CHAPTER IV

THE POLAR CAPS

Almost as soon as magnification gives Mars a disk that disk shows

markings, white spots crowning a globe spread with blue-green patches

on an orange ground. The smallest telescope is capable of this far-off

revelation; while with increased power the picture grows steadily more

articulate and full. With a two and a quarter inch glass the writer saw

them thirty-five years ago.

After the assurance that markings exist the next thing to arrest

attention is that these markings move. The patches of color first made

out by the observer are shortly found by him to have shifted in place

upon the planet. And this not through mistake on his part but through

method in the phenomena; for all do it alike. In orderly rotation the

features make their appearance upon the body’s righthand limb (in the

telescopic image), travel across the central meridian of the disk and

vanish over its lefthand border. One follows another, each rising,

culminating and setting in its turn under the observer’s gaze. A

constantly progressing panorama passes majestically before his sight,

new objects replacing the old with a march so steady and withal so

swift that a few minutes will suffice to mark unmistakably the fact of

such procession. But for all this ceaseless turning under his gaze,

after a certain lapse of time it is evident that the same features are

being shown him over again. With such recognition of recurrence comes

the first advance toward acquaintance with the Martian world. For that

in all their journeying their configuration alters not, proves them

permanent in place, part and parcel of the solid surface of that other

globe. This surface, then, lies exposed to view and by its turning

shows itself subject, like our earth, to the vicissitudes of day and

night.

In such self-exposure Mars differs from all the four great planets,

Jupiter, Saturn, Uranus and Neptune. Features, indeed, are apparent on

the first two of these globes and dimly on the other two as well, but

they lack the stability of the Martian markings. They are forever

exchanging place. In the case of Jupiter what we see is undoubtedly a

cloud-envelop through which occasional glimpses may possibly be caught

of a chaotic nucleus below. With Saturn it is the same; and the

evidence is that the like is true of Uranus and Neptune. What goes on

under their great cloud canopies we can only surmise. With Mars,

however, we are not left to imagination in the matter but so far as our

means permit can actually observe what there takes place. Except for

distance, which, through science, year by year grows less, it is as if

we hovered above the planet in a balloon, with its various features

spread out to our gaze below.

Attention shows these areographic features to be on hand with punctual

precision for their traverse of the disk once every twenty-four hours

and thirty-seven minutes. For over two hundred years this has been the

case, their untiring revolutions having been watched so well that we

know the time they take to the nicety of a couple of hundredths of a

second. We thus become possessed of a knowledge of the length of the

Martian day and it is not a little interesting to find that it very

closely counterparts in duration our own, being only one thirty-fifth

the longer of the two. We also find from the course the markings pursue

the axis about which they turn; and just as the period of the rotation

tells us the length of the Martian day so the tilt of the axis, taken

in connection with the form of the orbit, determines the character of

the Martian seasons. Here again we confront a curious resemblance in

the circumstances of the two planets, for the tilt of the equator to

the plane of the orbit is with Mars almost precisely what it is for the

Earth. The more carefully the two are measured the closer the

similitude becomes. Sir William Herschel made the Martian 28°,

Schiaparelli reduced this to 25°, and later determination by the writer

puts it nearer 24°. The latter is the one now adopted in the British

Nautical Almanac for observers of the planet. This is a very close

parallelism indeed; so that in general character the Martian seasons

are nearly the counterpart of ours. In length, however, they differ;

first because the year of Mars is almost double the length of the

terrestrial one and secondly because from the greater ellipticity of

Mars’ orbit the seasons are more unequal than is the case with us, some

being run through with great haste, others being lingered on a

disproportionate time. It is usual on the Earth to consider spring as

the period from the vernal equinox, about March 21, to the summer

solstice, about June 20; summer as lasting thence to the autumnal

equinox; autumn from this latter date, about September 20, to the

winter solstice on December 21; and winter from that point on to the

next spring equinox again. On this division our seasons in the northern

hemisphere last respectively: spring, 91 days; summer, 92 days; autumn,

92 days; and winter, 90 days. On Mars these become, reckoned in our

days: spring, 199 days; summer 183 days; autumn, 147 days; and winter,

158 days. If we had counted them in Martian days they would have

totaled about one thirty-fifth less in number each.

In its days and seasons, then, Mars is wonderfully like the Earth;

except for the length of the year we should hardly know the difference

in reckoning of time could we some morning wake up there instead of

here. Only in one really unimportant respect should we feel strange; in

months we should find ourselves turned topsy-turvy. But lunations have

nothing to do with climate nor with the alternation between night and

day; and in these two important respects we should certainly feel at

home.

