As we purpose for the present to confine ourselves exclusively within the

telluric sphere of nature, it will be expedient to cast a preliminary glance

over the relations in space of solids and fluids, the form of the Earth, its

mean density, and the partial distribution of this density in the interior

of our planet, its temperature and its electro-magnetic tension. From the

consideration of these relations in space, and of the forces inherent in

matter, we shall pass to the reaction of the interior on the exterior of our

globe; and to the special consideration of a universally distributed natural

power -- subterranean heat; to the phenomena of earthquakes, exhibited in

unequally expanded circles of commotion, which are not referable to the

action of dynamic laws alone; to the springing forth of hot wells; and,

lastly, to the more powerful actions of volcanic processes. The crust of

the Earth, which may scarcely have been perceptibly elevated by the sudden

and repeated, or almost uninterrupted shocks by which it has been moved from

below, undergoes, nevertheless, great changes in the course of centuries in

the relations of the elevation of solid portions, when compared with the

surface of the liquid parts, and even in the form of the bottom of the sea.

In this manner simultaneous temporary or permanent fissures are opened, by

which the interior of the Earth is brought in contact with the external

atmosphere. Molten masses, rising from an unknown depth, flow in narrow

streams along the declivity of mountains, rushing impetuously onward, or

moving slowly and gently, until the fiery source is quenched in the midst of

exhalations, and the lava becomes incrusted, as it were, by

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the solidification of its outer surface. New masses of rocks are thus

formed before our eyes, while the older ones are in their turn converted

into other forms by the greater or lesser agency of Platonic forces. Even

where no disruption takes place the crystalline moleculres are displaced,

combining to form bodies of denser texture. The water presents structures

of a totally different nature, as, for instance, concretions of animal and

vegetable remains, of earthy, calcareous, or aluminous precipitates,

agglomerations of finely-pulverized mineral bodies, covered with layers of

the silicious shields of infusoria, and with transported soils containing

the bones of fossil animal forms of a more ancient world. The study of the

strata which are so differently formed and arranged before our eyes, and of

all that has been so variously dislocated, conforted, and upheaved, by

mutual compression and volcanic force, leads the reflective observer, by

simple analogies, to draw a comparison between the present and an age that

has long passed. It is by a combination of actual phenomena, by an ideal

enlargement of relations in space, and of the amount of active forces, that

we are able to advance into the long sought and indefinitely anticipated

domain of geognosy, which has only within the last half century been based

on the solid foundation of scientific deduction.

It has been acutely remarked, "that notwithstanding our continual employment

of large telescopes, we are less acquainted with the exterior than with the

interior of other planets, excepting, perhaps, our own satellite." They

have been weighed, and their volume measured; and their mass and density are

becoming known with constantly-increasing exactness; thanks to the progress

made in astronomical observation and calculation. Their physical character

is, however, hidden in obscurity, for it is only in our own globe that we

can be brought in immediate contact with all the elements of organic and

inorganic creation. The diversity of the most heterogenous substances,

their admixtures and metamorphoses, and the ever-changing play of the forces

called into action, afford to the human mind both nourishment and enjoyment,

and open an immeasurable field of observation, from which the intellectual

activity of man derives a great portion of its grandeur and power. The

world of perceptive phenomena is reflected in the depths of the ideal world,

and the richness of nature and the mass of all that admits of classification

gradually become the objects of inductive reasoning.

I would here allude to the advantage, of which I have already

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spoken, possessed by that portion of physical science whose origin is

familiar to us, and is connected with our earthly existence. The physical

description of celestial bodies from the remotely-glimmering nebulae with

their suns, to the central body of our own system, is limited, as we have

seen, to general conceptions of the volume and quantity of matter. No

manifestation of vital activity is there presented to our senses. It is

only from analogies, frequently from purely ideal combinations, that we

hazard conjectures on the specific elements of matter, or on their various

modifications in the different planetary bodies. But the physical knowledge

of the heterogeneous nature of matter, its chemical differences, the regular

forms in which its molecules combine together, whether in crystals or

granules; its relations to the deflected or decomposed waves of light by

which it is penetrated; to radiating, transmitted, or polarized heat; and to

the brilliant or invisible, but not, on that account, less active phenomena

of electro-magnetism -- all this inexhaustible treasure, by which the

enjoyment of the contemplation of nature is so much heightened, is dependent

on the surface of the planet which we inhabit, and more on its solid than on

its liquid parts. I have already remarked how greatly the study of natural

objects and forces, and the infinite diversity of the sources they open for

our consideration, strengthen the mental activity, and call into action

every manifestation of intellectual progress. These relations require,

however, as little comment as that concatenation of causes by which

particular nations are permitted to enjoy a superiority over others in the

exercise of a material power derived from their command of a portion of

these elementary forces of nature.

