CHAPTER XII

TERRAQUEOUSNESS AND TERRESTRIALITY

With the vanishing of its seas we get for the first time solid ground

on which to build our Martian physiography. The change in _venue_ from

oceans to land has produced a complete alteration in our judgment of

the present state of the planet. It destroys the analogy which was

supposed to exist between Mars and our earth, and by abolishing the

actuality of oceans there, seems, metaphorically, to put us at first

all the more at sea in our attempt to understand the planet. But looked

at more carefully, it turns out to explain much that was obscure, and

in so doing gives us at once a wider view of the history of planetary

evolution.

The trait concerned is cosmic. Study of the several planets of our

solar system, notably the Earth, Moon, and Mars, reveals tolerably

legibly an interesting phase of a planet’s career, which apparently

must happen to all such bodies, and evidently has happened or is

happening to these three: the transition of its surface from a

terraqueous to a purely terrestrial condition. The terraqueous state is

well exhibited by our own earth at the moment, where lands and oceans

share the surface between them. The terrestrial is exemplified by both

the Moon and Mars, on whose surfaces no bodies of water at present

exist. That the one state passes by process of development into the

other I shall now give my reasons for believing.

In the first place the appearance of the dark markings both on the Moon

and Mars hints that though seas no longer, they were seas once upon a

time. On the moon, not only does their shape suggest this previous

condition, but the smooth and even look of their surfaces adds to the

cogency of the inference. More important, however, than either of these

characteristics, and confirmatory of both, is the fact that the great

tracts in question seem to lie below the level of the corrugated

surface, which is thickly strewn with volcanic cones. Their level and

their levelness fay in explanation into one another. The first makes

possible the former presence of water; the second speaks of its effect.

For their flat character hints that these areas were held down at the

time when the other parts of the surface were being violently thrown

up. That they can themselves be cooled lava flows, their extent and

position seem enough to negative; to say nothing of the fact that they

should in that case lie above, not below, the general level. Something,

therefore, covered them during the moon’s eruptive youth and

disappeared later. Such superincumbence may well have been water, under

which the now great plains lay then as ocean bottoms. Deep-sea

soundings in our own oceans betray an ocean floor of the same extensive

sort, diversified as on the moon. To call the lunar _maria_ seas may

not be so complete a misnomer after all; but only a resurrecting in

epitaph what was the truth in its day.

Only doubtfully offered here for the Moon, for Mars the inference seems

more sure. Here again the dark regions not only look as they should had

they had an earlier history, but they, too, seem to lie below the level

of the surface round about. When they pass over the terminator they

invariably show as flattenings upon it, as if a slice of the surface

had been pared off. Such profile in such pass is what ground at a lower

level would present. Undoubtedly a part of the seeming depression is

due to relative absence of irradiation consequent upon a more sombre

tint, but loss of light hardly seems capable of the whole effect. In

the case of Mars, then, as with the Moon, a mistaken inference builded

better than it knew, if, indeed, we should rightly consider an

inference to be mistaken which on half data lands us at the right door.

From the aspects of the dark regions we are led, then, to regard Mars

as having passed through that stage of existence in which the earth

finds itself at the moment, the stage at which oceans and seas form a

feature of its landscape and an impediment to subjugation of its

surface in its entirety. What once were ocean beds have become ocean

bottoms devoid of that which originally filled them.

That the process of parting with a watery envelop is an inevitable

concomitant of the evolution of a planet from chaos to world, we do not

have to go so far afield as Mars and the Moon for testimony. Scrutiny

reveals as much in the history of our own globe. Two signposts of the

past, one geologic, the other paleontologic, point unmistakably in this

direction. The geologic guides us the more directly to the goal.

Study of the earth’s surface reveals the preponderating encroachment of

the land upon the sea since both began to be, and demonstrates that,

except for local losses, the oceans have been contracting in size from

archaic times. So much is evidenced by the successive places upon which

marine beds have been laid down. This suggests itself at once as a

theoretic probability to one considering the matter from a cosmic

standpoint, and it is therefore the more interesting and conclusive

that, from an entirely different departure-point, it should have been

one of the pet propositions of the late Professor Dana, who worked out

conclusively the problem for North America, and published charts

detailing the progressive making of that continent.