Though the axis could be determined by the daily march of any marking

and thus the planet’s tropic, temperate and polar regions marked out,

the process is made easier by the presence of white patches covering

the planet’s poles and known, in consequence, as the polar caps. It is

from measures of the patches that the position of the Martian poles has

actually been determined. These polar caps are exactly analogous in

general position to those which bonnet our own Earth. They reproduce

the appearance of the ice and snow of our arctic and antarctic regions

seen from space, in a very remarkable manner. In truth they are things

of note in more ways than one and would claim precedence on many

counts. Priority of recognition, however, alone entitles them to

premier consideration. Among the very first of the disk’s detail to be

made out by man, they justly demand description first.

With peculiar propriety the polar caps have thus the _pas_. Not only do

they stand first in order of visibility, but they prove to occupy a

like position logically when it comes to an explanation of the planet’s

present physical state. It is not matter of hazard that the most

evident of all the planet’s markings should also be the most

fundamental, the fountainhead from which everything else flows. It is

of the essence of the planet’s condition and furnishes the key to its

comprehension. The steps leading to this conclusion are as interesting

as they are cogent. They start at the polar caps’ visibility. For their

size first riveted man’s attention and then attention to them disclosed

that most vital of the characteristics of the planet’s surface: change.

Just as almost all of the features we note are permanent in place,

showing that they belong to the surface, so are they all impermanent in

character. Change is the only absolutely unchanging thing except

position about the features the planet presents to view. It was in the

aspect of the polar caps that this important fact first came to light.

Not only did they thus initially instance a general law, they have

turned out to make it; for by themselves changing they largely cause

change in all the rest. But for a long time they alone exemplified its

workings. To Sir William Herschel we owe the first study of their

change in aspect. This eminent observer noted that their varying size

was subject to a regular rhythmic wax and wane timed to the course of

the seasons of the planet’s year. The caps increased in the winter of

their hemisphere and decreased in its summer and being situate in

opposite hemispheres they did this alternately with pendulum-like

precision. His observations were soon abundantly confirmed, for the

phenomena take place upon a vast scale and are thus easy of

recognition. At their maximum spread the caps cover more than one

hundred times as much ground as when they have shrunk to their minimum.

In the depth of winter they stretch over much more than the polar zone,

coming down to 60° and even 50° of latitude north or south as the case

may be, thence melting till by midsummer they span only five or six

degrees across.

In this they bear close analogue to the behavior of our own. Ours would

show not otherwise were they viewed from the impersonal standpoint of

space. Very little telescopic aid suffices to disclose the Martian

polar phenomena in this their more salient characteristics and convince

an observer of their likeness to those of the earth. Any one may note

what is there going on by successive observations of the planet with a

three-inch glass. Nor is the change by any means slow. A few days at

the proper Martian season, or at most a couple of weeks, produces

conspicuous and conclusive alterations in the size of these nightcaps

of the planet’s winter sleep. Resembling our own so well they were

early surmised to be of like constitution and composed, therefore, of

ice and snow. Plausible on its face, this view of them was generally

adopted and common sense has held to it ever since. It has encountered,

of course, opposition, partly from very proper conservatism, but

chiefly from that earth-centred philosophy which has doubted most

advances since Galileo’s time, and carbonic acid has been put forward

by this school of sceptics to take its place. We shall critically

examine both objections; the latter first, because a certain physical

fact enables us to dispose of it at once. In casual appearance there is

not much to choose between the rival candidates of common sense and

uncommon subtlety, water and frozen carbonic acid gas, both being

suitably white and both going and coming with the temperature. But,

upon closer study, in one point of behavior the two substances act

quite unlike, and had half the ingenuity been expended in testing the

theory as in broaching it this fact had come to light to the suggestors

as it did upon examination to the writer and had served as a touchstone

in the case. At pressures of anything like one atmosphere or less

carbonic acid passes at once from the solid to the gaseous state.

Water, on the other hand, lingers in the intermediate stage of a

liquid. Now, as the Martian cap melts it shows surrounded by a deep

blue band which accompanies it in its retreat, shrinking to keep pace

with the shrinkage in the cap. This is clearly the product of the

disintegration since it waits so studiously upon it. The substance

composing the cap, then, does not pass instantaneously or anything like

it from the solid to the gaseous condition.

This badge of blue ribbon about the melting cap, therefore,

conclusively shows that carbonic acid is not what we see and leaves us

with the only alternative we know of: water.

Mars and Its Canals · 第 4 / 16 章