If, on the one hand, it were necessary to indicate the difference existing

between the nature of our knowledge of the Earth and of that of the

celestial regions and their contents, I am no less desirous, on the other

hand, to draw attention to the limited boundaries of that portion of

spacefrom which we derive all our knowledge of the heterogeneous character

of matter. This has been somewhat inappropriately termed the Earth's crust;

it includes the strata most contiguous to the upper surface of our planet,

and which have been laid open before us by deep fissure-like valleys, or by

the labors of man, in the bores and shafts formed by miners. These labors*

do not extend beyond a vertical depth of somewhat more than 2000 feet (about

one third of a geographical mile) below the

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level of the sea, and consequently only about 1/9800th of the Earth's

radius.

[footnote] *In speaking of the greatest depths within the Earth reached by

human labor, we must recollect that there is a difference between the

'absolute depth' (that is to say, the depth below the Earth's surface at

that point) and the 'relative depth' (or that beneath the level of the sea).

The greatest relative depth that man has hitherto reached is probably the

bore at the new salt-works at Minden, in Prussia: in June, 1814, it was

exactly 1993 feet, the absolute depth being 2231 feet. The temperature of

the water at the bottom was 98 degrees F., which assuming the mean

temperature of the air at 49.3 degrees gives an augmentation of temperature

of 1 degree for every 54 feet. The absolute depth of the Artesian well of

Grenelle, near Paris, is only 1795 feet. According to the account of the

missionary Imbert, the fire-springs, "Ho-tsing." of the Chinese, which are

sunk to obtain [carbureted] hydrogen gas for salt-boiling, far exceed our

Artesian springs in depth. In the Chinese province of Szu-tschuan these

fire-springs are very commonly of the depth of more than 2000 feet; indeed,

at Tseu-lieu-tsing (the place of continual flow) there is a Ho-tsing which,

in the year 1812, was found to be 3197 feet deep. (Humboldt, 'Asie

Centrale', t. ii., p. 521 and 525. 'Annales de l'Association de la

Propagation de la Foi', 1829, No. 16, p. 369.)

[footnote continues] The relative depth reached at Mount Massi, in Tuscany,

south of Volterra, amounts, according to Matteuci, to only 1253 feet. The

boring at the new salt-works near Minden is probably of about the same

relative depth as the coal-mine at Apendale, near Newcastle-under-Lyme, in

Staffordshire, where men work 725 yards below the surface of the earth.

(Thomas Smith, 'Miner's Guide', 1836, p. 160.) Unfortunately, I do not know

the exact height of its mouth above the level of the sea. The relative

depth of the Monk-wearmouth mine, near Newcastle, is only 1496 feet.

(Phillips, in the 'Philos. Mag.', vol. v., 1834, p. 446.) That of the Liege

coal-mine, 'l'Esperance' at Seraing, is, according to M. Gernaert, Ingenieur

des Mines, 1223 feet in depth. The works of greatest absolute depth that

have ever been formed are for the most part situated in such elevated plains

or valleys that they either do not descend so low as the level of the sea,

or at most reach very little below it. Thus the Eselchacht, at Kuttenberg,

in Bohemia, a mine which can not now be worked, had the enormous absolute

depth of 3778 feet. (Fr. A. Schmidt, 'Berggestze der oter Mon.', abth. i.,

bd. i., s. xxxii.) Also, at St. Daniel and at Geish, on the Rorerbubel, in

the 'Landgericht' (or provincial district) of Kitzbuhl, there were, in the

sixteenth century, excavations of 3107 feet. The plans of the works of the

Rorerbubel are still preserved. (See Joseph von Sperges, 'Tyroler

Bergwerksgeschichte', s. 121. Compare, also, Humboldt, 'Gutachten uber

√∫erantreibung des Meissner Stollens in die Freiberger Erzrevier', printed

in Herder, 'uber Herantreibung des Meissner Stollens in die Freiberger

Erzrevier', printed in Herder, 'uber den jetz begonnenen Erbstollen', 1838,

s. cxxiv.) We may presume that the knowledge of the extraordinary depth of

the Rorerbuhel reached England at an early period, for I find it remarked in

Gilbert, 'de Magnete', that men have penetrated 2400 or even 3000 feet into

the crust of the Earth. ("Exigua videtur terrae portio, quae unquam

hominibus spectanda emerget aut eruitur; cum profundinus in ejus viscera,

ultra efflorescentis extremitatis corruptelam, aut propter aquas in magnis

fodin, tanquam per venas scaturientesaut propter seris salubrioris ad vitam

operariorum sustinendam necessarii defectum, aut propter ingentex sumptus ad

tantos labores exantlandos, multasque difficultates, ad profundiores terrz'

partes penetrre non possumus; adeo ut quadrigentas aut [quod rarissime]

quingentas orgyas in quibusdam metallis descendisse, stupendus omnibus

videatur connatus." -- Guilielmi Gilberti, Colcestrensis, 'de Magnete

Physiologia nova'. Lond., 1600, p. 40.)

