Thermal escape of carbon from the early Martian atmosphere
Observations suggest that Mars was wet and warm during the late Noachian, which probably requires a dense CO2 atmosphere. But would a dense CO2 early Martian atmosphere have been stable under the strong EUV flux from the young Sun? Here we show that thermal escape of carbon was so efficient during t...
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Veröffentlicht in: | Geophysical research letters 2009-01, Vol.36 (2), p.L02205-n/a |
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Format: | Artikel |
Sprache: | eng |
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