The potash salt crystallizes in quadrilateral prisms, needles

or plates, and is not deliquescent. The soda salt has similar

characters, and the ammonia salt crystallizes in needles. These salts

abundantly precipitate the acetate and muriate of iron of a red brown

colour; they precipitate sulphate and nitrate of zinc white; muriate

of manganese slightly of a clear brown colour; barytic and strontian

salts abundantly white; being mixed with strong solutions of muriate

or acetate of lime, they gradually produce an acicular crystalline

white precipitate; acetate of silver yields an abundant white

precipitate, which does not change colour in less than twenty-four

hours: they do not precipitate salts of glucina, magnesia, alumine,

uranium, nickel, copper, cobalt, gold or platina. This substance has

been named the lichenic acid, and is distinguished from boletic acid

by the different character of its vapour, and by forming an insoluble

salt with baryta.—_Bull. Univ._ A. viii. 270.

FOOTNOTE:

[133] About one hundred and twenty grains.

34. _Remarks on the Preparation of M. Gautier’s Ferro-prussiate

[p485] of Potash, as described in this Journal for_ July,

1827.[134]—It is stated in the above article, “numerous

investigations induced M. Gautier to conclude that when animal

matter is calcined alone, it yields but little cyanogen; that when

mixed with potash it gives more; that the _substitution of nitre_

for potash, and the addition of iron or scales of iron, augmented

the production of cyanogen and gave a ferro-prussiate. The following

is the process of manufacture to which M. Gautier has ultimately

arrived,” (for which see the Journal, 227.)

M. Gautier giving the proportions of materials, directs—

Blood in a dry state 3 parts

Nitre 1 "

Iron scales 1/50 of the blood employed.

Blood not being at hand, animal muscular fibre was substituted,

and the following results were obtained. I am not aware that the

dried parts of animal muscular fibre are more inflammable than the

coagulated and dried parts of blood:—

Muscular fibre 3 parts

Nitre 1 "

Iron filings 1/50 of the undried muscle employed.

The muscular fibre, nitre and iron filings were beat into a mass, and

partially dried by a moderate heat; they were then returned to the

mortar and reduced to a perfectly homogeneous greyish white powder.

This was dried and weighed, and appeared to be reduced to nearly

equal parts of nitrate of potash and animal fibre.

The desiccation having completed by a very moderate heat on a sand

bath, will not, as far as I am aware, differ materially from that

produced by exposing the mass in “an airy situation to dry,” as

nitrate of potash undergoes no decomposition by admixture with animal

matters at a low temperature.

When the desiccation was completed, the mixture was charged into an

iron cylinder, placed in the sand-bath, and though combustion was

not anticipated in this part of the process, yet the mouth of the

cylinder was turned towards the wall, lest an accident should occur,

(which appeared to me to be more than probable in some stage of the

process.) In about two hours after the cylinder had been heated, I

was surprised to see its contents ejected with considerable force,

in a state of brilliant combustion. Supposing something in the above

experiment had been overlooked, and that, if the materials had

been longer in contact previously to subjecting them to complete

desiccation, this inflammation would not have taken place, the

experiment was repeated with the following precautions: after the

muscular fibre had been subjected to the action of the pestle in

combination with the prescribed quantity of nitrate of potash, the

mass was boiled with water for some hours, and then gently evaporated

to dryness; even now, by applying a piece of red-hot charcoal, it was

found that the nitre was in a condition to enter [p486] into active

combustion, and if the cylinder had been again charged and subjected

to a temperature capable of producing ignition, there cannot be a

doubt, but that a similar inflammation would have taken place.

However this might be, this quantity of material was now mixed

with hydrate of potash to an equal weight with the nitre used; and

the mass subjected to the heat of a sand-bath for some hours, and

afterwards submitted to the action of a naked fire for rather more

than an hour, and the heat brought up to redness. No considerable

action took place, but some particles of the carbonaceous matter were

ejected, and produced brilliant scintillations in the fire, so that

we may conclude, notwithstanding the presence of so large a quantity

of potash, the properties of the nitre were not destroyed.

H. P.

_Canal-street, Birmingham_.

FOOTNOTE:

[134] Pages 207 and 208.

