside
of the tun. The arrangement will be better understood if the reader
pictures to himself one of those “ roundabouts,” on which children ride
at fairs, with the horizontal pole resting on rack-work, which is visible
in the plate. Along the rotating horizontal pole there are placed
several beaters, somewhat resembling the rakes upon a reaping ma-
chine, but armed with teeth on either side. I have sketched (Fig. 9)
one of these beaters with a portion of the horizontal pole, and by a
suitable mechanism the beaters are made to revolve vertically in the
* All the page plates are copied from photographs kindly lent me by the
Messrs. Allsopp.
308 Beer, Scientifically and Socially Considered. | July,
mash, whilst the pole to which they are attached rotates horizontally,
so that the whole contents of the tun are thoroughly beaten and mixed.
This operation has really a very novel and interesting appearance
to one who has never witnessed it before. As the observer stands
looking into one of the openings in the mash-tun, nothing appears to
be going on in the mash so long as the beaters are on the side opposite
to him, but presently a slight undulation of the surface announces
their approach. Slowly the pole, with its beaters, moves round
towards the side where the spectator stands ; the undulations become
more marked, until at length the revolving arms make their appear-
ance, breaking up the surface and creating a great commotion. After
the round is completed, the apparatus is stopped, and the mash is
left undisturbed for some time, the process being repeated at regular
intervals. But there is another rotating apparatus of a very simple
kind attached to the central spindle, and that resembles in appearance
and action the horizontal discharge-pipe at the back of a watering
cart. It is in fact a copper pipe, of a suitable shape, with holes
drilled along its whole length, and may be seen on looking through
one of the openings in the mash-tun (see Plate II.). After the
strongest portion of the “ wort ” is obtamed from the malt by the
mashing process already described, it is dosed with a shower of hot
water, poured upon it from this rotating pipe, which is called the
“ sparge,” the operation being termed “sparging.” At the bottom
of each mash-tun there are four pipes through which the wort is
drawn off, and these pipes lead into a main which conducts the
liquid into the “ underback,” an intermediate vessel between the mash-
tun and the boiling copper, where, as the name indicates, the process
of botling with hops is carried on.
The boiler is an open copper cauldron or kettle, set in brick, and
heated from beneath. It has a capacity of about seventy barrels;
and when the requisite quantity of hops is deposited in it, the wort
is admitted through a pipe connected with the “underback,” into
which the liquor has been run from the mash-tun, as already de-
scribed. The feed-pipe bends over the opening of the copper, whilst
at the bottom of the same vessel is another pipe, through which,
when the boiling is complete (and the liquor is well stirred during
the process), the boiled wort, or unfermented beer, is run off into the
“hop-backs.” These, again, are intermediate vessels, square wooden
cisterns, with false bottoms, which act as a sieve, and the object of
running the liquor into them is to free it from the spent hops with
which it is accompanied, before cooling and fermentation.
A word concerning the spent hops. After the liquor has been
allowed to drain from them in the hop-backs, they are placed in
hydraulic presses to extract any wort that may still remain in them,
and are then packed and sold as manure.
From the “hop-backs” the wort runs into the refrigerators.
PuaTE IT].—QUARTERLY JOURNAL OF Scrence, No. xxvii.
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1870. | Beer, Scientifically and Socially Considered. 309
of which there are two or three descriptions, some of them occupy-
ing the floors of enormous chambers, which are moreover open to
the external atmosphere through the peculiar construction of the
windows. ‘The principle of these refrigerators is, however, always
the same, the hot wort being allowed to flow over a series of tubes
through which cold water freely circulates. Sometimes the tubes
form a spiral coil, at others they run in parallel rows, covering the
entire floor of the chamber, but in every case they slope in an inclined
plane, so that when the wort is poured on at the higher end it flows
down slowly to the lower, becoming cooled in its passage. In
winter the cold air, which is admitted on all sides into the cooling |
chamber, suffices to reduce the temperature of the wort in its passage
down the inclined plane, but in summer it is necessary that the
water which flows through the pipes should be made as cold as
possible ; and at Messrs. Allsopp’s, water is cooled on a large scale
for this purpose by the evaporation of ether. This is done out-
side of the main building, and the water thus cooled is con-
ducted all over the brewery, not only into the wort-refrigerators,
but wherever a low temperature is found requisite in the brewing
process.
From the coolers the wort is next conveyed into the “fermenting
rounds,” capacious vessels, each holding from 15 to 90 barrels, and an
idea may be formed of the magnitude of the operations carried on at
Allsopps’, when it is mentioned that the new brewery (there are two)
has two fermenting rooms, each containing 136 such vessels, conse-
quently above 4000 barrels. of beer may be fermented at one time.
Plate III. represents a portion of one of these fermenting chambers.
The principle involved in fermentation has already been described, as
the conversion of the saccharme matter in the wort into carbonic
acid and alcohol. As my readers are no doubt well aware, it is
effected by adding to the wort a quantity of fresh yeast from a pre-
vious brewing, and such an amount of carbonic acid gas is generated
that the invisible gas occupies the whole space between the surface
of the fermenting liquor and the rim of the vessel. A very curious
effect shown to visitors is to pass a hat through the apparently
empty space over the liquor in the fermenting vessel. This hat at
once fills with the invisible gas, which may then be poured into
another belonging to a visitor, just as we see chemical lecturers
illustrate the specific gravity of the carbonic acid gas they have been
making, by pouring it from one glass vessel to another.
Let me, in passing, refer to the method in which, at Messrs.
Allsopp’s, the superfluous yeast is utilized, for it is only at these
large establishments that every waste product is turned to good
account. First, as much of the ale as possible is allowed to
drain from the yeast, and then it is press-packed. The soft yeast
is placed between suitable cloths and transferred to hydraulic presses
310 Beer, Scientifically and Socially Considered. | July,
of low power, which reduce it to pretty much the same consistency
as the imported Dutch yeast. In this condition it is packed and
exported to France for distilling purposes.
The rationale of the fermenting process is not as yet tho-
roughly understood, but it is known that the surface yeast is formed
by the nitrogenous matter contained im the wort being earried
upwards by the bubbles of the generated carbonic acid gas. When
this fermentation is carried on at a temperature of from 65° to 90°
Fahrenheit, as it is almost always in England, the yeast invariably
rises, and in Germany this is called “ Obergahrung,” or top-
fermentation ; but in Bavaria and elsewhere abroad, the fermenting
process is often carried on at a lower temperature, and then it is
called “Untergahrung,” or “bottom fermentation,” for in that
case the yeast does not rise, but the nitrogenous matter sinks to
the bottom and forms a slimy sediment. This is the essential
difference between the Continental and English methods of brewing ;
except perhaps that abroad a larger portion of saccharine matter is
left im the beer, which, under a cool temperature is gradually con-
verted into carbonic acid and alcohol in the vessels into which it
is subsequently conducted or poured, and the result is a rich effer-
vescing beverage. I am indebted to my friend Mr. Fenton, the
Secretary of our Embassy at Munich, for some interesting parti-
culars concerning the method of brewing in that city. ‘“ Obergah-
rung,’ or “ top-fermentation,” is there conducted at 15° to 17°
Reaumur = 66° to 71° Fahrenheit, and “Untergahrung,” or
bottom fermentation, at 12° R. = 59°F. The process is not carried
on as with us on the floors of the brewery, but in specially con-
structed subterranean chambers (“Gahrkammer”) in which the
temperature is kept low by means of ice, and thence the beer is
conducted by pipes into the vessels in which the fermentation is
completed.*
In England, as abroad, in the best breweries, the beer is
conducted after fermentation into barrels specially constructed for
the purpose, in which the fermenting process is completed. This
at Allsopps’ and other large breweries is called the “ Union”
system, long rows of barrels being connected together by a hori-
zontal pipe. The barrels are raised above the floor, suspended in
a frame, and are made to revolve on their axis precisely the same
as a revolving barrel-churn. The chamber in which they are
placed is called the “ Union-rcom,” or tunnery, and the reader
will form a fair idea of its extent and appearance by referring to
the Plate (1.). There are two rows of barrels as shown in the
* The German system of mashing is also entirely different from the English. I
believe that the best book published abroad on the Continental system of brewing
is ‘Die Bierbrauerei,’ by Heiss, published at Augsburg, 5th edition, 1869, price
5 florins; but I was unable to procure it in time for the preparation of this essay.
1870. | Beer, Scientifically and Socially Considered. 311
Plate, and above and between the rows runs a long tank, in which
the superfluous yeast is collected. This is done by means of a
“‘swan-neck ” pipe, a syphon acting inversely, and the arrangement
will be understood from the following woodeut (Fig. 10), where
Hig... 10.
Y=
|
I
|
LL
is one of the barrels containing the incompletely fermented beer,
B the swan-neck, ¢ a portion of the long tank or receptacle for the
yeast (Fig. 10). ‘The latter continues to rise slowly whilst the
beer remains in the barrel, being carried upwards (as during active
fermentation) by the escaping carbonic acid gas, and having risen
into the “swan-neck,” it may be seen slowly bubbling over into the
tank. The temperature of the beer during this process is regulated
by a flow of water through an ingeniously contrived tubular
apparatus, which can be inserted into or withdrawn at pleasure from
the barrel, through an oblong aperture in front (see Fig. 10); and
when the beer is cleared of the remaining impurities it is drawn off
by boys who creep underneath the barrels and open a tap attached
to a pipe, first into large vats and then into casks for sale.
The object of allowing the barrels in which fermentation is com-
pleted to revolve, is simply that they may be cleansed after each
operation.
It has, of course, been impossible for me within the short limits
of an essay, professing to deal with the social as well as the scientific
aspects of this question, to describe fully either the principles or
practice of brewing; but I hope enough has been said to convey to
the reader a fair idea of both; and there now remain to be con-
312 Beer, Scientifically and Socially Considered. [July,
sidered: 1st, how beer is injuriously affected during or subsequent
to its manufacture; and 2nd, what social results follow from its
adulteration or abuse. ‘Those who have mixed much with artisans
know well that they seldom drink the fine Burton ale, and if they
do, it is often adulterated after it leaves the brewery; but with a
view to ascertain what they really do drink, I have obtained from my
friend Mr. Norman Tate, F.C.S., Analytical Chemist of Liverpool,
who has interested himself deeply in this question, a report upon
the Liverpool beer, which is as follows :—
“The results of the examination of twenty-five samples of beer
of the kinds known as ‘sixpenny,’ and ‘eightpenny,’ purchased in
the ordinary way from public-houses in different parts of Liverpool,
showed that the quantity of alcohol varied in these samples from
2°2 per cent. (by weight) to 5°62 per cent., the percentage in
fourteen specimens being under 4, very little difference being
observable in this respect between the sixpenny and eightpenny.
The general results convinced me that fully half the samples were
not genuine preparations of malt and hops. One undoubtedly con-
tained tobacco; another, of a dark colour and rather hard unpleasant
taste, gave unmistakable evidence of the presence of sulphate of
iron ; whilst two others contained such a quantity of common salt
as could not be accounted for by the presence of that ingredient in
the water used for brewing, or by any other ordinary cause. Sugar
also appeared to have been added in one case, and in another car-
bonate of soda. ILdid not find in any of these specimens indications
of cocculus indicus, or picric acid, said to be frequently used for
adulterating beer (I have found picrotoxin, the active principle of
cocculus indicus on a previous occasion), but that other matters,
such as liquorice, gentian, and other drugs, not of an injurious
character, but nevertheless adulterants, were present I have not
the least doubt. Several of the samples were of an objectionable
character owing to bad brewing or bad keeping, and, in one or two
instances, the quality was so bad that it is difficult to imagine how
any persons can be fourd to drink such vile stuff. Only eleven
out of the twenty-five were of what I consider really good quality.
One of these was a sample which I purposely obtained, knowing it
to be brewed by a leading firm at Burton, and to have been kept
with great care by the person from whom I procured it.
“ With regard to bitter beers I obtained somewhat better results,
so far as general quality is concerned, with the exception, however,
that the use of other bitters than hops seemed to be rather the rule
than the exception. Although it is difficult or even impossible
always to detect these bitters by distinct chemical tests, yet my
experience of such drugs has made me so familiar with their taste
that I have no hesitation in saying that quassia, wormwood,
gentian, rue, camomile, and orange-peel had been used. Quassia
1870.] Beer, Scientifically and Socially Considered. 313
and wormwood, however, seemed to me to be the bitters in most
general use, the quantity of the latter m one case being so great as
to make the beer positively nauseous. One sample, which appeared
to me to be flavoured with orange-peel, possessed a warm, some-
what spicy taste, which was very apparent in the residue after
evaporation, indicating the addition of something more than the
ordinary ingredients.”
This report, it will be seen, affords experimental confirmation
of what was said by Mr. Glover at the Liverpool Workhouse
meeting, and it will therefore be interesting to inquire a little
further into the matter. Our authorities tell us that the following .
substances are employed to adulterate beer. “ Cocculus indicus
multum (an extract of coceulus indicus), colouring, honey, hartshorn-
shavings, Spanish juice, orange-powder, ginger, grains of paradise,
quassia, liquorice, carraway seeds, copperas, capsicum, mixed drugs.”
These, we are told, “ were seized at different breweries in London,
and at brewers’ druggists’ laboratories.”"* In addition, sulphuric
acid, alum, salt, Datwra stramonium, picric acid, and other sub-
stances are mentioned by different writers.
Of Datura stramonium Mr. Prescott says,t “It has been
frequently used by desperate characters for hocussing or stupefying
the intended victim of a robbery by surreptitiously adding it to his
beer at the public-house bar. It is the seed of the Thorn-apple, a
native of Greece, and belongs to the same family as the tobacco-
plant.” The same author also describes very minutely the micro-
scopical structure of the various seeds which ought, and which
ought not, to be used in the preparation of beer, including barley,
hops, cocculus indicus, grains of paradise, and Datura stramomum,
his object being to facilitate the detection of fraud and crime ; and
I would recommend my microscopical readers, who take an interest
in the question, to examine these various substances with the aid of
a microscope and Mr. Prescott’s beautiful diagrams.
Of the various adulterants named, sulphate of iron, alum, and salt
are employed to give beer a “ head” or froth (salt to stimulate the
thirst as well); sulphuric acid is used to “ bring it forward,” or
harden it, and impart to new beer the character of old; carbonate
of soda to neutralize acidity ; whilst coceulus indicus, quassia, worm-
wood, grains of paradise, and similar substances are mixed with beer
either to impart bitterness or pungency, and to disguise the true
character of the drink.
The necessity for all this doctoring has already been touched
upon, but it may be as well to explain its cause more fully. At
Allsopps’ and other large Burton breweries (and no doubt in many
* Report of Committee of the House of Commons.’ See Watts’s ‘ Dictionary
of Chemistry,’ vol. i., p. 537.
t ‘Strong Drink and Tobacco Smoke,’ p. 37.
314 Beer, Scientifically and Socially Considered. [ July,
smaller respectable country breweries) the capital embarked in the
trade is large enough to admit of the beer being perfectly fer-
mented and freed from impurities or substances likely to cause
acetification ; the beautiful system employed by Messrs. Allsopp
for that purpose has been described. But many brewers really sell
their beer, not at the brewery, but in their own public-houses, and
they have not sufficient capital (or it may be they are too anxious
to make money) to give their products sufficient time to become
fit for consumption. The beer is sometimes drawn off from the
fermenting vats into the barrels in which it is to be sent out, with
the bung holes open for the escape of superfluous yeast; as little
time as possible is given for it to “fine,” and it is sent out to the
public-house with orders to return any that is unconsumed when
it begins to turn sour. I do not pretend to be initiated into
the mysteries of “ brewers’ druggists’ laboratories,’ nor the secrets
of those who employ their fraudulent compounds; but certain it
is, that carbonate of soda is used to neutralize the acidity of the
spoiled beer, and various drugs and chemicals are then added to
impart to it an artificial flavour and counteract the alkaline taste,
until, as Mr. Tate remarks, it is “difficult to imagine how any
persons can be found to drink such vile stuff.” But when we
remember that three-fourths of the persons who do drink it are
drunk already, the mystery is solved. Not only are the lower
kinds of beer thus doctored, but they are often mixed with
Allsopps’, Bass’s, and other fine ales, so that it is the interest
of those firms not only to suppress adulteration, but to do their
best to assist in providing the humbler classes with a cheap pure
beverage, which it will not pay the vendors to sophisticate.
So far, repressive legislation has been a dead letter ; we hear
now and then of the Act of Victoria 23 & 24, c. 84, being put in
force to prevent the sale of grossly adulterated food, or tea, but
although brewers will tell us that the Excise would punish adultera-
tion severely, I do not recollect ever having noticed a prosecution.
Public analysts may be appointed under this Act, and it is to be
hoped that the time is not far distant when this course will be
adopted, and the doctoring of what is really the staple beverage of
our people may be reduced to a minimum, if not entirely prevented.
But we have another question to consider in connection with
the effects of beer upon our population, and that is its real or
reputed strength. For this purpose I have compiled the following
table, partly from the Dictionary articles referred to, and partly from
analyses made for me by chemical friends.
A glance at this table and a moment’s reflection will show why
English beer-drinkers are so often drunkards, whilst Germans, who
indulge in a similar beverage to the same extent, are comparatively
sober. It may be safely said that the percentage of alcohol in German
1870. | Beer, Scientifically and Socially Considered. 315
beer is on the average half as great as in the English, so that
where an Englishman drinks a pint, a German may partake of a
quart ; but when we look at the character of the beer drunk by the
intemperate classes in England, and compare it with that of the
poorer people abroad, we may unhesitatingly assert that less injury
Percentage of
Name of Beer.
Alcohol. Pam ae Water.
Strong Scotch Ale 8°5 10°9 0°15 80°45
Burton Ale .. 5°9 14°5 ae 13-6
Barclays London Porter 5'4 6°0 0°16 88-44
Dreher’s Vienna Beer* 4°62 . fe
Low Brussels Beer (Faro).. 4:9 2°9 0°2 92:0
Bavarian Draught Beer 3°8 o°8 0-14 90°26
Sweet Bohemian Beer (Prague) 3°9 10°9 oe 85°2
Liverpool Doctored Beer (Mr. Tate’ 'stest 2°2 oe Bt we
Berlin White Beer... 1:9 5°7 0°6 91°8
Sweet Brunswick Beer (Mum) .. 1°9 45-0 ae 53°1
|
would arise from drinking half-a-gallon of German beer than from a
pint of English ale. And again, when we compare the Berlin
“ Weissbier,” which contains 1-9 per cent. of alcohol, with the lowest
Liverpool beer, which Mr. Tate found to contain only 2°2 per cent.,
and consider that whilst the Prussian artisan may imbibe his beve-
rage all day long from quart tankards with impunity, an English
labourer will succumb to a few glasses of the public-house trash :
what other inference can be drawn, than that it is not the beer
but the drugs it contains which affect the brain? I have been
told that English labourers will not take kindly to German beer ;
it is not strong enough for them. This is quite true of the present
generation ; how should it be otherwise, when their taste has been
corrupted by cocculus indicus, tobacco, and salt? But unless the
advocates of temperance strenuously support the introduction of a
mild, pure, cheap drink (for the Englishman not alone buys bad
beer, but pays three or four, aye in some cases five or six times as
much for it as the German does for his unadulterated beverage),
unless, I say, a vigorous effort is made to change the taste of the
next generation as it grows up, the same difficulty will still remain
to be overcome by posterity.
And now let me, in conclusion, refer to the data which have
been given by an eminent Swiss social economist, to show (as I
have done elsewherej) that comparative sobriety is the result of
* For this test, I am indebted, through the kindness of Dr. Frankland, to
Mr. W. Valentin, of the Royal College of Chemistry.
+ ‘The German Working Man,’ p. 70, quoting Gustave Moynier, ‘Les Insti-
tutions ouvrieres de la Suisse. Cherbuliez : Paris,
VOL, VII. | Z
316 Spiritualism Viewed by the . alaly,
the introduction of beer, and the displacement of stronger drinks.
The canton of Soleure in Switzerland was formerly very imtem-
perate, now it is much improved. This is partly attributable to
the opening of small shops where good coffee (a thing unknown
to the poorer classes in England) along with small white rolls and
butter are sold; but concurrently with that, a change has taken
place in the alcoholic drinks of the people, which is represented by
the following figures, denoting a Swiss measure of 14 litre :—
Consumed in Swiss Wines. Foreign Wines. Beer and Cider, Brandy.
1863 oom Re Eh oy ee 637,166 .. 23,168 ie, ~~ Mectaaee
1865 ie 1483596 909,944" -.. S372 go) jee
The total consumption of alcoholic liquor, therefore, had in-
creased altogether nearly 30 per cent., but the beer consumed was
augmented threefold, whilst brandy had fallen off 4 per cent. !
Couple this experience with the fact that the Germans drink
certainly as much, if not more beer than we do, and are sober,
whilst we are perhaps the most drunken nation on the earth,
and I conceive no one will dispute the proposition so often ad-
vanced by me, that as claret and light Continental wines are slowly
reforming our middle classes, so will it be necessary to introduce
mild, pure beer as a staple drink, in order to attain the same end
amongst the labouring population. Until that is done, I am con-
vinced that not all the efforts of temperance advocates (whose
self-denial every one must admire and respect), neither lectures,
tea-meetings, denunciation, nor repressive legislation, will avail
anything beyond saving here and there a drowning wretch from
the flood of poisoned liquor with which our large towns are deluged,
but such a change as I have suggested being accomplished, I be-
lieve that, with the spread of education, and the introduction of more
rational amusements than those now offered to the humbler classes,
repressive legislation will be no longer needed; the ranks of our
criminals, paupers, and lunatics will be thinned, and it is to be
hoped the foulest blot will in time be removed from our national
escutcheon.
II. SPIRITUALISM VIEWED BY THE LIGHT OF
MODERN SCIENCE.
By Witi1am Crooxss, F.B.S., &e.
Some weeks ago the fact that I was engaged in investigating
Spiritualism, so called, was announced in a contemporary ;* and in
consequence of the many communications I have since received, I
think it desirable to say a little concerning the investigation which
I have commenced. Views or opinions I cannot be said to possess
* The ‘Atheneum.’
1870. | Light of Modern Science. 317
on a subject which I do not pretend to understand. I consider it
the duty of scientific men who have learnt exact modes of working,
to examine phenomena which attract the attention of the public,
in order to confirm their genuineness, or to explain if possible the
delusions of the honest and to expose the tricks of deceivers.
But I think it a pity that any public announcement of a man’s
investigation should be made until he has shown himself willing to
speak out.
A man may be a true scientific man, and yet agree with Prof.
De Morgan when he says,—“I have both seen and heard, in
a manner which would make unbelief impossible, things called —
spiritual, which cannot be taken bya rational being to be capable of
explanation by imposture, coincidence, or mistake. So far I feel the
eround firm under me; but when it comes to what is the cause of
these phenomena, I find I cannot adopt any explanation which has
yet been suggested. . . . The physical explanations which I have
Seen are easy, but miserably insufficient. ‘The spiritual hypothesis
is sufficient, but ponderously difficult.”
Regarding the sufficiency of the explanation I am not able to
speak. That certain physical phenomena, such as the movement
of material substances, and the production of sounds resembling
electric discharges, occur under circumstances in which they cannot
be explained by any physical law at present known, is a fact of
which I am as certain as I am of the most elementary fact in
chemistry. My whole scientific education has been one long lesson
in exactness of observation, and I wish it to be distinctly under-
stood that this firm conviction is the result of most careful investi-
gation. But I cannot, at present, hazard even the most vague
hypothesis as to the cause of the phenomena. Hitherto I have
seen nothing to convince me of the truth of the “spiritual” theory.
In such an inquiry the intellect demands that the spiritual proof
must be absolutely incapable of being explained away; it must be so
strikingly and convincingly true that’ we cannot, dare not deny it.
Faraday says, ‘“ Before we proceed to consider any question in-
volving physical principles, we should set out with clear ideas of the
naturally possible and impossible.” But this appears like reasoning
in a circle: we are to investigate nothing till we know it to be
possible, whilst we cannot say what is impossible, outside pure mathe-
matics, till we know everything.
In the present case I prefer to enter upon the inquiry with no
preconceived notions whatever as to what can or cannot be, but
with all my senses alert and ready to convey information to the
brain; believing, as I do, that we have by no means exhausted
all human knowledge, or fathomed the depths of all the physical
forces, and remembering that the great philosopher already quoted
said, in reference to some speculations on the gravitating force,
Z2
318 Spiritualism Viewed by the [July,
“ Nothing is too wonderful to be true, if it be consistent with the
laws of nature; and in such things as these, experiment is the best
test of such consistency.”
The modes of reasoning of scientific men appear to be generally
misunderstood by spiritualists with whom I have conversed, and
the reluctance of the trained scientific mind to investigate this
subject is frequently ascribed to unworthy motives. I think, there-
fore, it will be of service if I here illustrate the modes of thought
current amongst those who investigate science, and say what kind of
experimental proof science has a right to demand before admitting
a new department of knowledge into her ranks. We must not mix
up the exact and the inexact. The supremacy of accuracy must be
absolute.
The first requisite is to be sure of facts; then to ascertain con-
ditions ; next, laws. Accuracy and knowledge of detail stand fore-
most amongst the great aims of modern scientific men. No observa-
tions are of much use to the student of science unless they are
truthful, and made under test conditions; and here I find the great
mass of spiritualistic evidence to fail. In a subject which, perhaps,
more than any other, lends itself to trickery and deception, the
precautions against fraud appear to have been, in most cases, totally
insufficient, owing, it would seem, to an erroneous idea that to ask
for such safeguards was to imply a suspicion of the honesty of some
one present. We may use our own unaided senses, but when we
ask for instrumental means to increase their sharpness, certainty, and
trustworthiness under circumstances of excitement and difficulty,
and when one’s natural senses are liable to be thrown off their
balance, offence is taken.
In the countless number of recorded observations I have read,
there appear to be few instances of meetings held for the express
purpose of getting the phenomena under test conditions, in the pre-
sence of persons properly qualified by scientific traming to weigh
and adjust the value of the evidence which might present itself.
The only good series of test experiments I have met with were tried
by the Count de Gasparin, and he, whilst admitting the genuineness
of the phenomena, came to the conclusion that they were not due
to supernatural agency.
The pseudo-scientific spiritualist professes to know everything:
no calculations trouble his serenity, no hard experiments, no long
laborious readings ; no weary attempts to make clear in words that
which has rejoiced the heart and elevated the mmd. He talks
glibly of all sciences and arts, overwhelming the inquirer with terms
like “ electro-biologize,” “ psychologize,” “animal magnetism,” &c.
—a mere play upon words, showing ignorance rather than under-
standing. Popular science such as this is little able to guide dis-
covery rushing onwards to an unknown future ; and the real workers
1870. | Light of Modern Science. 319
of science must be extremely careful not to allow the reins to get
into unfit and incompetent hands.
Tn investigations which so completely bafile the ordinary observer,
the thorough scientific man has a great advantage. He has followed
science from the beginning through a long line of learning, and he
knows, therefore, in what direction it is leading; he knows that
there are dangers on one side, uncertainties on another, and almost
absolute certainty on a third: he sees to a certain extent in advance.
But, where every step is towards the marvellous and unexpected,
precautions and tests should be multiplied rather than diminished. |
Investigators must work; although their work may be very small
in quantity if only compensation be made by its intrinsic excellence.
But, even in this realm of marvels,—this wonder-land towards which
scientific inquiry is sending out its pioneers,—can anything be
more astonishing than the delicacy of the instrumental aids which
the workers bring with them to supplement the observations of their
natural senses ?
The spiritualist tells of bodies weighing 50 or 100 Ibs. being
lifted up into the air without the intervention of any known
force; but the scientific chemist is accustomed to use a balance
which will render sensible a weight so small that it would take ten
thousand of them to weigh one grain; he is, therefore, justified in
asking that a power professing to be guided by intelligence, which
will toss a heavy body up to the ceiling, shall also cause his
delicately-poised balance to move under test conditions.
The spiritualist tells of tappig sounds which are produced in
different parts of a room when two or more persons sit quietly round a
table. The scientific experimenter is entitled to ask that these taps
shall be produced on the stretched membrane of his phonautograph.
The spiritualist tells of rooms and houses being shaken, even to
injury, by superhuman power. The man of science merely asks for
a pendulum to be set vibrating when it is in a glass case and sup-
ported on solid masonry.
The spiritualist tells of heavy articles of furniture moving from
one room to another without human agency. But the man of
science has made instruments which will divide an inch into a
million parts; and he is justified in doubting the accuracy of the
former observations, if the same force is powerless to move the index
of his instrument one poor degree.
The spiritualist tells of flowers with the fresh dew on them, of fruit,
and living objects being carried through closed windows, and even solid
brick-walls. ‘The scientific investigator naturally asks that an addi-
tional weight (if it be only the 1U00th part of a grain) be deposited
on one pan of his balance when the case is locked. And the chemist
asks for the 1000th of a grain of arsenic to be carried through the
sides of a glass tube in which pure water is hermetically sealed.
320 Spiritualism Viewed by the | July,
The spiritualist tells of manifestations of power, which would
be equivalent to many thousands of “foot-pounds,” taking place
without known agency. The man of science, believing firmly in
the conservation of force and that it is never produced without a
corresponding exhaustion of something to replace it, asks for some
such exhibitions of power to be manifested in his laboratory, where
he can weigh, measure, and submit it to proper tests.*
For these reasons and with these feelings I began an inquiry
suggested to me by eminent men exercising great influence on the
thought of the country. At first, ike other men who thought little
of the matter and saw little, I believed that the whole affair was a
superstition, or at least an unexplained trick. ven at this moment
I meet with cases which I cannot prove to be anything else ; and
in some cases I am sure that it is a delusion of the senses.
I by no means promise to enter fully into this subject ; it seems
very difficult to obtain opportunities, and numerous failures cer-
tainly may dishearten anyone. ‘The persons in whose presence
these phenomena take place are few in number, and opportunities
for experimenting with previously arranged apparatus are rarer still.
T should feel it to be a great satisfaction if I could bring out light
in any direction, and I may safely say that I care not in what direc-
tion, With this end in view, I appeal to any of my readers who
may possess a key to these strange phenomena, to further the pro-
gress of the truth by assisting me in my investigations. ‘That the
subject has to do with strange physiological conditions is clear, and
these in a sense may be called “spiritual” when they produce
certain results in our minds. At present the phenomena I have
observed bafile explanation ; so do the phenomena of thought, which
are also spiritual, and which no philosopher has yet understood.
No man however denies them.
The explanations given to me, both orally and in most of the
books I have read, are shrouded in such an affected ponderosity of
style, such an attempt at disguising poverty of ideas in grandiloquent
language, that I feel it impossible, after driving off the frothy
diluent, to discern a crystalline residue of meaning. I confess that
the reasoning of some spiritualists would almost seem to justify
Faraday’s severe statement—that many dogs have the power of
coming to much more logical conclusions. Their speculations utterly
ignore all theories of force being only a form of molecular motion,
and they speak of Force, Matter, and Spirit, as three distinct
‘ * Tn justice to my subject, I must state that, on repeating these views to some
of the leading ‘‘spiritualists” and most trustworthy “mediums” in England, they
express perfect confidence in the success of the inquiry, if honestly carried out in
the spirit here exemplified; and they have offered to assist me to the utmost of
their ability, by placing their peculiar powers at my disposal. As far as I
have proceeded, I may as well add that the preliminary tests have been
satisfactory.
1870. ] Light of Modern Science. 321
entities, each capable of existing without the others; although they
sometimes admit that they are mutually convertible.
These spiritualists are certainly not much in advance of an
alchemical writer, who says—
We behad, “T asked Philosophy how I should
te? Have of her the thing I would.
She answered me when I was able
To make the water malliable,
Or else the way if I could finde,
To mesure out a yard of winde;
Then shalt thou have thine own desire,
When thou canst weigh an ounce of Fire;
Unless that thou canst do these three,
Content thyselfe, thou get’st not me.”
It has been my wish to show that science is gradually making
its followers the representatives of care and accuracy. It is a fine
quality that of uttering undeniable truth. Let, then, that position
not be lowered, but let words suit facts with an accuracy equal to
that with which the facts themselves can be ascertained; and in a
subject encrusted with credulity and superstition, let it be shown
that there zs a class of facts to be found upon which reliance can be
placed, so far, that we may be certain they will never change. In
common affairs a mistake may have but a short life, but in the study
of nature an imperfect observation may cause infinite trouble to
thousands. The increased employment of scientific methods will
promote exact observation and greater love of truth among inquirers,
and will produce a race of observers who will drive the worthless
residuum of spiritualism hence into the unknown limbo of magic
and necromancy.
If spiritualists would but attend to the teachings of their own
prophets, they would no longer have to complain of the hostile
attitude of Science; for hear what Thomas L. Harris urges, in his
‘Lyric of a Golden Age!’
‘The nearer to the practical men keep—
The less they deal in vague and abstract things,
The less they deal in huge mysterious words—
The mightier is their power.
* * * *
The simplest peasant who observes a truth,
And from a fact deduces principle,
Adds solid treasure to the public wealth.
The theorist, who dreams a rainbow dream,
And calls hypothesis philosophy,
At best is but a paper financier,
Who palms his specious promises for gold.
Facts are the basis of philosophy ;
Philosophy the harmony of facts
Seen in their right relation.”
( 322 ) [July,
Ill. THE RATE OF GEOLOGICAL CHANGE.
By H. M. Jenxrins, F.G.S., Secretary of the Royal Agricultural
Society of England.
PUBLIC opinion on questions of theoretical geology grows slowly,
and usually precedes the statement of important speculations.
The progress of discovery leads up to the induction, which, after
floating more or less hazily in the minds of geologists for a certain
time, is at last enunciated piecemeal at irregular intervals by the
more daring theorists. Finally the scattered fragments are col-
lected and arranged, bound together by the idea which connects
them, and placed on record as a complete whole. This last is the
task which I propose to attempt in reference to the progress of
public opinion on the subject at the head of this article.
But first, let me clear the way by a short summary of the ideas
which prevail amongst English geologists, so far as they bear on
this subject. The prominent feature of the favourite modern school
of geology in England—Uniformitarianism—is the belief that the
forces in operation at the surface of the earth in former times dif-
fered in no appreciable degree from those now in action. This
article of faith is, however, commonly restricted to what, for con-
venience of expression, has been termed “ Geological time’”—a
period which is entirely represented by the rocks found on the
earth’s surface, from the oldest to those now in course of formation.
According to this school, the rate of geological change has been
approximately equal throughout the vast period which has elapsed
since the deposition of the oldest stratified rock. Local variations
of this law would doubtless be admitted by even the most thorough
advocate of Uniformity, but the broad general principle character-
istic of the creed is equality in the rate of change throughout all
geological time.
Catastrophism, which is the name usually given to the other
great school of geologists, is distinguished broadly by the tenet
that in past times the forces in operation at the surface of the
globe were of far greater intensity than they are now, and that
great physical changes were then produced by more or less violent
cataclysms. Probably there are geologists who now-a-days reject
the catastrophes, but still cling to the belief that modern forces are
much less intense, and modern changes much less rapid and ex-
tensive, than those which occurred in former geological periods.
Therefore, whichever view we take of this theory, it is clear that
its advocates believe that the rate of geological change was greater
in past times than it is now; and the inference appears fair that,
according to this school, the rate of change has, on the whole, pro-
gressively diminished from the earliest down to modern times.
1870. | The Rate of Geological Change. 323
In his Anniversary Address to the Geological Society last year,
Professor Huxley defined a “third phase of geological speculation,
namely, Evolutionism.” This doctrine, in the words of the author,
“embraces all that is sound in both Catastrophism and Uniformi-
tarianism, while it rejects the arbitrary assumptions of the one, and
the, as arbitrary, limitations of the other.” ‘To my mind it cannot
well be distinguished from ordinary Theoretical Geology, unfettered
by the trammels of any school; but obviously, the Hvolutionist is
prepared to accept whatever theory on the rate of geological change
can be shown to be consistent with those known facts which can
fairly be quoted as evidence.
The title of this article is capable of more than one interpreta-
tion, and in its various meanings it has already been investigated
by speculative geologists. The late Professor Edward Forbes, in
his lecture before the Royal Institution, “On the Manifestation of
Polarity in the Distribution of Organized Beings in Time,”* en-
deavoured to show that the rate of development of generic types
reached its maximum intensity, firstly, during the earlier Paleozoic
periods, and secondly, during the later Neozoic periods; that is to
say, near the beginning and the end of the geological scale. Again,
the rate of development was shown to be at its minimum during
the later Paleozoic (Permian) and earlier Neozoic (Triassic) periods,
from which contiguous zero-points the development of generic types
was asserted to increase in both directions.t This relation Professor
Forbes termed “ Polarity,’ and he showed how in several of the
great divisions of the animal kingdom, two of their groups appeared
to exercise a kind of “ reciprocity,” as, for instance, our old friends
the Palzeozoic four-starred corals versus the Neozoic six-starred.
But Professor Forbes was careful to make the reservation that
“the numbers of species in a group or genus at an} given epoch is
to be excluded, not being an element in the discussion of the ques-
tion, though apt to be introduced through mistake of the nature
of the generalization attempted to be attained.” Indeed, the rela-
tions of individuals, species, and genera were favourite subjects of
speculation with this poetic and philosophical paleontologist ; and
the generalization we have just sketched was a sequel to some
other inquiries, in recording which he defines a genus as “an
abstraction—an idea—but an idea impressed on nature, and not
arbitrarily dependent on man’s conceptions.”{ Again, “a genus
consists of more or fewer of these manzes resulting from one
[species] linked together, not by a relationship of descent, but by
* “Notices of the Meetings of the Royal Institution,’ vol. i., p. 428.
+ This view may be correct; but at present, as at the time when it was
advanced, we have only negative evidence in support of it; and it is still very
possible that Permian and Triassic recks, rich in generic types, may be discovered
in some hitherto unexplored region of the earth.
t ‘Notices,’ &., vol. i. p. 196.
4
324 The Rate of Geological ee [ July,
an affinity dependent on a divine idea. m= Tt is necessary to bear
in mind these definitions of a genus in order to understand the
author’s generalization of “ Polarity ” in the “development of
generic types,’ and to prevent confusion with other ideas which I
shall attempt to elucidate in the following pages.
Before estimating the rate of geological change in successive
epochs, we must clearly understand the means by which that rate
is measured. Our geological chronology is divided into epochs of
greater or less extent, distinguished and characterized by certain
forms of animal and vegetable life, either peculiar to them, or pre-
ponderating in number and variety during their continuance. We
can conceive that in a previously unexplored country, far away
from any region whose geology is known, the explorer may meet
with diverse geological formations, each formation bemg charac-
terized by a sufficiently numerous and distinctive fauna. Lf forma-
tion A contains 1000 species, and is 10,000 feet thick, and forma-
tion B contains 5000 species, but is only 1000 feet thick, and if
the range of zoological rank in the 5000 species is approximately
the same as in the 1000 species, we should be justified in saying of
formation A, that, in comparison with formation B,—
(1) It was deposited very quickly ; or,
(2) During its deposition species changed very slowly.
Further investigation by our hypothetical explorer might pos-
sibly furnish him with evidence that, during the deposition of for-
mation A, the conditions of climate and physical geography had
remained more or less stationary, and that the strata were deposited
slowly. On the other hand, formation B and its fossils might yield
evidence of great changes in climate and physical geography, and of
comparatively rapid deposition. Under these circumstances, he
would be justified in the conclusion that, during the epoch repre-
sented by formation A, the rate of geological change was much less
rapid than during the ‘period represented by formation B.
This hypothetical contrast will assist the reader in appreciating
the significance of the following synopsis of the Paleozoic and
Mesozoic rocks and their fossils, and will enable him to estimate
how far these epochs agree with those which we have supposed to
be represented by formations A and B respectively.
Professor Phillips, in his Rede lecture, delivered before the
University of Cambridge in 1860,} remarks that if we select among
the marine classes of animals those which are represented in all the
great periods of geology, count the number of species yet discovered
in them in British strata, and refer them at present to only three
great periods, we find that the Paleozoic rocks contain 2729 species,
* Loc. cit.
+ Afterwards published under the title of ‘Life on the Earth. Macmillan.
1860. See pp. 59-62.
1870. ] The Rate of Geological Change. 325
the Mesozoic 2170, and the Cainozoic 1222. ‘The absolute
number of marine species appears thus to be greatest in the
Paleozoic strata; but when the thickness of the deposits, which
represents elapsed time, is taken into account, the variety of forms
in a given thickness or given period of time is very much less.”
This conclusion he illustrates by the following Table :—
Total Species in| Maximum Relative Number
eight Classes Thickness of Species to
g : : 1000 feet.
Cainozoic strata .. F228 2,240 545
| Mesozoic strata .. .. 2,170 23,190 164*
| Paleozoic strata... 2,729 57,154 41+
And he again observes (p. 62), “Thus it appears certain that the
variety of life estimated by the marine tribes existing in a given
period is greater in the more recent periods.’”{
* Should be 93. + Should be 47.
{ The editor of this Journal (Mr. James Samuelson) has asked me whether I
may not have overlooked the biological aspect of the case, and whether this may
not be the result of the laws of selection in the lower forms of life varying from
those in the higher forms, and the rate of change being perhaps more rapid in the
latter; e.g. low molluscs or acalephs having predominated in earlier times, might go
on multiplying for ages without material change, their conjugation being, like that
of plants, regulated by the elements, whilst in the fishes and higher molluscs, sexual
selection and destruction of each other would be very active and would produce
rapid change of species. It appears to me that at least two powerful arguments
may be advanced against this interpretation. First, geologically considered, the
interpretation would be erroneous because we are contrasting the abundance and
variety of life characteristic of the different great periods, and it cannot be said of
any one great period that it is characterized, for instance, exclusively by low mol-
luses, nor of any other that it is characterized exclusively by higher orders of that
class, as is shown in the following Table by Professor Phillips :—
Zoo- | Echino-| Crus- |Brachio-| Mono- | Dimy- | Gaste- | Cepha-
phyta. \dermata.| tacea. | poda. |myaria.| aria, | ropoda. | lopoda. Total.
Cainozoic .. 27 41 15 8 63 394 662 12 | 1222
Messozoic .. | 103 | 245 65 165 308 | 499 389 | 396 | 2170
Paleozoic .. | 379 225 218 | 632 196 | 342 | 401 336 | 2729
Thus the Paleozoic rocks abound both in the highest and the lowest orders
of the testaceous Mollusca, viz. the Cephalopoda and the Brachiopoda, while the
Tertiary deposits are characterized by the intermediate groups of Gasteropoda
and Lamellibranchiata. The oldest fishes are not regarded by the best autho-
rities as of uniformly lower types than the most recent; and with regard to the
power of sexual selection, the advantage is doubtless on the side of the Paleozoic
and Mesozoic representatives of the modern Claspers. But the weightiest argument,
to my mind, is to be derived from the improbability that sexual selection in such
animals (for, owing to our imperfect record, we are necessarily compelled to deal
almost exclusively with animals of no high zoological grade) was to any great
extent the result of direct volition, or that sexual selection was the determining
cause of change of species, although it no doubt was one means to that end.
It appears to me far more probable that changes in species have been rapid
326 The Rate of Geological Change. [ July,
These quotations show that so keen an observer and so
thoughtful a philosopher as Professor Phillips had not allowed this
subject to escape him; but Iam not aware that any other geologist
has discussed it from precisely the same point of view. ‘The figures
given by Professor Phillips show that the rate of geological change,
with regard to the relation between the deposition of strata and the
changes in faune, was neither uniform throughout all geological
times, as the Uniformitarians would have it, nor more intense in
the earlier periods, as the Catastrophists contend. On the contrary,
these figures prove, to the extent which they go, that the rate of
change was marvellously more rapid in the more recent periods,
and that the increase in rapidity was rapidly progressive, from the
earliest to the latest times. There are four times as many species*
belonging to the eight classes which are persistent through: all
geological periods, per 1000 feet, in the Mesozoic strata than in the
Paleeozoic, and there are three times the number { of such species
per 1000 feet in the Cainozoic strata that there are in the Mesozoic.
In the same year (1860), Professor Phillips, as President of the
Geological Society, delivered the Anniversary Address to the Fellows,
and again adverted to this subject, and the following quotation
gives his conclusions, as delivered before one of the most critical
geological audiences in Europe :—
“In the earlier periods of the world’s history, the changes of
life in the sea were accomplished at a rate much less rapid than
that which prevailed in later times,t which agrees with the acknow-
ledged very wide distribution of Paleozoic forms in geographical
space. Admitting the changes of life on the whole to be equal
from the Paleozoic to the Mesozoic, and from these to the Cainozoic
periods, we find the rate of progressive change § 75th for Paleozoic,
zsth for Mesozoic, and 3rd for Cainozoic time,—a conclusion of great
importance, and probably indicative of the greater influence and
or slow, in proportion as changes in climate and physical geography have been
frequent or seldom. In the Paleozoic periods we have reason to believe that
changes in physical geography were rare, while the climate and the nature of the
earth’s surface were very slightly diversified. In the Tertiary epoch, on the con-
trary, climate and physical conditions have been very diverse, and have frequently
varied; and these variations have been accompanied by proportionate changes of
species. If periods of small duration had been compared by Professor Phillips, it
is quite certain that the chances of error would have been very great; but by put-
ting in contrast only the three great epochs into which Geological 'Time has been
divided, I believe that those chances of error have been reduced to a minimum,
according to the well-known law of averages—H. M. J. With all deference to
so eminent a geologist as Professor Phillips, and to the author of this essay, it
appears to me that such a table is an unsafe guide in the present state of the
paleontological record. Here, for example, the fishes—the most important group
of all, biologically—are entirely omitted —Eprror.
* According to my calculation, twice as many. + I make it six times.
t{ The italics are mine —H. M. J.
§ Taking the unit of thickness such that it shall be =4,th of the ascertained
strata in which life-traces occur. :
1870.] The Rate of Geological Change. 327
superiority in early times of a slowly changing physical condition
of the whole globe over the partial and irregularly varying local
conditions, which were continually augmenting, and are still
augmenting in influence with the lapse of time.”
It may be objected to Professor Phillips’s figures that he
includes only the species belonging to the eight classes of animals
which have been represented in each of the three great periods. I
therefore give in the following Table the approximate total number
of species (excluding plants only) that have been discovered in
British stratified rocks up to the present time, with the result per
1000 feet, and the average number of feet per species in each
great period :—
- Relative Number} Number of
. Number of Maximum ;
ae Species: | Thickness, | Of Soeise Per) | eee
Cainozoic 1,500 2,240 670 5
Mesozoic... 4,000 23,190 173 0°8
Paleozoic 3,500 57, 124 61 16°3
‘The evidence yielded by the analysis of these figures is even more
in favour of the conclusion that the rate of geological change,
according to the evidence of animal life, has progressively increased
from the earliest to the latest times.
With one other numerical illustration I shall close the argument
drawn from the organic phase of the question. The late Professor
Bronn, in his prize essay, and in the third edition of his ‘ Lethea
Geognostica, gives the following as the total numbers of known
species in 1850, just twenty years ago :—Paleozoic 6681, Mesozoic
10,879, and Caiozoic 15,188. If we assume the maximum
thickness of the deposits of these periods to be 60,000, 25,000, and
10,000 * respectively, we get the following numbers of species as
occurring per 1000 feet of strata :—Paleeozoic 111, Mesozoic 435,
and Cainozoic 1513 ; thus showing exactly the same result almost
in the same proportions. | 3
The foregoing calculations are based on the assumption that
the time required for the deposition of 1000 feet of strata was
approximately the same in the Paleozoic, Mesozoic, and Cainozoic
periods, and so far the argument is Uniformitarian ; but the
received interpretation of the physical conditions which prevailed
in those periods renders it probable that the strata were deposited
more slowly in the earlier than in the later periods, which, a
fortiori, adds considerable strength to my conclusion.
The inorganic aspect of the subject has been discussed more
* I purposely make this number very large, so as not to run the risk of being
charged with making too much of my argument from this point of view.
328 The Rate of Geological Change. - [Tuly,
frequently than that phase which we have just reviewed ; but with
this striking difference, that no geologist has treated it from the point
of view of pure geology in the same direction as Professor Phillips
has from a paleontological standpoint,—the geological arguments
are all either purely Uniformitarian, or as purely Catastrophic.
In the second of two essays “On the Measurement of Geolo-
gical Time,” which were published in ‘ Nature’ only a few weeks
ago,* Mr. Wallace touches on this question. He remarks} that for
the last 60.000 years the eccentricity of the earth’s orbit has been
very small, and that therefore the opposite phases of precession, each
lasting 10,500 years, have during that time produced scarcely any
effect on climate. This state of things, however, is regarded by
him, as by Mr. Croll, as quite exceptional, for during nearly the
whole of the last three million years the opposite state of things has
existed, namely, a high eccentricity coupled with a change (in the
extra-tropical regions) every 10,500 years, from a very cold toa
very mild climate. Mr. Wallace therefore argues as follows :—
“This will necessarily have caused much migration both of plants
and animals, which would inevitably result in much extinction and
comparatively rapid modification. Allied races would be continu-
ally brought into competition, altered physical conditions would
induce variation, and thus we should have all the elements for
natural selection and the struggle for life to work upon and develop
new races. High eccentricity would therefore lead to a rapid change
of species, low eccentricity to a persistence of the same forms; and,
as we are now, and have been for 60,000 years, in a period of low
eccentricity, the rate of change of species during that time may be
no measure of the rate that has generally obtained in past geological
epochs.”
: I shall not stop to criticize Mr. Wallace’s attempt to measure
geological time, as Mr. Dawkins has already pointed out the fallacy
involved in the major premiss of this argument, v7z. that all climatal
change has depended solely on the eccentricity of the earth’s orbit.t
It is sufficient for my present purpose to point out that Mr. Wallace
recognizes the principle that the rate of change of species may have
varied in different geological epochs. ‘To refer the cause of its
variation to differences in the eccentricity of the earth’s orbit is pro-
bably erroneous, but that error of ultimate explanation by no means
diminishes the importance or the stability of the fact which is thus
sought to be explained.
Both Sir Charles Lyell and Mr. Wallace have attempted to
estimate the duration of the several geological epochs, basing their
calculations on a supposed rate of change in species of marine
mollusca. In this way Sir Charles Lyell concludes that “ we may
* February 17th and March 3rd. + Loc. cit., March 3rd, pp. 453 and 454.
~ See ‘ Nature,’ March 17, p. 505.
1870. | The Rate of Geological Change. 329
consider a million years to represent the twentieth part of a com-
plete revolution in species, and we might thus estimate the number
of years required for the elaboration of the successive Tertiary for-
mations.” Proceeding thus, Sir Charles Lyell calculates that two
hundred and forty millions of years have elapsed since the beginning
of the Cambrian period. Mr. Wallace, however, by taking the same
facts and figures, manipulates them differently, and comes to the
conclusion that the lapse of time is exactly one-tenth of that esti-
mated by Sir Charles Lyell. This difference of result is of very
little consequence, as both calculations are equally speculative, and
it is chiefly to a point of resemblance that I wish to draw attention.
Sir Charles Lyell and Mr. Wallace, however much they may
differ in other matters, whether they regard the revolution of species
as haying been accomplished in no less a period than twenty millions,
or in one no greater than two millions, are agreed in using the same
rate of change for the Paleozoic as for the more recent periods.
Taking the figures of the latter author, and calculating the time
required for the deposition of strata on his hypothetical rate of
change in species, we get at the following results :—
ons Duration 7 icles of b Bale of
er1oas. OCKS eposit; years
(Wallace). (bilan. uenttoek:
Cainozoic wig ok ia 6,000,000 2,240 2,678
MTESOZ0IC! se) fats 8,000,000 23,190 345
Paleozoic anh hee 10,000,000 57,124 175
It may be urged that the Tertiary rocks are comparatively thin
in England, owing to the absence of Miocene deposits; but the
same argument may be applied to each of the three periods with
greater or less force; and at any rate the relative rapidity of deposit
would not be very much disturbed if we took the maximum thick-
ness all over the world instead of those occurring in the British
Islands. Leaving denudation entirely out of the question, it does
not seem at all probable that the Paleozoic rocks should have been
deposited at the swift rate of one foot in 175 years; and if we
deduct from the calculation the period represented by “ breaks,”
which Professor Ramsay regards as longer even than that repre-
sented by strata, we shall have the conclusion drawn that the
Paleeozoic rocks were deposited at the rate of one foot in less than
a century! At the present day there are many localities peculiarly
favourable to the rapid accumulation of deposits over limited areas,
as, for instance, the deltas of the great rivers; but even in such
cases the rate of deposition is probably not more than what, accord-
ing to Mr. Wallace’s estimate, must have been general all over the
aquiferous surface of the earth during Paleozoic times.
330 Air-Pollution by Chemical Works. [ July,
Whether we measure the relative lapse of time occupied by the
successive events of Geological History by the known facts of the
accumulation of deposits, or by the comparative changes which have
occurred in the life of successive periods, we are led equally to infer
that the rate of geological change has been more rapid in the
later than in the earlier geological periods, and that that rate has
increased progressively from the earliest to the latest times.
Such an inference, though it may at first sight seem here-
tical, is in reality but the natural result of those conditions of the
earth’s surface which the most orthodox geologists regard as cha-
racteristic of successive periods. A greater uniformity of climate
and of surface in the earlier Paleozoic periods than at the present
day has long been considered the legitimate inference to be drawn
from the thick masses of uniform deposits spread over large areas,
and containing species of fossils possessing an enormous geographical
distribution. In ascending the geological scale the deposits gradu-
ally become more differentiated, and the fossils belong to species
which had a more restricted geographical range; these differences
are usually and properly regarded as the result of greater diversity
of climate and surface-configuration during the later periods, and
these more diversified conditions must have been accompanied by
a greater rapidity in the rate of geological change, if for no other
reason than that there were a greater number of centres of change,
acting and reacting on each other.
Ty. AIR-POLLUTION BY CHEMICAL WORKS.
A MANUFACTURER, having realized his primary object of making
what he can out of the materials which pass under his hands, and
having utilized all that he deems valuable in them, finds there is yet
another need to be fulfilled; he must get rid of his refuse, and that
as speedily as possible. Our present object is to watch this latter
operation, and, losing sight of the beautiful or useful results of his
work, to direct our attention to what is waste or refuse, and inquire
how he disposes of it. When this is solid and bulky, it must be
removed at the cost of much labour, and a place must be provided
where it can be deposited. When the refuse is a liquid, the pro-
cess of getting rid of it is generally less expensive ; it will flow away
in the water-courses if only proper drains and passages are provided.
When the refuse is gaseous, this process of removal is easier still ;
no passages need be cut, no culverts nor bridges built, the vapour
can be allowed to pass into the air, and is blown away.
In each of these cases the manufacturer’s object is attained; he
is rid of the refuse, and has room for renewed work. Unfortunately,
1870. ] Air-Pollution by Chemical Works. 331
however, although he is rid of it, his neighbours are not so; they
find, on the one hand, that the water of their brook is no longer fit
for use, nor pleasant to look at, and the air they breathe is polluted
with unsavoury and noxious vapours. Where a manufactory of this
kind stands alone, or where only those who are dependent on it for
their subsistence dwell in its vicinity, this state of things goes on for
a long time without calling forth much complaint. Sooner or later,
however, complaints must come; we cannot all live at arm’s length.
Population increases, we are pressed together, and valuable though
the various products of manufacturing industry may be, pure air
and pure water are more valuable still. Yet we cannot do without
the manufactory, unless we return to barbarism. A naked savage
eating uncooked roots erects no chimney to pour its black or acrid
vapour into the air; he discharges the liquor from no dye back into
the clear brook of the glen—but he remains a savage. We must
keep our manufactories; by their products we are warmly clothed, our
houses are firmly built and are decorated with colours; the wind is
shut out by panes of transparent glass; the paper on which we write
is white and fair. These and a thousand other things are the results
of many a mechanical or intricate chemical process, the waste
products from which, solid, liquid, and gaseous, are unpleasant
enough.
If, then, we will not go back to barbarism to get rid of our
smoke and our dirty water, can we go forward and by greater skill
diminish or suppress them? The answer must be “ Yes.” Yet those
only who have to work out the problem know with what difficulty
this answer has in many cases been given, whilst in many it is not
given yet.
The materials which the manufacturer throws away, we have
already classed in correct school-room fashion as solid, liquid, and
gaseous. With the first of these the manufacturer alone is con-
cerned, and it may be safely left in his charge. The more of it he
produces, the more must he expend im its removal, the more land
must he purchase on which to deposit it; and if he throws away
that which is valuable, he is the chief loser. We may, therefore,
safely leave him, with certain reservations, to look after his solid
refuse, knowing that no sharper impulse can be applied to induce
him to diminish its amount, or to save what is valuable in it, than
the spur of self-interest which already exists. We say it may be
safely left in his charge; but if, through some process of fermenta-
tion or change, a portion of it shall slip out of his custody, and
yield, after rain, a noxious liquid to drain into the nearest brook,
or a gaseous escape to contaminate the air around, it falls back into
the two other classes.
For the present we propose to direct attention to the latter of
these two classes only, the gaseous. In doing so, we would first dwell
VOL, VI. 2A
339 Air-pollution by Chemical Works. | July,
on the magnitude of the evil which may and does arise from the
pollution of the atmosphere by gases discharged during the carrying
on of various manufacturing processes; secondly, on the state of
our laws on the subject; and thirdly, as to the direction which
further legislation on the subject should take.
The evils complained of are not uniformly spread throughout
the country, and do not come under the observation of everyone.
Some districts are found to be specially suitable for carrying on a
particular manufacture, so throughout the country we find works of
a certain kind grouped together. Those who reside in the districts
known as “ manufacturing,” are too familiar with the evils arising
from noxious vapours floating in the air to need any setting forth
of their extent, unless indeed familiarity with these evils has dimmed
the perception of their magnitude. In Staffordshire, the so-called
“black” country is a district of many miles in extent, blasted by
the smoke of the iron furnaces; in it not a tree can be found, and
searce a blade of grass. Near St. Helens and Widnes in Lan-
cashire scarce a living tree is seen in the direction towards which
the prevailing winds blow, and in the valley of Swansea, thickly set
with copper works, not only are the hill-sides bared of the green
forests which once waved there, but the underwood, the shrubs, the
hedge-rows, the grass itself is gone, and, to complete the desolation,
when the roots and fibres which permeated the soil died and rotted,
the soil itself, no longer able to withstand the action of the rain,
was also washed away, leaving only bare heaps of stone and gravel.
These, more like huge railway embankments than natural hill-sides,
suffer yet another injury, for the rain, not now absorbed and held
back by tree, shrub, grass, roots, or soil, falls on the bare hill-side,
as on the slated roof of a house, and as quickly runs off it, plough-
ing the ground in its headlong course, making each rippling stream-
let into a torrent even durmg a moderate shower. And still the
desolation is not fully described, for when the even adjustment of
nature is disturbed, who shall say where the derangement will stop?
Here the grass, the soil is gone, and with these the insects and
birds, with the exception of a few sparrows.
The manufacturing processes which may give rise to noxious
vapours are numerous. The French, in the elaboration of their
sanitary code, enumerate seventy-four.
These noxious vapours may do injury of two kinds—injury to
animal life and to vegetation.
Injury of the former class, though real and widespread, is a
matter less easily brought to the measure of money than that of
the second class. People are annoyed at a vile smell arising from
some manufacturing process, and by its continuance are affected in
health, but they do not assess the damage in money and sue for it at
law, except in so far as property is injured. Where, however, in
1870. ] Air-Pollution by Chemical Works. 333
an already populous district a factory is established, the emanations
from which can be proved to be injurious to human health, there
is power for suppressing the nuisance; for, under the Sanitary Act
(18 & 19 Vict., c. 121), the “Local authority, when moved by its
Medical Officer of Health, or by two legally qualified practitioners,
or by ten householders residing in the district in which the nuisance
exists, is bound to complain to the magistrates (two lay, or one
stipendiary) and to prosecute the offenders. The penalty, if the
case is proved, is a fine of from 40s. to 5d. for the first conviction,
102. for the second, and for each subsequent conviction a sum double
the amount of the penalty imposed on the last preceding conviction,
but so that such cumulative penalty do not in any case exceed 2001.”
The operation of the law here is clear, and generally satisfactory.
This clearness, however, ceases when we turn to the working of the
law in cases of injury done to vegetation. The question is not now
whether any damage is done to the farmer’s crops and trees, but
how much; for if an important manufactory is carried on, giving
employment to a large number of workmen, producing articles of
general value, and returning a handsome income to the proprietor,
it would not be wise to put a stop to all this producing power,
because it of necessity entails a small amount of collateral damage.
Rather let those who carry on this lucrative manufacturing busi-
ness compensate those who are injured by it; and consider that
they have only fairly earned that amount which remains, when from
their gross profits they have deducted this charge. In this way
we have a gauge by which to determine the amount of forbearance
which the public shall exercise towards’a manufactory doing obvious
damage to the vegetation around it.
If a factory produces a revenue of 1000J. to its proprietors, and
at the same time injures neighbouring vegetation to the extent of
100/., it clearly does more good than harm. The farmer is com-
pensated, and 900/. is honestly earned after every one 1s satisfied.
Put, however, the figures the other way; suppose the works, while
earning 100/., to do 10002. worth of damage, and the proprietors
compelled to pay this, it will require no injunction from the Court
of Chancery to make them close the works, or else to improve the
manufacturing process so as materially to lessen the damage done.
But we have hitherto considered only the relations of the manu-
facturer and the farmer, imagining the smoking chimney to be sur-
rounded by corn or clover, orchards and hedge-rows. All these
have a known market value, and can be paid for with money. In
place of the farmer, with his marketable crops, imagine him or his
landlord dwelling in the old house of his fathers. The trees which
surround his cottage or his mansion are of ancient growth; the
place is his home. What money shall compensate for its loss? He
may be rich and put little value on pecuniary compensation. He
2A 2
334 Air-pollution by Chemical Works. [ July,
will feel himself grievously wronged when, his trees being killed,
he is offered money in place of them.
This might be said, however, in all cases where the sanctity of
private property is invaded. When a railroad is planned, which is
to carry a nation’s traffic, it will disturb many an ancient hall and
many a cottage home. The money equivalent is paid the owner,
but in his eyes this is often no sufficient compensation. He must,
however, bow to his fate and give way before the greater good of
the many. So in the case where a man sees every year the noble
trees vanish from his land, from the ancient domain that has been
held in quiet enjoyment by his family through many generations,
and feels himself driven from it by the advancing tide of manufac-
turers. He is much to be pitied; for, let him be paid ever so libe-
rally for the damage actually done to the estate, he is not compen-
sated. Yet he must submit and suffer personal loss for the public
benefit.
Fortunately, however, these cases are exceptional; generally
those interested in the land can be fully compensated in money for
all they lose. A farmer, who should get 100U/. for the produce of
his wheat-field, is content if it brings him in only 50/. in the market,
provided he can get the remaining 50/. by way of damages from the
neighbouring chemical manufactory. A question here at once arises,
Will he have much difficulty in obtaining from the manufactory the
50/., the proved amount of his loss? If the manufactory is standing
by itself, he probably will have no great difficulty. If the demand
is resisted, his course at law is plain. He proves that on a certain
day, or on many days, the smoke of the offending chimney was seen
to fall upon his land, that soon afterwards the crops were visibly
injured, in such a way as is known to be caused by chemical smoke ;
he also further proves, by the assistance of agricultural valuers, that
the amount of the damage done is an equivalent of the sum of
money he now claims. This chain of evidence is usually so con-
clusive that the farmer wins the day.
Suppose, however, that in place of one chemical work being
near the farm, there are several in a group, from all of which
the smoke approaches simultaneously. These works may be of
different kinds; there may be alkali-works and copper-smelting
works; glass-works and potteries, with chemical works whose
various processes and products defy enumeration, how shall the
farmer discriminate, or rather how shall he criminate ? how shall
he fix on the culprit among such a motley crowd of evil doers ?
Let us suppose him calling on the first in order, and making his
complaint against him, as the one he thinks most likely to have
been the offender ; the manufacturer explains to him in the clearest
manner that from the nature of the processes he carries on, and the
care with which all injurious vapours are avoided or condensed, he
1870.] Air-pollution by Chemical Works. = gee
cannot have injured the land; perhaps it was his friend of the
neighbouring works, whose processes are different from his own.
Doubtless this gentleman would be equally clear and conclusive
in his explanations, and would pass our farmer on once more, to be
sent in turn from one to the other, but to get redress from none.