[Illustration: Map of North America at the close of Archæan time,

showing approximately the areas of dry land. (From Dana’s “Manual of

Geology.”)]

So telling is this reclaiming by nature of land from the sea that it

will be well to follow Dana a little into detail, as the details show

effectively the continuity of the process acting through æons of

geologic time. At the beginning of the Archæan age, or, in other words,

at the epoch when stratified beds were first laid down, the earth

reached a turning-point in its history. Erosion, superficial and

sub-aërial, then set in to help restrict the domain of the sea. At this

juncture North America consisted of a sickle of terrane inclosing

Hudson’s Bay and coming down at its apex to a point not much removed

from where Ottawa now stands, in about latitude 45°—a Labradorian

North America only. This, the kernel of the future continent, curiously

symbolized the form that continent was later to take. For its eastern

edge was roughly parallel to the present Atlantic coastline, although

much within and to the north of it, while its western one was similarly

aligned afar off to the now Pacific slope. Besides this continent

proper, the Appalachian, Rocky Mountain, Sierra Nevada, and Sierra

Madre chains stood out of the ocean in long, narrow ridges of detached

land, outlining in skeleton the bones of the continent that was to be.

The Black Hills of Dakota and other highlands made here and there

islets in the sea.

Much the same backbone-showing of continents yet to be filled out was

true of Europe, Asia, and South America. In Europe the northern

countries constituted all that could be called continental land. Most

of Norway, Sweden, Finland, Lapland, existed then, while the northern

half of Scotland, the outer Hebrides, portions of Ireland, England,

France, and Germany stood out as detached islands. From this, which is

a fair sample of the proportion of land then to land now over the other

continents so far as they are geologically known, we turn to consider

more in detail the history of North America.

By the time the Upper Silurian period came in, the Appalachian

highlands there had been greatly extended and joined to the Labradorian

mainland by continuous territory; otherwise, no important addition had

occurred, though islands emerged in Ohio, Kentucky, and Missouri.

[Illustration: North America at the opening of the Upper Silurian.

(From Dana’s “Manual of Geology.”)]

At the commencement of the Carbonic era what are now the Middle states

had begun to fill up from the north, and Newfoundland, from a small

island in the Upper Silurian, had become a great promontory of

Labrador, while the Eastern states region and Nova Scotia had risen

into being. The movements closing Paleozoic time upheaved from low

islands the Appalachian chain. The earth’s crust here crumpled by

contraction upon itself; and the movement ended, as Dana says, by

making dry land of the whole eastern half of the continent, along

substantially its present lines.

[Illustration: Map of North America after the Appalachian Revolution.

(From Dana’s “Manual of Geology.”)]

Mesozoic time was the period of the making of the West. It was an era

of deposition and coincident subsidence, when the western land had its

nose just above water at one moment to be submerged the next. Though on

the whole this part of the continent was emerging, the fact was that,

synchronously with the sinking of the sea, much of the land from time

to time sank too. The contraction which raised the Appalachian Mountains

at the beginning of the period and that of the Rockies at its close

overdid the necessities of the case and caused subsidence elsewhere.

The southeastern portion of the continent suffered most, the West on

the whole materially gaining. In the Triassic and Jurassic eras the

gain was pronounced; it occurred in the Cretaceous also, but with much

alternation of loss. Finally, at the close of the Cretaceous, the

continent, except for a prolonged Gulf of Mexico and vast internal

lakes, was substantially complete.

[Illustration: North America in the Cretaceous period. (From Dana’s

“Manual of Geology.”)]

