The origins and early histories of planetary atmospheres.
Abstract
Ancient dry river beds detected on Mars by the Viking spacecraft suggest that the early Martian atmosphere may have been much more massive than at present. Degassing of a late-accreting, volatile-rich veneer may account for the primitive atmosphere of both Mars and earth. The primitive earth atmosphere could have produced a greenhouse effect sufficient to maintain temperatures above 273 K without NH3 and with low solar luminosity. The Venutian veneer, according to preliminary Pioneer results, was probably richer in noble gases relative to carbon and nitrogen than were the Martian and earth veneers. The highly evolved atmosphere of Titan, the large satellite of Saturn, is also discussed.
- Publication:
-
Evolution of Planetary Atmospheres and Climatology of the Earth
- Pub Date:
- 1979
- Bibcode:
- 1979epac.conf....1O
- Keywords:
-
- Atmospheric Temperature;
- Degassing;
- Planetary Atmospheres;
- Planetary Evolution;
- Abundance;
- Earth Atmosphere;
- Mars Atmosphere;
- Saturn Atmosphere;
- Titan;
- Viking Mars Program;
- Lunar and Planetary Exploration;
- Planetary Atmospheres