COMPARATIVE
GEOGRAPHY.

BY
CARL RITTER
LATE PROFESSOR OF GEOGRAPHY IN THE UNIVERSITY OF BERLIN.

Translated for the Use of Schools and Colleges

BY
WILLIAM L. GAGE.

PHILADELPHIA:
J. B. LIPPINCOTT & CO.
1865.

Entered, according to Act of Congress, in the year 1865, by
J. B. LIPPINCOTT & CO.,
In the Clerk’s Office of the District Court of the United States
for the Eastern District of Pennsylvania.

TRANSLATOR’S PREFACE.

The translator of Ritter’s “Geographical Studies,” which has received in its English dress the hearty greeting of our most cultured scholars, takes a renewed pleasure in giving to the students of our higher Seminaries a second volume from the pen of the great Geographer. The former work, addressed, as its contents mainly were, to the members of the Royal Academy of Berlin, was too recondite in thought and too abstruse and elaborate in statement ever to become, whether in German or in English, a popular work; but the present volume—the bright, compact crystal of Ritter’s life—will pass into a general circulation, and will be recognized as not merely a simple and perfectly intelligible treatise, but as a masterly application of the comparative method of Geography, and as philosophical as it is practical and interesting.

Besides the voluminous Erdkunda, which deals almost exclusively with Asia, and treats it with an exhaustive fullness, Ritter has left the world the volume already referred to, and three courses of Academical Lectures. One of these courses is now before the reader; one of the remaining two relates to the geography of Europe, and the other to the history of Geographical Science and of Discovery. Of these three courses, a distinguished American scholar[1] has said: “Free from excessive details, systematic, clear, bold, and fresh, they are better fitted to bring up to the mind Ritter, the university instructor, than all his other writings.” This praise is by no means excessive; and the student who shall, with the assistance of a good physical atlas, go through this work, will find himself master of a far larger number of special facts than the size of the volume would indicate; and also of a science of Geography, which subsidizes all detail, and makes it auxiliary to the comprehension of relations no less beautiful and singular than are revealed in the study of the other departments of Nature.

The peculiar difficulties attending the translation of the Geographical Studies have not been met in this volume; in the University lecture-room, Ritter’s style, which, before the Royal Academy, was extremely involved, poetical and inexhaustive, became simple, straightforward, and luminous. In style, Ritter carried neglect to the point of slovenliness; and the finish which Humboldt cultivated so assiduously, he rejected as unworthy of a true scholar. The highly figurative words with which he used so liberally to decorate his writings, I have generally had to render with a rather too bare fidelity to a prose style; for grateful and captivating as they were to his German hearers, they would look over-fanciful to an English reader, and obscure rather than illustrate the thought. It has been my earnest purpose to make this work fill a great void in our educational literature; and its convenient size gives it an incomparable advantage over the voluminous works of Sir John Herschel and Mrs. Somerville; while in rigid philosophical precision, in method, in natural growth—not to use that inevitable German word development, (Entwickelung)—even those eminent geographers would, doubtless, award it the palm.

The demands of the public may yet render needful the translation of other of Ritter’s works; meanwhile, the editor of this work purposes to prepare a biography of that great man, whose memory all his pupils revere, and whose life was not less beautiful to his friends than it was fruitful and valuable to the whole scientific world.

W. L. G.

July 5, 1864.

CONTENTS.

INTRODUCTION.

The subject of these lectures is Geography in its most enlarged and comprehensive sense. It will be necessary to preface them with some general observations, which shall serve to indicate the scientific basis on which the discussion will rest. Our starting-point will be with Nature herself and not with arbitrary geographical systems hitherto constructed.

By the word Nature will be meant the entire Creation. The grasping of Nature in all its objects and all its forces becomes, in conjunction with the agency of Time and Space, the comprehension of a great system. The inanimate creation may be represented under the term inorganic, the animate creation under the term organic. Yet there is not an absolute contrast between them; for in both there is ceaseless progress, no pause, but in a higher and comprehensive sense a cosmical life, the whole forming one great Organism, in which the inorganic world, so called, is only the foundation on which the animate creation stands.

To us, our own Earth is the most marked feature of Nature viewed on its inorganic side. To us it is the planet best known of all, or rather the only one closely known, the point whence we draw conclusions on the whole Universe, the resting ground for the glass that searches the Kosmos, to use Humboldt’s word, discerning the place which the Earth holds in it, and prying into the mysteries of the entire creation. Our globe is one of the major planets of our system, all of which gird the sun with great elliptic orbits, midway in which is our own. There begins the first popular division of the planets,—those that are within and those which are without our own orbit. This is one of the most simple of discriminations, one which we inherit from the ancients in an unmodified form. Humboldt retains this primary classification.

The external planets are those whose orbits embrace that of the Earth within their own. The minor planets are those whose orbits are embraced by that of the Earth. These are Mercury and Venus.

The ancients, counting both the sun and moon, reckoned only seven planets. At the end of the eighteenth century another was added, Uranus, an external planet. Through the instrumentality of improved telescopes, soon after, four minor ones were discovered, Ceres, Pallas, Juno, and Vesta; and by the still more perfect lenses recently introduced, and the assiduity and skill of astronomers, the number of these little planetary bodies, ranging between the orbits of Mars and Jupiter, has grown great. Beyond Saturn and Uranus is Neptune, discovered mathematically by Le Verrier, in Paris, and seen by Galle in Berlin, the 23d of September, 1846.

To these (now eighty) planets may be added the twenty to thirty moons of our solar system, and a number of comets.

The middle position of the Earth’s orbit is not without its consequences. The distance of the Earth from the Sun is, in round numbers, 92,000,000 of miles, nearly three times as far as that of Mercury, the planet nearest the Sun. Jupiter, on the other hand, is five times as far from the Sun as the Earth; Uranus about nineteen times as far, and Neptune about thirty-three times as far.

The time of the Earth’s revolution around the Sun is also equally removed from the extremes; its year is 365 days; Mercury’s being 87 days; Jupiter’s 11 of our years; Uranus 84 years; and Neptune’s 165 years.

The daily revolution of the Earth on its axis is also of only medium swiftness, consuming 24 hours. This, of course, controls the periods of waking and sleep of the entire animate creation on our globe. Some planets revolve slower, some more rapidly than our own; Jupiter’s revolution, for example, is accomplished in little less than 10 hours. This extreme rapidity seems to account for the much greater flattening at the poles of the planets than the Earth exhibits, occasioned doubtless during the formation processes, while those immense revolving masses were passing from their primitive fluid state into the more rigid forms in which we know them. Of all the planets, however, the Earth has most perfectly retained the spherical shape; and the spherical form is in one sense a medium form; i.e. it is removed from all extremes of angularity, and so falls in with the analogies which I am endeavoring to establish, springing from the position of the Earth’s orbit midway between those of the inner and outer planets. According to Plato, the beauty of form lies in symmetry, and our Earth is the most symmetrical of planets, and, unquestionably, the spherical shape is the one best adapted to the display of the largest number of phenomena possible.

The variations from the spherical form, produced by elevations and depressions, are only of medium magnitude in our globe compared with many others in our system. On the smaller planet of Venus, for example, the mountains are thought to rise to a height of many miles, while five is the greatest altitude of ours. According to Mädler’s conjectures, the mountains in our own moon rise to a height of over three miles, an altitude altogether out of proportion to the size of the moon as compared with the earth.

In respect to the number of its moons, too, our Earth is no extremist; it has but one: other planets, Mercury, Venus, Mars, have none. On the other hand, Jupiter has 4, Saturn 7, Uranus 6 at least, and doubtless more. The general law seems to be, the farther from the Sun the greater the number of moons; perhaps in the wonderful providence of God, to compensate the feeble light of those distant realms by the number of the reflecting bodies.

Now, summing up all that has been said, it will be seen that the Earth is equally far removed from every extreme. This fundamental classification, drawn from the place of its orbit in relation to those nearer the Sun or more distant from it, gives it a character which is felt and seen in many different things, and responds to analogies which it is not incorrect to mark. A medium is seen in all its attributes and relations: it is neither the largest nor the smallest of planets; neither the swiftest nor the slowest; neither the warmest nor the coldest; in nothing is it either at a minimum nor at a maximum point. And this very medium character brings the Earth into harmony with the system of which it forms a part; the symmetry of the one corresponding with the symmetry of the other, and specially fits it to become the temporary home of a race like ours, which makes the whole surface of the globe tributary during the short terrestrial life of man to his preparation for a celestial state of being. Our globe is certainly the only one of our system which could possibly be inhabited by man; and as his residence, and as the arena for his culture, it is worthy of being studied in all its features; no point is too trifling to be overlooked.

As man looks for a center to the system which evidently pertains to him, and in which our Earth plays no slight part, the Sun is clearly the source of a large share of what makes our life desirable. Thence we receive light, warmth, and indirectly, and yet directly too, life and the bloom of health. Nor can men, even if ignorant and degraded, help seeing the relation of the Sun to the Earth, and linking, in their rude thoughts, the heavens with the earth; and hence, before all higher Revelation, the worship of the Sun has been the primitive instinct of the oldest of nations.

Looking at the earth as simply one among the innumerable hosts of heaven, it, like each one of them, becomes to the imagination a mere point of light, a “star among stars.” But, when we shift our point of view, and leaving the cosmical or universal for the special, for what pertains to the individual life, the mere point of light flames up into a great, busy world, full of phenomena demanding investigation and thought. And yet this world, so attractive in its multiplicity of details, is almost a chaos at the first sight; a confused and inextricable mass, so large, so high, so deep as to defy human effort to compass or master it. Science alone, the gift and the growth of centuries, can measure the field; science alone can enter it and reduce the chaos to a beautiful and orderly grouping, and make a perfect picture of the whole; it alone can dispel crude ideas and give truer ones in their stead. To the rude dweller on the plain, the earth seems a gigantic floor, as it did to many a tribe in the past, and as it does to-day to thousands of wondering Arabs. The South Sea Islander, in the Pacific, takes his island or island group to be the whole earth; the world he considers an endless ocean plain, from which the Sun arises, and, when the day is over, into which it sinks. And even within the pale of civilization itself, the ignorant Neapolitan lazzarone considers his gulf the center of the world.

As men advance in their inquiries, and, ascending the sides of mountains, look out over a larger tract, or find new lands across the seas, they do not outgrow their first idea, the world merely expands from the narrow homestead to a larger circle, such as the Romans used to call their orbis terrarum. The conception of the earth as a vast, unsupported ball, careering through the heavens, was the possession, slowly won, of such great minds as Pythagoras and Aristotle, and slowly found its way among the ideas which whole nations accepted as true. Circumnavigators must sail around the globe and tell their story to the world before the conjectures of science could have real weight with the popular mind in a matter so remote from the crude speculations of the ignorant as this. And less than one century and a half ago (in 1727) another step was taken, and the theory was propounded by Newton, that the Earth is a spheroid and not a perfect sphere. Later investigations have determined that the spheroidal form is only an approximation to perfect accuracy, and that the Earth is a polyhedron, whose exact number of zodes has not yet been determined, and which may prove indeterminable. Bessel has assigned, as the great task of science for the coming century, to settle this question with perfect exactness. But what has been said is enough to indicate that in our knowledge, at present, certainly there is only progress, only approximation, no absolute exhaustion of the processes of discovery.

And just as in ruder lands each man looks at his own island, or village, as the center of the earth’s circle, so the ancients looked at the earth as the pivot of the universe, the central point around which all the heavenly hosts revolve. That was the fundamental principle of that Ptolemaic system which was older than Ptolemy; held in the most ancient times in Arabia, Babylon, Persia, and India, but first luminously expanded in the proportions and with the dignity of a system by Ptolemy. Its outlines were, in one word, this: there are seven planets, the Moon, Mercury, Venus, the Sun, Mars, Jupiter, and Saturn; each has its own orbit, in which it is in a limited sense supreme, but they all revolve around the common center, the Earth. Beyond the seven, and including them all, is the Firmament, in which the other stars stand like golden nails in an imperishable floor; the whole vast external Firmament is opaque and motionless.

The Ptolemaic system won and held the greatest regard in the ancient world. Mohammed established it in the Koran as a truth of religion. The advance of science revealed the falseness of the Ptolemaic scheme of the universe, and demonstrated the fact that the stars of heaven are not mere torch-bearers for us, and mere interpreters of human destinies, but are worlds like our own, our earth being but one of numberless thousands equally worthy of the Common Creator. The Copernican system, which was to re-create the whole domain of science, wrought this great change. The Sun, according to this theory, forms the central point around which, and not around the Earth, all the planets wheel. Copernicus, in 1543, left this imperfect and yet fruitful conception to his successors to unfold; and in the results gained by Kepler, in 1631, by Newton and Galileo, 1727, the Copernican system was firmly established. The vast improvements in the telescope removed the limits of the visible universe to a place till then unrevealed, and added inexhaustible fields to those which had been known before. The number of the planets was enlarged. The list of determined comets increases yearly. The number of the fixed stars has been determined by the extreme accuracy of such observers as Lalande, Lacaille, Bessel, Argelander, and Lamont. The great work of mapping and cataloguing the heavens has been accomplished. Many hundred stars, supposed to be single fixed stars, have been ascertained to be double stars, and some have been resolved into systems like our own. The 300-400, observed by Struve, have grown, through the labors of Herschel, in both the Northern and the Southern hemispheres, at the Cape of Good Hope, and elsewhere, to over 3000, and the number is constantly increasing. Nebulæ have been analyzed, and been shown to consist of worlds distinct and perfect as our own. Thus there is a steady and perceptible advance in man’s conception of the Earth, of Nature, of what we call the World and the Universe, though each individual, generation, and century are but dimly conscious of this progress.

The Earth as the Dwelling-place of Man.

The Earth draws our attention to itself, however, not as simply a unit in the planetary system, but as the home of the human race. The physical description of the globe includes the relations of the Earth as a star amid the heavenly hosts, while Geography, taken most comprehensively, regards the Earth as the dwelling-place of Man. From a geographical point of view, the world becomes to us the common home of our race, the theater, not of the operations of Nature in the most unrestricted sense, but the arena for the development of human life and history. The whole animate and inanimate creation is tributary, looked at geographically, to the fashioning of the destiny of Man. Without Man as the central point, Nature would have no interest to the geographer; without the Earth, constituted just as it is, the races of men and the course of human history could not claim his attention. The Earth is not only the best known of planets, but, as the home of man, infinitely the most interesting. The study of it is at the foundation of history as much as of physics.

No man of science can fail to regard it with the deepest interest.

More than a hundred years ago, George Foster remarked that European culture had ascended to that height, that it must include an intimate knowledge of all that is peculiar in the features and phenomena of the entire globe. How much more true is this remark in the middle of our nineteenth century! It is no longer European culture that demands this, but the welfare of all countries claims of scholars this knowledge far more imperatively than a hundred years ago. Still, it must be confessed that we are far from the attainment of a perfect science of Geography, in its largest sense; the science which regards the Earth as the field of human discipline; the science of which what was formerly called Geography is only an outlying, rudimentary part. The compass of what it holds as its goal is too large, and its contents too varied for his grasp whose existence is hemmed in by narrow bonds, and whose life is so brief. And though there have always been detailed descriptions of the different parts of the earth, many of them remarkable for their accuracy, yet there has been lacking a knowledge of the principle of organic unity which pervades the whole, and the mutual play and interdependency of all the parts. The whole subject of relations was unstudied. And it is a knowledge of the relations of things that leads to a scientific interpretation, not the description of detached parts. Geography was and continued to be mere description, not the teaching of the most important relations. Only now are we beginning to comprehend the true elements of geographical science, only now are the first efforts made to deal profoundly with this science, although the progress of discovery is still going on with unabated speed, leaving far behind us all the advances of our predecessors.

Geography as a Science.

The Earth, considered per se, is only a fragment of the Universe, of the Kosmos, in that wide use of the word which Humboldt has given to it in his celebrated work. The Earth is the grand floor, so to speak, of Nature; the home, or rather the cradle, of men and of nations, the dwelling-place of our race. It is not merely a region of immense spaces, a vast superficies, it is the theater where all the forces of Nature and the laws of Nature are displayed in their variety and independencies. Besides this, it is the field of all human effort, and the scene of a Divine revelation. The Earth must be studied, therefore, in a threefold relation: to the Universe, to Nature, to History.

And it is not only as a mere passive agent, but active, that it assumes this threefold relation. It is an inseparable, an integral, a working member in the great system of things. But higher than this, and grander than its relation to the system of things, is its relation to an unseen world, to an unseen hand, even that of the Creator. We view it not as the field of forces and laws and phenomena, but the crowning gift of God, displaying the tokens of perfect adaptation to our wants, full of beauty and excellence—a revelation of Divine wisdom, in the form of a visible world. How beautifully has the inspired David painted this in the 104th Psalm!

In relation to its inhabitants, crowned with the Imperial gift of reason, the Earth is not merely the place where they may stand, the cradle where they may sleep, the home where they may live, it is the school where they may be trained. This is one of the first and one of the greatest lessons that we learn from the history of the race. The Earth finds its highest mission, not in its relation to inanimate nature, but to the world of intelligence—the minds that dwell upon it, the spiritual world to which it gives bodies. And as the Earth alone of the planets is adapted to be the home of such a being as man, so in our world of animate and inanimate things, man alone partakes of a moral nature, incapable of being shared or even imitated by the lower creatures. The Earth was made to be the home of mind, soul, character. And Man was created to make this earth tributary to his largest growth in mind, and soul, and character. In this sense the Earth and its noble possessors are correlative. Each individual rises to his own appointed work, runs his own course, uses all the appliances of Nature, all the help with which God invests him, and then ceases from his mission here; but the Earth remains, the home of the advancing millions, helping them all onward, and granting them new power to fulfill the noble purposes of human life.

Nor can this constitution of things be the result of a happy accident. Evidently under the supreme power of a Divine mind and will, Nature is made subservient to Man. That mutual working and interdependence of things, which opens to our comprehension the History of our race, cannot be ascribed to a fortuitous combination of events. It can only be the result of Divine Providence. Had there been no wise ruling of the blind forces of nature, no subjection of the rough, unbridled powers of the air, and sea, and earth, the human race would have become extinct, as so many races of beasts have done. But there are no traces of the extinction of a human race in our Paleontology. The constitution of the globe is incontestably coincident with a plan to preserve and perfect Man. There are destructive agencies, it is true, but they do not operate on an extended scale; our earthquakes, and volcanoes, and great storms at sea affect but a fraction of the race, they are no longer universal in their action; while, on the contrary, the instrumentalities which favor mankind remain in force—the earth’s changeless garment of green, the uniform progress of generation among subordinate creatures, the ease of acclimatization, and of transferring seeds and germs, with undiminished fruitfulness, from one region to another. The very agencies which, in the dawn of history, brought death, have been changed to auxiliaries of life with us to-day.