[footnote continues] The absolute depth of the mines in the Saxon

Erzgebirge, near Freiburg, are: in the Thurmhofer mines, 1944 feet; in the

Honenbirker mines, 1827 feet; the relative depths are only 677 and 277 feet,

if, in order to calculate the elevation of the mine's mouth above the level

of the sea, we regard the elevation of Freiburg as determined by Reich's

recent observations to be 1269 feet. The absolute depth of the celebrated

mine of Joachimsthal, in Bohemia (Verkreuzung des Jung Hauer Zechen-und

Andreasganges), is full 2120 feet; so that, as Von Dechen's measurements

show that its surface is about 2388 feet above the level of the sea, it

follows that the excavations have not as yet reached that point. In the

Harz, the Samson mine at Andreasberg has an absolute depth of 2197 feet. In

what was formerly Spanish America, I know of no mine deeper than the

Valenciana, near Guanaxuato (Mexico), where I found the absolute depth of

the Planes de San Bernardo to be 1686 feet; but these planes are 5960 feet

above the level of the sea. If we compare the depth of the old Kuttenberger

mine (a depth greater than the height of our Brocken, and only 200 feet less

than that of Vesuvius) with the loftiest structures that the hands of man

have erected (with the Pyramid of Cheops and with the Cathedral of

Strasburg), we find that they stand in the ratio of eight to one. In this

note I have collected all the certain information I could find regarding the

greatest absolute and relative depths of mines and borings. In descending

eastward from Jerusalem toward the Dead Sea, a view presents itself to the

eye, which, according to our present hypsometrical knowledge of the surface

of our planet, is unrivaled in any country; as we approach the open ravine

through which the Jordan takes its course, we tread, with the open sky above

us, on rocks which, according to the barometric measurements of Berton and

Russegger are 1385 feet below the level of the Mediterranean. (Humboldt,

'Asie Centrale', th. ii., p. 323.)

The crystalline masses that have been erupted from active volcanoes, and are

generally similar to the rocks on the upper surface, have come from depths

which, although not accurately determined, must certainly be sixty times

greater than those to which human labor has been enabled to penetrate. We

are able to give in numbers the depth of the shaft where the strata of coal,

after penetrating a certain way, rise again at a distance that admits of

being accurately defined by measurements. These dips show that the

carboniferous strata, together with the fossil organic remains which they

contain, must lie, as, for instance, in Belgium, more than five or six

thousand feet* below the present level

p 160

of the sea, and that the calcareous and the curved strata of the Devonian

basin penetrate twice that depth.

[footnote] *Basin-shaped curved strata, which dip and reappear at

measureable distances, although their deepest portions are beyond the reach

of the miner, afford sensible evidence of the nature of the earth's crust at

great depths below its surface. Testimony of this kind possesses,

consequently, a great geognostic interest. I am indebted to that excellent

geognosist, Von Dechen, for the following observations. "The depth of the

coal basin of Liege, at Mont St. Gilles, which I, in conjunction with our

friend Von Oeynhausen, have ascertained to be 3890 feet below the surface,

extends 3464 feet below the surface of the sea, for the absolute height of

Mont St. Gilles certainly does not much exceed 400 feet; the coal basin of

Mons is fully 1865 feet deeper. But all these depths are trifling compared

with those which are presented by the coal strata of Saar-Revier

(Saarbrucken). I have found after repeated examinations, that the lowest

coal stratum which is known in the neighborhood of Duttweiler, near

Bettingen, northeast of Saarlouis, must descend to depths of 20,682 and

22,015 feet (or 3.6 geographical miles) below the level of the sea." This

result exceeds, by more than 8000 feet, the assumption made in the text

regarding the basin of the Devonian strata. This coal-field is therefore

sunk as far below the surface of the sea as Chimborazo is elevated above it

-- at a depth at which the Earth's temperature must be as high as

435ºdegrees F. Hence, from the highest pinnacles of the Himalaya to the

lowest basins containing the vegetation of an earlier world, there is a

vertical distance of about 48,000 feet, or of the 435th part of the Earth's

radius.