The filling up of these lakes and the reclaiming of land from the Gulf

of Mexico constituted the land-making work of Tertiary times. The

extent of the lakes in the Eocene era is held to show that the general

level of the mountain plateau was low and rose later. So that the gain

by the land at this time was greater than the map allows to appear. By

the beginning of the Quaternary epoch the continents had assumed their

present general area, and since then their internal features have alone

suffered change.

[Illustration: Map of North America, showing the parts under water in

the Tertiary Era; the vertically lined is the Eocene. (From Dana’s

“Manual of Geology.”)]

A similar rising from the sea fell to the lot of Europe, though it has

not been detailed with so much care. The skeleton of that continent was

at the beginning of depositary time much what it is to-day, but a great

inland sea occupied the centre of it, which, as time went on, was

gradually silted in and evaporated away, notably during the Upper

Silurian period.

From all this it is pretty clear that, side by side with alternating

risings and sinkings of the land, there was a tolerably steady gain in

the contest by which dry ground dispossessed the sea. We may, of

course, credit this to a general deepening of the ocean bottoms due to

crumpling of the crust, but we may also impute it to a loss of water,

and that the latter is, at least for a part, in the explanation the

condition of the Moon and Mars makes probable.

Paleontology has the same story of reclamation to tell as geology, and

with as much certainty, though its evidence is circumstantial instead

of direct and speaks for the growing importance of the land in the

globe’s economy since the beginning of depositary time, and thus

inferentially to its increasing extent. Fossil remains of the plants

and creatures that have one after the other inhabited the earth show

that the land has been steadily rising both in floral and faunal

estimation as a habitat from the earliest ages to the present day. The

record lies imprinted in the strata consecutively laid down, and except

for gaps reads as directly on in bettering domicile as in evolutionary

development.

In Archæan times we find no undisputed evidence of life either vegetal

or animal. But beds of graphite and of limestone point to the possible

existence of both. Even anthracite has been found in Archæan rocks in

Norway and also in Rhode Island. Whether Dawson’s Eozoon Canadense be a

rhizopod or a crystal, doctors of science disagree. Dana, while

admitting nothing specific, deems it antecedently probable that algæ

and later microscopic fungi related to bacteria existed then, living in

water well up toward the boiling-point. Indeed, it is practically

certain that invertebrate life existed, because of its already

well-developed character in the next era. The like antedating is

inferable for the whole record of the rocks. Relatively their history

is undoubtedly fairly accurate, but absolutely it must be shifted

bodily backward into the next preceding era to correspond with fact not

yet unearthed.

In the Lower Cambrian, when first the existence of life becomes a

certainty, that life, so far as known, was wholly invertebrate and

wholly marine; rhizopods (probably), sponges and corals, echinoderms,

worms, brachiopods, mollusks, and crustaceans grew amid primitive

seaweed and have left their houses in the shape of shells while

perishing themselves. Their tracks too have thus survived. The

trilobites, crustaceans somewhat resembling our horseshoe crab, were

the lords of the Cambrian seas and marked the point to which organic

evolution had then attained. Their aquatic character as well as their

simple type is shown by their thoracic legs having each a natatory

appendage.

In the next era, the Lower Silurian, the fauna and flora were still

marine, although of a higher order than before, and in the Trenton

period, the upper part of the era, the earliest vertebrates, fishes,

come upon the scene: ganoids and possibly sharks. Nothing terrestrial

of this period has yet with certainty been unearthed in America. Europe

would seem to have either been more advanced then or better studied

since, for there the first plant higher than a seaweed has been dug up,

one of a fresh-water genus betokening the land; while in keeping with

this the first insect, an hemipter, also has been disinterred. Both the

geography and the life of the Eopaleozoic period Dana styles

“thalassic.”