The investigation into the relations of the Earth, in this respect, and into the organization of all the natural laws and phenomena in their bearing on man, his life and history, must constitute a prominent department of true geographical science. When Geography ceases to be a lifeless aggregate of unorganized facts, and becomes the science which deals with the earth as a true organization, a world capable of constant development, carrying in its own bosom the seeds of the future, to germinate and unfold, age after age, it first attains the unity and wholeness of a science, and shows that it grows from a living root; it becomes capable of systematic exposition, and takes its true place in the circle of sister sciences. Philosophy gladly grants it a share in its own domain, and permits it to indulge in those soaring speculations, which it used to be thought that so simple a thing as Geography might not enjoy. Yet, it must not be denied that there has for some time been felt a need of bringing the earth, as an organization, more into the light of scientific investigation. The study of final causes, the tracing of infinite wisdom in the works of the Creator, the theories touching the first issue of all things, have grown out of this necessity. Many errors have, doubtless, drifted in during the course of these speculations; man has undertaken to measure the Divine plan with most imperfect data, and the illusion has been too fondly cherished of attaining final and profound results while men were scarcely in the possession of the elements of knowledge. It is for us, therefore, to enter upon our inquiries with investigation rather than theory, to test the knowledge of which tradition has put us in possession, and to advance, as we may, to the new and the unexplored.

Man is the first token that we meet, that our study of the earth must contemplate it as an organized whole, its unity consummating in him. As every individual must, in his own career, epitomize the history of the race, childhood, youth, manhood, and decrepitude, so each man mirrors in his own life the locality where he lives. Whether dwelling in the North or in the South, in the East or in the West, whether the shepherd of the Tyrolese Highlands, or the Hollander of the plains, every man is, in a manner, the representative of the home that gave him birth. In the people the country finds its reflection. The effect of the district upon the nature of its inhabitants in size and figure, in color and temperament, in speech and mental characteristics, is unmistakable. Hence the almost infinite diversity in the peculiarities of culture and attainment, as well as of tendency in different nations. Anthropology and Ethnography, the science of man and of race, are the running commentaries of Geography and Topography. The historian and the geographer work toward each other,—the historian going back from the acts of men to study the scenes which have conditioned their life, the geographer going forward from the study of the habitat of men to that of their deeds. The fundamental question of history is, in fact, What relation does the country bear to the national life? What relation to the civil structure, the state?

In fact, the whole constitution of Man is thoroughly connected with the Earth on which he dwells; the roots of his being run down into it in uncounted numbers. Man receives at birth from the earth not only a spiritual but a physical dowry, from which he cannot free himself, and of whose worth he becomes conscious more and more. It is, therefore, of course one of the first of the legitimate studies to learn the limits of the realm which Man makes his home, and to understand all its secrets, all its forces, so as to turn them to his own uses. Thus alone can he compass the sublime thought of his own freedom, the independence of his own will in the kingdom of Nature, and learn the majesty of his own spirit; for the knowledge of that freedom, which is the most noble of all God’s gifts to him, is the most direct key to the attainment of that place in the present, and that destiny in the future, which God has appointed for man. Without a preliminary training, amid the conditions of a limited life, can there be no step taken toward the enjoyment of the life without limitations which is to come. Without the capacity of breaking the higher law, there is no glory in obeying it, no freedom to be valued, even in the world of thought. There can be no true speculation, no philosophy of the unlimited and eternal, without inquiry into and knowledge of the limited and conditioned. He who knows not the earthly, cannot know the heavenly; he who knows not the finite, cannot know the infinite. Statement and counter-statement are the substance to the world of thought. Pythagoras investigated matters of number and weight, before he dealt with the mysteries of metaphysical speculation. Plato thought on the human soul, and the practical details of legislation, before he gave himself to the deepest things of Philosophy. Aristotle was a naturalist and physicist, before he became a logician and metaphysician. Kant was a mathematician and astronomer, before he dealt with the problems of transcendental science. Schelling went from natural philosophy to the study of the soul of things. If there have been evil results from this, it has not been from antedating metaphysical studies by physical, but by passing too quickly from the solid foundation-stones to the more unstable heights of the transcendental. Without these solid foundation-stones, philosophy falls, crushed by its own weight; but with this preparation, we may advance to the loftiest and yet most secure speculations.

What Geography as a Science has yet to accomplish.

Geography can just as little be contented with being a mere description of the Earth, and a catalogue of its divisions, as a detailed account of the objects in nature can take the place of a thorough and real natural history. The very word Geography, meaning a description of the Earth, has unfortunately been at fault, and has misled the world: to us it merely hints at the elements, the factors of what is the true science of Geography. That science aims at nothing less than to embrace the most complete and the most cosmical view of the Earth; to sum up and organize into a beautiful unity all that we know of the globe. The whole body of facts revealed by past and present discovery must be marshaled into harmony, before we gain the high pinnacle of Geographical Science. The Earth, in all its parts, must be known in all its relations, before we can speak of it as the scholars of our day ought to speak of the world they inhabit.

Moreover, the Earth is to be considered in two main relations—a relation, and an absolute relation; that is, we are to regard it in its connection with the greater whole, of which it forms a part, the Universe, and as a body standing alone, existing, as it were, for itself. It is the latter view which falls within the strict province of Geography. The very prominence of the old Greek word Γη indicates the pre-eminence which, in this science, our own planet, rather than others, receives. Ge-ography confines our attention to the Earth, and concentrates it upon the globe, regarded per se, rather than in its relations to the Universe. Taken, therefore, strictly, as already hinted at in the foregoing remark, Geography is the department of science that deals with the globe in all its features, phenomena, and relations, as an independent unit, and shows the connection of this unified whole with man and with man’s Creator. Should we go beyond this, and discuss the relations of the Earth to the Universe, (as is often done in our geographical treatises, in a singularly imperfect and unfruitful manner,) we should outrun the strict bounds of a single science, and should be encroaching on the domain of the sister science of astronomy. This we have no right to do. Yet, from time to time, we must borrow the results of other departments of learning to confirm our own. The field which we have to till has been immensely reduced in its proportions by the publication of “Kosmos,” which great work has almost exhausted the subject of the earth in its external relations. The limiting of our own department may, perhaps, give more opportunity for thorough investigation within itself.

The Earth, if discussed exhaustorily, must be spoken of in its relations to Time as well as to Space. The word by which we characterize it, in this regard, is History. The duration of the Earth outruns all measurement. By thinking of its beginning, is the only way we have of gaining a conception of Time. We cannot conceive of the universe as antedating the creation of our earth. By this indefinite, not to say infinite, duration of time, the Earth is discriminated from all that it contains; it is older than any of its parts; it antedates all its kingdoms. The nature of the whole is, therefore, radically different from that of any of its divisions. The Earth has had a development of its own; hence the too common error of treating it as passive and inorganic. The history of the Earth displays, in all the monuments of the past, that it has been subjected in every feature, in every division of itself, to ceaseless transformation, in order to show that, as a whole, it is capable of that organic development on which I lay so much stress. The natural powers which the earth includes are constantly obedient to the mechanical laws of chemistry and physics. The animate creation, plants, animals, man, come and go, in accordance with the laws of their being, and as subordinate dependents on the great forces which the earth holds locked up within her bosom. The earth, the mother of them all, has her own special advance, her own development, to use that overburdened German word. She has relations to herself alone; not simply to organized forms, plants, and animals; just as little to organic things; not simply to her own countries, her rocks, and her crystals. These are but isolated parts; or, if not isolated, yet bound together by a common tie. There is another tie above this; it is that which binds the earth to itself alone; that subordinates its parts to such an extent that they almost disappear. There is, above all this thought of parts, of features, of phenomena, the conception of the Earth as a whole, existing in itself, and for itself, an organic thing, advancing by growth, and becoming more and more perfect and beautiful. Without trying to impose on you anything vague and transcendental, I wish to lead you to view the globe as almost a living thing,—not a crystal, assuming new grace by virtue of an external law,—but a world, taking on grandeur and worth, by virtue of an inward necessity. The individuality of the earth must be the watchword of re-created Geography. To think of the Earth, as a seed sown from the hand of God himself on the great fields of space, and filled with a germinant power of life, which will transform it more and more, and make it more and more worthy of its noblest inhabitant, is the first, as it is the last, idea which we must take and keep in these inquiries.

Formerly, Geography was regarded as a mere auxiliary of History, Politics, Military Science, Natural History, the Industrial Arts, and Commerce. And in truth it does reach out and teach all these departments of knowledge and action; but only in the most recent times has it assumed the place of an independent branch of study. Only through the widening of the whole circle of sciences has room been made for this.

Geography used, for the sake of commerce, to be divided into three divisions: mathematical, physical, and political. This was at the time when it was thought that the whole frame-work of the sciences was a disjointed and sundered thing; before that minor principle of unity which binds them all together was recognized as one of the noblest conceptions that the mind can cherish. In the first two of these arbitrary divisions into which Geography was severed, the relations of astronomy, mathematics, and physics were studied, and their applications to the confused phenomena of the globe investigated. Yet the most important thing of all escaped notice; students overlooked their chief task, the tracing of causation and interdependence in the phenomena, and the relation of every one to the country which supplies its conditions of being. It was not suspected that each phenomenon was one link of a great chain of phenomena, the whole revealing a comprehensive law. Men discussed porphyritic formations, basaltic columns, hot springs, and a thousand features which dot the earth, and a thousand kinds of rock which rift the surface of the globe, and treated them singly as if each was a spore and the whole combination only a sporadic group. They did not discover that in the one feature was to be found the reason of the existence of its neighbor; that all the layers of stone owe their singularities of structure to one another rather than to themselves; that each one stands in the closest connection with the upheaval of the loftiest mountains, with the formation of great volcanic islands, and, in truth, with the building up of entire continents. And, in like manner, plants were discussed as if they were obedient to no law of grouping, as if they were scattered broadcast over the earth, having no relation to zones of vegetation, to isothermal and isochimenal lines; as if, in fact, there was no suspicion of any principle underlying the very existence of the whole vegetable kingdom. And so, too, with such phenomena as the Aurora Borealis; they were treated as isolated features, rather than in their relations to the globe; the connection was not seen between the maritime discoveries of voyagers and the great system of oceanic currents, on which voyagers are so dependent; in fact, the whole influence of the world of matter on the world of mind was unexplored.

And in order to study what was called Political Geography, a vast mass of materials was converted into a stiff, ritualistic frame-work, in the effort to impose some system and imaginal completeness on it, and not in order to grasp facts and truths in their mutual relations and inward life; they were merely arranged for convenient reference and for available use in the departments of military science, politics, statistics, and history; a method which is plainly our inheritance from the Middle Ages, and which bears the marks of those days. Thus from this arbitrary arrangement, made without reference to any indwelling necessity, sprang the three groups with which we are familiar: Chronography and Topography forming the first, Ethnography and Anthropology the second, and Statistics and History the third, or Political Geography.

From these three groups our ordinary text-books compile their usual aggregate of facts, and each becomes after its own pattern a motley in miniature. They contain variable quantities of this triple mass of materials, and follow no law but the demands of the time when they see the light; they favor, like our light literature, the whim of the hour, and are political, military, or commercial, as the public may demand. A systematic exposition of geography is very seldom to be found in them. A harmony of parts, a true harmony, is very rarely attained in their pages. They are at the foundation only arbitrary and unmethodical collections of all facts which are ascertained to exist throughout the earth. They are arranged according to countries, or great natural divisions; but the relation of one great natural division to another, the mutual and immense influence of one country on another, is never mentioned. The description of Europe follows in them to-day the same order in which Strabo set the pattern. The facts are arranged as the pieces of a counterpane, as if every one existed in itself and for itself, and had no connections with others. The setting out of these facts follows the rubrical method of grouping, according to boundary, soil, mountains, rivers, products, and cities. The beginning is usually made with boundaries which are generally most unstable and uncertain, instead of being made with some rudimental fact around which all others arrange themselves as a center.

If we compare these geographical treatises with those made in the interest of any other great department, we shall speedily discover that they indicate knowledge rather than science; they form a mere aggregation and index of rich materials, a lexicon rather than a true text-book. And therefore ensues, despite the undenied interest of the subject and its high claims, the mechanical and unfruitful method only too common—the crowding of the memory without judgment, without thought; thence comes it that Geography has taken so low a place among our school studies, worthy only of the youngest of the pupils, and presenting little stimulus even to them.

It will be my effort, in the course of these lectures, to exhibit the subject of relations rather than to detain you with descriptions; in one word, to generalize rather than to add new details. In the lack of a thoroughly excellent text-book of geography, I shall presuppose an acquaintance on your part with the materials, so to speak, of which the science is to be constructed.

It has been a customary method to treat geography in connection with epochs of time; dealing with it as it was in the past and as it is in the present. We hear of Ancient Geography, the Geography of the Middle Ages, and Modern Geography. In this course of lectures, it will be treated not as the property of one age or another, but rather as a growth of all time, from Herodotus down to our day. It is only in this way that we can ascertain what is permanent and what is ephemeral; only in this way can we subject geography to that comparative method which has given such an impetus to the advancement of the sister sciences of Natural History; only in this way can we see how the present is the birthright of the past. Archæology, ethnography, and civil science are all gainers by this method of treatment; in one word, the whole domain of cotemporaneous study. The less positive knowledge we possess of the formative processes of science, the more crude our hypotheses, the more flagrant our errors. This is constantly verified under our eyes; the errors of the past are the wisdom of the present, and the gradual upheavals of our knowledge become indices, not less of outgrown untruths than of truths yet to be revealed.

Sources of Geographical Science.

The sources of geography, as of history, are twofold—established memorials and continued investigations. The study of it has this great advantage at the outset, that the surface of the earth is a standing monument of the past. We are obliged to search where all lies open; where investigation must be crowned with success. No manuscripts in this great library have perished; they all exist as legible, as accessible as ever. Moreover, personal investigation must be made by every student in order to understand the results of the investigations of others. Wherever our home is, there lie all the materials which we need for the study of the entire globe. Humboldt hints at this when he says in his Kosmos: “Every little nook and shaded corner is but a reflection of the whole of Nature.” The roaring mountain brook is the type of the thundering cataract; the geological formations of a single little island, suggest the broken coast lines of a continent; the study of the boulders which are so thickly scattered in token of a great primeval deluge from the north, reveals the structure of whole mountain chains. The digging of every well may contribute to our knowledge of the earth’s crust; the excavations made in the building of railroads may, without the loss of time, labor, and expense, be a ceaseless source of instruction. In the structure of a spear of grass, of a rush, of a single monocotyledon, may be studied in miniature the palm-tree, prince of the tropics; in the mosses and lichens on our walls, the stunted growths of mountain tops may be investigated. A small range of hills may be taken as the type of the loftiest Cordillera. The eye may be easily trained to see all the greater in the less. The study of our own district is the true key to the understanding of the forms and the phenomena of foreign lands. Whoever has wandered through the valleys and woods, and over the hills and mountains of his own State, will be the one capable of following a Herodotus in his wanderings over the globe. He, and he alone, will be able, with true appreciation, to accompany travelers through all foreign lands. The very first step in a knowledge of geography is to know thoroughly the district where we live.

Unfortunately the text-books which we now possess do not discuss, with any approach to exhaustiveness, the districts where their readers live; and hence they cannot give any true inductive generalization of the large and the remote. In ancient times, the study of geography began with the world of nature, not with the world of books. Herodotus, being 444 years B. C., became, by virtue of his investigations on his wanderings, the first critical geographer of the Greeks. Polybius traveled through the Alps and Pyrenees, Gaul and Spain, to be able to write the history of Hannibal’s campaigns. He explored the Black Sea and Egypt, in quest of facts. He is the father of all military geography; the greatest strategists have busied themselves with writing commentaries on Polybius. Strabo, the most industrious geographer of his age, did not write till he had traveled from the Caucasus to the Rhone, and from the Alps to Ethiopia.

Philip Cluver, of Dantzig, who died in 1623, the true founder of classical geography, collected, by personal investigations, the materials of his great work on Germany, Italy, and ancient Sicily, all of which countries he traversed thoroughly, the classic authors in his hand.

Alexander von Humboldt has become, by his thorough studies of nature in Europe, Asia, and America, the founder of Comparative Geography. He was thoroughly acquainted with every geographical form in the neighborhood of his home, before he traveled into foreign lands. These examples show that personal investigation is one of the most reliable of all sources of geographical knowledge.

The second class of these sources is the accounts given in the published memoirs of travelers. In more primitive days than these, when very little was known regarding the earth, personal examination was easily completed, with a good degree of fullness, by almost any tourist. With the advance of knowledge, the narratives of travelers have increased, and the sum total of facts observed has become unwieldy; and, where facts have been wanting, the imagination has amply supplied their place. Of course, a single life soon became too short for the personal examination of every quarter of the globe; the narratives of those who had thoroughly explored any one were accepted as authoritative, and these accounts soon became the most generally available of all the sources of geographical knowledge. Yet, with this limitation, that now their abundance and their exactness tend to repress and almost to destroy any personal inquiry whatever. Nothing can take the place of some exploration and investigation on the part of the student of geography.

To the accounts of scientific travelers, may be added those maps and globes which indicate the contour and the vertical elevations and depressions of the earth or its divisions. The demand for perfect accuracy in these is now very great. The map must be a portrait, not a caricature. In its way, the map has a certain dictatorial authority; it is so decisive in its very character, that errors in it are far more dangerous than in the letter-press of books. The English excel in the beauty of their maps: there are none in the world engraved with the rare excellence of theirs; but their care to secure accuracy is not commensurate. The French and the Germans vie for the honor of perfectly transcribing nature.

The Sciences illustrative of Geography.

The sciences which are called in to illustrate the thorough study of geography have largely increased in number within the past few years. They are, for the most part, the same which illustrate history; to which may be added mathematics and natural history. It is a very great mistake to suppose that all that bears upon geography can be crowded within the covers of a single book. It is commonly supposed that geography is a matter of memory. Even in its elementary forms, it is capable of a constructive treatment. Many a teacher, who has not paid special attention to this department, dreams that he can qualify himself by running through a single text-book. No philologist would dream that, with a grammar and dictionary, he could grasp any constructive theory of language. There must first be the study, comparatively, of the great classes. And in geography, the personal study of the earth, with critical closeness, and in the comparative method, is the true way.

Another very common error is, that geography must subsidize what is most striking in other sciences, and thereby gain its charms and attain its uses. Thus geography becomes everything—history, statistics, statecraft, physics, a catalogue of all the possessions of natural history, in all its kingdoms. It takes on all colors, and meanwhile loses its own. It merges all its individuality in other provinces. In no way can it escape this disintegrating force, unless by holding fast to some central principle of being; and that is the relation of all the phenomena and forms of nature to the human race. It cannot exist, if it is to be merely an aggregate of all science, a mosaic of all colors. It is to use the whole circle of sciences to illustrate its own individuality, not to exhibit their peculiarities. It must make them all give a portion, not the whole, and yet must keep itself single and clear.

For the comprehension of mathematical geography, a knowledge of the elements of mathematics and astronomy is indispensable. For determining localities, and for using many needed instruments, there must be some skill in practical astronomy; for measuring distances, for projecting maps and charts, and locating geographical districts upon them, there must be some familiarity with trigonometry and the higher mathematics. No one can thoroughly study geography in foreign lands, and leave all astronomical instruments behind.

Political geography demands an acquaintance with history, and the same helps which the study of history requires. The civil status of no country can be determined without this. Büsching’s “Europe” was a master-piece of its time. But it was impossible for even that book to compress within its covers the whole history of that continent in its relation to the geography of Europe.