III. NATURAL HISTORY.

1. _Squalls of Wind on the African Shores_.—The following description

is by D. M. Milnegraden, from the relations of his father. “The

approach of the squall is generally foreboded by the appearance of

jet black clouds over the land, moving in a direction towards the

sea, at the same time that a gentle breeze blows towards the shore.

In these circumstances, the precaution which my father usually

adopted, was to take in immediately all sail, so as to leave the ship

under bare poles, and send the whole of the crew below decks. As the

tornado approaches nearer, the rain is observed to be gushing down

in torrents, and the lightning darting down from the clouds with

such profusion, as to resemble continued showers of electric matter.

When, however, the squall comes within the distance of about half a

mile from the ship, these electric appearances altogether cease; the

rain only continues in the same manner. As the tornado is passing

over the ship, a loud crackling noise is distinctly heard among

the rigging, occasioned by the electric matter streaming down the

masts, whose points serve to attract it, and I think that I have been

told, that when this phenomenon takes place at night, a glimmering

of light is observed over every part of the rigging. But when the

squall has removed to about half a mile beyond the ship, exactly

the same appearances return by which the squall was characterised

in coming off the shore, and before reaching the same distance from

the ship. The lightning is again seen to be descending in continued

sheets and in such abundance as even to resemble the torrents of rain

themselves which accompany the squall. These squalls take place every

day during a certain season of the year called the Harmatan season.

The jet black clouds begin to appear moving from the mountains about

nine in the morning, and reach the sea about two in the afternoon.

Another very singular fact attending these tornados is, that, after

they have moved out eight or nine leagues to sea, where [p487] they

become apparently expended, the lightning is seen to rise up from the

sea. The violence of the wind during the continuance of the storm is

excessive.”—_Jameson’s Journal_, 1823, p. 367.

2. _Destruction of an Oak by Lightning_.—M. Muncke describes a case

in which an oak, being struck by lightning, was rent and destroyed

in an extraordinary manner. The trunk of the tree was about fifteen

feet in height, a foot and a half or two feet in diameter at the

branches, and three feet in diameter at the root. The top of the

tree was separated as if by the stroke of a hatchet, and without

any appearance of carbonization: the trunk was torn into a thousand

pieces, exceedingly small in size when compared with the original

mass, and thrown to a great distance. The division and destruction

was such as to sustain the thought, that in certain cases the

lightning might cause the entire dispersion of the tree, an opinion

which was suggested by the circumstance that lightning which had

fallen at Le Chateau de Marbourg left no traces of a rafter that had

occurred in its course.—_Bull. Univ._ A. viii. 194.

3. _Description of a Meteoric Fire-Ball seen at New Haven by the Rev.

S. E. Dwight_.—The meteor appeared on Saturday evening, March 21,

1813, a little before ten o’clock. The sky was much overcast, but

the covering thin, and the stars were in full view towards the north

where the meteor appeared. Dr. Dwight was standing on a platform on

the north side of the house looking eastward, when the light first

broke upon him, and for a moment supposed it to be lightning, but was

instantly induced by its continuance to look at the luminary. The

following are the observations made at the time.

i. The meteor was at first about 35° above the horizon, and, judging

from the course of a fence near at hand, its direction about N. 20°.

E.

ii. Its figure nearly that of an ellipse, with the ends in a slight

degree sharpened or angular.

iii. The length of its transverse diameter appeared to be about equal

to the apparent diameter of the moon when on the meridian, and that

of the conjugate about three fourths of the transverse.

iv. The colour rather more yellow than that of the moon.

v. A tail of light, ten or twelve degrees in length, was formed

behind it; broadest near the body; decreasing in breadth very slowly

for about two-fifths of its length, after which it was uniform, and

about as wide as the apparent diameter of Venus. The direction of the

tail was coincident with that of the transverse diameter.

vi. The ball was far more luminous than the tail, and the part

connected with the tail scarcely less distinct than the opposite part.

vii. The light was such that all objects cast distinct shadows,

though less strongly marked than when the moon is full.

viii. Numerous sparks continually issued from the ball of the [p488]

meteor; they were of the apparent size, but much more brilliant

than the smaller stars, and after descending a little distance,

disappeared.

ix. The meteor was visible for about eight or perhaps ten seconds.

