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The thermal environment of the terrestrial planets /supplement 4/

K. Schocken

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Abstract

An atmosphere of Mercury of a light gas such as hydrogen would hardly seem possible.However, since a hydrogen atmosphere is cold, its dissipation o c c u r s slowly, and the l o s s of hydrogen can be compensated by the interception of s o l a r protons.The amount of water in Venus' atmosphere above i t s cloudThe uncerl a y e r is equivalent to a layer of liquid water 98 P deep.tainty amounts to -+ 5%.

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An atmosphere of Mercury of a light gas such as hydrogen would hardly seem possible.However, since a hydrogen atmosphere is cold, its dissipation o c c u r s slowly, and the l o s s of hydrogen can be compensated by the interception of s o l a r protons.The amount of water in Venus' atmosphere above i t s cloudThe uncerl a y e r is equivalent to a layer of liquid water 98 P deep.tainty amounts to -+ 5%.

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Available abstract

An atmosphere of Mercury of a light gas such as hydrogen would hardly seem possible.However, since a hydrogen atmosphere is cold, its dissipation o c c u r s slowly, and the l o s s of hydrogen can be compensated by the interception of s o l a r protons.The amount of water in Venus' atmosphere above i t s cloudThe uncerl a y e r is equivalent to a layer of liquid water 98 P deep.tainty amounts to -+ 5%.

Key concepts: Astrobiology, Planet, Terrestrial planet, Environmental science, Astronomy, Physics

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