The study of Man is, of course, in most intimate alliance with geography. It is only since the opening of this century that ethnography has become a prominent and clearly defined province of science, and enabled to become a great tributary of geography; in fact, the greatest tributary. Other departments are also drawn upon; there can be no close study of the soil, the structure of mountains and plains, without mineralogy and geology. Meteorology, too, the science which discusses the climatic conditions of countries and the effects of climate upon the organization of plants, animals, and man, is of no mean value in illustrating geography. Nor can one be a great geographer who does not understand the flora of the world. Not that he needs to be familiar with the myriads of plants, but the laws of growth and the characteristics of localization must be known. The geographer does not need to repeat in detail where the cereals and the palm-tree thrive. The general conditions which control the growth of plants are all that he has to concern himself with. The main auxiliary for this is furnished in the botanical garden, where the eye sees the products of all localities, arranged, according to their grouping, in the countries where they are indigenous. Botany and zoology and mineralogy are among the sciences most valuable in throwing light upon geography; they display best what wealth each country holds in store for the uses of man; for they are closely connected with the development of industry, the arts, and trade.

This brings us to the last province, commerce, the science of interchange. The study of minerals, of the distribution of plants and animals, is of little advantage, aside from commerce and its uses to man. It is the interchange of the products of one region for those of another which has had, on the whole, the greatest influence on the human race. Think, for an instant, of the transfer of the potato from America to Europe, of maize to Asia; of the far more ancient introduction of wheat and rice from Asia into Europe; and not these alone, but almost all the fruits. Think of the carrying from Asia to America, and, in fact, to all tropical lands, such products as sugar, coffee, and cotton. Think, too, of the results of the search for gold, ivory, and slaves in the interior of Africa, and of gold in California and Australia, opening such immense districts to settlements. The search after platina has disclosed the most guarded recesses of the Cordilleras and the Ural chain; while the need of copper first gave us our complete knowledge of the great system of American lakes. Without the expeditions to secure the whale, the walrus, and the seal, as well as the fur-bearing animals, the polar world would be still untraversed. The discovery of coal on a hundred shores otherwise unknown, led to the settlement of man in colonies from India and China southward to the Antarctic Continent, and northward to Nova Zembla, Spitzbergen, and Greenland.

And not the continents only, seas and oceans have been thoroughly studied, in order to secure a safe pathway for man to the regions which contain his spoils. In the furtherance of this, the highest praise must be awarded to the British government. Through its enterprise and liberality, almost every island group has been examined, a thorough study of marine currents undertaken, careful soundings made in all waters, and a most extensive chartography accomplished. The charts published by the English admiralty already are counted by thousands.

Yet the French have not been backward in like investigations. Understanding the value of commerce, their Dépôt de la Marine has not been inactive. Scandinavia has also done her part. The United States has accomplished one of the most thorough coast surveys ever undertaken by any nation; its difficulties are only to be measured by its extent. In fact, the whole civilised world has sent its messengers to the ends of the earth, and have united in this grand crusade of our age, the enriching of all men by a liberal system of interchange of the commodities of all climes.

COMPARATIVE GEOGRAPHY.

PART I.
THE SURFACE OF THE EARTH CONSIDERED IN ITS MOST GENERAL RELATIONS.

The Spheroidal Form of the Earth.

The measurements of, and investigations into the figure of the earth, have led, as already stated in the introduction, to no absolutely certain conclusion; yet they have made it certain that the earth is, in a general sense, a spheroid. There are many discrepancies, as were then stated, from the perfectly spheroidal shape; still it is in this sense a spheroid, that the polar diameter is not of the same length with the equatorial diameter.

The globular form of the earth, using that word in a loose sense, has been established with certainty since Newton’s time. The experience of circumnavigators, the uniform shield-shape of the shadow of the earth during eclipses of the moon, are witnesses to this. The gradual emerging and disappearance of objects, such as ships on the sea, in coming and going, caravans on the desert, of mountains as they are approached, establish the fact. These proofs are so well known that we but touch on them and pass to what is not so obvious.

As soon as the fact was established that the earth was a subordinate member of a system, it was brought into analogy with other planets, and their uniformly spherical shape was considered another valid reason for attributing the same to our globe. The discovery of the rotation of the earth on its axis was still another argument in the same direction. Mathematical measurements and observations of the pendulum, taken at different stations, have confirmed the same result.

To measure a spherical body, it is only necessary to take the length of a degree in one of its great circles, and to multiply its length by 360, the number of degrees. The method of measuring a degree on the earth’s surface is by taking two stars, just one degree apart, dropping, by astronomical and mathematical means, vertical lines upon the earth from them and measuring the distances apart of the points where those lines impinge upon the globe. This can be done with perfect accuracy. Such investigations show that the degrees are not all of equal length, as they would be were the earth a perfect sphere. Nearer the poles they are longer, nearer the equator they are shorter. The curvature of the earth is therefore greater as you approach the equatorial line, and less as you recede from it. In general terms, then, the earth is an oblate spheroid, as it would be a prolate spheroid were the lengths of its diameters reversed. By the most accurate measurements, those of the astronomer Bessel, if the equatorial diameter were divided into 289 equal parts, the polar diameter would measure 288 of them, being ¹⁄₂₈₉ shorter.

To this must be added what was said in the introduction, that the surprising accuracy of modern instruments and modern investigations, applied to meridian circles and parallels of latitude, have determined the fact that the spheroid is not a perfect one, (just as so often in nature the ideal is rather striven after than attained,) but an irregular polyhedron of an indeterminate number of sides. Still for all practical purposes, these minute inquiries have no value, and it is enough to treat of the earth as a perfect globe, so far, at least, as map-drawing is concerned. The deviation from a perfectly spherical shape is so inconsiderable that in an artificial globe of eighteen inches diameter it would hardly amount to the thickness of a sheet of paper; still, small as this is represented on a miniature scale, it has, doubtless, great importance on the great scale of a world like this, both in affecting somewhat the perturbation of other heavenly bodies which depend on the earth, as well as the perturbations in the earth’s own motion. Besides this, which is really not a small point in consideration of the possible results which the minutest perturbation of one little planet may have on the universe, there is one other, more appreciable in its results, the probable influence of this spheroidal, or rather polyhedrons form, in producing the unequal division of land and water upon the surface of the earth. The apparent want of any principle or reason for this inequality has long perplexed geographers, and there seems to be no more satisfactory solution than the one to which I have just alluded. In the course of future investigations into the yet undetermined exact mathematical form of the earth, the law which controls the division into land and water will be more thoroughly understood. Unquestionably the position of the great oceans depends upon their distance from the center of the globe, and although the present proportion of land and water seems fortuitous, undoubtedly it has a uniformly acting, and a thoroughly appreciable law.

The Threefold Covering of the Earth.

What may in the largest and most general sense be called the superficies of the earth, is threefold in character, and yet one in function; consisting of a highly elastic body, the atmosphere, water, and the solid ground. These three forms are variously proportioned; the more elastic is universal, the fluid form is more restricted, and the solid one prevails still less. The more dense the body, the nearer it is found to the center of the earth. The lightest of all floats over the entire periphery of the globe like a graceful mantle of cloud. Man, and in fact all organisms, live by contact with all three of these forms. The investigation of the elements, and phenomena of the air, regarded in themselves, is the province of meteorology. The mercury-column is the true language of the atmosphere, and tells us in distinct tones of all the changes there. Mineralogy and geology make us acquainted with all the qualities and all the elements of the soil, not in their relation to man, but regarded in themselves. Geography deals with the conflict of all these bodies, their relations to each other, their mutual action and reaction. Meteorology gives occasion for the study of climate, and for the observation of the phenomena of the lower strata of the atmosphere,—the fall of rain and snow, for example. Geology and mineralogy give rise to the study of plains and mountain formations, as well as of volcanic phenomena, affecting the surface of the earth as they do in earthquakes, upheavals of whole districts, and the opening of hot springs. Thus, geography has it own province clearly defined, and uses all this and studies it in relation to the organic world, and to man foremost of all.

The most highly elastic covering of the earth is unbroken, the other two are sundered, and each only occupies a part of the surface. Formerly, in most ancient times, the water seems to have covered the entire earth. The study of this is, however, within the domain of geology. We have to do only with the historic period which followed. We have to look at the earth in its present relations, and as the home of man. Now, the portions covered with water are, by far, the largest part of the surface; a little less than three-fourths are water, a little more than one-fourth land. The whole water-mass is composed largely of the oceans, which, in one sense, constitute a continent of their own: in looking at them as we do now, we are not to regard them as ceasing at the outlines of the great land-masses, but as penetrating these as far as to the springs which feed the rivers; for the world of waters, embracing springs, brooks, rivers, lakes, seas, and oceans, is one, and but one.

The water is, in some respects, a form between the other two; its peculiarities, weight, density, freedom of movement, and changeableness of form, are a mean between the opposing extremes of air and the ground. Water can pass to a more fluid or a more solid state; it can become vapor or ice. The measurement of the depth of the world of waters has lately been so clearly connected with the needs of civilization, that geographers have made many exceedingly accurate investigations. Formerly, this was much neglected; up to Captain Cook’s time 1500 feet was the greatest depth ascertained; in the course of the Arctic discoveries 7000 feet limited the plummet’s descent; Captain Ross sounded, near St. Helena, to a depth of 30,000 feet; and Captain Denhorn, in the South Atlantic, reached a point 46,000 feet from the surface—about twice the height of the loftiest mountains. And not single points alone, but entire ocean districts have been traversed; the temperature of these great depths has been studied, the currents, the density, in fact all the features which must be known preliminarily to the laying of great lines of submarine telegraphs, such, for example, as that proposed between North America and Europe.

The atmosphere, too, is by no means thoroughly known to us. It rises to a height between 85 and 95 miles from the earth, of which man has explored in balloons only about five miles, or the height of the loftiest mountains. At loftier heights than we can live, the bright light of mid-day even fades into a dim kind of twilight, and meteoric masses of iron are seen in full glow, there being oxygen enough even there to support their combustion, and very little resistance to overcome from the density of the atmosphere. Astronomers, Benzenberg in particular, have calculated the distance of the meteors to range from 23 to 100 miles from the earth, and have studied them[2] in respect to the time when they were visible, their locality, and their direction. The limits of the atmosphere must be at that point where the expansive power of air and the attractive influence of the globe neutralize each other. The form of the atmospheric body is therefore, like the earth, spheroidal, but far more oblate than the earth, in consequence of its much greater fluidity. At the poles, the distance is therefore much less from the surface of the earth to the confines of the atmosphere than at the equator. The effect of this upon the refraction of light must be very great.

The investigation of the interior of the earth is more difficult to us than that of the atmosphere even. We cannot say that we know thoroughly more than we can learn by penetrating ¹⁄₆₀₀₀ part of the distance to the center of the globe. Deeper than that our lowest shafts have not sunk. The coal mines of England penetrate perhaps the farthest below the sea level; for the deep mines in Germany, in the Hartz district, for instance, have their entrance hundreds of feet above it. One coal mine near Durham, England, descends to a depth of about 1584 feet, and reaches a point where the thermometer is 79° Fahrenheit. The deep coal mines of England have, however, one rival, in a shaft at Liege, which is sunk 1800 feet.

The modern Artesian well has gone to still greater depths, in the effort to procure brine for the manufacture of salt, or fresh water for the use of cities. At Rehme, in Porta Westphalica, a point 2160 feet from the surface has been reached, and water brought up at a temperature of 90° Fahrenheit, containing four per cent. of salt. By an ingenious application of mechanics to the process of well boring, doubtless a depth of 5000 feet could be attained. At Mondorf, in Luxemburg, a bore has been made through sandstone and the mineral formations lying beneath it, for a distance of 2700 feet, and water reached at 82° Fahrenheit.

The great upheavals caused by earthquakes and volcanoes disclose still vaster depths. In the eruptions of the latter, immense masses of the inner contents of the earth are thrown out, sometimes enough to form a not insignificant mountain, and to desolate large regions with their debris. As a general thing, the original mineral forms are lost and indistinguishable in the molten mass. Yet not seldom perfect specimens are hurled out, imbedded in lava and cinders; not always minute fragments, sometimes huge blocks, testifying not with any degree of completeness, yet clearly, to a certain extent, of the composition of the region bordering on the great inner sea of molten matter. Yet most of our knowledge upon this subject is hypothetical, and what we know only indicates painfully the great extent of that of which we are entirely ignorant.

The uniform increase of temperature, as we descend into the earth, at the rate of about 24° Fahrenheit for every 100 feet, the heat of some mineral springs, leads to the conclusion that, could we advance to a place about twenty-three miles from the surface, we should attain the limits where all becomes a molten mass. The cold surface, on which we walk in such security, seems, by all analogies, to envelop a liquid caldron which has been seething from the morning of the world. This internal mass is, of course, the source of all volcanic eruptions, and of all the phenomena to which I have alluded above. A distinguished geologist has well said that “light and heat are the two extremes of being: the farther man goes away from the earth’s surface, he encounters light; the farther he recedes inwardly from its surface, he encounters heat.” It is true we are not absolutely certain that the rate of increase is uniform, at the rate of one degree Fahrenheit for every 45 feet; but if it is, we should reach the boiling point of water at less than 10,000 feet from the surface, and the melting point of iron (22° Fahrenheit) a little over 120,000 feet. The relation of this thickness to the entire diameter of the earth is about as 1 to 344, about the ratio of the thickness of an egg-shell to the egg.

The Superficial Dimensions of the Land and Water on the Globe.

The equatorial diameter of the earth, 7925·6 miles, multiplied into the circumference, 24898·8, equals 197,339,590, the number of square miles on the earth’s surface, reckoning as if of a true sphere. The deduction to be made, in consequence of its spheroidal shape, has not yet been estimated with any approach to nicety. The sum indicated above is exact enough to satisfy geographical purposes; enough to lead to the laws of relative rather than to a minute individualization. The proportion even of land to water has not been determined, except with approximate accuracy. It has been commonly stated that two-thirds are water and one-third land; others have computed three-fifths to be water and two-fifths land. The most accurate measurements, those instituted by Humboldt, have left it in this statement, that if the whole be taken as one, the sea occupies ·734, the land ·265, or, reduced and simplified in almost unchanged form, a little more than three-quarters water, a little less than one-quarter land. Of course it is impossible, as yet, to attain to accuracy in these estimates, as our knowledge is imperfect regarding the polar regions; there are about 17,000,000 square miles unexplored.

The ascertaining of superficial areas with exactness is one of the most costly operations undertaken in the interest of science. The first mathematical survey of France, one hundred and fifty years ago, undertaken by Cassini, cost four millions; the second sixteen millions; a third, still more costly, has been made within the present century. Still, it must be said that few countries have expended money in this direction with as much prodigality as France. In Turkey, for instance, so little accuracy has been attained, that the survey of that country, undertaken by Beauchamp early in this century, resulted in establishing the Sultan in possession of 17,000 square miles which he had supposed were covered by the Black Sea. The recent surveys of Prussia have rectified similar mistakes, and, in the constantly increasing accuracy, have given hundreds of square miles to the Crown. Many countries, and in truth the most, have never been subjected to a strict mensuration. The jagged coast lines of islands and continents have been so great a barrier, that we have to speak with great uncertainty of the superficial contents which they inclose. The statements of these make no pretense, therefore, to accuracy. We must be content, at present, with the rudest approximation. This accounts for the discrepancy in our geographical compendia; no two of them agree, unless one servilely copies the other. The statistics relating to the superficial contents of continents, and of separate countries, must be taken with a great deal of allowance. The evil cannot be remedied at present; it will be, doubtless, at some future day. The discrepancies which it occasions will be seen, from the fact that the area of Europe has been computed to be between 3,254,800 and 3,870,500 square miles; that of Asia between 16,180,000 and 16,831,600; that of Africa between 11,257,200 and 11,513,600; that of America between 12,140,400 and 15,963,600; that of Australia between 2,756,000 and 3,201,200 square miles.

According to this, Asia is five times as large as Europe, and almost six times as large as the continent of Australia. Africa is three times as large as Europe. America is four times as large as Europe, and is as large as Africa and Australia combined. Europe would make about one-third of Africa, one-quarter of America, one-fifth of Asia. Our present knowledge does not allow us to speak more definitely nor exactly.

Contrast of the Land and Water Hemispheres.

Whether we divide the globe into northern and southern or eastern and western hemispheres, their relative amounts of land and water will be different The northern hemisphere contains (speaking approximatively as above) 38,541,600 square miles of land, and 59,619,700 of water; the southern, 12,847,200 of land, and 85,526,100 of water. The eastern hemisphere contains 36,760,800 square miles of land, and 61,401,000 of water; the western, 14,628,000 of land, and 83,533,300 of water.

Besides the division quantitatively, the division in respect to symmetry of shape is entirely irregular. Symmetry, as we usually use the word, consists in the arrangement of parts at equal distances, or two sides at least, from some central point or line. Mineral crystals are regarded in relation to the point where crystallization began; plants are viewed in relation to the stem-axis; animals in relation to the symmetry of the entire structure. A similar law of symmetry is entirely wanting to the globe; its arrangement is altogether unlike this; it is not nearly so perceptible at first glance, yet it is far more profound in design and comprehensive in its relations.

The land is broken up into masses, varying in size, and called, arbitrarily, continents and islands. Strictly speaking, there are but two continents, the old world forming one, the new world the other. Australia may be called the smallest continent or the largest island; it is the connecting link between the forms, and shows at a glance the arbitrary distinction. We might easily go further and call New Guinea, Borneo, Sumatra, Great Britain, and Java, continents, and, on the other hand, we might designate the old and the new world as islands. There is nothing absolute here but the usage of speech.

The continents and islands lie mainly in the northern hemisphere, (38,341,600 square miles,) scarcely a third part of their superficies (12,847,200 square miles) being in the southern.

The continents are so situated also that the eastern contains by far the largest body of land, (36,760,800 square miles,) the western being only about one-third as large, (13,628,000 square miles.) America, the western, it will be seen, has no first-class island lying near it; it stands isolated.

It is seen by this that the greatest mass of land lies in the northern hemisphere, dividing the earth in one way, and in the eastern dividing it in another; the smallest mass in the southern and the western. In the northeast the watery realm is the most contracted, in the southwest the least. We are thus enabled to speak of the land side of the globe, the land hemisphere, and a water side, the water hemisphere.

The central point of the water hemisphere is at the island of New Zealand. Toward this the points of all the continents are directed. The center of the land hemisphere is in the northwest of Europe, at a point near southeast of England, the northeast of France, and the coast of Holland. The dwellers around the North Sea are the antipodes of the New Zealanders. Great Britain is the country which, as a whole, is the middle point of the continental world. In the oceanic world, the islands lie like scattered dots, insignificant in respect to area, in comparison with the waste of waters which surrounds them, while, on the other hand, the land hemisphere is so solidly compacted, that even the Arctic Ocean becomes merely a broad channel.

Thus arises the first great contrast which we have to study: the first, and next to the great primary distinction between the North and South, the most important. The division into land and water, aside from commerce, must exercise the strongest influence on the distribution of heat and cold, affecting the temperature of all the zones. This influence has been fully noticed and brought before the world by Alexander von Humboldt. It is sufficient to refer to it now as a well-determined fact in physical geography.