The farmer soon learns that the only way in which he can
obtain compensation from any of the chemical manufacturers is to
fix on one of the works, perhaps the one nearest his land, or the
one with the highest chimney, and to watch till he thinks he can
distinguish the smoke from it come upon his farm. On that he
fixes, and, shutting his eyes to the other works and forgetting the
injury they probably do him, charges the proprietor with the whole
of the damage he has sustained. The judges and juries before
whom such eases come for trial are in great difficulty, they know
that the manufacturer in question has not done all the damage
alleged, yet they have no power of apportioning it between him and
other offenders, therefore, as some of the damage has been proved
to come from the defendant’s works they give a verdict for the
plaintiff.
Among chemical works, the largest, and those capable of doing
most harm to vegetation, are the alkali-works. In these works
soda, in its various forms of ash, carbonate, bicarbonate, crystal or
caustic, is extracted from common salt. Common salt consists of
soda in combination with muriatic acid. When it is mixed with
sulphuric acid and heated, muriatic acid is driven off asagas. In
the earlier days of the soda manufacture this acid was considered as
a waste product to be got rid of as speedily as possible. The easiest
way was to let it pass into the chimney and thence into the sur-
rounding atmosphere. Complaints were soon made that trees in
the neighbourhood were injured. The manufacturer therefore
raised his chimney, building it so high that the acid might be carried
away to a great distance by the wind and its effects lost sight of.
The result of this effort was not successful; on wet days the rain
passing through the smoke would wash down the acid and fall in
burning drops even at the foot of the chimney; while on fine days
the smoke would travel farther and though much spread out, still
powerful for evil, would carry on its destruction over a larger
area. A wiser plan was next adopted; by the use of the now famous
Gossage condensing towers the acid vapours were washed out of
the smoke and kept from contaminating the air altogether. Those
alkali manufacturers who carried out this method well sent out
scarcely any acid vapour to damage the farmers’ crops. Some of
the manufacturers, however, were behindhand in the movement,
and either from want of skill or of enterprise, did not condense
their acid vapours. Of the efficiency of this condensation in indi-
vidual cases the farmer could not judge; he found that his crops
336 Air-Pollution by Chemical Works. | July,
were still damaged, and therefore brought his action as before,
ossibly to recover from an innocent party. At this point the
ficken stepped in, and in the Alkali Act of 1863, passed a
measure which has worked well in the interests of both the manu-
facturers and the agriculturists. ‘The Act announces it to be the
duty of the manufacturer to condense 95 per cent. of the muriatic
acid he produces, and fixes a penalty of 50/. for each omission,
raising the penalty to 100/. after the first conviction. Inspectors
are appointed, whose duty it is to visit the works from time to
time and ascertain that the provisions of the Act are carried out.
It should be noticed that the Legislature in passing this Act stepped
out of its accustomed course. The common law maxim is that for
every injury a man may receive he has his remedy against some
one. He must, however, receive the injury before he can seek his
remedy ; but in this case, asit already has been shown, much injury
may be done which has no remedy. Who can replace an oak tree
of 100 years’ growth and restore the waving woods which adorned
the hill side? The law therefore here steps in beforehand, and no
sooner does the Inspector find that 95 per cent. of the acid is not
condensed, than he stops the process under the penalties mentioned.
The new law has been found to work very well, it has enforced the
condensation of muriatic acid to the benefit both of the manu-
facturer himself and of the public. It has protected the agricul-
turist against the manufacturer, and the manufacturer against the
agriculturist. The Inspector is received as a friend by both sides ;
he protects the farmer’s interests by enforcing care on the part of
the manufacturer, and he protects the manufacturer’s interest by
proclaiming the extent to which he carries the suppression of
noxious vapours. ‘The Act has had the effect of bringing up the
hindermost manufacturer to the rank of the most skilful. Before
this legislation took place many manufacturers condensed a portion
of their muriatic acid; now they all condense not a small portion
only, but fully 95 per cent., some indeed habitually condense 99
per cent. The manufacturer finds the visits of the Inspector an
assistance to him in keeping his condensing apparatus in efficient
order ; and an amount of acid escaping which would pass unnoticed
by the master or his workpeople is detected by the Inspector. It
should be understood that to point out leakage of muriatic acid is to
point out waste, for this acid is needed in the manufacture of bleaching
powder, and other products. The amount of acid thus saved by
the operation of the Act is very large. One manufacturer sells
muriatic acid annually to the amount of 1500/.—acid which pre-
vious to the passing of the Act was sent up the main chimneys of
the works to the destruction of all surrounding vegetation.
It may now be asked in general terms, has the Alkali Act, this
somewhat experimental law, succeeded ; does it accomplish the work
1870. ] Air-Pollution by Chemical Works. 337
it was intended to do? The reply is that it has done all and
more than its promoters or those who understood its provisions ex-
pected; but probably the public generally are not satisfied; they
fail to understand that a law which professes to shield them from
muriatic acid cannot also defend them from chlorine, sulphurous
acid, sulphide of hydrogen, and the host of nameless gases by which
their noses and their gardens are assailed ; still less can they under-
stand that an Act which should prevent the emission of muriatic
acid from the chimney of an alkali works, cannot also prevent the
escape of the same acid from copper-extracting works, a bottle
factory, or a pottery.
The Act must, however, not be blamed for omitting to do that
which it was never framed to accomplish ; let us be glad that a step
has been gained, that one noxious gas has been measured and sup-
pressed.
Some instances have occurred where manufacturers who are
not alkali makers have desired to place their factories under the
Inspector appointed under the Alkali Act. Their object being first
to know if, in his opinion, they were sending out an injurious amount
of noxious vapour, then, having diminished it so as to meet with
his approval, to gain his advocacy and defence when harassed by
their natural enemies the farmers. This has brought a certain
amount of volunteer work on the Inspectors, which they have cheer-
fully borne on account of the obvious good they could accomplish, by
diminishing on the one hand the escape of noxious acids, and pre-
venting litigation on the other.
In districts such as that around St. Helens, in Lancashire,
where alkali-works and copper-smelting works are found together,
the copper smelters look somewhat enviously at the alkali makers.
Before the passing of the Alkali Act, the farmers who thought
they had suffered loss through the mjury of their crops by acid
vapours, charged the damage sometimes against the alkali-works
and sometimes against the copper-works. Now, however, owing to
the improvements which have been made in the alkali-works under
the stimulus of the Act, and supposing the manufacturers to be
somewhat protected by it, the landholders direct their attacks ex-
clusively against the copper smelters. The amounts claimed by
each farmer are not always large, but the aggregate has reached
30002. a year against the six copper-works.
Besides these smaller claims an important action was lately
brought by the proprietor of an estate three miles from St. Helens
against a copper smelter, for damage done to his trees and crops by
the smoke from the works. The course the action took, so well
shows the present working of the law, and indicates perhaps the
direction in which it could be amended, that it might be well to give
some account of it here.
338 Air-pollution by Chemical Works. [ July,
The plaintiff proved he had received damage from smoke coming
from the direction of the defendant’s works, and alleged that the
damage he had sustained was wholly done by them, intimating that
if he gained a verdict in the present suit he should apply to the
Court of Chancery for an injunction to restrain the carrying on of
the works altogether, as he believed he would then be free from all
damage. In defence it was pointed out that the defendant’s works
lay in a straight line between the plaintiff's land and St. Helens, so
that the same wind which brought defendant’s smoke would also
convey the smoke from a large portion of St. Helens, and that in
general, as the plaintiffs park was subject to injury from all the
factories in the neighbourhood, it was unjust to charge the whole
damage upon the defendant.
It will be seen that the following question would at once pre-
sent itself :—Is it possible to determine the amount of damage which
each factory in a district contributes towards the damage done by
all ?
In other words, if a farmer sustains a loss of 100/. through his
crops being injured by the accumulated smoke of a manufacturing
district, is it possible to set down to each manufacturer the amount
which he ought to contribute towards this 1002. ?
Turning to the fifth of Dr. R. Angus Smith’s very able reports
under the Alkali Act, we find this question anticipated and an answer
given. Referring to the amount of acid vapours thrown up with the
smoke of factory chimneys, he says at page 25 :—“ Now it is easy to
estimate this amount, and it is easy to put down to every one in the
district the exact share of guilt so far as the acid is concerned. ... .
Perhaps we may also bring in the element of distance.”
In consequence of this Mr. Alfred E. Fletcher, the Inspector
under the Alkali Act for the district which includes West Lancashire,
was asked to apply himself to the question. He had to consider:
1st. The distance of each factory from the injured land.
2nd. The rateat which the increase of distance diminishes the
power of the smoke to do damage.
3rd. The number of days throughout the year on which the
wind blows from each point of the compass.
4th. The amount of acid vapour discharged from each factory
in a given time.
First, the distances; these are easily measured on the map.
Information on the second point was obtained in the following
manner. Ata time when the ground was covered with snow for a
week, lines were drawn, in a direction following the wind, from St.
Helens and from other groups of works, to a distance of two or
three miles. At each half-mile a sample of the surface snow was
collected and brought home for analysis, Also during a period of
rain, collecting vessels were set at regulated distances from a group
1870. ] Air-pollution by Chemical Works. 339
of works. A determination was then made of the amounts of mu-
riatic and of sulphuric acids collected by the snow and by the rain,
and these were compared with the distances at which the samples had
been obtained. It was seen that the amounts diminished in even
ratio with the increase of distance. Probably a sufficient number of
experiments of this nature have not yet been made, firmly to esta-
blish the law; for the undulations of the ground, the position of
trees, and any objects which interfere with the uniform motion of
the air, affect the even deposition of the acid vapours. More ex-
periments, it was said, were about to be undertaken in order to esta-
blish the law on a wider basis. Information on the third point may
be usually obtained at some neighbouring observatory. In the case »
of St. Helens the returns of the direction of the wind, published at
the Liverpool Observatory, on Bidston Hill, were depended on.
Fourthly, the amount of acid vapour discharged from each factory
in a given time can be known by periodical examination of the gases
which are passing up the various chimneys of the works. This is
already done as far as the alkali-works are concerned under the pro-
visions of the Alkali Act. In the cases of copper-smelting works,
elass-works, and others where systematic inspection has not been
carried on, the amounts of acid vapour thrown into the air can be
calculated from the materials used in the manufacturing processes
carried on.
The acid vapours discharged from the various works in the
St. Helens district are:—From ten alkali-works,—muriatic acid,
sulphuric acid, sulphurous acid, nitrous acid, chlorine, coal smoke ;
from nine glass-works,—muriatic acid, sulphuric acid, sulphurous
acid, vapour of common salt, coal smoke; from six copper-smelting
works,—sulphuric acid, sulphurous acid, coal smoke; from six col-
lieries, six iron foundries, two soap-works, 8000 dwelling-houses,
—coal smoke; from the Sankey Brook and the heaps of alkali
waste,—sulphide of hydrogen.
This is a formidable list, but the amounts of each may be calcu-
lated with a very near approach to accuracy, except the last item,
the sulphide of hydrogen, which varies continually with the amount
of rain-fall, and with the temperature of the air.
Having, then, collected the information as set forth under these
four heads, it became merely a question of figures to apply it to the
solution of the problem raised in the St. Helens law-suit. A list
was made out of the principal factories in the district capable of doing
injury to the plaintiff's land. Opposite these was set down the dis-
tance of each factory from the land and, in a parallel column, the
amount of acid vapour thrown up by each. On dividing the figures
in the second column by those in the first, numbers were obtained
which were proportioned to the share each one had contributed to
the total damage done by all to the plaintiff’s land.
340 Air-pollution by Chemical Works. [ July,
Further, a method was adopted by Professor Roscoe, of Owen’s
College, Manchester, which confirmed the accuracy of this calculation.
St. Helens lies, as has been said, three miles from the plaintiff’s
park, defendant’s works being half-way between them.
While the snow lay on the ground last February, the wind
blew mainly from the east. Professor Roscoe then took samples of
the snow lying three miles west of St. Helens, and also some of
that lying a mile and a half west of defendant’s works, that is, the
same distance to the west as plaintiff’s land is to the south-south-
east. He found that the proportion of the amount of acid con-
tained in the one to that contained in the other, agreed closely with
the proportion determined by Mr. Fletcher in the previous calcula-
tion. This was given as evidence at the trial, and it appears that
the jury acted on the principle here laid down, that a manufacturer
should only be called on to pay in proportion to the amount he
contributes to the total damage sustained, and that it is possible to
ascertain what that amount should be. Since this trial two other
similar cases have been decided by arbitration, in each of them the
arbitrator showed by his award that he adopted the principles here
set forth.
Having now given some account of the working of the Alkali
Act, the most recent legislation on the difficult subject of air-
pollution, and sketched the action of the law courts when mat-
ters of the kind are brought before them, it may be desirable to
discuss the course which further legislation should take in the
matter.
As regards the present Alkali Act, we would object that though
successful it is too limited in its application.
Secondly, the onus of carrying out its penal clauses rests on the
Inspector. We should havea noxious vapour Act applicable to every
mantfacture where injurious gases are thrown off. The duty of the
Inspector should be solely to imspect and to publish the results of
his inspection—the public should be the prosecutors.
Let us follow the working of such an Act. In every district
its Inspector would, from time to time, publish a list of the works,
together with the amounts of acid or other vapour escaping from
them. This would be given either as the amount in 1000 cubic
feet of the chimney gases, or the actual amount by weight of that
which escapes per month or per annum. The result of this to the
manufacturers would be that they would anxiously consult the
published list and exercise a wholesome rivalry as to who should
stand well in it. Moreover, these lists would form the basis for
assessment of damages in case of claims made by the neighbour-
ing farmers. A pecuniary stimulus would thus also be given.
To the neighbouring farmer or landholder these lists would be in-
valuable; they would show him where to apply with the best
1870.] De Mortuis. 341
chance of success for compensation for proved loss by noxious
vapours; or enable him to apportion his claim among several
works, in proportion to their places in the list and their relative
distance from his land.
Thus in place of the goading influence of a few isolated and
sudden prosecutions, a gradual pressure onwards would be felt, a
constant stimulus to improvement. All chemical manufactures can-
not be embraced in the provisions of an extended Alkali Act until
for each separate noxious vapour a process of suppression can be
described, and a limit for its working defined. But with such an
arrangement as is here proposed, all noxious vapours without the
task of enumeration would be at once legislated for. If there are.
several manufacturers carrying on the same processes in the same
district, and one of them by special ingenuity discovers some pro-
cess by which a large portion of the acid vapour he has hitherto
sent away may be condensed, he improves his place in the Uist, and
so enjoys immunity from actions for damage on the part of the
farmers. The other manufacturers would obviously be compelled
to follow him in the race of improvement. Thus all would be
brought up to the rank of the foremost, and there would bea con-
stant impulse to the manufacturer to reduce the noxious emanations
from his works within the smallest possible amount.
VY. DE MORTUIS.
By Henry Woopwarp, F.GS., F.Z.8., &.
In almost all countries, both among savage and civilized races, the
rites of sepulture have been looked upon as a debt so sacred that
those who neglected it were considered infamous.
The Greeks and Romans believed so strongly in the importance
of this obligation that they considered it to be fatal to their admis-
sion into Hlysium to neglect to do honour to the dead.
Nor can the practice of honouring the dead be claimed by these
classical countries alone, for throughout Egypt, Palestine, Persia,
India, and China, are monuments of the most lasting and costly de-
scription raised to the mighty dead.
That the more northern and western races of mankind possessed
the same traditions cannot be doubted, and although their monu-
ments are of a ruder character they display often a vast amount of
labour in their construction, and an equal care for the departed
whose remains they were intended to preserve.
On the rude but colossal “ Megalithic Structures of the Channel
Islands, their History and Analogues,” a very able and exhaustive
342 De Mortuis. [ July,
article by Lieut. 8. P. Oliver, Royal Artillery, F.R.S., appeared in
the ‘Quarterly Journal of Science’ for April last, to which it is only
needful here to refer our readers.*
Fortunately for the archeologist the uninviting exterior of these
northern and western tombs has been, until of late years, a means
of protecting them to a great extent from pillage; for within these
rounded dome-like hills of earth (Tumuli) are often discovered relics
of a period so remote that, save for these sacred depositories, we
never could have hoped to obtain any reliable information of the
builders, or to have learnt aught of their advance in civilization, or
of the arts they practised.
The rich and varied discoveries of the Swiss Lake habitations
indeed, have thrown much new light upon the early history of
Europe, yet many writers have nevertheless concluded that these
remains are, after all, not much more than two thousand years old,
seeing that similar lacustrine habitations were known to Hippocrates
(z.c. 460), and Herodotus (z.c. 404). But the careful researches
of Prof. Keller, and many other investigators, prove beyond ques-
tion that these settlements go back to the early Neolithic period, if
not to the paleolithic.
In speaking of the ages of Stone, Bronze, and Iron, however, we
should always guard against the notion that, at any one time, save
in the very earliest palzeolithic stage, one material for the manufac-
ture of implements was used exclusively over the whole of the
Continent. Not only does the “Iron age” stretch from our own
time back to an antiquity more remote than Nineveh, but the
“ Bone age” is still extant and has overlapped all the other divisions,
for horn and bone are still used by civilized man, and our most re-
mote ancestors we know discovered the economic value of the bones
and horns of the first animals they slew in the chase.
Therefore in the examination of all early remains many collateral
circumstances must be taken into account before we can justly assign
an approximate date to any discovery. or instance, if we grant
that the civilization of man actually ran its course through these
periods, just as they are mentioned above, yet it is certain that the
Bronze period of Northern Europe by no means agrees in time with
that of the middle and southern parts of this Continent.
Again, the Bronze age of Greece and Italy may be separated by
centuries from that of Egypt, which we may consider as the cradle
of western civilization. —
We may safely conclude, as the Danish antiquaries themselves
allow, that in the Scandinavian countries stone implements were for
a length of time used while the Bronze period was in full activity in
the more southern lands, and that Egypt, whose oldest monuments
indicate very clearly the use of i iron, and also Greece, had both ad-
* Vol. vii., p. 149.
1870. | De Mortuis. 343
vanced to the Iron period when Central Europe was in the Bronze
age. If, therefore, according to the testimony of ancient authors
and monuments, bronze and iron were used in the earliest ages in
the countries round the shores of the Mediterranean, the commence-
ment of these periods in the inland and northern parts of Hurope
was regulated entirely by the greater or less amount of intercourse
between these countries and those to whom we are indebted for a
knowledge of metals, so essential to civilization. We may even at
the present day observe a similar irregularity in the distribution of the
products of higher civilization and art. Nor do these divisions give
us any positive certainty ; for in very few burial places or early
settlements are the remains found so purely distinctive as to enable
us conclusively to attribute them to any one of the three periods.
It seems very certain that there was no hard line of demarcation
between the three periods, but that the new materials were spread
abroad like any other article of trade, and that the more useful tools
gradually superseded those of less value.* |
We should hardly, writes Sir John Lubbock,} have hoped to
ascertain much of the manner in which the people of the Bronze
age were dressed. Considering how perishable are the materials
out of which clothes are necessarily formed, it is wonderful that any
fragments of them should have remained to the present day. There
can be little doubt that the skins of animals were extensively used
for this purpose, as indeed they have been in all ages of man’s
history; many traces of linen tissue also have been found in English
tumuli of the Bronze age and in the Swiss lakes. Even a single
fragment throws much light on the manufactures, if we may call
them so, of the period to which it belongs; but fortunately we need
not content ourselves with any such partial knowledge as this, as
we possess the whole dress of a chief belonging to the Bronze age.
On a farm occupied by M. Dahls, near Ribe, in Jutland, are
four tumuli, known as Great Kongehoi, Little Kongehoi, Guldhoi,
and Treenhoi. This last was examined in 1861 by MM. Worsaae
and Herbst. It is about 50 ells in diameter and 6 in height, being
composed of a loose sandy carth. In it, near the centre, were found
three wooden coffins, two of full size, and one evidently intended
for a child. The coffin with which we are now particularly con-
cerned was about 9 feet 8 inches long and 2 feet 2 inches broad
on the outside; its internal measurements were 74 feet long and
1 feet 8 inches broad. It was covered by a movable lid of corre-
sponding size. ‘The contents were peculiar and very interesting.
While, as might naturally be expected, we find in most ancient
graves only the bones and teeth, all the soft parts having long ago
decayed away, in some cases—and this was one of them—almost
* Keller’s ‘ Lake-Dwellings:’ translated by J. E. Lee, F.S.A.
+ ‘ Pre-historic Times.’
344 De Mortuis. [July,
exactly the reverse had happened. Owing to the presence of water,
and perhaps to the fact that it was strongly impregnated with iron,
the soft parts of the body had been turned into a dark, greasy,
substance (adipocere ?); and the bones, with the exception of a few
fragments, were changed into a kind of powder.
Singularly enough, the brain seems to have been the part
which had undergone the least change. On opening the coffin it was
found lying at one end, where no doubt the head had originally
been placed, covered by a thick hemispherical woollen cap, about
6 inches in height. ‘The outer side of the cap was thickly covered
by short loose threads, every one of them ending in a small knot,
which gave the cap a very singular appearance. The trunk of the
corpse had been wrapped in a coarse woollen cloak, which was
almost semicircular, and hollowed out round the neck. It was about
3 feet 8 inches long, and broad in proportion. On its inner side
were left hanging a great number of short woollen threads, which
gave it somewhat the appearance of plush. On the right side of
the corpse was a box, closed by a lid, 74 inches in diameter, 64
inches high, and fastened together by pieces of osier or bark. In
this box was a similar smaller one, without a lid, containing three
articles, namely, a cap 7 inches high, of simply woven woollen stuff ;
a small comb, 3 inches long by 25 inches high; and a small simple
razor-knife. ‘The coffin also contained two woollen shawls, one of
them covering the feet, the other lying higher up; they were square
in shape, 5 feet long, 3 feet 9 inches broad, and with a long
fringe.
‘At the place where the body had lain was a shirt, also of woollen
material, cut out a little for the neck, and with a long projecting
tongue at one of the upper angles. It was fastened at the waist by
a long woollen band, which went twice round the body, and hung
down in front. On the left side of the corpse was a bronze sword
in a wooden sheath, 2 feet 3 inches in length, having a solid simple
handle. At the feet were two pieces of woollen stuff about 144 inches
long and 34 inches wide, the use of which does not seem quite clear,
though they may be supposed to be the remains of leggings. At
the end of the coffin were found traces of leather, doubtless the
remains of boots. In the cap where the head had been was some
black hair; and the form of the brain was still recognizable. Finally,
this ancient warrior had been wrapped round in an ox’s hide, and
so committed to the grave. The other two coffins were not examined
by competent persons, and the valuable information which they
might have afforded is lost to us. The more indestructible things
were, however, preserved; they consisted of a sword, a brooch, a
knife, a double-pointed awl, a pair of tweezers, a large double button
or stud, all of bronze; a small double button of tin, and a javelin-
head of flint.
1870.] De Mortuis. 345
The “ Kongehoi” contained four wooden coffins, in which were
bodies clothed in woollen garments, a bronze sword in a wooden
sheath ornamented with carvings, two bronze daggers, a wooden
bowl ornamented by a large number of tin nails, a vase of wood,
and a small box of bark.
There can, therefore, be no doubt that these very interesting
tumuli belonged to the Bronze age, and I am inclined (says Sir
John Lubbock) to place them somewhat late in the period, partly
on account of the knife and razor-knife, both of which are forms
referable to the close of the Bronze period, and to the beginning of
that of Iron. Bronze brooches are also very rarely found in the
Bronze age, and are common in that of Iron. The sword, again, ©
belongs to a form which Professor Nilsson regarded as being of late
introduction. The mode of interment may also be regarded as
unusual in the Bronze age, though commonly so found in inter-
ments of the Iron age.
In Denmark cremation appears to have been all but universal,
and seems plainly to betoken the south-eastern origin of the peoples
who practised it. Bateman and Sir R. C. Hoare, record a number of
instances of graves opened by them in England containing objects
in bronze which well illustrate the prevalence of burning the dead :—
Position
Body contracted. Burnt. Extended. Facets,
Number of cases.. 19 a 59 aA 7 ig 15
Canon Greenwell also mentions that out of 100 interments with
bronze ornaments, &c., examined by him, all were either burnt or
the body was placed in a sitting posture. Of the wide-spread practice
of interment in a sitting posture, we may find abundant instances
in Wilson’s ‘ Pre-historic Man’ Thus* in opening a Peruvian tomb
it is stated “the male mummy was that of a man in the maturity
of life, en the usual setting position, with the knees drawn up to the
chin.” We should certainly consider this mode of interment to be
the most primitive.
If ornaments, weapons, or coins in any number, be found in the
erave, or if much labour has been bestowed upon its construction, we
may justly infer that, to whatever period the grave may belong, it was
the last resting-place of a chief or warrior of the tribe; for the same
causes which operate now to deter the poorer classes from a lavish
expenditure upon the dead, acted in early times still more strongly,
when every article of dress and every weapon being required for
daily use were of so much greater intrinsic value, and consequently
the devotion which instigated their dedication to the use of the de-
parted must have been either the result of strong attachment, or a
display of the affluence of the family to which the deceased belonged.
There can be no doubt that the introduction of Christianity was
* At p. 440.
346 De Mortuis. [July,
the means, not only of putting an end entirely to the practice of
incremation, but also to a great extent to that of depositing votive
offerings in the graves of the departed. The introduction of such
sentences as those which our burial-service contains, against the
thought that we can take anything with us out of the world,
evidently when introduced by the early Church had reference to the
heathen practice of placing objects highly esteemed in the grave with
the dead.*
Schiller’s lines (translated by Lytton) well express this practice
so common among the aborigines of our own day :-—
* Here bring the last gifts! and with these
The last lament be said ;
Let all that pleased, and yet may please,
Be buried with the dead.
Beneath his head the hatchet hide
That he so stoutly swung ;
And place the bear’s fat haunch beside—
The journey hence is long!
And let the knife new sharpened be
That on the battle-day
Shore with quick strokes—he took but three—
The foeman’s scalp away !
The paints that warriors love to use,
Place here within his hand,
That he may shine with ruddy hues
Amidst the spirit-land.”
It not unfrequently happens that fragments of the bones of
sheep and other animals are found in cinerary urns associated with
the human remains. This is easily explained when we consider the
manner in which the rites to the dead were performed.
If the dead person were a chief or warrior of note, it was usual
to erect a funeral pyre of great size, upon which the corpse was
laid, surrounded by the bodies of various animals slain in honour of
the dead, together with costly unguents and perfumes. Frequently
a number of slaves and captives were also sacrificed to the manes of
the departed. Thus, in Homer’s ‘ Iliad,’ we have a graphic descrip-
tion of the death of Patroclus during the Trojan war, and the
honours paid to his body by Achilles and the Greeks :— 3
“ While those deputed to inter the slain
Heap with a rising pyramid the plain.
A hundred feet in length, a hundred wide,
The growing structure spreads on every side;
High on the top the manly corse they lay,
And well-fed sheep and sable oxen slay :
Achilles covered with their fat the dead,
And the pil’d victims round the body spread ;
* Rolleston ‘ Archzologia,’ vol, xlii.
1870. ] De Mortuis. 347
Then jars of honey, and of fragrant oil,
Suspends around, low-bending o’er the pile.
Four sprightly coursers, with a deadly groan
Pour forth their lives, and on the pyre are thrown,
Of nine large dogs, domestic at his board,
Fall two, selected to attend their lord,
Then last of all, and horrible to tell,
Sad sacrifice! twelve Trojan captives fell.
On these the rage of fire victorious preys,
Involves and joins them in one common blaze.”*
During the ceremony, decursions and games were celebrated,
often lasting several days, after which the osselegiwm, or gathering
of the bones and ashes of the dead, washing, anoimting, and deposit-
ing in urns, was performed. ;
Amongst refined and civilized peoples it is possible to conceive
that a certain sacredness was connected with this ceremonial, and
that such lines as the Salve Eternwm might form an appropriate
conclusion of such service :—
“Farewell, O soul departed !
Farewell, O sacred urn !
Bereaved and: broken-hearted,
To earth the mourners turn !
To the dim and dreary shore,
Thou art gone our steps before!
But thither the swift hours lead us,
And thou dost but awhile precede us !
Salve—Salve !
Loved urn and thou solemn cell,
Mute ashes !—farewell, farewell!
Salve—Salve ! +
But the incremation ceremony in western and northern Europe
was in reality more an occasion of feasting ; the slain animals being
chiefly cooked and eaten by the mourners. Thus we find in Anglo-
Saxon barrows and graves in England abundant remains of animals,
especially those of the horse, which have served as feasts.
To so high a pitch had this practice of the lyke-wake risen in
later times that it was severely denounced in numerous inhibitions
issued by the early Church.t}
Judging by the number of instances in which gold ornaments
have been found in graves, it seems probable that gold was the metal
which first attracted the attention of man. Its bright colour would .
certainly attract even the rudest savages, who are known to be very
fond. of personal decoration.
Silver does not appear to have been discovered until long after
gold, and was apparently preceded by both copper and tin, as it is
rarely, if ever, found in tumuli of the Bronze age; but however
this may be, copper seems to have been the metal which first became
of real importance to man; no doubt owing to the fact that its ores
* Pope’s Translation of the ‘ Iliad,’ Book xxiii.
+ ‘Last Days of Pompeii :’ Lytton.
t See Rolleston in ‘ Archeologia,’ vol. xlii.
VOL. VI. 2B
348 De Mortuis. [ July,
are abundant in many countries, and can be smelted without dit
ficulty ; and that, while iron is hardly ever found except in the form
of ore, copper often occurs in a native condition and can be beaten
at once into shape.*
There is no reason to suppose that the mound-builders, whose
earth-works occupy leagues in extent in the valleys of the Mississippi
and Ohio, were acquainted with the art of smelting copper; that
they mined it extensively on the shores of Lake Superior, and
wrought it into knives, spear-heads, chisels, and bracelets, and other
personal ornaments there can be no reasonable doubt, but having
no tin, they could not, like the ancient dwellers of the Swiss lakes,
Denmark, &c., impart to the alloy almost the hardness of steel. It
is doubtful, even, whether their metallurgic art extended to the smelt-
ing of copper; ‘for it often happens that the native copper of Lake
Superior encloses native silver, both metals existing side by side
chemically pure, which, if smelted, in whatever proportions, would
form a homogeneous compound. Bracelets have been found in the
mounds, in which this peculiarity is preserved, thus showing that
the material had not been sme!ted but simply hammered cold ; and
the ends are brought together by bending, without any evidence of
having been soldered.
Of the amount of gold found in the Chiriqui graves in Central
America probably no just estimate can be obtained. At the period
of Mr. Power's visit in August, 1859, about 250 lbs. weight of gold
had been extracted from the huacas at Bugabita, two-thirds being
tolerably pure gold, the remaining third what is called “ guanin,”
or gold alloyed with copper; the value of the whole was about
12,5007. In the summer of 1861, some fresh tombs were discovered
from which gold objects to the value of 16,0002. had been extracted.
Although, as must necessarily happen, these interesting remains
find their fate in the melting-pot wholesale, there are yet to be seen
in the Blackmore Museum at Salisbury, the Christy Museum, Vic-
toria Street, the British Museum, and elsewhere, many examples of
these curious American antiquities,
From a careful examination of many of the Ohio mounds and a
comparison of their characteristics with ancient Scandinavian tumuli,
it seems highly probable that, in some instances at least, the tomb
was formed by covering the dwelling in which the dead man had
lived with a mound of earth or a cairn of stones.
This would explain the curious sorted condition of many remains
in the American mounds. ‘Thus in mound No. 8, “ Mound City,”
may have been buried the body of some celebrated pipe-maker, with
all his stock-in-trade, which his friends no doubt believed he would
* Lubbock, ‘ Pre-historic Times,’ pp. 3-4.
+ Foster’s ‘ Mississippi Valley,’ p. 423. -
t ‘Flint Chips, by E. T. Bicgone pp: 285-6.
1870. ] De Mortuis. 349
find valuable to him for barter in the land of spirits as he had done
in this world. In others the stock of arrow-heads was so enormous
we may well suppose the occupier of the mound had been a maker
of flint arrow-heads.
The practices of modern savages often throw great light upon
these difficult points. |
Thus we find among the New Zealanders, if the owner dies, he
is commonly buried in his house with all it contamed.* The islanders
of Torres Straits also used their dwelling-huts as dead-houses.t
It is still more significant that the Esquimaux themselves frequently
leave the dead in the houses which they occupied when alive.
We cannot, says Sir John Lubbock, compare the plan of a Scan-
dinavian “ passage-grave ” with that of an Esquimaux snow-house,
without being struck with the great similarity existing between them.
Under these circumstances there seems much probability in the
view advocated by Professor Nilsson, the venerable archeologist of
Sweden, that these “ passage-graves ” are a copy or adaptation of the
dwelling-house ; that the ancient inhabitants of Scandinavia, unable
to imagine a future altogether different from the present, or a world
quite unlike our own, showed their respect and affection for the dead
by burying with them those things which in life they had valued
most ; with women their ornaments, with warriors their weapons.
They buried the house with its owner, and the grave was literally
the dwelling of the dead.§
From the foregoing premises we may venture to establish this
axiom, namely, that any people who accompanied the rites of inter-
ment of their dead by such evident indications of care and attention
as we find ina vast number of graves belonging to different periods
and races in Western Europe and America, may be safely concluded
to have possessed a notion of a future state, whatever may have been
the name they ascribed to it; and moreover they must have also
believed it possible, by their gifts and good offices, to assist their
departed friends into the spirit land.
* Tylor, ‘ New Zealand and its Inhabitants,’ p. 101.
+ M‘Gillivray, ‘ Voyage of Rattle-snake,’ vol. ii., p. 48.
{~ Ross’ ‘ Arctic Expedition,’ 1829-33, p. 290.
§ Lubbock, ‘ Pre-historic Times,’ pp. 126-7.
( 3850 ) [July,
VI. FOREIGN TREES AND PLANTS FOR ENGLISH
GARDENS.*
By Aurrep W. Bennyert, M.A., B.Sc, F.LS.
THE introduction of new forms of vegetable life into our gardens and
greenhouses has made considerable progress during recent years.
The Acclimatisation Societies of Paris and London have, it is true,
paid more attention to the domestication of foreign animals than of
plants; something, however, has been attempted in this direction,
and with considerable success. This branch of acclimatisation would,
indeed, seem likely to be the most fertile in results beneficial to
mankind. For one fresh animal introduced that will be of real
utility, there will probably be a dozen plants that yield important
economical products. ‘The early races of mankind appear to have
exhausted our powers over the lower animals—the horse, the ass,
the dog, the camel, the ox, the sheep, were all brought under sub-
jection to man at the earliest period of his history ; and within his-
toric times no important addition has been made to the number of
our domestic animals. Not so with plants. A large number of
the vegetable substances used as food at the present day, and of the
vegetable articles of manufacture, were unknown to the ancients;
and the field for further extension of our utilisation of the vege-
table kingdom seems indefinitely large. ‘The power of cultivation
in modifying plants is also much greater than any corresponding
power of domestication in modifying animals. The oldest extant
drawings of the horse, the ox, or the camel, scarcely point out any
distinctive features from their descendants now living; the potato
and the apple, on the other hand, may almost be considered as ma-
nufactured products; while many gardeners’ flowers, such as the
Pelargonium and the Tulip, differ so widely from their ancestors as,
in some cases, to obscure their parentage. The term Acclimatisation
has been objected to by some scientific men, on the ground that the
descendants of any animal or plant which has been transported from
one climate to another have no more power than their ancestor of
adapting themselves to that climate, unless the principle of Natural
Selection has come into play to eliminate the individuals least able
to adapt themselves to the new climate, those only surviving which,
from some cause or other, are most suited to the fresh conditions. Be
this as it may, there is no question about the fact that the farmer
* ‘The Planter’s Guide: Trees and Shrubs for English Plantations.’ By
A. Mongredien. London: J. Murray. 1870.
‘Alpine Flowers for English Gardens.’ By W. Robinson, F.L.S. London:
J. Murray. 1870.
‘Dendrologie: Baume, Straucher, und Halb-straucher welche in Mittel oder
Nord-Europa im Freien kultivirt werden. Kritisch bearbeitet von Karl Koch.
Erster Theil. Erlangen. Enke, 1869.
1870.| Foreign Trees and Plants for English Gardens. 351
and the gardener have it in their power to naturalise plants foreign
to our climate and our soil.
But the conditions of this naturalisation are by no means so
simple as might at first sight appear. It might naturally be sup-
posed that all we have to do is to introduce those plants which grow
spontaneously in a climate and a soil similar to our own, and that
they will necessarily flourish, and will scarcely be aware of the change.
Or, if they come from a warmer country, that all that is needed is to
protect them by glass and artificial warmth from the inclemency of
our winters. But in practice this is not found to be the case. A
plant will frequently obstinately refuse to become naturalised in a
country, the climatal and geological conditions of which are similar
to those that occur in the region where it is indigenous. Our
common daisy, a native of almost every country of Europe, is said to
have resisted all attempts to introduce it even into the gardens of the
United States. Some plants seem to have an unconquerable aversion
to the fostering hand of man, even in their own country. A well-
constructed and carefully-kept fernery will contain specimens, more
or less luxuriant, of nearly all our native ferns; the polypody and
hartstongue from shady banks and tree-stumps; the so-called male
and female ferns from the woods; the spleenwort from dry walls;
even the royal “ flowering-fern” from bogs; and some of the semi-
alpine species will flourish with the exercise of a little care. One
kind, however, is almost invariably absent, and that the most widely
distributed of all our ferns, the common brake, a native of every county
and almost of every parish in the country, but which can seldom
be induced to remain a denizen of soil that has once been brought
under man’s dominion. On the other hand, some of the greatest
favourites of our gardens, which display no coyness whatever in over-
running our flower-beds, are natives of countries where the climate
presents very different features to our own, or of very limited tracts
of our own country, to which they seem strictly confined by impas-
sable barriers of soil or meteorological conditions. To take instances
of the latter phenomenon :—There is no garden flower more cos-
mopolitan in its tastes, more certain to thrive under any conditions
of light or heavy soil, sun or shade, care or neglect, even in the
heart of a town, as its very name seems to indicate, than the London
Pride. Yet the Saaifraga umbrosa is one of the most restricted
in distribution of our native plants. Abundant enough where it
does grow, it is yet entirely confined to the moist equable climate
of the hilly country in the south-west of Ireland and a few other
similar localities, beyond which it is never found in the wild state.
Botanists will think themselves amply repaid for a toilsome day’s
march by gathering the beautiful Polemoniwm ceruleum in its
native habitat among the calcareous hills of the west of Yorkshire ;
yet the Jacob’s Ladder is an ornament of every garden on the very
3952 Foreign Trees and Plants [ July;
stiffest part of the London clay. Probably every piece of cultivated
ground, which contains a laburnum tree, produces each spring a
plentiful crop of self-sown young trees, which come up without
the least care or protection until destroyed in the process of weed-
ing; yet the laburnum shows no disposition to take a place among
the naturalised trees of our woods and hedges, although the seeds
must often be carried there by birds. It is remarkable that many
of our common vegetables, the cabbage, the asparagus, the sea-kale,
the celery, are natives of our own shores, never growing sponta-
neously out of reach of the salt spray; and yet requiring, when
transplanted into our gardens, no peculiarity of soil or treatment to
enable them to support a vigorous existence. These are instances of
plants to which our climate appears entirely congenial, and yet which
seem as if they could not propagate themselves with us or spread,
except under man’s protection. Others, again, appear to require only
to get a footing in a foreign soil to become established in it with
extraordinary rapidity, even to the overmastering or expulsion of
some of the indigenous inhabitants. When Australia and New
Zealand were first colonized by Europeans, their flora presented an
aspect of perfect strangeness, very few of the native trees or flowers
belonging even to genera common to Europe. ‘The seeds of some
of our English weeds were, however, introduced, intentionally or
accidentally, by the early settlers; and now the thistle covers the
waste lands of Australia as it does in England, and the clover and
the groundsel everywhere remind the Englishman of his far-away
home, and have become as completely at home as the mustangs or
wild-horses on the pampas of South America. In our own country
a very remarkable instance of this rapid naturalisation has occurred
in the case of the Hlodea canadensis or Canadian water-weed ; which,
introduced not many years since into our canals from Canada, has
now become such a pest in many places as seriously to impede the
navigation. Other instances might be mentioned of foreign plants
introduced with seed having in a very short time become common
weeds in all cultivated land. Indeed, many of the species included
in our handbooks of British plants are so entirely confined to arable
land or to spots in the immediate vicinity of human dwellings, that
it is impossible to say how many of them may be really indigenous
to the soil, and how many naturalised aliens.
There is no doubt we have a great deal to learn as to the mode
in which plants propagate themselves in nature, which may be of
the utmost value to our gardeners. Every one is familiar with the
fact of the apparently spontaneous appearance, in immense abun-
dance, of plants in soil when subjected to certain farming operations,
or on the sowing of some particular crop. Whenever a new rail-
way cutting or embankment is made, some plant unknown in the
neighbourhood is almost sure to appear, and either permanently
1870. ] for English Gardens. 353
establish itself or again disappear after a few years. The “sowing”
of land with lime is invariably followed by the appearance of a crop
of white or Dutch clover. When certain kinds of wood are cut
down, it is said that during the next year a particular species of
moss will always be found covering the ground. Immediately after
the great fire of London in 1666, the London Rocket (Sisymbriwm
Trio) sprang up in enormous quantities on the dismantled walls,
but is now no longer to be found in the metropolitan district. The
usual theory to account for this sudden appearance of new plants
is the existence in the soil of large ‘stores of seeds” ready to ger-
minate on the first favourable opportunity. In his Anniversary
Address to the Linnean Society in 1869, Mr. Bentham, however,
pynted out that if this explanation is the true one, it ought not to
depend merely on theory, but would be capable of easy practical
verification. He suggested whether a hitherto insufficiently acknow-
ledged part in the rapid dissemination of plants may not be played
by birds. The whole subject presents a wide field for further in-
vestigation, and must amply reward any one who takes up the
inquiry, if endowed with the qualities of accurate observation and
patient research. :
Mr. Mongredien’s ‘ Planter’s Guide’ deals chiefly with the intro-
duction into this country of foreign trees and shrubs. Within the
last twenty or thirty years the appearance of our lawns and planta-
tions has been greatly changed by the number of new forms which
have made their appearance. ‘The stately Wellingtonca, the formal
self-asserting “ Puzzle-monkey” or Araucaria imbricata, the
massive Deodar and Cryptomeria, the elegant Pinus insignis and
Cupressus Lawsoniana, are all still of too recent introduction to
permit us to judge of what their effect will be when grown to their
full stature. The number of cone-bearing trees from all parts of
the world, perfectly hardy in this climate, is extraordinary ; and,
partly from their graceful shape, partly from the evergreen character
of their leaves, the attention of cultivators has been perhaps too
exclusively confined to them, while deciduous trees have been com-
paratively neglected. Recent experiments have shown that in this
quarter also there is abundant room for an extension of our powers
of domestication. In one of the London Parks least frequented by
the upper ten thousand, that at Battersea, great success has attended
the introduction, during the last few years, of half-hardy trees and
shrubs, the precaution being taken of protecting their roots during
winter by a layer of some substance impervious to frost. The
French have paid more attention to the perfect naturalisation of
half-hardy plants than we have done: notwithstanding the greater
severity of their winter, species are grown by them out of doors
which are never seen with us except in greenhouses; even as far
north as Paris, the bamboo, for instance, is frequently met with in
dot Foreign Trees and Plants | July,
gentlemen’s gardens; and there is no doubt that many shrubs and
herbaceous plants, which we never think of attempting to grow
except under protection, might, with a very little care and attention,
become permanent denizens of our gardens and shrubberies. Pro-
bably few are aware that the common Camellia will stand with
impunity an ordinary English winter. Mr. Mongredien says that
“it protected during the first two or three years after being planted
out, and when once established, it proves in the climate of London
quite as hardy as the common laurel, and blooms as profusely as in
a conservatory. It is true that, from its habit of flowering early
in the spring, the blossoms are sometimes damaged by the nipping
easterly winds, but this occurs only in unfavourable seasons; and
even if the tree never flowered at all, its lovely foliage would still
make it one of the most beautiful evergreens of which our gardens
can boast. A plant of the variety Donkelari has stood out for
twelve years in a garden at Forest Hill with a northern aspect,
without the slightest protection during the severest winters, and
now forms a good-sized bush, densely clothed with magnificent
foliage. ‘The Camellia ought to be planted out in every garden,
and with a little attention for the first year or two, it would prove
quite hardy, at least in the more southern counties, and each
season it would increase in attractiveness.” —--
The climate of the south of England is far more congenial to
the introduction of foreign trees and shrubs than that of the
northern counties, not from the greater severity of the winters in
the north, for the minimum temperature of the year is often as
low in Kent or Hampshire as in Yorkshire or Northumberland,
but from the shorter and cooler summers. Many plants absolutely
require a considerable period of high temperature to enable them to
ripen their wood sufficiently to withstand the winter frosts, and
especially to induce them to flower. In many parts of Scotland,
however, the climate is as favourable to horticulturists as in any
district of England. In the Duke of Sutherland’s estate at Dun-
robin, on the east coast of Sutherlandshire, Hydrangeas, myrtles,
and other half-hardy plants, grow as freely and as unchecked out
of doors as they do in Devonshire or Cornwall. The equalizing
effect of the Gulf Stream on the temperature is no doubt the cause
of this special immunity from frost. The proximity of the sea-
coast is not generally favourable to the growth of trees and shrubs,
not so much from the saltness of the air as from the prevalence of
high winds, which are very injurious to growing vegetation. Young
and tender shoots which will bear a moderate amount of cold, will
sometimes be scorched as if by fire by a tempestuous night.
Mr. Mongredien’s book is intended as a repertorium of every-
thing connected with the choosing, planting, and treatment of Eng-
lish and foreign trees and shrubs, and contains an immense mass
1870. | for English Gardens, 355
of information for any one whose tastes lie in this direction. Its
defects are rather of omission than of commission. The plan pro-
mises a completely exhaustive treatment of the subject: in the first
place we have an alphabetical list, with brief descriptions, of 621 trees
and shrubs, selected as desirable for planting in the open air in this
country ; followed by a classification of them under a variety of
headings, as to their height, their foliage, their time of flowering,
the colour of their flowers, their fruit, their timber, and other points.
It is illustrated by a number of very pretty woodcuts, of which
we subjoin a specimen. The principle on which these 621 species
Abies nobilis ; Wimbledon.
have been selected is not always obvious. Why, for instance, is our
common Fuchsia (miscalled Fuchsia coccinea, as Dr. Hooker has
shown) excluded, forming as it does the glory of every cottage-garden
in the Isle of Wight and in Devonshire, the stems assuming almost
306 Foreign Trees and Plants [July,
a tree-like character; or the Berberis aquifolium, which, with its
glossy leaves and very early flowers, is so deservedly a favourite in
every shrubbery? In the enumeration of winter-flowering plants
we miss also the beautiful Forsythia, and several others which might
have been mentioned. An exceedingly useful list is that of ‘ species
which thrive in the smoke of cities,” in which Mr. Mongredien names
the horse-chestnut, Aclantus glandulosa, Virginian creeper, almond,
Artemisia abrotanum, Aucuba, Catalpa, Cydonia japonica, labur-
num, fig, ivy, Cape jasmine, privet, Paulownia imperialis, Phillyrea
media, plane, evergreen oak, Rhamnus Alaternus, samach, flowering
currant, Robinia pseudacacia (commonly called the acacia), Sophora
japonica, and guelder rose; a very useful list to cultivators of
suburban gardens, but again very incomplete. In London gardens
the lilac is everywhere the companion of the laburnum; magni-
ficent hawthorn-trees could be shown within two miles of Charing
Cross; the roads in the suburbs are everywhere adorned in early
spring with the beautiful hght-green foliage of the lime; while the
sides of the houses are gay in the summer with the gorgeous flowers
of the hardy passion-flower, or the gigantic leaves of the Aristolochia
Sipho; nor should the apple, the pear, and the cherry have been
omitted, if it is only for the wealth of their flowers. It is worthy
of remark that the smoke of an ordinary town is not nearly so de-
structive to vegetation as that poured forth from the chimneys of
manufactories or chemical works. Flowers will be found to thrive
in gardens in the very heart of London, which many a Lancashire
gentleman would give almost any money to establish even in his
ereenhouses. Notwithstanding the deficiencies we have named,
‘The Planter’s Guide’ is a book that should be in the hands of
every one interested in the subject; and we hope it may be the
means of attracting attention to the great value and importance of
ornamental planting in improving the character of our lawns,
shrubberies, and parks.
If we now turn from trees and shrubs to herbaceous plants, we
enter on a still wider field, and one more within the reach of every
lover of nature. Arboriculture, after all, must always be the pur-
suit of those only who have both money and space at their command ;
floriculture may be followed by every cottager, and even by every
dweller in a town who has a window-sill at his disposal; and we
doubt whether the latter does not derive the most pleasure from it.
Although many of the favourite flowers of the last two or three
generations will probably always hold a place in our gardens, and
deservedly, yet the number of species that have been introduced of
late years worth cultivating for their beauty, and within the reach
of every one who possesses a flower-pot, is very large; and as a
hand-book for this class of plants, though treating only of a section
of them, plants especially adapted for rock-work, we can most
Fe ee
1870.] for English Gardens. 357
cordially recommend Mr. Robinson’s ‘ Alpine Flowers for English
Gardens.’ ‘The easy and lively style in which it is written, no less
than the excellence of its matter, will commend it to every lover of
lants.
; Mr. Robinson is no mere enthusiast in his subject when he says :
—“ This book is written to dispel a very general error, that the ex-
quisite flowers of alpine countries cannot be grown in gardens, and
as one of a series of manuals having for their object the improve-
ment of our out-door gardening, which, it appears to me, is of in-
finitely greater importance than anything that can ever be accom-
plished in enclosed structures, even if glass sheds or glass palaces
were within the reach of all.” His first concern is with the struc-
ture of rockeries, in the mode of building which not only is the
taste still displayed, or at all events till quite recently, barbarous
and inartistic in the extreme; but it would seem as if the very
conditions necessary for the health of the plants were studiously
neglected. The ordinary idea of the treatment of rock-plants,
judging from the hideous monstrosities which may be seen in many
a gentleman’s garden, is that you have nothing to do but to poke
them in between the chinks of perfectly bare stones or clinkers piled
together in a promiscuous heap, in order to present them in their
native habitats. A gardener who commits such an absurdity as
this, can never have ascended a mountain with his eyes open. To
quote again from Mr. Robinson :—* Mountains are often bare, and
cliffs are usually devoid of soil ; but we must not conclude therefrom
that the choice jewellery of plant-life scattered over the ribs of the
mountain, or the interstices of the crag, live upon little more than
the mountain air and the melting snow! Where will you find such
a depth of well-ground stony soil, and withal such perfect drainage,
as on the ridges of débris flanking some great glacier, stained all
over with tufts of crimson saxifrage? Can you gauge the depth
of that narrow chink, from which peep tufts of the diminutive and
beautiful Androsace helvetica? No; it has gathered the crumbling
erit and scanty soil for ages and ages; and the roots enter so far
that nothing the tourist carries with him can bring out enough of
them to enable the plant to live elsewhere.” Alpine plants are
peculiarly exposed to sudden alternations of heat and cold, of moisture
and dryness. The cold, almost frosty night will be followed, in
July and August, by an unclouded day, when the rays of the sun
beat on the unsheltered surface of the rock with an intensity that
would scorch up many an English meadow plant. Only a very
small proportion of alpine plants are annuals ; and they are frequently
provided with a storehouse of nourishment in the form of rosettes
or tufts of thick succulent leaves; but their chief water-supply is
through their roots; and thus we find that while our garden
annuals have fibrous roots of insignificant dimensions, and even
308 Foreign Trees and Plants [July,
our forest trees will seldom strike their roots to a greater depth
than the height of their foliage, the roots of alpine plants scarcely
an inch in height will be found to penetrate the chinks between the
rocks full of rich earth, to the depth of sometimes more than a yard,
or forty times the height that they venture into theair. The neglect
of this most essential condition for the growth of alpine plants is of
itself amply sufficient to account for the failure which has generally
accompanied the attempts to introduce these lovely flowers to our
rockeries. A good depth of soil is indeed more indispensable to
these plants than the presence of rock and stone. They no doubt
prefer to expand their flowers and extend their green shoots over
the bare rock ; and where rock-work is artistically managed, this
faint attempt at a reconstruction of their native habitat adds greatly
to the picturesqueness of the effect. But many of them will flourish
equally well in open borders, and even when planted in pots, with
a few stones about them to protect the roots from the direct action
of the sun, if only the two requisites are attended to, of constant
moisture and perfect drainage; and hence they are invaluable ac-
quisitions to the cottage or window gardener. The Saxifrages, the
beautiful purple Awbrietia, with respect to which Mr. Robinson
says, ‘ rock-works, ruins, stony places, sloping banks, and rootwork
suit it perfectly; no plant is so easily established in such places,
nor will any other alpine plant clothe them so quickly with the
desired vegetation,” the various species of Arabis, the alpine
Primulas, all make excellent bedding plants. The ease with which
a new alpine can be domesticated in our climate is shown by the
rapid spread of the lovely early forget-me-not, Myosotis dissitiflora,
brought not many years since from the Alps near the Vogelberg,
now to be had from every nurseryman, and the treasure of many a
cottage garden, with its exquisite sky-blue flowers, continuing from
mid-winter till early summer.
But it is not alpine flowers only which will repay the small
amount of trouble necessary for their introduction. Many plants
which are never grown without the protection of a greenhouse, do
not require any elevation of temperature for their successful growth,
but merely an absence of great changes both of temperature and
moisture. ‘This is especially the case with not a few of the most
delicate ferns, such as the elegant maidenhair, and the two fragile
little filmy-ferns; and the requisite uniformity of temperature and
moisture can be obtained out of doors by the erection of a partially
underground grotto or ravine of rocks, through which water is per-
petually trickling, the entrance being protected by a screen of
foliage from the direct infiuence of the weather. It is astonishing
how equable a climate can be obtained by a simple device of this
kind. The drawing given on p. 359 is from such a rock-cave
constructed in the grounds of one of our most scientific and success-
1870. ] for English Gardens. 309
ful nurserymen near York, where he grows not only our royal so-
called “ flowering fern,” the Osmunda regalis, and several foreign
Entrance to Cave for Killarney Fern in Rock-garden.
allied species, but the most beautiful of all this beautiful tribe, the
moisture-loving Killarney fern, which clothes the soil of the damp
dark woods by the Tore waterfall.
The beauty of these horticultural experiments is that they can
be tried on so small a scale, and are thus within the reach of almost
every one ; yielding a source of pure and healthy enjoyment which
few other "pursuits will afford. Mr. Robinson almost promises us
that his little book shall be the first of a series of similar manuals
on different departments of gardening ; and we can hardly conceive
a greater service than this to a large number of his countrymen,
who merely require to be told how to set to work to cultivate this
fascinating science.
( 360 ) [July,
VII. A RECENT TRIUMPH OF SYNTHETICAL
CHEMISTRY.
Iv is not often that so legitimate a triumph of synthetical chemistry
as the artificial production of a natural substance becomes, at the
same time, an important national discovery, the money value of
which may be reckoned by millions. Such, without exaggeration,
it is not unlikely that the artificial production of Alizarine, the
colouring matter of madder, may become.
Madder is the root of a plant belonging to the order of Ru-
biacez, amongst which are included some valuable plants, such as
the cinchona, ipecacuanha, and coffee. The madder plant is the
rubia tincorum. It is estimated that its consumption reaches over
47,000 tons per annum, and this, at 45/. per ton, amounts to over
2,000,0007. sterling, one half of which is imported to England, and
the payment for which (1,000,0002.) goes out of this country mto
the pockets of foreign manufacturers. If now the essential con-
stituent for which madder is so valuable, its pure colouring matter,
can be economically prepared by chemical means from coal-tar, that
amount of money will naturally go into our own pockets—a not
unworthy reward for chemical ingenuity.
The value of madder in dyeing and calico printing depends upon
the many different colours which can be dyed by its means ; thus,
one mordant (iron) gives purple shades, from the most delicate
mauve to black; with another mordant (alumina), red shades are
produced, from the palest pink to deep crimson, including the
brilliant and well-known Turkey red; and by judicious admixture
of these mordants, combinations of all varieties of chocolate-brown
are produced. These colours are very permanent, whilst the high
price of the raw material to which they are due renders the dis-
covery of a substitute a problem of the highest commercial import-
ance. For these reasons the chemical investigations of madder have
been very numerous, the most valuable results having been obtained
by our own countryman, Dr. Schunck. This chemist found that the
root did not contain a colouring matter ready formed, but there was
in it, amongst many other bodies, a erystallme substance, which he
named rubianic acid. When the powdered madder is allowed to
stand in a moist state, or is gently heated with water in the dye-
beck, a peculiar fermentation sets up under the influence of a fer-
ment called erythrozyn, by which the rubianic acid is split up into
alizarine and glucose. Besides alizarine, there is another colouring
matter obtained from madder, called purpurine ; but as all the valu-
able shades and colours of madder are due to the alizarime, we need
only devote attention to the latter substance.
Alizarine is a brilliant scarlet substance, which crystallizes in
1870.] “| SOSGE Wee oring “1-35
Two substances physically distinct, but occurring together near
Brevig in Norway, have hitherto been confounded under the general
name of Esmarkite. One of these is a true Praseolite, but the other
ig an extremely rare mineral, which has received Des Cloiseaux’s
attention during his visit to Norway.t This acute crystallographer
has carefully examined authentic specimens of the true Esmarkite,
and pronounces it to be merely a laminar variety of the felspar—
anorthite.
Several new species recently described demand a cursory notice.
Glaucopyrite is Professor Sandberger’s name for a new mineral, ob-
tained from Guadalcanal in Spain, and consisting of an arsenio-
sulphide of iron, in which part of the iron is replaced by cobalt and
* “Analisi chimiche di alcuni minerali delle ,isole del mare toscano.”—
‘ Bollettino del R. Comitato geologico d'Italia,’ 1870, p. 82.
+ ‘Ann. d. Chim. et de Phys.,’ 1870, p. 176.
1870. | Mineralogy. 419
copper, while part of the arsenic gives place to antimony.* Herr
Boricky describes, under the name of Zepharovichite, a new,species
allied to Wavellite occurring in the sandstone of 'Trenic in Bohemia.{
Tschermak proposes the name of Stmonyzte for a salt lately found
at Hallstadt, closely related to Bloedite, from which it differs, how-
ever, in being stable when exposed to the air.t Finally, Dr.
Schrauf apples the name Simlacte to a mineral from Simla in
India, simular to meerschaum, but containing alumina, and belong-
ing to the group of halloysites.§
Two Cornish minerals have lately been analyzed by Professor
Church—the one a variety of kaolin, akin to lithomarge, and termed
Restormelite ; the other is the beautiful green mineral known as
chalcophyllite, or copper-mica.|| The formula of restormelite may be
written Al,O;.2 Si0,-++ 2 ag.; while the composition of the chalco-
phyllite may be thus expressed: 8 CuO. Al,O,.As,0, + 24 ag.
Attention is directed by Mr. 8. G. Perceval] to the occurrence
of topazes in the granite of Lundy Island, somewhat similar to the
well-known crystals from the granite of the Mourne mountains.
The writer of this Chronicle has for several years past been familiar
with specimens of both topaz and beryl from Lundy.
Professor How follows up his ‘ Contributions to the Mineralogy
of Nova Scotia’ by further notices of the two species—natroboro-
calcite and silicoborocalcite, now better known under Dana’s names
of Ulexite and Howlite.** Both minerals have been found good
substitutes for borax in welding.
We learn from the ‘ Levant Herald’ that a large meteorite fell
at Mourzouk, in Fezzan, on or about the 25th December, 1869.
The fall occasioned considerable consternation to a group of Arabs
who were standing near, and they immediately discharged their
muskets on the unwelcome stranger. }}
It seems likely that the Australian mineral lately introduced
under the name of Wollongongite will in future be known by some
more appropriate designation. The Rev. W. B. Clarke has pointed
out that some little error has arisen in assigning to this species a
local habitation anda name. In fact, the so-called Wollongongite
occurs not in Llawarra, but at a place called Petrolia, formerly
known as Reedy Creek, where it was recognized by Count Strzelecki
as far back as 1839. Under these circumstances the name ceases
to be appropriate, so that “ there can be no question, I think,” says
Mr. Clarke, “that Wollongongite is a misnomer, and that Professor
Siliman will change it.”
A good deal of common sense characterizes the little minera-
* ‘Jahrbuch f. Mineralogie,’ 1870, p. 196. ¢ Ibid., p. 229.
{ ‘Sitzber. d. Kais. Acad. d. Wiss., 1869. No. XXV.
§ ‘Corr, Blatt. d. z. Mineralog.’ V.in Regeusburg, 1870. p.
64,
|| ‘Chemical News,’ May 13, 1870, p. 223, q ‘Geolog. Mag.,’ 1870, p. 192.
** «Phil, Mag.,’ April, 1870, p. 275. tt ‘Nature,’ vol. i, p. 538.
420 Chronteles of Science. | July,
logical guide which Dr. A. M. Thomson has published in Sydney,*
for the assistance of explorers seeking to develop the mineral re-
sources of the colony. Plain directions are given for easily recog-
nizing the more important species—a task at all times extremely
embarrassing to the unassisted beginner.
10. MINING AND METALLURGY.
Munina.
THE newly drafted Bill amalgamating the Mines Regulation Bill
and the Metalliferous Mines Bill has been printed. We cannot but
think that this amalgamation will be found to be unfortunate.
Nearly all the conditions of a coal mine and a copper or tin mine
are so different, that it is quite impossible to apply the same legis-
lation to them with any hope of advantage. This is shown on the
face of the Bill itself. It now comprehends three sets of General
Rules: one applicable to all mines; the second, to coal mines only ;
and the third, to mines other than coal mines. The redrafted Bill
is supposed to embody the suggestions of the representatives of all
the interests affected—it is therefore probably now in that form
which will become law. In the last Quarterly Journal we suffi-
ciently entered upon the principles of the Mines Regulation Bill,
and therefore we need not occupy valuable space by enlarging upon
its clauses.
Tin mining has, once again, resumed its condition of high pros-
perity in our western counties; the prices of tin ore (black tin),
which have varied during the past quarter from 75/. to 85/. the ton,
being such as to leave a large profit to the miner. The result of
this is that numerous new tin mines are being opened, and the
miners have full employment and are getting good wages.
Copper mining is not in the same favourable condition. The
Clifford Amalgamated Mines, which employed a short time since
upwards of a thousand persons, are about to be abandoned, after a
long and profitable career. These mines—which comprehend the
United Mines, the Gwennap Consolidated Mines and Wheal Clifford
—were the most extensive copper mines in this country. The
levels were upwards of sixty miles in length, and from six to seven
miles of shafts had been sunk upon the lodes. This mine was re-
markable for the very high temperature of its lower levels. The
miners in some of the ends of the levels worked in temperatures
varying from 110° F. to 115° F., the water rising in those levels
being at the temperature of 120 F. This hot spring was remark-
* ‘Guide to Mineral Explorers in distinguishing Minerals, Ores, and Gems.’
By Alexander M. Thomson, D.Sc. Sydney, 1869.
1870. | Mining. 421
able for the great quantity of lithium which it held in solution.
All the lower parts of the mine are now filled with water ; a little tin
is being obtained from the shallow levels ; the machinery is being
removed ; and soon this scene of activity will become a silent ruin.
At Wheal Owles, in the mining district of St. Just, there have
lately been discovered some valuable samples of the oxide of ura-
nium, which have been sent into the market and realized high prices.
The Gold-fields of Nova Scotia—The declared returns of gold
for the whole province to the end of the year 1869 are as follows :—
Number of : Annual
Year. Yield of Gold. Miners daily | Quartz crushed. | 4V¥¢T@8e Yield | oaimings per
employed. per fon. man.
OZ. dwt. gr. No. cwts. oz. dwt. gr. $ c,
1862 .. 7.210 OO 500 134,800 SZ 291 00
1863 .. 14,001 14 17 877 340,035 0 18 10 319 30
1864 .. 20,022 18 13 810 428,700 1 0 20 494 36
1865 .. 25,454 4 8 683 ; 500,025 1 3 6 745 6
1866 .. 25,204 13 2 679 635,387 017 13 742 56
SBGfe eas oats EE TTL." | 702 666, 429 0 19 10 778 66
1868 .. 20,541 610 | 774 678,817 014 6 530 84
1869... 17,868 10 19 676 708,486 011 5 528 64
Total .. | 157,682 9 8 | 713 | 4,092,679 | 0 15 10 | 553 90
The gross yield of gold in Nova Scotia during the past ten years
has been 180,000 oz., representing, in round numbers, a value of
720,0002. sterling.