x. A second or two before its disappearance, three much larger

sparks or luminous fragments were thrown off at once, two of them

the apparent size of Venus, the third larger. These were the last

pieces which were seen to leave the body. Their paths were at first

nearly parallel with that of the meteor, yet beneath it. From this

direction, however, they all deviated constantly and rapidly, in

parabolic curves, until they seemed falling perpendicularly towards

the earth. Each fragment became less and less distinct until it

disappeared. The largest continued visible until about 20° from the

horizon.

xi. The meteor itself disappeared as suddenly as if, in one

indivisible moment, it had passed into a medium absolutely opaque,

or as if, at a given moment, it had left the atmosphere; but a few

moments afterwards there was a distinct and somewhat extensive

illumination over that part of the sky for about a second.

xii. When the meteor disappeared, it was about 30° above the horizon

in the direction of N. 45° E. or 25° east of the place where it was

first seen. The direction of the path was probably from W. by S. to

E. by N. The meteor was obviously going from the observer, its path

making an angle with the optic axis of about 60°.

xiii. Between eight and ten minutes after the disappearance of the

meteor, there was a loud and heavy report, accompanied by a very

sensible jar; it did not much resemble either thunder or the report

of a cannon, but was louder, shorter, and sharper than either, and

was followed by no perceptible echo.

xiv. A friend of Dr. Dwight’s, who was in Berlin at the time, about

twenty-three miles due N. of Newhaven, saw the meteor distinctly, but

made no particular observations. His account accorded generally with

that given; but the meteor appeared to him larger, more elevated, and

somewhat more to the east in its apparent place. No account could

be obtained of any fragments which had fallen from it.—_Silliman’s

Journal_, xiii. 35.

4. _Remarkable Meteoric Phenomenon, described by_ Chladni.—A noise,

resembling thunder in its rolling nature, was heard at Saarbruck

and the environs, about four o’clock on the 1st of April, 1826, the

atmosphere being clear, and the sun shining brightly. During the

sound, a greyish object, apparently about three feet and a half in

height, was seen in the air, rapidly approaching the earth, and there

expanding itself like a sheet; there was then silence for about a

minute, after which another sound, resembling thunder, was heard, as

if it had originated at the place where the meteor fell. Nothing was

found when the place was afterwards examined.—_Bull. Univ._ A. viii.

143. [p489]

5. _Aurora Borealis seen in the Day-time at Canonmills_.—The morning

of Sunday, September 9th, was rainy, with a light gale from the N.E.

Before mid-day the wind began to veer to the west, and the clouds

in the north-western horizon cleared away: the blue sky in that

quarter assumed the form of the segment of a very large circle,

with a well-defined line, the clouds above continuing dense, and

covering the rest of the heavens. The centre of the azure arch

gradually inclined more to the north, and reached an elevation of

nearly 20°. In a short time very thin fleecy clouds began to rise

from the horizon within the blue arch; and through these very faint

perpendicular streaks, of a sort of milky light, could be perceived

shooting; the eye being thus guided, could likewise detect the same

pale streaks passing over the intense azure arch, but they were

extremely slight and evanescent. Between nine and ten in the evening

of the same day, the aurora borealis was very brilliant: so that

there is no reason to doubt that the azure arch in the morning, and

the pale light seen shooting across it, were connected with the same

phenomenon.—_Jameson’s Jour._ 1827, p. 378.

6. _Aurora Borealis in Siberia_.—Baron Wrangle says, that in Siberia,

when shooting stars pass across the space occupied by polar lights,

fiery beams suddenly arise in the place traversed by the shooting

star: further, that when a polar beam rises high towards the zenith,

the full moon also being high, it gradually forms a luminous circle

around the moon, at a distance of 20° or 30° from her, remains in

this form for a short time, and then disappears.

7. _On the Presence of Ammonia in Argillaceous Minerals_.—Being

engaged in the examination of different specimens of gypsum, M. Bouis

observed, that traces of ammonia were evident in one containing

much argillaceous matter. The peculiar odour common to argillaceous

minerals when breathed upon, was very striking in this specimen of

gypsum; when a portion of it was moistened with solution of potash,

and muriatic acid brought near, white vapours were produced, and

reddened litmus paper was very quickly rendered of a blue colour in

its vicinity.