The heat equator is a little farther north than the mathematical equator, because the land hemisphere has a greater heat capacity (if we may use an awkward but apt word) than the water hemisphere. All other isothermal lines are modified in their greater or less coincidence with the parallels of latitude as they advance from the heat equator toward the maximum of the land hemisphere, or, in general terms, as they go northward. In the western hemisphere the isothermal lines follow much more exactly the parallels of latitude than in the eastern, which is pre-eminently the land hemisphere. In America the proximity of immense masses of water causes a perceptible reduction of the heat from that of the eastern where the land form prevails. And the heat diminishes more as we advance toward the South Pole, than toward the North, in consequence of the greater deficiency of land in the southern hemisphere; while in Lapland, Greenland, and in Siberia, even within the polar circle itself, men find sustenance and trees live, in the same latitude, at the South Pole, no vegetable life, worth mentioning, is found. The frigid zone and the temperate zone of the southern hemisphere are not coincident with those of the northern. The icebergs which are formed at the South Pole are carried much nearer to the equator than those found at the North Pole.

An important phenomenon, first pointed out by A. von Humboldt and Dove, is closely connected with what has just been said. The Atlantic shores of the old world are warmer than those in the same latitude of the new world. Norway, England, and France are warmer than Labrador and Canada; Spain, Portugal, and Morocco are warmer than Florida; Congo and Benguela are warmer than Brazil, although the countries brought in contrast all lie on the same parallel.

A similar analogy is drawn from the west shore of America: Northern California is warmer than Japan and Corea, which are in the same latitude. It is true, other factors are at work to produce this, such as winds, marine currents, elevations of land, etc., of which more will be said hereafter.

Both of the two great land divisions of the earth, it will thus be seen, have their peculiarities. But there is a great equalizer of their diversities, found in a great coast-belt, of which I must briefly speak. It passes from the Cape of Good Hope northeasterly at an angle of 45°, passing through the Mozambique channel, thence skirting the entire southeastern and eastern coast of Asia, taking in China, Corea, Japan, and South Kamtckatka; thence it turns southward, following the whole western shore of America to Cape Horn. This belt is broken at only two points—a brief break at the north, at Behring’s Straits, and a large one between Cape Horn and the Cape of Good Hope; in other words, at the points nearest to the North and the South Poles respectively. This coast belt has a relation to the habitable world similar to that held by the temperate zone as a mediator between the torrid and the frigid. It partakes of the character of the sea and the land, and shows the advantages of both. It does not run parallel with the lines of latitude, but crosses them diagonally, in the same direction with the ecliptic, though at a more acute angle. This belt moderates all extremes. Coincident with it are the paths of the sea and land winds, the course of the monsoons, the most fertile shores of the whole globe. It divides the surface of the globe into three great divisions, the two great bodies of water, and the great, and, comparatively speaking, unbroken (for the break at Behring’s Straits is of little importance) land-mass. On the great coast line referred to above is the center of the great natural acclivities of the globe. It is the most varied, the most stimulating, and the most productive in all departments of the vegetable and animal kingdoms. The Atlantic coast belt, which also has great influence on the eastern districts of the new world and the western districts of the old, crosses the great coast belt at almost right angles at the place of its great sundering between Cape Horn and the Cape of Good Hope.

If the contrast between the sea and the land has the effect indicated above on the general development of organic life, it must of course have great effect also on the life and character of man. Man eminently depends upon the conditions amid which his lot is cast. The inhabitant of one of the Pacific islands dwelt in a world whose utmost possibilities to him lay in the adjacent islands within view, and which his canoe could reach in a few hours’ sail. The difference in culture between him and those whose range of observation has been greater, must be immense. The compacted land division of the globe, the solid cluster of continents, must be the source of stimulus and culture, of which the isolated inhabitant of the Pacific islands knew nothing, till commerce had at length linked the world together. Only with the improvements in navigation could civilization reach him. The European had to carry his culture to the New Zealander, his antipode.

The ancients had little suspicion of all this. Yet the contrast between the land world and the water world did not escape Strabo’s keen glances, and he hints at its effects on man. It is glanced at in one passage of his 15th Book. He is speaking of the effect of the moist air of India in contrast with the dry air of Libya, and shows that he appreciates that these are not without their influence on the constitution of the Indian and of the Ethiopian. “Some,” he says, “rightly ascribe it to the sun, that, in the absence of moisture in their air, the rays burn so deeply into the body of the African; the Indian, on the other hand, is not jet black and curly-haired, because, in his country, he enjoys the moisture in the atmosphere.”

The Position of the Continents and its Influence on the Course of History.

Besides the three great forms spoken of above—the compacted land-mass, the great water-mass, and the subordinate water-mass—the position of the continents leads us to another discovery of prime importance.

The question arises, What relation have the continents, taken separately, to the entire mass which they constitute? What relation do they bear to each other? What influence does the proximity of great land forms exercise? What influence their remoteness from each other? Is the arrangement of the continents fortuitous, or adapted to great ends always held in view by the Creator? Has Nature been left in this to a wild, passionate caprice, or has she been subjected to law, and been compelled to subserve the interests of humanity? And is it not worthy of study, worthy of science, to investigate these things, to master their law, and observe here the workings of the Divine Mind?

In the solar system, we have for a long time minutely studied matters of size and distance, the approach and receding of planets, and observed the effects of all these things with an accuracy which could not be too thorough. In the study of our Earth, this has been neglected, because heretofore those great tracts of land and water have seemed of little mutual influence; because they are fixed forms. Yet they have a greater influence, perhaps, on this very account. Although there is in them no law of gravitation to study, yet there is in them the display of forces no less surprising than those of attraction, and which are to be read in the light, not of mathematics, but in the light of history. It indeed seems self-evident that a grouping of these great forms cannot be without an influence on the progression or retarded development of nations; on the amount of population, the progress of colonization, and the union of States in offensive and defensive alliance. Should a higher Power throw the continents out of their present position and relation to each other, a new history of the world would date from this day.

Here, then, is the primary element of history; the laws of continental arrangement are the starting-point. Mathematics has thrown a network of meridians and parallels over the surface of the globe; but these lines exercise little influence over the course of history. The symmetry and regularity which they suggest do not belong to the earth; the earth is not bounded, like a crystal, by right lines. There is a freer play than that mathematical mark of parallels and meridians suggests; there is an interdependence of the great land districts of the globe that these regular lines do not indicate; a higher law of order, evolving the most perfect results from elements seemingly the most discordant.

The Pyramidal Forms of the Great Land-masses, and their Southward Direction toward the Oceanic Hemisphere.

The great land-mass of the globe accumulates in size as we advance toward the North Pole. South of 55° S. lat., the continental form disappears, and the tracts discovered of late years in the neighborhood of the South Pole are apparently islands, or rather long ice-coasts, whose continental form is very doubtful. The great land division, embracing both the old and the new worlds, reaches to about 80° N. lat., and the extreme points come even yet nearer to the Pole. The distances of one body from another, as, for instance, from Greenland to Iceland, are very small, in comparison with the immense spaces which divide the southern points of the continent, where the hundreds of miles of separation at the north expand into thousands. Expansion of the land-mass is the law at the north, contraction at the south. The great land formations terminate in wedge-shaped extremities, a fact observed by Lord Bacon, J. R. Forster, and Steffens; America ending at Cape Horn, 55° S. lat., Australia, which may be considered to embrace Tasmania or Van Diemen’s Land, at the southern extremity of the latter, 45°, and Africa, at the Cape of Good Hope, 35° S. lat., respectively. Humboldt gave the name of “Pyramidal Structure” to this cone-shaped form of the great land-mass, which, it will be observed, all are directed toward the south. This pyramidal structure contributes very much, unquestionably, to the diminished heat of the southern hemisphere, and has given a great predominance to the population of the northern in comparison with the southern; and not in respect to number alone, but also to mental and moral force of character.

But not the southern extremities alone of the continents exhibit this wedge-like form; it is repeated also in the northern countries of Europe and Asia. In Europe we discover the working of the law in the peninsulas of Spain, Italy, Greece, the Morea, and the Crimea, and also in the great Scandinavian peninsula. The same phenomenon is repeated on a scale far more imposing in Asia, in the great countries of Arabia, India, and Farther India, Corea, and Kamtchatka; also in both halves of America. Exceptions are rare. In Great Britain, the pointed extremity is toward the north, and the greatest breadth at the south; but this is a peculiar case, and has its exceptional causes; and perhaps with reason, for this island has hitherto maintained an individual and exceptional character in the development of modern civilization.

Various explanations have been offered for the almost star-shaped figure which the combined body of great peninsulas assume, radiating, as it were, from the center of the land hemisphere. This is seen very strikingly in looking at a horizontal projection of the northern hemisphere, viewed from the North Pole. There has been evidently the working out of some great design in this, and the forces employed must have been of the first order of magnitude. Clöden attributes it to the rotation of the earth in its plastic, formative-state. Link ascribes it to electrical forces, generated at the time the earth’s crust was hardening into its present consistency. J. R. Forster finds an explanation in the theory, that formerly great currents, now not existing, passed, or sought to pass, from south to north or northwest. He attributes to these the parallelism of the great gulfs which indent the coast-line of the old world, the uniform abruptness of the shores at the south, and the gradual widening of all the great land-masses as we go north. The Atlantic is a channel cleft by those great currents. Behring’s Straits is a smaller one; but everywhere else the effort was incomplete, and no opening was effected, except in the straits of minor importance, which separate island from island, or from the main land. The fossils discovered by Pallas seemed to favor this theory, but later investigation has showed that they do not.

Link overthrew Forster’s theory, yet the phenomenon is worthy of study. Viewed on a map of the land hemisphere, constructed according to Mercator’s projection, it is a storehouse of interesting observations and studies, and is to be recommended to the student’s careful attention. We must pass over the theories; scholars disagree as to the cause; Pisis ascribes it to a hidden law of geometric construction; Necker, Brewster, and Dana, to magnetism. We must simply accept the facts for the present.

A careful study of the land surface of the globe suggests interesting comparisons with what we know of the heavenly bodies, Jupiter, for example, and our moon. Unquestionably, the entirely different grouping of what seem to be the great features of that luminary must have had an influence on the whole course of history there. We will not enter into speculations regarding this, however, referring the reader rather to the thorough investigations of Beer and Mädler.

Situation of the Continents in their Relation to Each Other and to their Collective Whole.

The relation which the continents bear to each other arises, primarily, from their position in reference to the cardinal points of the compass. This has been a principle from the earliest times, and the great laws of population may, in their working, be referred to this simple law of grouping.

Asia was known as the Orient, or, in the apt and beautiful German phrase, the Morgenland, or Land of the morning; Europe and the northern rim of Africa, as the Occident, or, in the German, the Abendland, or Land of the evening. In the south lay the torrid regions of the Ethiopians, in the chill north the country of the Hyperboreans. This fourfold division of the earth was for many centuries the only one known; the division into continents being made, according to Herodotus, by the Phenicians. And in very truth, a great principle lay in that rude and primitive division; it was in entire harmony with nature, and, up to the latest times and the opening of a new world, in entire harmony with history also. With Asia, the Orient, is connected indissolubly the development of the ancient world; with Europe, that of the modern. The contrast between these two great divisions is wonderfully analogous to that of morning and evening. The whole culture of the West had its root, its beginnings at the East. The East is not merely the place where the sun begins his daily course; it is the cradle of man, of nations, of dynasties of every sort, in politics, religion, and science. All the old royal houses came into Europe from the East; they are all “children of the sun,” no less than the princely families of India and Persia. The West merely witnesses the progress of what was begun in the East. From the most ancient times onward through the Middle Ages,—from Homer to Dante’s “Purgatorio,”—the West is associated with the kingdom of the dead, with “Hades,” and the “islands of the blest.” And within these two great divisions of Orient and Occident are comprised smaller ones, adapted to more limited conceptions of the extent of the earth, but growing out of the same root with the larger division. Bactriana and India constituted the Orient to the inhabitants of Western Asia, Syria their Occident; Asia Minor was the Orient of the Greeks, Italy and Sicily their Hesperia; while the Romans called Spain theirs.

Between the Orient and Occident, and yet to the south of both, lay the Libya of the ancients, exposed to the sun’s direct rays. In the very middle of the earth, on both sides of the equator, and not at the South Pole, is the true South. There we must seek the phenomena of the tropical world in their culminations. As high noon, the middle point in the hour, is the consummation of the day, so the torrid climes of the equatorial belt, at the very middle of the earth, afford the extremes of luxuriant growth.

The broad tracts of land at the northern polar regions formed the true physical contrast to the Orient and the Occident, as well as to the great South of central Africa. They lay around the North Pole like a vast shield of earth, unbroken except by the comparatively insignificant seas and gulfs of that region. And even where the water has broken its way and severed those northern lands, a submarine volcanic activity is, even now, constantly at work to restore the break, and bind the coasts together. At about 70° N. lat., all the countries of the north are brought into great nearness, and that parallel is a highway of little else than land crossing the North Cape of Europe, Cape Chelagskoy, in Tchooktchee, at the northeastern extremity of Asia, and touching Cape Bathurst, and the Fury and Heckla Straits of North America. North of this highway and of the Georgian Archipelago begins the great group of circum-polar islands.

The break between Asia and North America, at Behring’s Straits, is but fifty-six miles wide; it is the mere outlet of the Sea of Kamtckatka into the Arctic Ocean. The space between the northeast of America and the northwest of Europe is much greater indeed, but, in comparison with the distance between the southernmost points of the old and the new world, insignificant. The distance from northern Norway to Greenland is but about 940 miles.

It is noteworthy that, at the north of the great continental land-mass, where minor seas and channels break through, great volcanic forces are constantly at work, as hinted at above, to restore the unity. In the Sea of Kamtchatka lie the Aleutian islands, extending more than 950 miles, and forming what has been happily termed a bridge from the old world to the new. It consists of more than a hundred rocks and islands, some of which have been thrown up within the memory of man. In 1806, von Langsdorf and Tilesius witnessed the emergence of one of these, with a cone-shaped center, and about twenty miles in circumference. Grewingk has counted more than fifty volcanoes in activity within the limits of this island chain. The Curile islands, more to the south, form another similar volcanic group, extending from Japan to Kamtchatka. In this range there are known to be at least ten volcanoes, 10,000 feet in height.

The same high degree of volcanic activity must have formerly existed between Europe and America, for the traces of it are still visible. And not the traces alone, but a part of the same activity. And doubtless the shallowness of the waters between those continents hints at the same. More accurate explorations, then, will probably reveal multitudes of mountains, thrown up by these submarine forces, but not far enough to emerge and bear the name of islands. Yet many have emerged—those which fringe the shores of Norway, Scotland, and Ireland; the Orkneys, Shetland, and Hebrides islands; the Färoe group, with their blistered surface, their recesses, and volcanic rocks; Iceland, with its hot springs; and Mount Heckla; Jan Mayen, with its frightful craters, and the eastern coast of Greenland; one island, Sabrina, in the midst of the Azore group; which has had three upheavals within two hundred years, in 1638, 1723, and 1811,—all these plainly indicate the presence of tremendous forces, active in the past as well as in the present.

We thus fix the character of the arctic polar lands to be a close drawing together. Europe has, fortunately for itself, the least share in those inhospitable regions; only her pointed northern shores fringe the shores of the polar sea, leaving the great bulk of the great land-mass of the north to the broad shores of Asia and North America, with their neighboring island groups.

This polar world, as we may call it, in contradistinction to the Orient and the Occident, is not separated from more southerly regions by any great physical line of demarkation. The arctic circle is a mere mathematical line 66½° N. lat.; it has no geographical character whatever. The true polar world reaches in some places far beyond this mathematical barrier, bringing all its characteristics with it; while, on the other hand, it withdraws, at a few other places, nearer to the Pole. Were the polar world more broken up than it is by inland seas, and separated from the great land-mass by broad channels, it would be far more isolated in its whole character than it is. It is this immediate contiguity of the polar world with the great land-mass which opens it to whatever civilization it may be able to receive. And there is the same unity in the polar world that there is in the tropical world. The same phenomena which appear in one part of it are repeated in every other part. There are, of course, subordinate modifications found, but everything essential, which is discovered in one part, is discovered in every other part. There is no distinction into “new world” and no “old world;” the new world and the old coincide amid the arctic pole.

The characteristic of the polar world, next to this of unbrokenness, is the simplicity, or what might be called the monotony of its productions and all its features; the uniform reproduction of the same plants and animals, as well as of geological forms. Even Lapland, which is the farthest removed from the Pole of all the arctic regions, manifests, in its rounded and polished granite and gneiss and its deep and sharply-defined cuts, the same uniformity. The syenite found at Lake Imandra displays the same characteristics as that found on the islands in the White Sea, and on the shores of Greenland. The tops of the mountains, instead of being green, are all white with the lichen, commonly known as reindeer moss. And as with the geological formations and the vegetable kingdoms, so with the animal kingdom. Elsewhere are found bears, foxes, reindeer, seals, and walruses; the feathered tribes partake of the general monotony of structure, and man not less. The range of his development is extremely limited, and his character little different, whether in northern Asia or northern America.

America forms the real West of the great land-mass, the true Occident of the earth, young as yet, but to receive as its gift the entire culture of the East, and to advance by giant steps to a position of independent influence. Already it has far surpassed Asia in industry and civilization. The old world was the preparation for the new. Almost everything which the new world enjoys and values was the gift of the old. Its most ancient monuments of religion, architecture, and art are closely linked to those of the old world. Hieroglyphics have been found among the Peruvians and the Mexicans. In like manner embalming of princes, the engraving of astronomical data upon rocks, were borrowed from the East.

The historic character of America is more striking in respect to newness than the physical features of the water hemisphere. Buffon supposed that the American continent is of more recent formation than the old world, assigning for his opinion that it is more submerged, because smaller in area, than the eastern land-mass; because, also, the plants which demand moisture are predominant over those which depend on a dry climate; and because the forms of homologous animals—the elephant, rhinoceros, crocodile, turtle, apes, and serpents, for instance—do not attain the same size as in Asia and Africa. But waiving this, we use the name New World, only with significance in its connection with history.

With the discovery of America begins a new period in the history of man and of nations in their civil relations. The enlargement of territory occasioned by it was not greater than the enlargement of the bounds of thought. The old world had been developed earliest, had gone as far as it could go; it had to wait till another great step should be taken before it could go on in its course. The highest progress of the human race, the complete development of its possibilities, was not possible till man should, in his wanderings from east to west, compass the globe, and take possession of it, not for a day, but for all time. The primitive settlements in Mexico, Peru, and Yucatan could not sustain themselves in consequence of their isolation; navigation was in its rudest stages, and it needed to be in its highest before the world should be bound together closely enough to advance in all its parts toward the goal of a perfect civilization. Those primitive colonies perished therefore, as Canaan perished before Israel, and were replaced by others. The reason of this lay in the isolation of the land-masses of the earth. Had America been discovered and made accessible to the old world before the diffusion of the Gospel and the establishment of the Christian Church, it would have been too early, and heathenism might have had its grandest triumph and its loftiest temples in the new world. The way was not open as yet for the high moral development of the race; and the highways of civilization were not made till the most modern times, when all was in readiness for the great advance which we are witnessing now.