The produce of gold in Nova Scotia for the year ending 31st
December, 1869, in all the gold-producing districts, is shown in the
following Table :-—
A Value oe
: aily Average | #Verage yie
District. eee of ayeeene Quartz crushed.| yield “ ee
employed. One ployed at
$18°5 per oz,
| oz. dwt. gr. | No. tons. cwt.|oz. dwt.gr.| £ s. d
Stormont ..| 227 013 19 784 0/0 519| 4715 11
Wine Harbour | ALS VOR 0) 65 2 eo. be. | Ooo. 6 44 6
Sherbrooke .. | 5,546 11 16 134 PY O00 OO" Oo Ia 16a tae 6
Tangier .. 1,192 3 10 51 L332) 2 | O17 21 93 5 6
Montague .. 805 13 14 29 Oey 8 ay eS | Jad Be 7
Waverley sa 1,591 14 10 54 3,915 15; 0 8 3/117 18 1
Oldham .. | 1,394 16 0 56 1,730 2/;016 1 SNL Phoelll
Renfrew .. .. 3,097 Td". 7 112 7,208 9;0 812/110 12 9
Uniacke .. 1,867 3 12 71 5,171 13.| 0 11 18 | 105 3:10
Lawrencetown . 30 0 20 20 293 0:0 216 G6 148
aie ae aL a | 2,000 O'23 36 Woon te Oe te | ie eg
Unproclaime
poe a 394 11 19 29 622 9/0 623] 54 8 7
17,868 019 | 676 | 35,424 6/010 2/105 14 7
422 Chronicles of Science. [ July,
The produce of gold for the month of February, 1870, being
according to the Mineral Inspector’s Report, as follows :—
District. | Gold yield. Quartz crushed
(Colonial weight).
oz. dwt. gr. tons.
Sherbrooke .. .. .. 309.10-4:0 694°03
PAIGE se we. win, te 135 7 20 88-00
Olam fo0 ss. 104 7 14 200-07
Waverley Bed ee tee WAT 141-00
Eo i nr ee ff Spe ae | 223:°10
Musquodoboit ts ae 52 5 21 73°10
ACRE! ess” eh on 47 2 4 105-00
Wine Harbour 28 712 100°10
Isaac’s Harbour 21115 3°10
Mr. R. Brough Smith reports that the total quantity of gold
raised in Victoria in 1869 was 1,544,7574 ounces, and of this there
were exported 1,340,8384 ounces. The total imports into England
of Australasian gold in 1869 were of the value of 7,892,7571.
Since 1858 the imports have been as follows :—
£. Le
BSIS x2), os « Sy O%, 160 1364 oe) oni As Gdosane
$359" i. 8s. Sek, UU 1860°".. se. Ss 00l, bTU
1860 cv ibs 6,749, 000 1866.0\.5) 26 68365674
1861...) \2,...6,801,220 IBGT.. “wa ~wegi(\ BOIGZ07
TOU os we, VOg AE aoe 1868 .. .. 6,989,594
1863 .. .. 5,995,368
The increased returns of the last three years were due to the
opening of new gold-fields in Queensland, South Australia, and
New Zealand.
METALLURGY.
Mr. Spence, of Newton Heath, Manchester, has patented a new
process of separating copper from ores. He takes the solution of
chloride of copper as now obtained in extracting copper from ores
(by the wet process) which contains iron in variable proportions,
and generally contains free hydrochloric acid. This solution he
places in large open vats, and in another vessel of cast iron, fitted
with a revolving stirrer, he places a considerable quantity of the
vat waste of the alkali manufacture, or the spent lime from the gas
purifiers, and to this is added a solution of sulphate of ammonia, or
chloride of ammonium. The vessel or still being closed, a jet of steam
of from 20 to 30 lbs. pressure is blown into the mixture. Sulphide of
ammonium distils over, and is conveyed by a pipe into the vat con-
taining the metallic solution of copper and iron, by which sulphide
of copper is precipitated, and the ammonia combines with the
1870.] Metallurgy. 423
liberated hydrochloric acid. The process is continued until all the
copper is thrown down, which point is at once observed by sulphu-
retted hydrogen being evolved, when the process is stopped ; for if
continued, the ammonia would now neutralize the free acid, and the
iron would then be precipitated. The sulphide of copper thus ob-
tained is very nearly pure; it is washed and dried, and smelted into
copper by any of the usual methods employed.
A new process of calcining tin and other ores has been adopted
by Messrs. Oxland, F.C.S., and John Hocking. The ores are
introduced into a revolving iron cylinder, 4 feet in diameter and
30 feet long, lined with fire bricks, and supported at an inclination
of about 2 inch per foot on three pairs of rollers, on which it is kept
constantly revolving at a slow rate. ‘The fire passes from the fire-
place over a chamber into and through the tube. The ore having
been first dried on iron plates in suitable flues, at the back of the
calciner, is admitted in a steady stream into the higher end of the
cylinder, and the slow revolving motion imparted to it causes the
advance of the ore by its own gravitation, and it is discharged in a
continuous stream into a chamber between the fire-place and the
front of the tube. Great economy of fuel is said to be effected by
this furnace. The heat from the fuel has to traverse more than
double the distance over which it passes in Brunton’s calciner before
it escapes into the flues, and the tube presents nearly double the
amount of heating surface. None of the working parts are exposed
to the action of the fire. In working it is found to be economical
both as regards fuel and labour.
Several patents have been taken out of late relating to the
manufacture of iron and steel. Mr. Cowper, of Westminster, patents
improvements in treating cast iron for the production of wrought
iron and steel therefrom. By this process the purification of the
east iron is accomplished by a jet of superheated steam applied to
a stream of the liquid iron as it flows from the blast furnace, so as
to divide it up into small particles, and act upon them; the iron is
received into a hot box, and transferred to a calcining furnace, in
which it is kept hot whilst still exposed to an atmosphere of hot
steam ; such purified iron is mixed either hot or cold with liquid
cast iron, and afterwards used as cast iron, or made into steel or
wrought iron.
In the manufacture of steel Mr. Julius Baur, of New York,
patents a process of alloymg or combining metallic chromium with
metallic iron, so that chromium in a metallic state shall be present
in the finished product, which is said to impart valuable properties to
it. This process is distinguishable from that secured by Mr. Robert
Mushett for mixing oxide of chromium in the manufacture of steel.
Letters patent have also been granted to Mr. J. M. Stanley, of
Sheffield, for improved modes of utilizing the heat given off during
424 Chronicles of Science. [July,
the decarbonizing or converting process, the object of which is to
eave the consumption of fuel, and reduce the cost of the
metals.
There is also an invention whereby very superior iron and steel
are said to be obtained by smelting titanic iron ore, Imenite, in a
blast furnace, without the addition of any other metalliferous body ;
the alloy of iron thus obtained possesses a large percentage of car-
bon. Various methods are adopted to carry out this process, The
inventor is Mr. T. 8. Webb, of the Norton Iron Works. |
11, PHYSICS.
Licut.—Spectrum analysis has been applied by Vogelsang and
Geissler to the difficult question of determining the chemical nature
of the fiuid found enclosed, in minute quantity, in the cavities of
certain quartz-crystals. Fragments of quartz were placed in a
small retort, which was connected with an air-pump and exhausted ;
then, by the application of heat, the quartz decrepitated, and the
evolved vapour was examined in a Geissler-tube. The presence of
carbonic acid was thus abundantly proved, and this was confirmed
by the turbidity which it produced in lime-water.
A great improvement in the spectroscope has been made by
Mr. Browning, who calls his instrument the automatic spectroscope.
It is furnished with a battery of six equilateral prisms of dense
flint glass; all the prisms are joined together like a chain by their
respective corners, the bases being in this manner linked together.
This chain of prisms is then bent round so as to form a circle with
the apices outwards ; the centre of the base of each prism is attached
to a radial rod. All these rods pass through a common centre.
The prism nearest the collimator, 2. ¢. the first prism of the train,
is a fixture... The movement of the other prisms is then in the pro-
portion of 1, 2, 3, 4, and 5, the last or 6th prism moving five times
the amount of the second. All these motions are communicated by
the revolution of the micrometer screw, which is used for measuring
the position of the lines in the spectrum; and the amount of motion
of each, and of the telescope, is so arranged that the prisms are
automatically adjusted to the minimum angle of deviation for the
ray under examination. It is easy to test the efficiency of the
instrument in this respect. On taking the lens out of the eye-piece
of the telescope, the whole field of view is found to be filled with
the light of the colour of that portion of the spectrum which the
observer wishes to examine; while in a spectroscope of the usual.
construction, at the extreme ends of the spectrum, just where the
light is most required, only a lens-shaped line of light would be
1870. | Physies. 425
found in the field of view. As a consequence of this peculiarity,
the violet and deep-red ends of the spectrum are greatly elongated,
or rather, much more of them can be seen than in an ordinary
spectroscope, and the H lines, which are generally seen only with
difficulty, come out in a marked manner.
Drs. Roscoe and Thorpe have recently communicated to the
Royal Society the results of a series of determinations of the chemical
intensity of total daylight, made in the autumn of 1867, on the flat
plateau of the river Tagus, about 84 miles south-east of Lisbon,
under a cloudless sky, with the object of ascertaining the relation
existing between the solar altitude and the chemical intensity of the
light. The experiments were made as follows:—1. The chemical
action of total daylight was observed in the ordinary manner ;
2. The chemical action of the diffused daylight was then observed,
by throwing on to the exposed paper the shadow of a small,
blackened, brass ball, placed at such a distance that its apparent
diameter, seen from the position of the paper, was slightly larger
than that of the sun’s disk; 3. Observation No. 1 repeated;
4. Observation No. 2 repeated. Next, the means of observations
1 to 4 were taken. The sun’s altitude was determined by a sextant
and artificial horizon. One of the sets of 134 observations was
made as nearly as possible every hour. It has been already pointed
out, and proved by experiments made at Kew, that the mean
chemical intensity of total daylight, for the hours equidistant from
noon, is constant. The results of the present series of experiments
prove that this conclusion holds good generally. One of the chief
results arrived at is that, although the chemical intensity for the
same altitude, at different places and at different times of the year,
varies according to the varying transparency of the atmosphere, yet
the relation, at the same place, between altitude and intensity, is
always represented by a straight line.
A new and very ingenious graduating diaphragm for the micro-
scope has been contrived by Mr. J. Zentmayer. This exceedingly
ingenious arrangement is shown in the accompanying cuts, which
are taken from photographs; Fig. 1 showing the apparatus with
Pre. 1. Fie. 2.
|
———S re pet ——
ee 2... SS \ > -s
6 SS S22: — 2
eg =! =: == EF
= = Z = SS =
———=$4 = = = SSS SSNS
== Oz 6 =]_=E
ESS SS =: == SSS
———— == EEA =. ]S=
= = SS ——— >- Se
—S— ‘ ———— —— =
!
its largest, and Fig. 2 with its smallest opening. To obtain a
circular diaphragm which, like the eye, should expand and contract
426 Chronicles of Science. [ July,
gradually by a continuous change, and yet be made of rigid and
unchangeable material, might seem at first sight to be an impossi-
bility ; but, after all, when the result is accomplished, as in this
apparatus, we are surprised as much by the simplicity as by the
ingenuity of the means employed. ‘The woodcuts almost explain
the apparatus of themselves ; but we may say, in addition, that it
consists of two cylinders or rollers with parallel axes and surfaces
in contact, having similar conical grooves on their surfaces, and
fine teeth cut at one end of each, which, gearing together, cause
them to rotate in unison. There is, theoretically, an objection to a
diaphragm of this construction, from the fact that its opening will
not always be in the same plane—that is, the smallest cross-section
of the space between the rollers will not always be equidistant from
a plane at right angles to the line of sight and passing through the
axes of the rollers. With the larger opening, this cross-section will
be nearest to, and with the smaller, farther from, such a plane. In
practice, however, this difference is so small as to be entirely unim-
portant, and may even, in some cases, be turned to advantage.
Experiments have been made at Toulon by M. F. Silvas to try
to attach to life-buoys another floating body provided with phos-
phide of calcium, which, on becoming wet, gives off spontaneously
combustible phosphuretted hydrogen, thus emitting light to guide
the man, who might have fallen overboard and be in search of the
life-buoy.
Heat.—Dr. Guy has arranged in series the different poisonous
substances according to their melting and sublimation temperatures.
The arrangement is as follows:—(1) Sublimates formed without
any previous change of state of aggregation, and giving white
vapours; under this head are brought bichloride of mercury, calo-
mel, arsenious acid, and cantharidine. (2) Sublimates after pre-
vious fusion, and without leaving any residue—vwiz. oxalic acid.
(3) Sublimates after previous fusion, leaving a carbonaceous residue
—morphine and strychnine. (4) Fusion, change of colour, subli-
mation and deposition of carbonaceous residue, aconitine, atropine,
delphine, veratrine, brucine, digitaline, picrotoxine, solanine. (5) De-
crepitation ; slow and partial sublimation; tartar emetic.
Professor Morren has instituted some experiments on the com-
bustibility of diamonds, and the effect of a high temperature on
these gems. ‘The author, in a letter, first relates the following facts
as having given rise to his experiments. A jeweller at Marseilles
was requested to enamel afresh the gold bearings of two large
diamonds of great value, used as shirt buttons. Instead of taking
off the diamonds, always a delicate operation, the jeweller, who had
frequently executed such work previously, decided to enamel the
gold while the diamonds were left on their bearings. Not having
1870. | Physics. 427
charcoal at hand, the jeweller took coal for heating the mufile for
enamelling, an operation which succeeded most perfectly; but on
taking the buttons from the muffle, the jewels had become perfectly
black, and no amount of rubbing or friction restored them to their
pristine state. The jeweller was therefore obliged to dismount the
jewels, which looked like plumbago, and to send them to Paris,
when by the first touch of the lapidary’s wheel they became restored
to their former beauty ; while, curiously enough, their weight had
notchanged. Professor Morren who, through the kindness of MM.
Laurin, jewellers at Marseilles, was enabled to experiment with
several diamonds, placed them on a small platinum boat in a pla-
tinum tube, and tried the effect of a high temperature simultaneously
with different gases. Heated in coal-gas the gems become blackish,
increase in weight, and are found to be coated with a strongly-
adhesive layer of carbon, such as is deposited in gas retorts; in
pure hydrogen, the gems may be heated almost to the melting-
point of platinum without undergoing any change; heated in car-
bonic acid gas, the gems become dull and lose a little weight. ‘The
carbonic acid gas was found to be dissociated into carbonic oxide and
carbonic acid; this, the author found, was caused by the platinum
and not by the diamond. When the diamond is placed in oxygen
eas and ignited, it continues to burn, but remains white, appearing
as a piece of unpolished glass; the stone does not blacken, nor swell
up, and, if it is free from flaws or cracks, does not split asunder.
Dr. Janssen, who, it will be remembered, went to India for the
purpose of observing the total solar eclipse, has communicated some
observations on the artificial production of ice in India. In many
parts of the Indian continent, the natives dig shallow pits in localities
which are freely open to the sky and distant from trees. ‘The pits
are lined with straw, and upon the straw are placed dishes (made
of a very porous earthenware) filled with water. During the calm
and ¢lear nights prevailing in the period from November to the end
of February the water placed in the dishes freezes, yielding a solid
cake of ice, while the temperature of the air is + 10°. Dr. Janssen
has investigated this curious subject experimentally, and has found
that the freezing is principally due to the radiation during the night ;
but the evaporation of the water, aided by the porosity of the
earthenware employed, is at the same time not to be overlooked,
In order to exhibit the effect of the expansion of water when
freezing, F. Ridorff fills with distilled and previously well-boiled
and cooled water a cast-iron cylinder, having the following dimen-
sions:— Height, 160 millimétres ; diameter (external), 50 millimetres ;
thickness of solid iron, 15 millimetres, After having been filled
with water this apparatus is closed by means of a plug screwed into
the neck, and the cylinder is next placed in a mixture of three parts
VOL. VII. 26
428 Chronicles of Science. [July,
of snow or pounded ice, and one part of common salt; after about
forty minutes the cylinder bursts with a loud report. It is essential
for the success of this experiment that the plug fits very perfectly, and
that the cylinder, after having been filled with water, be placed for
some time in ice. ‘The wooden pail which contains the freezing
mixture should be roomy, and be covered with a stout towel to pre-
vent the spirting about of the contents at the time of the bursting.
Some experiments on the freezing of wine have been tried by
A. Rousselle. The reason why freezing improves wines, under
certain conditions, is, according to this author, because by partial
freezing the proportion of all the fixed substances in the liquid
Wine is increased ; and these are, moreover, thereby rendered more
fit for causing the combination of the acids with the alcohol, so as
to form those ethers to which wine owes its peculiarly distinct
flavour, aroma, and strength.
Dr. Hann has tried to solve by observation the problem of the
decrease of the temperature of the air in relation to the elevation
above sea-level, by comparing the average of temperature as observed
at certain groups of stations situated under the same mean latitude
and longitude, and by taking into account local influences. Seven
of these groups are situated in the western portion of the Alps, at
from 230 to 3330 metres above sea-level; four in the northern
part of Switzerland, at from 500 to 1780 metres above sea-level ;
three in the Rauhe Alps (Wurtemburg), at from 310 to 810 métres
above sea-level; four in the Erzgebirge (Central Germany), at from
180 to 850 métres above sea-level ; and four in the Harz (province
of Hanover and Brunswick), at from 70 to 1140 metres above sea-
level. The results obtained have proved that, in the instances
mentioned, the decrease of the temperature of the atmosphere near
the ground is really proportionate to the height of the locality above
sea-level. When the results of all the observations are duly con-
sidered, there is discovered a strongly marked annual periodicity,
and a very uniform decrease of temperature from below to above,
the average relation of the temperature reigning in December being,
to that of June, as 1 to 2.
Dr. Yon Wartha has obtained solid disulphide of carbon by the
rapid evaporation of this liquid itself, in the same way as solid car-
bonic acid is formed. The solid sulphide melts at 9° F’., and has the
appearance of small cauliflowers.
Some time ago M. Lamy proposed a pyrometer based upon the
dissociation of carbonate of lime. He now proposes to apply ammo-
niacal chloride of calcium, which gives off ammonia at low tempera-
tures. The instrument is to be connected with a manometer, which
will record the temperature. The contrivance is to be especially
adapted to record the temperature at different depths under the
1870. | Physies. 429
surface of the soil. In reference to this, M. Z. Becquerel and others
have very properly observed that better and far more accurate means
for accomplishing this purpose exist already, and are daily employed
with success.
A valuable substance for crucibles and fire-bricks has recently
been discovered. ‘There occurs, in the Département des Ardennes,
France, a variety of hydrated silica known by the name of gaize,
and geologically situated below the cretaceous deposit; the thick-
ness of this layer is 30 metres, and it extends over a distance of
24°85 English miles. The sp. gr. of this substance is 1°48 in crude
state, and after ignition 1-44. This stone is used as a building
stone; it is, at first, quite soft, so that it can be cut with a knife.
The material resists a very high temperature without fusion or
cracking, or, also, of perceptible contraction, either cubical or linear,
and it has consequently been recommended for the manufacture of
crucibles (on the lathe), for fire-bricks, and for furnaces.
Execrriciry.—A cause of error in electroscopic experiments has
been pointed out by Sir Charles Wheatstone, F.R.S. In the course
of some experiments on electrical conduction and induction the
author was frequently delayed by what at first appeared to be very
puzzling results. Occasionally he found that he could not discharge
the electrometer with the finger (or only to a certain degree), and
that it was necessary, before commencing another experiment, to
be in communication with a gas-pipe which entered the room. How
he became charged could not at that time be explained ; observation
and experiment, however, soon led Sir Charles to the true solution.
He was sitting at a table not far from the fire-place, with the electro-
meter (one of Peltier’s construction) before him, and was engaged
in experimenting with dises of various substances. ‘To ensure that
the one in hand (which was of tortoiseshell) should be perfectly dry,
it was held for a minute before the fire. Returning, and placing it
on the plate of the electrometer, it had apparently acquired a strong
charge, deflecting the index of the electrometer beyond 90°, and it
was then observed that the same thing took place with every disc
thus presented to the fire, whether of metal or any other substance.
The first impression was that the dise had been rendered electrical
by heat; but, on placing it in contact with a vessel of boiling water,
or heating it by a gas-lamp, no such effect was produced. The next
conjecture was that the phenomenon might arise from a difference
in the electrical state of the air in the room, and that at the top of
the chimney. That this conjecture, however, was not tenable was
soon evident, because the same deviation of the needle of the electro-
meter was produced by bringing the disc near any part of the wall
of the room. ‘This seemed to indicate that different parts of the
room were in different electrical states; but this, again, was dis-
2G 2
430 Chronicles of Science. [July,
proved by finding that, when the positions of the electrometer and
the place where the disc was supposed to be charged were inter-
changed, the charge of the electrometer was still always negative.
The last resource was to assume that the author himself had become
charged by walking across the carpeted room, though the effect was
produced even by the most careful treading. This ultimately proved
to be the case; for, resuming his seat at the table, and scraping the
foot on the rug, Sir Charles was able, at will, to move the index to
its greatest extent.
As a substitute for copper for the Daniell Electric Battery, Dr.
C. Stélzel proposes to take a piece of well-polished tin plate (sheet
tin, not tinned iron), immerse it in a very dilute solution of a copper
salt, and put it in connection with a weak galvanic current. After
the lapse of from fifteen to eighteen hours a layer of strongly
adhering metallic copper will have become firmly deposited upon
the tin plate ; and the latter, after having been bent into the required
shape, is an excellent, cheap, and durable substitute for the copper
cylinder in Daniell’s battery.
Considering the numerous experiments now being tried on wine,
it is to be hoped that the quality of the cheaper kinds of this be-
verage will shortly show some improvement. Whilst Dr. Rousselle
proposes to freeze wine, Dr. Scontettin prefers to electrify it. As
a very tangible proof of the gain obtained by the immediate con-
version of young wines into drinkable beverages by means of elec-
tricity, the author states that, considering that the annual production.
of wine of France amounts to from 60 to 70 millions of hectolitres
(each equal to rather more than 22 gallons), and that at least 10
francs per hectolitre is lost by vaporization during the time of the
maturity of the wine while in casks, this represents an amount of
from 600 to 700 millions of francs gained by rendering wine fit for
immediate consumption by the author’s electric process. We may
not inaptly apply here, “Si non e vero e bene trovato.”
Some useful electrolytic experiments have been tried by P.
Burckhard. After describing his arrangement, the author states
that oxide of bismuth is not a conductor of electricity unless it be
in a state of fusion, but in that case one of the copper electrodes
becomes coated with bismuth ; while, if platinum electrodes are
used, there is formed at one of the electrodes a very fusible alloy of
the two metals. Fused borax is not a bad conductor, although the
author confirmed the statement made by Dr. Tichanowitsch that
pure boric acid does not conduct electricity at all. When borax
in a fused state is experimented with, a series of compounds are
formed or volatilized ; but the main result is its decomposition into
soda, oxygen, and boron. Pyrophosphate of soda in a fused state
yields, among the products of electrolysis, phosphide of platinum,
1870. ] Zoology. 431
if a platinum electrode be applied; but the decomposition, which is
chiefly the result of the electrolysis of this salt, is its splitting up
into oxygen, phosphorus, and soda. Carbonate of soda in a fused
state is a good conductor of electricity ; it is decomposed into car-
bonic acid and soda, but a small portion of carbon is also formed.
A series of very accurate experiments, made with chemically
pure substances, have been tried by M. E. Becquerel, on the electro-
motive force of divers substances, as for instance, pure carbon, gold,
platinum, &c., in the presence of water and other fluids. Among
the curious facts elicited is this, that pure gold, obtained from the
French Mint, is acted upon by pure water in a manner not hitherto
explained, but which gives the author occasion to ask whether pos-
sibly gold does not contain another substance which has not been
discovered, or whether perhaps the slow action of the water is not
the cause of the disaggregation of the gold, thus explaining the fact
of its being found in rivers in the state of dust.
In a very lengthy paper on the properties of galvanically-pre-
cipitated iron, Kt. Lenz records a series of experiments, not only made
with iron, but also with copper. The results are stated as follows:—
Tron and copper, when reduced to the metallic state by electricity,
contain gases occluded, among which hydrogen is in largest amount:
the bulk of gas thus occluded varies considerably, but iron has been
found by the author to occlude as much as 185 times its own
bulk. The absorption of the gases is more considerable in the first
layers of metal deposited. On being heated, the iron loses gas,
even below 100°, the gas evolved at so low a temperature being
chiefly hydrogen. Iron which has been galvanically precipitated,
and then made red-hot and cooled, becomes oxidized when put into
water, that liquid being decomposed and hydrogen given off.
12. ZOOLOGY—ANIMAL MORPHOLOGY AND
PHYSIOLOGY.
MorpHonoey.
A new Ganoid Fish from Australia.—We have this quarter to
record what is certainly the most important zoological acquisition
which science has received since the finding of the Archopteryx
of Solenhofen. Mr. Gerard Kreft, the able curator of the Austra-
lian Museum of Sydney, who has already by his single exertions
shown us what a rich mine of new forms is still waiting to be
brought to the hands of science in the Australian continent, has sent
over photographs of a fish obtained in the rivers of Eastern Queens-
432 Chronicles of Science. [July,
land, which has at first sight very much the aspect of the African Pro-
topterus or South American Lepidosiren. The Queensland fish is,
however, larger than Lepidosiren, measuring nearly 5 feet in length.
A further examination of the photographs sent by Mr. Kreft shows
that the fins, which are long worm-like appendages in Lepidosiren,
with a very slight border of fin-rays, are here much more developed,
being broader and flat, with a large axial lobe and diverging rays,
something like those of Polypterus. The scales are large and solid-
looking—to judge by the picture—and with a wave-like sculpture on
the surface, recalling the paleozoic Holoptychius in this respect, as
well as in the long-lobed fin. The photographs of the skull display
a most formidable array of long, wedge-shaped teeth, with undulat-
ing edges, exceedingly like those of the Carboniferous Ceratodus.
The teeth are, in their limited number and position, very similar to
those of Lepidosiren, but have even a more marked resemblance to
Ceratodus than have the latter. Mr. Kreft was so struck with the
resemblance to Ceratodus that he has proposed to call this mar-
vellous fish, which he places with amphibians, Ceratodus Forster?,
after the gentleman who discovered it. The name Potamothawma
has, however, been also proposed, since we have no right to rele-
gate it to an extinct genus solely on the ground of agreement in
the teeth. It is impossible to exaggerate the importance of this
discovery with reference to the problems of the geographical distri-
bution of organisms, and the ancient relations of land and water.
On the other hand, this fish has an equal interest from the purely
zoological point of view. We believe that specimens are not very
difficult to obtain, so that some may soon be expected in this country.
How isit that no one has yet studied the development of Lepidosiren ?
Surely, now that in three-quarters of the globe such a fish has been
found, the eggs and. fry may be expected to be made known. It is
only quite recently that the development of Polypterus—the Ganoid
of the Nile—has been studied on the banks of its habitation, and
the fact that it commences life with large external gills like those
of a young Newt, or of a very young Tadpole, clearly established.
The Graphie Method in Odontology—tThe study of teeth, not
from the dentist’s but from the naturalist’s point of view, is of very
great importance, since by the power of drawing correct inferences
from a few teeth we are able to arrive at most weighty conclusions
as to the age of Tertiary and other strata. The study of teeth, par-
ticularly of mammalian teeth, has become quite a speciality—a little
field of knowledge requiring great care and perception of form for
its successful cultivation, and standing apart from other anatomical
work. So great is the amount of attention required in this study,
and so great the importance attached to it, that the late Dr.
Falconer occupied most of his life with the study of the teeth on
Elephas, Mastodon, and Rhinoceros; whilst a fellow of the Royal
1870. ] Zoology. 433
Society has been raised to that dignity because he had confined his
studies to the molar series of Rhinoceros and Hyena. Anything
which will simplify this study and reduce it to the level accessible
to ordinary minds must therefore be hailed with pleasure, and the
method which Mr. George Busk has devised is exceedingly valuable
in that way. Mr. Busk proposes to convert number into form in
the case of teeth, for increase of twentieths of an inch in breadth
using extension of a line, just as the mathematician proceeds in
drawing a curve representing progressive phenomena, The paper
ruled in fine squares of a tenth of an inch or so, which physiologists
and others make use of in recording rises of temperature or increase
of movement at successive intervals, is employed by Mr. Busk. To
obtain the odontogram of any mammal, you mark off as many hori-
zontal lines as there are teeth in the molar series; let each division
on the horizontal lines made by the perpendicular represent, say a
tenth of an inch; -then with compasses measure the breadth of your
first: molar, mark it with a dot on the first horizontal line in tenths
of an inch; then measure the second and mark it on the second line,
and so on for all seven—if seven there be. Your dots will now be
at various distances from the perpendicular zero line, according to
the breadth of each tooth: join the adjacent dots and you have an
irregular figure produced of definite form and characteristic of the
species. On the same set of lines you can now measure out the
lengths, or antero-posterior dimensions of the same teeth, and pro-
duce a figure overlapping your first figure, equally characteristic,
the two together giving an exceedingly accurate and trustworthy
means of comparing the dental series in allied species. With re-
gard to the teeth of some of the large pachyderms Mr. Busk hag
proposed certain points of measurement besides those of length and
breadth, which we may hope soon to see adopted. It would be an
inestimable boon to paleontologists if Mr. Busk would found a
system of measurements for all mammalian teeth, and publish at the
same time an authoritative series of such measurements with odon-
tograms of all the known recent and fossil mammalia. It at any
rate might be done with Rhinoceros and the Carnivora to begin with.
The Zoological Position of Sponges.—It is not three years since
in chronicling the discussions to which the glass-rope sponge, Hya-
lonema, gave rise, we had to mention that Ehrenberg the great
microscopist—who still is in Berlin outliving his age—holds to his
old belief that Sponges are Vegetals. We have now to record that
Professor Ernst Haeckel, of Jena, proposes to associate the Sponges
with the Corals and Hydromeduse, bringing them under the group
Coelenterata. Haeckel has attacked in former years that hetero-
geneous assemblage which we still know as the Protozoa; and he
removed from it the Infusoria proper, leaving the Sponges, the
Radiolarians, the Amceboids, the Foraminifera, the Gregarines, and
434 Chronicles of Science. [ July,
the Monera (a group of simplest forms which he himself discovered)
associated with the Flagellata and Diatomacez as Protista. Haeckel
now proposes—with very great propriety, we think—to remove the
Sponges from this company, with which they have no close relation
at all, their complex aggregated structure finding no parallel in any
of the other groups, and the fact that they are built up of amceboid
and ciliate cells in large measure, being absolutely as true for all
animals as for Sponges. ‘Two years since in the Canaries, Haeckel
was with his pupil, Miklucho-Maclay, and there the latter paid
particular attention to the calcareous Sponges, and both he and
Haeckel were much struck with the high degree of organization
which these forms presented. Haeckel has since studied the cal-
careous Sponges (which are represented by the genus Grantia on
our coasts) in the Adriatic; has found an immense number of new
forms, and has watched the development of a great number. He
now points out that the central orifice, or “osculum,” of such a
sponge as Grantia is homologous with the mouth of Ccelenterata ;
that the canals of the Sponge too are homologous with the canal-
system of Corals, though they open externally by the temporary
pores in the former. He describes a small form, Prosyewm, which
has not canals opening thus, but only the central orifice, and this
he considers very near to the common ancestor of the Sponges and
Nematophora (Corals, Hydre, Ctenophora), which he distinguishes
as Protascus. Haeckel can distinctly demonstrate an endoderm and
ectoderm in many Sponges, whilst in some of the Calcispongiz we
have the presence of those radiating septa or “antimera” so cha-
racteristic of Corals. The Calcispongize make the nearest approach
to Nematophora by the distinctness of the “persons” which they
present, each osculum, or mouth, and canal-system stands alone,
like a separate polyp. In other Sponges there is much fusion and
merging of persons into a common individuality—in various ways
which Haeckel explains—one of these consisting in the possession
of a single osculum by several persons. Professor Haeckel’s pro-
posal has already been attacked in England by Mr. Kent, of the
British Museum, who thinks that the osculum of a sponge cannot
be the homologue of the mouth of a sea-anemone, because the water
runs in at the latter but out at the former—really no reason at all
as far as homology is concerned. He also thinks Coelenterata differ
from Sponges in having free-will, which Sponges have not, and
declares the Sponges to be the head of the Protozoa.
Spermatophores in Fresh-water Annelids.—In the last number
of the ‘ Quarterly Journal of Microscopical Science,’ Mr. Ray Lan-
kester announces the discovery of these structures in the genera
Nais, Tubifex, Iimnodrilus, and Clitellis. Peculiar elongate bodies
fringed with slowly-moving cilia, and occurring in the seminal
receptacles of Clitellis and Limnodrilus, had been described under
1870. | Zoology. 435
the name Pachydermon by M. Claparéde as parasites, similar to
the well-known Opaline. Mr. Lankester having detected these
bodies in a new species of Limnodrilus living in ponds at Hamp-
stead, carefully examined their structure, and found that they were
simply closely-fitted masses of spermatozoa, held together by a
viscid cement, and with their tails projecting beyond this viscid
matter freely, and thus giving the appearance of ciliation. Further,
Mr. Lankester had observed exceedingly long coiling bodies in the
seminal receptacles of Nads, and he had no doubt from their struc-
ture that these also were spermatophores. This curious phenome-
non of the aggregation of the spermatozoa into definitely-shaped
masses after their complete development and separation from their
developmental aggregation, has been observed in Molluscs, Insects,
and Marine Annelids, but not hitherto in the Oligocheeta. It is
not easy to conjecture what purpose may be served in the worm’s
economy by this strange aggregation of the spermatozoa. The
appearance presented by the masses is very like that of a densely-
ciliated Infusorian, and they move gracefully along the stage of the
microscope as though endowed with an individual vitality, instead
of being but a spirally-interwoven mass of sexual particles. The
same number of the Journal contains an important paper by Pro-
fessor Cleland “ On the Structure of the Grey Matter of the Brain,”
and one by Dr. Van Beneden “On Nematobothriwm.”
Surface Life of the Ocean.— Lieutenant Ingram Palmer,
having a considerable talent for drawing, determined to investigate
the various minute forms of life which abound on the ocean surface.
He arranged a series of nets for towing behind the vessel to which
he was attached ; purchased a small microscope, and set to work to
examine everything and draw everything which came to hand.
The result is, a very large collection of beautifully-executed drawings
of minute crustacean larve, worms, Pteropodous Molluscs, Echi-
noderm larvee, and various adult Amphipods and Isopods of great
beauty, few being larger naturally than a pin’s head. The amount
of work and skill represented by these drawings is something enor-
mous, and yet they will probably prove of no scientific value. They
have been exhibited at the Geographical and Linnzan Societies, and
are now in a magnificent frame at the Admiralty. The talented and
persevering artist who produced them had absolutely no knowledge
of what he was drawing, and did not go to work with the critical
power of a zoologist, and hence he has drawn much that was well -
known before, and has often failed to give the details required for
zoological purposes, though his drawings are exceedingly clear and
accurate. A very little previous education in Natural History—
the opportunity for which ought to be given to every officer in Her
Majesty’s service—would have rendered Lieutenant Palmer’s great
talents available for science. It is to be hoped that the Admiralty
436 Chromeles of Science. [ July
will now grant him the time to study, so that when he again finds
himself afloat he may be able to do that service in zoological science
which his perseverance and artistic skill would ensure.
PHystoLoGy.
The Moving Force of a Single Cilium.—An interesting experi-
ment has been recently made by Dr. Jeffreys Wyman, of Cambridge,
Mass., and repeated by Dr. Bowditch, of Boston, now in Professor
Ludwig’s laboratory at Leipzig, which suggests to us the above
heading. If the ciliated membrane from the palate and fauces of
the common frog be carefully removed and stretched on a perfectly
smooth plate whilst quite fresh and moist, and on this surface a
weight be placed, its surface being carefully covered with a piece of
fresh peritoneum of the frog to prevent the contact of dead matter
with the cilia, it will be found that the weight is slowly moved
along by the force of the cilia, a weight of as muchas four grammes
being actually transported in this way—slowly but perceptibly.
Dr. Bowditch has varied the experiment by cutting off the head of
a frog and inserting a glass tube into the mouth, so that the ciliated
surface may work on the rod, and he has actually succeeded in causing
the head to move along the rod when ina horizontal position or but
very slightly inclined against the direction of movement, simply by
the ciliary power. It would be interesting to know the mechanical |
equivalent of asingle cilium ; that is to say, what fraction of a horse-
power, for instance, a cilium power may be.
The Movements of Wings in Fluight—lt is to Dr. J. Bell Petti-
erew, I'.RS., of Edinburgh, that the credit is due of first advancing
the view that during flight the movement of wings is such as to
describe a figure of eight if progression of the whole body be hin-
dered. In an elaborate investigation into the mechanism of flight
in yarious animals, insects, birds and bats, he demonstrated that the
structure was such as to provide for and necessitate this form of
movement; in fact, the wing should act as a reciprocating screw.
Whilst acknowledging that Dr. Pettigrew has the merit of first
giving this account of the movements of flight, Dr. Marey, of Paris,
the illustrious physiologist, who has so successfully applied the
graphic method to the study of the circulation and of muscular
contraction, has demonstrated the truth of Dr. Pettigrew’s inference
from structure by actual experiment. An insect’s wing being gilded
and a strong beam of light used, its movement could be followed
by the eye; also by allowing it to brush against a cylinder covered
with lamp-black, the figure of its movement was obtained. Dr.
Marey is now investigating by most ingenious methods the flight of
birds—with a view to determine exactly what is the effective part
1870.] Zoology. 437
of the stroke in the movement of the wing. The movement of the
wing itself is recorded by an arrangement with an electric current,
wires being connected with a small instrument carried on the bird’s
back. The impulse upwards or forwards is also recorded by means
of an elastic bag containing air, on the surface of which lies a piece
of lead: when a sudden movement occurs at right angles to the
plane of the lead plate, it compresses the air in the bag by its inertia,
and this movement is recorded by means of a tube, another bag and
a lever, as in the cardiograph.
Peregrinations of Cells in the Living Body.— The study of living
tissues to which Cohnheim’s views on inflammation (vz. that there is
no multiplication of the cells of connective tissue, but that pus cells
are extrayasated white blood corpuscles) have given rise, progresses
very rapidly in Germany under the hands of Von Recklinghausen
of Wurzburg, of Stricker of Vienna, of Rollet of Gratz, and their
pupils. It appears certain now that both white and red blood cor-
puscles do freely pass through the capillary walls in inflammation ;
but it is equally certain, from the admirable researches of Stricker,
that cells multiply in inflammation which are not white blood cells,
such as the stellate cells of the cornea, the corneal epithelium, the
connective-tissue cells of the tongue, and others which Stricker has
seen under his eyes commence and finish the act of division. Among
the most remarkable results recently obtained from this study of
living cells is the observation of Saviotti, that cells pass znto the
capillaries and small veins as well as out of them. He has seen
this frequently occur with the pigment cells of the frog’s web,
when inflammation was set up by dilute sulphuric acid, and the fact
was recently witnessed also in the laboratory of Professor Stricker,
of Vienna. . The pigment-cells deliberately advance to the capillary
wall, and passing through it are carried along in the circulation.
These facts as to living cells are so remarkable that some have been
inclined to suppose there is optical illusion. ‘They are, however,
now placed beyond doubt by repeated observation. Movements of
cells in the tissues may now be demonstrated in many parts as well
as the cornea, in the frog’s egg of the second day, in the brain, in
the foetal liver, in the skin (migrated cells of Besiadecki) ; and hence
K6lliker’s supposition that all cells at one time or other can exhibit
active movement is likely to be established. Recklinghausen has
kept an excised frog’s cornea alive for six weeks by supplying it
with fresh serum and attendimg to cleanliness; a wonderful proof
of independent vitality.
Physiology in Trinity College, Cambridge.—Trinity has lately
proved her claim to stand alone and at the head of the colleges in
Cambridge by the establishment of a preelectorship in pure physiology,
to which that able teacher, Dr. Michael Foster, of University Col-
lege, London, and Fullerian Professor in the Royal Institution, has
438 Chronicles of Science. [July,
been called. It is a peculiar source of gratification to Dr. Foster’s
friends that he is able to accept this chair, since at the beginning
of the year family bereayements and the threatening of serious ill-
ness held out but a gloomy prospect for future work. Dr. Foster
is now in good health and will enter on his duties at Cambridge in
October. When we remember that on former occasions as well as
quite recently, Trinity has expressed her willingness to make some
of her collegiate property available for the endowment of Professor-
ships in the University in natural sciences, and that her generous
intentions have been baulked by the ignorant parsimony of certain
of the smaller colleges, we cannot but congratulate her upon having
taken this step. It goes far to confirm the enumeration of Univer-
sities once given by a Trinity man, vzz. “ Dublin, Oxford, Cambridge,
and Trinity College.” We hope the college will provide Dr. Foster
with a large laboratory.
Laboratories in Amsterdam and London.—Professor Kuhne
has recently delivered an admirable discourse on the importance of
physiological research on the occasion of the opening of the grand
physiological laboratory which the city of Amsterdam has built for
him. ‘This laboratory and that of Professor Ludwig at Leipzig are
the most perfect in Europe, though there are many others coming
near to them. Ludwig’s laboratory is as extensive as the whole of
the Cambridge and Oxford laboratories taken together. There is
not even one physiological laboratory in England, though we may
hope to see one, at University College, as a memorial to Dr. Sharpey.
Kine’s College recently refused to build one, though Dr. Beale
offered to assist in the expense in a most generous way. A strong
attempt is being made to get something in the form of a laboratory
put up at the public expense through the Privy Council. Let us be
thanktul for any such movement.
1870.] (f4be-)
Quarterly List of Publications receited for Webiew.*
1. Researches on Diamagnetism and Magne-crystallic Action; in-
cluding the question of Diamagnetic Polarity. By John
Tyndall, LL.D., F.RS., &e. Longmans, Green, & Co.
2. Notes of a Course of Nine Lectures on Light, delivered at the
Royal Institution of Great Britain. By John Tyndall, LL.D.,
F.RS. Longmans, Green, & Co.
8. Other Worlds than Ours: the Plurality of Worlds studied under
the light of recent scientific researches. With Illustrations.
By Richard A. Proctor, F.R.A.S. Longmans, Green, & Co.
4, Alpine Flowers for English Gardens. By Wm. Robinson, F.L.8.
With Illustrations. John Murray.
5. Forms of Animal Life, being Outlines of Zoological Classification
based upon Anatomical Investigation, and Illustrated by
Descriptions of Specimens and of Figures. By George Rolles-
ton, D.M., F.RS., &e. Oxford: Clarendon Press.
6. Strong Drink and Tobacco Smoke: the Structure, Growth, and
Uses of Malt, Hops, Yeast, and Tobacco. With 167 original
Illustrations, drawn and engraved on Steel. By Henry P.
Prescott, F.L.S. Macmillan & Oo.
7. A Handbook of Phrenology. By ©. Donovan, Ph.D., &e. With
Illustrations. Longmans, Green, & Co.
8. Contributions to the Theory of Natural Selection. A Series of
Essays by Alfred Russel Wallace, F.R.G.8., &e.
Macmillan & Co.
9. The Ornithosauria: an Elementary Study of the Bones of Ptero-
dactyles, made from Fossil Remains found in the Cambridge
Upper Greensand. By Harry Govier Seeley. With 12 Plates.
Cambridge: Deighton, Bell, & Co. London: Bell & Daldy.
10. A Manual of Zoology for the Use of Students; with a General
Introduction to the Principles of Zoology. By Henry Alleyne
Nicholson, M.D., D.Sc. &c. Vol. I.: Invertebrate Animals.
R. Hardwicke.
11. L'Uomo e la Natura. Ossia la Superficie terrestre Modificata
per Opera dell Uomo. Di Giorgio P. Marsh.
Firenze: G. Barbera.
* We cannot undertake to acknowledge books and pamphlets
on purely theological subjects, nor such as concern betting
transactions.
440 List of Publications [ July,
12. Burton-on-Trent ; its History, its Water, and its Breweries. By
William Molyneux, F.AS. Triibner & Co.
13. The Fuel of the Sun. By W. Matthieu Williams, F.C.S.
Simpkin, Marshall, & Co.
14, Burton and its Bitter Beer. By J. S. Bushnan, M.D.
William S. Orr & Co.
15. A Star Atlas for the Library, the School, and the Observatory,
&e. With Two Index Plates with Coloured Constellation Figures.
Drawn by Richard A. Proctor, B.A., F.R.A.S., &., &e.
Longmans & Co,
16. On the Manufacture of Beet-root Sugar in England and Ireland.
By William Crookes, F.R.S., &e. Longmans & Co.
PAMPHLETS AND PERIODICALS.
On the Thermal Resistance of Liquids. By Fredk. Guthrie,
On Ocean Currents. By James Croll.
Records of the Geological Survey of India.
Notes of Fifteen Lectures (to Women) on Physics. Delivered by
Professor Guthrie at South Kensington Museum.
Descriptive Catalogue of One Hundred Microscopie Objects. Exhi-
bited at the Royal Microscopical Society by C. Stewart, F.L.S.
Notes on Diatomacez. By Professor A. M. Edwards. (Boston,
U.S.A., Natural History Society.)
Report presented to the Minister for Agriculture, &c., respecting the
Vaccinations performed in France in 1865 and 1867. Translated
by George 8S. Gibbs.
Report on the Present State and Condition of Pre-historic Remains in
the Channel Islands. By Lieut. 8S. P. Oliver, R.A., &e.
What Shall we Teach? or, Physiology in Schools. By Edwin Lan-
kester, M.D., F.R.S. Groombridge & Sons.
Biographical Sketch of the late Fredk. Penny, Ph.D., &c., Glasgow.
By James Adam, M.D.
The Currency Question. By Rigby Wason.
Report on the Agriculture of Belgium. By Dr. Augustus Voelcker
and H. M. Jenkins, F.G.S. (Reporter).
An Irish Farmer on the Land Difficulty. By J. E. Scriven.
On the Relative Safety of the Different Methods of Working Coal.
By Mr. George Fowler.
Stanford’s Geological Map of London.
A Guide to the Study of Insects. By A. S. Packard, jun., M.D.
Salem, Mass. London: Triibner & Co.
Notes on a Trip to the Nicobar and Andaman Islands. By V. Ball.
(Bengal Asiatic Society.)
1870. | received for Review. 441
Life and the Equivalence of Force. By J. Drysdale, M.D.
London: Turner, 77, Fleet Street. Liverpool: Holden.
Announcement of the Forthcoming Series of Annual International
Exhibitions. Science and Art Dept.
The Gardener’s Magazine.
Journal of Applied Chemistry. New York, éc.
The American Naturalist. Salem, Mass.
The Canadian Naturalist, and Proceedings of the Natural History
Society of Montreal. Montreal: Dawson Bros.
Revue Bibliographique Universelle.
The Geological Magazine. Triibner.
The Food Journal. Johns & Sons, Castle Court, Holborn.
The Popular Science Review. R. Hardwicke.
Scientific Opinion. 75, Great Queen Street, London.
The Westminster Review. Tribner.
Fraser’s Magazine. Longmans.
Longmans’ Notes on Books.
Williams and Norgate’s Foreign Book Circular.
PROCEEDINGS OF LEARNED SOCIETIES, &c.
Ofversigt af Kongl. Vetenskaps-Akademiens Férhandlingar.
Stockholm : Norstedét & Séner.
The Thirty-seventh Annual Report of the Royal Cornwall Polytechnic
Society. 1869.
Proceedings and Transactions of the Nova Scotian Institute of
Halifax, Nova Scotia. London: Reeves & Turner, 196, Strand.
First Annual Report of the American Museum of Natural History.
New York.
The Journal of the Historical and Archeological Association of
Treland. Dublin: McGlashan.
Transactions of the Geological Society, Glasgow.
Proceedings of the Bath Natural History Society and Antiquarian
Field Club. Bath: Chrenicle Office.
Proceedings of the Royal Institution of Great Britain.
s) » Royal Society.
Royal Astronomical Society.
22 99
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at a fixed charge of 30s. per sheet per 100 copies, including a
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’
x
ts
bins
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5
EDITORIAL ANNOUNCEMENT.
eee OS
Tuis number of the Quarterly Journal of Science brings to a
close a series which has for seven years been conducted under
one management, and as the periodical now passes out of the
hands of its present Editor, he craves permission to say a few
words concerning his stewardship.
Of the status which the Journal has acquired, it will be the
most becoming to say but little. The list of publications regu-
larly acknowledged in each number as having been received
from authors and learned societies in all quarters of the civilized
world, sufficiently indicates that it has found readers in every
clime and nationality, whilst the best criterion of its scientific
value is its list of contributors.
Amongst those who have from time to time communicated
to its pages the fruits of their labours or the result of their
reflections are the well-known names of ANSTED, CARPENTER,
Crookes, DAUBENY, FAIRBAIRN, FRANKLAND, GEIKIE, GLAD-
STONE, HerscHEL the Elder, Huaains, Hutt, Hunt, Lacaze
Dututiers, The LANKESTERS (father and son), MALLET, CHAL-
MERS Morton, NAsMyTH, ODLING, PENGELLY, PHILLIPS,
Ramsay, Rowiieston, Scott Russet, ScLATER, ANGUS
SmitTuH, SorBy, BALFouR STEWART, WILLIAM TURNER, ALFRED
WALLACE, and others hardly second to those in reputation.
Some of the foregoing, along with other earnest, sound, scientific
writers, have from quarter to quarter chronicled the progress
of scientific discovery, each in his particular branch, and only
once or twice during seven years does the Editor recollect
haying received a remonstrance for unfair criticism. But the
experience acquired during the past history of the Journal
clearly points to the necessity for a change in its management.
The names of CaurcHinL and Loneman are sufficient guarantees
that all has been done that was possible to make the Journal a
permanent contribution to our scientific literature. One defect,
however, has been the absence of its Editor from the centre of
English intelligence, and that will be henceforward removed.
In the interests of science only, the present Proprietors and
Editor have transferred the property and management of the
Journal to a gentleman whose name has been conspicuous on
its title-page from its commencement.
Mr. Witu1AmM Crooges, F.R.S., Editor of the ‘Chemical
News,’ of 3, Horse-shoe Court, Ludgate Hill, will henceforward be
the sole Proprietor and Editor of the ‘QuarTERLy JoURNAL OF
Science. He is a valued friend of the present Editor, who will
continue to give him his cordial and earnest support, and who
now solicits for his successor the same kind consideration as he
has himself received from his collaborateurs and from the
readers of the Journal.
~ Tue Eprror.
THE QUARTERLY
JOURNAL OF SCIENCE.
OCTOBER, 1870.
I, THE ECLIPSE OF AUGUST 7, 1869.—“ ANVIL”
PROTUBERANCE.
By W. 8. Gimmay, jun., New York.
THosE who observed the solar eclipse of last August with a sizeable
telescope will not soon forget the startling effect produced by the
appearance of the large oval protuberance on the western limb of
the moon. We were unusually favoured as to atmosphere at our
station near Sioux City, Iowa, and when in addition to this it is
stated that our observations were made by the aid of a 4-inch re-
fractor—one of Mr. Alvan Clark’s best—it will not seem strange
that the details about to be recorded were so readily obtained.
The “anvil” protuberance, for such the object is recorded in
my notes, was seen by one of our party several moments prior to
the totality. :
Several months’ study of the sun’s surface had prepared me to
expect the more remarkable protuberances in the southern hemi-
sphere, and having selected the south-western quadrant as an
especially favourable locality, from the presence of faculous ridges
near the limb two days prior to the eclipse, the bright “ anvil ”-
shaped mass instantly attracted my attention. Its extraordinary
brilliancy enabled me afterwards to keep it in view when a con-
siderable crescent of the reappearing sun had rendered the corona
invisible.
A hasty glance at other portions of the moon’s limb satisfied
me that the “anvil” protuberance possessed greater interest than
any other, and I therefore devoted my whole time to its considera-
tion, except so much as was employed in obtaining several outline
sketches of the corona.
In a forecast of the probable positions of protuberances, which
I made on August 5 (see Fig. 1), the double prominence at A
occupies very nearly the position of the object under discussion. In
Fig. 2 we have the appearance of the sun’s disc on the same day,
and near that part of the limb subsequently occupied by the
“anvil,” we notice a cluster of bright faculous spots. It was the
VoL. VII. 248
444 The Eclipse of August 7, 1869. [Oct.,
Bre, at;
OQ: ROSE PROTUBERANCES AS FORECASTED
AUGUST 5, 1869.
Fig. 2.
Solar disc, August 5, 1869.
1870. | The Eclipse of August 7, 1869. 445
intense whiteness of these objects that led me to suppose there
might be hovering above the solar surface in this region gaseous
exhalations that would appear during the eclipse. The white
meridian in this second diagram represents the limb of the sun
for the 7th of August, and it will be noticed that the cluster of
facule is just beyond this line. A similar white meridian in the
diagram giving the appearance of the sun on the 9th of August
(Fig. 3), indicates the eastern limb of the sun during the eclipse.
Fie. 3.
Solar disc, August 9, 1869.
In this latter instance we have the faculous ridges marked
I, G, F, E, which may be referred to prominences 4, 5, 6, and 7
of Prof. Mayer’s diagram. It is worthy of special notice that the
faculous masses at 1 are very irregularly disposed, the tortuous
windings of its parts suggesting whirling motions in the photo-
sphere. Prof. Mayer’s “Eagle” prominence is a fit object to
hover over such a curiously-agitated portion of the solar surface.
That my sketch gives a correct representation of the windings of
these ridges of facule I feel quite confident. While making the
observation the outline was likened to a rude drawing of a camel
(Fig. 4). The resemblance may appear to some if the page is
inverted, the camel being supposed to face to the left. |
Fig. 5 isa copy of my sketch of the spots on the sun’s disc, as
they appeared an hour previous to the eclipse. There was little or
no change in their form or position until after the close of the
phenomenon. The large spot near the eastern limb, enveloped
in a platform of facule, is the same as that visible on the 9th
(Fig. 3) near the same locality.
2H 2
446 The Eclipse of August 7, 1869. {Oct.,
I was particularly impressed with the stability of the protuber-
ance. It resembled a monstrous white-hot coal, and its outlme
=
Fig. 5.
DIAGRAM SHOWING SPOTS ON THE SUN DURING THE
ECLIPSE, AS SKETCHED ONE HOUR PREVIOUS TO THE
FIRST CONTACT.
was sharp and well defined. The appellation “sosy protuberance ”
struck me at the time asa misnomer. I detected only bright fire-
orange tints, like the glowing coals of an anthracite grate, with
delicate crimson flakes of surprising brilliancy scattered over the
southern part.
These flakes stood out against the bright background as if
totally disconnected from the rest of the phenomenon. In the plate
I have endeavoured to give their positions and the direction of their
axes, which latter coincided with the stratification of the protuber-
ance. I should estimate the length of these brilliant dashes of
crimson light at from 3” to 5”. Possibly in a future eclipse a
momentary spectrum of them may be obtained, as their extra-
ordinary brilliancy may make amends for their minute size.
The plate accompanying this article was prepared from my
observations of the great protuberance, with the exception of the
outline of the mass, which was obtained from the last Ottumwa
; i Achy Dh ry
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ah
Jr of Fr Inst: Vol. LIX. The Anvil Prominence
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.
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THE “ANVIL” PROTUBERANCE
OF THE TOTAL ECLIPSE OF AUG. 7 1869. FROM SKETCHES
AND NOTES MADE DURING TOTAiLIT Y
AT ST PAUL JUNG" IOWA.
OUTLINE TAKEN FROM THE PHOTOGRAPHS
1870. | The Eclipse of August 7, 1869. 447
photograph of the totality. In preparing this illustration the litho-
grapher has been very successful in copying my sketch, the plate
as given recalling the protuberance to my mind with great fresh-
ness and power. The flaky structure of the protuberance I have
endeavoured to indicate by a deeper tint of orange running diago-
nally across the flame. The southern end is more compact than
that turned towards the equator, which latter breaks up into
several smaller independent clouds, between which, and suspended
fully 10,000 miles above the solar surface, projects the tapering
point of the “anvil.” A casual glance at the sketch impresses one
with the idea of a down-rush of the glowing matter from the
southern end to the “anvil” point.
The details of the termination of this tapering end are wholly
from my notes, which record that this part of the protuberance
was composed of “fibrous lines of flame” apparently in motion
and emitting a tremulous light. I have now a vivid recollection
of the impressions produced upon my mind by this portion of the
phenomenon which riveted my attention for some moments. In
the photographs the tapering end of the protuberance terminates
in a misty ball, which is what we should expect if the fine lines
revealed by the telescope were really in motion.
~~ One word regarding the corona. By a slight movement of my
instrument its limits were brought into view, and its extent quickly
indicated on diagrams previously prepared. At the same time I
indicated by two heavy pencil-marks the positions of certain bands,
or inéervals, in the light of the corona on opposite sides of the
moon’s disc. These dark intervals deserve a passing notice.
In my coloured sketch of the corona, made immediately after
the eclipse, and which accompanies my report published by the
Washington Naval Observatory, I have indicated the positions
and character of these bands. The absorption bands of the solar
spectrum occurred to me at the time as an illustration of the
delicate striations in these portions of the corona. In the case of —
one gap a multitude of fine violet lines were compressed into a
space of about 10° in width, forming, to my mind, one of the most
beautiful features of the eclipse. The same striated appearance
was noticed in other regions of the corona, though in a less striking
degree.
These apparent gaps in the corona’s light I judged to be
opposite elevated portions of the chromosphere, from the fact that
there was a similar diminution of light above the great protuber-
ance, as my sketches show. ‘This point was not carefully examined,
however, from want of time. On my return from the south, in
February last, it occurred to me to compare my sketch of the
corona with the diagram of protuberances accompanying Professor
Mayer's report m the October number of the ‘Journal of the
L
448 The Surveys of India. — ~ [Oct.,
-Franklin Institute,’ published in Philadelphia. This I did, for
the first time, on the 9th of that month, finding a fair agreement
between the eauteea portions of his prominences 5 and 10, and
the dark bands given in my sketch. I have, therefore, little doubt
but that in locating these dark intervals in my original sketches, I
intended to place the western one near 285°, and the eastern one
near 120°, great exactness not being obtainable in the few moments
given to the observation. In speaking of these bands as dark, I
would be understood only as meaning that they were sufficiently so
to be readily seen.
A comparison of the Des Moines and Ottumwa pictures of the
“anvil” protuberance gives the following measurements. It will
be noticed that the figures are somewhat in excess of those obtained
from the last totality picture made at Burlington.
ry Miles.
Extreme length of the “anvil” .. . . 265 or 119-800
base of the “anvil”... .. 205 » 92°500
Greatest altitude above the sun’s surface ees hewn, RSE: Si, .) ee
Thus if, as is probable, the entire protuberance was not visible,
its base being beyond the sun’s limb, we have a bright cloud im the
solar atmosphere nearly, if not quite, equal in volume to the planet
Jupiter, and which in the direction of its length would sufiice to
reach more than half way to the Moon in her perigee.
THE SURVEYS OF INDIA.
II, THE TRIGONOMETRICAL SURVEY.
(With a Sketch-map.)
By F. C. Danvers, A.I.C.E.
Tue surveys of India may be divided into two classes—viz. the
Great Trigonometrical, and the Geological. In connection with the
former, other minor operations are undertaken under the title of
topographical and revenue surveys, to which we shall refer more
particularly in due course.
The idea of a great trigonometrical survey of a country, to be
undertaken by the Government of that country, was first conceived
by General Watson, at the suppression of the rising in Scotland in
1745. The execution of it was committed to General Ray, and
was originally intended to extend no farther than the disaffected
districts of the Highlands. The design, however, was subsequently
enlarged, and the grand trigonometrical survey of Great Britain
Quarterly Journal of Science N° XXVIII.
COREE MAP ©OF, .ENDIA
shewing the Principal Triangulation Series
of the
GREAT TRIGONOMETRICAL SURVEY.
AA. The Great Arc Series _
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NVIGVAV
1870.] The Geological Survey of India. 459
With his small band of Geologists, the Survey was carried on
with vigour, and periodical reports were published, accompanied by
maps, geologically coloured, and sections of the country described.
The value of the establishment was soon appreciated by the
public, and numerous applications for reports on geological matters
were made, as well as for aid in analyses of coal, minerals and ores,
of soils, water, and in assays. Such information and assistance was
given to many private individuals, as well as to Government depart-
ments and to companies.
The earlier observations were, as might be expected, fraught
with much difficulty. But few and isolated notices, compared with
the size of the country, had been written upon it. The labours of
Dr. Carter, of Bombay, of the Revs. Hislop and Hunter, Presby-
terian missionaries in Tinnevelly, and some others, had certainly
done a little towards paving the way for a classification of the
rocks; and Mr. Greenough had, in 1854, after many years’ labour
in compilation, prepared a map of India, upon which he had
depicted all that was then known concerning the geology of the
country.
Dr. Oldham,* however, found it necessary to establish several
new groups to receive (provisionally) the various rocks that were
met with, inasmuch as for many—and these some of the most
widely-extended and important groups of rocks—there was no
definite horizon from which to work either up or down. Over
thousands and tens of thousands of square miles not a fossil was
found, save some vegetable remains, affording, at the best, but very
imperfect evidence. The richly fossiliferous rocks of the Himalaya
and Sub-Himalaya being widely separated from all the rocks of the
Peninsula by the broad expanse of the Alluvium which unites the
valleys of the Ganges and Indus, it was impossible to trace out,
by their aid, any superposition. |
To endeavour to remedy this, it was found advisable to examine
many distinct tracts, and to make more or less rapid observations on
distant parts, which, although interfering with the continuous pro-
gress of the Survey, were generally of essential service in leading to
definite results on important geological points, which, in the ordinary
progress of the work, could not have been arrived at for many years
to come.
The climate of India necessarily restricts the work to certain
portions of the year. The working season lasts about seven months,
and differs very materially in the southern part of the Peninsula
from that in Bengal. In the latter district, the close of the Indian
financial year (the 31st March) nearly coincides with the close of
the field season. In Madras the season is then not half over.
* See Mr. Horner’s Anniversary Address to the Geological Society of London.
61.
VOL. VII. a i
460 The Geological Survey of India. [ Oct.,
Considering the great exposure to which all field-geologists
working in the open country are unavoidably subjected, and the
necessity for their visiting, and often remaining in, the most mala-
rious and unhealthy parts, it is not surprising to learn that the
whole staff are seldom at work at one time. The illness of one or
more, and the necessity for leave of absence, is generally recorded in
the Annual Reports. But it is grievous to learn the loss by death
of five or six officers since the Survey has been in operation, whilst
several have been forced to resign from ill-health.
These causes have occasioned much loss of time. It is seldom
possible, Dr. Oldham remarks, to meet with persons qualified to
supply the vacancies immediately. There is, moreover, absolute
necessity for a considerable amount of training, occupying gene-
rally a year, before any newly-appointed Assistant can become
really useful, and able to carry on alone the mapping of a district.
The pecuniary temptations furnished to individuals to join the
Survey are not very great, the maximum ratio of pay being 500
and 600 rupees per month, but this is only obtainable after eight
or ten years’ service. The salary, as on the British Survey, is very
fair to commence with, but equally discouraging in prospect.
The latest report of Dr. Oldham, dated the 3rd January, 1870,
is accompanied as usual by an index-map, showing the area surveyed,
and published to the end of 1869, and that in progress. A reduced
copy of this map accompanies our notice.
The Atlas of India, which includes Burmah and the Malay
Peninsula, comprises about 180 sheets, portions of about 64 of
which have been mapped, while others have been visited and re-
ported upon.
A very large area has not yet been surveyed topographically,
so that the direction of the detailed mapping by the Geological
Survey has some restrictions. ‘The size of the sheets is 3 feet
41 inches by 2 feet 34 inches, and each contains an area of about
17,824 square miles.
The principal part of the work has been carried on in Central
India. The faultiness of the existing maps of the country was found
a serious drawback to successful progress, but so far as possible they
were corrected, and every effort was made to render them of the
utmost service. It was soon found, however, that the character of
the geological work must be suited to the available maps of the
district, and with very imperfect maps to attempt great detail
would be useless. For all practical purposes, the boundaries of
the geological formations could generally be fixed with sufficient
accuracy.
But few sheets have been entirely surveyed. This, however,
would be accounted for by the necessity, previously stated, of ex-
amining many different and distant parts for the purpose of arriving
1870] The Geological Survey of India. 461
at a classification or knowledge of the order of superposition of
the rocks in India; and when the vast area embraced by each sheet
is taken into consideration, it is not surprising that few have been
completed.
A glance at the map best shows the amount of field-work that
has been done, and considering the many difficulties and dangers
that have had to be encountered—not forgetting the disturbed state
of the country during the Indian mutiny in 1857—we must con-
eratulate the Survey on the great progress it has made.
