By uniting, under one point of view, both the phenomena of our own globe and

those presented in the regions of space, we embrace the limits of the

science of the 'Cosmos', and convert the physical history of the globe into

the physical history of the universe, the one term being modeled upon that

of the other. This science of the Cosmos is not, however, to be regarded as

a mere encyclopedic aggregation of the most important and general results

that have been collected together from special branches of knowledge. These

results are nothing more than the materials for a vast edifice, and their

combination can not constitute the physical history of the world, whose

exalted part it is to show the simultaneous action and the connecting links

of the forces which pervade the universe. The distribution of organic types

in different climates and at different elevations -- that is to say, the

geography of plants and animals -- differs as widely from botany and

descriptive zoology as geology does from mineralogy, properly so called.

The physical history of the universe must not, therefore, be confounded with

the 'Encyclopedias of the Natural Sciences', as they have hitherto been

compiled, and whose title is as vague as their limits are ill defined. In

the work before us, partial facts will be considered only in relation to the

whole.

p 56

The higher the point of view, the greater is the necessity for a systematic

mode of treating the subject in language at once animated and picturesque.

But thought and language have ever been most intimately allied. If

language, by its originality of structure and its native richness, can, in

its delineations, interpret thought with grace and clearness, and if, by its

happy flexibility, it can paint with vivid truthfulness the objects of the

external world, it reacts at the same time upon thought, and animates it, as

it were, with the breath of life. It is this mutual reaction which makes

words more than mere signs and forms of thought; and the beneficent

influence of a language is most strikingly manifested on its native soil,

where it has sprung spontaneously from the minds of the people, whose

character it embodies. Proud of a country that seeks to concentrate her

strength in intellectual unity, the writer recalls with delight the

advantages he has enjoyed in being permitted to express his thoughts in his

native language; and truly happy is he who, in attempting to give a lucid

exposition of the great phenomena of the universe, is able to draw from the

depths of a language, which, through the free exercise of thought, and by

the effusions of creative fancy, has for centuries past exercised so

powerful an influence over the destinies of man.

This material taken from pages 56 to 78

COSMOS: A Sketch of the Physical Description of the Universe, Vol. 1

by Alexander von Humboldt

Translated by E C Otte

from the 1858 Harper & Brothers edition of Cosmos, volume 1

--------------------------------------------------

p 56

LIMITS AND METHOD OF EXPOSITION OF THE PHYSICAL DESCRIPTION OF THE UNIVERSE.

I HAVE endeavored, in the preceding part of my work, to explain and

illustrate, by various examples, how the enjoyments presented by the aspect

of nature, varying as they do in the sources from when they flow, may be

multiplied and ennobled by an acquaintance with the connection of phenomena

and the laws by which they are regulated. It remains, then, for me to

examine the spirit of the method in which the exposition of the 'physical

description of the universe' should be conducted, and to indicate the limits

of this science in accordance with the views I have acquired in the course

of my studies and travels in various parts of the earth. I trust I may

flatter myself with a hope that a treatise of this nature will justify the

title I have ventured to adopt for my work, and exonerate me from the

reproach of a presumption that would be doubly reprehensible in a scientific

discussion.

Before entering upon the delineation of the partial phenomena

p 57

which are found to be distributed in various groups, I would consider a few

general questions intimately connected together, and bearing upon the nature

of our knowledge of the external world and its different relations, in all

epochs of history and in all phases of intellectual advancement. Under this

head will be comprised the following considerations:

1. The precise limits of the physical description of the universe,

considered as a distinct science.

2. A brief enumeration of the totality of natural phenomena, presented

under the form of a 'general delineation of nature.'

3. The influence of the external world on the imagination and feelings,

which has acted in modern times as a powerful impulse toward the study of

natural science, by giving animation to the description of distant regions

and to the delineation of natural scenery, as far as it is characterized by

vegetable physiognomy and by the cultivation of exotic plants, and their

arrangement in well-contrasted groups.

4. The history of the contemplation of nature, or the progressive

development of the idea of the Cosmos, considered with reference to the

historical and geographical facts that have led to the discovery of the

connection of phenomena.

The higher the point of view from which natural phenomena may be considered,

the more necessary it is to circumscribe the science within its just limits,

and to distinguish it from all other analogous or auxiliary studies.