The contrast to the great continental hemisphere is found in Australia, a land-mass of no insignificant size, situated at the center, or very nearly at the center of the great oceanic hemisphere, and surrounded by hundreds of groups of islands, generally of quite unimportant magnitude. The name Australia was fitly chosen; it indicates its true relations to the Southern or Austral ocean. As Africa is the true South to the eastern hemisphere, Australia is the true South to the great continental land-mass of the whole globe. As the earth has two magnetic north poles, and two north poles of cold, one of the former in Siberia, north of Lake Baikal, and east of Cape Taimura, 110° east of Greenwich; the other in the neighborhood of Melville Island, in North America, 102° west longitude from Greenwich, so there are, in a physical sense, two south poles, (we do not refer to the magnetic ones and the poles of cold,) a continental south pole in Africa, a marine or maritime south pole in Australia.

This country, the largest of islands or the smallest of continents as we may choose to designate it, the most remote of all the great divisions from the center of the land hemisphere, has been the last to feel the pulses of civilization. There, therefore, is to-day the most rapid, the most amazing advancement to be witnessed on the earth; it has crowded centuries into decades, and with its shores adorned even now, in its youth, with states and cities, it cannot longer be called a land left behind in the world’s advance. It has inherited all that was finished in the knowledge and culture of the continental world; what the people of that world have toiled for years to win, becomes at once the birthright of the Australians. It is only an instance of the truth of Humboldt’s remark, that the more full the world is of ideas, the more rapid is its progress—a remark which throws the strongest light upon the connection of geography with history.

The Historical Element in Geographical Science.

While so many a spot in the great continental land-mass was once the home of a high culture, and from being a cradle of arts and sciences has become a deserted waste, the civil and political condition of many people in the remote districts on the oceanic side of the globe has advanced with unprecedented rapidity. The course of development has been very different from what it was formerly. Distances, natural influences, natural productions even, yield always to the victorious march of man, and disappear before his tread; or, in other words, the human race is more and more freed from the forces of nature; man is more and more disenthralled from the dominion of the earth which he inhabits. The history of specific districts and of entire continents confirms this.

The first inhabitant of the sandy valley of the Nile was a dweller in a waste, as the nomadic Arab is to-day. But the later and more cultivated Egyptians transformed that waste, through the agency of irrigation and canals, into the most fruitful garden of the world. They not only rose themselves, but raised their own country, hitherto so sterile, into a place of the first importance, and did it by the simplest of means,—the bringing the water and the land into more intimate relations. Through neglect and the tyranny of successive kings, the fruitful valley sank again into its waste condition. The district around Thebes became a desert, the fruitful Mareotis a swamp; similar phenomena occurred in many parts of Europe and Asia.

Another example of man’s subjugation of nature is found in great mountain chains. During the first centuries after Christ, the cultivated south of Europe was separated from the uncultivated Celtic and Teutonic north by a great natural barrier, the unbroken, untraversed Alpine chain, which passed through all central Europe from west to east. At the south lay the rich states of the old world, beyond the Alps was the cold and barren north. But this old formidable barrier has vanished, as the thronged cantons of Switzerland and the crowded villages of the Tyrol yearly bear witness; and they draw thousands of tourists instead of repelling them. What a mighty change! From Provence to Styria run the stately forms of the Alpine chain; but the deep recesses and the lofty highlands are thickly peopled, the forests are thinned, the obstructing rocks removed. No longer a barrier between the north and the south, as it was in the time of Julius and Augustus Cæsar, Switzerland has become a country of stupendous highways. The peaks which were once unapproachable, and around which merely eagles idly flew, are now the passes of Mount Cenis, the Simplon, Saint Gothard, the Splügen, and Saint Bernard; while the snowy heights of Ortler, in eastern Alps, now give place to a public road. Over the Semmering Alp a railway even passes. Just as the wild horse of Toorkistan has given up his freedom and has become the tame and useful servant of civilization, so this Alpine segment of the globe has changed all its relations to the adjacent countries. The influence of the most stupendous natural objects is weakened every year. The physical dimensions may and do remain unchanged, but their influence on life and on history is undermined by those new conditions which operate so powerfully in freeing man from the dominion of nature. The power of man makes him master of the earth, and gives even the key to the subjection of the grandest mountain chains into his hands.

In further illustration of this, take the Ural chain, which was and still is the eastern division line of one continent, and the western barrier of another, but which has become, since the days of Peter the Great, a grand center of labor and commerce, a great avenue of civilization in its return passage from Europe to Asia. And so everywhere, from the wild Caucasus and the Himalayas to the grand Cordilleras of America, the same progress is seen; man becomes more and more the conqueror over nature. And not in mountains alone, but in the great forest regions of central Europe, in the primitive wilderness of North America, and in the marshes of the Netherlands, does man vanquish the forces which once fettered him. The once fearful wastes of Sahara have become the track of caravans; the sterile plains of Australia and California have drawn great colonies to their gold mines; the ice seas at the north have become, through the efforts of Parry, Franklin, and others, the scene of heroic exploits and of grand struggles of man with nature; indeed, the greatest victories of modern civilization have been there, and the playgrounds of polar bears and walruses have witnessed the noblest humanities, and the loftiest courage, and the most disinterested heroism of the age.

The continents and oceans have witnessed still greater transformations. The seas were once the impassable barriers of nations. The birds of the air only traversed the great distances which separated shore from shore. The metallic stores of the earth, the vegetable and animal kingdoms were not transferred to any extent from place to place; the sea brought nothing from lands remotely foreign but drift-sand, cocoa-nuts, floating wood, ice masses, and seaweed, swept by the great currents from shore to shore. But now the seas are no barriers; they do not separate the continents but bind them together, and unite the destinies of nations in the closest manner. The great improvements in ocean navigation have entirely changed the relations of the entire globe. The isolated island of St. Helena, which was for centuries at the very confines of the known world, became, within the second decade of the present century, a prison-house for the great European robber, and lay guarded under the eye of Europe. The Cape of Good Hope, which was for centuries the limit of Portuguese navigation, has become a mere halting-place for sailing ships and steamers. The voyage from England to China has been narrowed, within one hundred years, from an eight months’ to a four months’ sail. These great changes have been mainly effected by the agency of steam. Steam has transformed the smaller seas into mere bridges, and England and France are securely joined, Marseilles and Algiers; while Prussian Stettin is brought into proximity with Swedish Stockholm and Russian Petersburg. The voyage to America, that remote land, which before the days of Columbus was as inaccessible as the moon, was made by him in seventy days, but is now accomplished in ten. Even Australia cannot be said to be distant; a steamer needs but seventy-five days to reach it, and ten of those are consumed on the Isthmus of Suez. No island now lies beyond the world of commerce. The most active traffic exists between places the most remote. The wool and the wheat of Australia control the price of those commodities in London, and the value of cotton in America fixes that of woven goods and even of bread in Europe.

The great rivers too have been curtailed of their relative importance, and have been shortened by steam sixfold. They can be stemmed too, which is an immense gain, for in the primitive stages of navigation they could only be sailed upon downward, from source to mouth. In 1854, four hundred steamers traversed the Mississippi and its branches, and came into contact with a region one-third as large as Europe. The Indus, Ganges, Irrawaddy, Nile, La Plata, and even the Amazon, the monarch of rivers, which drains a country half as large as Europe, are now more or less open to steam navigation. The great river systems of central Europe too are thoroughly navigated; and Southern Germany, Trebizond, Mayence, Cologne, and London may be grouped as neighbors. The land-locked seas are reduced to insignificance, and their shores are now covered with villages and cities, from the Platten-See of Hungary up to the Caspian and the great lakes of North America.

To sum all up in one word, the mighty influence of Time on the geographical development of the earth is displayed in the clearest manner. But this influence is not the same for all localities on the globe. While there are some people and some places which are left behind, there are others which have made wonderful progress, and have taken and now hold a foremost place. And such a position is that of Europe at the present moment. Europe, the most central of all continents, in relation to the great land-mass of the earth, and also the one most equally removed from the middle point of the great water-mass, touches the whole remaining world at the greatest number of points, and this, in conjunction with her remarkably broken coast-line, so favorable to the purposes of navigation, have given her her place of command, and have assigned to England her evident role of mistress of the seas.

And looking from the present to the past, we see that as some great tribes of men have given the whole fruits of their natural existence to the world for its future use, so some places, and those of no insignificant size sometimes, have conferred upon the world, the trust which they once held, and now recede, as it were, from view. They were great in the past, and the results of their greatness are now incorporated in the world’s life. The earth is one; and through the agency of what we may call either time or history, all its parts are in ceaseless action and reaction on each other. Though some great districts seem now to have no part to play, the element of time draws them into the great cosmos; they once had a great share in the world’s affairs, and the fruits which they brought to completion are merely in other hands. The earth is, therefore, as was stated in the introduction, a unit, an organism of itself: it has its own law of development, its own cosmical life; it can be studied in no one of its parts and at no special epoch of its history. The past and the future, the near and the remote, are all blended in a system of mutual interdependence, and must be looked at together.

This is shown clearly in the past of Asia, and the present of Europe and some parts of the new world, while the history of all central Africa seems to lie wholly in the future. Heretofore it has enjoyed no progress excepting along its northern rim. The middle portion of the old world has outlived its primitive ethnographical impulse, and sunk back into a state of slumberous inaction. Asia, to call this region by its recognized name, has projected its own life from the center to the circumference; by this I mean, that while it seems to be exhausted of its old vigor, other countries inherited its power. The population of Asia is much less than it was in the time of Alexander the Great, much less than during the Mohammedan and Mongolian conquests, when all the habitable parts of that immense continent were bound together by highways of commerce and travel. On the other hand, the coasts are now of much more value and significance than they were in ancient times, and navigation has dotted her sea outline with splendid and populous cities. These seem, by reason of the facilities which steam affords, to be brought near to Europe; while the natives who inhabit central Asia are not only widely separated from the civilized world, but are divided up and set against each other by religious and political enmities of the most bitter kind. This is displayed in its fullest force by the comparative inapproachability of the great mountain chains, the Ural, the Taurus, and the Caucasus, and yet more by the unchanged barbarism of the central tribes, the hostile political relations, lacking all of the amenities and mutual dependencies of European policy, and the deadly antagonism of Mohammedanism and Christianity. This last is the curse which the natives of the earth have brought upon themselves. It is the clashing of religious faiths which has put the extinguisher on Asiatic progress, annihilated her enterprise, and set her in her present isolation. Still this barrier is not absolutely settled and for all time, but already it shows that it is capable of some modification. The politico-religious system of the Chinese is rending under our eyes; the old bonds which Mohammedanism once laid on Asia are now sensibly relaxed. The great highways of travel through the country of the Euphrates and Tigris and the extended archæological investigations of modern times have operated mediatorially between Europe and Asia; while steam navigation on the Danube has brought Turkey, a hitherto undissolved Asiatic element in European life, into closer relations with the great powers of the West. The great missionary enterprise, too, of modern times, has been laboring to remould the ideas of the Asiatic nations, while navigation has operated on the material and more appreciable interests of commerce and industry.

There are no possible limits to be assigned to the perfectibility of the globe as the abode of man; no possible bounds to his enterprise. The construction of a canal through the Isthmus of Panama would bring the eastern coast of Asia seven thousand miles nearer than it is now to the Atlantic shores of America and Europe. By saving the mere doubling of Cape Horn, one-third of the periphery of the globe would be annihilated, so far as the labor and expense of navigation are concerned. North America would nearly double its resources when its Atlantic and Pacific coasts stand in close connection and interdependence. The projected canal at Suez would exercise an unbounded influence over Asia in binding it anew to Europe. The building of highways through the passes of the Ural, the Caucasus, and Himalayas is yet to be accomplished; and only now are great roads constructing over the Rocky Mountains, welding North America together. The construction of railways on the high plateaus of central Africa will transform that vast undeveloped district, so rich in resources for the future. The changes which art is yet to effect on our globe are beyond all possible computation, and it might be said, beyond any possible exaggeration.

We turn away from these glances into the future to look upon the past, the long ages when men lived in rudeness and ignorance, having no art, and knowing nothing beyond the little tract where they were born, and to which they remained chained. There was no binding of shore to shore, and of continent to continent, through the mediatorial agency of seas and oceans. And this gave to the continents a far greater individuality than they have now, and a much higher degree of apparent influence than now when we cannot view them excepting as parts of the great complex which forms the world. The wanderings of the old nomadic races, the enlarging of the domains of culture, the transfer of the natural productions of all climes, as well as the traditional ideas of all lands, proceeded from the central portions of the ancient world toward the extremities. The manner of this progress, following as it does the order of history, displays more clearly than almost anything else the close dependence of all national development upon geographical conditions, and their indissoluble connection. Without this connection the order of historical events would have been completely changed. In no instance has there been self-evolved progress in the North, East, South, or West; it uniformly began at the geographical center, at the point of conflict between the Orient, the Occident, and the tropical South.

Western Asia, northern Africa, and southeastern Europe were the homes of the earliest culture, and it is to them that all other parts of the world owe the light which they enjoy, though they may have received it at second or third hand. The territory of which I speak extended from the highlands of India to Italy, and from the Nile to the Don, including the valleys of the Euphrates and the Gihon. This broad and fertile reach of territory has been the fruitful mother of the world’s present thought and culture. Nor must we overlook the fact that, despite what was said above, regarding the oceans as the greatest barriers to the spread of civilization, that smaller seas aided it, for the very country of which I speak was intersected by five important seas, and to them it is under immeasurable obligations for its development. This Asiatic-Africo-European belt has exercised the greatest influence on all the course of human affairs, on all colonization, on the differing of races and languages, and the arts of war and of peace, over the habitable world. This territory lies as the background of all the events of history, and has given to every one its distinctive character and its appropriate place. Nor can we in the future dispense with the element involved in this, of historical occurrences yet to come dependent on past geographical conditions, although this will be far less marked than it has been in the past. It demands and will demand a far larger measure of investigation and thought than it has yet received. Whatever independent progress the New World and Australia may seem to be making, and whatever interest they may awaken in the minds of students, not even they can be looked at without regard to their relations to the ancient historical lands, the source of all the inherited culture which they are enjoying in their vigorous youth. India, Egypt, Palestine, Greece, and other countries still stand out as the formative lands of all modern history, and we cannot study the present without studying them. They are to the student what Plutarch’s Lives are to the biographer, the imperishable and unequaled models which gain new luster as time rolls on. It is therefore not without reason that ancient geography ought to be subjected to a more systematic treatment than the geography of the Middle Ages. The latter, though not unworthy of a large place, had no relations of special importance to the whole world, to the study of the physical conditions of the most imposing objects of nature, to the connection as cause and effect of events past, present, and to come.

From these foundation principles, we advance to a more full study of the configuration of the surface of the globe, for which we are now in a measure prepared.

PART II.

A more extended Investigation regarding the Earth’s Surface.

It is the province of Hydrography to deal with the oceanic world; Geography proper concerns itself simply with solid forms. The Hydrography of the globe we must pass over, however. Aside from the fact that it would lead us into studies of the most protracted nature, it forms strictly one department of nautical science. Besides, there is the less occasion to speak of it here at length, that works of great excellence have been published, relating to that branch. We turn therefore to the land, and shall study the world of waters only so far as it exerts influence on the land.

By land we mean the islands as well as the continents, for, as remarked before, the difference between them is merely relative. To the land division of the globe, however, belong all rivers and the internal fresh water lakes, however large. The basis of difference does not lie in the fact that one part of the globe is water, the other part land, but in the fact that one is a tract of uniform evenness, the other of constantly varying surface, the internal rivers and lakes only being frills, so to speak, to the elevated region, and not sharing the sea level of the great oceanic mass. Uniformity of surface is then the chief characteristic of the sea; a lack of it, of the land. A mathematical level is a thing unknown on extended districts, and an approximation to it is very rare. Even the basins of former seas do not display a perfectly level bed. The plains of North Germany are characterized by this billowy rolling. The flats along the Danube, in Hungary, and along the Po, in North Italy, have really important deviations from a true level, though the eye is not able to discern them. Milan is four hundred feet above the Adriatic; but the eye does not discern that it is not at the center of a plain as perfect as the surface of the sea itself, and yet that plain does shelve gradually away till the Adriatic checks and defines it. Pesth is two hundred and fifteen feet above the ocean level, yet the gradual decline to the Black Sea is undiscernible to the eye. The immense plains along the Amazon, even the celebrated llanos on the Orinoco, which Alexander von Humboldt likens to inland seas of verdure, have a not insignificant slope from west to east. The middle point of these llanos near the City of Calabozo, about 100 geographical miles from the sea, he found to be 180 feet above the sea level; far lower indeed than Milan or Pesth, relatively, yet at a perceptible elevation. All of these plains were once the bottom of the sea; the Adriatic laved the base of the Apennines and the Cottian Alps, and the Atlantic swept westward over the llanos of the Orinoco and the Essequibo, having the Sierra de Venezuela on the north and the Sierra Parima on the south, till it was checked by the Cordilleras of Merida and Pamplona.

Depression and elevation, then, are the characteristics of the land. They are both measured from the level of the sea; their absolute altitude is reckoned from the imaginary sea level, extended over the whole globe. Their mutual relations to each other are determined from their relative heights. The absolute elevation above the level of the ocean can be determined in a number of ways. If the heights to be measured are in the immediate vicinity of the sea, a simple system of triangulation will effect it. If they are removed from the sea, the difficulties are greater, and increase according to the distance from the sea. The heights of great inland mountains are determined by complicated operations with the spirit-level, protracted trigonometrical calculations, the unwearied and skillful use of the barometer, and constant appeal to the boiling point of water. The description of these methods falls within the province of Physics.

As the determination of the heights of the loftiest mountains could not be made before the appointments of scientific explorers have attained to a certain degree of accuracy and delicacy, the knowledge of them in former times was almost wholly relative. The inquiries of La Condamine, Saussure, and de Luc, in the Andes and the Swiss Alps, are almost the only ones to be trusted among those of the older observers. All unscientific travelers without accurate instruments confounded absolute heights with relative heights, and innumerable errors crept therefore into the earlier text-books. It is only within the most recent times that Hypsometry has attained to the dignity of a science.

To meet and counteract the errors alluded to above, and current in the loose language of popular speech, we shall use a new and indeed arbitrary terminology,—arbitrary because the data which mensuration will sometimes furnish are now, in part, wanting. We will divide the earth not relatively, but absolutely, into highlands and lowlands. The great districts often met, whose elevations are very moderate, we call lowlands. They are, for the most part, immense plains, varied but little above the level of the sea. The great districts which inclose mountain ranges we call highlands, and sometimes plateaus. True highlands can often embrace very extended and elevated plains, and these plains again may include hills and mountains. This does not affect their character as highlands, which lies in the fact of elevation rather than in more or less modified variation of surface. There may be vast variety in the physical manifestations of a great plateau district, entirely independent of the relative effects produced by the distribution of its surface into plains, rolling land, hills, and mountains.

In the lowlands there may exist hills to some extent, and these may even be combined in ranges, provided only that they do not violate the uniform characteristics of the district in which they are found.

The highlands are generally met with in the interior of the continents; the lowlands at the coasts. Yet there are exceptions to this.