Besides the preparation and publication of the geological maps,
the Survey now maintains three periodicals of letter-press.
The first part of the ‘Memoirs’ appeared in 1856, and since
then six volumes have been completed, containing thirty-two geolo-
gical reports (over 2200 pp. of letter-press), and the first part of
vol. vil. has recently been published. All are well illustrated with
maps and sections.
Particular attention has been given to the coal-bearing deposits.
The ‘ Memoirs’ contain reports on the Coal-fields of Talchir, Rani-
gun], Jherria, Bokaro, Ramgurh, &c.
The coal-fields of Bokaro and Ramgurh belong to the ordinary,
or Damuda series.
In the Jherria coal-field, the two series, Talchir and Damuda, are
developed.
The lower, or Talchir, contains no coal.
The Damuda series contains many seams, very irregular, and
varying in thickness from a few inches to 20 feet and more. Nume-
rous coal-seams are much injured by trap-dykes, which have ramified
through them, and which have rendered the coal useless. There
is also a general tendency to ignition in all the seams, owing, it is
thought, to the presence of iron pyrites, which gives rise to spon-
taneous combustion. Metamorphism is produced in the shales in
proximity, giving to them the character of well-burnt bricks.
Dr. Oldham calculates that there is an available quantity of coal
in this Jherria field of about 465,000,000 cubic yards, or, roughly,
tons of coal.
In Sinde there is a lignitic coal of Lower Tertiary age, but not
worth working. In one of his earlier reports Dr. Oldham noticed
the existence of Tertiary coal by the river Irrawaddy, near Prome.
Coal of excellent quality has been found in Assam, which lies
near the river Brahmapootra, convenient for transport by water.
Considerable doubt attached to the age of the coal-fields of
Damuda, Talchir, and Nagpur. ‘The reported discovery in them
of certain plants was thought to place them in the Triassic or
Oolitic period. But it has since been ascertained that these re-
mains occur in shales above and distinct from the Coal-measures.
Comparisons have been made of late between the several series
ya
462 The Geological Survey of India. [ Oct.,
of sandstones, &c., associated with the coal in Bengal and those of
Central India. ‘The vast extension and great constancy in mineral
character of the Talchir rocks (which form the base of the great
coal-bearing series) have been fully established, and the thinning
out of the beds in passing to the west has received further support.
The entire Coal-formation, which in the east gives five well-marked
subdivisions (in ascending order, Talchir, Barakar, Ironstone shales,
Ranigunj, and Panchet), becomes, at a short distance to the west,
only a threefold series, comprising the Talchir, Barakar, and Panchet
subdivisions. Additional proofs have been brought forward to show
that on the large scale, the present limits of these Coal-measures
coincide approximately with the original limits of deposition, and
are not the result of faulting, or even mainly of denudation.
And Dr. Oldham expresses his opinion that the great drainage
basins of India were on the large scale marked out, and existed (as
drainage-basins) at the enormously distant period which marked the
commencement of the deposition of the great plant-bearing series.
In this point of view, local variations in the lithological type, local
variations in the thickness of the groups, and even their occurrence
or non-occurrence, are only necessary consequences of the mode and
limit of formation.
In 1861 Dr. Oldham gave a summary statement of the amount
of coal raised throughout India for the past three years, which was
about 850,000 tons. The total amount of coal raised in India gene-
rally was, in 1858, about 226,140 tons; in 1859, about 347,227 tons;
and in 1860, about 370,206 tons. Of this quantity the Ranigunj
field yielded by far the greater part. The only mode of transport,
however, from this field was by the river Damuda, a stream only
navigable during the freshes of the rainy season, after which it be-
comes so dry that no more coal can be sent to market until the
next season.
In 1867 Dr. Oldham made a report on the Coal-resources of
India.* The extensive fields which occur are not distributed gene-
rally over the country, but are almost entirely concentrated in one,
a double, band of coal-yielding deposits, which with considerable
interruptions extends more than half across India, from near
Calcutta towards Bombay.
Little more than surface workings are carried on—the deepest
pits scarcely exceed 75 yards, while certainly one-half of the Indian
coal which has been used up to the present date has been produced
from open workings or quarries.
Dr. Oldham concludes that out of the whole series of Indian
coals, the very best of them only reach the average of English coals,
and that on the whole they are very inferior to them. It should,
however, be borne in mind that until all the fields are carefully
* Being a return called for by the Right Hon. the Secretary of State for India.
1870.] The Geological Survey of India. 463
mapped, any estimates of the Coal-resources and production of British
India must be defective.
Besides the coal-reports, the ‘ Memoirs’ contain papers on the
gold-bearmg and other economic deposits, also many describing
the geology generally and physical geography of particular areas.
Some few treat of paleeontology.
One very important paper describes the Vindhyan series, as
exhibited in the North-Western and Central Provinces of India.
The district described included the greater part of Bundelkund. The
Vindhyan series is divided into an upper and a lower division, the
former gives rise to great table-lands, the latter furnishes more
diversified scenery. The area affords many striking instances of
the power and effects of subaérial denudation on a grand scale. As
yet the Vindhyan rocks have yielded no fossils; they appear to be
older than the Talchir, and may possibly turn out to belong to a
period about the age of the Devonian. Lithologically they consist
of alternations of limestones, shales, sandstones, and conglomerates,
often distinguished by local names, as for instance the “ Bijigurh
shales.” Some of the beds furnish good building stone.
Tn order to gain a more rapid publication of many isolated facts
noticed during the progress of the Geological Survey, and which
were scarcely adapted to the ‘ Memoirs,’ a new publication called the
‘Records’ was started in 1868. The series contains notices of the
current work of the Survey, lists of contributions to the Museum
and Library, &c., and it is intended also to publish analyses of such
books published elsewhere as bear upon Indian geology, and gene-
rally to notice all facts which come to light illustrative cf the
geology of Hindostan. The third volume is now in course of
publication.
Among the numerous published Reports the following appear
most worthy of special notice.
The Surat Collectorate,in the Bombay Presidency, although a
comparatively flat country, possesses many features of geological
interest. Traps, ranging from basalt to a soft shaly-looking amyg-
daloid, are met with, and resting unconformably upon these is the
great Nummulitic series. This consists of sandstones, conglome-
rates, and limestones, with nummulites, molluscs, fossil-wood, and
fragments of bone. Alluvium covers a large extent of the district,
and the cotton (or black) soil covers it over many large tracts of
the country. This soil seems to be the residuum left by the decom-
position of an alluvium largely composed of volcanic (trappean)
débris. It usually occurs in districts in which trap-rocks abound,
as for example in the Poorna valley, West Berar.
The Poorna alluvium is of considerable depth, in places about
150 feet. Much of it produces efflorescences of salts, chiefly of
soda; and in many places the wells sunk in it are brackish or salt.
464 The Geological Survey of India. [ Oct.,
Comparisons have recently been drawn between the Alluvial
deposits of the Irrawadi and the Ganges. Every river that dis-
charges its waters into the sea has the character of its deposits
influenced according to whether the area be im a state of subsidence,
quiescence, or of elevation. Generally in every large river-basin
two distinct alluvial deposits will be met with. The older of these
may be either marine (estuarine) or fluviatile (lacustrine), or of a
mixed and alternating character ; but the newer group is essentially
fitivio-lacustrine, and directly produced by the existing river. While
no very great thickness of the newer stratum can anywhere have
been deposited without a corresponding subsidence of the area, a
very large accumulation of the older or estuarine deposit may have
taken place during an elevation of the area covered by it.
The Ganges and Irrawadi present examples of rivers subjected,
respectively, to the former and latter conditions. The alluvium of
the Ganges, as ascertained from a well-boring at Fort William, con-
sists of 70 feet of the newer or fluviatile deposit, resting on the
denuded surface of the “‘kunker clay.” This clay is regarded asan
estuarine deposit accumulated durmg an upward movement of the
land. The Gangetic area is now considered to be undergoing de-
pression at a rate adequately counterbalanced by the accession of
sediment brought down by the river. The alluvium of the Irrawadi
belongs almost entirely to the older group, this river-delta being at
the present time in precisely the same condition as was the delta of
the Ganges when the first layers of its alluvium, 70 feet below the
present surface at Calcutta, were being deposited. The difference
in the fertility of the two areas is attributed to the greater richness
of the newer alluvium, and hence the inability of the delta of
the Irrawadi to compare with that of the Ganges in agricultural
produce.
The geology of the neighbourhood of Madras is noticed in the
third volume of the ‘ Records.’ The greater part of this district is
occupied by rocks of Secondary, Tertiary, and Recent ages, the re-
mainder is taken up by metamorphic rocks, forming part of the great
gneissic series of Southern India. Some time previously, beds of
magnetic iron-ore were pointed out in the metamorphic gneiss rocks
of the Madras Presidency, the supply of which was considered to be
practically inexhaustible.
The Rajmahal plant-beds consist of conglomerates, sandstones,
gritty clays, and shales.
The Laterite deposits are also pointed out. They comprise
clayey conglomerates, gravels, and sands, which graduate one into
the other. The gravels contain pebbles of quartzite and gneiss,
mixed with pisiform ferruginous pellets. Other deposits called the
Conjeveram gravels are noticed; they differ from the laterite beds
in the absence of ferruginous matter. Both appear to contain imple-
1870. | The Geological Survey of India. 465
ments of human manufacture in the shape of axes and spear-heads
made of chipped quartzite pebbles, and of the same types as those
which occur in the gravels of Western Europe. ‘They were spread
rather widely over a large extent of area in the country to the west
and north of the city of Madras, and have been made of the best
substitute which this portion of the country could afford for flint,
vamely, the very hard and semi-vitreous quartzites of the Cuddapah
series.
In gravel, situated near Pyton on the banks of the Godavery,
an agate-flake has been found, which is undoubtedly an artificial
form. It is figured in vol. i. of the ‘ Records.’
We have but briefly and imperfectly noticed a few of the more
important results arrived at by the energetic labours, in the field, of
Dr. Oldham and the officers of the Geological Survey. This work—
superintended by Dr. Oldham—has been carried out by the many
able assistants who have served under him, among whom we may
mention H. B. and J. G. Medlicott, H. J. and W. F. Blanford,
C. AX. Oldham,* W. Theobald, jun., F. R. Mallet, A. B. Wynne,
KR. B. Foote, T. W. H. Hughes, W. King, jun., I’. Fedden, &c.
We will now turn our attention to the paleontological work.
A Museum of Economic Geology was established at Calcutta in
1840, and in 1856 it was placed in connection with and under the
same superintendence as the Geological Survey of India. There are
also Museums at Madras, Bombay, and Kurrachee.
During the progress of the Survey numerous fossils have been
collected, and specimens are being constantly added to the Museum.
Indeed Dr. Oldham reports that they increase so rapidly that no
room can be found for their proper exhibition, and in the examina-
tion and description of them it is impossible to keep pace. During
the year 1869 more than 20,000 specimens passed through the
hands of the curator and his assistant. A suitable building is, we
are informed, now in course of erection at Calcutta, where the fine
collections already brought together will be properly arranged and
exhibited.
One of the more richly fossiliferous tracts is at Spiti and Rushpu
in the Himalayas, where representatives of Silurian, Carboniferous,
Triassic (Lilang series), Rheetic (Para limestone), Lower and Middle
Lias, and three subdivisions of the Jurassic period, and also Creta-
ceous rocks are believed to occur.
In order to figure and describe the species of organic remains
collected by the Survey, the ‘ Palzeontologia Indica’ was instituted.
This quarto publication is issued in fasciculi, each containing about
six plates, and published once every three months. Five series of
these fasciculi have been published.
_ * This able geologist died 30th March, 1869, aged 37 years. See Obituary,
‘Geol. Mag.,’ vol. vi., p. 240.
466 The Geological Survey of India. | Oct.,
The jirst series was printed in 1861, and treated of the Fossil
Cephalopoda of the Cretaceous rocks of South India, containing the
Belemnitidz and Nautilide, by H. F. Blanford ; the Ammonitidz,
by Dr. F. Stoliczka, formed matter for the third series.
The Cephalopoda were found to include 146 species, of which
nearly one hundred were Ammonites, three only Belemnites, whilst
of Nautilus there were 22 species, &c. Thirty-seven of these
species were found identical with species Known in Europe and
other countries. Ninety-six quarto plates are devoted to the illus-
tration of these fossils.
The Gasteropoda of the Cretaceous rocks form the subject of the
jifth series; they are illustrated with sixteen plates, and are de-
scribed by Dr. Ferdinand Stoliczka.
Two hundred and thirty-seven species of Gasteropoda are de-
scribed. Among them, four species of Helicide are deserving of
special attention from the rarity of land-shells in these Cretaceous
rocks, and particularly as they are said to belong to types still found
living in the same or neighbouring districts.
Dr. Stoliczka considers that the South Indian Cretaceous deposits
only represent the Upper Crgtaceous strata, beginning with the
Cenomanien. The larger number of representative species were
found to agree with the Turonien. The original notion of repre-
sentatives of Neocomian beds existing in South India loses support
from the more complete examination and comparison of the species.
The second series of the ‘ Paleontologia Indica’ is devoted to
the Fossil Flora of the Rajmahal series (Jurassic), six iasciculi of
which have been published. The descriptions are by Dr. Oldham
and Professor Morris. The Rajmahal beds occur near Madras, in
Bengal, and Kutch. Ai Madras the beds contain no carbonaceous
matter, which in their equivalents in other parts of India occurs so
largely as to form coal-seams. The plant-remaims occur chiefly
in a white shale. They include Palzozamia, Dictyopteris, Tzni-
opteris, Pterophyllum, Pecopteris, Stangerites, Poacues, &c.
The fourth series on the Vertebrate Fossils of the Panchet rocks
is by Professor Huxley, and is illustrated with six plates. These
remains consist of numerous fragmentary and sometimes rolled
bones, the majority being vertebre, with a few teeth, portions of
crania, &c. They were discovered in a stratum of conglomerate
sandstone exposed by the Damuda river near Deoli, fifteen miles
west of Ranigunj, and they are of great interest as being the first
remains of vertebrata discovered in the great group of rocks associ-
ated with the coal-bearing formations of Bengal. They proved to
belong to a peculiar group of fossil reptiles (Dicynodontia) hitherto
only known from South Africa. The strong analogy which these
South African rocks offer to some of the Indian rocks had been
insisted on by Dr. Oldham, before this discovery, on the strength of
1870. | Rainfall in England. 4.67
the plant-remains alone, and this has been strangely confirmed by
the discovery of reptiles of the same type (Dicynodontia).
Very many years must necessarily pass away before the Geolo-
gical Survey of India is completed, nor can Dr. Oldham and his
present staff hope to see its accomplishment, but they have done
sufficient already to indicate the great geological features of the
country, and we may hope to see in one of their future publications,
a table of succession of the Indian strata as far as at present deter-
mined, with their probable European equivalents.
IV. RAINFALL IN ENGLAND.
By W. Pencetty, F.R.S.
As regularly as the new year comes, and very speedily afterwards,
come Mr. Symons’s ‘ British Rainfalls, containmg the well-tabu-
lated results obtamed by many hundreds of rain observers whose
gauges are spread over Great Britain and Ireland, as well as the
adjacent isles.
The data contained in these annual publications are of great
interest, not only in themselves and as they stand, but because they
are capable of being worked up and discussed in various ways, some
of which I will now proceed to illustrate.
The Rainfall of England and Wales——During 1869, there
were in Great Britain south of the Tweed and Solway no fewer
than 1093 gauges at work, giving an average of about 21 for each
county, but, as may be supposed, without any approach to uni-
formity of distribution. They were most thickly strewn in Middle-
sex, and most sparingly in Montgomeryshire, there being one gauge
for every 59783 acres in the former, and for every 284,060 acres in
the latter ; that is relatively about forty-seven times as many gauges
in the one as in the other. On the average, there was in the entire
kingdom one gauge on every 34,149 acres; hence, were the distri-
bution uniform, each gauge in England and Wales might be supposed
to occupy the centre of a square measuring 7:3 miles in the side.
It is eminently creditable to the zeal and perseverance of their
meteorologists that the mountainous and thinly-populated counties
of Carnarvon, Cumberland, and Westmoreland, were amongst those
in which the relative number of gauges exceeded the average for the
entire country; thus for every ten gauges in England and Wales
as a whole, there were 10°5 in Carnarvonshire, 18°4 in Cumber-
land, and 25:5 in Westmoreland. In the last, moreover, there
were no fewer than twelve gauges on ground upwards of 1000 feet
above the sea, three upwards of 2000 feet, and one at the height of
468 Rainfall in England. [ Oct.,
3200 feet. Westmoreland had five gauges more than 1000 feet
high ; and though Carnarvon had none exceeding 850 feet in height,
the returns from every gauge in the county were in every respect
complete, as they contained full information as to height above the
sea and the ground, the total annual rainfall, the number of wet
days, and therefore of the average wet-day rate of rain.
The stations varied in height from the sea-level, at Hull, to
3200 feet above it, at Scafell Pike in Cumberland. ‘The least
county average height was 53 feet, in Cambridgeshire; the greatest
was 715 feet, in Radnorshire; whilst that for the entire kingdom
was 297 feet. This general average was surpassed in twenty-five
counties, but not reached in the remaining twenty-seven.
The tops of the gauges were by no means at one uniform height
above the ground on which they stood. In several cases they were
level with the surface, whilst one at Cockermouth was 100 feet
above it. ‘Taking the counties as separate wholes, the least average
height was 13 inches in Leicestershire, and the greatest 8 feet
7 inches in Cambridgeshire; while the mean height for the entire
country was 2 feet 9 inches. This general average was exceeded in
twenty-four counties, but not reached in twenty-six.
During the four years ending with December 31st, 1869, the
least annual rainfall at any station was 7°84 inches—the receipts in
1869 of a gauge at Sheerness, the top of which was 70 feet above
the ground and 79 feet above the sea; whilst the greatest was
207°49 inches, received in the same year, in a gauge 6 inches
above the ground, and 1077 feet above the sea, at the Stye in
Cumberland. During the four-year period just named the average
annual rainfall in the different counties as separate wholes varied
from 68°91 inches in Cumberland to 22°55 inches in Bedford-
shire; the average for the entire kingdom being 35°37 inches.
The three numbers were as 195: 63:100. The general average
was exceeded in eighteen counties but not reached in thirty-four ;
the former, or “ wet” counties, being to the latter, or “dry” ones,
as 1:2 nearly.
According to the Registrar-General, England and Wales con-
tain 37,324,915 statute acres; hence, with an average rainfall of
35°87 inches, they every year receive 4,792,261,544,086 cubic feet
of rain; that is, a quantity sufficient to fill a canal having an
uniform breadth and depth equal to those of the Thames at low
water at London Bridge (700 x 12°5 feet), and a length of
103,721 miles, or more than four times the circumference of the
earth. ‘Taking the weight of a cubic foot of water at 1000 oz. av.,
England and Wales annually receive 133,712,677,011 tons of rain.
Were the entire rainfall of the year converted into a hailstorm it
would be a globe having a diameter of 4730 feet = -9 miles.
The eighteen “wet” counties are, in descending order, Cumber-
1870. | Rainfall in England. 469
land, Merionethshire, Westmoreland, Montgomeryshire, Carnarvon-
shire, Cardiganshire, Cornwall, Pembrokeshire, Monmouthshire,
Glamorganshire, Caermarthenshire, Lancashire, Devonshire, Breck-
nockshire, Radnorshire, Anglesea, Derbyshire, and Somersetshire—
those, in short, which, with the exception of Cheshire, Denbighshire,
and Flintshire, form our western coast from the Solway to the Land’s
End, including the Bristol Channel to the eastern margins of Mon-
mouth and Somerset shires, together with the inland mountain
counties of Montgomery, Brecknock, Radnor, and Derby. Obviously
our rains come from the west and south-west; high lands have a
greater rainfall than those which are low; and, as a corollary, dis-
tricts having loftier lands between them and the Atlantic must receive
less rain than those not thus sheltered,—a truth well illustrated by
the comparative dryness of Cheshire, Denbigh, and Flint shires,
which lie on the dry side of Carnarvonshire, Anglesea, and Ireland.
In the provisional language of meteorologists, those days are
termed “wet” on which not less than ‘01 inch of rain falls in the
twenty-four hours. During the four years already mentioned, the
greatest number of wet days recorded in one year at any station was
315 in 1866, at Patterdale Hall, in Westmoreland; and the least
number was 77 days at Beeston Lock, Nottinghamshire, in 1868.
The greatest county annual average for the same period was
207 days in Merionethshire, the least 137 days in Bedfordshire,
whilst for the entire kingdom it was 169 days: the three numbers
being as 122 : 81:100.
In twenty-two counties the general average number was ex-
ceeded, whilst it was not reached in twenty-eight ; the former group
included all the counties of excessive rainfall, with the exception of
those of Brecknock and Pembroke. }
From what has been stated above, it appears that the county
of greatest average rainfall was not that of the greatest average
number of wet days, and that the difference between the rainfall
extremes was greater than that between those of the number of wet
days, it being 132 per cent. in the former, but no more than 41 per
cent. in the latter case. In other words, though a great annual
rainfall, and a great number of wet days may be said to go together,
the former, instead of depending entirely on the latter, depends also
on the average wet-day rate of rain.
Cumberland, as we have seen, received, on the average, 68°91
inches of rain on 192 days per year; hence its average wet-day rate
of rainfall was 36 inch (= 68°91~+192), and this was the maximum.
The minimum was that of Cambridgeshire, amounting to no more
than *15 inch; whilst the average for England and Wales, as a
whole, was *22 inch; the three numbers varying as 164:68:100.
Fourteen counties, all of them having excessive rainfalls, ex-
ceeded the general average wet-day rate.
470 Rainfall in England. [ Oct.,
It may be convenient here to recapitulate in a tabular form the
principal facts just established in connection with the three pluvial
elements of England and Wales, and which show that the rainfall
of a district depends on the wet-day rate of rain rather than on the
number of wet days.
Max | Min Mean.
Average annual relative rainfall .. peers 195 63 100
Average annual relative number of wet days. Bc gaeee 122 81 100
Average relative wet-day rate ofrain .. .. .. « 164 68 100
On taking the “ wet” and “dry” counties as two distinct wholes,
their pluvial elements stand as below :— |
ACTUAL. RELATIVE.
Wet. Dry. Wet. Dry.
Annual average rainfall,. .. ss | eo 22 io 28°68 im. 7) 0
Annual average number of wet days .. | 185 days | 160 days | 116 | 100
Annual average wet-day rate of rain .. °27 in. -18 in. | 150 | 100
The Influence of Height above the Ground on the Rainfall
It has long been known that at the same station a gauge on or near
the ground receives more rain than one higher above it. Dr. Dalton
stated, in 1802, that the ratio of the quantity of rain collected on
the top of St. John’s steeple, Manchester, to that collected on the
ground in the vicinity, about 50 yards below, was 1n summer as 2:3
nearly, and in winter as 1:2 nearly.*
Mr. Symons’s ‘ British Rainfall’ extends over the ten years be-
ginning with 1860; and at several of the stations whence he receives
returns there are two or more gauges at different heights above the
ground. Omitting all whose vertical distances are less than 10 feet,
and taking the highest and lowest only at the same station, there
werein Great Britain and Ireland 226 cases spread over the ten
years which are available for the discussion of the question imme-
diately under notice.
The “ vertical gauge-distances” varied from 10 feet to 99:5 feet,
and averaged 40°5 feet. The total amount of rain received by all
the lower gauges was 6812-02 inches, and by the upper ones
5707°98 inches; showing an actual defect of 1104-04 inches, or a
relative defect of 16°3 per cent. This, divided equally between the
226 cases, gives a total deficit of 4: 885 inches each per year. Di-
viding, again, by the average gauge-distance, or difference of height
* «Monthly Magazine,’ vol. xiv., p. 5. 1802.
1870. ] Rainfall in England. 471
(40°5 feet), the result is an annual average deficit of *12 inch,
or ‘4 per cent., for every foot of elevation above the ground. In
other words, if the rainfall, received during a year by a gauge on, or
a few inches above, the ground, be divided into 1000 equal parts,
for every foot a second gauge is placed vertically above this, it will,
on the average, receive four such parts fewer.
It is obvious that this wniform average “ foot-defect” of +4 per
cent. of the receipts of the lower gauge presupposes that the lower
gauges are all at the same small height above the ground, and that for
a given depth or zone of atmosphere the actual deficit is the same,
whether the zone be at a high or low level. The first is unfortu-
nately anything but true, as some of the lower gauges are level with
the surface, whilst others are as much as 8°5 feet above it.
Waiving this however, interesting information on the second
point is contained in the returns, tabulated below, from Southampton,
Oxford, and Preston, and which have been selected from the entire
list simply because they extend over a greater number of years than
any of the others, and because the difference in the heights of the
gauges, that is, the depth of the zone of atmosphere on which the
experiments were made, was not the same at any two of the stations.
Wertital Relative Foot-defects.
Stations. gauge. |
Sees | 1860. |1861.| 1862. |1863. | 1864. | 1865. | 1866. |1867. 1968. 1869. |Means.
| ft. in |
Southampton | 18 1 | 1:03] °92| 1°19 | -97 | 1°03 | 1°33 | 1°04 | 55 | -66 | 63 | :93
Oxford . .| 22 9 -64-|-59 | -65 | -78 | -<81| 669 | =86)1 230) ..ai| “28 | “60
Preston . .| 49 5 23 | +27 32 | ‘31 25 27 34 | 34 | 42 | -26 | -30
|
An inspection of the Table shows that whilst at each station
there were fluctuations from year to year, the foot-defect was
invariably an inverse function of the vertical gauge-distance. In
other words, if a series of gauges be placed vertically above one
another, at uniform distances, the first or lowest will receive, on
the average, more rain than the second, which in its turn will
receive more than the third, and so on; but the difference between
the receipts of the first and second will be greater than that
between those of the second and third, and so on.
The foregoing Table contains twenty-nine annual returns from
the three stations collectively. Jf with them we include all the
annual returns from stations having gauges differing in height from
10 to 70 feet, and form them into six groups, such that the first
shall be made up of those only having a gauge-distance of from 10
to 20 feet, the former alone inclusive; the second, of those whose
distance ranged from 20 to 30 feet; and so on to the sixth or last ;
we get the following Table, in which the Southampton returns just
472 Rainfall in England. [ Oct.,
given, obviously belong to the first group, those from Oxford to the
second, and those from Preston to the fourth :—
Vertical gauge-distances. Number of Average Foot-defect,
in feet. Annual Returns. per cent.
|
Brom 10 to 20... 22 °939
3 SAGO OU Ow. 53 oa be
wd eSOete AOS ois. 50 “395
ee ee 35 -378
eer atto OO... 19 305
| » 60t070 .. .. 13 ‘374
From the foregoing figures, it appears that if the contents of
the lower gauge be divided into 100,000 equal parts, the upper
gauge will, on the average, receive 939 fewer such parts for every
foot of elevation, provided such elevation be not less than 10 nor
more than 20 feet; or 512 fewer such parts per foot provided the
vertical gauge-distance be not less than 10 nor more than 30 feet,
and so on.
A glance at the last or right-hand column shows: Ist, that, with
one exception, the foot-defect diminishes with increased vertical
gauge-distance; 2nd, that the difference between two consecutive
foot-defects becomes less and less with increase of difference of
elevation, and almost disappears at the height of 70 feet.
At certain stations, as Cardington and Cockermouth, there are
three gauges, each at a different height above the ground, whose
receipts are tabulated below :—
Height | Actual Rainfall in inches. Mean | Mean
Stations, of | Relative S a
Gores | 1865. | 1866. |. 1867. | 1868, | 1869. | Means, (Rainfall. ior cent,
: Bo we | a
Cardington 0 0O | 27°25 | 26°88 | 23°57 | 21°94 | 21-25 | 24-18| 100 ie
: 3 6 | 26-18 | 25-53 | 22-26 | 21-30 | 20°33 /23-12| 96 | 1:14
3 35° 0 ee aes 19°05! 79 | +58
| |
Cockermouth} 0 6| .. |50°77| 88°35 | 50:12 | 46°31) 46°39| 100 i
95 6 6 48-19 | 36°29 | 48-02 | 44°48 / 44-24} 95 *83
55 100 0 | ped eit ZO Oo oo *49
| |
Here, as before, the receipts of the gauges, at the same stations,
were greater when nearest the ground.
The difference of receipts increased with increased difference of
elevation.
The deficit, per cent. per foot, became less as the difference of
height became greater.
And on comparing the results from the two stations, it appears
1870. | Rainfall in England. 473
that whilst a difference of 3°5 feet in vertical gauge-distance gave a
foot-defect of 1:14 per cent. at Cardington, a distance of 6 feet gave
a foot-defect of only *83 per cent. at Cockermouth; and that
whilst a vertical gauge-distance of 36 feet at the former gave a foot-
defect of *58 per cent., a distance of 99°5 feet at the latter gave a
foot-defect of no more than *45 per cent.
Enough has probably now been said to show, what indeed has
long been known to meteorologists, the importance of the height of
the gauge above the surface on which it stands, with the consequent
absolute necessity of this height being everywhere the same if we
are to attach any meaning to the “ Rainfall of District,” or if rain-
fall statistics are to be of any scientific value.
Devonshire, for example, is one of the “wet” counties of South
Britain, and, from its situation, Plymouth might have been expected
to have been one of the “wet” stations of the county. This ex-
pectation is quite in harmony with the popular belief, which finds
expression in such remarks as “It always rains at Plymouth.”
“Don’t forget to take your umbrella when you go to Plymouth,” and
soon. Nevertheless, the published returns do not confirm it. The
average annual rainfall of the county during the four years ending
with December 31st, 1869, was 42°40 inches, whilst at Plymouth
it was no more than 39°45 inches, that is a deficit of 7 per cent.
If the figures are to be trusted then, Plymouth is for Devonshire a
“dry” station, at least so far as the annual rainfall is concerned,
whatever it may be with regard to the number of wet days, about
which no returns are made. ‘The case is rendered by no means less
remarkable when we turn to the other stations in the neighbour-
hood, all of which confess that they are “wet.” Thus Ham,
Saltram, and Ridgeway are all within 4 miles of it—the first in a
north-westerly, and the second and third in a north-easterly direction
—all farther from the sea, and all have their gauges on less elevated
ground ; all, in short, have conditions likely to betoken a less rain-
fall, yet their average annual falls, during the four years so —
frequently spoken of, have exceeded the county mean by 4, 9, and
16 per cent. respectively. The solution of the problem, however, is
not far to seek; it lies in the fact that whilst all the other stations
have their gauges very near the ground, the Plymouth gauge is
30 feet above it.
Two other Devonshire stations, Tavistock and Mount Tavy, tell
the same story. They are barely a mile apart, and very nearly at
the same height above the sea, but the average rainfall of the latter
exceeds that of the former by upwars of 12 per cent.—a fact for
which no other explanation can or need be given than the sufficient
one that the Mount Tavy gauge is only one foot, whilst that at
Tavistock is 20 feet, above the ground.
In this age, so famous for the application of science to commercial
474 Rainfall in England, [ Oct.,
purposes, it surely ought to be possible to turn to account the
defective receipts of rain gauges high above the surface; and in
the absence of a better, perhaps the following suggestion may be
of service :—Watering-places and other towns of fashionable and
wealthy resort, are always naturally desirous of advertising their
attractions. Knowing that their visitors dislike rain, their business
is clearly to prove that they are remarkably exempt fromit. It is
true that a wet day is comfortless and a bore simply because it 7s
wet, not because the rain is or is not heavy; hence all that is
necessary is to place the town gauge high above the ground, make
no record of the number of wet days, publish the annual rainfall
thus ascertained, and with it those of towns which have no tempt-
ation to this form of utilization. The rainfall will undoubtedly
stand in very favourable contrast with that of any of the other
towns, and the general public will readily conclude that the wet days
were correspondingly few.
Seriously, however, our method of collecting rainfall data is
anything but satisfactory, and the figures must fail in the nigid
accuracy which science requires.
In concluding this part of my paper, I venture to express the
hope that at no distant day all observers will employ gauges of the
same size and construction, which shall be tested before being
located ; that they shall all be at one uniform small height above
the surface : that the ground on which they are placed shall be at
least approximately level, and quite unoccupied for some distance
from them; that none of them shall be placed on buildings, since
these, especially when large, cannot but be thermal agents and
affect the rainfall; that, with the ex-
ee ee ception of a few very elevated stations,
—SSeeenr-_ the number of wet days shall be duly
SS ==7 ~-s recorded; and that, tor ascertaining
the exact relation of rainfall to height
above the surface, a series of such
gauges shall, at least, at one station
in each county, be placed practically
in the same vertical line at uniform
successive distances, say of 10 feet.
Without intending to express any
doubt respecting the accuracy of other
gauges, it may be stated that probably
none are to be preferred to the “ five-
inch gauge” made by Mr. Casella,
under the auspices of the British
Association, and which, through the
kindness of the maker, is figured above. It consists of a Receiver,
a Reservoir, and a Metre. ‘The last, of course, requires no descrip-
1870. | Rainfall in England. 475
tion ; and the reservoir may be dismissed with the remark that it is
a bottle of stone or glass, 9°7 inches high. The Receiver is a
copper circular funnel, 5 inches in diameter, 4°8 inches deep, and
terminating in a tube 8°5 inches long and ‘3 inch in internal
diameter. Outside this, and soldered to the bottom of the funnel,
is a cylindrical phlange, 2°25 inches deep, and having between it
and the tube a space for the reception of the head of the reservoir,
which it exactly fits, so that when united a horizontal section
through the phlange would disclose three tightly-fitting concentric
tubes. The phlange keeps the receiver steady, prevents the rain
which falls on the outside of the funnel from leaking into the
bottle, and reduces to a minimum the evaporation of the contents
of the reservoir. When fitted together the height of the instrument
is 14-1 inches; but when in use it is placed firmly in the ground,
and should have its top 9 inches above the surface.
Supposed Influence of the Moon on the Rainfall—That the
moon is very influential in, or at least closely connected with, all
changes of the weather, is a belief at once widely spread and deeply
rooted. Our satellite can neither be full, nor new, nor “ fill her
horns,” without, as is popularly believed, causing or indicating some
alteration in the state of the weather. If she is caught “lying on
her back,” or, in other words, if, when she is less than a semicircle,
her cusps are pointed upwards so that the straight line joming them
is more or less approximately parallel to the horizontal plane, the
fact is supposed to be an indication if not the cause of rain. If she
submits to be “towed by one star and chased by another,” that is, if
she is between and near two conspicuous stars, so that the three bodies
are at least nearly in a straight line, the fishermen expect a storm.
Though meteorologists show no favour to these and many
similar beliefs, some of them admit that it is neither unphilosophical
nor contrary to fact to regard the moon as a meteorological agent.
Thus, Sir John Herschel, from his own observations, regards it as _
a meteorological fact that the clouds have a tendency to disappear
under the full moon, and adds that a slight preponderance in
respect of quantity of rain near the new moon over that which falls
near the full, would be a natural and necessary consequence of a
preponderance of a cloudless sky about the full.* M. Arago, who
concurs in this opinion, states that the expression “the moon eats
the clouds,” is common in France among country people, and espe-
cially among sailors.| The latter philosopher adds that the results
obtained from meteorological observations in Germany and in Paris,
were that the maximum number of rainy days occurred between the
first quarter and full moon, and the minimum between the last
* ‘Outlines of Astronomy,’ par. 432, and note, p. 285. Sth edit. 1858.
+ ‘Popular Astronomy,’ Smyth’s Translation, vol. ii., ch. xxiii., pp. 311-313,
1858.
VOL. VII. Die
476 Rainfall in England. [ Oct.,
uarter and new moon; the ratios being 100 : 121-4 in Germany,
and 100 : 126 in Paris ; but that in the south of France the mini-
mum number of rainy days occurred between the full moon and the
last quarter. He concludes with the remark that “the question
requires to be examined afresh.” *
Having by me an unbroken series of carefully-made rainfall
observations from the beginning of 1864 to the present time, I have
tabulated the results below so as to show the amount of rain, the
number of wet days, and the wet-day rate of rain in each of the
four quarters of the seventy-four complete lunations, beginning with
the new moon on January 9th, 1864, and ending with January Ist,
1870—a period of 2185 days.
The word “ quarter,” as used here, may be defined thus :—The
first quarter begins with the day of the new moon, and ends with the
day immediately preceding that on which, according to the almanac,
the moon reaches the first quarter, and so on for the others.
| QUARTERS. |
Sahie Lee ho ae me Totals
First. | Second. Third. | Fourth. /
ah is al ts A a ee _ .
Actual rainfall in inches... .. .. | 56-66 | 58-87 | 57-30 | 55-90 | 228-73
Relative rainfall : ; | 2477 | 2547 | 2505 | 2444 | 10000
Number of times rainfall was ‘more)
than 25 per cent. .. wa 30t | os -
Number of times rainfall was les}
than 25 per cent. = ei = ue a
Number of dry days .. 274 301 241 266 1082
Number of wet days.. .. .. 274 248 307 274 1103
Relative number of dry days .. 253 278 223 246 1000
Relative number of wet days .. - 248 225 278 248 1000
Mean wet-day rate of rain in sities | -2141 | -2374 | -1866 | | +2043 | -2073
Relative mean wet-day rate of rain | | 98 100
103 115 | 90
|
From the foregoing Table, it is obvious that with regard to the
three pluvial elements, in South Devon, during the six years ending
with January Ist, 187 0, the four quarters of the seventy-four moons
may be arranged, in descending order, as below:
Rainfall. | Number of Wet Days. Wet-day Rate of Rain.
Second. (greatest) | Third. (greatest) Second. (greatest)
Third. Second. Fi
irst.
First. Fourth. Fourth.
| Third. (least)
Fourth. (least) First. (least)
* «Popular Astronomy,’ Smyth’s Translation, vol. ii., ch. xxxv., pp. 317, 318.
+ The rainfall of one “second quarter” was exactly 25 per cent. of that of the
lunation.
Quarterly Journal of Science N° XXVET.
:
How the Earth is presented towards the Sun, during
- the Eclapse, and the path of the Moon's Shadow.
&
ITER RANEAN
. Nes
The course and shape of the Moon's Umbra.
Litho Whiteman k Bass, London
1870. | The approaching Total Solar Kelipse.. 477
This tabular summary shows :—
1st. That the quarters arrange themselves in an entirely dif-
ferent order under the different heads, with the single exception of
the second being the quarter of greatest average rainfall and also
of greatest average wet-day rate of rain.
2nd. That the least average rainfall was in the quarter imme-
diately preceding the new moon, instead of being, as Sir J. Herschel
supposes, about the full moon.
8rd. That the maximum number of wet days was in the third
quarter, and the minimum in the first; thus differmg in every
particular from the results stated by M. Arago to have been
obtained in Germany and Paris, on the one hand, and in the south
of France on the other, which, as we have seen, differed from one
another.
This discussion may be appropriately closed, perhaps, by echoing
Arago’s remark, that “the question requires to be examined
afresh.”
V. THE APPROACHING TOTAL SOLAR ECLIPSE.
By R. A Procror, F.R.AS., &e.
Tue eclipse of next December is less remarkable in many important
respects than the two total solar eclipses now commonly known as
the Indian and American eclipses of 1868 and 1869. The former
of these was distinguished among all the eclipses of recent times by
the exceptional extent to which the lunar dise overlapped, during
central totality, the concealed disc of the sun. For more than six
minutes at some stations no direct solar light was visible. The
eclipse of last year was not distinguished in this particular way,
though the duration of totality—at some stations exceeding four
minutes—was far from inconsiderable. What rendered the Ameri-
can eclipse so extremely important, even more important than the
Indian one, was the fact that a large proportion of the track of
the moon’s shadow lay across a region dotted over with well-armed
observatories. It is probable that on no previous occasion has so
large an array of practised observers been employed in scrutinizing
the phenomena of a total eclipse; and it is absolutely certain that
so many appliances had never before been employed to render the
researches of the observers effective.
In both respects the approaching eclipse is less important. The
greatest duration of total obscuration will be but 2m. 11s.; and
the track of the moon’s shadow only skirts the region within which
the principal European observatories are situated. In fact, the only
parts of Kurope traversed by the shadow are the southern provinces
of Spain and Portugal, Sicily, the southern extremity of Italy, and
2K 2
478 The approaching Total Solar Eclipse. [ Oct.,
parts of Greece and Turkey. And of these regions only those in
the Spanish peninsula and Sicily are practically available, because
in the others the duration of totality will be less and the sun will
have but a small elevation. In Greece, for instance, and Turkey,
though the phenomena of totality may chance to be well seen, yet
the chance is not such as would justify an expedition from the prin-
cipal astronomical centres of Europe. The best places of all for
observing the eclipse will undoubtedly be those along or near the
track of totality in Algeria. These, however, will probably be left
to the astronomers of France.
Fig. 1 shows the actual presentation of the earth towards the
sun, and the course and shape of the moon’s shadow on Decem-
ber 22nd next. The hour is supposed to be solar noon at Green-
wich. The earth must be conceived to be rotating in the direction
shown by the arrow (on the equator), and at such a rate that any
meridian line in the figure will reach the place occupied by the
next meridian towards the right in two hours. The black spot to
the west of Spain represents the shadow of the moon at the hour
named. This shadow is surrounded by the penumbra, a portion of
which, however, remains throughout the eclipse beyond the northern
limits of the earth’s disc. The course of the shadow is indicated by
the curved line taken through the black spot. If an observer on
the sun could trace the apparant path of the moon’s centre across
the earth’s dise, he would not find it curved in this way, but appre-
ciably straight. As the earth is rotating, however, the disc turned
towards the sun undergoes an appreciable change during the dura-
tion of central eclipse, and the motion of the different points of the
earth along parallels curved like those shown in the figure, causes
the path of the moon’s centre with reference to the earth’s globe
(distinguished here from her disc as seen from the sun) to have the
shape indicated in the figure. |
Central eclipse begins on the earth generally at twenty-six
minutes before noon,—in other words the black shadow shown in
the figure as already well advanced is supposed to have entered on
the disc twenty-six minutes before the epoch corresponding to the
figure. Central eclipse concludes for the earth generally at twenty-
one minutes past one, or eighty-one minutes after the epoch corre-
sponding to the figure. The total interval during which the moon's
shadow (as distinguished from her penumbra) falls upon the earth
is thus 1h. 47 m.; and the amount of motion due (during this in-
terval) to the earth’s rotation can be conceived by remembering
that the southern extremity of Spain moves during totality from
a place below the dark spot in the figure (and on the proper
parallel, of course) to about the place occupied in the figure by
Sicily.
it will be evident from a further consideration of the relations
1870. | The approaching Total Solar Eclipse. 479
presented in Fig. 1, that there are two respects in which this
eclipse is unfavourable. First of all, the track of the shadow lies
far from the centre of the disc. It is clear that, pro tanto, the
shadow is rendered smaller by falling near the outer parts of
the disc; because these parts lie farther than the centre from the
sun. Secondly, the elevation of the sun at the time of eclipse is
not considerable. Since the sun is vertical at the place which
occupies the centre of the earth’s illuminated disc, and on the
horizon for any place which lies on the circumference of that disc,
it is obvious that when the track of the moon’s shadow lis as in
Fig. 1, the sun’s elevation is relatively small during total obscura-
tion. In the present eclipse, at the stations where the chief
observing parties will be placed, the sun’s elevation will be about
30 degrees, amply sufficient for ordinary observing purposes, but
not altogether so great as might be desired for spectroscopic and
polariscopic researches, and still less satisfactory for photography.
Fig. 2 presents on a larger scale the track of the moon’s shadow,
and the actual oval shape of the black spot which seen foreshortened
in Fig. 1 appears as a circle. It will be seen that Odemira in
Portugal, Cadiz and Xeres in Spain, Oran and Ratna in Africa, and
Syracuse in Sicily, are the principal towns which lie very close to
the central line. But it is probable that the stations will be selected
without special reference to the proximity of towns ; indeed for many
purposes the less inhabited regions of a country are best suited for
such observations as have to be made during eclipse.
Although Mount Etna is not very close to the central line, there
are reasons for believing that a party stationed on the summit of
this mountain would be enabled to make important observations.
They would be more than twice as far raised above the sea-level as
those observers were, who during the American eclipse obtained
such favourable views of the solar corona from the summit of
White Top Mountain. It will be remembered by our readers that
General Myer reports the extension of the corona as seen from this
station to have exceeded more than twofold the extension observed
by those at lower levels. As there will probably be an English
observing party near Syracuse, it would be a matter of the utmost
interest and importance to compare their observations of the corona
with those made at the summit of Etna.
At present, it may be mentioned in passing, there seems every
reason to believe that two important expeditions will be sent from
England to observe the eclipse. As we write, the arrangements are
not complete, and there still remains a possibility that the whole
undertaking may fall through. But it is hoped that this may not
be the case, and that the large array of volunteers whose names
appear in the list of the two proposed expeditions may be enabled to
devote their energies to the work they have severally undertaken.
480 The approaching Total Solar Eclipse. [ Oct.,
The main object of the astronomers of this and other countries
will be to determine the nature of the corona. For this purpose,
each of the English expeditions is to be divided into four parties.
First, there will be the spectroscopists ; secondly, the polariscopists ;
thirdly, the photographers; lastly, there are the general observers,
who in our opinion are very far from forming the least important
portion of the expedition.
The spectroscopic evidence obtained during the Indian and
American eclipses is contradictory and unsatisfactory. Let it be
remarked in passing, however, that it is not altogether so contra-
dictory as has been asserted. The American observers appear to
have been misled into the supposition that Major Tennant saw the
ordinary solar spectrum—that is, that the Fratinhofer lines could
be seen in the spectrum of the corona. And indeed in Prof. Roscoe’s
treatise ‘On Spectrum Analysis,’ it is stated that Major Tennant
saw the ordinary solar spectrum, whereas “ Professor Pickering, on
the other hand, saw only a continuous spectrum.” But Major
Tennant’s account expressly asserts that the spectrum he saw was
continuous. He says, “ What I saw” (the italics are his) “was
undoubtedly a continuous spectrum, and I saw no lines. There
may have been dark lines, of course, but with so faint a spectrum
and the jaws of the slit wide apart, they might escape notice.”
Thus the continuous spectrum seen by some of the American
observers is in perfect accordance with Major Tennant’s observation.
Indeed the mistake is rather fortunate than otherwise, because it
led the American observers to search specially for dark lines such
as they supposed Tennant to have seen ; and, therefore, their failure
to recognize any may be regarded as all but decisive of the matter.
Where Major Tennant’s observations are not accordant with
those made by the American observers, these latter observations are
themselves wanting in accordance. For Professor Young saw three
bright lines in the coronal spectrum, and Professor Harkness saw
one bright line; whereas Professor Pickering, like Major Tennant
in 1868, saw only a continuous spectrum. This discrepancy will,
we may fairly trust, be cleared up during the approaching eclipse.
It may perhaps be found that different parts of the corona give
different spectra. It may be noticed, however, that the bright line
seen by Harkness and the bright lines seen by Young were delicate
objects, and would almost certainly have escaped notice had these
observers used a much narrower or a much wider slit than they
actually employed. Professor Harkness failed to see the line till
he had slightly opened the slit; but he would probably have lost
it equally had he widened the slit too much.* May not Major
* The total quantity of light from the bright lines would be increased by widen-
ing the slit; but the intrinsic brilliancy of the broadened bands would be no greater
than before. On the other hand, the intrinsic brilliancy of the continuous back-
ground would be increased by the change.
1870. | The approaching Total Solar Eclipse. 481
Tennant have failed through such a course? He says, “ thinking
that want of light prevented my seeing the bright lines which [
had fully expected to see on the lower strata of the corona, I opened
the jaws of the slit.” It is worth noticing that failure may arise
from this very adjustment. ‘Too narrow a slit is clearly unfavour-
able, because a certain quantity of light is required for distinct
vision; but on the other hand too wide a sht is equally unfavour-
able, because a certain relative superiority in the brightness of the
lines (or in this case bands) over the background of the continuous
spectrum is equally requisite. The obvious conclusion is, that a
telescope of large aperture and therefore of high light-gathering
power should be employed, and the light of the continuous back-
ground reduced as much as possible by increasing the dispersion.
As respects the polariscopic operations, there is a similar con-
tradiction to be explained during the approaching observations.
The observers of the Indian eclipse assert positively that the hight
of the corona is polarized in a plane through the sun’s centre ; the
American observers, on the other hand, as positively deny this.
The Astronomer Royal (than whom no higher authority—on this
particular subject—exists) solves the difficulty summarily by ex-
pressing his belief that the observers in India were not sufficiently
familiar with the principles of polariscopic research to interpret
what they saw. In this case, and assuming a similar state of
things in the case of the American observers, we must look forward
to the approaching eclipse as likely to supply the first really reli-
able information yet obtained respecting the polarization of the
corona. We cannot doubt that the observers next December will
not fail from want of knowledge, since not only has the Astronomer
Royal called special attention to the necessity of their carefully pre-
paring themselves beforehand, but the government of the party has
been assigned to Professor Pritchard, who is nothing if not a master
of the science of theoretical optics. Our great fear is, however, lest
the methods of testing light at present in vogue may not be suffi-
ciently effective for the resolution of the somewhat difficult pro-
blems depending on the polarization of the corona. Whatever
advantage there may ordinarily be in the use of well-tried methods,
it may be questioned whether in this particular case more powerful
instruments than the polariscopes at present in use might not be
devised and employed with advantage.
We pass over the photographic department of the expedition ;
in the first place because there is every reason to feel confidence
that under the able supervision of Messrs. Browning and Brothers
(at Gibraltar and Syracuse respectively) the photographic arrange-
ments will be exceptionally successful, and in the second because as
regards the inquiry, which is the main purpose of the expedition,
photography can teach us comparatively little. Unless the whole
482 The approaching Total Solar Eclipse. [Oct.,
duration of totality were given to a single negative—which would
be clearly unwise—no satisfactory picture of the corona could be
obtained. :
The chief promise of the expedition, in our opinion, lies in the
number of skilled observers who have joined the two parties which
are to devote their energies to general observation. The names of
Mr. Lassell, Lieut.-Colonel Strange, and others (it is almost in-
vidious to particularize), afford a sufficient guarantee not only of
skilful observation, but also of a thoughtful study beforehand of the
modes of observation likely to be most successful. We cannot sup-
pose for a moment that such observers will be content merely to
renew the observations which have been made so often and to such
little purpose,—to tell us merely the oft-told tale respecting the
beauty and splendour of the corona, its colour, extent, shape, and
so on. Something much more definite is required, and that some-
thing, if it can be obtained (of which we have no doubt whatever),
is surely to be expected from the skilful astronomers who have pro-
mised to take part in the general observations to be made on the
corona.
Let us consider a few of those points on which it is most desir-
able that information should be obtained.
It has been observed by some astronomers that the structure of
the corona seems in places to be marked by the presence of curves
and striations, and sometimes even of complex portions, which have
been compared to “hanks of thread in disorder.” It is most im-
portant that adequate telescopic power should be applied to deter-
mine how far this appearance is real, and what peculiarities may be
recognized in the curves, hanks, and striations, under telescopic
scrutiny. For this purpose the disc of the moon ought not to
occupy (as has been usually the case) the centre of a large field;
but the brighter part of the corona close by the moon’s limb should
be kept altogether out of the field of view. Further, different
powers should be employed, and the focussing for each should be
very carefully noted. For even those who reject wholly (as we
confess that we do) the theory that the corona is merely a pheno-
menon of the earth’s atmosphere, must recognize the fact that the
appearance of the corona may be, and probably is, very much
affected by our atmosphere, through which it is necessarily seen.
So that some of the peculiarities which apparently belong to the
corona may in reality appertain to our own atmosphere. In this
case the focussing suitable for clear recognition of the causes of such
peculiarities would correspond to the relatively small distance of the
upper parts of our atmosphere, and would thus differ appreciably
from the focussing for celestial objects. It has been suggested that
“the use of a telescope of low magnifying power but first-rate de-
finition, a comet eye-piece being employed, would be desirable in
1870. ] The approaching Total Solar Kelipse. 483
studying the corona. ‘The telescope should be accurately driven by
clockwork, and a dark iris-disc, 1f one may so describe an arrange-
ment which would be the converse of an iris-diaphragm, might be
employed with advantage to hide the light of the prominences and
chromosphere. If the field of view were several degrees in diameter,
and the dark disc at the beginning of totality concealed a circular
space extending a degree or so beyond the eclipsed sun, the observer
might first examine with great advantage the outer parts of the
corona, and gradually extend his scrutiny to the very neighbour-
hood of the prominences.”
A question of extreme importance, which seems fairly within
the range of the available modes of research, consists in the deter-
mination whether the outer and extremely faint parts of the corona
show any sign of prolongation towards those regions where, as we
know, the zodiacal light extends. The whole of that portion of the
heavens along which (speaking with reference to the place of the
sun) the zodiacal light is ordinarily visible, is above the horizon
during most total eclipses. Further, the dark region corresponding
to the place occupied by the moon’s shadow in our atmosphere,
extends at the beginning and end of totality over a very wide range
of sky, first on the western and then on the eastern side of the
lunar disc. Along this region the faint glow of the zodiacal light
ought to be perceptible if sought for under favourable circumstances.
Among such circumstances are, of course, a clear sky and an elevated
station. But there is one condition which, so far as we know, has
never yet been attended to. The maximum darkness of a solar
eclipse comes on so rapidly that the eye is yet dazzled by the light
when totality is in progress. Nor does totality last long enough
for the eye to acquire the power of recognizing faint differences of
illumination. This fact serves to explain the failure of observers,
hitherto, in detecting the delicate phenomenon we are now consider-
ing. There appears to be good reason for believing that the search
would be conducted with a much better prospect of success if the
observer who undertook it were in the first place to keep his eyes
as much as possible in darkness until totality had fairly commenced ;
and in the second, to hide the whole of the corona from view while
searching for the zodiacal light. This could be very easily managed
by arranging beforehand a black disc so as to conceal the sun at the
time of totality from an eye placed at a certain aperture, through
which the observer should conduct his search, during totality, for
the faint light along the ecliptic. This method seems so promising,
and the inquiry itself is so full of interest, that we cannot but hope
some observer will be willing to devote himself specially to this par-
ticular subject. ;
But we may safely expect from those who have volunteered to
take part in an expedition which will probably be by no means a
484 The Controversy on Spontaneous Generation: — [Oct.,
pleasure trip (remembering the season and the nature of the voy-
age) the thoughtful consideration beforehand of all those means by
which the expedition may be made successful. They will be fully
aware that the astronomical world will expect from them something
more than the renewal and confirmation of former observations. We
may hope from them therefore results of extreme interest, throwing
new light on important problems of solar physics, and perchance
even revealing unexpected truths respecting the economy of the
solar system itself.
VI. THE CONTROVERSY ON SPONTANEOUS
GENERATION: WITH RECENT EXPERIMENTS.
By James Samvuetson, Editor.
THERE is perhaps no biological question, excepting the origin of
species, which has been so warmly debated in England and abroad,
as the mode in which the lowest known types of animal and plant
life come into existence, and probably one reason why these in-
quiries have been productive of so much excitement, is their indirect
theological bearing.
The developmental theory recently elucidated by the researches
and arguments of Darwin gave a fatal blow to the ancient beliefs
concerning the first appearance and presence of the animal and
plant races on the earth’s surface, and rendered unnecessary the
special intervention of the Creator to account for the production of
new species ; whilst the hypothesis of spontaneous generation, or
the creation de novo, in organic infusions of the lowest known types
of plants and animals in our time, seems, to impetuous and super-
ficial thinkers, to put the divine influence altogether out of sight,
and almost to degrade what have hitherto been regarded as living
beings and vital forces to a level with the unconscious physical
forces and inert forms of matter.
With these considerations, however, scientific men have no
concern, and whether or not the creation of a living thing from
organic or inorganic materials, by what may be termed artificial
means, be regarded as a sacrilege, the investigation must be under-
taken without apprehension or prejudice, and the verdict given, not
by theology or theologians, but on the evidence of strict experi-
mental research, and from unprejudiced inductive reasoning.
Scientific men being, as a rule, regarded as ruthless iconoclasts,
anxious only to lacerate the feelings and undermine the most sacred
aspirations of true believers, it may be supposed that these remarks
are prefatory to an argument intended to overturn all our precon-
ceived views as to the higher nature of life, and to hand over the
Quarterly Journal of Science N° XXVIII.
200 drs
Litho. Whiteman & Bass, London
Organisms found in infusion of Orangejuice , and in
)
purée Rain Water.
1870.] with recent Hxperiments. 485
task of creating living beings to the chapter of accidents and to the
blind physical forces of nature. My task is, however, not of such a
painful character. In the first place, it must be remembered that
if it should turn out that living beings are capable of springing into
existence through the direct transformation of decaying organic
matter, those beings are, so to speak, merely the instruments upon
which the higher psychical faculties play ; from dust they come and
to dust they return. And again, every advanced thinker is pre-
pared to admit that even the higher races which animate, beautify,
or transform the earth’s surface, are fed, grow, and decay through
the direct operation of the physical forces, and that they are exqui-
sitely constructed machines, lable to injury, accident, and destruc-
tion, and need fuel and reparation just as any humanly-constructed
mechanism. What difference, then, can it make to any but the
most timid or bigoted thinkers whether the first appearance of the
lowest types of animal and plant life is due to the direct action of
the physical forces upon matter which has once been organized and
is undergoing decomposition, or to the same forces or some unknown
modification of them acting in the first instance m or upon almost
inconceivably minute pre-existing germs ?
I can, however, offer to such timid philosophers the crumb of
comfort, that it is not unlikely the ultimate result of the discussion
which now agitates the scientific world will be to show that the
lowest known living types are not now created de novo, but that
their germs are almost omnipresent and ineradicable; and this
conclusion has been arrived at by me, not from the experiments
with varying and contradictory results which have been tried by
different investigators, but from a calm consideration of the whole
question, renewed at intervals, over a space of nearly fifteen years.
And this reflection causes me to draw attention to a peculiar cir-
cumstance connected with the controversy on spontaneous genera-
tion; namely, that we hardly ever hear of the work of any observer
extending over a lengthened period. In most cases we have a set
of experiments tried by an investigator of greater or less eminence
now a zoologist, then a chemist, which are published along with his
views, usually of a very decided and dogmatic character, and then he
rushes out of the arena, and we hear nothing more of him on that
subject. Of course he has settled the question to his own satisfac-
tion and to the satisfaction of those who agree with him, and there
is no need of further investigation until some new circumstance or
some fresh set of experiments invalidates all previous evidence and
raises up a new host of combatants and disciples on either side.
We are at present in the very thick of such an intellectual con-
test, and no doubt there are many true believers in heterogenesis who
regard as conclusive the recently-published experiments and obser-
vations of Dr. Bastian which have startled the boldest thinkers and
486 The Controversy on Spontaneous Generation : [ Oct.,
some of the most profound biologists; but after bestowing upon
them the careful consideration which they well deserve, and trying
such experiments as seemed to me to throw light upon some of the
mysterious appearances described by him, I have come to the con-
clusion that, so far as he is concerned, the argument stands just
where it was, and that the question is likely to remain an open one
for a long time to come. :
Many will, no doubt, remember that some years since Professor
Huxley, influenced by the astounding revelations of organic che-
mistry, and by the facility with which one form of organic matter
after another was being synthetically produced by chemists in their
laboratories, ventured on the bold speculation that possibly experi-
mentalists might one day be able “ to take inorganic matters such as
carbonic acid, ammonia, water, and salines in any sort of inorganic
combination, and be able to build them up into protein matter, and
then that that protein matter ought to begin to live in an organic
form ;’* but Dr. Bastian believes that he has accomplished even
more than this, that he has taken solutions of saline substances in
proportions which he details most circumstantially, has exterminated
in them all the germs which they might possibly be said to contain,
and by excluding the atmosphere has prevented the entrance of new
ones which might be said to be floating in that medium; and that,
yet, after intervals varying from nine or ten to forty days there have
been spontaneously produced in and from those substances, not par-
ticles of protoplasm as it was hinted possible by Professor Huxley,
but truly organized plants and small ciliated infusoria.
But, in the first place, his own account of these experiments is
often very vague. For example, he tells ust that he prepared a
solution of crystallized white sugar, tartrate of ammonia, phosphate
of ammonia, and phosphate of soda, which was boiled for twenty
minutes and kept am vacuo nine days; and, to use his own words,
“when examined microscopically a few monads and bacteria were
found in the first drops of the liquid which had been poured out
before the whole was shaken.”
So far, after nine days’ exposure he found only what has been
seen by a score of observers over and over again, and cautious in-
vestigators, such as Dr. Child, Dr. Beale, and others (as I ventured
years since to predict), have refused to admit many of these minute
moving specks to be living organisms at all. But he goes on to
say, “The remainder was then poured into a conical glass, and
after having been allowed to stand for a time, the supernatant fluid
was removed and the last few drops containing the sediment were
* “On our Knowledge of the Causes of the Phenomena of Organic Nature ;’
being Six Lectures to Working Men. By Professor Huxley, F.R.S. London:
R. Hardwicke.
t ‘Nature,’ July 7, pp. 195-6.
1870. ] with Recent Experiments. 487
examined.” Itis to be regretted that we are not informed how long
the fluid was allowed to stand exposed to the air, for although
in the case under consideration the only result of the exposure was
the appearance of many “ bacteroid particles” (whatever that may
mean—for a bacterium itself is the minutest speck perceptible to the
eye with high microscopic powers), “and monads of different sizes
exhibiting the most active movements,” yet I will show presently,
that when certain fresh infusions are exposed under favourable cir-
cumstances only for a few hours, they become filled with perfectly-
organized plant forms in different stages of growth. In addition
to those “bacteroid” particles and monads, Dr. Bastian also found
“irregular-shaped particles” which were active, and the conclusion:
at which I am constrained to arrive, is that his enthusiasm in the
cause of heterogenesis has led him, there at least, to confound the
atomic motion of organic and inorganic particles with the move-
ments of similar objects, of which it is always necessary to trace the
growth and development before they can be safely pronounced to be
the germs of infusoria or of lowly plants.
Let me, in passing, recommend those investigators who are
reviving the experiments of Pouchet, Pasteur, Schulze, Joly, Musset,
Wyman, and others, all of whom have failed to convince the scien-
tific world, that they should not only examine their infusions, as
heretofore, some days after they have been sealed up, but some
hours afterwards, and I have reason to believe that the comparison
will change their views as to the result of closing and preserving
those infusions. Pitta
Again, some of Dr. Bastian’s experiments are strikingly adverse
to the hypothesis that the types observed and described were created
de novo. In experiment No. 13, a solution of tartrate of ammonia
and phosphate of soda, which had been kept twenty days an vacuo,
was found to contain a fungus, &c., whilst another solution, which
had been prepared in the same manner and at the same time, was
opened on the thirty-fifth day, and “yielded no organisms of any
kind;” but mark! when a third solution of the identical sub-
stances was so treated as to give free access to the air, and was
examined on the thirty-eighth day, there was found what the
observer calls “a spirally-twisted organism.” It seems to me that
it would hardly be possible to adduce more convincing evidence
against heterogenesis and in favour of the atmospheric germ theory
than is afforded by these results, and a very striking confirmation
of this view is to be found in a circumstance which has recently
been discovered in another quarter, affording evidence, all the
more valuable, because it was not intended to influence this con-
troversy. Mr. Wood, of Middlesbrough, in his efforts to preserve
tartaric acid solutions in a state fit for chemical experiments,
has found that whilst such a solution will, under ordinary circum-
488 The Controversy on Spontaneous Generation : [ Oct.,
stances, become mouldy, it will not undergo that change if pre-
viously boiled and filtered—but it must in fairness be added that
he says, even if exposed to the air. Whether he means constantly
exposed to the air, or only occasionally, I am unable to say. How
such substances become mouldy will be seen presently, and it will
be found to have a direct bearing on the argument.
Before proceeding to describe my own recent investigations,
however, I desire to make one more reference to the published
opinions of Dr. Bastian, to show how necessary it is to be cautious
before we construe the microscopical appearances connected with this
inquiry.
In speaking of the pellicle which appears on the surface of
infusions, Dr. Bastian says,* “What Burdach named the pro-
ligerous pellicle of organic solutions, is made up of an aggregation
of monads and bacteria in a transparent jelly-like stratum on the
surface of the fluid. It constitutes at first a thin scum-like layer,
and although the monads and bacteria entering into its composition
are motionless, M. Pouchet and others were not warranted in
assuming from this fact alone that they were dead. There is
indeed good reason for believing to the contrary, since, as pointed
out by Cohn, when any of these particles are set free from the
broken edge of a pellicle, they always resume their movements.
