CHAPTER XIX.

LUMINOUS SHOWERS.

In many old works, accounts are found of so-called showers of fire,

during which the entire heavens seemed filled with gleaming drops, that

threatened to burn every living thing, but were in reality harmless;

the exhibition being merely another instance of this strange phenomenon

of heatless light.

Some years ago a party of peasants were making the ascent of one of

the high peaks of the Alps, when they were caught in a rain-storm,

which produced a demoralizing effect upon them. As the rain fell, it

seemed to become luminous, and drops of fire apparently ran from their

clothing and beards. Their attempts at brushing it away, while adding

to the startling nature of the phenomenon, showed, however, that it was

perfectly harmless.

Dr. Phipson records some interesting instances of this kind of

phosphorescence, of which the following may be cited:--

M. de Thielan observed on Jan. 25, 1822, near Freyburg, a most

extraordinary spectacle. A heavy snow had been falling during the

early part of the evening, and the trees, branches, limbs, and leaves

quivered and scintillated with a resplendent bluish light, while the

drops of rain upon the grass left golden trains as they dripped to the

ground.

[Illustration:

PLATE XXIII.

DEEP SEA ANGLER.

(_Melanocetus johnstoni, Gth._)]

Arrago records similar occurrences: In 1731 a priest named Hallai, who

lived at Lessay, near Constance, states that he observed one evening

during a severe thunder-storm, rain falling which looked like _drops

of red-hot liquid metal_.

Bergman, the eminent Swedish chemist, communicated to the Royal Society

of London, in 1761, that late in the afternoon upon two occasions,

though hearing no thunder, he had seen rain which glittered as it fell

upon the ground, making it look as if covered with waves of fire.

M. Pasumot, on May 3, 1768, was overtaken, while walking near

Arnay-le-Duc, on an open plain, by a very heavy storm. The rain

collecting on the brim of his hat, he stooped his head to allow it to

run off, when to his astonishment, as it encountered that which fell

from the clouds, at about twenty inches from the ground, _sparks were

emitted_ between the two portions of liquid.

During January, 1822, Lampadius was told by the miners of Freyburg,

that they had observed during a storm, _sleet_ which _emitted light_

when it fell upon the ground.

A friend of Howard, the meteorologist, stated to him, that while going

from London to Bow on the 19th of May, 1809, there came up a very

severe storm; and he observed the rain emit light as it struck the

earth.

On the 28th of October, 1772, the Abbé Bertholon, who was travelling

to Lyons from Brignai, early in the morning was overtaken by a violent

storm of rain and hail. The _rain and hail-stones emitted light_ as

they fell upon the metallic mounting of his horse’s trappings.

Luminous hail has often been observed; and when we remember that

hail-stones sometimes attain great size, we can imagine the scene

occasioned by a fall where each stone is phosphorescent. Ordinary

hail-stones are the size of small peas, but they occasionally occur

large enough to kill human beings; and I have seen them so large in the

Sierra Madre Mountains that any shelter was preferable to exposure to

them. In 1707 a hail-storm occurred at the town of Como, Switzerland,

doing an incredible amount of damage, some of the stones weighing

nearly ten ounces. Darwin describes a storm upon the South American

pampas, in which the stones that fell were large enough to kill

powerful animals.

Ice has often been observed to emit luminous sparks; and probably one

of the grandest spectacles ever witnessed, is the luminous cap of a

snow-covered mountain. The glaciers of the Alps have been seen bathed

in a soft phosphoric glow, the icy rivers being distinctly marked by

the phenomenon, which is so brilliant, at times, that the appearance

of a second sunset is occasioned. Not only are the summits of Alpine

peaks and the glaciers luminous, but the valleys of Piedmont, Valais,

and others have been seen to emit from their covering of snow a soft

blue light of singular beauty. So intense is this light about the cap

of Mount Blanc, it has been photographed. Luminous vapors or mists

may be mentioned in this connection. Several times in the history of

this country, luminous mists or fogs have been recorded. Massachusetts

was visited by one some years ago, in which the fog was so dense that

observers a few feet away were invisible, yet darkness was not an

accompaniment; the mist seemed to be light-emitting itself, having a

reddish, metallic hue. Others described it as a fiery red or yellow,

while to some it appeared to be composed of faintly luminous matter.