In the transitions from lowlands to highlands there is great diversity. We can speak of three distinct bases of discrimination: a sudden and abrupt ascent; a rise in elevation so gradual as scarcely to be perceived; and a terrace formation. Yet in these there is a blending of one variety with another; there is no place sharply marked, where we can say that one form ends and another begins. There are constantly found modifications of these three transitional phases. The plains along the Indus and the Ganges rise sharply to the plateaus of Thibet The flat Pacific coast of South America is exchanged with equal abruptness for the highlands of Peru. The transition is a gradual one from the lowlands of North Germany, along the Baltic and the North Sea, through Saxony and Bohemia to the Bavarian highlands, north of the Alps. The Spanish highlands form a series of terraces, increasing in height from south to north. The immense plateaus of central Asia are also terrace formations, of diminishing elevation, as they advance to Siberia; so, too, are the eastern plateaus of Peru, falling off in altitude toward the plains of the Amazon.

Just as varied are the heights taken from the sea level of the leading plateaus. Yet they never rise to a point of elevation comparable with those of isolated mountain peaks or ranges. These attain, in no insignificant numbers, the height of 24,000 feet, while some ascend thousands of feet beyond that. In Mount Everest, of the Himalaya chain, the loftiest summit yet measured (29,000 feet) is found; although it may be that future investigations more to the south will disclose yet greater heights.

Highlands.

Continuous highlands or plateaus seldom attain an elevation greater than a half or a third of the loftiest mountains; the most elevated range in altitude, from 8000 to 12,000 feet above the sea level. On an average, they lie about 4000 to 5000 feet above the sea. We take the last height as a convenient point of demarkation between the two classes of highlands—those of the first and those of the second magnitude. It is an arbitrary point, of course, and the division there must remain, without a natural base to rest upon, till more results in Hypsometry shall have determined the real point of average between the combined lowlands and the combined highlands of the earth’s surface. Meantime this division will be of great service to us in enabling us to bring into a definite and appreciable classification many facts which would otherwise not be so well understood in their relations.

Highlands or Plateaus of the First Class.

By plateaus of the first class, we mean those high, continuous plains which lie at the elevation of more than from 4000 to 5000 feet above the sea level. The extreme height to which such plateaus rise is a fact yet to be ascertained. At an elevation of from 4000 to 5000 feet the highlands of the first class merge into those of the second. The point of transition is, of course, very difficult to fix with precision.

The high plateaus of Asia rise more than 14,000 feet. They inclose the head-waters of the Ganges and the Indus. All central Asia is a vast congeries of highlands; but, as a body, they by no means belong to the most elevated of the globe. They are colossal in their length and breadth, but not in their uniform altitude. In the latter respect, they are far more varied than is generally supposed.

The plateau of Thibet attains, in its whole great extent of 1800 miles in length and 500 miles in breadth, an average elevation of 10,800 feet above the sea level. In some cases it rises, of course, much higher, as, near the holy lake Manasarowar, for instance, where it is 14,000 feet above the sea. Others sink, as at Ladakh, in Little Thibet, to an altitude of about 9000 feet; so, too, Gertope, in the region remarkable for its goats and the rich shawls manufactured there, and Shiffke, are about 9804 feet above the sea. The plateau of Great Thibet, east of Lassa, the capital, and north of the Upper Brahmapootra or Yam-Dzangbotscha, is 9000 feet in elevation. There are also districts filled with mountain groups of great heights, but where the depressions sink to the level of the valleys of the Indus, Sutlej, Brahmapootra, as low indeed as 5460 feet, as at Cashmere, so that there is no lack of diversity in the great plateau of Thibet.

The plateau of Mongolia, or more exactly the desert of Gobi, can be ranked only on its lower edges, where it touches the Chinese frontier, as of the first class, although in extent it is twice as large as the great plateau of Thibet. Only near the north bend of the Hoang-Ho and near Peking does it reach an altitude of 8000 feet, and gradually sinks away as it advances toward the northern frontier of the Chinese territory, to 5100 feet, and farther north to 4000 feet; in the middle portions of the great table-land it is depressed to a height of 2400 to 3600 feet; it rises again at the head-waters of the Orkhon and the Toola to an elevation of 4620 feet, and falls off in terraces toward Kiakhta, near the northern boundary, where it is 1330 feet high, Selenghinsk, on the Selenga, where it is 1632 feet high, and Berch-Udaisk, where it is 1458 feet high, till it reaches Lake Baikal, 1332 feet above the sea level according to Humboldt, though Erman makes it greater.

Western Mongolia, (west of the meridian of Lassa, and west of the point where the Tarine flows into Lake Lop,) upper Bokhara, and upper Toorkistan were formerly considered to be a highland district; this is now subject to doubt. We shall discuss this further on.

Africa, too, has highlands of the first class, which, however, do not rise to the extreme height of the plateau of Thibet. As in Asia, so in central Africa, the old supposition of the existence of a plateau of colossal extent has been very much done away with by the more exact and critical modern investigations. The strip of territory lying between 4° and 10° north latitude has been demonstrated by Barth and Vogel to be destitute of highlands. The range of mountains announced as discovered by Mungo Park, and called the Kong Mountains, is proved to have no real existence, and of course his statement fails of verification that that range is the northern limit of an elevated central plateau. The peaks which really do rise in the Kong territory form no continuous ridge; they are mere isolated groups of moderate height. Between these groups the lowlands continue toward the south, in an unbroken level, for an immense distance. How far south of the equator the central African plateau begins, is yet unascertained, for the snow-tipped peaks of Kilimandjaro and Kenia, discovered by Rebmann and Krapf, in the parallel of Mombas, 1° to 3° south latitude, are of immense height, it is true, but they do not demonstrate the existence of a plateau of the first class there. They rise out of table-land about 2000 feet above the sea level, which Krapf explored in the year 1849.

The Abyssinian plateau, on the contrary, takes rank among the most elevated on the globe. At 10° north latitude, south of the sources of the Blue Nile, lies Upper Abyssinia, or the kingdom of Shoa, with its capitals, Ankobar and Angolalla, 10,000 feet above the sea. Still farther to the north, in the ancient kingdom of Gondar, the German naturalist Rüppel ascertained the level of Lake Tzana to be 7000 feet above the ocean; to the southward of that the land rises to a still greater height, and northward of Gondar the plateau ascends to an elevation of 8000 feet, and mountains are met with 14,000 feet high. The terrace of Axaw on the east is 6650 feet above the Red Sea, which lies along its border.

To the south of Shoa lie the highlands of Kaffa and Enarea. All travelers agree in the statement that the inhabitants of that region are light-complexioned; and Johnson draws from this the conclusion that the central plateau must rise to a height of over 10,000 feet to harbor people of a whiter hue than the dwellers of the less elevated localities. He saw a number of men of light complexion who came as far as from the fifth degree south latitude, not from mountain homes, but from high table-lands.

The plateau of South Africa rises at Lattakoo, in the country of the Bechuanas, north of the Orange River, to the height of 6000 feet. To the east, near the Snow Mountains, where the river has its source, it ascends to an altitude of over 10,000 feet. To the north, discovery had made great progress since 1849. There, on a broad plateau, Oswell and Livingstone brought to the knowledge of the world the existence of Lake Ngami, whose surface is 2825 feet above the level of the sea. The plateau which includes this lake at its place of deepest depression cannot be less than 3000 feet high, and at some localities yet higher. Still more to the north, at latitude 14° south, on the water-shed between the Zaire or Congo on the west and the Zambeze in the east, the plateau reaches an elevation of 5000 feet, according to Livingstone. Yet farther to the west, it rises still higher and takes undisputed rank among plateaus of the first class. There, at 18° south latitude, Galtne, on his journey of discovery in 1850, ascended the table-land of Ovompâ, a region of great natural productivity. On the way thither, going from south to north, at 21° south latitude, and therefore in the parallel of Lake Ngami, but about 500 miles westward, he ascended north of the Swakop River, the table-land of Demara, which he found to be 6000 feet high. From that plateau mountains, Koniati and Ometako, for instance, rise to a height of 8800 feet. From the Swakop River to Lake Ngami there is a continuous plateau.

The high table-land of southern central Africa does not then extend, as was once supposed, as far north as 9° north latitude, nor even to the later limit of 4½° north latitude; but at about 4° 10′ the distinction between lowland and highland seems to be sharply drawn, as the cataracts which terminate the navigation of the White Nile indicate. Here Father Knoblecher turned back in 1849, but he ascended the first of the mountains which there began to rise; his eye reached onward to mountains very near or on the equator. He says that those high mountains stand upon an elevated table-land. Thus, here at the source of the White Nile we have a plateau seemingly of the first rank. From such a plateau it is probable that the snow-capped mountains, seen by Rebmann and Krapf in the neighborhood of the equator, rose, which they thought, approaching from the eastern coast, held the source of the Nile.

At the northwest of Africa, too, at 10° north latitude, the territory which feeds the springs of the Senegal and the Niger is supposed to be a plateau of great elevation and of great extent. But at present our lack of knowledge prevents our attaining certainty regarding it. No thorough system of measurement has been yet applied there.

America possesses a number of plateaus of the first class. To the most prominent of these belong the ones which were first thoroughly studied by Alexander von Humboldt. It is to him that we owe our first accurate impressions of table-lands which, before his day, had been indiscriminately confounded with mountains, and had had no place assigned to them in the department of Geography. Doubtless, too, great prominence was given to plateaus at the outset; they were pushed into unseemly proportion to other matters as well worthy of investigation, but they have come into their true place, and now only wait the development of new facts regarding the size and height of some, to be properly understood and appreciated.

The measurements made in North, Central, and South America give the following results; much more complete, it may be remarked, than the results yet gained in Asia and Africa.

To the plateaus of the first class belong in America, at latitude 0°, the plain of Quito, almost 9000 feet above the sea, (Los Pastos in the north being near 11,000 feet,) and to the south, at 17° south latitude, the plateau of Upper Peru. Here the great Lake Yiticaca is found, 12,000 feet above the sea; eastward of the lake, the table-land rises yet higher, and at Alto de Toleda it is 14,000 feet in elevation, as high as the highest part of Thibet. At 20° south latitude, south of Lake Yiticaca, is the City of Potosi, whose streets are 12,822 feet above the Pacific.

In Central America is found, at 20° north latitude, the extended table-land of Mexico, 500 miles wide, rising to a height of 7000 feet, and farther to the north, in New Mexico, the plateau of Santa Fé, 35° north latitude east of the Rocky Mountains, and 7100 feet above the sea. The table-land on the west side of the mountains, and toward the Great Salt Lake, is undoubtedly just as elevated.

Europe and Australia are wanting in plateaus of the first rank, and in general the whole immense flat northern districts of the globe, though we are not yet quite familiar enough with the extreme north of America to speak with entire confidence regarding it.

Plateaus of the Second Class.

Elevated plains which are at once continuous and bounded by a definite line of demarkation, and which do not attain an altitude of more than 4000 or 5000 feet, are considered plateaus of the second class. They are far more general over the whole earth than plateaus of the first class; in every one of the great divisions of the globe they appear in the utmost possible diversities of elevation, sometimes so gradually ascending that the lowest limit is hardly to be perceived. This makes it not only expedient but necessary to assign to plateaus a fixed though arbitrary system of classification, for without it we could attain to no thorough view of all their relations. This general system must afterward be confirmed and justified by protracted special investigations.

That not all the vast plains of Central Asia, from Thibet to the Altai Mountains, and from the Belur range to the Chinese Gobi, belong to the first class of plateaus, has been demonstrated by the Russian measurements, made by Fuss and Bunge in 1832, between Lake Baikal, Kiakhta, and Peking, and rendered highly probable by the investigations of Klaproth, Humboldt, and Zimmermann. Toward the northwest the plateaus generally sink from the moderate elevation of the Middle Gobi, 4000 feet, to Lake Baikal, 1332 feet above the sea, Lake Zaison, not 1000 feet above the sea, and the border of the plateau at Choimailocha, the Chinese frontier post on the Siberian line, 1000 feet above the sea, then to the lower border of the plateau of Bookhtarminsk (936 feet) and Semipalatinsk on the Irtish, (708 feet,) where the great Siberian plain begins. In the valley of the Tarim and of Lake Lop, pomegranates and grapes thrive, and cotton, which has been raised of an excellent quality in Eelee, is found at a height of from 1200 to 2000 feet. And in contrast with the great arctic plain of Northern Asia, not 500 feet above the level of the sea, this central plateau will take its place as distinctively of the second rank.

The plateau of Persia lies on the border of both classes; for while the central portion touches 4000 feet, some parts rise much higher and some sink much deeper than the normal point. These balance each other, and the average is about the maximum elevation of plateaus of the second degree.

East of the Persian plateau lies the plateau of Cabool, 6000 feet above the sea. On the northern edge of Afghanistan is the plateau of Bamain, 7500 feet in elevation. More to the south is the high plain of Candahar, being 3500 feet, and the City of Candahar, 3264 feet above the sea. The plateau of Kweltah west of the Bolan Pass is 5220 feet. Still farther to the south is the great plain of Beloochistan, 7000 feet, with the City of Kelat, 5418 feet above the sea.

In the central part of the eastern Persian plateau in ancient Gedrosia, Drangiana, and Parthia, and Lake Zareh, the depression is the lowest. At Lake Zareh the elevation is 2100 feet; at Herat, more to the north, 2628 feet. In West Persia, on the meridian of the Caspian Sea, it rises higher; on the northern edge at Teheran it is 3672 feet; at Schabred, southeast of Astrabad, it is 4000 feet; at Kasbin, west of Teheran, it is 4000 feet; and at Samegon, 5700 feet. The lowest depression at Com and Kashan is not 2000 feet above the sea. Toward the northwest Persia thrusts up a short arm into the adjoining territory of Armenia. This is the highland of Ayerbaijan, Zoroaster’s “Land of Fire.” This connecting plateau of 7000 feet elevation belongs to the first class. To the west of this the plateau of Armenia extends in varying range of elevation, from that of Lake Van, 5124 feet, to the plain of the Aras, (the ancient Araxes,) on which the double cone of Ararat rises to a height of 14,656 feet. But the table-land at the northern base of Ararat, the site of Erdschmiazin, is only 2860 feet high, Erivan a little higher, and Erdzeroune, on the plateau of the Taurus, the plain of the Upper Euphrates, 5730 feet.

The plateaus of Asia Minor embrace wide plains extending through the whole of the country, at an elevation toward the east, in ancient Lycaonia and Cappadocia, of 3000 feet, and sinking toward the west to 2000 feet.

To the plateaus of Armenia and Lycaonia, Strabo, whose home was there, and who carefully studied them, gave the expressive name of ὀροπέδια, i.e. mountain plains, a term which corresponds remarkably with our word plateau, but which, as Humboldt has remarked, was not of much use among the ancients. Strabo, however, directed attention also to the Oropedia of Sicily and India.

In India, Deccan displays similar formations, which rise gradually from south to north in Mysore, in Poonah of the Mahrattas, and in the table-land of Vindhya and Malwah, to 2000, 3000, and even 4000 feet. Deccan enjoys an admirable climate and the richest abundance of all natural productions. China too must have plateaus, for the Chinese word youen indicates very clearly a large elevated plain.

In Arabia the plateaus of the second class are largely found, and their height ascends from north to south, instead of from south to north as in Deccan. The Syrian Hauran is 2000 feet high, the plateau of Damascus 2200 feet, the plateau of Taif, above Mecca, 3000 feet, the plateau of Sapaa, in Southern Arabia, 4000 feet.

In North Africa that portion of the great Sahara which has heretofore been considered a low plain, lying between Tripoli and Lake Tchad, has been ascertained by the German explorers, Overweg and Vogel, to be a table-land of the second class, ranging in elevation from 1000 to 2000 feet. It begins at the Chorean plateau (2000 feet) in the south of Tripoli, and sinks to an elevation of 800 feet in the neighborhood of Lake Tchad. The average altitude is about 1500 feet. This moderate elevation of Sahara corresponds with the equally high plateau of Cyrenaica, 2000 feet.

The Atlas plateau, in the northwest of Africa, rises to a greater height—2000 to 3000 feet; the upper course of the Draa, near the Sahara, being 3000 feet; the high, broad table-land on which Timbuctoo lies, according to Renon’s measurement, is 1500 to 1800 feet above the sea.

In south Africa the low, or rather the moderate plateau, which borders the district of the Bechuanas on the north, rises, as it advances toward the lower rim of Africa, at Cape Colony, to an altitude of 3000 feet.

America has many plateaus of the second range of elevation, but her highlands of the first class are so imposing in extent, as well as in elevation, that they have been more carefully observed than the table-lands of the second class.

Along the eastern slope of the Andes, on the same parallel with the great plains of the Orinoco, the Amazon, and the La Plata, these plateaus extend, touching the base of the mountains, and appearing rather as terraces, or vast plains of transition, from the highlands to the lowlands, than as independent forms. Where Alexander von Humboldt measured them, west of the low plains of the Amazon, he found their height, measured from the sea, to range from 1050 to 1200 feet; he describes them as having the appearance of vast plains, and as differing from the lowlands of the Amazon only in their greater elevation; their slope toward the narrowing of the Pongo de Mauseriche being too slight to be appreciable.

Between the threefold forks of the Northern Andes, Humboldt ascertained the heights of ten plateaus, extending as far as the plains of Orinoco, and called by the various names, according to their elevation—Tierras templadas, or temperate districts, Tierras calientas, or warm districts, and Tierras frias, or cold districts—varying in height from 1800 to 6600 feet, the highest belonging clearly to the first class of plateaus.

The mountains of Brazil are interspersed among plateaus of the second class. The Brazilian mountains are not true ranges, but lie in groups, their height varying from 2700 to 5700 feet, and between them are the vast elevated plains, called Campas, which are true plateaus of the second class.

The southern point of South America, south of the Rio Negro, as far as the Straits of Magellan, known as the plateau of Patagonia, is a true table-land of from 1200 to 1400 feet in height. It is composed of ragged strata of porphyry or of vast lava-masses, and has been explored by Captain Fitz Roy, in 1837, from the mouth of the Santa Cruz River to the snow-capped Andes in the west. The plateau diminishes gradually in elevation from west to east, till it touches the sea line.

In North America the broad plateau extending through Northern Texas and the Indian Territory, and lying on both sides of the Arkansas River, increases in elevation gradually from St. Louis, on the Mississippi, less than 500 feet above the sea, to Santa Fé, on the upper course of the Rio Bravo, 7000 feet above the sea. It ascends so slightly that the rise is imperceptible to the eye, the broad plains there taking the name of prairies. St. Louis is 420 feet in absolute elevation; the eastern Arkansas plateau 1500 to 3000 feet; the high western Arkansas table-land from 3000 to 7000 feet, where, at the point of greatest altitude, lies the City of Santa Fé, in the Territory of New Mexico, 7047 feet above the sea. This broad, sloping tract reaches out to a great extent at the north, crossing the Missouri, and embracing the colossal North American lakes. Lake Huron and Lake Michigan, about 578 feet deep, and Lake Superior, 627 feet deep, lie in vast hollows in that great continuous plateau, which extends into the British Possessions, rises again to 800 or 1000 feet in elevation, and is rocky and craggy, yet not enough so as to take the name of a mountain chain, but simply to form a clearly-marked water-shed, which Fremont and Nicollet have measured.

In Australia and Europe plateaus of the second grade of elevation are not wanting. In Australia, however, they are limited to the triangular district in the southeast, which has become the place of settlement for the chief English colonies, and which, bearing the name of King’s Table-land, rises to a height of 2500 feet, and occupies the largest area of all the Australian table-lands.