Motion, therefore, may simply be prevented by the presence of the
transparent jelly-like material in which they are imbedded, although
the particles may be undoubtedly living.”
Under what circumstances the observers examined this so-called
“proligerous pellicle,” I am unable to say, and Dr. Bastian him-
self says, that owing to his observations being carried on in winter,
he was not able to witness those changes observed by Pouchet; but
he describes certain other changes in this pellicle on infusions
which, according to his account, resulted in the development of
unicellular organisms.
Now, with all deference to the eminent observers quoted by
Dr. Bastian, I venture to say that the appearances referred to have
no bearing whatever upon the controversy, inasmuch as they are
by no means confined to infusions.
Long before I had heard the expression “ proligerous pellicle,”
or was aware that this phenomenon was supposed by the advocates
of heterogenesis to precede the creation, de novo, of living forms, I
had myself observed a precisely similar appearance in pure distilled
water exposed to the atmosphere. This was recorded at the time, as
follows, in a paper read before Section D of the British Association
in 1863 :-— .
“Let me, however, briefly refer to the results of the exposure of
distilled water only, in July, for that experiment has not been re-
* ‘Nature,’ June 30, p. 172.
1870. | with Recent Haperiments. 489
peated with such satisfactory results. The glasses containing the
water were so placed in a box divided by three partitions and covered
with lids of blue, red, and yellow glass, that the panes intercepted
all dust falling perpendicularly, and for several days very little dust
reached the contained water. A deposit of dust had meanwhile
accumulated on the panes of glass. Finding little or no life in the
distilled water, I washed the dust from the glass lids into the re-
spective vessels, and on the following day repeated the examination.
As usual, I observed particles of silex and fragments of organic sub-
stances, and, with a low power, these seemed to be imbedded in a
gelatinous film. I had placed the little glass vessels themselves
under the instrument, and after pouring off the water, examined the
deposit with a power of about fifty diameters. On covering the
sediment with a thin glass, and bringing a higher power to bear,
I found the gelatinous film to consist of motionless transparent
monads or cells, and carefully restoring the contents of the vessels,
pouring back the water, I left them until the following day. Dur-
ing the night and day, the cells or monads had become endowed
with rapid motion, and an examination of the water showed it to
be peopled with myriads of active moving germs.”
Here, then, is another phenomenon supposed to be attendant
upon the creation de novo of lowly organisms in infusions, which I
had observed and recorded years since in pure distilled water ex-
posed to atmospheric action.
And this brings me to my recent investigations, conducted
during the months of June, July, and August last. As considerable
doubt has been thrown upon the existence of germs in the atmo-
sphere by certain observers, in their anxiety to prove the sponta-
neous production of the lowest plants and animals, I first repeated
my former simple experiments with distilled water, and this time I
used open saucers, small glass well-dishes (those used to hold ink),
and even test tubes.
On the 21st June I first exposed two saucers of distilled water
to the air, and two days afterwards I found it to contain a little
sediment of dust. On examination with the microscope, a drop of
the water presented the appearance so frequently described by me.
There were fragments of silex, soot, and minute moving germs.
The latter I shall not attempt to dignify with scientific names;
suffice it to say that the contrast between their movements and the
molecular motions of particles of organic and inorganic matter af-
forded: sufficient proof of their being endowed with life. I then filled
two test-tubes with portions of this water, closed the opening of
one with a sheet of cotton-wool, and left the other exposed to the
air. From the 23rd June to the 5th July the weather was cold
and rainy, conditions very unfavourable for the development of
living germs; but between the 5th and 7th July the temperature
490 The Controversy on Spontaneous Generation : [ Oct.,
had risen considerably, and I then examined the tubes. (It should
be added that I had in the meantime added distilled water to that
in the open tube to compensate for evaporation.)
The exposed water contained numerous zoospores, and uni-
cellular forms. Some of these were quiescent and attached toge-
ther in clusters; others in active motion. ‘There were some small
amoebze, small particles of protoplasm, with elastic cell-walls, well
known to micro-zoologists. In these, not only the characteristic
changing prolongations were visible, but I clearly followed the
rhythmical movements of the contractile vesicle. From the other
tube, the cotton-wool appeared to have excluded the dust and
germs—the former having collected on the cotton, for I found no
organisms of any kind. It is right, however, to mention that
cotton-wool does not permanently exclude the germs; and in an-
other case, where the conditions of development were favourable (if
the view be correct that they are conveyed by the atmosphere), it
will be found that the substance referred to failed to exclude them.
As to my saucers of distilled water, on going to examine them
I found the contents dried up, but a considerable quantity of dust
remained. ‘This I scraped together; retained it until my return
from a journey on the 19th July, and then submitted it to the
following process in the laboratory of my friend Mr. Tate, of Liver-
pool, aided by his assistant :—
First we heated the dry dust in an open tube to 480°C., and
then, allowing it to cool, we heated it again to 280°C. It had
then caked, and after loosening it with a wire we added distilled
water, and boiled it for a few minutes. Then I closed the tube
containing the liquid temporarily with a little stopper of cotton-
wool.
The same evening, on examining the sediment with a power of
200 diameters, I observed many of the appearances described by
investigators who have opened infusions after they have been kept
in vacuo several days; some, for example, similar to those described
by Dr. Bastian in his first experiment recorded in ‘ Nature’ of
July 7th. But I did not feel justified in attributing the movements
of the particles to their beg endowed with life.
I then divided the chief part of the water containing the dust
into two tubes, closing one with cotton-wool and leaving the other
exposed, and a little of it was left in an open wine-glass. The open
tube I examined on the 22nd, 23rd, and 24th July. The tempe-
rature was very high—82° in the shade—and the development of
the little Cercomonas, so frequently described by me in former
years * was very rapid, so that on the 25th its movements were
clearly traceable amongst other lowly types.
The water in the wine-glass was again dried up, but the effect
* «Journal of Science,’ vol. i., p. 607, and elsewhere.
1870. ] with Recent Haperiments. 491
of the high temperature was surprising, and two hours after I had
added a little distilled water to the dust I found it to contain clearly-
defined and active monads and other living types. JI may here
mention that the very warmth of the hand in which the slide is
held will often render active and instinct with life little unicellular
organisms which, on being first examined with the microscope,
appear inanimate and motionless.
On the 28th and 29th July I again examined the tubes, open-
ing the closed one on the latter day, and found that although the
number of forms in that was much less than in the one that had
been exposed, they were alike in character, and I showed to two
astonished visitors who had never seen such appearances, active
amecbe in water taken from both tubes.
Here my experiments with pure distilled water terminated, and,
so far, they are not only confirmatory of what had been observed
and described by me many years since, but they satisfied me that
the solid floating contents of the atmosphere may be submitted to
an exceedingly high temperature in the dry as well as moist condi-
tion without exterminating the living germs; and that when dis-
tilled water is added and the sediment is examined, either imme-
diateiy or after a few days’ exposure, even if the air has been
excluded, it exhibits most of the phenomena believed by the advo-
cates of heterogenesis to be proper to infusions which have been
boiled and kept 7m vacuo.
And now I have to describe a second set of experiments, which
may perhaps serve to throw hght upon the appearance of those
fungi which are frequently found upon decaying substances in the
form of mould or mildew, and which Dr. Bastian believes he has
been instrumental in creating spontaneously in organic and inor-
ganic infusions. Two announcements recently made by the advo-
cates of heterogenesis influenced the direction taken by my investi-
gations. One was the statement contained in Dr. Bastian’s
account of his experiment No. 5,* that he had discovered in an —
infusion of turnip 7m vacuo which had been hermetically sealed five
days, a reticulated substance which he calls “ Leptothrix’ filaments.
The other was the discovery by Mr. Wanklyn, the chemist, of suffi-
cient albuminous matter in a pint of air to render it highly probable,
from that circumstance alone, that the atmosphere is charged with
living germs. Mr. Wanklyn strangely enough cites his discovery,
triumphantly, as conclusive evidence of the absence of such germs,
inasmuch as the quantity of albuminous matter was found to be very
insignificant ; but Dr. Beale, one of our most experienced micro-
scopical observers, has expressed the view | that Mr. Wanklyn has
found a volume of such matter, which, insignificant as it may appear,
renders it highly probable that of the air tested by him “not a
* Reported in ‘ Nature,’ July 7. + ‘Nature, July 28, p. 255.
VOL. VII. 2 L
492 The Controversy on Spontaneous Generation : [ Oct.,
thimbleful could be taken without containing several” germs.
Mr. Wanklyn’s evidence certainly reads very much like that of a
scientific witness for the defence in a case of murder, who seeks to
show that the deed could not possibly have been committed upon a
certain clean deal floor where it is said to have been perpetrated,
inasmuch as he had carefully examined a square inch of the floor,
and had only discovered the minutest spot of blood !
As to the “ Leptothrix” which Dr. Bastian found in turnip-
juice, 1 may mention in passing that it is considered by microscopic
botanists to consist of the mycelial filaments of mildew fungi,* and
I believe from my own investigations, to be described presently,
that if he had followed the growth of his “ Leptothrix” he would
have found it to be one of those plants. Now these mildew fungi
are found not only in and upon decaying organic matters, but also
upon bare stones and rocks, where they cannot be created de novo,
but must necessarily result from atmospheric spores moistened by
showers of rain. Coupled with the two circumstances just men-
tioned, the account given by Dr. Angus Smith of his mode of
testing atmospheric air opened out to me a new field of inquiry.
Dr. Smith’s system of washing the air is admitted to be tedious and
imperfect, though it may be the best in the cases with which he
deals; but it seemed to me that no better method could be devised
for ascertaining the nature of those substances which are held in
suspension in the atmosphere than the one which nature provides
in the form of rain collected as it falls from the clouds.
Two circumstances are well established as regards falling rain.
The first is that at the commencement of a shower after a long-
continued drought the rain brings down much more organic and
inorganic matter than later on; and secondly, that after a heavy
shower the atmosphere is for some time comparatively free from
such matters.
Then as regards the discovery of filaments in infusions, I had
tried some experiments with infusions of orange-juice, orange-peel,
apple-juice, and cabbage-juice, in distilled water, freely exposed to
atmospheric influences, in 1862 and 1863, and when Dr. Bastian’s
observations were published I recollected having found such a
mycelium in orange-juice, and having corresponded with Professor
Hoffmann about it, but as he could throw no light upon the appear-
ance of the mycelium and I was unable to account for it, I dropped
the investigations. A record of these observations was however
kept, and was discovered by me amongst some old papers whilst I
was making the following experiments, and they will now be found
of some service.
On the 4th of August, after a long continuance of intensely
hot weather, we had a violent thunderstorm. I had been expecting
* *Micrographie Dictionary’ (Van Voorst), article ‘‘ Leptothrix.”
1870. | with Recent Haperiments. 493
and preparing for this, and at once proceeded to catch the rain as
it fell, and at the same time to prepare an infusion of filtered
orange-juice 7m pure distilled water. This infusion I divided
between two glass-wells, one of which I closed with cotton-wool,
whilst the other was freely exposed to the atmosphere ; and side
by side with these I placed a tall champagne glass full of the rain-
water which I had collected during the shower, and which contained
numerous particles of dust.
None of these liquids showed any undoubted signs of life when
I examined them with the microscope, before exposure. ‘The
infusion contained organic yellow particles ; the rain-water organic
particles, fragments of minerals, empty sheaths, empty cell-walls,
and minute moving specks.
The very next day, however, August 5th, I was astonished to
find in the open infusion of orange-juice the mycelium figured
and described by Dr. Bastian as having been present in his infu-
sion of turnips, or one closely resembling it; and in my infu-
sion if was accompanied by innumerable minute unicellular oval
organisms, the careful examination of which satisfied me beyond
a doubt that they were an earlier stage of the thread-like filaments.
Some of them were single, others were undergoing subdivision into
two or more segments, whilst on the other hand some of the fila-
ments were giving off cells exactly resembling the smaller detached
ones.
During a long course of microscopical observation of biological
changes, I never was so much astonished as on that occasion to find
with what rapidity Nature (or that I may not be misunderstood—
Nature’s Ruler) brings back to active life the decomposing materials
which have been its previous stronghold; and had I been led away
by momentary impressions I could not have conceived it possible that
the change had been produced in that case by any other process than
heterogenesis, or the elevation of a portion of the organic infusion
into organized types, without the auxiliary influence of pre-existing
germs. But a little reflection reminded me that it is just these
first surprises and impulses which lead men to disseminate erroneous
views, as it was no doubt the extraordinary appearance of maggots
and flies on some decaying carcase which gave rise to the idea of
those insects being spontaneously generated there. I therefore
contented myself with figuring the cells and the mycelium as they
appeared under varying powers of the microscope on the day in
question and the four following days (Figs. 1 and 2), and during
that time the mycelium gradually developed into a true mould or
mildew fungus, some of which floated on the surface. At the same
time numerous ciliated infusoria made their appearance.
On the 9th August I opened the other glass-well containing
the infusion, and found it covered in like manner with mildew. I
2h 2
494 The Controversy on Spontaneous Generation : | Oct.,
carefully removed a portion and delineated one of the dry full-
grown filaments with a cluster of spores in its spore-case at the
extremity (Fig. 3). Of course I was surprised to find the pro-
gress which had been made in this closed infusion, but on con-
sideration it soon occurred to me that if on the one hand the
ingress of the first germs was impeded by the cotton-wool, on the
other, the same agency prevented their egress when they were
produced there, and compelled them to fructify in the vessel in
which they were confined ; and moreover, whilst I had been daily
disturbing the organizations in the open vessel, and adding distilled
water to compensate for evaporation, the other had remained un-
disturbed during the whole period. 4
Then on examining, for the first time after exposure, the rain-
water in the champagne glass, I there discovered large numbers of
the same unicellular organisms as in the two infusions, some single,
others undergoing subdivision, precisely as in the cases described
(Fig. 4), and the natural inference to be drawn from this arcum-
stance would be, of course, that the mildew fungi were the result,
not of spontaneous generation, but of the introduction of germs from
without. But here again it was necessary to exercise caution before
coming to a conclusion. In the first place, the very fact which
I have been trying to demonstrate, wz. the existence of innumer-
able atmospheric germs, at once suggested the probability that
the germs in the rain-water which stood close to the infusions
might have been wafted into it from the fungi growing in those
infusions. And secondly, the slightest residuum in my dipping
tubes, which I might not have cleansed properly, would suffice to
account for the appearance of these cells. These doubts were
partly cleared up at once.
On tasting the infusion which had been covered with cotton, I
found signs of acid fermentation, and I examined drops from the
surface as well as from the bottom of the liquid, for recent investi-
gations on another subject had taught me that during such fermen-
tation the biological phenomena vary in different parts of the fluid.
At the bottom of the fiuid I found clusters of large globular cells
(Fig. 6), and on or near the surface groups of smaller elongated
ones (Fig. 5). I was at once induced to compare these with the
cells of the yeast fungus (Torula cerivisiz) which are delineated
in the ‘Micrographic Dictionary, and were said to have been
found by the observer at the bottom and on the surface of fresh
brewer's wort in which fermentation had just commenced. I
could hardly find any difference between the two sets of cells, and
in both cases those from the bottom of the fluid were round,
whilst the surface cells were elongated. This is of course no proof
of identity ; and although I strongly suspected that in the one case
as in the other the germs had been introduced from without, I
1870. | with Recent Haperiments. 495
guarded myself from considering this as more than prima facie
evidence. Another circumstance tended to show the correctness of
this observation.
I had just found the notes of my experiments with infusions in
1863; and these entries had been made in connection with the
infusion of orange-juice :— :
“ Aug. 3. Mycelium with minute cells.”
“ Like yeast-cells, ‘ Micr. Dict.,’ Plate 20, Fig. 25.”
“Aug. 7. The flocculent deposit tastes like mould.” “ No acid
taste.”
This description and the sketches which accompany it leave me
in no doubt that the appearances were precisely those which I had
observed last month, and the Plate and Fig. referred to m the
‘Micrographie Dictionary’ are strangely enough the same as I had
a second time consulted after an interval of seven years, and which
will be found copied in an article recently published by me on the
manufacture of Beer.*
The same notes contained the following entries :—
1. In regard to an infusion of cabbage-juice exposed July 27th,
and examined August 2nd—
“ Homogeneous cellules.—Little or no motion, and nothing to
indicate whether they were spontaneously produced from cabbage.
Closely resembled sessile monads in dust exposed under coloured
glasses. See paper before Academy ” (des Sciences).
2. Concerning pure distilled water exposed August 2nd, 1863,
examined 7th (temperature 70°)—
“A little mycelium, same as in organic matters.”
The only difficulty I experienced was this. It seemed to me
incredible that the same specific germs which (as I believed) had
floated in the atmosphere in 18638, and had then found their way
into and had become developed in infusions of orange and cabbage
juice as well as in distilled water, should again be present in an
infusion of orange-juice and in distilled water in 1870, but a further
investigation soon decided the matter.
On the 22nd of August last, again, after continued warm dry
weather, the rain set in, and during the first hour I succeeded in catch-
ing some direct from the clouds in two distinct localities: at my
own house, which is in Everton, at the very outskirts of Liverpool,
with gardens about, and trees and fields close at hand; and also in
Vauxhall Road, one of the most unhealthy of the lower parts of the
town, where, notwithstanding the efforts of the sanitary authorities,
the atmosphere is charged with smoke and other emanations from
factory chimneys.
* “ Beer :” see ‘Journal of Science,’ July, 1870.
496 The Controversy on Spontaneous Generation. [ Oct.,
On examining the rain which had fallen in both these localities
I found, naturally enough, no animal or plant germs in that from
the lower part of the town, although it was highly charged with
soot and various kinds of dirt; but in that which had been collected
near my house, I found on the same day a few of the unicellular
organisms as before, some single, others undergoing sub-division ;
also a little soot and silex. On the following day I expected these
germs would have sprouted, and I was not mistaken. I had cleansed
my tubes weil with sulphuric acid, after having made them red-hot,
and had taken every possible precaution to avoid fusion of the fluids
or their contents; but the result was unmistakable. ‘The particles
of soot and silex were present in the Vauxhall Road water, but no
germs of any kind, nor any mycelium; whilst that caught in Everton
was full of unicellular organisms in various stages of growth and sub-
division, and the particles of soot had become beds, as it were, in
which the germs were sprouting, for out of them grew fibrous fila-
ments precisely resembling those which I had first observed in the
infusions (Fig. 7). On the 24th (the following day) these filaments
had assumed the form of a straggling mycelium, not so thick as in
the former infusions, and not so much interlaced, but the identity
of the organisms was quite undoubted. ‘There were also swarms of
minute rapidly-moying infusorial germs along with somewhat larger
ciliated infusoria.
Coupling, then, my experiments of former years with those
recently tried by me, the results, as far as they bear on this con-
troversy, are as follows :—
In 1863. I found in infusions of orange and cabbage juice the
germs and mycelium, which constitute the earlier stages of mildew
fungi, and at the same time I found those lowly plant forms in
pure distilled water which had been exposed to the atmosphere.
Recently I again found this plant type in an infusion of orange-
juice, and traced its growth into a mildew fungus. I also found it
in pure distilled water, and afterwards, well developed, in rain-
water caught as it fell direct from the clouds. This plant, or one
closely allied to it, Dr. Bastian believes to have been spontaneously
generated in an infusion of turnip-juice contained in vacuo in a
closed tube.
Again in 1862-3. Dr. Balbiani in Paris, and I in Liverpool,
found simultaneously in pure distilled water exposed to the atmo-
sphere, and in dust taken from window-panes and elsewhere, various
infusorial animalcule, especially one well-defined type, which I have
again recently found in pure distilled water, and in dust which had
been submitted to a high temperature. And that such animal
germs are present in the atmosphere in all parts of the world, I
showed some years since, by submitting to microscopical observa-
1870.] The Devonshire Association. 497
tion the dust shaken from rags which had been picked up in the
streets of Tunis, Trieste, Melbourne, Bombay, and other places from
which such rags are imported. These animal types, too, are
believed by some to be spontaneously created in infusions.
Here I leave to the judgment of men of science the results of
my experiments, which any boy possessed of a. microscope may re-
peat as effectually as I have performed them. And if the believers
in spontaneous generation still insist that their hypothesis has not
been refuted, and that, assuming my observations to be correct, their
view of the case has not been fully disproved, I am not prepared to
deny this; but on the other hand I must be permitted to retort that
their experiments have only proved, so far, their inability, notwith-
standing all their precautions, to exclude invisible germs from their
infusions. As to the mysterious appearance of these microscopical
types on their solutions ¢ vacuo, what is it compared with the pre-
sence of some of the internal parasites of man and the lower animals?
And who would have credited twenty years since, the story of the
wanderings and metamorphoses which those forms undergo before
they find their way mto the final habitat designed for them by
Nature? ‘There is, however, very little chance of the controversy
coming to an end at present. It is fascinating and exciting, and
in so far quite in accordance with the spirit of the age. Nor is it
desirable that it should cease, for it is causing microscopical observers
to direct their attention more and more to the beginnings of life,
and to the development of those living types which are visible only
with the aid of the lens; and I knowof no subject more worthy of
the consideration of biologists.
ag
Vil. THE DEVONSHIRE ASSOCIATION FOR THE
ADVANCEMENT OF SCIENCE, LITERATURE, AND
ART.
Earty in 1862, it occurred to a few scientific men, residents in
Devonshire, that they might with advantage establish in their own
county an institution resembling the British Association, of which
they had for several years been more or less active members. The
idea having been favourably received in some of the principal towns
of the county, a meeting was held at Plymouth, which, though not
largely attended, was thought to be of sufficient weight to inaugu-
rate the proposed Association, to draw up a provisional constitution,
to elect officers for the first year, and to announce that the first
annual meeting would be held at Exeter on the 14th and 15th of
August, 1862. |
From that time, meetings have been annually held in different
498 The Devonshire Association. [ Oct.,
towns of the county, the number of members and of papers have
steadily increased, and several distinguished men have accepted
the office of President. In short, the Association is not only well
established in the county, but it is also fully and cordially recog-
nized by the scientific world generally.
We proceed to give a brief sketch of its history, constitution,
and operations, believing that there would be little or no difficulty,
and very great advantage, in establishing kindred institutions in the
other counties of the kingdom.
Being limited to a single county, it was decided not to restrict
it to science. It was accordingly named “The Devonshire Asso-
ciation for the Advancement of Science, Literature, and Art,” and
its objects were declared to be “To give a stronger impulse and
a more systematic direction to scientific inquiry in Devonshire ;
and to promote the intercourse of those who cultivate science, lite-
rature, or art, in different parts of the county.” There can be no
doubt that this decision was wise, as it was calculated to enlist a
greater number of members, and to secure more numerous and a
greater variety of papers, whilst it enabled men who might other-
wise regard themselves as unqualified, to accept the office of Pre-
sident.
The number of members has steadily increased from 69 in 1862
to little short of 300 at present; and almost every part of the
county is represented by them.
Each member pays ten shillings annually, or a life composition
of five pounds, and is entitled to tickets of admission for himself
and a lady, as well as to a copy of the annual ‘Transactions.’ Not
only has this small sum been found sufficient to cover all expenses,
but at the meeting held on July 26th, 27th, and 28th, of the
present year (1870), under the presidency of Mr. J. A. Froude,
the eminent historian, the treasurer reported a balance in hand of
upwards of ninety pounds, besides property, in the form of ‘ 'Trans-
actions’ in stock, to the amount of upwards of one hundred and
sixty pounds.
As the Association was not established for the purpose of accu-
mulating money, there is reason to hope that it may very shortly
be in a position to vote small sums for the purpose of conducting
or aiding researches within the county. Devonshire, it is well
known, is rich in bone caverns and barrows which would well repay
investigation, and its moorlands abound in megalithic structures, of
which at least accurate models should be made and placed in the
museums at Exeter, Plymouth, Torquay, and Barnstaple.
' The Presidents are ineligible for re-election. The following is
the entire list, as well as of the dates and places of meeting, from
the beginning :— | 2
1870.] The Devonshire Association. 499
Dates. | Places. Presidents,
1862, August 14th .. .. | Exeter .. .. | Sir J. Bowring, LL.D., F.R.S.
1863, July 29th .. .. | Plymouth .. | Mr.C. Spence Bate, F.R.S., F.LS.
1864, July 20th .. .. | Torquay .. | Mr. E. Vivian, M. A.
1865, June 28th .. .. | Tiverton spill ror. Daubeny, M.D., FBS.
1866, August 8th .. .. | Tavistock .. | Earl Russell, K.G., F.RS.
1867, July 23rd —=—siw«w~S iw. ~ | Barnstaple .. | Mr. W. Pengelly, ERS EGGS:
1868, July 28th .. .. | Honiton .. | Sir J. D. Coleridge, M.A., Q.C.
1869, July 20th .. «.. | Dartmouth ...| Mz..G, P. Bidder, C.E.
1870, July 26th .. .. | Devonport .. | Mr.J.A. Froude, M.A.
The earlier part of the first day of each annual meeting is
devoted to business, and in the evening the President delivers his
address, and thus “reads himself in.” ‘The next day is occupied,
from eleven to four o'clock, with papers and the discussions they
originate; and in the evening the members dine together. The
third day is also devoted to papers, and the meeting closes about
five o'clock.
During the first five years the papers were disposed of in one
day, but since 1866 they have been so numerous as to furnish full
employment for the second day, and it is now understood that the
meeting will last three days.
During the nine years a total of 152 papers have been read,
which may be classified thus :—
Geology and Paleontology .. 40 | Literature —.. 4
Archeology and History .. 35 , Architecture .. 2
Botany and Zoology .. .. 23 ATE Mee Ae 2
Moetesrolopyy sias ops 4 (dary ion HLS Engineering .. 2
Economic Science... .. ., 12 Mental Philosophy 2
EYRICS on. es cat ee ace ALO Biography .. 1
didneations: 9.20) a ele “ate
The Association claims “ the right, at its discretion, of printing
in extenso in its ‘Transactions’ all papers read at the annual meet-
ing,” and this right has been exercised ever since the first year,
when abstracts only of the papers were printed. ‘The copyright of
the papers, however, remains the property of the authors.
One of the laws provides that the Association shall, within
three months after each annual meeting, publish its ‘ Transactions,’
imcluding the Rules, a Financial Statement, a List of the Members,
Obituary Notices of all Members who have died during the year,
the Report of the Council, the President’s Address, and such papers,
in abstract or a eatenso, read at the annual meeting, as shall
be decided by the Council. ‘The annual volumes are accordingly
in the hands of the members within the stipulated time.
The ‘Transactions’ for the first year was a pamphlet of fifty-
four pages, whilst that for 1869—the last which has yet been
500 The Devonshire Association. | Oct.,
printed—was a portly octavo volume of 537 pages. Up to this
time the annual issues form three goodly volumes; and the first
part of the fourth volume, or the fourth volume complete, according
to the quantity of matter, will be printed before the end of October.
They contain a vast amount of information respecting the county
of Devon, together with matter of a more general nature.
Every author receives gratuitously twenty-five reprints of his
paper, and may arrange with the printer for any greater number.
The next annual meeting will be held at Bideford, commencing
August 2nd, 1871, when the Rey. Canon Kingsley will be the
President.
The inhabitants of the towns in which the meetings have been
held have always given the Association a cordial welcome. A large
amount of both public and private hospitality has been displayed,
a conversazione has commonly occupied one of the evenings, and the
day after the close of the meeting has usually been spent in some
picnic or féte.
It may be stated, in conclusion, that the Devonshire Association
originated with men who were and still are members of the British
Association, and whose active work for the offspring has not caused
them to work a whit the less for the parent.
1870.] (501 )
NOTICES OF SCIENTIFIC WORKS.
Researches on Diamagnetism and Magne-crystallic Action, includ-
ing the Question of Diamagnetic Polarity. By Joun Tynpatt,
LL.D., F.R.S., Professor of Natural Philosophy in the Royal
Institution. London: Longmans, 1870.
Tris work is the first instalment of a complete collection of the
original memoirs on experimental physics, which the learned author
has published during the last eighteen years. It contains not
only a record of his own work on the subject of diamagnetism, but
also extracts from the writings of Faraday, Plucker, Becquerel,
Matteucci, Weber, and other experimental philosophers, bearing
upon the same phenomena, so that the reader has before him every-
thing necessary for a complete understanding of this very intricate
subject. The second part of the book contains letters, essays, and
reviews, relating to magnetism and electricity, and includes among
others a discussion on the existence of a magnetic medium in space,
the relation between magnetism and the electric current, an account
of the polymagnet, and one of the clearest descriptions of Ohm’s
theory which we have ever read.
We are so accustomed to see a magnetic substance like iron or
a magnetic needle point north and south, rush to the poles ‘of a
magnet when brought near to one, or arrange itself axially when
suspended between the poles, that it is difficult to imagine that the
vast majority of substances possess almost diametrically opposite
qualities. When brought near to a magnet of sufficient power they
are repelled from it, and when suspended freely between its poles
they swing round, if of an elongated form, and arrange themselves
equatorially or at right angles to the line joming the two poles,
apparently with the object of getting as far away from them as
possible. This action was named by Faraday “ Diamagnetism,”
the common phenomena exhibited by iron being named “ Paramag-
netism,” whilst Magnetism is used as a general term to include the
whole range of both phenomena. Paramagnetic bodies are few in
number, but they include some of extraordinary energy, iron, nickel,
cobalt, and oxygen for instance; whilst diamagnetic bodies include
the greater number of the metals, and such substances as rock
crystal, heavy spar, sulphate of magnesia, marble, alum, common
salt, saltpetre, carbonate of soda, Iceland spar, tartaric acid, citric
acid, water, alcohol, ether, the mineral acids, glass, iodine, phos-
phorus, sulphur, resin, spermaceti, sealing-wax, turpentine, india-
rubber, sugar, starch, gum arabic, wood, fresh beef, blood, apple,
bread, &c. In fact, could a marble statue, or its living prototype,
502 Notices of Scientific Works. | Oct.,
be suspended between the poles of a sufficiently powerful magnet it
would set equatorially, or east and west instead of north and south.
Of all diamagnetic bodies bismuth has attracted the most attention,
owing to the comparative power which it exhibits. Its diamagnetic
properties, although vastly inferior to the paramagnetism of iron,
are yet sufficiently marked to enable its properties to be observed
with small permanent magnets weighing a few ounces; whilst a
bismuth needle freely suspended will set itself parallel to the wires
of a galvanometer. ‘The property is not one possessed permanently
by the bismuth, but is simply induced by the proximity of the
magnet, nothing being communicated which the bismuth can carry
away.
aeog shown almost complete antithesis between the mag-
netism of iron and bismuth, the question naturally arose, Is this
extended to polarity? Faraday worked long and earnestly at this
question, and we believe to the last he was not satisfied that the
question of polarity in diamagnetic bodies was settled, although the
experiments with Weber’s exquisitely beautiful apparatus were tried
in his presence by Professor Tyndali. In a letter to Matteucci,
dated November 2, 1855, Faraday wrote, ‘‘ All Tyndall's results are
to me simple consequences of the tendency of paramagnetic bodies
to go from weaker to stronger places of action, and of diamagnetic
bodies to go from stronger to weaker places of action, combined with
the true polarity or direction of the lines of force in the places of
action.” On the other hand, it would appear as if these two philo-
sophers were looking at the subject from entirely different points of
view. Faraday had his mind fixed on lines of magnetic force, the
use of which, as true representations of nature, he said never failed
him ; whilst Tyndall limited his view to that doubleness of action
in which the term polarity originated. But these were apparent
differences only, not differences in reality, for in the letter just
quoted, Faraday said, “I differ from Tyndall a good deal in phrases,
but when I talk with him I do not find that we differ in facts.
That phrase polarity in its present undefined state is a great
mystifier.”
Considerable space is given to the description of the beautiful
instrument devised by M. Weber in order to submit this question
to a crucial test, the design of which was ably carried out by
M. Leyser, of Leipzig. Clear engravings of it are given, and the
experiments are described in full detail. With it not only has dia-
magnetic polarity been proved to exist in the case of bismuth, but
the same result was obtained with cylinders of calcareous spar,
statuary marble, phosphorus, sulphur, heavy glass, distilled water,
bisulphide of carbon, and other non-conductors of electricity, remoy-
ing the scruples of those who saw in the first experiments of this
sort an action produced by induced currents. By these experiments,
1870. | Notices of Scientific Works. 503
Professor Tyndall concludes that a body of evidence has accumulated.
in favour of diamagnetic polarity, which places it among the most
firmly-established truths of science.
This being the case, it would be of interest to ascertain on
which side exists the fallacy of reasoning by which Professor
Thompson has reduced the existence of diamagnetic polarity to an
apparent absurdity ; the paradox is well stated in the following quo-
tation from a paper by Faraday, “On some Points of Magnetic
Philosophy,” published in the ‘ Philosophical Magazine’ for Feb-
ruary, 1855 :—“ If a globe of bismuth be placed without friction in
the middle of the magnetic field, it will not point or move because
of its shape ; but if it have reverse polarity, it will be in a state of
unstable equilibrium ; and if time be an element, then the ball,
being once moved on its axis ever so little, would then have its
polarity inclined to the magnetic axis, and would go on revolving
for ever, producing a perpetual motion. I do not see how this con-
sequence can be avoided, and therefore cannot admit the principles
on which it rests. ‘he idea of a perpetual motion produced by
static forces is philosophically illogical and impossible, and so I
think is the polarity opposed or adverse static condition to which
I have already referred.”
Of course if time does not enter as an element in diamagnetic
induction the above argument falls to the ground ; but it appears
to be so firmly established a fact that an exertion of physical force
occupies time, that it can scarcely be doubted that it is concerned
here also; that was Faraday’s opinion, although he admitted that
it seemed to be so brief in period as to be inappreciable by the
means he had employed.
We should have liked to give an extended notice of the second
subject included in the title of this work; namely, Magne-crystallic
action,—the phenomena of which were at first so paradoxical as to
bafile the ingenuity of the most acute experimentalists, but, thanks
to the labour of Professor Tyndall and other physicists, now dedu-
cible with as much care and certainty from the action of polar forces
as the precession of the equinoxes is from the force of gravitation.
In the author’s language, “The whole domain of magne-crystallic
action is thus transferred from a region of mechanical enigmas to
one in which our knowledge is as clear and sure as it is regarding
the most elementary phenomena of magnetic action.”
The magne-crystallic force is one by which certain crystals are
caused to set themselves with certain of their axes parallel or trans-
verse to the lines of magnetic force acting on them. This force acts
at a distance, and is by no means so weak as might be at first sup-
posed, for just as a crystal is moved by the magnet at a distance, so
can the crystal also move the magnet at a distance. Faraday ob-
tained the latter result by converting a steel bodkin into a magnet
504 Notices of Scientific Works. [ Oct.,
and suspending it freely in the neighbourhood of the crystal. The
tendency of the needle was always to place itself parallel to the
maegne-crystallic axis.
Neither will space permit us to refer, except in the briefest
manner, to the results obtained by preparing bars of magnetic and
_ diamagnetic substances, by reducing them to fine powder, and then
compressing them in moulds in such a manner that the line of
greatest compression is in different directions along or across the
bar. A bismuth bar so prepared, squeezed flat within the jaws of
a vice and suspended between the poles, will turn with the energy
of a magnetic substance into the axial position; whilst a bar made
up of powdered carbonate of iron (magnetic) compressed in this
manner will recoil from the poles as if violently repelled. It thus
appears that the line of magnetic action has a near relation to that
of the closest contact among the material particles, and this rela-
tionship is traced in many different ways, and appears related to
the cleavage of crystals.
It would be of interest to try some of these experiments on
diamagnetism with the metal Thallium, a metal which, whilst i
rivals, if it does not surpass, bismuth in diamagnetic energy, is as
soft and amorphous as lead, and lends itself with the same facility
to moulding and compression. Probably many of the apparent
anomalies of diamagnetism which observers at first encounter, owing
to the highly crystalline nature of bismuth, would disappear if
thallium were the metal selected for experiment.
We cannot close this book without expressing the profound
admiration which it leaves in the mind for the author’s philosophical
acumen and experimental skill. He moreover possesses one valu-
able quality, which we regret to say is as rare amongst scientific
men as the combination of the two former,—that of placing his views
and describing his experiments in such clear language that the
profoundest mysteries of nature seem under his treatment to become
clear and simple to a child’s comprehension. Speaking as one who
never loses an opportunity of listening to this philosopher on
whom the mantle of Faraday has so worthily descended, the writer
scarcely knows which gives him greater pleasure—to listen to one of
Dr. Tyndall’s lucid expositions of some hitherto hidden mystery of
_ nature, or to hear him in his clear logical manner quietly put down
a scientific opponent who has ventured to differ from some of his
conclusions.
1870. ] Notices of Scientific Works. 505
ON SAVAGES.*
Wnrat Sir Charles Lyell has accomplished for the student of
Geology, Sir John Lubbock is now achieving for the student of
Ethnology. His ‘ Pre-historic Times ’} first excited and awakened
public attention by the clearness of its descriptions and the able
and masterly manner in which the author dealt with the questions
relating to primitive man.
Tn the present work Sir John Lubbock has adopted the same
inductive method of reasoning which has been so ably applied to
geological investigations by the illustrious Lyell in his ‘Prin-
ciples,’ vez. that of explaining the monuments of the earth’s past
history by the “living present.” Thus, from the habits and
customs of modern savages we are enabled to understand the
meaning and uses of the various relics of early man met with in
civilized countries where no primitive races now exist, and we can
thus more accurately picture and more vividly conceive the manners
and customs of our ancestors in bygone ages.
Founded upon a course of lectures, originally delivered at the
Royal Institution in 1868, the author proposes in the present
volume “ more particularly to describe the social and mental condi-
tion of savages, their art, their systems of marriage and of rela-
tionship, their religions, language, moral character, and laws.”
Sir John promises in a future volume to publish those portions of
his lectures which have reference to their houses, dress, boats, arms,
implements, &e.
“The study of the lower races of man,” writes the author,
“apart from the direct importance which it possesses in an empire
like ours, is of great interest from three points of view. In the
first place, the condition and habits of existing savages resemble in
many ways, though not in all, those of our own ancestors in a period
now long gone by; in the second, they illustrate much of what is
passing among ourselves, many customs which have evidently no
relation to present circumstances, and even some ideas which are
rooted in our minds, as fossils are imbedded in the soil; and thirdly,
we can even, by means of them, penetrate some of that mist which
separates the present from the future.” :
On the subject of savage intellect, it seems difficult to realize
the extreme mental inferiority of the lower aborigines; the mind
of the savage, like that of the child, is of wonderfully small capacity
and limited in its powers of taking in ideas; it is easily fatigued
by exercise, and is generally in a dormant state. Curious instances
* «The Origin of Civilization, and the Primitive Condition of Man’ (Mental
and Social Condition of Savages). By Sir John Lubbock, Bart., M.P., F.B.S., &c,
8vo. Pp. 380. London, 1870. Longmans and Co.
+ Originally published (in part) in the ‘Natural History Review.’
506 Notices of Scientific Works. [ Oct.,
of this are mentioned from the accounts of various travellers; in-
deed, the number of authorities quoted under each chapter is truly
surprising. No fewer than 178 authors and upwards of 200 works
have been consulted and are referred to in these pages, the author in
every case being cited, and credited with the statement made on his
authority.
The cosmopolitan character of some customs has induced a
strong belief in the unity of origin of the races among which such
practices prevail; for example, among many races a woman is
absolutely forbidden to speak to her son-in-law. Another curious
custom is that known in Bearn under the name of “ La Couvade.”
It would seem to be a very wide-spread custom for the father, upon
the birth of a child, to be put to bed instead of the mother. The
ideas among savages respecting the influence of food are equally
ludicrous. Thus the Malays give a large price for the flesh of the
tiger, not because they like it, but because they believe that the man
who eats tiger acquires the sagacity as well as the courage of that —
animal. For the same reason the New Zealand baby at its baptism
is made to swallow pebbles, so that its heart might be hard and
incapable of pity. The reflexion of many of these ideas still linger
with children and uneducated persons. A little girl was heard to
say to her brother, “If you eat so much goose you will be quite
silly.” To take the portrait of a native is looked upon as most
injurious, and the better the portrait the worse for the sitter; so
much life could not be put into the copy except at the expense
of the original. Pictures are also considered as efficient charms.
Writing is believed to be even more magical than drawing.
Mungo Park on one occasion profited by this idea; a Bambarran
offered him a supper of rice if he would write him a charm on his
writing-board, to protect him from wicked men. The proposal was
at once accepted. Park wrote the board full from top to bottom
on both sides. The Bambarran, in order to secure the full force of
the charm, washed the writing from the board into a calabash with
a little water, and having said a few prayers over it, drank the
powerful draught; after which, lest a smgle word should escape, he
licked the board until it was quite dry.
The science of medicine, indeed, like that of astronomy, and
. like religion, takes among savages very much the character of
witchcraft. Many savages do not believe in disease or natural
death, but if a man die, however old, they conclude that he must
have been the victim of magic.
Twins are considered as a bad omen, and in most cases one, in
some others both are killed.
The belief in the attributes of life appertainmg to inanimate
objects is also very wide-spread.
A hook that has once caught a big fish is preferred to twenty
1870.] Notices of Scientifie Works. 507
that have never been tried. ‘Two fish-nets are never put together,
for fear they should be jealous. The story of the natives of Tahiti
who sowed some iron nails given them by Captain Cook, hoping
thus to obtain young ones, reminds the writer of the story of a little
boy of his own family, who planted his hair in his garden expecting
it would bring forth a crop of little boys like himself. The ability
or inability to draw seems to vary in one and the same tribe of
aborigines; the absence of perspective is also very general, and
extends to many people otherwise in a highly advanced state of
civilization, such as the Egyptians, Assyrians, and the modern
Chinese.
The earliest traces of art yet discovered belong to the Stone
age—to a time so early that the Reindeer was abundant in the
south of France, and that probably, though on this point there is
some doubt, even the Mammoth had not entirely disappeared.
These works of art are sometimes sculptures, if one may say so, and
sometimes drawings or etchings made on bone or horn with the
point of a flint.
The Esquimaux etchings of the present day appear to approach
most nearly to these early relics from the caves of France, but they
lack the spirited style of execution of the latter.
Upon the marriage rites, if such they may be called, much
information is collected, but, as the author truly observes, many of
the facts which he has recorded are very repugnant to our feelings,
although it was impossible not to mention them in such a work.
Marriage by capture appears to be very general all over the world,
and where not attended by real violence the pretence of using force
and even blows is kept up in form. The practice of carrying off
the bride to the woods may yet linger among civilized nations, as,
for example, in our own custom of the wedding tour.
The position of women among savage nations generally is very
deplorable, nor can any amount of romance render savage life other-
wise than revolting to an educated and civilized man.
Notwithstanding our advanced state of civilization, it is impos-
sible, however, to deny the fact that—
“Tn many of our ideas and tastes we are still influenced by the
condition of our ancestors in bygone ages.”
“What that condition was,’ says the author, “I have in this
work endeavoured to indicate, believing as I do that the earlier
mental stages through which the human race has passed are illus-
trated by the condition of existing or recent savages. The history
of the human race has, I feel satisfied, on the whole been one of
progress. I do not of course mean to say that every race is neces-
sarily advancing: on the contrary, most of the lower ones are
almost stationary ; and there are, no doubt, cases in which nations
have fallen back; but it seems an almost invariable rule that such
VOL. VII. 2M
508 Notices of Scientific Works. [ Oct.,
races are dying out, while those that are stationary in condition are
stationary in numbers also; on the other hand, improving nations
increase in numbers, so that they always encroach on less progres-
sive races.”
It would be impossible in this brief notice to convey a very
adequate idea to the reader of the mass of well-arranged facts upon
which Sir John Lubbock has established his conclusions, but we
give them in his own words.
“The facts and arguments mentioned in this work afford, I
think, strong grounds for the following conclusions, vz. :—
‘“‘ That existing savages are not the descendants of civilized
ancestors ;
“That the primitive condition of man was one of utter
barbarism ;
“That from this condition several races have independently
raised themselves.”
Sir John Lubbock thinks we shall not be the less inclined to
adopt these conclusions on account of the cheering prospects which
they hold out for the future.
We heartily thank the author for his interesting book, which
has afforded us not only much instruction, but also much real
amusement in its perusal.
THE SCIENCE OF BUILDING.*
THe science of building is so comprehensive, and has been treated
by so many able writers, that we must be prepared for some dis-
appointment when perusing a work whose title would lead us to
believe that the whole subject is included in its pages.
Since the application of iron to building purposes, a new study
has presented itself to the architect, and Mr. Tarn’s book contains
many formule with which those who belong to his profession
would do well to make themselves acquainted; for it is not un-
common to find such errors committed by them, as the loading of
cast-iron girders to their full breaking weight, or a waste of metal
in making them stronger than is necessary.
Whilst we commend the work to persons entering the building
trade, we consider it right to mention that the study of mechanics,
such as may be followed with the aid of ‘Tate’s Exercises in
Mechanics, would be even more useful to builders than Mr. Tarn’s
book, as it would sooner make them acquainted with the elements
* ‘The Science of Building: an Elementary Treatise on the Principles of Con-
struction” By E. Wyndham Tarn, M.A., Land Architect. Lockwood and Co.
1870. | Notices of Scientific Works. 509
of mechanics which are indispensable to all who follow the pro-
fession.
In the chapter on retaining walls, the author should have
directed the student’s attention to the various methods of con-
structing them, and should have explained the difference between a
vertical wall having its beds horizontal or perpendicular to its face,
and one with an inclined face, and the transverse section of joint,
perpendicular to that face. Also, in a brick retaining wall some
advantage would be derived from the disposal of the length of brick
or style of bond, and to the architectural student those are matters
of great importance, for in many cases practice seems to defy
theory. The author does not extend his chapters to the relative
strength of brickwork, nor to an account of the various kinds of
bricks made throughout England; details which are now essential
in such a work, as bricks rank in these days amongst the most
important materials of construction. His chapter on arches might
also with advantage have been extended to the flat soffit and head
or cambre arch, showing the limit of span for a given depth and
breadth of face and soffit; also to observations on the grom arch,
which would have imparted originality to his work.
The remarks on mortar and cement are limited, and it would
have been well to refer to their tenacity and resistance to com-
pression, their suitability for various situations; and the advantage
of the application of concrete to bad foundations.
The information on centering of arches is also too much re-
stricted and too indefinite. The pressure of the voussdirs in a
pointed arch could not act on the centre at any of the angles in
the manner named by the author, and it would have been better
had he named the description of arch to which his remarks have
reference, as the pressure of the vousséirs differs considerably in
elliptic, pointed, and semi- or segmented arches.
The chapter on iron does not refer to the segmental or curved
girder which is applied with much advantage in engineering, in
railway and other works. There is also room in the chapter for
observations on the trussed girder and the advantage or disad-
vantage of applying wrought-iron flitch-plates to wood beams.
All these matters should have been referred to, so that the student
of the ‘Science of Building’ (a title by the way which is likely to
mislead those who purchase it into the belief that it is an advanced
treatise) might be prevented from committing many errors into
which architects and builders are too prone to fall.
2m 2
( 510 ) [Oct.,
CHRONICLES OF SCIENCE,
Including the Procerdings of Learned Societies at Home and Abroad;
and Zotices of Recent Scientific Piterature.
1. AGRICULTURE.
Tue drought of 1870, though not so utterly destructive of succu-
lent growth during the summer season as that of 1868, has been
more injurious on the whole. Beginning earlier and ending later,
it has spoiled both the hay crop and the aftermath ; and the wheat
crop too, generally so able to withstand a dry summer, has materially
suffered. The returns from the correspondents of the ‘ Agricultural
Gazette’ declare the wheat crop to be below an average; and all
other grain crops, except barley throughout Scotland, and perhaps
the pea crop throughout the country generally, are still more below
an average. Neither in its return of food for man nor in its pro-
mise of food for beast, does the harvest of 1870 compare favourably
with its predecessors. Mr. Lawes, of Rothamsted, who has for
twenty-seven years subjected the wheat crop to specific treatment
of many different kinds, reports upon the other hand his produce
to be this year above the average. There has been, he says, a
splendid seed-forming and seed-maturing season, acting however in
many cases upon an insufficient amount of plants, and it is probable
therefore that some of the heaviest and some of the lightest crops
ever known in England have been grown this year.
Among the leading agricultural events of the past quarter are
the great annual meetings of the Royal Agricultural Societies of the
three kingdoms. The English Agricultural Society at Oxford and
the Highland Society at Dumfries have had capital meetings. The
Irish Agricultural Society was less successful. One of the most
interesting circumstances of the Oxford meeting was the award of
a valuable prize to the best-managed farm of the district. It has
been somewhat of a surprise and perhaps a disappointment to the
agricultural optimists of the day, that the very competent jury ap-
pointed by the Society to examine the competing farms should have
placed highest upon the list one which owes but little to the im-
proved stock and implements whose use and introduction the
Society has fostered. It is a somewhat old-fashioned style of
management which has been thus decorated. ‘The four-course rota-
tion of wheat, turnips, barley, and clover in succession is the crop-
ping of the farm; the live stock is inferior, and comparatively few
modern implements are in use. The visitor who in the morning
1870. | Agriculture. 511
left the showyard of the Society full of the best specimens of the
finest breeds of all kinds of farm stock and every new agricultural
machine, saw nothing of either on the “ best-managed farm” which
he walked over in the afternoon. He saw, however, magnificent
crops of grain, and roots, and grass, obtained without their aid, and
he might conclude that what was wanted for the improvement of
English agriculture was not a Society stimulating the production
of the best machines and live stock, but an agency for making
farmers more energetic and laborious in the use of the common
means already everywhere at their command.
This agency it is plain exists in an improved relationship between
the landlord and the tenant. The nature of the best farm agreement
has been the subject latterly of frequent discussion in the agricultural
journals. ‘The lease for a term of years, with freedom to cultivate
the land as the tenant chooses up till within a few years of the close
of the term, is certainly the system which gives freest scope to the
intelligence and energy of the tenant, and most likely therefore to
result in industrious and successful cultivation.
An interesting paper “On Wheat Flies” appears in the ‘ Agri-
cultural Gazette, from which we learn that Cecedomyia tritici, to
which Professor Henslow drew attention thirty years ago as the
most destructive wheat midge of his time, is no longer prevalent ;
and that the complaints now common of injury from the wheat
midge are due to Lasitopteryx obfuscata. The former is a yellow
fly, the latter black. ‘The insect is not easily bred, neither Mr.
Kirby, Mr. Curtis, nor Professor Henslow having succeeded. The
successes of Miss Eleanor Ormerod, of Sedbury Park, Chepstow,
which are recorded in the ‘ Agricultural Gazette,’ seem to have
been wholesale, notwithstanding her failures in detail. She placed
on earth in different flower-pots, grubs and pup, with the ears and
stalks to which they respectively adhered, as well from wheat as
barley, protecting each with a covering of gauze or muslin. These
were kept in the most natural conditions, and carefully watched
and tended all through the winter and spring, without producing
anything; but a small heap of wheat rubbish, which had been as-
certained to be well supplied with grubs and pupe, was left in an
out-of-the-way corner by itself, and early in June was found to be
swarming with a cloud of these small Cecidomyia-looking midges,
viz. Lasiopteryx. “ Numbers of these,” says the writer whom we are
quoting, ‘“‘ were also obtained, and sent to us from the wheat fields at
different dates, but not a single specimen of the Cecedomyia tritiet
reached us. Now, is this abundance of Lasvopteryx and scarcity of
Cecidomyia confined to the neighbourhood of Chepstow, or is it
general over the whole country? If so, another question, which
however, we can scarcely hope to fathom, is—when Cecidomyia
ceased to be prevalent, and Lasiopteryx took its place. It may
512 Chronteles of Science. | Oct.,
even be a question whether Cecidomyia ever was generally pre-
valent—it may have been so only in Kigsy’s time and the London
district.”
The Rivers Pollution Commissioners have issued a report upon
the so-called “A BC” process for defecating sewage. They pro-
nounce it a failure. The sewage treated on this plan is not defecated,
and the manure produced is extremely poor. The only advantage
derived from its adoption is a somewhat quickened subsidence of
the suspended matters which town sewage carries with it, but as
every 10 cwt. of these are rattled through the sewers of a town,
borne along in the case of a town with ordinary water supply in a
thousand tons of water, it is not likely that these suspended matters
can retam much that is soluble or valuable on their exit from
the sewer system of a town. And in point of fact the solid matters
of town sewage are of very little agricultural value indeed. It is
the liquid portion that contains the elements of the food of plants ;
and it is this, therefore, in which these substances are present in
too dilute a form to be precipitated that must be carried to the
land, if either a nuisance is to be abated or a valuable property to
be turned to good account. The Commissioners pronounce sewage
wrigation to be the only method known to them by which both these
results can be attained.
There has been an unusual prevalenee of cattle disease during
the past quarter. During the severely restrictive system under
which alone cattle traffic was permitted during the prevalence of
the cattle plague, the more common diseases, the foot-and-mouth
affection and pleuro-pneumonia, almost disappeared. They have
resumed their frequency and virulence with the relaxation of the
rules affecting cattle-markets.
2. ARCH AOLOGY (Pre-Hisroric).
Primeval Monuments of Peru.*— Mr. E. G. Squier, the well-
known American archzologist, has lately explored the early mega-
lithic monuments of Peru. The great plateau of the Andes, elevated
15,000 feet above the sea, and fenced in with high mountains and
frigid deserts, possesses nevertheless a number of stone structures
belonging to what is regarded through the world as the earliest
monumental period, comcident in style and character with the so-
called cromlechs, dolmens, and “Sun” or “ Druidical” circles of
Scandinavia, the British Isles, France, and Northern and Central
Asia
Considerable importance attaches to these remains, as indicating
* By E. G. Squier, MLA., F.S.A.. &. From ‘The American Naturalist,’
vol. iy., 1870, p. 1. -
1870.] Archeology. 513
the existence at one time in Peru of a population identical in the
degree and stage of their constructive development with the people
who raised corresponding lithic and megalithic structures in other
parts of the world, and who, if not the progenitors of the semi-
civilized nations found in Peru at the time of the conquest, certainly
preceded them in the occupation of the country. Mr. Squier
suggests that, “if it should be found that there has been a gradual
development of any of the rude remains into elaborate and imposing
monuments, corresponding with them in their purpose or design,
or a gradual change from the rough burial-chamber of uncut stones
into the symmetrical sepulchral tower, built of hewn blocks ac-
curately fitted together, and in general workmanship coinciding
with the other and most advanced and admirable structures of the
country, then we may reasonably infer that the latter were con-
structed by the same people that built the first, and that, monument-
ally at least, the civilization of Peru was indigenous and gradually
developed, and not introduced.”
The first and simplest form of burial monument, and which the
author assumes to be the oldest, consists of flat unhewn stones of
various lengths set firmly in the ground, projecting above it from
1 to 2 feet, so as to form a circle, more or less regular, about 3 feet
in diameter. In this circle, the body was buried in a crouching
posture, with a vase of pottery or some other utensil or instrument
at its feet. Sometimes a few flat stones were laid across the upright
ones, so as to form a kind of roof. These rude tombs were some-
times placed side by side in long rows, and stones afterwards heaped
over them. A more advanced form of tomb consists of large slabs
of stone projecting 4 to 6 feet above ground, and set in a circle
from 6 to 16 feet in diameter. The top is roofed by blocks of stone
which lap over each other inwardly until they touch, forming a
rude arch or vault. At Quellenata, N.E. of Lake Titicaca in
Bolivia, and at many other places in the ancient Callao, these same
tombs occur, but they are enclosed in a circular wall, varying from
10 to 30 feet in height, the stones broken so as to conform to the
outer curve of the tower, and the whole cemented together with
clay. These round chulpas are of varying excellence in workman-
ship and design, and lead up to the square chulpas of Escoma, the
sides of which are vertical with a projecting cornice near the summit,
and divided internally into two stories or chambers. At Sillustani
the largest and best-built chulpas occur, constructed of great blocks
of trachyte and other hard stones fitted together with unsurpassable
accuracy, the structure nevertheless preserving some of the charac-
teristic features of the first and rudest form of chulpa. ‘The stones
forming the dome are not only cut on accurate radii, but the curve
of the dome is preserved in each, tending to give compactness and
strength to the whole structure.
514 Chronicles of Science. [ Oct.,
Mr. Squier also mentions that many stone structures exist in
Peru, corresponding with the so-called Cyclopean monuments of Italy.
He describes many sun-circles, some composed of simple upright
stones, others having in addition a regular causeway of slabs, form-
ing a platform of stone more or less hewn and fitted together.
In the ancient town of Chicuito, a singularly fine and massive
rectangular monument exists, measuring 65 feet on each side. The
author considers this to be the most advanced megalithic structure
in Peru, and proposes in a future work to illustrate it more fully.
When the whole of Mr. Squier’s drawings are published, he believes
all students of these archaic monuments will agree with him, that
there exist in Peru and Bolivia, high up among the snowy Andes,
the oldest forms of monuments, sepulchral and otherwise, known to
mankind, exact counterparts in character of those of the “old
world,” having a common design, and all of them the work of the
same peoples found in occupation of the country at the time of
the conquest, their later monuments being developed forms of those
by their ancestors, and the earliest the productions of primitive man
in all parts of the world, and not derivative.
Mr. Squier has thus furnished another admirable illustration of
the well-established law that “man under analogous circumstances
will act in a similar manner irrespective of time or space.”
Stone Implements from Burmah.—Myr. W. Theobald, jun., of
the Indian Geological Survey, has communicated some notes on the
stone implements of Burmah, to the Asiatic Society of Bengal.
The implements are curious as differing in form and type, not only
from anything found in India, but from anything hitherto de-
scribed from any part of Kurope, though any implement yet found
in India has its precise analogue in Europe. These implements
are not only singular in form, but also in the material out of which
they are manufactured ; being fashioned either of basalt or some
schistose rock, quite unlike anything met with in the district where
the implements occur: a fact which seems to indicate that they were
brought down from Upper Burmah, where such implements are
common, by the original settlers of the country. ‘The same super-
stition which connects these implements with the “thunderbolt”
prevails in Burmah, where they are called “ mogio,” or thunder-
bolts. Curious traditions prevail as to the virtues possessed by
these heaven-born stones: such, for instance, as preserving from
lightning, fire, shipwreck; conferrmg invulnerability upon the
wearer; great medicinal virtues, a chip administered internally
cuxing inflammation of the liver; it is also a specific for oph-
thalmia, &c. The types of these Burmese instruments described
by Mr. Theobald are:—1. A rough, stout, wedge-shaped instru-
ment, closely resembling the better finished specimens of fiimt-
hatchets, of the type which occurs in the Danish kjokkenméddings.
1870. | Archeology. 515
This form is very rare. 2. A hatchet with flat sides converging
towards the base which is square, and with a segmental edge, much
hike the common German form. ‘This type is common. 3. A long
adze with square, slightly converging sides, and a bevelled seg-
mental edge, in character much resembling some of the implements
discovered in Java, Borneo, and Sumatra, and also a New Zealand
‘form. 4. Implements of the same character, so far as the edge and
sides are concerned, but having tne butt end reduced in width so as
to produce a square shoulder on each side of the blade. In some
this reduction in width extends more than half the length of the
blade, so as to produce a T-shaped form. These shorter speci-
mens are the most common. This form appears to be peculiar to
- Burmah.
Mr. John Evans, F.R.S., F.S.A., offers some valuable critical
notes upon Mr. Theobald’s discovery, in ‘ Nature.’* He says:—
“In some cases the lashings used to fasten them to their hafts
have left traces on the stone. The implements are usually picked
up on the surface of the hills, and in the fields, or clearings made
for cultivation, and not in the plains.
“Mr. Theobald seems inclined to doubt whether, without the
use of iron also, those who made these implements could have
effected clearances in the gigantic forests of Pegu; but it may be
urged against this view that by calling in the aid of fire the effi-
ciency of such tools is almost as great as if they had been formed
of metal, and it is difficult to conceive a people in possession either
of bronze or iron bestowing the necessary time and trouble on the
fashioning of stone tools when those of metal were at their com-
mand, which, whether fire were employed in the clearance or no,
were for general purposes so much more effective. If the makers of
those stone tools had been in possession of other means for clearing
the hill-sides, then Mr. Theobald would be inclined to regard the
stone relics as agricultural implements used in hand agriculture, at
the end of sticks, as a kind of spade, to form the shallow holes for
the cultivation of ‘hill rice.” If not explained in this manner, he
argues, we must regard them as weapons of the chase and war,
though this use is, he thinks, negatived by their thoroughly ineffi-
cient character for such purposes.
“To this may be objected, first, that the material of which they
are usually formed is basalt, a stone constantly used as a material
for cutting-tools ; secondly, that the presence of the square shoulders,
so like those on the horn sockets for hatchets of the Swiss Lake-
dwellers, seems to testify to the tools having been used as adzes or
axes, or possibly chisels ; and thirdly, that if they had been required
merely for hoeing or digging, the trouble of grinding and polishing
might and would have been saved.”
* Vol. ii., No. 32, p. 104.
516 Chronicles of Science. [ Oct.,
The Cheesewring threatened with Destruction.* —This very
remarkable pile of rocks, six or seven miles north of Liskeard in
Cornwall, is threatened with imminent destruction by quarrying
operations at its foot. Will no one prevent its demolition? A
committee was formed some time since for the express purpose of
arresting by all possible means the Vandals who are everywhere
plotting the overthrow of our ancient megalithic monuments,
Surely the preservation of this fine dolmen is worth an effort.
The Meenas of Central India.—Lieut.-Colonel Showers has
communicated to the Asiatic Society of Bengal an account of the
Meenas, a wild tribe of Central India occupying the hilly and
jungly country of Jehazpoor, where they appear to have maintained
their independence and carried on a marauding life for centuries.
They are described as a fine race of men, endowed with great per-
sonal courage, and addicted to the use of arms. They marry freely
with other tribes, but never allow their daughters to marry out of
their own tribe. Polygamy is allowed, each man having three or
four wives. The aggregate male adults in the tribe is about
24,000.
Roman London.—Numerous remains of oxen and horned sheep
were found some few years since on the site of old London Wall,
near Moorgate Street. They had been all killed with the blow of
a blunt instrument on the forehead, probably a stone celt. From
associated relics there can be little doubt that this was one of the
slaughtering places of the ancient inhabitants of London in Roman
times. The Wall-brook evidently ran here, as the foundations of
the old wall was built on piles. Another and recent excavation
repeats the same story, and shows an old river-bed of silt, with
numerous bones of animals.
ETHNOLOGICAL SOCIETY.
At the Ethnological Society papers have been read during the
past quarter by Mr. C. Spence Bate, F.R.S., “On the Pre-historie
Monuments of Dartmoor.” Mr. Bate gives a melancholy account
of the wanton destruction of the cromlechs in this district, and
suggests obtaining legal protection for them before they are all
demolished.
Dr. Caulfield records the discovery of copper celts near Butte-
vant, Co. Cork, and describes a supposed Ogham inscription from
Rusglass, Co. Cork. _
Lieutenant 8. P. Oliver reports the recent destruction of another
cromlech in Jersey.
Professor Huxley gave an interesting account of “the chief
modifications of mankind, and their geographical distribution.”
* ‘Nature,’ vol. ii., p. 101.
1870.] Astronomy. 517
The characters of greatest value are—colour, character of hair, and
form of the skull. The author described five distinct types. 1.
The Australioid. 2. The Negroid. 38. The Xanthochroic, with
fair skin and blue eyes. 4. The Melanchroic, a type with dark
complexion, occupying an area between the Xanthochroic and
Australioid peoples; and 5. The Mongoloid. ‘The paper was
illustrated by a large coloured map showing the distribution of these
five groups and their subdivisions.
Professor Busk described the opening of the Park Cwm Tumulus
in the peninsula of Gower, South Wales.
The Rey. Canon Greenwell read a paper “ On his Exploration
of Grimes’s Grave, Norfolk” (see last Chronicle, p. 383).
Mr. Boyd-Dawkins gave an account of some remains of Platy-
cnemic or Flat-shinned people in Denbighshire. The remains were
found in two bone-caverns, a refuse-heap, and in a tumulus. Simi-
larly-formed bones have been obtained from Cro-Magnon Cave in
France, and the caves of Gibraltar.
Colonel Lane Fox described the Dorchester dykes and Sinodun
Hill, and showed the works were British, and not Roman.
Mr. David Forbes, F.R.S., described the Aymara Indians of
Bolivia and Peru. In stature they are small, massive, and thick-
set, with large heads and short limbs. ‘The trunk is disproportion-
ately large, and the capacity of the thorax enormous, being adapted
to meet the requirements of respiration at an altitude of 8000 to
16,000 feet above the sea-level, where the atmosphere is propor-
tionately rarified. Many interesting customs, &c., relative to this
people were recorded by the author.