Physical cosmography is founded on the contemplation of all created things

-- all that exists in space, whether as substances or forces -- that is, all

the material beings that constitute the universe. The science which I would

attempt to define presents itself, therefore, to man, as the inhabitant of

the earth, under a two-fold form -- as the earth itself and the regions of

space. It is with a view of showing the actual character and the

independence of the study of physical cosmography, and at the same time

indicating the nature of its relations to 'general physics, descriptive

natural history, geology, and comparative geography', that I will pause for

a few moments to consider that portion of the science of the Cosmos which

concerns the earth. As the history of philosophy does not consist of a mere

material enumeration of the philosophical views entertained in different

ages, neither should the physical description of the universe be a simple

encyclopedic compilation of the sciences we have enumerated. The difficulty

of defining the limits of intimately-connected studies has been increased,

because for centuries it has been customary to designate various branches

p 58

of empirical knowledge by terms which admit either of too wide or too

limited a definition of the ideas which they were intended to convey, and

are, besides, objectionable from having had a different signification in

those classical languages of antiquity from thish chey have been borrowed.

The terms physiology, physics, natural history, geology and geography arose,

and were commonly used, long before clear ideas were entertained of the

diversity of objects embraced by these sciences, and consequently of their

reciprocal limitation. Such is the influence of long habit upon language,

that by one of the nations of Europe most advanced in civilization the word

"physic" is applied to medicine, while in a society of justly deserved

universal reputation, technical chemistry, geology and astronomy (purely

experimental sciences) are comprised under the head of "Philosophical

Transactions."

An attempt has often been made, and almost always in vain, to substitute new

and more appropriate terms for these ancient designations, which,

notwithstanding their undoubted vagueness, are now generally understood.

These changes have been proposed, for the most part, by those who have

occupied themselves with the general classification of the various branches

of knowledge, from the first appearance of the great encyclopedia

('Margarita Philosophica') of Gregory Reisch,* prior of the Chartreuse at

Freiburg, toward the close of the fifteenth century, to Lord Bacon, and from

Bacon to D'Alembert; and in recent times to an eminent physicist, Andre

Marie Ampere.**

[footnote] *The 'Margarita Philosophica' of Gregory Reisch, prior of the

Chartreuse at Freiburg, first appeared under the following title: Aepitome

omnis Philosophiæ, alias Margarita Philosophica, tractans de omni generi

scibili. The Heidelberg edition (1486), and that of Strasburg (1504), both

bear this title, but the first part was suppressed in the Freiburg edition

of the same year, as well as in the twelve subsequent editions, which

succeeded one another, at short intervals, till 1535. This work exercised a

great influence on the diffusion of mathematical and physical sciences

toward the beginning of the sixteenth century, and Crasles, the learned

author of 'L'Aperçu Historique des Methodes en Géometrica' (1837) has

shown the great importance of Reisch's 'Encyclopedia' in the history of

mathematics in the Middle Ages. I have had recourse to a passage in the

'Margarita Philosophica', found only in the edition of 1513, to elucidate

the important question of the relations between the statements of the

geographer of Saint-Die, Hylacomilus (Martin Waldseemuller), the first who

gave the name of America to the New Continent, and those of Amerigo

Vespucci, Rene, King of Jerusalem and Duke of Lorraine, as also those

contained in the celebrated editions of Ptolemy of 1513 and 1522. See my

'Examen Critique de la Gegraphie du Nouveau Continent, et des Progres de

l'Astronomie Nautique aux 15e et 16e Siecles', t. iv., p. 99-125.

[footnote] II Ampère, 'Essai sur la Phil. des Sciences', 1834, p. 25.

Whewell, 'Philosophy of the Inductive Sciences', vol. ii., p. 277. Park,

'Pantology', p. 87.

p 59

The selection of an inappropriate Greek nomenclature has perhaps been even

more prejudicial to the last of these attempts than the injudicious use of

binary divisions and the excessive multiplication of groups.

The physical description of the world, considering the universe as an object

of the external senses, does undoubtedly require the aid of general physics

and of descriptive natural history, but thecontemplation of all created

things, which are linked together, and form one 'whole', animated by

internal forces, given to the science we are considering a peculiar

character. Phyical science considers only the general properties of bodies;

it is the product of abstraction -- a generalization of perceptible

phenomena; and even in the work in which were laid the first foundations of

general physics, in the eight books on physics of Aristotle,* all the

phenomena of nature are considered as depending upon the primitive and vital

action of one sole force, from which emaate all the movements of the

universe.

[footnote] * All changes in the physical world may be reduced to motion.

Aristot., 'Phys. Ausc.', iii., 1 and 4, p. 200, 201. Bekker, viii., 1, 8,

and 9, p. 250, 262, 265. 'De Genere et Corr.', ii., 10, p. 336.

Pseudo-Aristot., 'De Mundo.' cap. vi., p. 398.