In Europe this physical feature is displayed most distinctly in the Spanish plateaus, which occupy by far the largest proportion of the entire peninsula. Madrid lies on one of these plateaus, at a height of 2100 feet, five times as high as Paris, on the Seine, and as high as Innspruck, in the very heart of the Tyrol; Toledo, in the valley of the Tagus, is 1734 feet above the sea. The average elevation of New Castile, the central part of Spain, is 2000 feet. Old Castile, which borders it on the north, separated from it by the Guadarrama ridge, is about a thousand feet higher. Burgos, in the center, is 2700 feet above the sea; Segovia, to the south, 3100 feet. The average elevation of Old Castile is 3000 feet.

Then comes in natural order the Bavarian plateau, in southern Germany, ranging from 1500 to 1600 feet high, a broad table-land, on which lie Munich and Augsburg. It extends along the course of the Danube from west to east, from Lower Switzerland to Ratisbon.

According to the mean measurements of Humboldt, the lower plateau of Auvergne, in southern France, is 1040 feet in elevation; still less in altitude (840 feet) is the plateau of Burgundy and Lothringia, between the Vosges and the Ardennes. Limousin, Aveyron, la Forez, Monts, and Côte d’Or are plateaus.

The plateau of Lothringia, whose mean elevation is 648 feet, lies between the Rhine and the Moselle. The plateau of Luxemburg extends northward to the Eifel, where Prum lies, and to the Ardennes, where Malmedy, Eupen, Namur, Liege, and Aix-la-Chapelle lie.

In Middle Germany, a series of plateaus of the second grade begins in Upper Hesse, and extends eastward, crossed by mountains and valleys, traversing Upper Silesia and Galicia, and running along the northern side of the Carpathian Mountains to Podolia, on the Dnieper, thus embracing a strip extending through the larger part of central Europe.

A line of plateaus begins still farther to the north, at the low hills of Jutland, crossing Holstein, Mecklenberg, the whole southern edge of Pomerania, and extending to Lithuania and the Valdai Hills. It is characterized by a band of inland lakes, whose basins it incloses, and is crossed by the valleys of the Oder, Vistula, Niemen, and Duna. It has been called the Pomerania lake country. In the hollows where the lakes lie, (whose surfaces are, at the highest, not more than 300 feet above the sea,) and yet more in the depressions, where rivers break through, the level descends to as low a point as that of the great plain of Central Europe; but at other places it rises to an elevation as high as 500 feet, and so touches upon the limits of plateaus of the second range. Many parts of this broad upland may possibly be formed of shifting sand dunes which have been gradually piled up along the sea line. The plateau reaches its highest point at the eastern end, in the Valdai Hills, where it averages 1000 feet in elevation. The highest point is 1100 feet. East of the Volga, which rises at the eastern side of these hills, the plateau falls off by imperceptible steps, till it is lost in the great Russian plain.

In the peninsulas of Southern Europe, as in the Morea, (2000 feet,) and in the Crimea, (800 to 1200 feet,) the plateau again appears in not insignificant proportions.

The lower range of plateaus, it will be seen, is far more frequently met with through all parts of the earth than the higher, yet both combined occupy a larger share of the surface of the globe. We can designate them as sharply defined and broadly massive elevations, in contradistinction to the long, narrow, and broken masses which have received the name of mountain chains. The latter have too often been confounded with the former and have received from geographers a treatment disproportionately full in relation to their claims. The plateau has been until recently an almost forgotten geographical element. Humboldt restored it to its rightful place; by many hundreds of measurements he has accurately settled its form, its effect on climate, on isothermal lines, on agriculture, on the physical and moral life of nations, and even on the course of human history.

In closing this attempt at a general consideration of plateaus, I must confirm the reproach which Humboldt has cast upon most geographers of this day for their abuse of the word plateau. And I must at the same time admit that it is justly due to some parts of my own “Erdkunde,” where I have considered the plateau systems of Central Asia and Africa. When I wrote the pages of that work, thirty and more years ago, there were no scientific measurements then made of those regions, and the general ignorance led to a premature generalization, in which I used the ascertained features of the New World as probably in analogy with the unexplored center of the Old World. This use of really untrue analogies was carried by others to great lengths, and choratographers went so far as to depict the country according to the hypothesis of those who had written at first hand, and after using all the lights then existing, but who had never supposed that what they had indicated in general terms, would be afterward made so definite and real to the public eye. Those untrue statements of my own, I must leave however just as they are, and rejoice that the great advance of science has led to the accurate knowledge of the great plateaus of which the civilized world then knew but little. One word more: I set the lower limit of plateaus of the second grade at 500 feet, lower therefore than the great master in Physical Geography set his.

“Elevations of the soil,” says Humboldt, “which do not display a marked difference in climate and vegetation from the country around them, are not rightly called plateaus.” His meaning is, that the name does not relate to absolute height measured from the sea, but harmonious climatic relations existing between contiguous districts, one of which is more elevated than the other. Highland and lowland are therefore to him words of unfixed meaning, if they do not stand in the contrast of height, climate, relief, and rates of temperature. Humboldt therefore did not consider the depression of Central Asia, at the Taringol, as a plateau; and table-lands from 200 to 1200 feet in absolute elevation, i.e. from the sea level, are passed over by him as not worthy of the same name which he applied to the plains 6000 to 10,000 feet above the sea.

Dealing as I do with the elementary features and the physical contrasts of countries which for the most part are now thoroughly explored, I prefer, for the purpose of elucidating the subject of Physical Geography, to consider the plateau as beginning at 500 feet above the level of the sea. By comparing the plateaus of both hemispheres it is not difficult to deal with a variety of features, and to make a number of discriminations which, without an absolute standard, it would be impossible to make.

We pass to the consideration of the much more varied and more imposing characteristics of mountains.

Mountains and Mountain Lands.

Mountain lands cannot, in the strict use of language, be compared with plateaus, except in way of contrast, because they are not uniform, broad, and sharply defined tracts, but extend in a linear direction, having as their chief feature the longitudinal axis of the mountain chain. Groups of mountain ridges may be separated from each other, or may be united in any coherent way which does not make them continuous, and yet, despite the want of continuity, form a perfect whole.

Mountains, with their fissures, chasms, abysses, valleys, ravines, clefts, precipices,—in a word, their varied diversities of feature, broken through in every direction, the whole chain rent into fragments by these transverse breaks, are in direct contrast with plateaus. They have quite often a common range of elevation, which, measured from the sea level, is not unfrequently much greater than the districts lying at their base. Yet this relation is only incidental, it is not essential. There is no necessary connection between the height of the outlying plateau and the height of the mountain range. In Switzerland the mountains rise to the altitude of 13,000 or 14,000 feet; the country at the foot of the Alps is but 1000 to 2000 feet above the sea. Here the distance between the summit and the plateau at the base suggests no relation between them.

The distinctive characteristic of a mountain land is the height of isolated groups. Great differences of elevation within small distances characterize mountain regions; small differences within great distances characterize plateaus. The plateau depends upon uniform evenness of surface, or an approximation to it, over a large extent of territory. The mountain range is the exact opposite, the development of all kinds of extremes within a limited space, and the consequent individualization of the locality where it stands. Mountain lands cannot therefore be identified with the type of the highland and the plateau. The mountain chain has a character of its own, whether existing in unbroken unity, or subdivided into subordinate ranges, ridges, and spurs, and whether the summits are conical or sharply pointed,—whether also of moderate, medium, or loftiest elevation.

And high as mountains rise, their height is equivalenced by the depth of the depressions which form their valleys; the higher the mountain, the deeper the abyss which cleaves to the base. The immensely elevated peaks of the loftiest chains find their correspondence in the narrow ravines and the mountain lakes at the foot; the precipitous summits of the great American chain have their barrancos in the Andes and their cañons in the Rocky Mountains. The valleys are in natural contrast with the summits. They have just as little of the uniformity of lowland plains as the mountain tops have of the uniformity of elevated table-lands. They are infinite in variety, highly individualized, and always adapt themselves to the characteristics of the chain which conditions them. The mountain, too, has no uniformity in its character; it embraces within the smallest compass the production of all climes, and unites the characteristics of both highland and lowland. Mountain regions have therefore had a great influence in history and in the development of humanity, even greater than the more monotonous plateaus, which in general harbor nomadic races and give little encouragement to permanently settled people. For this reason the geographer cannot, like the geologist, classify high table-lands and mountains together; he cannot draw the same inferences from the plateau as from the mountain range; to the geographer the plateau is not a lower type of mountain, but the two, in their relations to man and to history, suggest entirely different results and condition entirely different processes.

And yet it must be confessed that mountains do stand in intimate connection with plateaus of both classes, and that the transitions from the one form to the other are well worthy of study. Yet the present lack of correct measurements has made this little understood.

It is not the element of height alone which gives mountains their significance. There are many other features, which are little studied, yet of real import. It is, however, not a matter of indifference whether a chain thrusts up its peaks 1000, 5000, 10,000, or 20,000 feet, and the height has been made and will continue to be made a subject of careful investigation. In reference to height, we distinguish what, in a general sense, we call mountains,[3] into hills, mounts, and mountains of various degrees of magnitude. Yet the height of the highest range, in comparison with the diameter of the earth, is insignificant, only about ¹⁄₁₇₀₀, and the combined mass of mountains are of no more account in comparing them with the entire mass of the globe, than the roughnesses on the rind of an apple, or perhaps more exactly still, than those on the shell of an egg. The combined mountain systems in the world would not suffice, if transferred to the North and South Pole, to fill out the earth to such an extent that the polar and equatorial diameters would be equal.

In following out his profound scientific investigations, Alexander von Humboldt, in order to ascertain the center of the earth’s gravity, taking into account the existing elevations above the ocean level, was led to the conclusion that too great importance was formerly assigned to mountains in their relations not to the course of history, but to the earth as subject to mathematical laws. Very careful observations revealed the fact to him that all the mountains of France, if reduced to a level and spread out, would raise the grade of the whole country to a height not more than 816 feet above the sea line. All the mountains of Europe, distributed in like manner, would raise the level to only about 630 feet. In Asia the same process would make the vast plain only 1080 feet high, in North America 702 feet, in South America only 1062 feet; while the mountains of the entire globe would raise the level to only 947 feet above the level of the sea. So insignificant are the combined mountain systems of the earth in respect to size, in comparison with the immense body on which they stand, though their importance is great when we regard their influence on the localities where they are found. Yet in this last regard, mountains deserve careful study, for they not only exercise and have exercised a great influence over nature and man, but they serve as our best key to open to our view the internal structure of the earth.

Some mountains, though of great height and broad base, like Etna, Vesuvius, Teneriffe, and many volcanoes, belong to no true mountain system; and even when they lie near together, and yet have no inner principle of unity, they are not spoken of as a chain or a range: they make merely a mountainous district. It is the repetition of the common type and the existence of a continuous valley which gives a right to use the names chain and range.

The linear extent and height of mountain ranges vary very much; no definite limits to these can be assigned. Yet there are few chains which are less than 25 miles long and 1500 feet high. Other features are necessary in order to determine the strict application of the word chain or range; one is a ridge-like or comb-like aspect; (that it should be a water-shed is not essential, although very common;) another feature is that the rock composing it should be of the same geological formation. Sand dunes, although occurring in regular and ridge-like uniformity, like those in Holland, and looking from a distance like a mountain chain, are not to be reckoned as mountain chains, though like the tells on the Syrian steppes and dunes in the Netherlands and along the Baltic coast, they sometimes rise to the height of a thousand feet. In South Germany and in the neighborhood of lofty mountains, such elevations are called mere hills; at the north foot of the Alps, yet greater heights are almost always called level land. In judging of the fitness with which the word mountain is used, it must always be remembered whether he who employs it dwells among the Himalayas or on the lowlands of eastern Europe; and in order to give any fixedness to the use of the word, it is necessary to take into account other physical characteristics besides height. By common usage, however, the Alps have become the standard of comparison for all the mountains of the world, mainly because, besides having their imposing height, they are found in the middle of the temperate zone; they are the most convenient to study of any great system on the globe. In respect to height, we divide these into four grades: the lowest from 2000 to 5000 feet above the sea; the next from 5000 to 8000; the next from 8000 to 10,000; and the highest from 10,000 on to the height of Mont Blanc.

Another standard might be found in the colossal Himalaya chain of Asia, and the Cordilleras of both Americas, which could easily be brought into unison with the Alpine chain of Switzerland.

The linear direction of a mountain chain, the axis of elevation as we might say, (so sharply hinted at in the very word mountain-chain,) brings out relations which vary not only according to the longitudinal direction itself, but to the lateral extent, the number of mountains, the situation, and the ramification of the chain. If the direction be a straight one, we can rightly speak of an axis of elevation. According to Humboldt’s measurements, this axis in the Pyrenees is 230 miles in length; in the Alps, from Mont Blanc to the Hungarian frontier, 515 miles; the Ural Mountains, 550 to 2042 miles; the Scandinavian Mountains, 1100 miles; the Altai Mountains, 9900 miles; the Kuenlun, 1600 miles; the Thian-Shan, in Inner China, 1700 to 2150 miles; the Himalayas, 1600 miles; the Yablonoi Chrabet, 550 miles; the Aldan, 400 miles; the Ghauts, 760 miles; the Andes of South America, 4400 miles; and the whole Cordillera of North America, 9200 miles. There is often much doubt about the true beginning and ending of a mountain chain, and judgments differ according as they rest on the fact of elevation or on the geological traces of upheaval where they begin to be manifest. Geographers are not agreed, for example, whether the Ural Mountains continue as far north as Nova Zembla, and whether one or two chains in America are to be spoken of as traversing the plateau of Mexico.

If there are parallel ranges, it is correct to speak of a transverse axis, running at right angles with the main axis. There is, it is apparent, a marked difference between simple chains and the accumulated parallel chains, where breadth is a prominent element, as in the Vosges, the Black Forest Mountains, the Fichtel range, the Hartz, the Ardennes. The parallel rows form a mountain system. Yet all great chains are made up of smaller ones, of groups at least, and so are mountain systems. Often the grouping is seemingly irregular, a lawless aggregation, but only because our knowledge is incomplete, and the law of arrangement concealed from us. This law is traced in the very geological qualities of the chain, not in the later form. The outer form is often very deceptive, the very convulsions which indicate the surer signs having served to obliterate what we should suppose the most prominent marks. The present of mountains must often be studied in the light of their past. Orography must be interpreted by geology. But the geological surveys of the earth are as yet very imperfect; the outer form has often to be accepted as the only guide. Orography and geology are two sciences which now go on hand in hand.

In the simple mountain chain it is easy to discriminate between the parts which make it up; the base is easily ascertainable and the ascent to the comb-like ridge is readily traced; the eye does not fail to see the relation between the special prominent heights and the chain from which they rise, and to trace the manner in which spurs and outlying mountains are connected with the main chain. Small isolated collections of mountains are especially valuable as elementary studies, for they always have a unity of their own. And all the greater and well-known chains are made up of smaller, simple chains, whose connection and mutual relations are, however, sometimes exceedingly difficult to trace. But the character of the whole is not sometimes ascertainable with this preliminary knowledge of the parts.

The true base of a mountain chain, the line of periphery, in consequence of the general unevenness of the adjacent country, must be ascertained by very exact measurements with the level. The geologist does not begin with this step, he strikes deeper, and seeks the place where the structure diverges from that of the more level land lying near; and, in the search after the basis of structure, he discovers the unity of the range from the foot to the summit. The whole geological district which has been upheaved into mountains, Leopold von Buch found to be generally ellipsoidal in form, the longer axis being far more prominent than the shorter one. The axis of most mountain chains is, then, the longer axis of an ellipsoid. The Swiss Alps display about a dozen such ellipsoids, of different characteristics, and arranged according to no perceptible law of harmony. Each is developed from its own base, as the trunk of a tree grows out of its root. These separate bases lie contiguously, but the peaks which shoot up are widely sundered. The forms of the mountain groups resulting from this are, of course, various. Some of them I will briefly characterize.

1. The longer axes of the subordinate chains may run in parallels, as in one portion of the Swiss Alps, the Jura, the Ural Mountains, the Mexican Cordilleras, and the Himalayas.

2. The chains may diverge or converge. The Alps diverge at the east, and the forks run northeast and southeast respectively; the Rocky Mountains, toward the Arctic regions, divide into from five to seven diverging chains. Converging ranges may come together at varying angles, and these can mass themselves into confused mountain knots, the summits of which soar to amazing heights, as the West and Middle Alps do around Mont Blanc. Alexander von Humboldt distinguishes five of these mountain knots in the Andes, Porco, Cuzco, Pasco, Assuay, and Los Pastos, whose construction, carefully studied, he considered, gives the key to the structure of the whole chain. Side chains often display this knotted form, as in Upper Peru around Lake Titicaca, the three branches of the Ural, at the Irmel Tau, the Himalaya, Kuenlun, and Hindoo Koosh chains, in upper Afghanistan, and the ranges of Swiss Alps, which converge around St. Gothard. Yet the convolutions which these mountain chains make at their point of convergence are never regular, never mathematically exact, but to be measured in sections, and the traces of a linear direction to be carefully sought with the compass. The whole has, to the eye, a labyrinthine appearance, and the law of structure is only ascertained, with exactness, by the geological features, the direction of the strata, and the like. The geographer must call in the geologist to help him solve his problems.[4]

3. If from some high central point the mountain ranges radiate in the form of a star, they form a new variety of system called, for convenience, by the name “star-shaped.” In volcanic mountains this configuration is common, as in Mont d’Or and in Auvergne. The southwestern Alps, known sometimes as the Sea Alps, the Ural at the Arctic Ocean, the Quito range of the Andes, are types of this form.

4. The ring-shaped system is in direct contrast with the last. It is found where mountain chains are arranged in a circle, inclosing a plateau of larger or smaller extent. There are two marked examples of this form in Europe: Bohemia and Transylvania. The ring of mountains around the former is made up of a number of ranges, which dovetail together at the ends, making a unit, but only a rude circle, speaking with mathematical exactness. The inclosed basin is only relatively a lowland; it is rigid with hills and low mountains, yet of such little importance, in comparison with the rim of peaks, that the common name, the “Bohemian Kettle,” has begun to have an accredited significance, and is stronger than the more loosely-used word Basin. Transylvania, too, partakes of similar characteristics. Its border consists of a number of minor ranges, of varying heights, up to 1800 feet; and the central hollow, which is much more strongly marked by hilly land than Bohemia, lies 2200 feet above the Adriatic. The ring-shaped system is one of the rarest met of all. They are, however, observed in abundance on the moon.

5. Just as rare is the form where ranges intersect in the form of a cross, those running, for example, from north to south, meeting those running east and west. As an instance of this, Humboldt cites the confluence of the Himalaya, the Kuenlun, the Hindoo Koosh, and the Belor or Belurtagh Mountains. The belt between 35° and 40° N. lat. is remarkable for its gridiron-shaped mountain system, the points of conjunction being marked by knots of peaks of colossal height. The most remarkable one of these is the lofty Pamir Pass, between 37° 30′ and 40° 5′ N. lat., and 18,000 feet high, known, historically, from the sixth century, and described by Marco Polo, as well as by the ancient Greek historians. The Persians dwelling in the neighborhood term it the Roof of the World. Elsewhere the same feature is observable, though on a scale of less magnitude. So in the Altai range at Lake Yetzkoi, in the western Swiss Alps, and in the porphyritic chain of Room-Elee, known to the ancients as Rhodope, and now as the Despoto Dagh. This gridiron-shape of some mountain systems seems to be the result of upheavals at different times, which necessarily occasions the most broken configuration at the point where a chain of more recent formation has been projected through one of older date.