ANTHROPOLOGICAL SocImHty.
Dr. Hudson read a paper “On the Irish Celt;” Mr. G. H.
Kinahan “On the Race Elements of the Irish People;” and
Dr. Beddoe “On the Kelts in Ireland.” Dr. Beddoe describes the |
Trish as a dark-haired but light-eyed race, and he argues that
wherever there is light hair it may be accounted for by the Danish
or English intercrossing. The dark hair of the Irish may be, partly
at least, attributed to the Gaelic Kelts.
3. ASTRONOMY.
(Including Proceedings of the Astronomical Society.)
As we write, the prospects of the eclipse expeditions hardly appear
so favourable as could be wished. It seems doubtful whether Go-
vernment will be willing to aid the expeditions by supplying the
518 Chronicles of Science. 7 [Oct.,
means of transport,—the reason suggested for the expected refusal
being the war which is at present devastating France. We can
scarcely believe, however, that the Government will abide by this
resolution. Remembering that some of the most important of those
researches which adorn the annals of English science have been
prosecuted under Government protection, and with Government
aid, while England has been in the throes of deadly warfare—nay,
when the very existence of England has been at stake—we refuse to
believe that the mere risk of war should cause our Government
to refuse a single ship in aid of scientific observations of extreme
interest and importance. |
Unfortunately, the mere report of such a probability has sufficed
to check the process of preparation ; and despite our confidence that
England is not destined to suffer shame in this matter, we are com-
pelled to recognize the possibility that the only systematic observa-
tions of this important eclipse will be made by French astronomers
in Algeria.
Further on will be found an account of the extent to which the
eclipse will be partially visible in this country.
Dr. Zoilner, known as one of the most successful students of
solar physics, has been inquiring into the evidence which the form
and dimensions of prominences afford respecting the temperature
and physical condition of the sun. He points out that prominences
may be divided into two classes, the cloud-formed and the eruptive
prominences. Those belonging to the latter class are so obviously
due to real eruptive action that we may fairly refer them to the
same general cause as terrestrial eruptions, that is, to a difference
between the pressure in the region whence the erupted matter flows
and the pressure in the space into which that matter passes. But
this view requires us to believe that there is a barrier-layer (Tven-
nungschicht) by which one region is separated from the other—a
stratum limiting the compressed hydrogen below the chromosphere
from the free atmosphere of hydrogen which constitutes a propor-
tion of that envelope. |
Starting with this hypothesis, Dr. Zéllner proceeds to apply the
mechanical theory of heat to determine the temperature of different
portions of the sun’s globe. We see that the prominences are pro-
jected to a certain height, and we have therefore a means of de-
termining the force exerted in the propulsion of the compressed
hydrogen. The equations for this purpose are those resulting from
the law of Mariotte and Gay-Lussac, and those which are deduced
from the theory of heat. Certain assumptions have to be made, the
probability of whose truth depends on the imterpretation of tele-
scopic and spectroscopic observations of the sun.
Some of the results are of great interest, especially as, even
though the fundamental suppositions should be importantly im error,
1870. | Astronomy. 519
the conclusions would still be but slightly affected. Zollner finds
the minimum temperature of the base of the solar atmosphere to be
about 27,700° Centigrade, and the corresponding temperature in the
region whence the prominences are projected to be about 68,400°
Cent. He calculates the pressure in this last-named region at
4,070,000 atmospheres, while the pressure outside the stratum en-
closing this region he calculates at 184,000 atmospheres. He then
shows that whereas these results have been obtained on the suppo-
sition that the pressure at the base of the chromosphere is but that
corresponding to about 7 inches (180 mm.) of the mercurial baro-
meter, the actual pressure of the nitrogen and oxygen atmospheres _
at this level must be almost infinitely minute. But he remarks that
this alone does not suffice to explain the absence of the lines of these
elements from the spectrum of the sun, since the lines of volatilized
metals are seen. He attributes the visibility of the latter lines to
the fact that the vapours of the metallic and alkaline elements have
a much greater emissive power, and consequently a much greater
absorptive power than those of the permanent gases.
To proceed further with the discussion of his researches would
bring us upon ground altogether removed from astronomy. We
may remark, however, that there is one point which seems to us to
have been too little considered in these and similar researches. It is
assumed that spectroscopic researches enable us to determine the
actual pressure at the base of the chromosphere. As a matter of fact,
we have no means of knowing whether the estimated pressure belongs
to the base of the chromosphere or to a height of ten, a hundred, or
even a thousand miles above the solar photosphere. It must be re-
membered that 1000 miles at the sun’s distance subtends little more
than two seconds of are, the minuteness of which distance will be
appreciated by those who have examined double stars two or three
seconds apart, even with very powerful telescopes. Assuming that —
with the magnifying power employed (magnifying power being an
essential element in such applications of the spectroscope as we are
here considering) an arc of two seconds could be recognized, yet the
tenth part of such an arc would be wholly inappreciable. Now the
increase of pressure within a distance of 100 miles from the base of
the chromosphere is probably more considerable than that occurring
throughout all the thousands of miles of chromospheric height above
that level.
The most important astronomical event of the next quarter is un-
doubtedly the great eclipse of December 22nd next. In England
it will be considerable though not total. The following are the data
for the principal places in the British Isles:—
At Greenwich the eclipse will begin at 11h. 8m. a.m, reach its
ereatest phase at 12h. 25m. (when 0°814 of the sun’s dise will be
concealed by the moon), and end at 1h. 42 m. p.m.
520 Chronicles of Science. | Oct.,
At Cambridge the eclipse will begin at 11h. 9m. a.m. (mean
time at Cambridge), reach its greatest phase at 12h. 26m. (when
0 808 of the sun’s disc will be concealed), and end at 1 h. 42 m. p.m.
At Oxford the eclipse will begin at 11h. 1m. a.m. (mean time
at Oxford), reach its greatest phase at 12h. 18 m. (when 0°813 of
the sun’s dise will be concealed), and end at 1h. 35m. p.m.
At Liverpool the eclipse will begin at 10h. 52m. a.m. (mean
time at Liverpool), reach its greatest phase at 12h. 8m. (when
0-804 of the sun’s disc will be eclipsed), and end at 1h. 24 m. p.m.
At Edinburgh the eclipse will begin at 10h. 53m. a.m. (mean
time at Edinburgh), reach its greatest phase at 12h. 7m. (when
0-788 of the sun’s disc will be concealed by the moon), and end at
Lh, 21m. p.m.
Lastly, at Dublin the eclipse will begin at 10h. 34m. a.m.
(Dublin mean time), reach its greatest phase at 11h. 50m. a.m.
(when 0-812 of the sun’s disc will be eclipsed), and end at
Lh. 6m. p.m.
We may remind our readers that on the 12th, 13th, and 14th
of November, shooting stars may be looked for. A year or two back
it was possible to indicate somewhat more definitely the time when
the display was to be expected ; but it needs only a careful study of
the phenomena presented by the successive showers, since the great
one of 1866, to prove that the meteor-system has been widening
out, growing in the meantime less and less rich: so that while we
may be tolerably certain of seeing many November meteors, there is
small chance of a display resembling that of the year 1866.
The planet Jupiter will be well situated for observation during
the next quarter, coming to opposition on December 13th. Saturn
on the contrary is passing away from our nocturnal skies, and will
be in conjunction with the sun on December 22nd. Mars is return-
ing, but only at the end of the year will he be near enough to be
worth studying telescopically. He comes into opposition on March
19th, 1871.
PROCEEDINGS OF THE ASTRONOMICAL SOCIETY.
Lieut. Brown supplies an important paper on December weather
in the neighbourhood of Gibraltar. It appears from the meteoro-
logical observations he records that there is every reason to antici-
ate favourable weather during the eclipse of December 22nd next.
From the 15th to the 31st December there were in 1860, 6 very
good days; in 1861,3; in 1862,10; m1863, 13; in 1864,5; in
1865, 12; in 1866, 6; in 1867, 8; in 1868, 11; and in 1869, 7;
—the bad days in those years numbered, respectively, 5, 9, 1, 1, 2,
1, 2,3, 1,1. So that in all there were 81 good days and but 254
bad ones, the remaining 644 being indifferent.
1870. | Astronomy. 521
Commander Ashe endeavours to show that the Council of the
Astronomical Society were not justified in expressing the opinion
that “in photographs 3 and 4” (of his set of 4, illustrating the
American eclipse) “there is evidence of the disturbance of the tele-
scope during the exposure of the sensitive plate. But there seems
every reason to accept the opinion of the very able committee ap-
pointed by the Council to consider the matter, and the members of
this committee “unanimously report that in their opinion there was
a decided moyement of the instrument at the time the photograph
was taken; a conclusion arrived at from an examination of the
chromosphere close to the moon’s limb, as well as from an examina-
tion of the prominences.” |
In a description of the occultation of Saturn by the moon on
April 19, 1870, Captain Noble dwells on the exceeding sharpness
of Saturn’s definition; the most delicate details being perceptible,
even In contact with the moon’s limb. ‘The crape ring C was seen
most perfectly where the dark limb of the moon crossed it. “I
never was more impressed,” remarks this skilful observer, “ with the
absolute absence of a lunar atmosphere of any appreciable density
than I was on this occasion.”
Mr. Penrose, from observation of the star Algol, concludes that
the period of 2°86727 days assigned to this remarkable variable in
Herschel’s ‘Outlines of Astronomy’ requires to be slightly corrected.
The minima occurred nearly three hours earlier than the epochs
calculated with the above period from a minimum which occurred
on January 3, 1844. The shortening of the period of this variable
is certainly a remarkable and interesting circumstance. Observers
should watch from time to time the occurrence of the well-marked
minimum, in order to see whether the reduction of the period is
steadily progressing, or to detect signs of its being eventually trans-
mitted into the reverse process, as in the case of planetary pertur-
bations.
Mr. Proctor, in a paper “On the Resolvability of Star-groups
regarded as a Test of Distance,” points out that there is good reason
for doubting whether we can form any opinion whatever respecting
the distance.of a cluster of stars from the telescopic power necessary
to completely resolve it. He shows that a star-group may be so
constituted that let its distance be ever so great it cannot appear
nebulous, or again that conceiving its distance to be increased so
that it passed eventually beyond the range of our most powerful
telescopes, it would pass from irresolvability to resolvability and
again to irresolvability through the mere effect of a continually in-
creasing distance. The question of the resolvability of a star-group
depends not on distance alone, but on the relation between the
magnitudes of the component stars and the distances separating
them. If the magnitudes are such that the stars would vanish in-
522 Chronicles of Science. [Oct.,
dividually through increase of distance, before their distances from
each other became evanescent, the group (or the special order of
stars considered—as the case may be) could not possibly present a
nebulous appearance, at any stage of its recession, with whatever
telescopic power it was studied. On the other hand, if the distances
between the stars became evanescent before the stars vanished in-
dividually, the group or order of stars must necessarily become
nebulous when it reached a certain distance. In the case of a
group consisting of several orders of stars, one order might thus
become nebulous at a certain distance, but with yet greater increase
of distance this nebulosity would vanish, and the question whether
any new nebulosity would replace it would depend wholly on the
question whether the next higher orders of stars belonged to one
or other of the classes considered above. Considerations thus ap-
plied to a group of stars passing away from the eye, may obviously
be extended to star-groups at various distances; and since we could
not judge of the distance of the moving group from its resolvability
or irresolvability, so neither can we place any reliance on those
estimates of the distances of nebule which have been founded on
their resolution.
Mr. Williams describes some early telescopes made by Giuseppe
Campani which he purchased at the sale of the late Dr. Lee’s in-
struments. Jeaders of the ‘ Celestial Cycle’ and its ‘ Prolegomena’
will not need to be reminded that these instruments were tested by
the late Admiral Smyth. .
Mr. Powell communicates a paper “On the Double Star a
Centauri.” The companion has recently reached its lesser maximum
of distance, and has commenced its return towards the primary.
Thus an exactitude of determination has become possible, which
(as Captain Jacob used to remark) was impossible while it remained
unknown how far the companion would pursue its northerly ex-
cursion. The following are the elements which Mr. Powell now
assigns to the orbit :—
Longitude of periaster .. 38°°40 BEMGaxIS. .. “ee p73 207-13
Hecentrieity |<) 2G Fer esgee 7° Pertod 2-899 76°25
Risme node 2)-.npiee 9) 240718 | Periastral passage .. 1874°2
UmGMNALIOR, 6 oe a cechin as WEL tee
These results differ somewhat importantly from those obtained by
Sir John Herschel, Hind, and formerly by Mr. Powell himself.
Mr. Seabroke endeavours to show that Mr. Lockyer’s theory
that the corona is a phenomenon of the earth’s atmosphere “is quite
possible.” For this purpose he considers how far such spectroscopic
results as Major Tennant obtained during the Indian eclipse, might
be accounted for on that theory. It is unfortunate that in place of
dealing with the actual circumstances of that eclipse, Mr. Seacombe
determines “what spectrum we ought to obtain from a corona at
1870.] Astronomy. 523
a point on the earth where the limbs of the sun and moon are in a
line; that is, where the eclipse is total exactly.” In any given
total eclipse the coincidence of the limbs of the sun and moon is
necessarily a momentary phenomenon; and the state of things at
the moment is altogether exceptional. What has to be explained
before Mr. Lockyer’s strange theory can be admitted, is the observed
state of things when lines from the sun’s limb to the moon’s disc
fell eighty miles or so from the observer's station. Mr. Lockyer
himself has begun to recognize the necessity of explainng away
this difficulty, and he now supplements his theory by introducing
“a possible action at the moon’s limb,” though what the nature of
that action may be he forbears to indicate.
Mr. Browning gives an account, accompanied with illustrations,
of his ingeniously devised automatic spectroscope referred to in our
last. When this paper was read before the Royal Astronomical
Society, Professor Pritchard stated that he had given several hours
to the examination of the optical relations of the new instrument,
but could not definitely assert that minimum deviation is secured
for rays of all orders of refrangibility. Although the instrument
is probably as perfect practically as it can be made by whatever
further refinements may be adopted, it requires but little considera-
tion to show that it does not in its present form theoretically secure
true minimum deviation for all rays. The fixity of the first prism
(the collimator being also fixed) suffices to prevent this. We believe
that Mr. Browning is now at work on a modification of his instru-
ment which has been suggested to him, in which this objection is
obviated.
Fr. Perry, of the Stoneyhurst Observatory, gives an account
of an observation made on Winneeke’s new comet (discovered on
May 30, at Carlsruhe). He had searched in vain for D’Arrest’s
comet. Mr. Hind sends the elements (calculated by Winneeke
himself) of the former comet, which is described as a round pretty
bright nebula, about 24 minutes in diameter.
Lieut. Hill, on May 22, saw three large spots on the sun, with
the naked eye. On the following day a fourth spot was visible.
We believe that this is the first instance on record in which so many
spots have been seen without telescopic aid.
In a paper on the stereographic projection, Professor Cayley
points out that the very same circles which in the direct stereo-
graphic projection of a hemisphere (viz. that wherein the projection
is on the plane of a meridian) represent the meridians and parallels
respectively—represent also in the oblique projection of the hemi-
sphere meridians and parallels respectively.
Mr. Lynn discusses the proper motion of the star “ Groombridge,
1830.” He finds as the final result of his examination of the
VOL, VI. 2N
524 Chronicles of Science. [ Oct.,
Greenwich records of this star, the following mean annual proper
motions in four several intervals :—
Years. Proper Motion in R. A. Proper Motion N. P. D.
1845-1850 ee +05°*358 ee os +5'-82
1850-1860 a gee 0°343 EE rk 9°73
1860-1864 er 0-336 foe oo 5°93
1864-1869 ee re +0°338 AP wee! +5°71
We may fairly assume that the mean of these values (properly
weighted) represents the true value of the star’s motion—which it
will be seen is exceptionally large.
4, BOTANY.
Evaporation of Water from Plants.—Some researches have recently
been undertaken by Von Pettenkofer on the amount of evaporation
which takes place from the foliage of plants. The experiments
were made in the case of an oak tree, and extended over the whole
period of its summer growth. He found the amount of evapora-
tion to increase gradually from May to July, and then decrease till
October. The number of leaves on the tree were estimated at
751,592, and the total amount of evaporation in the year at 539-16
cubic centimetres of water for the whole area of the leaves. The
average amount of rainfall for the same period is only 65 cubic
centimétres; the amount of evaporation is thus 84 times more
than that of the rainfall. The excess must be drawn up by the
roots from a great depth; and thus trees prevent the gradual
drying of a climate, by restoring to the air the moisture which
would otherwise be carried off by drainage.
Germination of Palms.—Mr. J. W. Jackson, Curator of the
Museum at Kew, has published a useful paper “On the Germina-
tion of Palms.” This is incorrectly described in all the botanical
text-books commonly in use. The peculiarity consists in the end
of the cotyledon remaining in the seed, whilst its stalk is pushed
out, carrymg with it the radicle, which germinates in the usual
manner at a little distance from the seed. In the double cocoa-nut,
Lodoicea, the protruded end of the cotyledon is as much as 12
or 18 inches long. The sheath or socket at the base of the stem
of this palm is shown not to be peculiar to it, as has been supposed,
though more developed than in other species, and to be formed by
the vascular bundles of the rudimentary and early leaves.
Existence of a Formative Layer in the Leaves of Plants.—
M. Cave has recently pointed out that a formative layer exists in
the leaves of plants, similar to the well-known cambium layer,
which, in exogenous plants, intervenes between the bark and the
1870. | Botany. 525
wood, and from which the new wood is formed. He finds it not
only in the leaves, but in all foliar or ‘‘appendicular”’ organs,
normal or modified, as for instance the flowers, but occupying a
different position to the cambium layer, namely, between the tissue
of the organ itself and the epidermis. The knowledge of this fact
M. Cave applies to determine a morphological question which is
often a matter of controversy, whether a particular organ belongs
to the axis, to the foliage, or to both sets of organs combined ; and
he shows that if the formative layer is exterior to the fibro-vascular
system, the organ belongs to the leaves; if interior to it, to the stem.
The application of this test proves that the receptacle-like peri-
gynous calyx of many plants is a dependency of the axis; while
the pericarp of superior fruits is always formed of metamorphosed
leaves and nothing else; this is also the case with the axile and
parietal placentze; but the free central placenta, as in the case of
Primulacez, is a prolongation of the axis. Fruits proceeding from
an inferior ovary are composed of two parts, varying in their mutual
proportion in different plants, a receptacle-like calyx and carpellary
leaves. It is noteworthy that M. Cave found this formative layer
to occupy the same position in the leaves and fruits of endogens as
in those of exogens.
Changes in the Colour of Flowers produced by Ammonia.—
M. Vogel has recently published the results of some experiments
on the changes produced by ammonia in some vegetable colours,
especially those of flowers, which he thinks may be of practical
importance in the manufacture of vegetable colouring matters of a
character similar to the aniline dyes. The colouring matter he
states to be of two kinds, united with a different degree of persist-
ence to the tissue of the flower itself, and requiring a shorter or
longer time to produce any alteration. The change produced in
the colour of some flowers, as the rose and phlox, by the fumes of
tobacco, is entirely due to its ammoniacal element. M. Vogel
found that some colours are altogether unchanged by lengthened
exposure to ammonia; as, for instance, yellows, all reds (except in
the case of the Zinnia, which is converted into a brown-red), and
dark violets. Blue is sometimes unaltered, sometimes changed into
a dirty green and then bleached. In some cases, not only the
colour but the tissue of the flower is destroyed. The changes are
generally the same as those that take place during the withering
of the flower.
Electricity in Plant Life-—A writer in the ‘Gardener’s
Chronicle’ points out the important part played by electricity in
the phenomena of vegetable life. He states that every hair and
sharp point in the vegetable kingdom is necessarily a conductor of
electricity, which must always be present wherever water rises in
the form of vapour. Hence all the young and growing parts of
2N 2
526 Chronicles of Science. { Oct.,
plants are clothed with delicate hairs; and the same is generally
the case with those fruits or other parts which have a very fine
and delicate scent or flavour, these qualities being, the writer
believes, greatly developed by the agency of electricity.
Poisoning by Ginanthe crocata.—Myr. Worthington G. Smith
records an instance of poisoning by the water dropwort, Ginanthe
crocata, a common Umbelliferous plant in the South of England.
A carter, whilst at work, ate some of the roots, supposing them to
be wild parsnips; in about an hour he became unconscious and
convulsed, and death occurred in another half-hour, before medical
assistance could be obtained. The man had fed his horse with roots
of the same plant, and the animal also expired about two hours
after eating them. The plant belongs to that group of narcotico-
acrid poisons comprising the Solanacez (Belladonna, Hyoscyamus,
&c.), and characterized by producing convulsions with delirium.
The juice of the plant was in this instance of a yellow colour; it
has been stated that a variety of the plant with colourless juice is
a less virulent poison. ‘The taste of the root is said to be inter-
mediate between that of celery and turnip.
Mistletoe on the Oak.—Dr. Bull records, in the ‘ Transactions
of the Woolhope Naturalists’ Field Club,’ a very interesting case of
this extremely rare occurrence. ‘The tree grows in the hedge-row
of a field called the Harps, at Haven Aymestry, in the ancient
forest of Deerfold, in Herefordshire. It was discovered in the
spring of 1869, but the mistletoe must have been growing on the
oak for some years. The oak is of the variety sesseliflora, and may
be some fifty or sixty years old. The mistletoe is a female plant,
and grows high up on the main stem. It forms a large spreading
bunch, with a diameter of 3 feet 6 inches, and springs out from
the oak in a single stem, nearly 4 inches in circumference. ‘The
mistletoe is also growing on a thorn close by, and has probably
sprung from a seed dropped by a bird from above. The great
rarity of the growth of mistletoe on the oak is proved by the fact
that there are put eight examples which have been well authenti-
cated as existing at the present time; the localities being Eastnor
Park, Herefordshire ; Tedstone Delamere, Herefordshire; Forest of
Deerfold, Herefordshire; Frampton-on-Severn, Gloucestershire ;
Sudbury Park, Monmouthshire; Dunsfold, Surrey; Hackwood
Park, Hants; and one near Plymouth,
The Cinchona in the West Indies.—In a recently-issued Colo-
nial Blue-Book, Sir James P. Grant, the Governor of Jamaica,
states that the cinchona plantation in that island may now be pro-
nounced a complete success. Cinchona plants were first received
in 1866. By the close of 1867 the number of young plants had
so much increased, that it became necessary to provide land for
their final establishment on a planter’s scale. Six hundred acres of
1870. | Botany. 527
virgin forest in the Blue Mountain were acquired early in the year,
and were set apart for the purpose of a cinchona plantation, for
which the place is in every way admirably suited. The elevation
varies from 4000 to 6000 feet. It is well watered, has the best
aspects, and possesses a soil reported to be admirably adapted to
the requirements of the cinchona. Fifty acres were cleared, of
which forty were filled with cichonas in the course of the year;
about 20,000 plants of five different species having been planted.
By the latest accounts all of these were in full vigour, and the plan-
tation must by this time be doubled in extent. The plants have
stood one of the driest seasons that has ever been remembered on
Blue Mountain, without suffering in the least. There is now no
doubt that the cinchona can be successfully reared in Jamaica.
Origin of Prairie Vegetation.—Professor Winchell, of the Uni-
versity of Michigan, has recently promulgated a new theory re-
specting the origin of the vegetation of the American prairies,
namely, that it dates back beyond the historical epoch to the Glacial
period. He believes the origin of the prairies to be lacustrine; but,
contrary to the generally-received opinion, he maintains that lacus-
trine sediments contain no living germs. JDiluvial deposits, he
states, on the contrary, are found everywhere replete with living
germs, which, when hidden away from the influence of light and
moisture, retain their vitality or power of germination for an in-
definite length of time. These living germs of the diluvial deposits
he believes to have been buried during the glacial period, in the
course of which the surface was ploughed up by glaciers, and
afterwards exposed to the commotion of the sea, which overspread
the land, burying everything in promiscuous ruin; but yet by this
very means storing away the seeds which, when brought to the sur-
face after the lapse of a geological age, are possessed of vitality, and
able to reclothe the barren earth with verdure and beauty. ‘Thus,
in proportion as the diluvial surface became exposed, the flora of
the pre-glacial epoch was reproduced. In support of this theory, he
brings forward the argument that the fossil plants which have been
discovered in the tertiary deposits show a correspondence of genera,
and in some cases even of species, with those existing at the present
time.
The Herbarium of the British Musewm.—The Curator of the
British Museum Herbarium has just published his annual report of
the national collection. A considerable number of families have
been re-arranged, and collections incorporated in the general her-
barium from Mexico, New Granada, Nicaragua, Ecuador, California,
India, and other countries. The most important additions to the
herbarium have been 2000 plants from Abyssinia, and upwards of
2000 from South Africa, as well as more than 1000 European
plants, and a number of smaller collections. Various portions of
528 Chronicles of Science. | Oct.,
the British herbarium, and the collection of fruit and seeds, have
been re-arranged, and the recent and fossil Coniferz and Cycadex
have been examined and arranged.
The Botame Garden at Brussels—The Belgian Government
recently purchased the magnificent collection of dried plants of the
late Von Martius as the nucleus of a national herbarium. It
has more recently concluded the purchase of the Botanic Garden
belonging to the Horticultural Society of Belgium; and has thus
commenced the formation of a national establishment intended to
rival those of Paris and London.
5. CHEMISTRY.
Or all the non-metallic elements, fluorine appears the most dif-
ficult to bring under the domain of organic chemistry ; very few
compounds of this element with carbon, hydrogen, and nitrogen
being known. Dr. R. Schmitt and H. von Gehren have recently
succeeded in preparing Fluorbenzoic acid and Fluorbenzol. Fluor-
benzoic acid is prepared from diazo-amidobenzoic acid by treating
that substance at a high temperature in a platinum basin with
hydrofluoric acid. The fluorbenzoic acid thus obtained resembles,
as far as its physical properties are concerned, benzoic acid; it is,
however, far more volatile, fuses at 182° C., is difficultly soluble in
cold, readily in hot water, and soluble also in ether and alcohol;
its aqueous solution exhibits a strongly acid reaction to test-paper
and decomposes inorganic carbonates very readily ; the acid does not
act upon glass, and is a very fixed substance, which may be even
dissolved in concentrated sulphuric acid without decomposition.
Fluorbenzol is a crystalline solid, boiling at about 183° C., fusing
at 40°, insoluble in water, and specifically heavier than that liquid,
readily soluble in ether and alcohol.
Whilst organic chemistry is aptly called the chemistry of
carbon, Drs. Friedel and Ladenburg are engaged in researches
which tend to place silicium parallel to the former element. They
have succeeded in preparing what they call silico-propionic acid, a
compound wherein a large percentage of the carbon of propionic
acid is replaced by silictum. The physical aspect and many of
the properties of this body are akin to silica; but it is a com-
bustible substance, insoluble in water, but soluble in a hot and
concentrated solution of caustic potassa. M. Dumas observed, in
reference to this paper, that it is not impossible that there exist in
nature organic compounds of silica, a remark which gave rise to
some observations on Dr. Friedel’s ‘Memoir, by P. Thenard. The
author begins with stating that M. Dumas is quite right, and
1870.] Chemistry. 529
relates further that he (M. Thenard) is at present engaged on
researches of organic acids which contain even 24 per cent. of
silica entirely disguised. When ulmic acid is treated by ammonia,
azhumie acid is formed ; this contains nitrogen so fixedly, that it is
only eliminated at a temperature of about 1200°: This acid is pos-
sessed of the remarkable property of readily dissolving silica, and
combining therewith in the same manner as the compound alluded
to above by Dr. Friedel. The author also states that although his
researches on this subject are not yet quite concluded, he is justified
in stating that all arable and garden soil, and far more so farmyard
manure, contain similar organic silicious compounds which play an
important part in the feeding of the plants.
That indefatigable savan, the Abbé Moigno, has recorded that
when picric acid is introduced into a vessel containing ozone, a
violent detonation instantaneously takes place, a new proof of the
danger attending experiments with nitrogenous compounds contain-
ing nitrogen only loosely bound.
The utility of mixig peroxide of manganese, for which, how-
ever, may be substituted substances such as peroxide of iron, oxides
of zinc and tin, burnt gypsum, and others, provided they are pre-
viously well dried (best by ignition) with chlorate of potassa, is
based according to Dr. G. Krebs upon the fact that the substances
alluded to, which are infusible by themselves, are the carriers and
transferers of heat to the chlorate of potassa, each particle of which
is surrounded with a source of heat, which aids its rapid decom-
position. The peroxide of manganese is prevented from being -
itself decomposed, because the chlorate of potassa withdraws from it
heat, for the purpose, first of its own fusion, whereby heat becomes
latent ; secondly, by its decomposition. The author states that
when oxide of iron, or peroxide of manganese, is strongly heated
in a crucible, and chlorate of potassa very gently fused at the same
time by itself in a porcelain dish, the addition of the moderately
hot oxides to the fused chlorate causes the evolution of oxygen to
set in instantaneously, and with so great violence, that unless this
experiment be performed in open vessels and with small quantities
at a time, serious explosions may occur.
A compound of hydrogen and mercury, which the discoverer
calls Hydrogenium-amalgam, has been prepared by O. Loew, by
shaking together in a vessel, to be kept very cool, a mixture of
mercury containing from 1 to 2 per cent. of metallic zinc, along
with an equal bulk of a solution of chloride of platinum containing
10 per cent. of solid chloride. A slimy mass is obtained, devoid of
metallic lustre and prone to decomposition, owing to the presence
of zine and some compounds of that metal; but on treating the
mass with dilute hydrochloric acid, a body having the consistence
530 Chronicles of Science. | Oct.,
of butter is obtained, which according to the author is a true
amalgam of mercury and hydrogenium. The author describes at
length several reactions of this body, which in many of its pro-
perties is akin to hydrogenium-palladium. Professor C. A. Seeley,
speaking of this amalgam and the allied ammonium amalgam, gives
it as his firm opinion that they are only mechanical mixtures of
mercury and gases. In illustration of this he describes an im-
portant experiment to prove that if ammonium amalgam be subjected
to varying pressure, its volume changes, apparently, in accordance
with Mariotte’s law of gaseous volume. To illustrate this, a glass
tube 4 inch in diameter, 20 inches long, and fitted with a plunger,
was employed. Mercury containing a little sodium was poured
into the tube to 4 inch in depth ; and upon this was poured a strong
solution of chloride of ammonium occupying about 2 inches in
length of the tube. The ammonium amalgam was completely
formed in a few minutes, and occupied several inches of the tube.
On adjusting and depressing the plunger, the volume of the
amalgam progressively diminished till it closely approached the
original volume of the mercury. Also, it was notable that
the amalgam progressively gained fluidity and the mirror surface
till, at the greatest pressure, the original volume and appearance of
the metal were resumed, whilst on reducing the pressure below
that of the air, the amalgam still expanded until it rose above the
surface of the liquid in the tube. If the great pressure be main-
tained, more ammonium amalgam will be formed, the mass expand-
ing progressively, apparently in accordance with the fact that the
absorption or adhesion of gases to liquids is favoured by pressure.
By means of the simple apparatus used, a pressure of ten atmo-
spheres or a good vacuum are easily and at once obtaimable, and the
experiments with itare very striking. The considerations regarding
ammonium amalgam are evidently equally applicable to Loew's
hydrogenium amalgam; both may be only metallic froths. The ex-
pansion of palladium observed by Graham, on its absorption of hydro-
gen, is probably analogous to the case in question. In both cases,
the gases concerned are condensed, by reason of their attraction
to the metal; and if the molecules of palladium were made free
to move, as those of mercury, it is probable that Graham’s hydro-
genium alloy would become a palladic froth, more remarkable than
the corresponding mercuric froth. |
The presence of manganese as an essential constituent of milk
and blood (human as well as animal) has been known for about
twenty years past, but HE. Pollacci gives some particulars about the
method of detection of this metal in the two animal fluids referred
to. The milk which contains this metal in the largest proportion
is first evaporated to the consistency of a paste; this is carbonized
by heat in a platimum crucible; the charcoal thus obtained is
1870.] Chemistry. 531
pulverized and next completely incinerated ; the ash is triturated
in an agate mortar and lixiviated with water ; the residue is treated
with very pure nitric acid, and the solution thus obtained is
evaporated to dryness and calcined in a test-tube; after cooling, a
few drops of nitric acid are added, and the contents of the tube again
boiled ; next a few grains of puce-coloured oxide of lead are added
and the liquid again boiled ; a more or less deeply purplish-coloured
liquid appears on leaving the tube at rest for a short time, which
is due to the formation of permanganic acid. No quantitative re-
searches have as yet been made by the author.
All chemists must have suffered inconvenience by finding that
their test-solution of tartaric acid had become mouldy. Many re-
medies for this decomposition have been suggested, but none appear
so simple as the one proposed by William H. Wood, of Middles-
bro’-on-Tees. This chemist has made known that if a solution of
tartaric acid in water, whether mouldy or not, be filtered and then
boiled for a short time (say ten minutes), it will not afterwards be-
come mouldy, whether corked or stoppered up im a bottle, or left
exposed to the air. This statement will, if confirmed, be important
as bearing on the so-called “spontaneous generation” controversy,
and may throw some light on it.
The production of a crystalline alloy of zinc and calcium hag
been observed in the preparation of calcium by the process of
M. Caron, in which an excess of zinc was employed. It contains
about 95 per cent. of zinc and 5 per cent. calcium, corresponding
to the formula Zn,,Ca. These crystals are small octahedrons with
square bases. They are acted upon by water with the liberation
of hydrogen.
Dr. W. Stein has devised an easily-executed process for the
detection of madder colours upon cloth or by themselves. He
boils the cloth with a concentrated solution of sulphate of alu-
mina, whereby a liquid is obtained of reddish colour, exhibiting
a golden-greenish fluorescence, due to the presence of purpurine ;
the behaviour of the colouring matters of madder towards sulphate
of alumina is so characteristic that this salt may serve as an effec-
tive test for these substances; the alizarine may be readily rendered
soluble by treating the dye material or dyed cloths with alcohol
acidified with hydrochloric acid.
As a result of a lengthy series of experiments, M. Ei. Baudri-
mont concludes that tin-foil, in consequence of its impermeability
for water, may serve with great effect to protect various substances
from the effects of the atmospheric moisture, as well as act as a
protective against the alterations fruit undergoes by evaporation of
the fluids therein contained ; tin-foil also protects against the oxi-
dizing action of the oxygen of the atmosphere, and may hence serve
532 Chronicles of Science. [ Oct.,
to keep fatty substances from becoming rancid, while it may use-
fully serve in laboratories to wrap up caustic lime, bisulphite of
soda, and similar substances, which may thus be preserved for a
great length of time without deterioration.
The cause of the precipitation of muddy matter from water by
the aid of dilute saline solutions has been investigated by Dr. Ch.
Schlasing. Water otherwise pure, but contaminated simply with
clay (as may be the case with the water of rivers after heavy rain
or fall of snow), becomes at once clarified by very minute quantities
of some salts of lime: z/5oth part of chloride of calcium for 1 part
of water effects this purpose in a moment; the nitrate, bicarbonate,
and caustic lime act in the same manner. The precipitated sub-
stance may be readily separated from the water by filtration,
whereas the filtration of the water containing the suspended matter
is very difficult, because the pores of the filters become choked. The
practical importance of this matter is very great, since it is, for
instance, a well-known fact that the water of some rivers (the
Durance being notorious in this respect) does not, in winter time,
and after heavy rainfall or snow-storms, become quite clear, even if
left at rest in large ponds for a considerable time. The same is the
case with the water of the Rhine, which in its lower course is often
turbid for weeks together, simply from the effects of very finely-
divided clay beg suspended even after the water has been at rest
in tanks. The water of the river Durance supplies Marseilles with
fresh water, the latter being brought to that city by a magnificent
series of works, among which may be mentioned the celebrated
Aqueduc de Roquefavour. Certain bitter vegetable substances have
been applied both in Egypt and in India, for the purpose of ren-
dering the waters of the Nile, Ganges, Indus, and other large rivers,
potable, many centuries before the rationale of the action of these
substances was understood.
6. ENGINEERING—CIVIL AND MECHANICAL.
The Mitrailleur.—Unfortunately the peaceful progress of Kngineer-
ing Science has, within the last few weeks, been suddenly inter-
rupted by the outbreak of hostilities on the Continent; and
prominence has consequently, for the time, been obtained by that
branch of engineering which devotes its energies to the production
of warlike engines and materials. For some years past attention
- has been given to the improvement of our artillery, and the revival
of breech-loading cannon, which for a while was received with much
favour, is already beginning to find strong opponents from the fact
that, as a rule, they possess less precision than the old muzzle-
1870. | Engineering—Civil and Mechanical. 533
loaders. Steel and chilled iron also appear likely again to give
place to bronze as a material for field guns. The arm of the day
is, however, the mitrailleur, or mitrailleuse as it 1s sometimes called,
which has already performed such bloody work in the present war.
The mitrailleur belongs to the same class of weapon as the revolver,
having, however, this advantage, that its barrels may be fired almost
simultaneously. One of the earliest of this class of weapon was
the American Gatling gun, which was first seen in Europe at the
Exhibition of 1867. This consists of six barrels mounted in two
rings of iron, fixed on a central axis; at the rear of these are two
half-cylinders of iron, bolted together, which serve to enclose and
protect the mechanism; within these a cylinder revolves, with
grooves into which cartridges fall as it is turned round, and by a
selfacting mechanism they are pushed forward into the barrels,
fired, and the empty cases subsequently extracted. A continuous
and rapid fire can thus be maintained as long as there remains
ammunition at hand to continue feeding the breech. The mitrailleur
which has recently been subjected to comparative and experimental
tests at Shoeburyness, is of Belgian origin; it was introduced into
this country by Major George Fosbery, V.C., of the Bengal Staff
Corps. It was invented in 1867 by M. Montigny, but has received
several modifications and improvements since that date. ‘This
weapon consists of thirty-seven steel barrels, of an hexagonal form
exteriorly, fitted and soldered together, and finally surrounded by a
wrought-iron tube. To the tube or barrel thus constituted a breech
attachment is screwed, and the two together, with the movable
breech-block and its lever, form the gun. In outward appearance
the gun looks like a solid steel block about four feet long, pierced
with thirty-seven holes. A cartridge holder, consisting of a steel
plate with holes corresponding in position with the barrels of the
gun, being filled with central-fire cartridges, is inserted in the breech-
piece and held in its place by suitable arrangements, whilst by the
movement of a handle on the right-hand side of the gun, corre-
sponding plungers are released, and striking their respective cart-
ridges fire the gun. According to the rapidity with which this handle
is moved the barrels may be fired one by one, or in a volley. The
weight of each projectile is 600 grains, and the charge 115 grains.
It would be premature at present to give any results of the experi-
ments now being carried on. It may be here stated that Major
Fosbery estimated the speed at which the mitrailleur could be fired
at ten rounds per minute, but this rate has not yet been nearly
attained in practice.
Steam and Air Engines.—Although the union of steam and
air for the purpose of effecting economy in engine working is by no
means a new invention, yet the means adopted for effecting this
object which have recently been made public, appear to be so far
534 Chronicles of Science. | Oct.,
superior to what has previously been introduced, as to warrant some
prominence being given to the subject. Some years ago a steam-
engine used in an industrial establishment at Muhlhouse in France,
was converted into an aéro-steam engine by the simple addition of
a pump to force air into the boiler ; a considerable increase of power
was stated to have been thereby secured, but its success does not
seem to have continued long, and the experiment did not then
secure much general favour. Recently, however, the subject has
been revived, and two inventors claim the support of the public on
behalf of their respective inventions. The first of these is Parker’s
steam and air engine, and the second Warsop’s aéro-steam engine ;
the general principles involved in each are the same up to a certain
point, but the methods of applying them differ considerably. In
Parker’s engine the air is drawn directly into the steam-pipe, lead-
ing from the boiler to the engine, by means of the force of the
steam passing through it; this steam-pipe is sometimes passed
through a small coke fire, in order to raise the temperature of the
united steam and air, but this is not considered in any way essential
to the utility of the apparatus. Experiments made with it are
reported to have resulted in considerable economy of fuel combined.
with increased efficiency of engine power.
Warsop’s aéro-steam engine consists in the use of an air-pump,
worked either by the steam-engine itself, or by a donkey-engine ;
this pump takes in cold air which, after beg compressed, is forced
on through an air-pipe passing through the smoke-box, or some
other part of the boiler where heat can be taken up from contact
with the waste gases. The highly-heated air passes a self-acting
clack-valve into the bottom of the boiling water, and is so distributed
by simple mechanical means, that it rises constantly through the
water. On rising above, the air is saturated by the steam, and
the two together pass on to their duty in the cylinder. From a
series of experiments carried out with this engine at Nottingham,
it appears that in the amount of useful work done for fuel expended,
the advantage rested with the combined steam and air system, as
compared with when steam only was employed.
Thames Embankment.—Upwards of eight years have now
elapsed since the reclamation of the foreshore of the Thames between
Westminster and Blackfriars Bridges was undertaken by the Metro-
poltan Board of Works. This magnificent boulevard was opened
on 15th of July last. It consists of a roadway 100 feet in width
throughout, haying on the river-side a foot pavement 20 feet wide,
and on the opposite side one of 16 feet; the former is edged by a
row of trees, planted at intervals of 20 feet. The total amount of
land reclaimed is 372 acres, of which the carriage-road and footways
occupy 19; 8 acres will be converted into ornamental gardens for
the public use, and the remaining 103 acres pass over to the original
1870. | Engineering —Civil and Mechanical. 535
proprietors of the foreshore. From the official description of the
Victoria Embankment, it appears that the works and material em-
ployed comprise 144,000 cubic yards of excavation, 1,000,000 cubic
yards of earth fillmg, 140,000 cubic yards of concrete, 80,000
cubic yards of brickwork, and 650,000 cubic feet of granite. The
total cost of the works has been 1,260,000/., and the amount paid
for compensation 450,000. Beneath the roadway lies hidden a
portion of the London main sewage system, above which is a sub-
way, behind the embankment wall; on the opposite side, the works
of the Metropolitan District Railway have been carried on con-
temporaneously with the Embankment, and there are four stations,
namely, at Westminster, Charing Cross, the Temple, and Blackfriars,
accessible direct from the roadway. Communications will no doubt
shortly be completed between the Embankment and the several
roads leading southwards from the Strand, as without such connec-
tions this handsome new boulevard would be deprived of half its value
as a means of communication ; according to an existing Act of Par-
lament, however, the right to make such connections is prohibited.
Chatham Dockyard Hatension.—For some time past extensive
works have been in progress for the extension of Chatham Dock-
yard. They are being executed upon 380 acres of land, and com-
prise, amongst other works, the reclamation of a marshy tongue of
land known as St. Mary’s Island, which was formerly submerged at
high water; in addition to which the scheme includes the construc-
tion of a series of three extensive docks along the line formerly
occupied by St. Mary’s Creek, and the erection of workshops. The
reclamation of St. Mary’s Island has necessitated the erection of a
considerable portion of embankment and river-wall, the latter con-
sisting of a brickwork face with concrete backing; the island was
then raised, by means of spoil tipped upon it, to a level well above
high-water mark. ‘The first basin, next Chatham Reach, has an
area of 22 acres; it will be used for repairs, and is furnished on its
south side with four large graving docks, the first stone of which
was laid on 21st April, 1868. The middle, or factory basin, 20
acres in extent, will be provided with factory buildings on the
southern side, including fitting and erecting shops, boiler shops,
smithy, foundry, stores, &c.; whilst on the northern side will be
the camber for a floating dock, a docking platform, and ten slips
for laying up frigates, with the necessary worksheds. The third,
or fitting-out basin, into which vessels entering for repairs will pass
to be dismantled prior to going into the other basin, or, if leaving,
they will be rigged and receive their supplies and stores, is 33 acres
in area. The repairing basin, with its graving docks, and the com-
munication with the factory basin, are expected to be opened in
April next. The factory basin will probably be opened by the end of
1871, and the works of the other basin are also in a forward state.
536 _ Chronicles of Science. [ Oct.,
MEETINGS OF SOCIETIES.
Institution of Mechanical Engineers.—The meeting of this
Society was held at Nottingham on the 3rd August last. Amongst
the papers read were the following :—“ On Self-acting Machinery
for Knitting Hosiery by Power,” by Mr. Arthur Paget, of Long-
borough ; “ On the mode of working Coal in the Midland Counties,”
by Mr. George Fowler, Manager of the Hucknall Colliery ; “ Con-
clusions derived from the Experience of Recent Boiler Explosions,”
by Mr. E. B. Marten, Chief Engineer of the Midland Boiler Assu-
rance Company; and “On a Self-acting Safety and Fire-extin-
guishing Valve for Steam-Boilers,” by Mr. G. D. Hughes. Space
will not admit of our giving a reasonable abstract of all the above
papers; we shall therefore confine ourselves to a few remarks on
the first and last two mentioned subjects. Mr. Fowler's lectures
are reviewed elsewhere.
Self-acting Machinery for Knitting Hosiery by Power.—The
date at which appliances for knitting have been brought within the
limits of machinery is very recent. It is one of the greatest pecu-
liarities of the hosiery manufacture that it shapes wearing apparel
without the intervention of the tailor or of the milliner ; thus there
exists a necessity that the machines employed should be easily
adapted to make articles of very great variety of shape, thickness,
and degrees of elasticity. Mr. Paget gave a description of a self-
acting power-frame of his own invention, which, on account of its
necessarily great complication of parts, it would be impossible to
describe without illustrations. A skilful framework knitter with
his hand-frame would, it was stated, knit about 5400 stitches per
minute ; whereas a girl could, on the same work, attend to three of
Mr. Paget’s self-acting machines, making in the aggregate 40,500
stitches per minute.
Boiler Explosions.—Mr. Marten remarked that from the result
of the experience of the last four years, he was enabled to confirm
the opinion he previously held, that all boilers, however good in
original construction, are liable, in the course of time, to get into
bad order and explode. The causes of explosions appear to be
three, viz.—1l. Faults in construction or repair; 2. Faults in work-
ing, which creep on insidiously and unnoticed ; and 3. Faults which
might be seen and guarded against by careful attendants. Nearly
all the faults would be detected by periodical examination, which is
indeed the only true safeguard against explosions. Hach cubic foot
of water has the explosive effect of one pound of gunpowder, and
the explosion of a boiler assimilates more nearly to that of gun-
powder than of any other explosive agent. Mr. Marten enters into
some detail regarding the various explosions that have come under
1870.] Geology and Palxontology. 537
his notice, and sums up with some very excellent rules for the avoid-
ance of such disasters.
Safety-Valve for Steam-Boilers——This apparatus is intended to
serve the double functions of fusible plugs and low-water alarums.
An internally loaded valve of spherical form is placed in a steam-
chamber, and a pair of steam-pipes connect this chamber with the
furnace crown of the boiler. The safety-valve is dead weighted, and
should the pressure of steam lift it up, it escapes into the chamber
and down the pipes into the furnace. Any over-pressure is thus
dealt with, and the motion of a float is made to act in a similar
way on the same safety-valve. Another independent safety-valve
is adjusted to blow off at a pressure somewhat lower than that at
which the dead weight is adjusted.
Inverpool Polytechnic Society.—A very interesting paper was
recently read before this Society by Mr. T. B. Thorburn, C.E.,
Surveyor to the Birkenhead Commissioners, “On the method
adopted in Birkenhead for Ventilating Sewers, and carrying away
the Gaseous Emanations generated therein.” This paper, which it
would be impossible to follow im detail, contains an account of the
extent of the Birkenhead sewers, and not only states the different
ventilators employed, but gives also the cost of constructing them
according to the several arrangements adopted.
7. GEOLOGY AND PALAZONTOLOGY.
(Including the Proceedings of the Geological Society and Notices
of Recent Geological Works.)
Professor John Phillips, M.A., D.C.L., LL.D., F.RS. &c.—Few
men have by their own labours contributed a larger share to the
advancement of scientific knowledge than Professor Phillips, and
we are glad to obtain a sketch of his career,* which is probably as
full of noble achievements as that of any scientific man we have
ever known. Brought very young (by the death of his father)
under the care of his uncle, William Smith, originally known as
“Strata Smith,” and afterwards called “the father of English
Geology,” he was early led to take delight in the identification of
strata by their fossil contents, and accompanied his uncle through
the greater part of England during his geological investigations,
which resulted in the first geological map of England and Wales.
Few men of science have had a more distinguished career. Ap-
pointed Keeper of the Yorkshire Philosophical Society’s Museum
in 1825, that Society grew and flourished under his care, and led in
* «Geol. Mag.,’ vol. vii., 1870, p. 301.
538 Chronicles of Science. ‘[Oct.,
1831 to the establishment of the British Association, of which he
became the Assistant General Secretary in 1832, and continued to
act in that capacity until 1863. In 1834 he became Professor of
King’s College and a Fellow of the Royal Society. In 1840 he re-
signed York Museum, and entered upon the duties of the Geological
Survey of England and Wales, to which he contributed Memoirs
on ithe Palaeozoic Fossils of Cornwall, Devon, and Somerset, and
afterwards on the Malvern Hills, &e. In 1844 he became Professor
of Geology in the University of Dublin. In 1849 he was appointed
one of Her Majesty's Commissioners to inquire into and report upon
the system of ventilation employed in mines. In 1853 he com-
menced the duties of the Chair of Geology at Oxford, which he has
continued to hold ever since the death of Dr. Buckland. In 1859
he was elected President of the Geological Society of London; in
1865, President of the British Association. His various geological
works are above seventy in number, and his astronomical and other
papers are also very numerous. Besides the York Museum which
enjoyed the advantages of Professor Phillips’s attention, the present
Oxford Museum may be said to have been created by him, and is
a model for any city in the world to copy.
Lecture on Voleanoes.—Mr. David Forbes, F.R.8., recently *
delivered an interesting lecture at St. George’s Hall on Volcanoes.
Speaking of the relative energy displayed by volcanic forces in the
older geological periods, Mr. Forbes said, “We must bear in mind
that we still have voleanoes whose craters, several miles in diameter,
send forth at times streams of molten stone forty miles and more in
length, or showers of ashes which bury the surface of the ground
to a depth of 400 feet below them, and, furthermore, see volcanic
mountains and islands literally rising up before our eyes to an
elevation of even thousands of feet, in what, geologically speaking,
is but a second of time, it does not to me seem at all necessary to
assume that such internal or cataclysmic forces were so much more
energetic in any other period than at present.”
The author believes that sufficient importance has not been
given to the effects produced by the cataclysmic action of volcanoes.
He points out that all the chief features of the earth’s surface are
due to the elevatory forces within, and that volcanoes not only form
the most lofty mountains in the world, but that the backbone of
most of the others is composed of eruptive rocks. Jt must therefore
be admitted that the changes effected in the physical geography of
the world have resulted from a combination of two great but most
opposite agencies, the internal and external, igneous and aqueous,
cataclysmic and uniformitarian; and that all the phenomena of
nature result from a combination of one or more forces, the same
phenomena, at times, being the result of totally different agencies.
* June 19, 1870.
1870. | Geology and Palxontology. 539
Mr. Hopkins’ Method of Determining the Thickness of the
Earth's Crust—Having been some time since challenged by M.
Delaunay,* a distinguished French astronomer and mathematician,
the late Mr. Hopkins’ friend, Archdeacon Pratt, F.R.S.,f writes in
his defence and shows what he conceives to be a flaw in M. Delau-
nay's objections ; namely, that the earth is not a simple shell with
a fluid interior always revolving in one plane (in which case he
admits there would be no possible objection to M. Delaunay’s argu-
ments in favour of a comparatively thin rigid crust and a fluid
interior), but that it is ever being disturbed by the forces of pre-
cession and nutation; and before the rigid crust and the fluid
interior could arrive at a state of equilibrium in one position, the
axis would begin to assume a new position, and the fluid interior
would again be unconformable in its motion to the external shell ;
and the earth’s motion would again be retarded in a small degree,
sufficient to interfere with the axial variations to which the earth is
ever subject by the laws of precession and nutation. As science
advances it is absolutely imperative that in all these questions our
conclusions should be in accord with the laws of chemistry and the
known terrestrial conditions, as well as the laws of dynamics.
A New Fossil Snake in Grreece.—A new fossil Python has been
lately described by Dr. Ferd. Roemer} from the Island of Eubea.
This is the second fossil ophidian found in Greece, and adds greatly
to the interest of the Miocene fauna of this old continent, already
rendered so important by the discoveries at Pikermi of such a
remarkable series of types of African Mammalia, together with the
Hipparion by M. Gaudry.
A New Labyrinthodont Amphibian from the Coal-shale near
Neweastle-upon-Tyne.—Mr. Thomas Atthey, well known to geo-
logists as one of the most indefatigable investigators of the fossil-
remains of the Newcastle Coal-shales, has again been successful in
bringing to light the skull of a new and remarkable Labyrinthodont
reptile, which the authors of the paper,§ Messrs. Atthey and —
Hancock, have named Batrachiderpeton lineatum. The lower jaw
was discovered three or four years since, but the cranium has only
now been obtained.
It is impossible to contemplate the structure of the roof of the
mouth of this curious Labyrinthodont, without being reminded
of the arrangement of the parts in that of Siren, Proteus, and
Azolotl. The well-armed vomer in particular is very striking.
The extensive development of this vomerine armature and the
deficiency of bony maxille, would seem to ally Batrachiderpeton
i ‘Geol. Mag.,’ vol. v., p. 507. + Ibid., vol. vii., p. 421.
t ‘ Abdruck a. d. Zeitschr. d. Deutschen Geologischen Gesellschaft,’ Jahre,
1870.
— ‘Ann. and Mag. Nat. Hist.,’ Series 4, vol. vi., No. 31, p. 56, Pl. I, July,
VoL. VI. 20
540 Chronicles of Science. [ Oct.,
to Siren and Proteus; while the relationship of the vomers to the
pterygoids, and the form of the latter, are very similar to what
obtains in Azolotl ; and the alliance with this last-named interesting
form would be rendered still stronger, if it should turn out that our
new genus has really bony maxille, particularly as the premaxille
are armed with teeth. In Siren and Proteus the premaxillaries
are quite minute and are devoid of teeth. This is not the only
instance in which a Labyrinthodont has been found to exhibit an
approximation to the Siren-type of structure. Pteroplax is so
related, although its approach is by a different line from that of
Batrachider peton.
Petrified Forest near Caivo.—The fossil-wood which covers the
desert to the east of Cairo has long filled the passing traveller on
this great eastern high road with surprise. The immense quantity
of what seems to be decaying wood in a region described as a
“dreary arid expanse, treeless and almost shrubless, rugged with
dark-coloured knolls, and intersected by a few dry rain-channels,”
excites, by the remarkable contrast of the present with what is
apparently the not far-distant past, the wonder of the most careless
observer. They have, of course, been referred to by travellers in
many published books. Burkhardt thought they were petrified
date-trees, Holroyd referred them to the Doom-palm, Murray's
‘Handbook’ also speaks of them as palms. Gardimer Wilkinson
refers to branched and thorn-bearing trees as well as palms, also to
some jointed stems resembling bamboos. A careful examination by
the late Prof. Unger, however, failed to elicit more than a single
species, after a most searching examination of a very large series
of specimens, and after a personal visit to the spot.
This form, which he named Nicolia Egyptiaca, has just been
supplemented by a second species brought home by Prof. Owen
during his recent visit to Egypt with the Prince and Princess of
Wales. Mr. Carruthers has figured and described it as Nicola
Owenti,* after its discoverer.
Ttalian Tertiary Brachiopoda,—Mr. Thomas Davidson, F.B.S.,
our great authority upon “ Lamp-shells,” has taken up his pen and
crayons to illustrate the Tertiary Brachiopoda of Italy, which he is
carrying out most completely in the ‘Geological Magazine.” In
his introduction he refers to the much-discussed question of deve-
lopment of species. ‘“ We are,” he says, “far from having disco-
vered the laws which regulate the gradual succession of life; and
we are, I fear, much too apt to guess at the origin of species, and
to interpret those unknown laws from a small number of incomplete
observations. The assiduous researches which, for many years, I
have made among the living and fossil species of Brachiopoda have,
to a certain extent, imbued my mind with the idea that an indivi-
* See ‘Geol. Mag., vol. vii., p. 306, 1870.
1870. ] Geology and Palxontology. 541
dual species may have been gradually very much modified in time,
so as to suit the conditions under which it had to exist; but at the
same time everyone who has studied with any degree of care any
class composing the animal kingdom, must frankly admit that there
are so many inexplicable sudden appearances of entirely distinct
forms, with no apparent links connecting them with those that
were antecedent or even contemporaneous, that it is impossible to
arrive at any definite conclusions as to what extent species are de-
rived from their predecessors.”
New British Brachiopod.—Mr. E. Ray Lankester describes a
new species of Terebratula from the (Portlandian ?) “ Drift” of East
Anglia, which he has named T. rea; it is a remarkably large form.
Cephalaspis Dawsoni, sp. nov.—The same gentleman describes
a nearly perfect Cephalaspidean Fish from the Silurio-Devonian
beds on the north side of Gaspé Bay, Canada, associated with
plant-remains. It is named after Principal Dawson, of Montreal.
The Structure of the Crinoidea, Cystidea, and Blastoidea.—
We have lately received considerable additional information upon
this subject from the pen of Mr. E. Billings, the able Palzontolo-
gist to the Geological Survey of Canada.* In the first part of his *
paper Mr. Billings considers the position of the mouth in relation
to the ambulacral system.
Earlier paleontologists described the large lateral aperture in
the Cystidea as the mouth. Von Buch, Forbes, Hall, and Billings
himself, in his first paper, adopted the view that this was not the
mouth, but an ovarian aperture, and that the smaller orifice, usually
situated in the apex, from which the ambulacral grooves radiate,
was the true oral orifice. Subsequently (nm 1858) Mr. Billings
re-investigated the subject, and came to the conclusion that the
lateral aperture was really the mouth, or serving as both oral and
anal aperture in those species not possessing distinct orifices. The
small apical orifice was determined to be an ambulacral aperture.
To this view Prof. Wyville Thomson demurs, on the ground
of the want of analogy in the rest of the class. Mr. Billings re-
plies that in this class the position of the various organs in relation
to each other, and also to the general mass of the body, is subject
to very great fluctuations. Thus the mouth and vent are separated
in some of the groups, but united in others; while either or both
may open out to the surface directly upward or downward, or at
any lateral point. The ovaries may be either dorsal or ventral,
internal or external, and associated with either the mouth or the
anus, or with neither. ‘The ambulacral skeleton may be imbedded
in and form a portion of the general covering of the body, or lie
upon the surface, or be borne upon free-moving arms. Although
these characters are constant, or nearly so, in the same family, in
* See Silliman’s ‘ American Journal of Science.’
202
542 Chronicles of Science. | Oct.,
different orders, or remotely allied families, they are extremely
variable.
The author proceeds to cite a number of instances in support of
his conclusions in which the mouth was altogether disconnected
from the radial system, and he figures Batocrinus acosidactylus,
Amphoracrinus, sp. Caryocrinus ornatus, &e.
Mr. Billings next discusses the functions of the pectinated
rhombs and calycine pores of the Cystidea. Upon this subject a
very able and exhaustive paper was written by Mr. J. Rofe,* to
-which Mr. Billings refers, and accepts the decision of Dr. Dana,
Mr. Rofe, &., and concludes them to be respiratory organs. The
author proceeds to describe these organs in Codaster, Pentremites,
&c., and then endeavours to show the homologies which exist
between the respiratory organs of these paleozoic forms and recent
Echinoderms, and lastly, the nature of the “convoluted plate” of
the Crinoidea. This plate, like the pectinated rhombs, seems to
have been connected with the respiratory system. There can be
no doubt that the true explanation of why these respiratory organs
occupy so large a proportion of the body of the animal is to be
found in the fact that the food was obtained by the motion of the
vibratile cilia of the arms, which thus fulfilled, as in so many other
invertebrates, the double function of bringing fresh streams of the
circumambient respiratory medium into intimate contact with the
fluid within the general cavity of the body of the animal; and at
the same time of conveying minute animalcule and other organic
particles to the mouth in order to serve as food.
GEOLOGICAL Society oF Lonpon.
The present number of the ‘Proceedings of the Geological
Society’ contains a rich store of paleontological information, both
British and foreign. We have illustrations of Mammalia, Reptilia,
Mollusca, Corals, and Plants; and those who delight in long lists
of fossils can also fully satisfy their appetites. Nor need the field-
geologist grumble, for he also may regale himself on the Neocomian,
the Oolite, or the Lias to his heart’s content. A valuable contribu-
tion to our knowledge of Fossil Corals is from Dr. P. Martin
Duncan, “On the Madreporaria of the Australian Tertiary Deposits.”
The series described is from the province of Victoria, the Geolo-
gical Survey of which was (until lately abolished) so ably con-
ducted by Mr. Selwyn (now. Director of the Geological Survey of
Canada). The species described do not belong to the reef-building
forms, but to such as*now occupy the sea-bottom from low spring-
tide mark to the depth where Polyzoa abound. It is interesting to
* ‘Geol, Mag.,’ 1865, vol. ii., p. 245.
1870. ] Geology and Paleontology. 543
note that twenty genera are now found in the Australian seas, only
three of which, however,, have species in the Tertiaries, viz. the
eosmopolite T'rochocyathus, Flabellum, and Amphihelia, but the
fossil species are quite distinct from those now living. If we may
judge by the wide geographical distribution of some of these species
we may with safety infer that their range in time was also very
much greater than has hitherto been assumed. Allied forms are
found living in Japan and China, the Red Sea, the West Indies,
and Europe in Miocene times.
The descriptions of the new species are illustrated by thirty-two
figures, occupying three double-octavo plates. ,
There is reason to believe that the Wealden vertebra, now
described and figured by Mr. J. W. Hulke, belongs to the same
large animal—distinct from any of the known Dinosawrs—of which
there is a single vertebra preserved in the British Museum, and
named by the late Dr. Mantell Streptospondylus. The texture of
the bone is like the coarse diploé of the elephant’s skull, and has led
to the belief, by Mr. H. G. Seeley, that it represents a gigantic
Pterosaurian; but Mr. Hulke reminds us that an extremely light
skeleton does not necessarily prove endowment with flight, and also
that all the known flying-reptiles have proccelian vertebrae, whilst
the vertebra of Streptospondylus is amphicelian in type. The
supply of new and wonderful reptilian remains furnished by the
Wealden of the Isle of Wight seems almost inexhaustible, but it is
much to be regretted that by far the greater part of these have,
of late years, fallen into the hands of a local collector in the island,
unable to describe them himself and unwilling to allow them to be
worked out and described by anyone else.
Our knowledge of Fossil Botany has been increased by an inte- —
resting description of a new fossil fern-stem, so like the recent
Osmunda, as to justify its describer, Mr. Carruthers, in placing it
in the Osmundaceze. The specimen was silicified so effectually that
even the starch-grains in its cells, and the mycelium of a fungus |
traversing some of them, were perfectly represented. The fossil
(which was probably derived from the upper part of the Thanet
Sands) has been named Osmundites Dowkeri, after Mr. George
Dowker, its discoverer.
Professor Owen has ventured upon the difficult task of deter-
mining the remains of a number of fossil Mammalia upon the
evidence furnished by a series of detached teeth brought home by
Mr. Robert Swinhoe, H.B.M. Consul at Formosa, and obtained by
him from the apothecaries’ shops at Shanghai and at Chung-king-foo
(Eastern Szechuen) on the Yangtse-kiang River. They included
two species of Stegodon, a new Hyzxna, a new Tapir, a new Lhino-
ceros, and a species of Kaup’s genus Chalicotherium. From a
general agreement in colour, chemical condition, &c., Professor Owen
544 Chronicles of Science. | Oct.,
concluded they all belonged to one and the same period, either to
Upper Pliocene or Post Pliocene. Strong objections were raised as
to the soundness of the species by Professor Busk, especially to
Stegodon, Hyzna, and Rhinoceros; it was also objected by Pro-
fessor Boyd Dawkins, that there was no proof of their contempo-
raneity. These teeth, which are extremely various, are sold by the
Chinese apothecaries as a very valuable medicine when pounded to
a powder. They are described by Mr. Daniel Hanbury in his
account of the Chinese Materia Medica.
Mr. Hanbury mentions that Mr. Waterhouse, of the British
Museum, has determined the following species:—Molars of the
lower jaw of Rhinoceros tichorhinus, tooth of Mastodon ; of Elephas
insigmis (?); molars of Hquus; teeth of Mippothertum (two
species ?); teeth of sheep, stag, bear.*
They are said to come from the provinces of Shen-si and Shan-si,
but the demand for them is so great that they are believed to be
largely imported from the East Indies, and notably from Borneo.