If we compare these subterranean basins with the summits of montains that

have hitherto been considered as the most elevated portions of the raised

crust of the Earth, we obtain a distance of 37,000 feet (about seven miles),

that is, about the 1/524th of the Earth's radius. These, therefore, would

be the limits of vertical depth and of the superposition of mineral strata

to which geognostical inquiry could penetrate, even if the general elevation

of the upper surface of the earth were equal to the height of the

Dhawalagigi in the Himalaya, or of the Sorata in Bolivia. All that lies at

a greater depth below the level of the sea than the shafts or the basins of

which I have spoken, the limits to which man's labors have penetrated, or

than the depths to which the sea has in some few instances been sounded (Sir

James Ross was unable to find bottom with 27,600 feet of line), is as much

unknown to us as the interior of the other planets of our solar system. We

only know the mass of the whole Earth and its mean density by comparing it

with the open strata, which alone are accessible to us. In the interior of

the Earth, where all knowledge of its chemical and mineralogical character

fails, we are again limited to as pure conjecture, as in the remotest bodies

that revolve round the Sun. We can determine nothing with certainty

regarding the depth at which the geological strata must be supposed to be in

state of softening or of liquid fusion, of the cavities occupied by elastic

vapor, of the condition of fluids when heated under an enormous pressure, or

of the law of the increase

p 161

of density from the upper surface to the center of the Earth.

The consideration of the increase of heat with the increase of depth toward

the interior of our planet, and of the reaction of the interior on the

external crust, leads us to the long series of volcanic phenomena. These

elastic forces are manifested in earthquakes, eruptions of gas, hot wells,

mud volcanoes and lava currents from craters of eruption and even in

producing alterations in the level of the sea.*

[footnote] * [See Daubeney 'On Volcanoes', 2d edit., 3848, p. 539, etc., on

the so called 'mud volcanoes', and the reasons advanced in favor of adopting

the term "salses" to designate these phenomena.] -- Tr.

Large plains and variously indented continents are raised or sunk, lands are

separated from seas, and the ocean itself, which is permeated by hot and

cold currents, coagulates at both poles, converting water into dense masses

of rock, which are either stratified and fixed, or broken up into floating

banks. The boundaries of sea and land, of fluids and solids, are thus

variously and frequently changed. Plains have undergone oscillatory

movements, being alternately elevated and depressed. After the elevation of

continents, mountain chains were raised upon long fissures, mostly parallel,

and in that case, probably cotemporaneous; and salt lakes and inland seas,

long inhabited by the same creatures, were forcibly separated, the fossil

remains of shells and zoophytes still giving evidence of their original

connection. Thus, in following phenomena in their mutual dependence, we are

led from the consideration of the forces acting in the interior of the Earth

to those which cause eruptions on its surface, and by the pressure of

elastic vapors give rise to burning streams of lava that flow from open

fissures.

The same powers that raised the chains of the Andes and the Hiimalaya to the

regions of perpetual snow, have occasioned new compositions and new textures

in the rocky masses, and have altered the strata which had been previously

deposited from fluids impregnated with organic substances. We here trace

the series of formations, divided and superposed according to their age, and

depending upon the changes of configuration of the surface, the dynamic

relations of upheaving forces, and the chemical action of vapors issuing

from the fissures.

The form and distribution of continents, that is to say, of that solid

portion of the Earth's surface which is suited to the luxurious development

of vegetable life, are associated by intimate connection and reciprocal

action with the encircling

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sea in which organic life is almost entirely limited to the animal world.

The liquid element is again covered by the atmosphere, an aërial ocean in

which the mountain chains and high plains of the dry land rise like shoals,

occasioning a variety of currents and changes of temperature, collecting

vapor from the region of clouds, and distributing life and motion by the

action of the streams of water which flow from their declivities.

While the geography of plants and animals depends on these intricate

relations of the distribution of sea and land, the configuration of the

surface, and the direction of isothermal lines (or zones of equal mean

annual heat), we find that the case is totally different when we consider

the human race -- the last and noblest subject in a physical description of

the globe. The characteristic differences in races, and their relative

numerical distribution over the Earth's surface, are conditions affected not

by natural relations alone, but at the same time and specially, by the

progress of civilization, and by moral and intellectual cultivation on which

depends the political superiority that distinguishes national progress.

Some few races, clinging, as it were, to the soil, are supplanted and ruined

by the dangerous vicinity of others more civilized than themselves, until

scarce a trace of their existence remains. Other races, again, not the

strongest in numbers, traverse the liquid element, and thus become the first

to acquire, although late, a geographical knowledge of at least the maritime

lands of the whole surface of our globe, from pole to pole.