The varying relations of length, breadth, direction, connection, and severance of mountain ranges give great diversity to them, and impart to every system a character of its own. To the features just indicated must be added vertical or precipitous descents, for the influences which they exert upon the possibility of man’s constructing mountain roads, are very great. The extent of these sudden depressions, or, more exactly, the relation which the distance from the base to the pass bears to the distance from the base to the summit, gives a key to the uses of certain mountains as adjuncts of civilization, and shows how some ranges rather than others may become the abode of men, and produce marked effects on human culture and the world’s history.

I have before alluded to the comb-like structure of most mountain chains. The resemblance is more striking than may appear; for not only do the peaks correspond in general uniformity of height with the teeth of the comb, but the equally uniform height of the passes from the base corresponds with the uniform thickness of the solid part of the comb. The relation, however, of the distance from the base to the passes, to the distance from the base to the peaks, is widely various. Humboldt has estimated it in a few leading chains as follows:—

In the Alps and Caucasus the relation of the height of the pass to the height of the chain is as 1 to 2; in the Himalaya, Quito Cordillera, and Alleghany Mountains, as 1 to 1·8; in the Pyrenees and Cordillera of Bolivia, as 1 to 1·5. In the Alps, therefore, where the pass is only half as elevated as the chain, the communication is the most direct, and the least barrier is put to the purposes of man,—a fact of great import in relation to human culture. The Pyrenees are in direct contrast in this respect, the most unapproachable, the most sundering of mountains.

The position of mountain chains is a matter of the first importance in relation to the welfare of man, and the solution of many of the most important problems in history. Whether interior ranges like the Ural and the Atlas, or ranges connecting two seas like the Caucasus, or those like the Mexican Sierras, lying between two oceans, are most open to human approach and use, is a question which we will not here stop to consider; but it may be said that, whether situated in the relations just indicated, or whether they are meridianal ranges like the Ural, the Scandinavian chain, the Alleghanies, or the great Cordillera of both Americas, which extends from the tropical world to both polar zones; or whether they run in the same direction with the parallels of latitude, turning one side to the colder north, and another side to the sunnier south; or whether they assume a diagonal direction like the Swiss Alps, from southwest to northeast, or like the Caucasus, from northwest to southeast, is a matter of the first importance to ascertain. Of not less consequence is it to discover whether the chain is the edge or rim of a plateau, and can have, therefore, only a one-sided development, like the Himalayas toward the south, or the Anti-Taurus toward the north, because the existence of a plateau on the reverse side dwarfs the slant distance, and gives but a fractional part of what, without the plateau, would be open and clear.

As plateaus usually display this edge on both sides, the border has been aptly compared to a double ledge or rim, between the two sides of which the table-land lies, often tolerably high above the sea level. If these rims, like mountains, are not contiguous to the plateau; if they are separated from it by a valley of greater or less width and depth, running parallel with the edge, they form what Humboldt has called natural circumvallations. Of such the Altai range, on the north side of the Asiatic central plateau, is an example. The hollow between the range and the plateau just mentioned is partly filled with inland seas. The Caucasus may, in like manner, be regarded as the circumvallation of the American plateau, separate from it by the Koor and the Aras (ancient Araxes) rims. Yet in the Caucasus another modification occurs—a partial linking of the plateau with the range at the west extremity, by the connecting chain of the Moschic Mountains. In like manner the Pyrenees, in their eastern half, form a circumvallation around the north side of the Castilian plateau, separated from it by the basin of the Ebro, and forming a perfect ring around Upper Castile and the elevated province of Biscay.

In cases where a mountain chain rests upon a plateau, rising up in the very heart of it, its summits seem to be not high, although the basis, the true foot of the chain, may not be at the level of the plateau, but far lower, and such mountains may, therefore, be of great absolute height. The name superimposed mountains has been given to them. Such are the Kuenlun and the Thian-Shan ranges of Central Asia, the Guadarrama chain between Old and New Castile, and the Rocky Mountains in North America. These superimposed ranges often run near to and parallel with the rim or edge of the plateau, and seem to give it more completeness and breadth.

The geologist employs the word “sutures” to designate such forms, because they serve to unite those parts of a plateau which are at different heights above the sea level. He regards the mountains as rising to fill enormous clefts which great convulsions have rent in the earth, and as passing up, while in their fluid state, to a height above the level of the plateau, and bridging over the abyss. In this way our mountains which rest on plateaus seem to have been formed, as indeed is indicated by their geological structure.

The smaller plateaus display analogies kindred to those seen in the larger superimposed mountain ranges. The extinguished volcanic group of Auvergne rests upon the central plateau of southern France, which, according to Remond, has an average elevation of 1000 feet. The now silent volcanic group of the northern Rhine broke through the moderately elevated gray-wacke formation of that locality, and is, therefore, a superimposed range.

Mountain chains which diverge from plateaus and their serrated rims seem, nevertheless, to have some relation to them, even though they cannot be considered continuations of them. The Lebanon chain, for instance, which turns away at a right angle from the Taurus range, and runs southward through Syria and Palestine; the Lutznetskia and the Alatau Mountains, mineral ranges running from the Altai northward to Tomsk; the Yablonoi and the Stanovoi Chrabet ranges running to the northeast; the still unknown or little known range of Farther India, traversing the whole peninsula of Malacca, come under this head.

Completely unlike the groups thus far considered, are the isolated mountain systems, with uniform slopes on all sides, and with a roof-like form, distinguishable to the base. The mountains of Europe are mostly of this class—the Ural, Carpathian, Scandinavian ranges, the Alps, Apennines, and, in part, the Pyrenees. They give rise to rivers, not on one side alone, as do the Himalayas and the Andes; they are rich in resources of all kinds for the student and the economist, and thus make up in part for their comparatively unimportant dimensions. Their double-sidedness gives them a large influence on civilization, since rivers flow from them in all directions; while from the Himalayas they only flow to the south, and from the Andes to the east.

Plateaus and mountains, different as they are in appearance and characteristics, yet constitute, in their mutual action and reaction, and in their forms of transition from the one to the other, the highland system of the globe. Their relations are inexhaustible as Nature herself. We cannot study them without profit; but we can never come to a perfect knowledge of them all.

The Relations of Plateau Systems.

Like mountain systems, plateaus are not to be estimated in respect to elevated and superficial area alone, but in respect to form and position as well.

The American plateaus are elongated from north to south, but are of disproportionate breadth from east to west. The Asiatic plateaus, on the contrary, are not only of great length, but also of great breadth. The Spanish plateau, that of the Atlas system, and that of Asia Minor have their length and breadth nearly equal.

The surface of plateaus is exceedingly varied. It sometimes assumes the aspect of elevated plains, sometimes of rolling land, sometimes of horizontal strata of naked rock, as in Patagonia and the western Sahara. In one place it displays sand-hills, as in parts of the Gobi Desert; in others barren steppes, as in portions of Persia. Sometimes we find a gradual ascent of minor plateaus or terraces; sometimes single mountains rising out of the plateaus, as does Demavend; sometimes we find a chain of colossal peaks emerging from the heart of a plateau, like Thian-Shan and Bogdo-Oola. Sometimes there are plateaus broken up into crags and patches of level ground, like Persia; sometimes plateaus with deep valleys or river basins, like the plateau of Yoorkistan and Gobi, including the River Tarim, and reaching its greatest depression at Lake Lop, or, like the plateau of Afghanistan, including the River Hirmend and Lake Zareh; again, we have plateaus traversed by water-courses which forced their way in times of flood, and leave in the rainless seasons the traces of the former violence. Such are some of the less elevated plateaus of France and Bavaria.

Especially important are the combinations and groupings of plateaus, as well as their relation to adjacent lowlands.

In Africa the plateau form embraces the larger southern half of the continent. Low plains are, on the contrary, the prevailing form in the north, broken, however, by the Sahara, and the high coast plateaus of the Atlas range, and of Barca.

In Asia there is a vast central plateau with gradual declivities toward the east, toward Yoorkistan and Persia on the west, and toward Lakes Baikal and Zaisan on the north. On the south the descent is abrupt to the Indian lowlands.

In Europe there are, for the most part, scattered and disconnected plateaus of small size and little elevation, often passing by an imperceptible gradation to the other forms. The Spanish plateau is, however, a marked exception, and has the sharply-defined character of the northern African plateaus. In eastern Europe the central situation of the isolated Valdai plateau, whose elevation is very moderate, but 840 to 1080 feet, is remarkable, and is of very great influence in determining the hydrographical character of the great Russian lowlands. And in fact, the hydrographical influence of both mountains and plateaus is so great, that it is worthy of careful and special study.

The combinating and grouping of plateaus in different continents give rise to great contrasts, observable most distinctly in Asia and America.

Asia, with all its great internal depression from Cashgar to Lake Lop, yet displays such immense districts of plateaus, all ranges of elevation, low, moderate, and very great, that the very grandeur and extent of its colossal mountain chains are subordinate in comparison. Asia is the land pre-eminently of plateaus.

America displays, not in its central but on its western coast, the greatest chain of mountains on the globe, flanked by plateaus of great elevation, but of superficial area quite out of proportion to the length of the mountain chain, and to the extent of the lowlands of both the northern and the southern divisions. And while in Africa the regions of depression are in the north, and in Asia around the great central plateau system, in the Americas, both North and South, they are thrown into the eastern portion.

Australia, in perfect contrast again, is, with the exception of its southeastern corner, a vast tract of unbroken lowland. No diversity is possible there, no change in the condition of life, but a ceaseless uniformity of monotonous but prodigal gifts.

Is not the imposing grandeur of these harmonious, provisional arrangements for the use of man calculated to fill the soul with admiring wonder, and to lead us to suspect, above all this display of cause and effect, above all this working out of a manifestly preconceived plan, the existence of a great and active Being, who has planned and executed it all with higher ends and a loftier purpose than to satisfy the mere earthly life of man?

Primeval Formation of Plateaus and Mountains.

To enter upon a discussion of the manner in which plateaus and mountains were formed, would make it necessary to resort to such judgments as we could draw from their external appearance and their internal structure. The rapid progress of geology does indeed afford us many probabilities thoroughly grounded. A few of these may have been briefly indicated in connection with some elevated regions, where the massiveness is striking, and where the axis of elevation is prolonged to a considerable extent. In such cases the influence exerted on the world is more evident than it could be elsewhere.

Origin of Plateaus.

Alexander von Humboldt has employed the term Intumescence, to indicate the manner in which plateaus have been upheaved. Plateaus appear as long, often wide, mostly level, sometimes rolling, sometimes hilly elevations, presenting an appearance as if the earth had swelled with confined gases, and with depressions here and there as if, in the casting of the molten mass within, a natural external subsidence had followed. They have, therefore, viewed in their internal structure, an unbroken wholeness, and are free from those vast fissures which characterize mountains, rending the earth for hundreds of feet down. The utmost want of uniformity is seen in the gradual depressions which often harbor the large internal lakes found in great plateaus. Varied as they are in configuration, they always retain marks enough to indicate that they owe their upheaval to steady, gentle, and not tumultuous forces within, exerted at the time of the primeval cooling of the earth’s crust; in contrast, therefore, with mountains, which were thrust up from beneath, through huge seams made by the bursting through of pent-up vapor and gases. These elevations of the earth’s crust, whether in the form of mountain or plateau, must correspond, in order that the symmetry of the globe may be preserved, to the depressions found in lowlands and beneath the water of oceans and seas.

It is observable that the great plateau upheaval of the Old World has taken the shape of a belt, which runs in a northeasterly direction along its whole southeastern shore, crossing the equator at an angle of 45°, broken, however, at some places, but never so much as to destroy the coherence of the belt. The diagonal of the rhomboidal plateau of eastern Asia, passing due northeast through the table-land of Thibet, indicates the direction of the whole band of highlands. This band drops toward the south in uniformly steep declivities; while toward the north it falls away with gradual steps of transition, reaching at length the regions of the greatest depression—Libya, northern Arabia, the Caspian, Siberia, and, at last, the low regions around the north pole.

In this belt or chaplet of plateaus lie the high table-lands of South and Northeast Africa, Abyssinia, South Arabia, Persia, Beloochistan, North Deccan, Afghanistan, Thibet, East Tangut, and eastern Gobi, in Mantchooria.

Correspondent with this immense plateau belt, in the New World, is the great American chain, once a wholly volcanic, and though differing so much in structure, direction, and hydrographical influence, yet giving the globe a wholeness, a unity in diversity, which is strikingly apparent.

The Origin of Mountains.

The linear regions of elevations of the earth’s surface, as we may term them, in contradistinction to the plateaus which are characterized by breadth rather than by length, have been projected in the form of mountain chains, as has been already hinted, through huge fissures made by the rending of the earth’s crust. The upheaval to fill the seam has, in some cases, been all made at once; in others, in a succession of periods. The uniform agreement of all the geological strata or their diversity decides this point. Sometimes the rocky strata are laid bare and easily investigated. Often, however, the observer is obliged to draw conclusions from a part to the whole. Yet in all cases the mountain, in contradistinction to the adjacent plateau, is the tract which has been thrust through the crust. The frequent steep and lofty precipices show the immensity of the internal force required to lift the mountains from their places, while the lines of stratification indicate the direction of upheaval. The rifting of a seam in the earth’s crust was the first step in the formation of mountains; the filling up of the seam by liquid matter, the second step. The upheaval of Asia, from the Persian plateau to Gobi, in a line 60° N. E., seems to be connected with the most ancient revolution which the earth’s crust ever experienced. The mountains there are, therefore, more modern in origin than the plateau on which they stand. The direction of the chain, in all cases, seems to have been dependent on the direction of the fissure in the earth’s crust, which the mountain range afterward fills. The breaking through the crust necessarily occurred when the pressure beneath the surface was very great, or when a moderate pressure was exerted beneath a thin crust, where the resistance was slight.

The latter case seems to have been prevalent in most plateau regions. Their own gradual upheaval probably thinned the surface, and made it more liable to fracture. This accounts for the fact that the greatest mountains of the globe are found contiguous to plateaus. And the broader the original seam in the crust was, the broader the mountain range which rose to fill it, either at a single upheaval, or in a series of convulsive throes projecting successive masses of molten matter from below. In the latter cases the strata thus formed lie on each other like the leaves of a book, their constitution changing according as the more advanced stages of melting in the vast internal caldron throw out more metamorphosed rocks. These later layers rose to a greater or less height on the sides of the partially-formed mountain, according to their specific gravity, their more or less fluid state, and their rapidity of cooling, as we can now see by examining the layers in their present permanent condition.

Thus far we can conjecture, with great security, taught by the manifestly wild and fierce convulsions which once threw up the mountains, since in them distortion is the rule and regularity of structure the exception, and also by the equally manifest quiet and sustained process of upheaval, when the plateaus were formed; their strata being in a state of regularity and unbroken repose.

When the great vents produced by the outward pressure of internal volcanic forces occurred beneath the sea, they were filled up in the same manner as on the dry land, excepting that the summits of the mountains emerge above the surface in the form of isolated islands, or when there was a chain or group of mountains upheaved, as an archipelago. When there was no rifting of the surface, and no forcing up of whole chains of peaks through a thinned crust, the fierce action of the internal heat appears to have necessitated the upheaval of solitary volcanoes here and there, in some cases even rows of them, to give vent to the pent-up steam and gases, and to convey away the molten tide within. When such volcanic series rose in parallel ranges, they lifted, or may have lifted up the whole district between them, as if upon their shoulders, and so formed the American type of plateaus, of less breadth and greater length than the Asiatic, and in height corresponding with the volcanic peaks which form their rim, and to which they are probably indebted for the form of their structure.

It needs hardly to be added to what has been said above, that the general direction of existing mountain chains depends upon the direction of the primitive seams made in the earth’s surface by internal forces. The Ural Mountains, the Scandinavian chain, the Alleghanies, the Ghauts, run on meridian lines; others more or less transversely.

The various kinds of rock which have been thrown up in mountains enlighten us as to the process and results of the internal heat of the earth; the successive formations display not only the various eruptions of molten matter, and its discharge in new layers above what had been thrown out before, but reveal the relative age of the various formations. We have in a single chain sometimes a whole volume of history, marking off the epochs of upheaval with the most perfect legibility and exactness. Many crystallised rocks result evidently from the gradual process of cooling after the ancient exposure to the intense heat of the inner portions of the earth—granite, porphyry, gneiss, slates, and the so-called metamorphosed rocks. These used to be considered the oldest formations, but the upheaval theory treats them as the latest formed.

Most mountain chains have been uplifted to their present height by a succession of upheavals. To accomplish this has been labor of uncounted thousands of years. Only a very few—the main Carpathian range, for instance—seem to have been upheaved at a single convulsion, and to have assumed their present appearance at once. Where there were incessant eruptions accompanied with flames, and masses of molten matter (lava) have been ejected from the crest or from single summits, these volcanoes and volcanic ranges have been the result. Elsewhere no such phenomena have been visible. Possibly, in such cases, the masses cooled so rapidly as to extinguish or fill up what may have been embryo craters, and the plutonic acclivities may have been repressed, leaving us the traces of primeval eruptions, but no vestiges of any dangerous forces remaining till now. Of mountains formed in this manner, may be mentioned the Puys de Dome, the Bohemian basaltic peaks, trachyte Transylvania Alps, the Katak Kaumene, (“Burnt Tract,”) of Asia Minor, and Hauran, Iceland, parts of the great American chain, parts of the Sunda chain, the South Sea Islands, and Bagdoola, and its range of extinct volcanoes in the Thian-Shan chain.

But other forces besides fire were competent to form mountains and plateaus, to spread layers of clay and sand and various deposits at the bottom of the sea, afterward to harden into strata of rock. In contradistinction to plutonic formations, these have been called neptunic, because formed at the bottom of the sea. The oldest of the neptunic or stratified rocks have been upheaved by the subterranean forces, and now are found in the elevated plateaus or mountain ranges, still having, however, their unbroken irregularity of structure. Also, after the stratification has been complete, and plutonic acclivities have opened the seams in the earth of which I have already spoken, and molten masses have rushed up to fill them, fragments of the primitive stratified rocks have been caught up and raised, together with the molten masses, to the very summits of lofty mountains; so that the geologist finds fossils there more or less perfectly preserved, the stratified rocks which contain them surrounded by the plutonic rock upheaved from below the surface. Chalk layers full of mollusca and infusoria have been found by Humboldt and von Buch on the very summits of the Andes, and corresponding with those which have been discovered by Ehrenburg in the deposits at the bottom of the sea.

Other older and more recent oceanic deposits are found in their primitive condition at the bottom of the sea, or in very low places on the land. In such localities the surface of the earth is composed of horizontal or slightly inclined layers or strata, of secondary formation, and whose origin in deposits from water cannot be denied. These are the beds of chalk, clay, sand, marl, gypsum, and other common substances; and these strata again have been overlaid with more recent accumulations, the result of diluvium or alluvium, continuing even up to the present time.[5]

Lowlands.