Mr. Sharp’s paper, ‘‘ On the Oolites of Northampton,’ is prin-
cipally of importance because of the recent discovery in this district
of vast bands of ironstone, the economic quarrying of which has
yielded a characteristic fauna with a decidedly Inferior Oolite
facies, in beds which had been mapped as Great Oolite (“ North-
ampton Sands”) by the Geological Survey, and in which—until
quite recently—not a trace of a fossil remain was known to exist.
Mr. Sharp has carefully described the district illustrating his
observations by numerous sections and a good sketch-map of its
geology, together with lists and localities of the fossils he has been
so successful in obtaming. As a rider to the paper, Dr. Wright
describes a new and very finely-preserved star-fish (Stellaster
Sharpiz), from the ironstone of the Inferior Oolite, Northampton.
Mr. J. W. Judd, of the Geological Survey of England and
Wales, has devoted much time and attention to the Neocomian
strata of Lincolnshire and Yorkshire and their correlation with
those of north-western Germany and elsewhere. He now gives us
the result of his studies, carefully prepared and illustrated with
maps, sections, and tables. ‘The Neocomian beds of Yorkshire, &c.,
appear to be the extreme westerly development of a great mass of
strata of the same age stretching over a wide area in Northern
Europe. It is also seen that in Yorkshire and in Brunswick the
Neocomian series is complete, but in the intermediate districts its
lowest member is absent, being replaced by the fresh-water deposits
of the German Wealden.
Mr. Ralph Tate supplies two papers, on the Middle Lias in
Ireland, and the Lower and Middle Lias in Gloucestershire. No
higher member of the Jurassic series is known in Ireland than the
* «Journal of the Pharmaceutical Society,’ 1860.
1870.] ~ Meteorology. 545
Lower Lias. The Middle Lias occurs as drift on cultivated fields,
&c. Mr. Tate suggests that this drift may have been transported
from the Hebrides by glacial action. In the case of Gloucestershire,
Mr. Tate endeavoured to apply the numerical test as to the distri-
bution of organic remains in order to show that the zone of Ammo-
nites Jamesoni belongs to the Middle Lias, and A. raricostatus
to the Lower Lias. For the present it is exceedingly difficult to
follow these minute divisions until more of their contained fossils
have been identified and figured.
In addition to these, we have abstract notices of the Crag of
Norfolk and Associated Beds, by J. Prestwich, Esq., F.R.S. Cap-
tain 8. Hyde on Deep-mining in §.W. Ireland. Dr. E. Bunzel on
a Reptilian Skull from Griinbach. Mr. R. J. Lechmere Guppy on
Trinidad Fossils. M. Coumbary on the Fall of an Aerolite in
Fezzan. Dr. A. A. Caruana on a further discovery of Fossil
Elephants in Malta. The Journal is a very stout one, numbering
468 pp. and having fourteen lithographic plates.
8. METEOROLOGY.
THE Meteorological Office has issued Part I. of its new publica-
tion, ‘The Quarterly Weather Report,’ for the first three months
of 1869. The chief features of novelty presented by this Report
are the fac-simile representations of the curves of the self-recording
instruments. It should be stated that the preparation of plates
such as those referred to has been rendered possible by an invention
of Mr. Francis Galton’s. This isa pantagraph which is capable of
effecting reductions simultaneously in different proportions along
two rectangular co-ordinates. The proportions selected for the
plates have been 4 for the horizontal or time scale, and } for
the vertical scale. By this means all the information for five days
from the seven observatories is condensed into the space of two 4to
plates, one for the barograms and wet and dry bulb thermograms, —
the other for the wind and rain. Scales on both the British and
metrical systems are given at each side, so that the readings of the
barometers and thermometers may be determined for any epoch.
For the wind the scales are in statute and geographical miles.
The letter-press consists of (1) an introduction containing some
general remarks, especially on the difficulty of obtaining trustworthy
records of wind at land stations ; (2) the Report itself, which is
a chronicle of the weather for the three months, derived from all
sources which were available to the office, with tabular statistics of
storms ; (3) the tables for the year 1869, giving the monthly and
the five-day means of various elements, derived from the hourly
tabulated readings of the instruments.
546 Chronieles of Science. | Oct.,
In the appendix Mr. Scott has given a notice of some late
easterly storms, which is an attempt to classify them and possibly
discover traces of their origin. The number of storms investigated
is only twenty-five, evidently far too few to allow of important
deductions being drawn, but some very interesting facts come out
in the discussion, and we hope that the paper may be followed by
others of a similar statistical character.
The price of the Report is very moderate, being only 5s. a —
number. It is published by Stanford.
The Third Annual Report of the Committee has also lately
appeared. It shows steady progress in the three departments of
the operations of the office—Ocean Meteorology, Storm Warnings,
and Land Meteorology of these islands. With regard to the last
of these we regret to see that Dr. Stewart has found himself
obliged to resign his position as Secretary to the Committee. His
services in organizing the system of self-recording observation has
been of extreme value to the cause of meteorology in England.
In Part II. of the Report we have the description of some new
instruments— Mr. Galton’s Pantagraph, above noticed; Beckley’s
Self-registering Rain-gauge, which is to be introduced at all the
observatories ; and Dr. Miller’s Deep-sea Thermometer, to which we
have alluded in a previous number.
The last number of the ‘ Journal of the Scottish Meteorological
Society ’ is mainly occupied with a paper by Mr. D. Milne Home,
“ Suggestions for Increasing the Supply of Spring Water at Malta,
&c.” In our notice of the last paper by the same author, in
No. XXYV. of this Journal, we said, “ The paper consists of a series
of extracts from the reports of various observers,” and the same
words will apply exactly to that now under consideration. Mr.
Home in his remarks suggests the old and well-known remedy for
local drought, vzz. extensive plantations. It seems rather a pity
that when the Society, as we learn from another part of the journal,
is endeavouring to obtain funds from the Government, any portion
of its means should be expended in publishing papers on foreign, or
at least colonial, meteorology.
In our last number we noticed Dr. R. Angus Smith’s paper
“On the Detection and Estimation of the Impurities of Air, by
the Analysis of Rain Water, and by Washing Bottles of Air.” His
Sixth Report, as Alkali Inspector under the Board of Trade, has
just appeared, and contains much valuable information on the
subject, which is, however, too foreign to meteorology to require
further notice here.
Mr. Blanford, Meteorological Reporter to the Government of
Bengal, has published a paper in the ‘Journal of the Asiatic
Society,’ “ On the Relations of Irregularities of Barometrical Pres-
sure to the Monsoon Rainfall of 1868-9.” He finds that in both
1870. | Meteorology. 547
years an area of relative depression existed in Lower Bengal which
took its rise at the beginning of the south-west monsoon in April.
“ Tts position was different in the two years, being in the former in
the north-west corner of the Bay of Bengal, in the latter in the
hilly country to the west of the Delta. It influenced the vapour-
bearing winds from the south by deflecting them towards it; and
necessarily, by determining an ascending current, it produced an
excessive rainfall to the north of its position, the maximum fall
being at from 50 to 150 miles distance from the place where
the barometer was lowest. Finally, it impeded the passage of the
vapour-bearing winds to the north-west provinces, and thus deprived
that region of a great part of its usual annual supply.”
Considering the extreme importance to India of the periodical rain-
fall, papers like this of Mr. Blanford’s are of great value and interest.
The Third Annual Report of Mr. Blanford’s office has also
appeared ; it shows a steady progress in the way of systematic
organization of the various observing stations in Bengal. We may
now hope that the example shown by this Presidency will soon be
followed in the other districts of Hindostan.
M. Harold Tarry has published notices of the fall of red rain
in Italy on various occasions. The papers first appeared in the
‘ Bulletin of the Association Scientifique,’ and then in the ‘ Comptes
Rendus.’ His object is to prove that the occurrence is due to
previous dust-storms in the desert of Sahara, and not to the advent
of cosmical dust from the regions of space, as Arago and Quetelet
formerly maintained. He has examined three recent instances of
the phenomenon, viz. March 10, 1869, March 24, 1869, Feb-
ruary 14, 1870. He says that the sequence of circumstances is
the same in all cases. A barometrical depression and a storm
advances from north to south across western Europe to Africa,
where the sand of the Sahara is set in motion in clouds of dust.
A few days subsequently a reverse action takes place: a storm
advances from Africa to the south of Europe, carrying the dust
with it, which comes to the earth with the rain.
The paper is very interesting, but we must say that M. Tarry
has not quite proved his case as yet.
The later numbers of the ‘ Journal of the Austrian Meteoro-
logical Society ’ do not contain much that is suitable for extraction
for this Chronicle. The editors have adopted the practice of giving
abstracts of meteorological data from isolated stations, and these
cannot be rendered intelligible without the insertion of a large
amount of tabular matter. The districts for which such informa-
tion is afforded are very various. M. Rayet’s paper “On the
Meteorology of the Isthmus of Suez” is reproduced, in abstract,
from the ‘ Atlas Météorologique’ for 1868. Then follow several
papers by M. Wojeikoff “On the Meteorology of Russia,” which he
548 Chromeles of Science. [Oct.,
has ‘compiled from various disconnected registers of local observa-
tions for short periods lying at the observatory of St. Petersburgh.
The stations are very widely distributed over Europe and Asia.
The Report of the Central Physical Observatory, by Prof. H.
Wild, the Director, consists mainly of an account of the condition of
the observatory, anda catalogue and description of instruments. As
no report had been published since 1864 it was necessary to take
stock, and to publish the account for the information of the Russian
public. The only matter of general interest is that Prof. Wild
appears to have finally decided not to employ photographic self-
recording instruments at the normal stations, owing to their serious
initial cost and the expense and trouble of working them.
Dr. Prestel, of Emden, has published a pamphlet entitled ‘ Der
Sturmwarner, in which he commences by discussing the facts of
storms, and the possibility of giving telegraphic intelligence of their
approach. On reading this part of the paper we are disappoimted
to find that Dr. Prestel has not made himself acquainted with the
latest facts of the subject. The principle of his storm-warner is
similar to that of Piddington’s horn circles.
He makes four assumptions.
I, That the barometrical reading at the centre of the storm is
28:78 ins. on the mean.
II. That the wind blows in circles round it.
III. That the diameter of the storm is nearly constant.
IV. That the difference between barometrical readings for a given
distance in all parts of the storm, or the “ gradient,” is constant.
If these four postulates be oranted, the use ‘of the transparent
diagram is perfectly simple and intelligible, but as there is no foun-
dation for any one of them, the whole reasoning falls to the ground.
Another book the utility of which we fail to discover, although
it has been favourably noticed in some newspapers, 1s ‘ The Wind in
his Circuits,’ by Lieut. R. H. Armit, R.N.
The author proposes to subvert Maury’ s theory of the wind by
facts drawn from his own experience. A few examples will suffice
to show the character of his arguments. The italics are his :-—
“The trade winds are very damp moist winds, heavily charged
with vapour: every cubic inch of them containin g millions upon
millions of minute globules of water. On entering the equatorial
calm belt, the process these globules undergo is simply that of being
turned into steam.”*
“The easterly wind is formed of compressed vappowr or steam.’ a)
“Lightning and thunder are caused by the ‘ Arctic current’
descending to fill any vacuum that may suddenly be formed in the
warm currents belowit...... The ‘ Arctic current’ in rushing
down would grate against the sides of the warm air of the under
* P24, + P.57.
1870. | Meteorology. 549
currents, causing ‘ friction’ and ‘lightning, the sudden shock of the
impenetrable masses the ‘thunder.’ ”’*
“ Regarding our atmosphere as a homogeneous metallic body.” t
Our readers will be ready to admit that Capt. Maury has not
much to fear from opponents like Mr. Armit.
We are glad, however, to be able to record a contribution to
theoretical meteorology of a character very different to the foregoing.
This is ‘ Physical Geography in its relation to the Prevailing Winds
and Currents,’ by Mr. J. Knox Laughton. We regret that we can
only very briefly allude to its contents. Mr. Laughton gives a
concise account of the existing winds, and then discusses the accepted
theories of the origin of the great currents of air and water which
exist on the globe. He shows that Hadley’s theory of the trade
winds, as developed by Dove, is insufficient to explain the facts
observed. ‘The air does not flow towards the region of highest
temperature for the time being. In the old continent this district
is the north of Africa and Arabia, towards which the trade wind
does not blow. Secondly, he concludes that the rotation of the
earth does not materially affect the direction of the currents of air,
because “ the friction between the air and earth is so great, that the
air almost instantaneously acquires the velocity of the points of
the earth to which it is transplanted,” and because Dove's theory
will not explain due easterly or westerly winds any more than
north-westerly or south-easterly winds in the northern hemisphere
(S.W. or N.E. in the southern). The laws of motion of flowing
water are next described, and the action of obstacles in altering
the direction of the current, and producing reverse currents or
backwaters. After giving an account of the currents of the sea,
similar to that previously given of the winds, the author concludes
“that wind, acting not only on the surface of the sea, but, by means
of intense friction, to a considerable depth, is the chief ”—he will
not say the only —“ cause of the numerous oceanic currents.”
The final theory which Mr. Laughton adopts is thus stated :—
“'The whole atmosphere, relatively to the surface of the earth,
continually moves, or tends to move from west to east; and the
prevalent local variations from that direction are either eddies, or
deflections, formed in accordance with the principles which regulate
the motion of fluids.” .
Our space will not allow of our criticizmg Mr. Laughton’s
reasoning in detail, but we cannot omit to give him credit for
having collected a most valuable series of facts from the most
authentic and most recent sources, and discussed them with thorough
conscientiousness. Although we may not agree with all his conclu-
sions, we feel that he has produced a very useful and interesting work.
+ PGs: j P11,
550 Chronicles of Science. | Oct.,
9. MINERALOGY.
WuueE the colony of Victoria has year after year been eagerly ex-
plored by many a miner in quest of its golden wealth, it is notable
that the number of mineral species hitherto brought to light has
been strangely incommensurate with the activity of these mining
operations. In spite, however, of this poverty of materials—a
poverty which is the more striking when contrasted with the pro-
digality of species distributed through the ore-deposits of many
other mining countries—some good mineralogical work has already
been done in the colony. This is due especially to the exertions of
Mr. Ulrich, one of the geologists who, under Mr. Selwyn’s guid-
ance, were carefully working out the structure of the country, until
the colonists were tempted, in an evil hour, to disband their staff
of Geological Surveyors. Mr. Ulrich’s recent observations on the
minerals of Victoria have been thrown into the form of a little
brochure,* which may be regarded as forming a sequel to an essay
on a kindred subject prepared by the author for the Intercolonial
Exhibition of 1867.
In the pamphlet now before us we find descriptions of three
species which are entirely new to mineralogical science. One of
these is a native alloy of gold and bismuth found in the Nuggetty
Reef at Maldon, and hence termed Maldonite:+ the second is a
green mnassive mineral allied to serpentine, consisting of a hydrous
silicate of alumina and sesquioxide of chromium, found in Upper
Silurian rocks on the flanks of the Mount Ida range, and named
Selwynite, in compliment to the Director of the late Geological
Survey; while the third new species is Talcosite, a mmeral which
resembles tale and occurs in seams traversing the Selwynite. In
addition to these newly-discovered species, many other Victorian
minerals described by Mr. Ulrich merit attention, either from their
crystalline forms—such as the splendid specimens of Herschelite
examined several years ago by Dr. von Lang, of which some addi-
tional forms have been lately discovered—or from their peculiar
mode of occurrence, such as the crystals of Struvite recently found
in the guano which covers the floor of the Skipton caves in Balla-
rat, and appears to have been derived in great measure from the
excrement of bats which resort to the caverns as a hiding-place
during the day. Among gem-stones, Victoria can boast of possess-
ing the diamond, ruby, sapphire, topaz, and garnet—some crystals
of the last being notable for their singularly distorted and conse-
quently deceptive appearance. The study of Australian gems is
one which the Rey. Dr. Bleasdale has made peculiarly his own.
* ‘Contributions to the Mineralogy of Victoria’ By George H. F. Ulrich,
F.G.S. Meibourne, 1870. Pp. 32.
+ ‘Quart. Journ. Science,’ October, 1869, p. 556.
1870. | Mineralogy. 551
Passing to-another of our colonies, we find materials for mine-
ralogical work afforded by the many meteorites which from time to
time have fallen in India. One of these has lately been analyzed
by Mr Waldie.* In February, 1867, a shower of about forty
stones fell near Khettree in Rajpootana. Alarmed at the shower,
and attributing it to the vengeance of an offended deity, the natives
at once collected the stones, reduced them to a fine powder, and
scattered it to the breeze. Diligent search, however, led to the
discovery of a piece which luckily had escaped destruction, and it is
this fragment which formed the subject of Mr. Waldie’s analysis.
The stone is of a light bluish-erey colour, darker in parts, and
contains disseminated metallic particles and granules of a greenish-
‘mde colour. Its general composition was found to be as fol-
OWS :—
Nickel iron Pees. a «fay wate ERPS
Troilite, and. schreibersite .. . .. ss», = <<. Sieve
Earthy matter soluble in acids Pree paar is alls)
Die moolwhie: i. 62. eae A ey Sa eb
LOL-31
For eighty years a specimen has lain in the Wirzburg collec-
tion, under the name of an arsenical ore. Prof. Sandberger’s recent
examination shows, however, that it is really a new species, which
he terms Isoclase.t The mineral—which is said to have come from
the mines of Joachimsthal, in Bohemia—crystallizes in the oblique
system, and consists of a hydrous phosphate of lime having the
following formula, and therefore analogous to the species Libe-
thenite and Tagilite, among the copper phosphates: 4 CaO. PO,
+ 5 HO.
Another new phosphate of lime is described by the same author
under the name of Collophane. This is an amorphous substance
found in cavities in the altered coralline rock of Sombrero, and has
the following composition: 3 CaO. PO; + HO.
The energetic French chemist, M. Pisani, has published an
analysis of the new Algerian mineral described by M. Flajolot as
Nadorite—a name which has reference to the Djebel Nador, in the
province of Constantine, where the mineral in question was found.
While Flajolot regarded it as a compound of the oxides of lead and
antimony, Pisani finds that it contains chlorime—a point of great
interest, since this is the first mimeral in which chlorine has been
detected in a compound containing antimony. In fact, Nadorite is
an antimonial Mendipite, or oxychloride of lead, and may be thus
formulated:{ (Sb,O;.PbO) + PbCl.
Rabdionite is Von Kobell’s name for a new mineral from the
* ‘Chemical News,’ xxi., No. 551, p. 278.
+ Leonhard and Bronn’s ‘ Jahrbuch fiir Mineralogie,’ 1870, Heft IIT., p. 306.
t ‘Comptes Rendus,’ Aug. 1, 1870, p. 319.
552 Chronicles of Science. | Oct.,
mines of Nischne Tagilsk, in the Urals.* -It occurs in small dull
black rods, and contains in a hydrated form the protoxides of copper,
manganese, and cobalt, with the peroxides of iron and manganese.
In writing the name of this species we have followed the author’s
mode of orthography, but the etymology of the word clearly de-
mands the form Lhabdionite (pa8diov, diminutive of fpaBédos, a
rod).
picts! publishes the results of his examination of the Russian
mineral Lawrowite,} which tend to show that it is really a diop-
side, coloured bright green by the presence of 4:2 per cent. of
hypovanadate of lime. Accompanying this mineral, he finds a new
species of analogous composition, but containing much more vana-
dium. ‘This species, which he proposes to name Vanadiolite, may
be regarded as formed of three molecules of augite associated with
one of hypovanadate of lime. The same author describes, under
the term Phosphorchromite, a Russian mineral containing chromate
of lead and phosphate of copper.
A new British locality is announced for the beautiful mineral
avanturine-quartz.t Mr. Traill is said to have found it in Orkney,
on the S. and §.W. shores of Inganess Bay.
According to the ‘ Brighton Herald,’ a large deposit of the sub-
sulphate of alumina, called Websterite, has been recently found in
Brighton during certain excavations for deep drainage.
Professor Streng’s recently-published ‘ Mineralogical Notices ’§
describe the prehnite of Harzburg, and certain pseudomorphs of
calcite and asbestos, after apophyllite, also from Harzburg.
The attention of the crystallographer may be directed to Dr.
Werner’s paper “On the Theory of the Hexagonal System ;” || to
Dr. Klein’s ‘ Note on some Forms of Galena ;’4] and to Herr Groth’s
‘Dissertation on the Topaz of certain Tim-ore Deposits, especially
those of Altenberg and Schlaggenwald, in Bohemia.’ **
10. MINING AND METALLURGY.
Mrninc.
In our Chronicles for July we noticed the proposed amalgamation
of the Mines Regulation Bill and the Metalliferous Mines Bill, re-
marking on the unfortunate character of this attempt to legislate by
one Act for two dangerous industries, differing in all their essential
* ¢ Journ. f. prakt. Chimie,’ 1870, p. 423. t Ibid., p. 442.
t ‘Geolog. Mag.,’ Sept., 1870, p. 444.
§ Leonhard and Bronn’s ‘ Jahrbuch,’ 1870, Heft IIL., p. 314.
|| Ibid., p. 290. q Ibid., p. 311.
** « Zeitschr. d. d. geolog. Gesell.,’ XXIL, p. 381.
Erratum in Chronicles last quarter, p. 417, line 8 from bottom: for “the
several species,” read “ the several plagioclastic species,”
1870.] Mining. 558
points (except that they are both subterranean employments) as
widely as possible from each other.
We have much pleasure in recording the fact that this amalga-
mated Bill has been withdrawn. The attention of the House of
Commons will no doubt be called early in the next session to some
system of legislation for collieries and mines. Let us hope that any
Bills which may be framed, will be submitted to some persons
familiar with the perils of mining, who may so organize the rules as
to render them effective and Waeneek
The Colliery Inspectors have recently issued their reports of the
fatal accidents and deaths in and about the coal and ironstone mines
of Great Britain during the year 1869. ‘The following is a con-
densed summary of their tabular statement of accidents in collieries:
In July we stated that tin mining in our western counties had
resumed a condition of high prosperity. This has, unfortunately,
: MISCELLANEOUS.
| EXPLOSIONS. ee. INSHARS sa a
| Underground. } On Surface.
| ae ‘Deaths, er foe a Deaths. ar eves Acci- Deaths.
od | es ) Le |
Northumberland, | |
Cumberland, and Pie) ee Gio ABN -2Btddel? B41 18 fo te ete
North Durham | |
. South Durham 1 2 30 | 31 6 6 24 Zany es 15
North and East
3.{ a i ee Oe ee
West Lancashire = Pie
4. eae Wales gs |128| 43| 45| 20| 20] 21] 32| 9 | 9
5. Yorkshire... 1 if 38 | 41 6 v4 12 15 5 5
Derbyshire, | |
Nottinghamshire
Leicestershire, ’ | 5 6 ol 5! Mi 12 19 22. + i
Warwickshire
North Staffordshire, = |
Chester, Shvopdine : a2 ae 7 | q 7 - - :
South Staffor dshire,
« Worcestershire | GA ee rt alaars |e : 2 = =
Monmouthshire,
Gloucestershire, 6 23 oO. OF ue Es; = 5 5 3
Somersetshire |
10. South Wales.. 9 70 62 63 14 15 Pil 21 9 12
11. Scotland—East . a 19 il 29 30 8 8 10 10 7 9
12. Scotland—West .. 4 | 4 28 | 28 6 6 me ee 1 if
Total in Collieries ee 48 | 257 | 451 | 466 | 123 | 1294) £59 | GO 7 85
9 Jronstone Mines; .. | .. 2h ae eee. SA EO TO 3 3
Gross Total... | 48 | 257 | 480 495 | 135 | 141 ma] 169 | 189 | 76 | 88
Total fatal accidents .. .. 908 in 1869 _ .. 928 in 1868
‘Total deaths<..! (20) se ee, st = MOBO m5,
554 Chronicles of Science. [ Oct.,
been exceedingly short lived. The influence of the Continental
war has led to a reduction of from 12/. to 15/. a ton in the price of
tin ore, and consequently the tin miner is dispirited, and tin mines
are not at all in favour with speculators.
: The following were the purchases of tin ore in each month of
1869 :-—
Tons. Tons.
JomMUety Asie. 4d, Se ed UULY i sat)» Sistvse my ec alee atacnes
Kebruarye a. 1.» b 20% AUSUS i ee Oe Ok
March he eae 976 September... .. 1, 144
ADE es a | sits alle, ORD Oetoberivin4. ¢ ss
MVE iit th wd. , dep oe ee November... ... L279
Ue sh een ee Oe | December... .. 1,112
Total for 4869). yaad. Senn! ae 25
Some interesting mining operations are now being prosecuted at
a colliery belonging to the Earl of Dudley. We copy the follow-
ing particulars from the ‘ Birmingham Gazette :’"—This section of
the Dudley estate has probably been the most prolific in the world
so far as the actual yield of coal is concerned. It has been in work
for more than a hundred years, and yet its resources hold out satis-
factory promises of reward to the persevering efforts of those en-
gaged in the present experiment. In some parts of the district on
the east side of Dudley, coal is not to be found until the mine
reaches a depth of 250 yards; in other parts, as in the celebrated
twelve-yard-thick measure at Fox-yards, near Sedgeley, the coal
crops out at the surface, and may be carted away for almost the cost
of loading. In most cases the coal lies in a pretty nearly level con-
dition, and may be worked in the ordinary way, wz. by a pit-shaft
sunk perpendicularly into the earth, from the bottom of which
“oate roads” are driven; but in some instances the coal lies in such
an oblique position that to “ win” it in that manner involves great
cost and danger. ‘To overcome the difficulties of getting the coal
where it lies in this oblique position, the experiment under notice
has been resorted to. It consists of two tunnels driven from the
surface of the earth into the mine, at an angle of about thirty
degrees ; these tunnels are lined with substantial brickwork, and the
“skips” and their contents are drawn up the inclined railway, which
is laid down for the purpose, by an ordinary stationary engine fixed
on the surface. The coal already got in this way is only a few
yards from the surface, and it is found to be of a good serviceable
quality. Similar experiments were made near Bilston twelve
months ago, and the works are now in successful operation there.
The discovery of a coal of good quality in Japan is of moment.
This Japanese coal has been discovered in the Takasima Colliery at
Nagasaki. According to the analysis of Dr. Jas. Martin, the con-
stituents of this coal are in the following proportions :—Carbon,
1870.] Mining. 555
82°07; hydrogen, 5°30; oxygen, 3°35; nitrogen, 2°72; sulphur,
1°64; ash, 4°90; loss, 0°02. The samples taken from the level
drives, showing a specific gravity of 1°231, are scarcely less satis-
factory. On first firing up, the coal is said to give out smoke rather
freely, but this soon passes off, and its deposits of soot are not more
than would accrue from good English coal. The following remarks
of Mr. Madden, chief engineer of Her Majesty’s ship ‘ Ocean,’ are
very conclusive as to its merits:—“ Keeping steam with ease at
50 Ibs. pressure. Full speed for five hours with a continuous steam
exhaust blast from four cylinders, being a very severe test of evapo-
rative qualities for bituminous coal, which involves large quantities
of smoke each firing for a short time, but if used in ordinary boilers,
without blast and slow combustion this would be considerably
reduced. I consider the two samples as tested above to be equal in
general steaming properties to English North Country; and com-
pared with Welsh, repeatedly tested under same circumstances, as
shown to be best Welsh 5 cwt. = 7 cwt. Takasima.”
We have recently visited the Hayle Foundry Wharf at Nine
Elms to see the operation of some pneumatic stamps. The import-
ance of introducing the utmost economy into the ore-dressing
arrangements of the tin mines of Cornwall renders this invention of
the highest importance. The following is a brief description of the
machine :—
In the pneumatic stamp the motion is conveyed from the crank
to cap and guide cross-head, on piston-rod, by an ordinary connect-
ing-rod. Attached to its lower end is the piston-rod, and piston
packed with double reverse cup-leather packings; the piston is
41 inches diameter, and operates freely in the upper part of a gun-
metal cylinder 34 feet in length; attached to the bottom of this
cylinder, by a socket in the usual manner, is the round stamp-head
of chilled cast-iron, 9 inches diameter. The upper end of the
cylinder is bored, to receive the piston, to a depth of 14 inches ;
the piston-rod plays air-tight through the cylinder cover, which is
screwed metal to metal on the cylinder. The working barrel of
cylinder is pierced with two sets of small holes, for the ingress and
egress of air, discharging the air behind the piston after it has been
once used as an elastic cushion. Suppose the head to be set in
motion with the crank in a horizontal position, the piston being in
the middle, vertically, of the working barrel of cylinder, and mid-
way between the two sets of air-holes referred to. As the crank
and attached piston rise, the air is compressed between the piston
and cylinder cover, and the cylinder, with stamp-head attached, is
forced upwards. When in rapid motion, the elasticity of the com-
pressed air between the piston and cover flings the cylinder, with
head, some inches above the range due to the motion of the crank ;
on the descent of the piston below the bottom set of holes in the
VOL. VII. 2P
556 Chronicles of Scrence. [ Oct.,
cylinder, the air is compressed in a similar manner, and the cylinder
is forced down by the compressed air between the piston and cylin-
der bottom, until the stamp-head strikes the ore in a coffer-trough ;
thus, whether the quantity of ore be large or small, the blow is
always effective, the only difference in the working of the machine
being a shorter or longer vertical play of the cylinder and head.
The committee appointed by the North of England Institute of
Mining Engineers to mvestigate the action of safety cages and
hooks have made their report. After a most careful investigation
of all the inventions which were brought before them, and they
were very numerous, they have arrived at the following conclusion :—
“That there are really but two different classes, namely, those which
come into operation every time the chain is slackened, and those
which do so only when the cage is actually falling or descending at
a speed almost equal to that of a falling body. Inventions of the
first class are very numerous; the second class has one sole expo-
nent, Calow, and both depend on the action of springs (which are
always subject to derangement) to initiate the grip, which intensi-
fies itself by being drawn more and more into gear by friction on
the guides. Both systems have their advantages and disadvantages ;
for even Calow’s, although it does not wear so much as the others
by being constantly in motion at the top and bottom of the pit, yet
is apt to stick in the shaft if by any cause the cage receives a
sudden jerk.”
In conclusion the committee say :—“ It must be admitted that,
with every desire to see some efficient apparatus in use at every
colliery to prevent the lamentable loss of life that occasionally occurs,
your committee have felt an instinctive distrust of the various modes
hitherto proposed for doing so, which distrust has not been alto-
gether overcome by the investigation that has been gone into. Up
to the present time there seems some element wanting to perfect these
machines (some of which are excessively ingenious) and render them
really reliable, and it 1s much to be desired that such an improvement
may be arrived at speedily. With this feeling your committee can-
not express an opinion as to the necessity for the adoption of any
of these provisions for safety, and can only lay before you the facts
they have acquired, with such deductions from statistics and obser-.
vations as have presented themselves, and which it is hoped will
materially assist in considering the merits of new inventions.”
Papers on the Theory and Practice of Coal Mining. By
George Fowler, M.E. W.M. Hutchings. London.—Mr. Fowler
has read before the Institution of Civil Engineers, and other
societies, papers “On the Relative Safety of different Modes of
Working Coal,” and on kindred subjects. These papers are now
gathered together, and, reconstructed, are presented to the public
in a very useful form. Each mode of working coal is carefully
1870. | Metallurgy. 557
described, and the author’s views are given as to the relative values
of the several systems. It is not practicable, did we even deem it
advisable, to enter into any discussion on these questions. We
must refer all of our readers who are interested in the subject of
mine ventilation to the book itself, which they will find very full
of useful information. :
METALLURGY.
It is our duty to record such of the numerous attempts as are
made from time to time to improve the make of iron and steel as
may appear to possess merit. It is not a new idea to use the alka-
line metals for removing deleterious ingredients from iron; but we
are not aware that it has hitherto been proposed, as is now done by
Girard and Poulain, to force the vapour of potassium or sodium
through the molten metal. ‘They propose to saturate the fuel with
carbonate of soda, and dry it, or to mix common salt with the fluxing
materials. These inventors, however, appear to place most confi-
dence in a process for blowing those vapours mixed with moist air,
or moist carbonic oxide, through the melted metal in a Bessemer
converter. Pure iron or steel is said to be thus obtainable at
pleasure. If experience proves this, we shall soon hear more of this
process.
The continually-increasing demand for high-class pig-iron and
iron ores, caused by the extension of the Bessemer process, has
brought into notice the red hematite and magnetic ores of Norway
as a possible source of supply for the Continent. According to a
statement published in the ‘ Berggeist,’ a paper representing the
metallurgical interests of Westphalia and the Rhine provinces, it has
recently been suggested to employ the magnetic ores raised in the
neighbourhood of Arendal for the production of Bessemer iron on
the spot, the total output of which the mines are capable being
estimated at 50,000 tons of 40 per cent. annually, which it is pro-
posed to smelt in two moderate-sized furnaces with coke made on
the spot from washed English small coal. Whether such a proposal
is likely to be commercially successful may be doubted; but the
point is in so far of interest as showing how completely iron making
is now governed by the item of cheap fuel; the making of char-
coal pig-iron even in a thickly-wooded country like Norway being
nearly at an end, for out of fifteen blast-furnaces in the southern
part of the country only five are now in blast, the cost of produc-
tion of pig-iron being nearly 67. per ton, owing to the high price of
charcoal... On the system proposed, the cost of No. 1 grey Bessemer
iron is computed at 68s. 6d. per ton, which, could it be realized,
would leave a fair margin on the selling price of hematite pig-iron
in our north-eastern ports. ee
P
558 Chronicles of Science. [ Oct.,
The question of the exact nature of the changes involved in the
conversion of pig-iron into steel in the Bessemer process, or rather
of the composition of the pig-metal employed, is still a matter of
great uncertainty. That sulphur, phosphorus, and copper are in no
degree removed during the process, and that consequently these
impurities must be absent from the metal treated, is proved by all
the analytical investigations made in this country as well as in
Sweden and Austria. As regards the question of silicon, Professor
Jordan, of Paris, has recently pointed out, in a memoir published
in the ‘ Revue Universelle,’ the probability that the enormous heat
developed in the process is mainly due to the combustion of this
element, because the whole of the heat produced by the burning of
silicon to silica, of silicate of protoxide of iron in the slag, and the
subsequent formation is entirely retained in the metallic bath, while
that produced in the combustion of the carbon to carbonic oxide is
in great part carried out in the current of flame and heated gases
issuing from the mouth of the converter. The exactitude of this
view cannot of course be positively demonstrated, because neither
the calorific power of silicon nor its specific heat has yet been
determined. If, however, we assume with Professor Jordan, which
is not improbable, that these factors are the same for silicon as for
carbon, it can be shown that in the conversion of a pig-iron contain-
ing 4°25 per cent. of carbon and 2 per cent. of silicon that the
amount of heat developed by the combustion of the latter element is
more than six times as much as that obtained from the former. In
proof of this statement it is asserted that the Bessemer process could
only be successfully carried out at Terrenoire in France when the
metal was run direct from the blast-furnace to the converters, the
small proportion of silicon, about 14 per cent., present being not
sufficient to allow it to be cast into pigs and remelted, as is usually
done. The dark grey No. 1 Bessemer pig-iron produced in Cum-
berland and Lancashire contains generally from 2:6 to 2:7 per cent.
of silicon.. It appears to be probable, however, that when too much
silicon is present, or rather when its proportion as compared with
that of the carbon is too high, it may not be entirely removed in the
blowing.
The separation of sulphur and phosphorus from iron has long
been a problem of much interest, especially so since the introduction
of the Bessemer process. At the Working Men’s International
Exhibition at the Agricultural Hall, London, is a display of speci-
mens of iron obtamed, by a process invented by Sir Antonio Brady,
from some of that dockyard refuse irreverently described as “ Seely’s
pigs,” and which has been the subject of discussion both in Parlia-
ment and by the press. ‘These pigs were of different qualities, but
were all largely contaminated with phosphorus and sulphur, and
were supposed to be of little or no value. The presence of phos-
1870. ] Metallurgy. 559
phorus renders iron brittle when it is hot ; the presence of sulphur
renders it brittle when it is cold. The pigs containing both were
worth in the market about 2/. 5s. a ton. By Sir Antonio’s process
the sulphur and the phosphorus is said to be extracted at a cost of
about 35s. a ton, and the residual iron is described as “superb.”
One of the pieces exhibited is stated to have been beaten cold to the
thinness of writing paper at one end, drawn to a point at the other,
and then twisted by hand eight turns in an inch at a single heating.
Massive bars are said to have been beaten cold until the surfaces on
each side of the bend came into perfect contact, and a plate six inches
wide and half an inch thick to have been beaten till its edges were
in contact, the flat surface remaining horizontal. In neither case
was there any trace of a flaw, either at the convexity of the curve,
where the metal was stretched, or at the concavity, where it was
compressed. Holes in a thick plate are labelled as having been
enlarged by driving cones into them, and, in a word, the iron is
described as having been knocked about in every possible way. At
a very low estimate it is affirmed to be worth 14/. a ton, and as
there is plenty of the raw material to be had, the profit of the
invention seems likely to be great.
A remarkable steel casting was made recently at the works of
Messrs. Thomas Firth and Sons, Sheffield, which deserves a record:
This casting is to form the shaft of the screw of the Dublin Steam-
Packet Company’s vessel ‘ Munster,’ and is about 15 feet in length
by nearly 4 feet in diameter, and weighs over fifteen tons. This ig
one of the largest blocks of steel ever cast in this country.
The work of melting commenced about eight o'clock, in no
fewer than five hundred and forty-four crucibles, each containing
64 lbs.—the total quantity of steel beg 34,816 Ibs. At half-past
twelve the work of casting began, and was rapidly completed, by
the joint and perfectly organized action of 300 men. This metal-
lurgical operation was a perfect triumph of mechanical skill.
The enormous difficulty and expense caused by the ever-accu-
mulating mountains of slag produced by iron furnaces worked on
the modern scale, often amounting to as much as 60 tons per furnace
per day, has led to different proposals for utilizing these unpleasant
ejecta, and we remember certain glowing descriptions of valuable
results to be got by converting the despised slags into materials
rivalling the finest porphyries and other ornamental rocks. The
less ambitious but more practical plan of using them as paving
stones has been for some time past under trial in Brussels, and,
according to Kennis, with such success that they are to be employed
generally in the repavement of that city. The process employed ig
simply that of allowing the cinder to run from the furnaces into
an excavation sufficiently large to contain the whole daily yield of
several furnaces, and the cooling is retarded by covering the surface
560 Chronicles of Science. [ Oct.,
with earth when the pit is filled. When cold the mass is found to
leave a widely-radiated structure, recalling that of natural volcanic
rocks, and the texture is that of a finely crystalline or granular
porphyry, having a mean specific gravity of 2:77. The surface is
said to wear in such a manner as not to become slippery under
traffic, and the cost to be 20 per cent. less than that of ordinary
stone paving. It is very much to be desired that experiments of
this character should be carried out in the only district in this
country where blast-furnace slags are used as a road material to
any great extent, viz. in Northamptonshire, where, according
to the present method, the general character of the roads may be
represented by a series of parallel ruts filled with broken glass,
owing to the slag used being cooled in small masses, producing a
vitreous substance unfitted for road making, but which is used
owing to the difficulty of obtaining natural stone for the purpose.
A new process of casting metals has lately been attracting con-
siderable attention. In July a number of gentlemen met at the
Lancashire Engineering and Compression Casting Works, at St.
Helens Junction, to witness the new process of casting in brass
and iron chased and embossed work of the most elaborate descrip-
tion. The process, which was here for the first time exhibited in
England, is an American invention, and its utility was shown to
consist in this—that any design, whether in high or low relief,
chased on metal of any required pattern or shane, whether flat as a
door-plate or round as a vase, can be produced by castings from it
ad infinitum, and each casting will show upon it all the sharpness
and beauty of the original chasing. Moulds are made with a pre-
paration of fine clay from tlie articles to be reproduced. The
making of one of these moulds takes a person from five to ten
minutes. The moulds have then to stand twenty-four hours ex-
posed to dry air, after which they are baked in a furnace for eight
hours. These clay moulds, into which the metal is afterwards
poured, are, to all intents and purposes, encaustic tiles. The
moulds are placed in a box, and the air is extracted from them so
as to form a vacuum, after which the molten metal is forced into
them, and in this way, in ten minutes, a casting can be completed.
When the casting is taken out, the design, however intricate, is
found to be perfectly represented, with the exception of removing a
slight surface of clay from it, which can be done in half an hour,
and the article is then ready to be sent to the bronzer, instead of
having to be kept in the chaser’s hands. In this way an enormous
amount of cost and labour on ornamental articles in metal is saved.
A new process for refining and desilvering lead has been intro-
duced by Gustave Luce, Son, and Bozan, of Marseilles. The
invention consists in the application of steam. For this purpose
the crude argentiferous lead is melted down in a vessel heated by a
1870. | Metallurgy. 561
fire, and provided at its lower end with a spout, closed with a slide,
through which, when the lead is melted, 1t is caused to flow down
into a lower vessel or vat, heated only at times directly by a special
fire, and at other times by the waste heat from the fire of the upper
vessel. When the lower vessel is full, steam is introduced through
a central pipe, leading down to near the bottom of the vessel,
where it is provided with a cock turned by a rod from above,
and with a disc, for the purpose of dividing the steam as it enters.
The steam, in passing up through the molten lead, effectually
oxidizes all impurities, which then rise in the form of scum to the
top of the metal, whence they are removed. The introduction of
the steam at the same time produces a violent ebullition of the lead,
causing it to crystallize; and when this crystallization has taken
place to a sufficient extent the introduction of steam is stopped by
closing the cock on the steam-pipe, and the remaining liquid portion
of the lead, in which the greater proportion of the silver will be found
concentrated, is run off through one or more spouts into troughs
turning on pivots for conducting the lead into a series of ingot
moulds. During this time a fresh charge of lead, containig a
percentage of silver approximating to that of the crystals in the
lower vessel, has been melted down in the upper vessel, and is run
into the lower vessel as soon as all the liquid portion has been
removed therefrom. Steam is then again introduced, effecting a
further purification and separation of silver, and this process is
continued until, by the repeated crystallization, one part of the lead
is rendered comparatively free from silver, to be used as merchant
lead, while the lead run off is sufficiently rich in silver for the
cupelling process. The duration of each operation for twelve or
thirteen tons of argentiferous lead is about from two and a half to
three hours. 3
The Iron and Steel Institute, whose first provincial meeting
was held at Middlesbrough last year, has just held (September,
1870) another such meeting at Merthyr Tydfil, the chief seat of
the coal, iron, and steel industries of South Wales. The formal
business meetings of the Institute extended over two days, and
other two days were devoted to the inspection of the iron and steel
works at Swansea and Ebbw Vale. Although the Institute has
not yet been in existence two years, there are already upwards of
350 members enrolled, a large proportion of whom were present at
Merthyr, notwithstanding its great distance from the other prin-
cipal seats of the iron-trade, and the difficulty attending the means
of reaching it. At the meeting just held, the Duke of Devonshire
presided, and Mr. Henry Bessemer was elected to the presidentship
for the ensuing two years. The Council of the Institute have
resolved to discontinue the publication of the ‘ Transactions of the
Institute, and to issue instead a quarterly journal devoted to the
562 Chronicles of Science. [ Oct.,
science and practice of the iron and steel manufacture, both at
home and abroad. The foreign editorship of the journal is to be
conducted by Mr. David Forbes. Several very interesting and im-
portant papers were read and discussed at the Merthyr meeting.
We can only find space to indicate the subjects upon which they
treated.
I. “The Geological Features of the South Wales Coal-field.”
By Mr. William Adams, Cardiff. In this paper the extent of the
coal supply of South Wales was put down at 36,000,000,000 tons,
even after making a very liberal allowance for faults, waste, loss in
working, &c.
II. “On Pumping and Winding Machinery at the Castle Pit,
Cyfarthfa.” By G. C. Pearce, Cyfarthfa Iron-works. This was a
short paper describing some recently-erected machinery of a superior
character, and which was carefully inspected in operation by the
members.
III. “On the Condition of Carbon and Silicon in Iron and
Steel.” By Mr. Geo. J. Snelus, Associate of the Royal School of
Mines. This was the longest and most elaborate paper read at the
meeting. In it the author showed that he had struck out a new
path, a method, or rather methods, of mechanically separating the
carbon and silicon contained in iron and steel, which will doubtless
prove to be a valuable supplement to the ordinary methods of
chemical research.
IV. “Ona New Form of Pyrometer.’ By Mr. C. W. Siemens,
C.E., F.R.S. The author described several kinds of pyrometers,
and then described and exhibited one constructed upon a plan
involved in the principle that the pure metals have the property of
offering an increasing resistance to the passage of an electrical
current with increase of temperature.
V. “On the Efficiency and Durability of Plain Cylindrical
Steam-Boilers.” By Mr. Jeremiah Head, Middlesbrough. The
author of this paper gave an account of a new method of suspend-
ing or supporting plain cylindrical boilers so as to prevent explo-
sions. Out of nearly 18,000 boilers on the books of the boiler
insurance companies, 22:7 per cent. are of this sort, thus showing
that they are much in request. A method of ensuring their safety
is therefore a thing much to be desired.
Other two papers were set down for reading, but there was no
time left for them. One of them was by Mr. F. Kohn, C.E., and
the subject was, “ On the Production of Alloys of Iron and Manga-
nese, and on their Application to the Manufacture of Steel.”
¢
1870. | Physics. 563
TLIO PEYSICS.
Liaut.—A new substance possessing fluorescent properties in a
very high degree has been prepared by Professor A. H. Church
from the Cyclopia vogellii, one of the plants used by the African
Boers for tea. It possesses acid properties, and the discoverer calls
it cyclopic acid. Its action on light is best seen when a crystal or
two of the new body is dropped into a solution of caustic soda and
viewed in sunlight. An intense greenish-yellow fluorescence is
perceived at first, but disappears in the course of some hours.
A new artificial light which has recently been successfully ex-
perimented with, called the Philipp carbo-oxygen lamp, and its
recent trial at Cologne, was such as to win approval on every hand.
The light is generated by the combustion of a liquid chemical com-
pound in a current of oxygen, arrangements for the purpose being
constructed in a suitable lamp. The gas is derived from the
atmosphere either by chemical or mechanical means; the chemical
methods being to absorb the oxygen of the air with chloride of
copper (Mallett’s method), or with manganate of potash (Tessie du
Mothay’s method), while the mechanical mode is that of utilizing
the different degrees of solubility of nitrogen and oxygen in water
or other liquids. By compressing atmospheric air into receivers
filled with water, a portion of the nitrogen is taken up by the
water, while the oxygen remains insoluble in the water; the air
thus containing a goodly proportion of oxygen is forced into a
second reservoir of water, where a further amount of nitrogen is
absorbed, and after the operation has been repeated seven or eight
times, an atmosphere is obtained containing 97 per cent. of oxygen.
The nitrogen which has been separated is made use of in a well-
constructed apparatus as an auxiliary to the motive force. Hxpe-
riments have established the fact that a flame fed with air contain-
ing 53 per cent. of oxygen yields a light equal in brillancy to that
obtained with pure oxygen, and with diluted oxygen of this kind
the Philipp flame has a brilliancy of 90 to 100 candles, or ten
times that of an ordinary gas jet. The light is of a bluish-white,
resembling very much that of electricity or burning magnesium.
The liquid employed consists of liquid hydrocarbons very rich in
carbon; it costs but little, burns economically, and can be em-
ployed only in this particular direction. The flame is made to
assume the form of a star, and any heating of the wick-holder
thereby prevented ; if of the size and power above mentioned, the
quantity of gas consumed is 54 cubic feet per hour. As to the
lamp, no special attention is necessary beyond that of filling it with
liquid, as the wick is of a very durable nature, and needs no trim-
ming.
564 Chronicles of Science. [ Oct.,
An optically-neutral sugar has been prepared by EH. J. Mau-
mené. He mixes equal parts of pure sugar-candy and neutral
nitrate of silver, both previously dissolved in water, and evaporates
the mixture upon a water-bath. He states that neither at 100°,
nor even at 140°, any decomposition ensues or any reduction of
silver takes place, provided the sugar be free from inverted sugar.
The sugar, rendered syrupy by the process described, is optically
neutral. The silver-salt is separated from the sugar by means of
pure chloride of calcium, and the nitrate of lime is separated from
the sugar by the addition of alcohol and placing this mixture under
a bell-jar along with quick-lime. In this manner, by slow concen-
tration, two layers of different specific gravity are formed: the
upper being an alcoholic solution of nitrate of lime, the lower a
viscous saccharine liquid. The former is poured off, and, by a
slight washing with cold distilled water, the thick sugar solution
is freed from any adhering nitrate of lime. The sugar obtained
does not crystallize.
In a lengthy paper on the optical properties of benzyl, and of
some substances belonging to the camphor groups, in the crystal-
line state and in solution, M. des Cloizeaux describes a series of
experiments, the chief results of which are that benzyl and perio-
date of soda possess, when in the solid crystalline state, strongly-
marked rotatory powers, and are devoid thereof in the state of
solution. Quartz, chlorate, and bromate of soda act the same.
Sulphate of strychnia possesses rotatory powers in crystals as well
as in solution, while ordinary camphor, patchouli camphor, cam-
phor of oil of mint, Borneo camphor, tere camphor, and monchlor-
hydrate of turpentine possess rotatory power when in solution, but
not in the crystalline state.
O. Loew has found that when aqueous sulphurous acid is ex-
posed in sealed tubes to the action of sunlight, it is gradually
reduced to sulphur, but the oxygen is not liberated, another part
of the acid having been oxidized by it to sulphuric acid.
According to J. Girard, who has made several voyages on the
Mediterranean Sea, its peculiar colour, ranging from pale blue
through all shades of that colour to black (viz. when seen from a
ship’s deck), is entirely due to the mode of reflexion of the sun’s
rays according to the lower or higher position of that luminary
above the horizon, so that at mornings and evenings, when the rays
fall more obliquely and pass therefore through a larger bulk of
water the colour is deepest, provided it be at such distances from the
shore that the depth of the sea is sufficiently great.
At one of the recent meetings of the Franklin Institute, Pro-
fessor Morton exhibited in the lantern some pictures on gelatine
prepared in a manner devised by Mr. Holman. For this purpose
1870. | Physics. 565
a sheet of gelatine, such as is used for tracing by engravers, was
securely fixed over an engraving, and with a sharp steel point
(made by grinding down the end of a small round file), the lines
of the original traced pretty deeply on the transparent substance.
Lead-pencil or crayon dust was then lightly rubbed in with the
finger, and the picture was at once ready for use. A number of
such drawings could be easily carried between the leaves of a book,
each in succession being held in a frame or cell made of two plates
of glass separated by a frame of thin card or three edges, and united
by paper or muslin pasted around the same edges. ‘The effect of
these drawings in the lantern was excellent, and their ease of pro-
duction very great.
A most valuable adjunct to the microscope has been made by
Mr. J. Zentmayer. It is a mechanical finger, which in the study
of diatoms forms a substitute for the clumsy fingers of the human
hand, to do the delicate work of picking up rare and valuable dia-
toms detected by the microscope, and to transfer them to a slide for
preservation. The instrument may be readily understood on reference
to the accompanying cut.
: L
A is the top plate of —-
the mechanical stage; the ——
circular plate is omitted. ie = —
The cap B is fitted to the
lower body below the stage,
into which cap the new
sub-stage cis fastened by a
narrow tube, wide enough — =A Lim
to admit illumination from fammiil camapegisnssecl
the mirror. As the lower ~~ — =
body is movable up and al Jar e
down by a rack, another ie l I
movement is gained which
is necessary to accomplish the result. The difference of the size
of the aperture of the stage and the diameter of the tube which
connects the sub-stage with the cap A is equal to the movement of
the mechanical stage, and this is found more than sufficient. D is
the clamp by which the finger is attached to the stage by means of
the screw E. A steel cylinder, a, is nicely fitted into the top and
bottom of the tube F, leaving room inside for a light spring to press
the steel cylinder upwards. To prevent turning, the spring J is
provided at u with a steel pin, accurately fitted into the fork at the
top of the tube Fr. By turning the nut x the spring J is elevated
and depressed, giving nice adjustment to the needle N in case the
finger is to be attached to a microscope not having rack movement
to the cap B, to bring the end of the hair and the object in close
approximation. ‘The end of the spring 3 forms a little rg, with
566 Chronicles of Science. [ Oct.,
a screw cut inside into which a cork m is screwed to receive a
needle n, to which a hair is fastened by wrapping gum paper
around. Turning the cork facilitates the adjustment of the hair to
the proper inclination. A slight pressure on the button 1 brings
down the hair, and the spring inside of F instantly lifts it again
when the pressure is removed. The tube F turns in the clamp D in
order to adjust the hair and cork more conveniently, and when
brought back again it is tightened by a set screw. Complicated as
it may appear, only one movement is added to the microscope stand
by this instrument, the one, namely, which gives the vertical motion.
When the apparatus is to be used, the material to select from is
placed on the sub-stage c and focussed, then the point of the hair is
approximately brought over the selected object by means of the
stage movements and turning of p; this brings the hair nearly in
focus too, because it is almost in the same plane with the object.
Next adjust the hair precisely over the selected shell, press down
the button 1, and the shell will adhere to the hair. Now remove
the slide with the material and substitute a glass slide moistened by
breathing on it, and having brought it in proper position briskly
dip down the button x again and the shell will be deposited on the
glass slide. If the mechanical stage has a graduated indicator, the
finger may be moved along regularly and shells may be placed at
equal distances in lines. After the cover glass is carefully placed
over it, Canada balsam may be run in by capillary attraction with-
out disturbing the position of the shells.
Hzat.—Dr. J. D. Boeke, Teacher of Chemistry at the Hoogere,
Burgerschool at Alkmaar, opposes the statement of Mr. Loew that
ozone is formed by rapid combustion. On repeating Mr. Loew’s
experiment with this slight modification, that a stream of oxygen
instead of azv was blown through the luminous flame of a Bunsen’s
burner into the mouth of a glass balloon, he really found that the
air in the balloon had assumed a peculiar odour, and the property
of colouring blue a mixture of starch paste and of potassium. But
it appears that both changes are the result of the formation of a
compound of oxygen and nitrogen (probably dinitric trioxide or
nitric dioxide), not from the formation of ozone, as Mr. Loew asserts.
So when Mr. Loew declares that he was able to “identify the for-
mation of ozone by its intense odour and the common tests,” he was
somewhat rash in this conclusion. Still Mr. Loew’s experiment is
a yery interesting and easy one, and will soon take its due place in
the series of lecture-experiments intended to elucidate the complex
phenomena of combustion.
H. Sainte Claire-Deville relates at great length a series of ex-
periments which may be summarized as follows:—Perfectly pure
iron kept at temperatures varying from 150°-1600°, is treated with
1870. | Physics. 567
vapour of water of a known tension and temperature. Under these
conditions results are obtained which prove that the decomposition
of vapour of water by iron while red-hot is rigorously subject to all
the laws which govern the tension of saturated vapours.
M. E. Cappel has published a lengthy paper on the influence of
the temperature on the sensitiveness and delicacy of spectrum
reactions. ‘The main result is, that the temperature most suitable
for the spectrum analysis of the alkalies is that of the oxyhydrogen
flame, and for the rest of the metals the heat of the electric spark.
The higher the temperature the more distinct the reactions.
In some observations on the batswing-burner flame, Dr. A.
Baudrimont states that the flame consists of two distinct portions,
one of which (the interior) has a comparatively low temperature
while it is surrounded by a luminous envelope, the temperature of
which exceeds that of molten platinum. Indeed the author found
that a platinum wire ,1,th mm. thick, when properly placed in this
flame, fused immediately.
General Morin has experimented at the Conservatoire des Arts
et Métiers on some fire-clay stoves; the results are said to be
highly satisfactory. The useful effect of heat given off by the fuel
amounts to 93 per cent. The air in the rooms where these stoves
were placed was not at all vitiated so as to incommode those pre-
sent, notwithstanding the interior of the stoves became thoroughly
red-hot. The author says that, takmg all in all, these stoves,
when suitably connected with flues, will afford a cheap and in
every respect wholesome mode of heating apartments.
A new material for the manufacture of crucibles is described by
M. J. Desnoyers. The substance known as gaize, or pierre morte,
is a mineral largely met with in the departments of the Ardennes,
where it forms a deposit of some 100 metres thickness. Its specific
erayity is 1:48. It is on being dug up quite soft, so that it can be
cut with a knife, but becomes hard on drying and very hard when
exposed to red-heat, whereby its specific gravity is reduced to 1-44.
This material is essentially a substance capable of withstanding high
temperatures; and the author exhibits crucibles made from the
gaize which have been used successfully for melting iron. Dr. La
Salvelat, the celebrated chemist of the Imperial Porcelain Works
at Sévres, states that layers of similar material exist in the central
parts of France, and that these minerals are of great value for the
construction of blast and other furnaces.
By the term “rochage,” H. Caron understands a peculiar pro-
duction of sparks, best seen when molten cast-iron is run off from
the blast furnace into moulds. In a lengthy paper the author
describes a series of experiments undertaken with the view to prove
that since steel and cast-iron, when molten in an atmosphere of
568 Chronicles of Science. | Oct.,
hydrogen or oxide of carbon, never emit sparks, the production of
the latter cannot be due to an evolution of reducing gas absorbed
during the fusion, but is due, according to the author, to the forma-
tion of oxide of iron at the moment the molten metal comes in
contact with air. This curious phenomenon is well known to those
engaged at blast furnaces. The sparks are known by the workmen
as “jumpers,” and their presence is usually held to indicate an
approximation to white iron. These sparks are absent during the
running of grey iron from the furnace, and only begin to make their
appearance when the iron is about No. 4, the usual degree of grey-
ness preferred in South Staffordshire for puddling. ‘The sparks are
best observed during the running of white iron from the furnace,
especially if the molten metal is not very fluid, at which times a
vast number are produced, particularly in the channel; and some-
times after the pigs have “set,” little jets of sparks are continuously
discharged for many minutes, which discharge is accompanied by a
hissing sound. M. Caron’s view may probably be correct, but a
correspondent of the ‘Chemical News, who signs his name T. B.,
says that he is inclined to attribute the production of these sparks
to the combustion of carbon and not of iron, as there is an entire
absence of the peculiar scintillations displayed by burning iron.
A very striking mode of demonstration in the lecture-room that
burning bodies increase in weight has been contrived by H. Kolbe.
A glass rod is fastened in a horizontal position to one arm of a
balance. Upon this is fastened a glass cylinder in which a candle
is burnt, connected with which, by a glass tube, there is a V-tube
for condensing the vapour, a flask filled with lime-water for carbonic
anhydride, and two more V-tubes containing soda-lime. The last
are connected by an india-rubber tube with a Bunsen’s pump, by
which a steady current of air is drawn through the apparatus. The
beam is first counterpoised; as the candle burns away the arm of
the balance to which it is attached sinks down until its progress is
arrested by the table.
Mr. W. T. Suffolk, the well-known microscopist, has experi-
mented during a pedestrian tour on the most advantageous methods
of boiling water, and has come to the conclusion that the very best
arrangement is an “Etna” of French construction made of very
thin copper, electro-plated, and weighing, with a store of 6 oz. of
spirit, 14 lb. The time occupied in boiling half a pint of water is
from seven to ten minutes, and the consumption of spirit about
two fluid drachms. The apparatus requires a perfectly calm atmo-
sphere for its proper action; this may be secured by building a
small cromlech of flat stones, which are always at hand in hilly
countries, and with the help of a large handkerchief as a further
protection against the wind, no difficulty will be found in securing
1870. | Physics. 569
efficient performance ; other contrivances will suggest themselves
where stones are not procurable. Although it would seem that
alcohol is consumed to a disadvantage without a wick, yet practi-
eally the “Etna” boils water with a smaller consumption of spirit
than any contrivance yet tried, a good argand lamp requiring at
least half an ounce to do the same work as the Htna. The Russian
blast lamp is still more wasteful, consuming nearly 2 ounces. The
superior economy of the Ktna is attributed to the low temperature
of the wickless flame and the manner in which the boiler is wrapped
in the fire, no more heat being supplied than can be taken up by so
bad a conductor as water. The defect of all lamps giving an
intense flame being that heat is wasted by being supplied too
quickly, so that the apparently feeble fire in the gutter of the tna
is more efficient than the heat of powerful lamps, as well as more
economical ; the latter quality is very important to the pedestrian,
to whom every ounce of weight is a consideration.
P. Lewald, referring to the phenomenon first observed by Dr.
Fritsche, says it is not at all a correct statement that the blocks of
tin exposed toa cold of — 35° should alter their state of aggregation
from that cause; the real cause is that the blocks of tin usually of
250 cubic inches capacity are cast in iron moulds, and as a conse-
quence thereof the tin contracts unequally, and so as to leave in the
inside of the blocks cavities often so large as to occupy 40 cubic
inches. These hollows are lined by a crystallized metal at a high
degree of tension. The tin at St. Petersburgh was laying heaped
block upon block, and the effect of the cold was simply a remote cause
to what took place, the weight of the blocks of metal placed on each
other being such as to produce necessarily a pressure too great to be
borne by the undermost blocks. The author says, if tin is molten
and allowed to cool, so as to shrink uniformly, no cold, even of — 40°
or less, will have the effect observed in the locality alluded to.
L. Cailletet has studied the variation of compression of air and
hydrogen between 1 and 800 atmospheres. Up to 80 atmospheres’
pressure, air is more compressed than it should be if it followed the
law of Mariotte ; and at 680 atmospheres’ pressure it only occupies
two-thirds of the space which it ought to do theoretically. The
method by which the author is enabled to measure the volumes
occupied by a gas in an opaque apparatus is very simple. The glass
tube is enclosed in an iron one; the former, containing the gas, is
lightly gilt. The mercury which serves for the transmission of
pressure, whitens the gold, leaving a well-defined mark on it after
the pressure ceases.
Exectriciry.—In a letter to M. Dumas, Professor de la Rive
states that he has just finished a series of experiments on the mag-
570 Chronicles of Science. [ Oct.,.
netic rotatory power of liquids, the results of which will be shortly
published. The first portion of this work is devoted to the descrip-
tion of the apparatus and processes of experimentation ; the second
part contains the results of the determination of the magnetic
rotatory power of some liquids. As a curious anomaly the author
mentions that taking water as unit, the coefficient of the magnetic
rotatory power of monohydrated sulphuric acid is 0°750, and that
coefficient is, for liquid anhydrous sulphurous acid, equal to 1-240
at a temperature of 12°. The third part of this work is devoted to
the study of the influence of the temperature on the magnetic rota-
tory power. In the fourth part, the author gives the results of his
investigations of the magnetic rotatory power of a mixture of two
liquids as compared with that each of these liquids possesses sepa-
rately. The fifth part contains the results obtained by experiment-
ing with two isomeric liquids.
In some experimental researches on the length of duration of
the electric spark, MM. Lucas and Cazin employ two transparent
discs placed upon the same axis. One of these discs is a fixture,
while a more or less rapid rotatory motion can be imparted to the
other. Upon both discs are painted the same number of opaque
stripes in the direction of the radius. When, therefore, an electric
spark is observed through these discs, a certain amount of speed
having been imparted to the movable one (the apparatus being
placed in a darkened room), it is clear that by the light emitted by
the spark a certain number of coincidences of the movable and fixed
stripes may be observed, and these coincidences may serve to calcu-
late the period of duration of the spark.
Dr. Demayes describes at length an apparatus constructed by
him, which appears to be an improvement on Siemens’ electro-
magnetic apparatus; while making from 250 to 280 revolutions a
minute, the lifting power of the magnet is 70 kilos., and under
similar conditions a platinum wire, 0°8 mm. thick and 20 centim.
long was rendered red-hot, and iron wire of the same thickness
fused ; the machine produces per second of time half a cubic centi-
métre of gas by the decomposition of water.
In a recent instalment of his researches on electro-capillary
action, which have occupied M. Becquerel for a series of years, he
announces the artificial formation of the oxychloride of copper in
crystalline state, and exactly similar to that found in the copper
mines of Peru and Chili, and known as atacamite. This formation
has taken no less than fifteen years.
Mr. E. W. Blake, jun., has described a method of producing by
the electric spark figures similar to those of Lichtenberg. The
method consists in throwing the discharge upon the surface of a
fusible non-conducting body. If the body be near its fusing-point
1870. | Physies. 571
the figure appears at once; if cold, a latent image exists, which
may be developed by heat. ‘The non-eonducting surface is prepared
by coating a plate of metal with an even film of pitch. Pieces of
sheet tin, 3 inches square, coated with films of pitch of a thickness
varying between 0°01 and 0°02 inch were used; the pitch was
the ordinary article of commerce freed from sand, &c., by being
melted and strained through a muslin bag. ‘The author gives cuts
of the figures as produced by frictional electricity and the induction
coil,
Metallic iron, as obtained by the electric current, has been ex-
amined by C. Collas. He employs a weak solution of chloride of
iron, which is decomposed by the aid of a Bunsen battery ; perfectly
pure iron is thus obtained, which is very friable, highly oxidizable,
especially when moisture is present. When this iron in the state
of fine powder is poured in a bottle when the atmosphere is very
moist, the iron is instantaneously oxidized, water decomposed, and
the evolution of hydrogen causes the bursting of the bottle.