In the year 1783 all Europe and a portion of Asia were enveloped in a

dense fog of a most remarkable nature. It was termed “dry,” as even at

night no dampness was observed. It was first seen at Copenhagen, its

coming being heralded by severe storms. A few weeks later it appeared

in various parts of France, and rapidly seemed to spread over Europe

and portions of Asia. During the day it had a metallic glow, which at

night changed to a phosphorescent light, so brilliant that ordinary

print could be read by it. Many attempts to explain it were made by the

savants of the day, and it was universally supposed to be due to the

earthquakes and volcanic eruptions which were of unusual severity that

year.

A somewhat similar fog appeared in the United States, a portion of

Europe, and Africa in August, 1831. The daylight was perceptibly

diminished, while at night a conspicuous phosphorescent light was

emitted. A remarkable luminous fog occurred in Switzerland in 1859. M.

L. F. Wartmann of Geneva states that the strange light was observed on

five successive nights, and apparently proceeded from a heavy dry fog

that hung over Geneva during the time. The light was so brilliant that

this gentleman distinguished the smallest objects upon his table with

perfect ease, no other light being in the apartment. The light caused

general comment in the places in which it appeared, and a traveller

between Geneva and Annemassi stated that he readily found the road by

its means. Dr. Verdeil of Lausanne describes a fog which diffused so

much light that distant objects were perfectly visible at night.

Among the phenomena which attended the eruption of Vesuvius in 1794 was

one which did not tend to allay the fears of the people. During the day

a fine dust filled the air about Naples, which was not particularly

noticeable; but as night came on, it emitted a pale though distinct

phosphorescent light. An English gentleman sailing near Torre del Greco

noticed that where the dust collected upon his hat it was luminous, and

no little consternation was caused among the superstitious sailors by

the occurrence.

Luminous dust-showers have been noticed in several localities; and the

peculiar glows that were seen in this country a few years ago were

accredited by many to them, the supposition being that dust, perhaps

from volcanic eruptions, was floating about in the upper strata of the

atmosphere. Many other explanations were given, and the literature upon

the subject is extremely voluminous and interesting.

The amount of material floating about in the upper regions of the air

is perhaps little realized by my young readers, and some reference to

the phenomenon may be of interest.

Professor Nordenskjöld has for many years been a close observer of

dust of all kinds that has fallen upon the earth in rain or snow; and

it was his good fortune, during the expedition of the “Vega,” to prove

beyond a doubt the presence of cosmic dust. For many years we have

been assured by astronomers that the earth was being bombarded, as it

were, continually, by innumerable meteors. The moment they enter our

domain, we observe the spectacle of their ignition. In a moment they

are reduced to ashes, and the fine impalpable dust drops slowly, an

invisible shower, upon the earth. When such showers are intensified, it

is not impossible that some outward and visible phenomena may be the

result.

In the search for this cosmic dust, the far North, where the surface

is covered by an almost continuous coating of snow and ice, offers

a wide and promising field for investigation. Here no other dust

prevails. Professor Nordenskjöld first found cosmic dust in the North

at Spitzbergen. The second discovery, off the Taimar coast, seemed to

be in the form of yellow specks lying on the snow. They were at first

supposed to be diatomaceous ooze;[49] but when placed in the hands

of Dr. Kjellman, he pronounced them to be pale yellow crystals, and,

curious enough, formed of carbonate of lime. “The original composition

and origin of this substance,” says Professor Nordenskjöld, “appears

to me exceedingly enigmatical. It was not carbonate of lime, for the

crystals were rhomboidal, and did not show the cleavage of calcite.

