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The kinetic theory of planetary atmospheres
Author(s) -
George Hartley Bryan
Publication year - 1900
Publication title -
proceedings of the royal society of london
Language(s) - English
Resource type - Journals
eISSN - 2053-9126
pISSN - 0370-1662
DOI - 10.1098/rspl.1899.0111
Subject(s) - planet , atmosphere (unit) , mars exploration program , astrobiology , kinetic energy , physics , kinetic theory , astrophysics , theoretical physics , thermodynamics , classical mechanics
The application of the kinetic theory to the atmospheres of planets dates from the paper of Waterston, who gave an investigation based on the then only possible assumption of equal velocities for all molecules, an assumption since known as Clausius’ law. Of later papers reference is due in especial to Dr. Johnstone Stoney’s memoir “Of Atmospheres on Planets and Satellites,”* in which the test of permanence of a gas in the atmosphere of a planet is made to depend on the ratio of its velocity of mean square to that relative velocity which would enable a suitably projected body to escape from the planet’s attraction. If it be admitted, as Dr. Stoney assumes, that helium cannot exist in our atmosphere, it follows that vapour of water cannot exist on Mars.

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