The terrestrial portion of physical cosmography, for which I would willingly

retain the expressive designation of 'physical geography', treats of the

distribution of magnetism in our planet with relation to its intensity and

direction, but does not enter into a consideration of the laws of attraction

or repulsion of the poles, or the means of eliciting either permanent or

transitory electro-magnetic currents. Physical geography depicts in broad

outlines the even or irregular configuration of continents, the relations of

superficial area, and the distribution of continental masses in the two

hemispheres, a distribution which exercises a powerful influence on the

diversity of climate and the meteorological modifications of the atmosphere;

this science defines the character of mountain chains, which, having been

elevated at different epochs, constitute distinct systems, whether they run

in parallel lines or intersect one another; determines the mean height of

continents above the level of the sea, the position of the center of gravity

of their volume, and the relation of the highest summits of mountain chains

to the mean elevation of their crests, or to their proximity with the

sea-shore. It depicts the eruptive rocks as principles of movement, acting

upon the sedimentary rocks by traversing, uplifting, and inclining them at

various angles; it

p 60

considers volcanoes either as isolated, or ranged in single or in double

series, and extending their sphere of action to various distances, either by

raising long and narrow lines of rocks, or by means of circles of commotion,

which expand or diminish in diameter in the course of ages. This

terrestrial portion of the science of the Cosmos describes the strife of the

liquid element with the solid land; it indicates the features possessed in

common by all great rivers in the upper and lower portion of their course,

and in their mode of bifurcation when their basins are unclosed; and shows

us rivers breaking through the highest mountain chains, or following for a

long time a course parallel to them, either at their base, or at a

considerable distance, where the elevation of the strata of the mountain

system and the direction of their inclination correspond to the

configuration of the table-land. It is only the general results of

comparative orography and hydrography that belong to the science whose true

limits I am desirous of determining, and not the special enumeration of the

greatest elevations of our globe, of active volcanoes, of rivers, and the

number of their tributaries, these details falliing rather within the domain

of geography, properly so called. We would here only consider phenomena in

their mutual connection, and in their relations to different zones of our

planet, and to its physical constitution generally. The specialties both of

inorganic and organized matter, classed according to analogy of form and

composition, undoubtedly constitute a most interesting branch of study, but

they appertain to a sphere of ideas having no affinity with the subject of

this work.

The description of different countries certainly furnishes us with the most

important materials for the composition of a physical geography; but the

combination of these different descriptions, ranged in series, would as

little give us a true image of the general conformation of the irregular

surface of our globe, as a succession of all the floras of different regions

would constitute that which I designate as a 'Geography of Plants.' It is

by subjecting isolated observations to the process of thought, and by

combining and comparing them, that we are enabled to discover the relations

existing in common between the climatic distribution of beings and the

individuality of organic forms (in the morphology or descriptive natural

history of plants and animals); and it is by induction that we are led to

comprehend numerical laws, the proportion of natural families to the whole

number of species, and to designate the latitude or geographical position of

the zones in whose

p 61

plains each organic form attains the maximum of its development.

Considerations of this nature, by their tendency to generalization, impress

a nobler character on the physical description of the globe, and enable us

to understand how the aspect of the scenery, that is to say, the impression

produced upon the mind by the physiognomy of the vegetation, depends upon

the local distribution, the number, and the luxuriance of growth of the

vegetable forms predominating in the general mass. The catalogues of

organized beings to which was formerly given the pompous title of 'Systems

of Nature', present us with an admirably connected arrangement by analogies

of structure, either in the perfected development of these beings, or in the

different phases which, in accordance with the views of a spiral evolution,

affect in vegetables the leaves, bracts, calyx, corolla and fructifying

organs; and in animals, with more or less symmetrical regularity, the

cellular and fibrous tissues, and their perfect or but obscurely developed

articulations. But these pretended systems of nature, however ingenious

their mode of classification may be, do not show us organic beings as they

are distributed in groups throughout our planet, according to their

different relations of latitude and elevation above the level of the sea,

and to climatic influences, which are owing to general and often very remote

causes. The ultimate aim of physical geography is, however, as we have

already said, to recognise unity in the vast diversity of phenomena, and by

the exercise of thought and the combination of observations, to discern the

constancy of phenomena in the midst of apparent changes. In the exposition

of the terrestrial portion of the Cosmos, it will occasionally be necessary

to descend to very special facts; but this will only be in order to recall

the connection existing between the actual distribution of organic beings

over the globe, and the laws of the ideal classification by natural

families, analogy of internal organization and progressive evolution.

It follows from these discussions on the limits of the various sciences, and

more particularly from the distinction which must necessarily be made

between descriptive botany (morphology of vegetables) and the geography of

plants, that in the physical history of the globe, the innumerable multitude

of organized bodies which embellish creation are considered rather according

to 'zones of habitation' or 'stations', and to differently inflected

'isothermal bands', than with reference to the principles of gradation in

the development of internal organism. Notwithstanding this, botany and

zoology, which constitute

p 62

the descriptive natural history of all organized beings, are the fruitful

sources whence we draw the materials necessary to give a solid basis to the

study of the mutual relations and connection of phenomena.