Nor can there be a question of its being arragonite, because this

mineral might indeed fall asunder of itself; but in that case the newly

formed powder ought to be crystalline. Have the crystals originally

been a new hydrated carbonate of lime formed by crystallizing out at

a temperature of ten or twenty degrees above the freezing point? In

such case they ought not to have been found on the surface of the

_snow_, but lower, on the surface of the _ice_. Or have they fallen

down from the inter-planetary spaces to the surface of the earth, and

before crumbling down have had a composition differing from terrestrial

substances, in the same way as various chemical compounds found in

recent times in meteoric stones? The occurrence of the crystals in

the uppermost layer of snow, and their falling asunder in the air,

tell in favor of this view. Unfortunately there is no possibility of

settling these questions; but at all events this discovery is a further

incitement to those who travel in the high North, to collect with

extreme care, from snow-fields lying far from the ordinary routes of

communication, all foreign substances, though apparently of trifling

importance.”

The investigations of the Swedish naturalist in this field are of

exceeding interest. His first attempt to obtain meteoric dust was at

Stockholm, where, in December, 1871, there was a great fall of snow,

the heaviest ever known. On the last days of the storm, after the

atmosphere had been presumably purified of extraneous substances, he

collected a cubic metre of snow, melted it over a fire, and found that

after the water had evaporated a residue of black powder remained,

in which were many grains of metallic iron, that were attracted by a

magnet. In 1872 his brother made a similar examination of the snow, in

a quiet locality near the remote village of Evois, Finland. The snow

upon being melted also gave the same black powder and metallic iron.

The investigations of Nordenskjöld himself, conducted in Spitzbergen,

as previously mentioned, were the most satisfactory. The observations

were made in 80° north latitude, and 13° to 150° east longitude, in

the layer of snow that covered the ice. An imaginary section was as

follows: (1), new fallen snow; (2), a layer of hardened old snow,

eight millimetres in thickness; (3), a layer of snow, conglomerated to

a crystalline granular mass; and (4), common granular hardened snow.

Layer three was full of small black grains, among which were found

numerous metallic particles, that were attracted by the magnet, and

found to contain iron, cobalt, and possibly nickel also.

In his visit to Greenland in 1870, Nordenskjöld found in the dust

that lay on the inland ice, grains of metallic iron and cobalt. “The

main mass,” he says, “consisted of a crystalline, double refracting

silicate, drenched through with an ill-smelling organic substance.

The dust was found in large quantities at the bottom of innumerable

small holes in the surface of the inland ice. This dust could scarcely

be of volcanic origin, because by its crystalline structure it

differs completely from the glass dust that is commonly thrown out of

volcanoes, and is often carried by the wind to very remote regions;

as also from the dust which, in March, 1875, fell at many places in

the middle of Scandinavia, and which was proved to have been thrown

out by volcanoes in Iceland.” Professor Nordenskjöld’s estimate of the

quantity of dust shows that it has been in past ages a not unimportant

factor, perhaps, in its addition to the crust. He says, “I estimate the

quantity of the dust that was found on the ice north of Spitzbergen, at

from .01 to 1 milligram per square metre; and probably the whole fall

of dust for the year far exceeded the latter figure. But a milligram on

every square metre of the surface of the earth amounts for the globe

to five hundred million kilograms (say half a million tons). Such a

mass, collected year by year during the geological ages, of a duration

probably incomprehensible by us, becomes a consideration too important

to be neglected, when the fundamental facts of the geological history

of our planet are enumerated. A continuation of these investigations

will perhaps show that our globe has increased gradually from a small

beginning to the dimensions it now possesses; that a considerable

quantity of the constituents of our sedimentary strata, especially of

those that have been deposited in the open sea far from land, are of

cosmic origin; and will throw an unexpected light on the origin of the

fire-hearths of the volcanoes, and afford a simple explanation of the

remarkable resemblance which unmistakably exists between plutonic rocks

and meteoric stones.”