Neopaleozoic time, beginning with the Upper Silurian, marked the

emergence of the continents, and following them the emergence of life

from the water on to this land. In the lower beds of the Upper Silurian

in America we find only the aquatic forms of previous strata, but in a

higher one we come in marshes upon plants related to the equiseta or

horsetails. In England land plants appear for the first time in these

latest Silurian beds and in the schists of Angers have been preserved

ferns. In both the old world and the new fossil fishes are found and

the oldest terrestrial species of scorpions. But the great bulk of

forms was still marine; corals, crinoids, brachiopods, trilobites

constituting the principal inhabitants. At this time the seas were

warm, having much the same temperature between 65° and 80° north as

between 30° and 45°; the prevalence of a general temperate tropicality

being shown by the fact that the common tropical chain corals lived in

latitude 82° north.

In the Devonian era, the Old Red Sandstone, fishes grew and multiplied,

increasing in size apparently through the era, and in the last period

of it reaching their culminating point. These pelagic vertebrates much

surpassed in structure the terrestrial population of the time, which

was of a low type and consisted of invertebrates such as myriapods,

spiders, scorpions, and insects; for the land was only making. In the

mid-Devonian, forests of a primitive kind covered such country as there

was, an amphibious land, composed of jungles and widespread marshes.

Tree ferns made the bulk of the vegetation, but among them grew also

cycads and yews. Mammoth may-flies flitted through the gloom of these

old forests, but no vertebrate as yet had left the sea.

Following upon the Old Red Sandstone were laid down the Carbonic

strata, and with the Carbonic entered upon the scene the advance scouts

of an army of progress evolutionarily impelled to spy out the land—the

first amphibians. They made their début in the Subcarboniferous section

of the era, the oldest of the three periods into which the Carbonic is

divided, crawling out of the sea to return again and leaving but

footprints at first on the sands of time. In the second period, the

Coal-measures proper, they ventured so far as to leave their skeletons

on terra firma, or rather infirma, while their tracks there show them

to have been now in great numbers. In this manner the ancestors of the

oldest land inhabitants began to struggle out of the sea. In the

Permian, the third and latest period of paleozoic times, we find their

descendants established in their new habitat, for in it we come upon

the first reptiles. Such possession marks a distinct step up in

function as in fact, for while amphibians visited dry land, reptiles

made it their home. The getting out of the water had now, in the case

of the more evolved forms, become an accomplished fact. The reptiles

were, indeed, the lowest and most generalized of their class,

Rhynchocephalians, “beak-headed” species that by their teeth proclaim

their marine origin and their relationship to the great amphibians that

still felt undecided where to stay. Meanwhile, in Europe dragon-flies,

two feet across, possessed the air; while amphibians there, as here,

ancestrally preceded reptiles in occupying the land.

Mesozoic times were, _par excellence_, the age of monsters; for the

Triassic (the New Red Sandstone), Jurassic and Cretaceous eras marked

the reign of the reptiles. Great dinosaurs sleep still in the Triassic

strata of the Atlantic border and in the Jurassic of the Western

states, to be unearthed from time to time and be given mausolea in our

museums. Gigantic they were and very literally possessed the earth. In

Europe they were substantially as in America during these mesozoic

eras, and showed their dominance by long survival in time as well as

world-wide distribution in space; for they lived all the way from

Kansas to New Zealand and from the Trias to the Upper Cretaceous. It is

supposed by Professor Osborn that many of them, like the herbivorous

brontosaurus, waded in marshes, not wholly unlike in habit to the

modern hippopotamus. Others were land-stalking carnivores, like the

megalosaurs of a little later date. Of enormous size, the largest

exceeded any animal which has ever lived, the whales alone excepted;

the biggest, the atlantosaurus and the brontosaurus, reaching a length

of sixty feet. For all their bulk they had scant brains, just enough to

enable them to feed and wallow, probably. It is interesting to note

that many of the reptiles, the less adventurous, apparently reverted to

the sea. For though the crocodilians existed already in the Trias, the

plesiosaurians did not come in till the Middle Trias in Europe, and the

sea-serpents (mosasaurus) till the Upper Cretaceous.

