Other Worlds eBook

This eBook from the Gutenberg Project consists of approximately 180 pages of information about Other Worlds.

Other Worlds eBook

This eBook from the Gutenberg Project consists of approximately 180 pages of information about Other Worlds.

The subject of the atmosphere of Mars can not be dismissed without further consideration than we have yet given it, because those who think the planet uninhabitable base their opinion largely upon the assumed absence of sufficient air to support life.  It was long ago recognized that, other things being equal, a planet of small mass must possess a less dense atmosphere than one of large mass.  Assuming that each planet originally drew from a common stock, and that the amount and density of its atmosphere is measured by its force of gravity, it can be shown that Mars should have an atmosphere less than one fifth as dense as the earth’s.

Dr. Johnstone Stoney has attacked the problem of planetary atmospheres in another way.  Knowing the force of gravity on a planet, it is easy to calculate the velocity with which a body, or a particle, would have to start radially from the planet in order to escape from its gravitational control.  For the earth this critical velocity is about seven miles per second; for Mars about three miles per second.  Estimating the velocity of the molecules of the various atmospheric gases, according to the kinetic theory, Dr. Stoney finds that some of the smaller planets, and the moon, are gravitationally incapable of retaining all of these gases in the form of an atmosphere.  Among the atmospheric constituents that, according to this view, Mars would be unable permanently to retain is water vapor.  Indeed, he supposes that even the earth is slowly losing its water by evaporation into space, and on Mars, owing to the slight force of gravity there, this process would go on much more rapidly, so that, in this way, we have a means of accounting for the apparent drying up of that planet, while we may be led to anticipate that at some time in the remote future the earth also will begin to suffer from lack of water, and that eventually the chasms of the sea will yawn empty and desolate under a cloudless sky.

But it is not certain that the original supply of atmospheric elements was in every case proportional to the respective force of gravity of a planet.  The fact that Venus appears to have an atmosphere more extensive and denser than the earth’s, although its force of gravity is a little less than that of our globe, indicates at once a variation as between these two planets in the amount of atmospheric material at their disposal.  This may be a detail depending upon differences in the mode, or in the stage, of their evolution.  Thus, after all, Dr. Stoney’s theory may be substantially correct and yet Mars may retain sufficient water to form clouds, to be precipitated in snow, and to fill its canals after each annual melting of the polar caps, because the original supply was abundant, and its escape is a gradual process, only to be completed by age-long steps.

Even though the evidence of the spectroscope, as far as it goes, seems to lend support to the theory that there is no water vapor in the atmosphere of Mars, we can not disregard the visual evidence that, nevertheless, water vapor exists there.

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Other Worlds from Project Gutenberg. Public domain.