Such enormous masses of material could well explain the rosy and other

curious lights that are from time to time observed. But cosmic dust

is not the only matter in the air that could occasion the phenomena;

the atmosphere is constantly filled with innumerable forms caught up

by currents and carried to inconceivable heights, and thus to great

distances, to be precipitated to the earth in hail, snow, or rain.

Near St. Domingo, Darwin tells us, the atmosphere became thick and

hazy from the impalpable fine dust that actually injured their

astronomical instruments. “The morning before we anchored at Porto

Praya,” he says, “I collected a little packet of this brown-colored

dust, which appeared to have been filtered from the wind by the gauze

of the vane at the masthead. Mr. Lyell has also given me four packets

of dust which fell on a vessel a few hundred miles northward of these

islands. Professor Ehrenberg finds that this dust consists in great

part of _infusoria_ with siliceous shields, and of the siliceous

tissue of plants. In five little packets which I sent him, he has

ascertained no less than sixty-seven different organic forms. The

_infusoria_, with the exception of two marine species, are all

inhabitants of fresh water. I have found no less than fifteen different

accounts of dust having fallen on vessels when far out in the Atlantic.

From the direction of the wind whenever it has fallen, and from its

having always fallen during those months when the harmattan is known to

raise clouds of dust high into the atmosphere, we may feel sure that

it all comes from Africa. It is, however, a very singular fact, that,

although Professor Ehrenberg knows many species of _infusoria_

peculiar to Africa, he finds none of them in the dust which I sent him;

on the other hand, he finds in it two species which hitherto he knows

as living only in South America. The dust falls in such quantities

as to dirty every thing on board, and to hurt people’s eyes; vessels

even have run ashore, owing to the obscurity of the atmosphere. It has

often fallen on ships when more than a thousand miles from the coast

of Africa, and at points sixteen hundred miles distant in a north and

south direction. In some dust which was collected on a vessel three

hundred miles from the land, I found particles of stone, above the

thousandth of an inch square, mixed with finer matter. After this fact,

one need not be surprised at the diffusion of the far lighter and

smaller sporules of cryptogamic plants.”

The extent to which dust and ashes can be taken up and held by air

currents is shown in volcanoes. In 1810 the ashes from a volcano at

St. Vincent were wafted to Barbados, nearly a hundred miles; and in

1835 the material thrown from a volcano in Guatemala to Jamaica, eight

hundred miles. As intimated, these showers are not all inorganic, but

are often living or fossil animals or plants that are floating about.

Such are the reddish or gray showers that are frequently met with off

the African coast, and when in the snow they are called “blood-rains.”

The one in 1755, near Lago Maggiore, covered over two hundred square

leagues, causing a panic among the inhabitants. For a distance of nine

feet below the surface, the snow was blood red, the atmosphere appeared

red and fiery, while at sunrise and sunset a rosy hue pervaded every

thing. When this shower fell and there was no snow, the earthy deposit

accumulated an inch deep; and it has been estimated that, supposing it

to average two lines in depth, there would be for each square mile an

amount equal to nearly three thousand cubic feet. A similar panic was

caused some years ago by a swarm of butterflies. Everywhere they left

a drop of blood-colored fluid, so that the fences, houses, and cattle

were covered with it. The insects were so numerous that they obstructed

the vision.

In the “blood-rains” of Italy, and generally in such instances, the

red hue comes from red oxide of iron. At a single shower in Lyons in

1846, Ehrenberg estimated that seven hundred and twenty thousand pounds

of material fell, ninety thousand pounds of which were microscopic

organisms, including thirty-nine species of siliceous diatoms, and many

others of great beauty of form and shape.

