Thermal escape of carbon from the early Martian atmosphere
Article first published online: 31 JAN 2009
Copyright 2009 by the American Geophysical Union.
Geophysical Research Letters
Volume 36, Issue 2, January 2009
How to Cite
2009), Thermal escape of carbon from the early Martian atmosphere, Geophys. Res. Lett., 36, L02205, doi:10.1029/2008GL036513., , and (
- Issue published online: 31 JAN 2009
- Article first published online: 31 JAN 2009
- Manuscript Accepted: 31 DEC 2008
- Manuscript Revised: 10 DEC 2008
- Manuscript Received: 29 OCT 2008
- energetics and dynamics
 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 the early Noachian, 4.1 billion years ago (Ga), that a CO2-dominated Martian atmosphere could not have been maintained, and Mars should have begun its life cold. By the mid to late Noachian, however, the solar EUV flux would have become weak enough to allow a dense CO2 atmosphere to accumulate. Hence, a sustainable warm and wet period only appeared several hundred million years (Myrs) after Mars formed.