I have thus, before we enter on the individual characters of that portion of

the delineation of nature which includes the sphere of telluric phenomena,

shown generally in what manner the consideration of the form of the Earth

and the incessant action of electro-magnetism and subterranean heat may

enable us to embrace in one view the relations of horizontal expansion and

elevation on the Earth's surface, the geognostic type of formations, the

domain of the ocean (of the liquid portions of the Earth), the atmosphere

with its meteorological processes, the geographical distribution of plants

and animals, and, finally, the physical gradations of the human race, which

is, exclusively and every where, susceptible of intellectual culture. This

unity of contemplation presupposes a connection of phenomena according to

their internal combination. A mere tabular arrangement of these facts would

not fulfill the object I have proposed to myself, and would not satisfy that

requirement for cosmical presentation awakened in me by the

p 163

aspect of nature in my journeyings by sea and land, by the careful study of

forms and forces, and by a vivid impression of the unity of nature in the

midst of the most varied portions of the Earth. In the rapid advance of all

branches of physical science, much that is deficient in this attempt will,

perhaps, at no remote period, be corrected and rendered more perfect, for it

belongs to the history of the development of knowledge that portions which

have long stood isolated become gradually connected, and subject to higher

laws. I only indicate the empirical path in which I and many others of

similar pursuits with myself are advancing, full of expectation that, as

Plato tells us Socrates once desired, "Nature may be interpreted by reason

alone."*

[footnote] *Plato, 'Phaedo', p. 97. (Arist., 'Metaph.', p. 985.) compare

Hegel, 'Philosophie der Geschichte', 1840, s. 16.

The delineation of the principal characteristics of telluric phenomena must

begin with the form of our planet and its relations in space. Here too, we

may say that it is not only the mineralogical character of rocks, whether

they are crystalline, granular, or densely fossiliferous, but the

geometrical form of the Earth itself, which indicates the mode of its

origin, and is, in fact, its history. An elliptical spheroid of revolution

gives evidence of having once been a soft or fluid mass. Thus the Earth's

compression constitutes one of the most ancient geognostic events, as every

attentive reader of the book of nature can easily discern; and an analogous

fact is presented in the case of the Moon, the perpetual direction of whose

axes toward the Earth, that is to say, the increased accumulation of matter

on that half of the Moon which is turned toward us, determines the relations

of the periods of rotation and revolution, and is probably contemporaneous

with the earliest epoch in the formative history of this satellite. The

mathematical figure of the Earth is that which it would have were its

surface covered entirely by water in a state of rest; and it is this assumed

form to which all geodesical measurements of degrees refer. This

mathematical surface is different from that true physical surface which is

affected by all the accidents and inequalities of the solid parts.*

[footnote] *Bessel, 'Allgemeine Betrachtungen uber Gradmessungen nach

astronomisch-geodätischen Arbeiten', at the conclusion of Bessel and

Baeyer, 'Gradmessung in Ostpreussen', s. 427. Regarding the accumulation of

matter on the side of the Moon turned toward us (a subject noticed in an

earlier part of the text), see Laplace, 'Expos. du Syst. du Monde', p. 308.

The whole figure of the Earth is determined when we know the amount of the

p 164

compression at the poles and the equatorial diameter; in order, however, to

obtain a perfect representation of its form it is necessary to have

measurements in two directions, perpendicular to one another.

Eleven measurements of degrees (or determinations of the curvature of the

Earth's surface in different parts), of which nine only belong to the

present century, have made us acquainted with the size of our globe, which

Pliny names "a point in the immeasurable universe."*

[footnote] *Plin., ii., 68. Seneca, 'Nat. Quaest., Praef., c. ii. "El

mundo espoco" (the Earth is small and narrow), writes Columbus from Jamaica

to Queen Isabella on the 7th of July, 1503: not because he entertained the

philosophic views of the aforesaid Romans, but because it appeared

advantageous to him to maintain that the journey from Spain was not long,

if, as he observes, "we seek the east from the west." Compare my 'Examen

Crit. de l'Hist. de la Geogr. du 15 me Siecle', t.i., p. 83, and t. ii., p.

327, where I have shown that the opinion maintained by Delisle, Freret, and

Gosselin, that the excessive differences in the statements regarding the

Earth's circumference, found in the writings of the Greeks, are only

apparent, and dependent on different values being attached to the stadia,

was put forward as early as 1495 by Jaime Ferrer, in a proposition regarding

the determination of the line of demarkation of the papal dominions.

Cosmos: A Sketch of the Physical Description of the Universe, Vol. 1 · 第 18 / 45 段