Ehrenberg enumerates a very large number of these showers, referring

to Homer’s “Iliad” for one of the earliest known; and asks, with such

facts before us, how many thousand millions of hundred-weight of

microscopic organism have reached the earth since Homer’s time? The

whole number of species made out is over three hundred. The species, as

far as ascertained, are not African; fifteen are North American. But

the origin of the dust is yet unknown. The zone in which these showers

occur covers Southern Europe and Northern Africa, with the adjoining

portion of the Atlantic, and the corresponding latitudes in Western and

middle Asia.

When blown along by the wind, these showers perform another office

besides affecting, perhaps, the color or tint of the atmosphere; they

wear away rock, and polish and furrow it. Such work can be seen in the

granite rocks at the San Bernardino Pass in California. Quartz is

polished, and hard gems left weathered out; while at Cape Cod ordinary

sand has been known to wear holes through glass windows by continually

blowing against them.

[Illustration:

PLATE XXIV.

PELICAN FISH.

(_Eyrypharyx pelecanoides._)]

An ingenious instrument has been invented to capture these flying

objects of the air. It is called by the inventor, Doctor Miguel, the

æroscope, and is really a net for animals invisible to the naked eye.

Many objects are phosphorescent when struck, or when divided into

thin laminæ. Some simple materials for such experiments are chlorate

of potash, fluor-spar, feld-spar, sugar, etc. By placing any of

these in a mortar, and grinding them in the dark, flashes of light

will be seen, powdered sugar often making a striking display. A

beautiful and effective exhibition can be produced by placing a small

amount of phosphuret of calcium in water; decomposition follows, and

phosphuretted gas is evolved. As the bubbles of gas rise and come in

contact with the atmosphere, they seem to take fire. If in a dark room,

luminous rings are seen rising, and they can be made to take various

shapes by using a fan. A trick often performed by magicians is to hand

around a marble, and then pretend to render it luminous by blowing upon

it. This trick consists in having small balls at hand, of a material

that can readily be rendered luminous by the application of heat. These

substances can be easily made.

A fine light is produced by taking,--

Barium sulphate (C P.) 32 parts

Magnesium carbonate (C P.) 1 part

Sulphur (C P.) 1 part

Gum tragacanth q. s.

This should be made into balls of a convenient size, dried at a

moderate temperature, and kept in a crucible at a red heat for about an

hour. Allow them to cool slowly, and then place in a glass-stoppered

bottle before their heat has disappeared. When required for use, expose

them to the sun or any strong light, and they will become luminous, and

continue so for many hours.

Another formula is:--

Strontium sulphate (C P.) 22 parts

Sulphur (C P.) 1 part

Gum tragacanth q. s.

This should be heated as above described.

A most interesting experiment is to make a selection of artificial

flowers, and, having brushed them over with glue or mucilage, dust

them with the powder from one of the balls made as described. If

the flowers are exposed to the sun a short time, they will emit a

phosphorescent light, each flower standing out in the darkness with

extreme brilliancy,--a striking and remarkable spectacle.

Canton’s phosphorus is easily made by calcining clean oyster-shells,

until they are perfectly white, in a crucible. The clearer and finer

portions should then be reduced to powder, and placed in layers with

alternate layers of flowers of sulphur in a crucible. Cover, and heat

to a dull redness for about half an hour, then allow to cool slowly.

Luminous “ink” or liquid can be made by placing a small piece of

phosphorus about as large as a pea in a test-tube with a small quantity

of olive oil; hold the tube in a water-bath until the oil becomes

heated, and the phosphorus liquefies; then shake it until the oil will

take up no more phosphorus, and, when it becomes clear, pour into

a bottle with a glass stopper. When it is to be used, take out the

stopper, and admit the air. The oil can be used with a brush, and in

the dark will appear luminous.

Water may be rendered phosphorescent by dissolving a small piece of

phosphorus in ether for several days in a glass-stoppered bottle; then

by immersing a piece of sugar in the solution, and placing it in water,

the latter becomes vividly phosphorescent. It should be remembered that

phosphorus and ether are both extremely dangerous, and experiments with

them should be conducted with care and judgment.