It was now suspected that all mineral substances, emitting an

argillaceous odour, contained ammonia; a great number of specimens

were tried, being moistened with solution of caustic potash, and

examined by litmus paper. In no case was ammonia absent, and with

common clay it continued to be evolved for more than two days.

Amongst the substances tried, were pipe clay, other clays, numerous

gypsums, Paris plaster, steatite, &c. The antiquity of the mineral

seemed to have no relation to the ammonia.

M. Bouis concludes that, in all cases, the argillaceous smell

of minerals is connected with, and dependent upon, the presence

of ammonia, the latter being the vehicle of this particular

odour.—_Annales de Chimie_, xxxv. 333. [p490]

8. _Composition of Apatite_.—According to M. Rose, the apatite from

the following localities gave the annexed proportions of chloride and

fluoride of calcium, the rest being phosphate of lime with occasional

traces of iron and magnesia:—

S. G. Chlo. Calc. Fluor. Calc.

Apatite from Suarum in Norway 3.174 4.280 4.590

Cabo de Gota in Spain 3.235 0.885 7.049

Arendal 3.194 0.801 7.010

Greiner in the Tyrol 3.175 0.150 7.690

Faldigl, ditto 3.166 0.100 7.620

St. Gothard 3.197 trace 7.690

Ehrenfriedersdorf 3.211 trace 7.690

_Annales de Chimie_.

9. _Burmese Petroleum Wells_.—“The gentlemen of the mission examined

carefully the celebrated Petroleum Wells, near which they remained

for eight days, owing to the accident of the steam-vessel taking the

ground in their vicinity. Some of the wells are from thirty-seven to

fifty-three fathoms in depth, and are said to yield at an average,

daily, from 130 to 185 gallons of the earth-oil. The wells are

scattered over an area of about sixteen square miles. The wells are

private property, the owners paying a tax of five per cent. of the

produce to the state. This commodity is almost universally used

by the Burmans as lamp oil. Its price on the spot does not, on an

average, exceed from fivepence to sevenpence halfpenny per cwt. The

other useful mineral or saline productions of the Burman empire are

coal, saltpetre, soda, and culinary salt. One of the lakes affording

the latter, which is within six or seven miles of the capital, was

examined by the gentlemen of the mission.” Crawford’s Mission to

Ava.—_Jameson’s Journal_, 1827, p. 366.

10. _Direction of the Branches of Trees_.—Professor Eaton remarks

that all trees with spreading branches accommodate the direction

of the lower branches to the surface of the earth over which they

extend, as may be seen in orchards growing on the sides of hills,

and in all open forests; and inquires what influence can the earth

have upon the branches on the upper side of a tree, which causes them

to form a different angle with the body of the tree from the angle

formed by the branches on the lower side, so that all the branches

hold a parallel direction to the earth’s surface.—_Silliman’s

Journal_, xiii. 194.

11. _Effects of Light on Vegetation_.—The following observations by

Professor Eaton are dated Rensselaer school, Troy, April 30, 1827.

“Clouds and rain have obscured the hemisphere during the last six

days. In that time the leaves of all the forests which are seen from

this place have greatly expanded. But they were all of a pallid hue

until this afternoon. Within the period of about six hours, they have

all changed their colour to a beautiful green. As the only efficient

change which has taken place, is that we have a [p491] serene sky,

and a bright sun, we may say with confidence that this change of

colour is produced by the action of the sun’s rays.”

“Seven years ago, next month, I had a still more favourable

opportunity to observe this phenomenon in company with the Hon. J.

Lansing, late Chancellor of this State. While we were engaged in

taking a geological survey of his manor of Blenheim, the leaves of

the forest had expanded to almost the common size in cloudy weather.

I believe the sun had scarcely shone upon them in twenty days.

Standing upon a hill, we observed that the dense forests upon the

opposite side of the Schoharie were almost white. The sun now began

to shine in full brightness. The colour of the forest absolutely

changed so fast that we could perceive its progress. By the middle of

the afternoon, the whole of these extensive forests, many miles in

length, presented their usual summer dress.”—_Silliman’s Journal_,

xiii. 193.