A new method of copper extraction and its separation from other
metals is published by Mr. J. Elkington. The principle consists
in applying electricity for dissolving the copper contained in the
crude metal obtained by the usual smelting methods, and for de-
positing that metal galvanically upon plates of copper, causing the
other foreign metals to fall to the bottom of the vessels in which
the operations take place; copper containing very small quantities
of silver may be advantageously treated thus for the recovery of
the last-named metal.
An improvement in galvanic batteries has been devised by Mr.
W. Poole Levison, of Cambridge, Mass. While making use of a
small bichromate of potash battery he discovered that the addition
of nitric acid to the mixture of potassic bichromate and sulphuric
acid contained in its porous cups, conferred upon it the virtue of
steadiness without involving the evolution of annoying fumes. For
over two months during last summer the author had in almost
constant action a combination of twenty-three large Bunsen cells
charged with dilute sulphuric acid and the triple mixture mentioned,
and “set up” openly upon the floor of the room. Not only did he
work about it with perfect comfort, but left choice brass instruments
in its immediate neighbourhood with impunity. Its energy never
fluctuated, but after remaining for some time steady declined, pre-
cisely as if the electro-negative plates were bathed in nitric acid
only. To a cooled mixture of potassic bichromate solution and
sulphuric acid (perhaps preferably in atomic proportions) add nitric
acid. The proportion of nitric acid may be greatly varied, as its
office is merely to transfer oxygen.
A research on the best methods of tinning of iron without the
VOL. VII. 2 Q
572 Chronicles of Science. [ Oct.,
aid of heat has been carried out by J. B. A. Daubié. The chief point
of interest is that the tinning of iron in the cold cannot succeed at
all, unless the bath used for that purpose contains in solution or
suspended an organic substance like starch or glucose, although no
precise scientific explanation of this indispensable condition has been
hitherto given. The author employs the following bath: To 100
litres of water are added 3 kilos. of rye meal ; this mixture is boiled
for half an hour, and next filtered through cloth. To the clear but
thickish liquid are added 106 kilos. of pyro-phosphate of soda,
17 kilos. of protochloride of tin, 100 to 120 grammes of sulphuric
acid ; this liquid is placed in well-made wooden troughs, and serves
more especially for the tinning of iron and steel wire for the use of
carding-machines. When instead of the two salts of tm just named
cyanide of silver and cyanide of potassium are taken, the iron is
perfectly silvered.
12. ZOOLOGY AND MORPHOLOGY.
The Zoological Position of the Brachiopoda—Leuckart, Haeckel,
and Gegenbauer do not include the Polyzoa among the Mollusca,
as is done by Huxley, but class them as also the Tunicata among
the great heterogencous group of Vermes. Mr. Morse, an American
naturalist, who has devoted much study to the Molluscoida, pro-
poses to turn over the Brachiopoda into the same position. In
doing so he unconsciously meets an argument advanced in favour
of the retention of the Polyzoa among Mollusca by Professor
Rolleston, viz. that they present close affinities to the Brachiopoda,
especially to the larval Brachiopod described by Fritz Miler.
Mr. Morse has by perseverance obtained the great advantage of
studying living specimens of Lingula, a species of which he obtained
in quantity on the North Carolina coast. He compares the sete
which frmge the mouth of Lingula to those of Annelids (in this
he is probably misled), the lophophor with its cirrhi to the cephalic
appendages of tubicolous worms, the oviducts with their trumpet-
shaped openings to the funnel-like oviducts of many worms; the
embryo of Thecidium, with its four segments and eye-spots, 1s
adduced, as also the embryo of Discina, which, according to Fritz
Miiler, has projecting bristles like the temporary bristles of some
Annelid-larve. Mr. Morse says it is a startling discovery that the
vascular fluid of Lingula is red, and seems to think that this
colour gives this Brachiopod some affinity to worms. It is, how-
ever, not at all surprising, though Lingula is an interesting
addition to the category of invertebrata with red blood, including
as it does already the molluscs Planorbis and Arca. Probably
1870. ] Zoology. 573
the coloration is due to Hemoglobin as in the eases of Molluscs,
Insects, Crustacea, and Vermes with red blood, investigated by
Mr. Ray Lankester. Mr. Morse’s proposition to classify Brachio-
poda with Vermes deserves full consideration, but we shall look
for some solid reasons in the memoir which he promises on the
subject. ,
New Sponges.—Sponges continue to occupy a great deal the
attention of naturalists. Dr. Perceval Wright, Mr. Carter, Mr.
Charles Stewart, and others, have lately described new genera and
species. Mr. W.S. Kent, of the British Museum, who two months
since made an expedition to the coasts of Portugal in the yacht of
Mr. Marshall Hall, has described three new species (two belonging
to new genera) of that very important and interesting group, the
silicious sponges or Vitrea of Professor Wyville Thomson. The
Vitrea are represented by the notorious Hyalonema, or glass-rope
sponge ; by Huplectella, the beautiful lace-sponge ; and by Professor
Thomson’s new genus, Holtenta. Mr. Kent would recognize Dr.
J. E. Gray’s division of the Corallispongia im preference to that of
Vitrea proposed by Professor Wyville Thomson. In describing a
new species allied to that author’s Holtenia Carpenteri, he points
out that the genus Holtenca must give place to Pheronema, previ-
ously proposed by that most distinguished of American naturalists,
Dr. Leidy, of Philadelphia. There appears to be no doubt that the
sponge described under this name by Dr. Leidy is generically iden-
tical with Wyville Thomson’s subsequently described Holtenca. Mr.
Kent's new species is called Pheronema Gray, and was obtained by
him in the deep sea off the coast of Portugal. Two other inter-
esting vitreous sponges were also detected, and have been fully
described by Mr. Kent. ‘The Royal Society assisted Mr. Kent in
the outlay necessary for dredging apparatus, &c., and these new
sponges are among the first of the fruits of his voyage which he
has made known. The Society has done well to entrust some of its
funds to this promising naturalist; and zoological science is much |
indebted to Mr. Marshall Hall for using his yacht for its advance-
ment.
Bathybius and the Coccoliths.—The organism which Professor
Huxley described two years ago as being so widely spread in the
ooze of the ocean bottom, consisting of a simple ramified network
of protoplasm, has been recognized and fully established by no less
an authority than Professor Haeckel, of Jena. Professor Haeckel
gives figures of the protoplasmic network, and then discusses the
propriety of associating with this organism the Coccoliths and
Coccospheres, as Huxley has done. He does not arrive at definite
conclusions on this pomt; but re-figures all the various forms
of Coccoliths, Cyatholiths, and Discoliths described by Huxley.
Haeckel would at present definitely establish Bathybius on the
Para apy
574 Chronicles of Science. | Oct.,
protoplasmic network, and leave the exact origin of the Coccoliths
doubtful. A very remarkable observation which he has made neces-
sitates this ; for he has discovered a new genus of oceanic Radiola-
rians, in the centre of each specimen of which he finds a mass of
concretions which really cannot be distinguished from a Coccosphere.
In fact, we may say that Coccospheres are found inside these new
Radiolarians. At present there is nothing to show how they got
there: whether they are secretions of the Radiolarian, or whether
they have been taken in by it. Meanwhile the Coccoliths have
been observed in other oceanic accumulations besides the Atlantic
mud and the Chalk.
MiIscELLANEOUS.
Mr. Darwin and the French Academy.—At the outbreak of the
present war between Germany and France, the claims of our great
naturalist, to be elected a corresponding member of the French
Academy, were under discussion in that body. There is nothing
which has so fully illustrated the difference between the scientific
attitude of France—or rather let us say Imperial France—and
‘Germany, as the manner in which the views of Mr. Darwin have
been treated in these two countries. In Germany their almost
universal adoption has been the signal for the most active and
valuable investigations “fur Darwin ;” and the brilliant researches
of Fritz Miller, Haeckel, Kowalewsky, and others have proceeded
directly from this as a cause. Imperial France on the other hand
has, with a rare exception here and there, treated Mr. Darwin with
scorn and even insult. M. Flourens, the late perpetual secretary
of the French Academy, made a most unseemly attack upon Mr.
Darwin some years since, which Professor Huxley showed up for
the amusement of English readers in an article in the ‘ Natural
History Review,’ which is reprinted in his volume of ‘ Lay Sermons.’
In the recent discussion on Mr. Darwin’s claims, MM. Milne-
Edwards and De Quatrefages did justice to his merits as an observer,
though they do not accept evolution; but Brongniart, Robin, and
Emile Blanchard, appear to have expressed a very low opinion of
him : he was called ‘amateur, an ‘ inaccurate dreamer ;’ and Eli de
Beaumont, whose theory of mountain chains has been so completely
crushed by Lyell, said that Darwinism “is all fizz ”—“cest la
science moussée.” And yet it is a fact that Cuvier and Lamarck
were Frenchmen.
A New Manual of Zoology—Dr. H. Alleyne Nicholson, of
Edinburgh, lecturer on zoology in one of the medical schools, has,
with excellent intentions, produced a manual of zoology. He has
not done rightly, for the book is almost entirely an abridgment of
Huxley’s lectures published in 1856 in the ‘ Medical Times and
1870. | Zoology. 575
Gazette, of Greene’s ‘Manuals of the Coelenterata and Protozoa’
published eleven years since, and of Woodward's ‘ Mollusca’ pub-
lished fourteen years since. The only additions appear to relate to
the geological range of the various groups of animals. No attempt
is made to give any of the later results of investigation, nor to seek
information from original memoirs. ‘The writer gives his state-
ments at third-hand, and with the exception of some rough diagrams,
his figures have appeared in many a manual of zoology published
during the last twenty years.
Chioral, the New Opiate.—It is little more than a year since
Liebreich suggested the use of the hydrate of chloral as an anodyne,
and a few grains of it were obtained at the Exeter meeting of the
British Association, through the Pharmaceutical Association, for
experiment. Within six months of that time, such is the rapidity
with which the medical profession avails itself of any new and
valuable discovery, chloral was im daily use in nearly every London
and provincial hospital. However much we may complain of back-
wardness in England in some scientific matters, we cannot but ex-
press admiration at the remarkable activity of our medical men. It
has been urged upon the bodies who are sending relief to the
wounded soldiers in France, to forward chloral and chloroform.
Any individual who should go the round of the hospitals, or even
on the battle-fields themselves, and administer chloral to those suffer-
ing from the pain of wounds, would be able to spare an immense
amount of agony, and save many lives. This is one of the adjuncts
of war which science offers as a set off to her mitradleurs. Chloral
has also lately been used with much success in some cases by Dr.
Robert Caton, in making various physiological experiments in place
of curare or chloroform. His methods of studying the tissues of
living animals under the microscope, are published by him in the
last number of the ‘ Quarterly Journal of Microscopical Science.’
We hear also that Dr. Sanderson, F.R.S., and Professor Stricker,
of Vienna, who is now on avisit to this country, have succeeded by
the use of chloral, and by proper precautions for maintaining
temperature, in studying the living circulation of small mammalia,
so as to extend to the mammalia the inquiries commenced by Waller,
lately renewed by Cohnheim, as to the emigration of blood-corpuscles
from the blood-vessels in inflammation. This is most important
as bearing on human pathology and physiology, for hitherto such
observations had been confined to the cold-blooded vertebrata—
almost entirely, in fact, to fish and frogs, or toads.
576 Chronicles of Science. | Oct.
MorPHOLOGY.
Homogeny and Homoplasy.—In the July number of the ‘ Annals,’
Mr. Ray Lankester proposes to use these terms to signify certain
relations of parts in organisms which have hitherto been confused
under the one head of homology. Homogeny is applied to such
structures as owe their identity in arrangement and relation to
inheritance from a common ancestor ; parts which are thus rendered
similar in two organisms are said to be homogenous one with the
other. Many structures present, however, a very close similarity
in their relations to surrounding parts in two organisms without
being so inherited; the similarity beng due merely to a com-
munity of external conditions in the two cases, necessitating similar
corresponding internal arrangements. These agreements are said
to be due to “homoplasy,” and are called homoplastic one with
another. ‘The fore-limbs of all vertebrata are thus broadly homo-
genous, that is, are inherited from a common ancestor. But the
four cavities of the heart of the mammal and of the bird are not
homogenous each with each. The hearts as a whole are so, but
since the common ancestor of birds and mammals had in all proba-
bility a heart with three cavities, the four cavities cannot be due
to inheritance in the two cases. They are homoplasts; they are
due to similar exigencies in the mammalian and ornithosaurian
stock after their divergence from a common stock. Various in-
stances of homogenetic and homoplastic agreement are distinguished
in Mr. Lankester’s paper, and it is pointed out that what are called
serial homologies belong to the category of homoplasts; thus, the
fore and hind limb of vertebrata agree in many of their details of
structure on account of the mechanical arrangements required in
fore and hind limb being to a very great extent identical. In a
subsequent number of the same periodical, Mr. St. George Mivart,
F.RS., writing on the use of the term homology, accepts the
terms homogeny and homoplasy, though he would retain Professor
Owen’s word homology, in a wide sense, distinguishing homogenetic
homologies and homoplastic homologies. He also proposes to dis-
tinguish “ancestral homogeny” and “developmental homogeny.”
But it appears that “ancestral homogeny” is all that the term
homogeny was defined to include. What Mr. Mivart calls “de-
velopmental homogeny,” when it is not accompanied by ancestral
homogeny, falls simply under the category of homoplasy. The
subject is a little abstruse, but is of importance, since the doctrine
of homology as propounded by Professor Owen has sunk very
deeply into the mind of British anatomists; and now that so many
have accepted the doctrine of evolution, and the doctrine of creation
by types is no longer in favour, it becomes necessary to remodel
our terminology in accordance with new ideas.
1870. ‘ak cian
Quarterly List of Publications receited for Mebietv.
1. The Origin of Civilization and the Primitive Condition of Man.
Mental and Social Condition of Savages. By Sir John Lub-
bock, M.P., F.R.S. Longmans, Green, & Co.
. On Microscopical Manipulation. Being the Subject-matter of a
Course of Lectures delivered before the Quekett Microscopical
Club. With 49 Engravings and 7% Lithographs. By W. T.
i)
Suffolk, F.R.MLS. Henry Gillman.
3. Heat as a Mode of Motion. By John Tyndall, F.R.S. Fourth
Edition. Longmans, Green, & Co.
4. Class-Book of Inorganic Chemistry. By D. Morris, B.A.
Phillip & Son.
5. Chemical History of the Six Days of Creation.
New York: The American News Company.
6. Papers on the Theory and Practice of Coal-mining. By George
Fowler, Mining Engineer. Wm. Hutchings.
7. Notes of a Course of Seven Lectures on Electrical Phenomena and
Theories, delivered at the Royal Institution of Great Britain.
By John Tyndall, LL.D., F.R.S. Longmans, Green, & Co.
8. Annual Report of the Smithsonian Institution.
Washington: Government Printing Office.
PAMPHLETS AND PERIODICALS.
Mineral Statistics of Victoria. Melbourne.
Smithsonian Contributions to Knowledge :—
The Transatlantic Longitude as Determined by the Coast Survey
Expedition of 1866. By B. A. Gould.
The Indians of Cape Flattery. By James G. Swan.
The Gleddon Mummy Case. By Charles Pickering, M.D.
The Orbit and Phenomena of a Meteoric Fire-ball. By James H.
Coffin, LIZDs : Washington: Smithsonian Institution.
Index to his Observations on the Genus Unio. By Isaac Lea, LL.D.
Philadelphia: T, K. Collins.
On the Size of Red Corpuscles of the Blood of Moschus, &e. By
G. Gulliver, F.R.S.
First Report of the River Pollution Commissioners. (Blue Book.)
578 List of Publications | Oct.,
Narrative of a Journey to Musardu. By Benjamin Anderson.
New York: S. W. Green.
Remarks on Prof. Owen’s Monograph on Dimorphedon. By Harry
G. Seeley, F.G.S. Taylor & Francis.
On the Artificial Formation of Organic Compounds. By J. Campbell
Brown, D.Sc. Lond.
On Ailanthus Excelsa; a new Indian Remedy. By Mr. Narayan
Daji. Bombay: Asiatic Press.
A System of Botanical Analysis applied to the Diagnosis of Natural
Orders. By W. H. Griffiths, Ph.D. Wyman & Sons.
A Sketch of a Philosophy. Part IIJ.: The Chemistry of Natural
Substances. By John G. Macvicar, LL.D., D.D.
Williams & Norgate.
A Lecture on Malt Liquor. By Joseph Livesey.
Public School Reforms. By M. A. B.
Biology versus Theology. By Julian.
Statement of a recently-claimed Discovery in Natural Science. By
Research. Melbourne.
Railway across the Himalaya, projected by R. Stirling, Esq., F.R.S.
Contributions to the Mineralogy of Victoria. By George H. F. Ulrich,
E.GS. Melbourne: John Ferres.
Report of the Examiner of Coal-fields in New South Wales. In the
‘Newcastle Pilot’ (Australia).
Metropolitan Board of Works. Report on Steam Road-Rolling. By
F, A. Paget, C.E.
Notes on Books. Longmans.
On the Cause of the Motion of Glaciers. By James Croll.
On the Scientific Use of the Imagination. By John Tyndall, LL.D.,
F.R.S. Longmans.
The Technologist. New York: The Industrial Publication Company.
The Canadian Naturalist. Montreal : Dawson Brothers.
The Food Journal. London: Johnson, 3, Castle Court, Holborn.
The American Naturalist. Salem: Peabody Academy of Science.
The Geological Magazine. Tribner & Co.
Scientific Opinion.
The American Chemist. New York: Baldwin & Co.
The English Mechanic.
The Westminster Review.
Revue Bibliographique Universelle,
Fraser’s Magazine.
The Popular Science Review.
1870. | received for Review. 579
PROCEEDINGS OF LEARNED SOCIETIES, &c.
Vargasia. Boletin de la Sociedad de Ciencias fisicas y Naturales de
Caracas. Caracas : Imprenta del Estado Bolivar.
Ofversigt af Kongl. Vetenskaps-Akademiens Forhandlinger.
Stockholm: Norstedt & Sons.
Proceedings of the Lyceum of Natural History in the City of New
York.
The Journal of the Historical and Archeological Association of
Treland.
Transactions of the Woolhope Naturalists’ Field Club.
Fifth Report of the Quekett Microscopical Club.
Proceedings of the Royal Society.
» Royal Institution of Great Britain.
Monthly Notices of the Royal Astronomical Society.
-( 580 )
INDEX TO
A.
A B C Sewage Process, 512.
Asicu, Herr, on Crystallized Hail-
stones, 122.
Aboriginal Tribes of the Nilgiri Hills,
586.
Aborigines of America and Extermina-
tion of, 244.
Abyssinia, Geology of, 119, 408.
Acclimaiization of Half-hardy Plants,
100.
Acid, Hydrochloric, in the Stomach, 140.
Apams, W., Inaugural Address before
the Society of Engineers, 267.
Appis, W. J., on Single Rail Permanent
Way, 403.
Acassiz, Prof., on Reef-building Corals,
274.
Agricultural Prospects, 376.
—— Statistics, 243.
Agriculture, Belgian, 242.
—— Chronicles of, 87, 241, 376, 510.
Air, Compression of, 569.
—— Physical Analysis of, £00.
Pollution by Chemical Works, 330.
Atry, Prof., on Atmospheric Chromatic
Dispersion, 97.
Arey and Spos, Messrs, New Eye-
piece, 293.
Albolith, 399.
Albumen, Manufacture of, 105.
Algez, Japanese, 105.
Algol, Variable Star, 521.
Alps, Climate of the, 413.
America, North, Extinct Reptilia and
Batrachia of, 116.
American Eclipse Observations, 249.
Amylic Alcohol, Detection of, 398.
Anesthetic, New, 261.
Andaman Islands, Ancient Kitchen
Middens in the, 383.
Animal Life, Forms of, 363.
Physiology and Morphology, Chro-
nicles of, 139, 290, 431, 572.
Animals and Plants, Distribution of,
255.
Anthropological Society, Annual Meeit-
ing, 248.
“Anvil” Protuberance of Eclipse of
Aug. 7, 1869, 443.
[Oct.,
VOL. VII.
Apatite, 281.
Arborescent Forms in Stones, 130.
Archzological Discoveries in Yorkshire,
247.
Archeology, Chronicles of, 90, 244, 379,
512.
International Congress of Pre-his-
toric, 90.
Arctic Flora, 101.
AsHzE, Commander, on the Total Eclipse
of 1869, 251.
Aspidolite, a New Mica, 127.
Astronomy, Chronicles of, 94, 249, 389,
517.
Atrinson, J. C., Danish Element in
the Population of Cleveland, 384.
Atmospheric Electricity and Recent
Phenomena of Refraction, 229.
Aurora, on the, 250.
Australasia, Production of Gold in, 130.
Australia, Geology of, 272.
New Ganoid Fish from, 431.
Auvergne, Rocks of, 128.
Axinite, Constitution of, 127.
Aymara Indians of Bolivia and Pern,
516.
B.
Basrxetos, Prof. on the Flora of Ice-
land, 255. 955.
Bate, M, Heat from die Moon, 138.
Banceort, R. M., on the Renewal of
King’s Cross Station Roof, 268.
Bazses, S., on Atmospheric Electricity
avn Recent Phenomena of Refraction,
Bagg ty, Sir H., Flora of Round Island,
Mauritius, 256.
Baneetr, W. F., Light and Sound,
Baryta,
Bathybius and the Coccoliths, 573.
Batrachia and Repiilia, Extinct, of
North America, 116.
Bavuprmonxt, A., Examination of
Flame, 567.
— E., Uses of Tinfoil, 531.
Bxgcul, "Prof, Analyses of Beryl and
Tourmaline, 418,
i
1870.]
BrcqveEREL, E., Electro-capillary Action,
570.
on Electro-motive Forces, 431.
Beer Scientifically and Socially Con-
sidered, by J. Samuelson, 299.
Belgian Agriculture, 242.
BeEnEDEN, Prof. Van, on Commensalism,
291.
BENNETT, A. W., on Foreign Trees and
Plants for English Gardens, 350.
Benzyl], Optical Properties of, 564.
Bert, M., Physiology of Sepia, 291.
Beryl, Analysis of, 418.
Bessemer Process, 557.
Birt, Mr., on Lunar Crater Plato, 394.
Blackfriars Bridge, 111.
BuakE, E. W., Electric Spark Figures,
570.
BuanrorD, W. J., Geology of Abys-
sinia, 119, 408.
Origin of a Cyclone, 121.
Blast Furnaces, 192.
Blast-iurnace Slag, Utilization of, 260.
Blood, Origin of Fibrin of the, 139.
Bioxam, T., Ignition of Sodium on
Water, 106.
Buivm, Dr., on Pseudomorphs, 127.
Boeke, J. D., Formation of Ozone by
Combustion, 566.
Boiler Explosions, 536.
Incrustations, Prevention of, 109.
Boiling Liquids, Bumping of, 136.
Water, Best Method of, 568.
Bonney,'Rey. T. G., Pholas-burrows in
the Ormes Head, 118.
Bontemrps, M., Action of Light on
Glass, 286.
Bonwick, Mr., on the Origin of the
Tasmanians Geologically considered,
246,
Botanic Garden at Brussels, 528.
Botanist, Leonardo da Vinci as a, 100.
Botany, Chair of, at College of Science,
Dublin, 258,
—— Chronicles of, 99, 254, 394, 524.
Boulder Drift, on the, 275.
Bousstncautt, M., Colouring Matter
of the Emerald, 417.
Brachiopoda, Italian Tertiary, 540.
Zoological Position of the, 572.
Brapy, Sir A., Purification of Iron, 558.
Breidden Hills, Notice of, 116.
Bridges and Roofs, Wrought Iron, 72.
Bristow and WHITAKER, Messrs., on the
Formation of the Chesil Bank, 117.
British Conchology, or an Account of
the Mollusca which now Inhabit the
British Isles and Surrounding Seas,
79.
Brogpen, Mr., Comparative Merits of
Large and Small Trams for Colliery
Use, 267.
Index.
581
Broveuton, Mr., on the Cinchona, 258.
Brownine, J., Automatic Spectroscope,
390, 424, 523.
Change of Colour, 253.
sy Changes of Colour on Jupiter,
Spectrum Micrometer, 254.
ede Mr., Mines Regulation Bill,
Brusu, Prof., on Durangite, a New
Mineral, 126,
— on Hortonolite, 2 New Mineral,
126.
— Meteoric Stone, 126,
Bubbles of Mercury, 108.
Bucuwan, Mr., on the Mean Pressure of
the Atmosphere and the Prevailing
Winds over the Globe, 275.
Fi ae, Rainfall of South of Scotland,
16.
Bupp, J. P., on the Removal of Silicon
from Pig-Iron, 133.
Building, the Science of, 508.
Buu, Dr., Mistletoe on the Oak, 526.
BurcxuarD, P., Electrolytic Experi-
ments, 430.
Burmah, Stone Implements from, 514.
Burt, Mr., Action of Coloured Light on
the Mimosa Pudica, 285.
Buss, G., Caves of Gibraltar, 90.
ego ees Method of Odontology,
32.
C.
CamLLeret, L., Law of Compression of
Air, 569.
Cairns near Bangor, Opening, 384.
Calcining Kilns, 192.
Calcium and Zine, Alloy of, 531.
Calvarize, Ancient, 245, 247,
CaLveErt, Dr., Preparation of Nitrogen,
108.
CampBELL, D. J., on Polygamy, its In-
fluence in Determining Sex, and its
Effects on the Growth of Population,
248.
Campin, F., on the Principles and Con-
struction of Machinery, 406.
Canal, Suez, 110.
Cane, Mr., Formative Layer in Leaves
of Plants, 524.
Cannibalism in Namur, 384,
Carre, E., Influence of Heat on the
Delicacy of Spectrum Reactions, 567.
Carbonic Acid, Combustion of Magne-
sium in, 107.
Decomposition of, by Plants, 103.
Carboniferous Limestone, Geology of,
115.
582
Caron, H., on “ Rochage,”’ 567.
2 Alloy of Zine and Calcium,
531.
CarrincTon, Mr., Description of his
Observatory, 253.
Casting Metals under Pressure, 560.
Cavern of Bruniquel, 93.
Caves of Gibraltar, 90,
CayLey, Prof., on the Geometry of
Solar Eclipses, 393.
Cells in Living Bodies, Peregrinations
of, 437.
Cellulose, Solvent for, 261.
Cements, on, 113.
Cemetery at Frilford, Ancient, 386.
Cephaiopoda, Chief Groups of the, 116.
Cervide, New Genus of, 292.
Chalchihuitls, Mexican, 280.
Channel Islands, Megalithic Structures
of the, 149.
Pre-historic Monuments of the,
245,
Chatham Dockyard Extension, 535.
Island, Aborigines of, 248.
Cheesewring, threatened Destruction
of the, 516.
Chemical Climatology, 416.
— Works, Air Pollution by, 330.
ome Chronicles of, 105, 258, 398,
28.
Chesil Bank, Formation of the, 117.
Cuester, Rev. G., Shell Implements
and other Antiquities of Barbadoes,
245.
Cuevrier, M., Action of Vapour of
Sulphur on various Gases, 106.
Chloral, Hydrate of, 261.
—— the New Opiate, 575.
Preparation of, 108.
Chlorine and Sodium, 259.
Chlorophyll, Movements of, 256.
Chromatic Dispersion, Atmospheric, 97.
CHRONICLES OF SCIENCE :—
Agriculture, 87, 241, 376, 510.
Archeology (Pre-historic) and
Ethnology, 90, 244, 379, 512.
Astronomy, 94, 249, 389, 517.
Botany and Vegetable Physiology,
99, 254, 394, 524.
Chemistry, 105, 258, 398, 528.
Engineering, Civiland Mechanical,
110, 265, 402, 532.
Geology and Paleontology, 114,
269, 406, 537.
Meteorology, 120, 275, 413, 545.
Mineralogy, 124, 280, 417, 550.
Mining and Metallurgy, 128, 282,
420, 552.
Physics, Light, Heat, and Elec-
tricity, 134, 285, 424, 563.
Zoology and Animal Physiology,
139, 290, 431, 572.
Index.
| Oct.,
Cuurcu, Prof. A. H., a New Fluor-
escent Substance, 563.
Cilium, Moving Force of a, 436.
Cinchona, Cultivation of, 258, 400.
in the West Indies, 526.
CLaARgEE, C. B., Cultivation of Cinchona,
258.
CLELAND, J., Significance of the Cranial
Characters in Man, 143.
Cleveland, Metallurgical Industry of,
186.
Climate and Soil, Influence of, on
Plants, 254.
— Influence of Winds on, 276.
of Sitka, 122.
Climatology, Dove’s, 277.
Climbing Plants, 257.
Coal, Breaking Down, 132.
Mining, Theory and Practice of,
556.
Supply, Future, 284.
Coccoliths and Bathybius, 573.
Cotas, C., Electro-deposited Iron, 571.
Collodion Balloons, 401.
Combustion, Increase of Weight during,
137.
Comet of 1683, 393.
—— Discovery of a, 96.
— Winneceke’s, 523.
Comets, Theory of, 250.
Commensalism, 291.
Conchology, British,
Jefireys, F.R.S., 79.
Concrete, on, 113.
Conifers, Leaves of, 104.
Continental and English Intercom-
munication, 112.
Copal, Recent and Fossil, 397.
Corr, E. D., Extinct Batrachia and
Reptilia of North America, 116.
Copper, Depositing, on Paper, &ec., 139.
—— Extraction, 571.
—— Mining in England, 420.
Separating, 422.
Substitute for, in the Daniel
Battery, 430.
Corals, on Reef-building, 274.
Cornish Minerals, 419.
Corona, Mr. Seabroke on the, 522,
Observations on the, 94.
Spectrum Observations on the,
during Eclipse, 38.
and Zodiacal Light, 392.
Covumpary, M., Meteorological Service
in the Turkish Empire, 123.
Counter-pressure Steam-breaks, 268.
Courter, M., Manufacture of Fuclisine,
263.
Couret, M., Manufacture of Disulphide
of Carbon, 263. 2
Cranial Characters in Man, Significance
of, 148.
by J. Gwyn
1870. ]
Crookes, W., F.R.S., &c., Spiritualism
viewed by the Light of Modern
Science, 316.
-— a Recent Triumph of Synthetical
Chemistry, 360.
— on the Total Solar Eclipse of
August, 1869, 28.
Cuckoo’s Eggs, 142.
Cyclone, Origin of a, 121.
Cyclopzedic Science simplified, 85.
D.
Daxyns, J. R., Geology of North
Derbyshire and Yorkshire, 115.
Danish Element in the Population of
Cleveland, 384.
Danvers, F. C., on the Survey of India,
448.
Dardistan, Visit to, 247.
Dartmoor, Pre-historic Monuments of,
516.
Darwt1y, Mr., and the French Academy,
O74.
Davsré on Tinning Iron, 571.
Davipson, Mr., on Brachiopoda, 274.
Davis, Dr. B., and E. A. Wetcn, on the
Aborigines of Chatham Island, 248.
Dawsins, B., Antiquity of the Tron
Mines of the Weald, 92.
—— Flint Flakes and Flakes of Chert,
246.
Daylight, Chemical Intensity of, 425.
DeueEratn, P. P., on the Evaporation
of Water and Decomposition of Car-
bonic Acid by Plants, 103.
De wa Rive, Prof., Magnetic Rotatory
Power of Liquids, 569.
Dexavrier, M., Concentrating and
Utilizing the Heat from the Sun,
138.
De.timAN, Dr., Electricity of Clouds,
415.
De rrno, Prof., on the Relation between
the Distribution of Plants and of
Animals, 255.
Demayes, Dr., Electro-magnetic Appa-
ratus, 570.
De Mortuis, by H. Woodward, 341.
De Rance, C.E., Geology of Lake Dis-
trict, 118.
Des Crotseaux, M., Crystals of Gado-
linite, 127.
—— Optical Properties of Benzyl,
564.
DersHayes, M., Award of the Wollaston
Gold Medal to, 275.
Devittze, H. Sre. Criame-, Oxygen
Dissolved on Fusion of Platinum,
287.
— Reactions of Iron and Steam, 566.
Index.
583
Devonshire Association for the Advance-
ment of Science, 497.
D’Hercourt, G., on Salt in the Atmo-
sphere of Monaco, 262.
Diamagnetism, Tyndall on, 501.
Diamond, Researches on the, 426.
Diamonds, Discovery of, 282.
Origin of, 124.
Diatom Markings, 144.
Dinornis Contemporary with Man, 244.
Dinosauria, Prof. Huxley on, 273.
Dises of Stars, Measuring, 98.
Disinfectant, a New, 260.
Dispersion, Atmospheric Chromatic,
9
Dotrus-GaLiine, M., Manufacture of
Albumen, 105.
Double Star a Centauri, 522.
Dove, Prof., Klimatologische Beitrage,
277.
Draper, H, N., Ether as an Intoxicant,
260.
Drought of 1870, 510.
Ducuartre, M., Turning of Plants
towards the Light, 395.
Duckweed, Hibernation of, 102.
Duncan, Dr., on Corals, 270.
— on the Geography of Western
Europe during the Mesozoic and
Cainozoic Periods, 274.
— P.M., F.R.S., on Idiocy, 49,
on Insanity, 165.
Durangite, a New Mineral, 126.
E.
Earth, Fuller’s, in the South-West of
England, 68.
Earth’s Crust, Determining Thickness
of, 539;
Ecxuarp, Prof., on the Secretory Nerve
of the Parotid Gland, 141.
Eclipse, Approaching Total Solar, 389,
477, 517, 519.
— of August 7, 1869, the “ Anvil”
Protuberance, 443.
—— of Moon, 97.
—— Observations, on the American,
249,
—— Prominences, Spectroscopic Notes
on the, 34, 39.
— of Sun, of December 24th, 1870,
389, 477, 517, 519.
—— of the Sun, Partial, 97.
— Total, of the Sun, of August, 1869,
94,
oe Solar, of August, 1869, on
the. By W. Crookes, F.R.S., 28.
Eclipses, Geometry of Solar, 393.
— Records of Chinese, 253.
Edible Fungi, 99.
084
Eeerton, Sir Partie, Two New Species
of Gyrodus, 119.
Eiecrrtz, M., on Sulphur in Iron and
Steel, 259.
Eges, Cuckoo’s, 142.
Electric Currents in Muscle, 291.
—— Spark, Duration of, 570.
Figures, 570.
Electrical Decomposition of Water with
Silver Poles, 138.
Electricity, Atmospheric, and Recent
Phenomena of Refraction, 229.
—— — at Haiti, 288.
— Chronicles of, 138, 288, 429, 563.
in Plant Life, 525.
of Clouds, 415.
Electrification of Wine, 430.
Electro-Capillary Action, 570.
Electrolytic Experiments, 430.
Electro-magnetic Apparatus, 570.
Electro-motive Forces, on, 431.
Electroscopic Experiments, Cause of
Error in, 429.
Exincton, J., Copper Extraction, 571.
Emerald, Colouring Matter of the, 417.
EmmeEr.inc, Dr., Action of Water on
Glass and Porcelain, 106.
Encetmann, Dr. Th., on the Develop-
ment of Gas in Protoplasm, 140.
Engineering, Chronicles of, 110, 265,
402, 532.
— New York, Society of Practical,
113.
English and Continental Intercommu-
nication, 112.
Epiboulangerite, 282.
Erosion, Intra-glacial, near Norwich,
120.
Esmarkite, 418.
Ether as an Intoxicant, 260.
Ethnology of Great Britain, 385.
Exhaustion of Soils, 378.
Explosive Powder, New, 129.
Hye-piece, New, 253.
¥,
Farabay, his Life and Letters, 232.
Favre, M., Occlusion of Hydrogen by
Palladium, 105.
Fem, Mr., on Heavy Flint Glass, 286.
Felspars, Constitution of, 417.
Fermentation, Pasteur’s Views on, 291.
Ferns, Fertilization of, 395.
Fertilization, Cross, 394.
—— of Ferns, 395.
of Winter Flowering Plants, 100.
Festiniog Railway, 265.
Fibrin of the Blood, Origin of the, 139.
Fixed Stars, Distances of the, 252.
Flame, Examination of, 135, 567.
Index.
[ Oct.
‘Flint Chips” By EH. T. Stevens, 379.
Flakes in Somerset, 246.
— Glass, Heavy, 286.
—— Implements, 383.
—— —— in the Drift of Norfolk and
Suffolk, 120.
Flora, Arctic, 101.
Fossil, 406.
of Iceland, 255.
of Round Island, Mauritius, 256.
Fiower, J. W., Flint Implements in the
Drift of Norfolk and Suffolk, 120.
Flowers, Change in Colour of, 525.
Fluids in Crystals, Determination of,
by Spectrum Analysis, 125.
Fluor Spar, &c., Reflexion of Heat from,
138.
Fluorescent Substance, New, 563.
Fluorine, Organic Compounds of, 528.
Forpss on Volcanoes, 538.
Forest, Petrified, near Cairo, 540.
Submerged, at Blackpool, 93.
Forestry, French Imperial School of, 60.
Formic Acid, Synthesis of, 400.
Fostrr, C. Li Nerves, Geology of North
Derbyshire and Yorkshire, 115.
Fow.err, Mr., Manufacture of Oxygen,
107.
Fox, Col. L., Opening Cairns near
Bangor, 384.
D. M., on the San Paulo Railway,
404.
FREEDEN, Herr Von, ‘ Norddeutsche
Seewarte ’ for 1869, 278.
— Weather Calendar for North-West
Germany, 122.
French Imperial School of Forestry, 60.
FRiepet and Laprnsure, Drs., Organic
Compounds of Silicium, 528.
Frilford, Ancient Cemetery at, 386.
Fuchsine, Manufacture of, 263.
Fuller’s-earth in the South-West of Eng-
land, 68.
Fungi, Alternation of Generation in, 257.
Edible, 99.
—— Parasitic, 397.
G.
Gadolinite, Crystals of, 127.
GatFFE, M., Electro-plating with Nickel,
289.
Gaize, Uses of the Mineral, 567.
Galvanic Batteries, Improved, 571.
Battery, Leclanché, 288.
Zaliwski’s, 288.
Ganoid Fish, from Australia, 431.
Gardens (English), Foreign {Trees and
Plants for, 350.
Gasin Protoplasm, Development of, 140,
Lighting Mines with, 131.
1870.]
Gas Supply of Berlin, 287.
Gases, Occlusion of, 431.
GEISSLER and VoGELsanG, MM., Deter-
mination of Fluids in Crystals by
means of Spectrum Analysis, 125.
Gelatin, Magic-lantern Pictures on, 564.
Generation, Alternation of, in Fungi,
257.
Geography of Western Europeduring the
Mesozoic and Cainozoie Periods, 274.
Geological Change, the Rate ef, 322.
Memoirs, 409.
Survey, Memoirs of the, 114.
Geology and Revelation, 238.
— Chronicles of, 114, 269, 405, 537.
— of Country around Shelve (Shrop-
shire), 116.
Gerorces, M., Preservation of Meat, 261.
Gibraltar, Caves of, 90.
Gitman, W. S., on the “Anvil” Pro-
tuberance of the Eclipse of August 7,
1869, 443.
GrrarD, J., Colour of the Sea, 564.
GuaisHER, Mr., on the Rainfall of Green-
wich, 416.
Glass, Action of Light on, 286.
Action of Water on, 106.
Coloration of, by Sunlight, 134.
Glaucopyrite, on, 418.
Gold, Depositing, on Paper, &c., 139.
Gold-fields of Nova Scotia, 421.
Gold from Victoria, 130.
Production of, in Australasia, 130.
GoprrerT, Dr., on the Origin of Dia-
monds, 124.
Gor, G., F.R.S., Practical Scientific
Instruction, 215.
Green, A. H., Geology of North Derby-
shire and Yorkshire, 115.
Greenland, Lichens of, 102.
Gruner, L., on Phosphorus in Steel,
898.
Guy, Dr., Melting and Subliming Tem-
peratures of Poisons, 426.
Gyrodus, two New Species of, 119.
H.
Haast, Dr., on the Contemporaneity of
the Dinornis and Man, 244.
on some Stone Implements in New
Zealand, 245.
Habit and Intelligence in connection
with the Laws of Matter and Force,
73.
Harcket, E., Zoological Position of
Sponges, 432.
Hail-stones, Crystallized, 122.
Haiti, Atmospheric Electricity at, 288.
Hangury, D., New Species of Jalap,
398.
Index.
585
Hany, Dr. J., on the Climate of the
Alps, 413.
— on the Winds of the Northern
Hemisphere and their Influence on
Climate, 276.
Relation of Temperature to Sea-
level, 428.
Harmer, F. W., and S. V. Woop, on
Intra-glacial Erosion, 120.
Harrison, J. T., on Railway Expen-
diture and Income, 267.
Heat, Apparent Paradox on, 136.
—— Chronicles of, 135, 287, 426, 563.
—— Emission of, from the Moon, 138.
of Sun, Concentrating, 138.
of Union of Carbon, Boron, and
Silicon with Oxygen, 287.
re nae of, from Fluor Spar, &c.,
—— Relation of, to Work in Human
Body, 290.
Herbarium of the British Museum, 527.
Hermann, Prof., Absence of Currents
in Uninjured Inactive Muscle, 291.
cae a Sir J., on the Solar Spots,
OL.
Lieut., on Dark Objects crossing
the Solar Dise, 392.
Secs on the November Meteors,
Herynstvs, Dr., Origin of the Fibrin of
the Blood, 139.
Hibernation of Duckweed, 102.
Hippopotamus major, Molars of, in Kent's
Cavern, 93.
Hodgson’s Wire Tramway, 404.
Hormann, Dr., Increase of Weight
during Combustion, 137.
Holborn Viaduct, 112.
Homes, M., on Rotatory Storms, 121.
Home Island, Vegetation of, 101.
Homogeny and Homoplasy, 576.
Hopkins, Mr., Determining Thickness
of Earth’s Crust, 539.
Horsrorp, Prof. Free Hydrochloric
Acid in the Stomach, 140.
Hortonolite, a New Mineral, 126.
ree M. A., on Oxygenated Water,
98.
Houxxe, J. W., F.B.S., Fossil Remains
of Saurians, 119.
Hutt, E., F.R.S., on the Triassic and
Permian Rocks of the Midland
Counties of England, 114.
Recent Observations on Under-
ground Temperature, on the Causes
of Variation in Different Localities,
207.
Houxtey, Prof., Modifications of Man-
kind, 516.
on the Ancient Relations of Land
and Water, 411.
586
Hvx.ey, Prof., on Dinosauria, 273.
— on the Ethnology of Great Britain,
385.
Hydraulic Machines for breaking down
Coal, 132. ve
Hydrochloric Acid, free, in the Stomach,
140.
Hydrogen, Occlusion of, by Palladium,
105.
— Peroxide of, 399.
Phenomena during the Combus-
tion of, 137.
Hydrogenium Amalgam, 529.
-——— Dr. Loew on, 400.
Hypophosphoric Acid, Use of, in Agri-
culture, 261.
cL
Ice in India, Production of, 427.
Iceland, Flora of, 255.
Ichthyodorulites, on two New, 118.
Idiocy, on, by P. M. Duncan, F.RS.,
4
9.
India, Rainfall of, 546.
—— Surveys of, 448, 458.
Insanity, on, 165.
Intercommunication, English and Con-
tinental, 112.
Iodide of Potassium, Decomposition of,
in the Light, 135.
Tron and Steam, Reactions between,
566.
—— and Steel Institute, 561.
—— —— Patents for Manufacture of,
423,
Sulphur in, 259.
clad Ships, their Qualities, Per-
formances, and Cost, 269.
Electro-deposited, 571.
— making, Stages of, 186.
—— Mines of the Weald, Antiquity of
the, 92.
— Purification of, 557, 558.
—— Pyrites of Piedmont and Elba,
281.
Removal of Silicon from, 133.
Irrigation, Sewage, Principles
Methods of, 17.
Isinglass, on, 399.
Isoclase, New Mineral, 551.
and
J.
JAcKsON, J. W., on the Germination of
Palms, 524.
Jacor, Dr., on the Natives of Naga,
247.
Jalap, New Species of, 398.
JANSSEN, Dr., Production of Ice in
India, 427.
Index.
| Oct.,
Japan, Coal in, 554.
Japanese Sea-weeds, 105.
JEFFREYS, J. Gwyn, F.R.S., British
Conchology, 79.
JENKINS, H. M., the Rate of Geological
Change, 322.
JouNsTONE, K., Handbook of Physical
Geography, 276.
Jones, Dr. H. Bence, F.B.S., Life and
Letters of Faraday, 232.
JOUGLET, A., Waterproofing
261.
—— on Explosions caused by Ozone,
9
Paper,
Jourpary, M., Inritability of Stamens,
396.
Jupiter, 97.
—— Changes of Colour on, 253, 393.
—— Visibility of, 251.
K.
Kent's Cavern, Literature of, 93.
Kernier, M., on the Influence of
Climate and Soil on Plants, 254.
KessLeER, M., Combustion of Magnesium
in Carbonic Acid, 107.
Kilns, Calcining, 192.
Kine, W. R., Aboriginal Tribes of the
Nilgiri Hills, 386.
Kirk, D., on Recent and Fossil Copal,
397.
Kirxwoop, Prof., on Meteors, 391.
Kitai, Account of the Race, 246.
Kitchen Middens, Ancient, in the
Andaman Islands, 383.
Knitting Machine, 536.
Kosei, Von, on a New Mica, 127.
Kose, H., Increase of Weight by
Burning Bodies, 568.
Koords and Armenians, Account of the,
245.
Kosmann, on Apatite, 281.
KowaA.eEvsky on the Kinship of Verte-
brates and the Ascidian Molluscs,
142.
Kress, G., Preparation of Oxygen, 529.
L.
Labiatex, Peloria in, 104.
Laboratories in Amsterdam and London,
438.
Labyrinthodont, a New, 539.
LaLLemMAnD, M., Action of Sunlight on
Sulphur, 285.
Land and Water, Ancient Relations of,
411.
LaNKESFER, E. R., on Comparative
Longevity, 373.
1870.]
LANKESTER, Ray, Machairodusin Forest
Beds of Norfolk, 118.
—R., on the Cephalaspidee of the
Old Red Sandstone, 270.
Spermatophores in Annelids, 434.
Larpiay, J. W., Pre-historic Dwelling
on the Coast of Haddingtonshire,
382.
Larret, E., Reliquizse Aquitanice, 381.
Lawes, Mr., on Exhaustion of Soils,
378.
Waste of Food during Respira-
tion, 377.
Lead, Desilvering, 560.
Native, in Metaphyre, 124.
in Victoria, 124.
Leaves of Conifers, 104. ;
of Plants, Formative Layer in, 524.
Scorching, by Wind, 105.
Variegation of, 257.
—— Viridescence of, 104.
Lr CuaTecier’s Plan of Using Counter-
pressure Steam as a Break, 268.
LeEcLANCHE Battery, 288.
Leitner, Dr., Visit to Dardistan, and
Account of the Shina Race, 247.
Lenz, R., Occlusion of Gases by Metals,
431.
LEONARDO DA VINCI as a Botanist, 100.
Ler Svrcr, Mr., Phenomena of Star 7
Argus, 390.
Lerverrrier’s‘ Atlas Météorologique, 123.
Prof., Dismissal of, 249.
Levison, W. P., Improved Galvanic
Batteries, 571.
Lévy, P., on Climbing Plants, 257.
Lewatp, P., Action of Cold on Tin,
569.
Lichens of Greenland, 102.
Liesic, Prof., on Pasteur’s Views on
Fermentation, 291.
Life-buoys, illuminated, 426.
Light and Sound, an Examination of
their Reputed Analogy, by W. F.
Barrett, 1.
—— Chronicles of, 134, 285, 424, 563.
Coloured, Action of, on Mimosa
Pudica, 285.
Decomposition of Iodide of Potas-
sium by, 135.
New Artificial, 286, 563.
—— of Coal Gas, relation of, to Volume
consumed, 286.
— on Glass, Action of, 286.
— Turning of Plants towards, 395.
Lighting Mines, 131.
Limes and Cements, on, 113.
Liquids, Bumping of Boiling, 136.
Lithology and Mineralogy, 82.
Liver, Endings of Nerves in the, 141.
Lockyer, Mr., on the American Eclipse
Observations, 249.
VOL. VII.
—_—_——
Index.
587
Loew, O., Action of Light on Sulphur-
ous Acid, 564,
on Hydrogenium, 400.
on Hydrogenium Amalgam, 529.
Longevity, Comparative, 373.
Looking-glasses, Platinizing, 262.
Lussock, Sir J., on Savages, 505.
Lucas and Cazrn, on the Duration of
the Electric Spark, 570.
Lunar Crater Plato, 394.
M.
Machairodus on Forest Beds of Norfolk,
118
Madacasses Race, Affinities of the, 247.
Madder Colours, 531.
Root, Sugar in, 260.
Magne-crystallic Action, Tyndall on,
501
Magnesium, Combustion of, in Carbonic
Acid, 107.
Magnetic Rotatory Power of Liquids,
569.
Maaenus, G., on Reflexion of Heat from
Fluor Spar, &c., 138.
Malta, Water Supply of, 546.
Man, Cranial Characters in, 143.
Pre-historic, Remains of, in Ar-
gyleshire, 246.
Manganese in Milk, 530.
Manure Adulteration, 242.
Manures, Falsification of, 376.
MarcuanpD, M., on Scorching of Leaves
by Wind, 105.
Marry, Dr., Movements of Wings in
Flight, 436.
Marriages, Consanguineous, 385.
Martin, M., Use of Hypophosphoric
Acid in Agriculture, 261.
Martius, Dr., Preparation of Chloral,
108.
Masters, Maxwetu J., Vegetable Tera-
tology; an Account of the Principal
Deviations from the usual Construc-
tion of Plants, 84.
Mavment, E. J., Optically Neutral
Sugar, 564.
Meat, Preservation of, 261.
Meena, T., on the Leaves of Conifers,
104.
Meenas of Central India, 516.
Megalithic Structures of the Channel
Islands, 149.
Melaplhiyre, Native Lead in, 124.
MENDELSSOHN-BarrHoLpDy, M., Prepara-
tion of Chloral, 108.
Mercury, Bubbles of, Floating on Water,
108.
“Mere,” the, a New Zealand Weapon,
245,
a
588
Metallurgical Industry of Cleveland,
186.
Metallurgy, Chronicles of, 128, 282, 420,
d02.
Meteoric Stone, on a, 126.
Meteorite, Fall of a, 419.
Meteorites, Analysis of, 280.
in India, 551.
Meteorological Instruments, Self-record-
ing, Results of, 122.
Memoirs in France, 123.
—— Office, Weather Report of, 545.
—— Servicein the Turkish Empire, 123.
Meteorology, Chronicles of, 120, 275,
413, 545.
of North-West Europe in 1868, 123.
Progress of, in France, 278.
Meteors, 391.
November, 96.
Mexican Chalchihuitls, 280.
Mica, a New, 127.
for Furnace Doors, 287.
Micrometer, Spectrum, 254.
Microscope, Graduating Diaphragm for,
425.
—— Mechanical Finger for the, 565.
Milky Way, New Theory of the, 253.
Mitarvet, M., on the Sensitiveness of
the Mimosa, 396.
MiLiincen, Major, on Negro Slaves in
Turkey, 248.
Millstone Grit, Geology of, 115.
Mimosa, Sensitiveness of the, 396.
Mineral Statistics of the United King-
dom, 128.
Veins of Country around Shelve
(Shropshire), 116.
Mineralogy and Lithology, 82.
Chronicles of, 124, 280, 417, 550.
Mines Regulation Bill, 212, 420, 952.
Mining, Chronicles of, 128, 282, 420,
592.
——,, Legislature on, 282.
—— Operations at Dudley, 554.
Mistletoe on the Oak, 526.
Mitrailleur, the, 532.
Monn, Prof.,on Sea Temperatures, 415.
Mo toy, Rev. G., Geology and Revela-
tion; or, the Ancient History of the
Earth considered in the Light of
Geological Facts and Revealed Re-
ligion, 238.
Molluscs, Ascidian, Kinship of Verte-
brates and, 142.
Monaco, Atmosphere of, Salt in, 262.
Monxman, C., Archeological Disco-
veries in Yorkshire, 247.
Moon, Eclipse of, 97.
Emission of Heat from the, 138.
Heat from, 287.
Morphology, Chronicles of, 142, 290,
431, 572,
Index.
[ Oct.,
Bate taek M. E., Variegation of Leaves,
ie
Variegation and Double Flower-
ing, 396.
Researches on the Diamond, 426.
Mortars, on, 113.
Morton, G. H., Geology and Mineral
Veins of Country around Shelve
(Shropshire), 116.
: rik Manufacture of Oxygen Gas,
64,
Miter, Dr, H., F.R.S., Preventing the
Bumping of Liquids, 136.
M., on Hydrate of Chloral, 261.
Mvre, Cuamonp, and Guirre, MM.,
Thermo-electric Apparatus, 288.
Murruy, J. J., Habit and Intelligence
in their Connection with the Laws of
Matter and Force, 75.
Muscles, Starch in, 141.
Ni
Nadorite, Analysis of, 551.
Naga (Philippine Islands), Natives of,
247
Naphthaline, Utilization of, 259.
Nass, M., Starch in Muscles, 141.
Naupry, M., Acclimatization of Palm
Trees, 397.
Nebule, Distribution of the, 98.
Needles, Ancient, 381.
Negro Slaves in Turkey, 248.
Neptune, Spectrum of, 286.
Nerves, Endings of, in Liver, 141.
Trophic, 200.
Ness, W., on the Coal-field of Fife, 284.
Newman, M., Rendering Woven Tissues
Impermeable to Water, 107.
Prof., on Cuckoo’s Eggs, 142.
New York Society of Practical En-
gineering, 113.
New Zealand Weapon, 245.
Nickel, Electro-plating with, 288.
NickiEs, M., Preparation of Caustic
Baryta, 109.
Nitrogen, Preparations of, 108.
Noste, Capt., on Planet Venus, 393. -
Nova Scotia, Gold-fields of, 421.
Minerals of, 419.
Norsey, P. F., on English and Conti-
nental Intercommunication, 112.
O.
Ocean, Surface Life of the, 435.
Odontology, Graphic Method in, 482.
O«uE, Dr., on Cross-fertilization, 394.
OnRESsER and SeputcHre, MM., Utili-
zation of Blast-furnace Slag, 260.
1870.]
Oldhamite, 281.
O.rver, Lieut. S. P., on the Megalithic
Structures of the Channel Islands,
149.
Oprert, Dr., Description of the Kitai,
246,
ORIGINAL ARTICLES :—
Light and Sound; an Examination
of their Reputed Analogy. By
W. F. Barrett, F.CS., 1.
On the Principles and Methods of
Sewage Irrigation, 17.
The Total Solar Eclipse of August,
1869. By William Crookes,
F.RS., &e., 28.
Instruction in Science for Women,
On Idiocy. By P. Martin Duncan,
E.RS., 49.
The French Imperial School of
Forestry. By A. Pengelly, B.A.,
60
The Fuller’s Earth in the South-
West of England. By R. Tate,
F.GS., 68.
Megalithic Structures of the Chan-
nel Islands, their History and
Analogues. By Lieut. S. P.
Oliver, 149.
On Insanity. By P. Martin Dun-
can, F.R.S., &c., 155.
The Metallurgical Industry of
Cleveland, 186.
On “ Trophic Nerves.” By G. Rol-
leston, F.R.S., 200.
Recent Observations on Under-
ground Temperature, or the
Cause of Variation in Different
Localities. By E. Hull, F.R.S.,
207.
Mr. Bruce’s Mines Regulation Bill,
212
On Practical Scientific Instruction.
By G. Gore, F.R.S., 215.
Atmospheric Electricity and Re-
cent Phenomena of Refraction.
By S. Barber, 229.
Beer Scientifically and Socially
Considered. By J. Samuelson,
299.
Spiritualism Viewed by the Light
of Modern Science. By William
Crookes, F.R.S., &., 316.
The Rate of Geological Change.
By H. M. Jenkins, 322.
Air Pollution by Chemical Works,
330.
De Mortuis. By H. Woodward,
341.
Foreign Trees and Plants for Eng-
lish Gardens. By A. W. Bennett,
390.
Index.
589
ORIGINAL ARTICLES—continued,
A Recent Triumph of Synthetical
Chemistry. By William Crookes,
E.BS., &e., 360.
The Eclipse of August 7, 1869,
“Anvil” Protuberance. By
W. S. Gilman, jun., 443.
The Surveys of India. II. The
- Trigonometrical Survey (with a
Sketch-map). By F.C. Danvers,
A.I.C E., 448.
The Geological Survey of India
(with a Sketch-map). By H.
Woodward, F.G.S., 458.
Rainfall in England. By W. Pen-
gelly, F.R.S., 467.
The Approaching Total Solar
Eclipse. By R. A. Proctor,
F.R.AS., 477.
The Controversy on Spontaneous
Generation; with Recent Expe-
riments. By J. Samuelson, 484.
The Devonshire Association for the
Advancement of Science, Litera-
ture, and Art, 497.
Osbornite, 281.
Other Worlds than Ours, 367.
Ort, Dr., on the Preservation of Timber,
263.
—— Utilization of Naphthaline, 259.
OweEN, Prof., on the Lias Pterosauria
and on Cetacean Remains, 271.
on Two New Ichthyodorulites,
118.
OxuanpD, Mr., Calcining Tin Ores, 423.
Oxygen Gas, Manufacture of, 107, 264,
529, 563.
Oxygenated Water, 398.
Ozone, Explosions caused by, 399, 529.
Formation of, by Combustion, 566.
—— Testing for, 155.
P.
Paring, Mr., on the Total Eclipse of
1869, 251.
Paleocoryne, on, 407.
Paleontographical Society, Monographs
of, 269.
Paleontology, Chronicles of, 114, 269,
406, 537.
Palladium, Occlusion of Hydrogen by,
105.
Palm Trees, Acclimatization of, 397.
Palms, Germination of, 524.
Paper, Electro-deposition of Copper,
Silver, and Gold on, 139.
Paquet, M., on Oil of Thymol, a New
Disinfectant, 260.
Parotid Gland, Secretory Nerve of the,
141.
oR o,
590
Patterson, Mr., on Collodion Balloons,
401.
‘* Pattoo-Pattoo,” a New Zealand Wea-
pon, 245.
Pav, M., on Hydrate of Chloral, 261.
Peloria in Labiate, 104.
PencELLY, A., The French Imperial
School of Forestry, 60.
—— Mr,, Literature of Kent’s Cavern,
—— W., Rainfall in England, 467.
Peprer, J. H., Cyclopzdic Science
simplified, 85.
Permanent Way, Single Rail, 403.
Permian and Triassic Rocks of the
Midland Counties, 114.
Perseus, the Cluster in, 97.
Peru, Primeval Monuments of, 512.
PrErerseN, Herr, Autimonial Sulphide
of Silver, 125.
PETTENKOFFER, Prof., on the Relation
of Heat to Work in the Human Body,
290.
on the Evaporation of Water from
Plants, 524.
Pettigrew, Dr., Movements of Wings
in Flight, 436.
PeyritscH, J., on Peloria in Labiate,
104.
Priucer, Prof., on the Endings of
Nerves in the Liver, 141.
Putirp, Carbo-oxygen Light, 563.
Puitires, Prof. J., Career of, 537.
on the Oxford Clay Belemnites,
270.
Pholas-burrows in the Ormes Head,
118.
Phosphorus in Steel, 398.
Phosphuretted Hydrogen, 106.
Photographie Operations during Total
Solar Eclipse of August, 1869, 40.
Physical Observatory at St. Petersburg,
122.
Physics, Chronicles of, 134, 285, 424,
563
Physiology, Animal, and Morphology,
Chronicles of, 139, 290, 431, 572.
— in Trinity College, Cambridge,
7.
—— Vegetable, Chronicles of, 99, 254,
394, 524.
Picort, Dr. R., on Podura Scale Mark-
ings, 144.
Prat, Dr. O., the Cluster in Perseus, 97.
Prre, L. O., on the Psychica]l Elements
of Religion, 247.
Plants, Acclimatization of Half-hardy,
" 200.
—— and Animals, Distribution of, 255.
—— Climbing, 257.
Deviations from the usual Con-
struction of, 84.
Index.
[ Oct.
Plants, Evaporation of Water and De-
composition of Carbonic Acid by, 103.
—— Fertilization of Winter Flowering,
100.
a: Influence of Soil and Climate on,
254.
—— Mimetic, 397.
Variegation and Double Flowering
of, 396.
Platinizing Looking-glasses, 262.
Platinum, fused, Oxygen dissolved by,
287.
Piummer, Mr., on the Comet of 1683,
393.
Pneumatic Stamps, 131, 555.
Podura-scale Markings, 144.
Poisoning by CEnanthe Crocata, 526.
Poisons, Melting and Subliming Tem-
peratures of, 426.
Potxacci, E., Manganese in Milk, 530.
Polyargyrite, New Silver Ore, 126.
Polygamy, its Influence in Determining
_ Sex and its Effects on the Growth of
Population, 248.
Porcelain, Action of Water on, 106.
PoseLcEeR, M., Damage to Trees, 107.
Potash, Extraction of, from Suint, 260.
Powe.t, Mr., on the Double Star a
Centauri, 522.
Prairie Vegetation, 527.
Precious Stones, Handbook of, 81.
Pre-historic Archeology, 244.
International Congress of, 90.
Dwelling on Coast of Haddington-
shire, 382.
Pressure, Mean, of Atmosphere and
Prevailing Winds over the Globe,
275.
Pritiievx, M., on the Movements of
Chlorophyll, 256.
on the Viridescence of Leaves, 104.
Proceedings of the Metropolitan Learned
Societies :—
Anthropological, 247, 385, 517.
Astronomical (Royal), 97, 251, 392,
520.
Ethnological, 245, 384, 516.
Geological, 119, 272, 542.
Institution of Civil Engineers, 112,
266, 404.
—— Mechanical Engineers, 268,
405, 536.
Proctor, R. A., the Approaching Total
Solar Eclipse, 477.
on the Corona and Zodiacal Light,
392.
—— on the Distribution of the Nebule,
98.
— on Measuring the Discs of Stars,
8
—— New Theory of the Milky Way,
253.
1870.]
Proctor, R. A., Other Worlds than
Ours, 367.
— on Star-drift, 251.
— on the Sun’s Motion in Space, and
on the Relative Distances of the Fixed
Stars of various Magnitudes, 252.
— Transit of Venus, 97, 253.
Prominences, Eclipse, Spectroscopic
Notes on the, 34, 39.
Protoplasm, Development of Gas in, 140.
Pseudomorphs, on, 127.
Pyrometer, Novel, 428.
Q.
Quartz, Artificially Crystallized, 125.
R.
Rabdionite, New Mineral, 551.
Railway Accidents and Means of Pre-
venting, 113.
—— Expenditure and Income, 267.
—— Festiniog, 265.
San Paulo, 404.
Railways, Light, 265.
Rainfall in England, 467.
of Greenwich, 416.
of South of Scotland, 416.
RAMMELSBERG, Dr., on Axinite, 127.
M., on Gadolinite, 282.
Ranxine, W. J. M., Inaugural Address
before the Institution of Engineers in
Scotland, 268.
Rave, J. B., on Diatom Markings and
Podura-scale Markings, 144.
Red Rain, Falls of, 547.
Redruthite, 117.
Reep, E. J., Our Iron-clad Ships: their
Qualities, Performances, and Cost, 269.
Refraction, Recent Phenomena of, and
Atmospheric Electricity, 229.
Ren, H., ‘A Practical Treatise on Con-
crete, and how to make it; with Ob-
servations on the Uses of Cements,
Limes, and Mortars,’ 113.
Reimann, Dr., on Albolith, 399.
Religion, Psychical Elements of, 247.
‘ Relique Aquitanice,’ 381.
Repertorium fiir Meteorologie, 278.
Reptilia and Batrachia, Extinct, of
North America, 116.
Resolvability of Star Groups, 521.
Respiration, Waste of Food during, 377.
Reviews oF RECENT SCIENTIFIC WoRKS.
‘ Wrought-iron Bridges and Roofs,’
By W. C. Unwin, 72.
‘Habit and Intelligence, in their
Connection with the Laws of
Matter and Force.