Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008dps....40.1406t&link_type=abstract
American Astronomical Society, DPS meeting #40, #14.06; Bulletin of the American Astronomical Society, Vol. 40, p.408
Astronomy and Astrophysics
Astronomy
Scientific paper
We investigate the response of CO2-rich upper atmospheres of early Mars and Venus to the extreme solar EUV radiation from the young Sun by using a newly developed 1-D, multi-component, hydrodynamic thermosphere-ionosphere model (Tian et al. 2008a,b). It is shown that the weak gravity field of Mars, in combination with the strong solar EUV radiation from a young Sun, makes the thermal escape of atomic carbon and oxygen efficient. As a result, it would have been unlikely for the planet to have maintained a dense CO2 atmosphere during the early Noachian - prior to 4.1 billion years ago (Tian et al. 2008c). Without a dense CO2 atmosphere early Mars would have remained cold, until mid or late Noachian. In contrast, a CO2-rich atmosphere of early Venus was much more stable.
Table of Contents
References
Tian, F., J.F. Kasting, H. Liu, R.G. Roble, Hydrodynamic planetary thermosphere model:. 1. The response of the Earth's thermosphere to extreme solar EUV conditions and the significance of adiabatic cooling, J. Geophys. Res., 113, E05008 doi:10.1029/2007JE002946 (2008a)
Tian, F., S.C. Solomon, L. Qian, J. Lei, R.G. Roble, Hydrodynamic planetary thermosphere model: 2. coupling of an electron transport/energy deposition model, J. Geophys. Res., 113, E07005, doi:10.1029/2007JE003043 (2008b).
Tian, F., J.F. Kasting, S.C. Solomon, Fast thermal escape of carbon and oxygen from a dense, CO2-ruch early Martian atmosphere. Science (2008c), under review.
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