12. _Organization and Reproduction of the Trufle_.—The trufle,

according to the account given of it by M. Turpin, in a memoir read

to the Academy of Sciences, is a vegetable entirely destitute of

leafy appendages or of roots; it is nothing more than a rounded

subterraneous mass, absorbing nourishment upon every point of its

surface, and the reproduction of which is dependent upon bodies

generated within its substance. The trufle is composed of, i.

globular vesicles, destined, to the reproduction of the vegetable;

ii. short and barren filaments, called by M. Turpin, _tigellules_.

The whole forms a substance, at first white, but which becomes brown

by age, with the exception of particular white veins. This change of

colour is dependent upon the presence of the reproductive bodies or

_trufinelles_. Each globular vesicle is fitted to give birth, on its

internal surface, to a multitude of these reproductive bodies, but

there are only a few of them which perfect the young vegetable. These

dilate considerably, and produce internally other smaller vesicles,

of which, two, three, or four increase in size, become brown, are

beset with small points on their exterior surface, and fill the

interior of the larger vesicle. The small masses thus formed, are the

_trufinelles_, and become trufles after the death of their parent.

Thus the brown parts of the trufle are those which contain the

trufinelles, and the interposed white veins are the parts which are

destitute of trufinelles. The parent trufle, having accomplished its

growth and the formation of the reproductive bodies within, gradually

dissolves and supplies that aliment to the young vegetable which is

proper for them; the cavity originally occupied by it in the earth

is then left occupied by a multitude of young trufles, of which the

stronger starve or destroy the others, whilst they frequently adhere

together, and, enlarging in size, reproduce the phenomena already

described.

The reporters of this memoir to the Academy state that they have

verified M. Turpin’s account, but point out a circumstance in the

natural history of the trufle, which is still unexplained. If the

[p492] method described be the only mode in which the trufle

is reproduced, then it is difficult to comprehend the enormous

multiplication of that vegetable in certain parts of France, where

immense quantities are annually collected without exhausting or even

diminishing the race. If the plant has no means of progression, how

can the young trufles leave the place of their birth, and become

disseminated over the soil? The Mémoire received the approbation of

the Academy.—_Revue Ency._ xxxv. 794.

13. _Alteration of Corn in a subterraneous Repository_.—An inhabitant

of Deneuvre in the department of Merthe, whilst excavating in the

locality of the ancient citadel of that town, found a large quantity

of corn which appeared to have been carbonized. A portion was sent

to M. Braconnot for examination, but without any particulars of the

cavity containing it. The grain was smooth on the exterior, and

unchanged in form, but its aspect announced the entire destruction

of its proximate principles. It floated on water, could be crushed

between the finger to a black powder, and when rubbed on paper left

traces resembling those of black chalk.

Being analysed, it was found to consist principally of a substance

resembling ulmine in its properties, ulmate of lime and carbonaceous

matter: the proportions were

Ulmine 26.5

Ulmate of lime, containing some phosphate of lime

and a little oxide of iron 42.0

Carbonaceous matter 30.0

Muriates of potash and lime 1.5

Nitrates of potash and lime 1.5

Fatty matter of the consistency of wax, undetermined.

-----

100.0

Although the time during which this corn has been stored up is

probably very long, still M. Braconnot thinks the principal cause of

the change in it has been humidity; and thinks also that the same

may have been the case with the corn lately found in an Egyptian

tomb[135], and quotes the known fact of corn having been found at

Scarpone, an ancient Roman station, preserved in good condition,

during eighteen centuries, in a reservoir constructed of Roman mortar.

The best use that could be made of the carbonized corn of Deneuvre

was to apply it as a manure, for it contained the best elements of

a substance of this kind, and M. Braconnot had long since observed

the presence of ulmine in good manure, its acid properties, and its

effects on vegetation. He adds also that Bruyères earth of excellent

quality gave one-fourth of a combustible matter formed of ulmine

and a carbonaceous body but little soluble in potash, the remaining

three-fourths being a pure siliceous sand without a trace of lime.

Yet so effectual is this earth, that, where it cannot be obtained,

certain exotics cannot be cultivated.—_Annales de Chimie_, xxxv. 262.

[p493]

FOOTNOTE:

[135] See p. 210 of the last Number.

The Quarterly Journal of Science, Literature and the Arts, July-December, 1827 · 第 48 / 51 段