While this is a mere toy, luminous paint is of great value. It is

easily made, and can be applied to many purposes.

Schade of Dresden has quite recently patented an invention, which

enables him to produce paints that are luminous without affecting

the tint by day. This is accomplished, according to the inventor, as

follows:--

Zanzibar or Kauri copal is melted over a charcoal fire. Fifteen parts

of the melt are dissolved in 60 parts of French oil of turpentine, and

the filtered solution is mixed with 25 parts, previously heated and

cooled, pure linseed-oil. The varnish which is thus obtained, is used

in the following methods, in the manufacture of luminous paints, by

grinding between granite rolls in a paint-mill. Iron rolls should be

avoided, because particles of iron, which are liable to be detached,

would injure the luminous properties.

Varnishes, as they occur in commerce, generally contain lead or

manganese, which would destroy the phosphorescence of calcium sulphide.

_A pure white luminous paint_ is prepared by mixing 40 parts of the

varnish obtained in the abovedescribed process with 6 parts prepared

barium sulphate, 6 parts prepared calcium carbonate, 12 parts prepared

white zinc sulphide, and 36 parts good luminous calcium sulphide in

a proper vessel, to an emulsion, and then grinding it very fine in a

color-mill. For _red luminous paint_, 60 parts varnish are mixed with

8 parts prepared barium sulphate, 2 parts prepared madder lake, 6

parts prepared realgar (red arsenic sulphide), and 30 parts luminous

calcium sulphide, and treated the same as for white paint. For _orange

luminous paint_, 46 parts varnish are mixed with 17.5 parts prepared

barium sulphate, 1 part prepared Indian yellow, 1.5 parts prepared

madder lake, and 38 parts luminous calcium sulphide. For _yellow

luminous paint_, 48 parts varnish are mixed with 10 parts prepared

barium sulphate, 8 parts barium chromate, and 34 parts luminous calcium

sulphide. For _green luminous paint_, 48 parts varnish are mixed with

10 parts prepared barium sulphate, 8 parts chromium oxide green, and 34

parts luminous calcium sulphide.

_A blue luminous paint_ is prepared from 42 parts varnish, 10.2 parts

prepared barium sulphate, 6.4 parts ultramarine blue, 5.4 parts cobalt

blue, and 46 parts luminous calcium sulphide.

_A violet luminous paint_ is made from 42 parts varnish, 10.2 parts

prepared barium sulphate, 2.8 parts ultramarine violet, 9 parts

cobaltous arsenate, and 36 parts luminous calcium sulphide.

_For gray luminous paint_, 45 parts of the varnish are mixed with 6

parts prepared barium sulphate, 6 parts prepared calcium carbonate, O.5

parts ultramarine blue, 6.5 parts gray zinc sulphide.

_A yellowish-brown luminous paint_ is obtained from 48 parts varnish,

10 parts precipitated barium sulphate, 8 parts auri pigment, and 34

parts luminous calcium sulphide.

_Luminous colors for artists’_ use are prepared by using East India

poppy oil in the same quantity, instead of the varnish, and taking

particular pains to grind the materials as fine as possible.

_For luminous oil-color paints_, equal quantities of pure linseed oil

are used in place of the varnish. The linseed oil must be cold-pressed,

and thickened by heat. All the above luminous paints can be used in

the manufacture of colored papers, etc., if the varnish is altogether

omitted, and the dry mixtures are ground to a paste with water.

The luminous paints can also be used as _wax colors for painting on

glass_ and similar objects, by adding, instead of the varnish, ten per

cent more of Japanese wax, and one-fourth the quantity of the latter

of olive oil. The wax colors prepared in this way may also be used for

painting upon porcelain, and are then carefully burned without access

of air. Paintings of this kind can also be treated with water-glass.

Living lights · 第 19 / 20 章