We will here subjoin one important observation by way of elucidating the

connection of which we have spoken. The first general glance over the

vegetation of a vast extent of a continent shows us forms the most

dissimilar -- Graminae and Orchideae, Coniferae and oaks, in local

approximation to one another; while natural families and genera, instead of

being locally associated, are dispersed as if by chance. This dispersion

is, however, only apparent. The physical description of the globe teaches

us that vegetation every where presents numerically constant relations in

the development of its forms and types; that in the same climates, the

species which are wanting in one country are replaced in a neighboring one

by other species of the same family; and that this 'law of substitution',

which seems to depend upon some inherent mysteries of the organism,

considered with reference to its origin, maintains in contiguous regions a

numerical relation between the species of various great families and the

general mass of the phanerogamic plants constituting the two floras. We

thus revealed in the multiplicity of the distinct organizations by which

these regions are occupied; and we also discover in each zone, and

diversified according to the families of plants, a slow but continuous

action on the aerial ocean, depending upon the influence of light -- the

primary condition of all organic vitality -- on the solid and liquid surface

of our planet. It might be said, in accordance with a beautiful expression

of Lavoisier, that the ancient marvel of the myth of Prometheus was

incessantly renewed before our eyes.

If we extend the course which we have proposed, following in the exposition

of the physical description of the earth to the sidereal part of the science

of the Cosmos, the delineation of the regions of space and the bodies by

which they are occupied, we shall find our task simplified in no common

degree. If, according to ancient but unphilosophical forms of nomenclature,

we would distinguish between 'physics', that is to say, general

considerations on the essence of matter, and the forces by which it is

actuated, and 'chemistry', which treats of the nature of substances, their

elementary composition, and those attractions that are not determined solely

by the relations of mass, we must admit that the description of the earth

comprises at

p 63

once 'physical' and 'chemical' actions. In addition to gravitation, which

must be considered as a primitive force in nature, we observe that

attractions of another kind are at work around us, both in the interior of

our planet and on its surface. These forces, to which we apply the term

'chemical affinity', act upon molecules in contact, or at infinitely minute

distances from one another,* and which, being differently modified by

electricity, heat, condensation in porous bodies, or by the contact of an

intermediate substance, animate equally the inorganic world and animal and

vegetable tissues.

[footnote] * On the question already discussed by Newton, regarding the

difference existing between the attraction of masses and molecular

attraction, see Laplace, 'Exposition du Systeme du Monde', p. 384, and

supplement to book x. of the 'Mecanique Celeste', p. 3, 4; Kant, 'Metaph.

Anfangegrunde der Naturwissenschaft, Säm. Werke', 1839, bd. v., s. 309

(Metaphysical Principles of the Natural Sciences); Pectet, 'Physique', 1838,

vol. i., p. 59-63.

If we except the small asteroids, which appear to us under the forms of

aerolites and shooting stars, the regions of space have hitherto presented

to our direct observation physical phenomena alone; and in the case of

these, we know only with certainty the effects depending upon the

quantitative relations of matter of the distribution of masses. The

phenomena of the regions of space may consequently be considered as

influenced by simple dynamical laws -- the laws of motion.

The effects that may arise from the specific difference and the

hererogeneous nature of matter have not hitherto entered into our

calculations of the mechanism of the heavens. The only means by which the

inhabitants of our planet can enter into relation with the matter contained

within the regions of space, whether existing in scattered forms or united

into large spheroids, is by the phenomena of light, the propagation of the

force of gravitation or the attraction of masses. The existence of a

periodical action of the sun and moon on the variations of terrestrial

magnetism is even at the present day extremely problematical. We have no

direct experimental knowledge regarding the properties and specific

qualities of the masses circulating in space, or of the matter of which they

are probably composed, if we except what may be derived from the fall of

aerolites or meteoric stones, which, as we have already observed, enter

within the limits of our terrestrial sphere. It will be sufficient here to

remark, that the direction and the excessive velocity of projection (a

velocity wholly planetary) manifested by these masses, render it more than

probable that

p 64

they are small celestial bodies, which, being attracted by our planet, are

made to deviate from their original course, and thus reach the earth

enveloped in vapors, and in a high state of actual incandescence. The

familiar aspect of these asteroids, and the analogies which they present

with the minerals composing the earth's crust, undoubtedly afford ample

grounds for surprise,* but, in my opinion, the only conclusion to be drawn

from these facts is that, in general, planets and other sidereal masses,

which by the influence of a central body, have been agglomerated into rings

of vapor, and subsequently into spheroids, being integrant parts of the same

system, and having one common origin, may likewise be composed of substances

chemically identical.

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