Though the dinosaurs dominated life in those days, higher forms, their

descendants, unnoticed were gradually creeping in, eventually to

supplant them. For brain was making its way unobtrusively in the

earliest of the mammals, diminutive creatures at first and of the

lowest type. First appearing in the Trias as something approaching the

missing link between reptiles and mammals, they later developed into

monotremes and marsupials, not rising in differentiation above the

latter order to the end of Mesozoic times. And this both in the old

world and the new. In the Jurassic, too, flying lizards and the first

birds appeared, showing their pedigree in their teeth.

With Cenozoic times we come upon the first true or placental mammals

with their culmination up to date in man. In the Eocene they were of a

primitive type; they were also of a comprehensive one, fitted to eat

anything. From this they specialized, some evolving and some on the

whole devolving; the whale, for instance, taking to the water in the

Eocene through the same degenerate proclivity that had characterized

the sea-saurians ages before. The earth was growing colder, though

still fairly warm, and with the fall in temperature the higher types of

life antithetically rose, evolution gradually fitting them to cope with

more advanced conditions. In this manner did the land supplant the sea

as the essential feature of the earth’s surface, first, in coming into

being, and then, by offering conditions fraught with greater

possibilities, as the habitat of the most advanced forms of life, both

plants and animals.

The possibility of advance in evolution was largely due to the fact

that the land did thus supplant the sea. Spontaneous variation, the as

yet unexplained _primum mobile_ in the genesis of species, is probably

to be referred to chemism and is likely later to receive its solution

at the hands of that science. In the meanwhile it is evident that

unless the variation obtain encouragement from the environment no

advance in type occurs. Now the land offers to an organism sufficiently

evolved to benefit by it, opportunities the sea does not possess. First

of these, undoubtedly, is the care it enables to be given to the young.

To cast one’s brood upon the waters is not the best method of insuring

its bringing up. There is too much of the uncertainties of wave and

current to make the process a healthy one, and even when attached to

rocks and seaweed, the attachment to a mother is to be preferred.

Without a period of infancy, when the young is unable to do for itself,

no great development is possible. In the only striking exception, the

case of the whales, dolphins, and porpoises, size has probably counted

for much in the matter, while the development of the cetaceans is far

behind that of the majority of land mammals.

Change of place, not in distance, but in variety, is another factor.

The sea is same as a habitat, one square mile of it being much like

another, except for gradually changing temperature. The land, on the

other hand, from its accidented surface, presents all manner of

diversity in the conditions. And the more varied the conditions to

which the organism is exposed, the greater its own complexity must be

to enable it to meet them.

That the terrestrial stage of planetary development is subsequent to

the terraqueous one, and must of necessity succeed it if the latter

ever exist on a body, follows from the loss of internal heat on the one

hand and from the kinetic theory of gases on the other. To which of the

two to attribute the lion’s share in the business is matter for doubt;

but that both must be concerned in it we may take for certain.

So long as the internal heat suffices to keep the body fluid, the

liquid itself sees to it that all interstices are filled. As the heat

dissipates, the body begins to solidify, starting with the crust. For

cosmic purposes it undoubtedly still remains plastic, but cracks of

relatively small size are both formed and persist. Into these the

surface water seeps. With continued refrigeration the crust thickens,

more cracks are opened and more water given lodgment within, to the

impoverishment of the seas. The process would continue till the

pressure of the crust itself rendered plastic all that lay below,

beyond which, of course, no fissures could be formed. How competent to

swallow all the seas such earth cuticle cracks may be we ignore; for we

cannot be said to know much of the process. We can only infer that to a

certain extent internal absorption of surface seas must mark a stage of

the evolution by which a star becomes a world and then an inert mass,

one of the dark bodies of which space is full.

Of the other means we know more. We are certain that it must take

place, though we are in doubt as to the amount it has already

accomplished. This method of depletion is by the departure of the water

in the form of gas, in consequence of the molecular motions. If we knew

the temperature and the age of Mars and also the amount of atmosphere

originally surrounding it, we could possibly predicate its state.

Reversely, we can infer something as to age and temperature from its

present condition.

Mars and Its Canals · 第 12 / 16 章