Atmospheric Escape from Planetary Atmospheres

Details Atmospheric Escape from Planetary Atmospheres Atmospheric Escape from Planetary Atmospheres

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agufmsa53b1170t&link_type=abstract

American Geophysical Union, Fall Meeting 2005, abstract #SA53B-1170

Astronomy and Astrophysics

Astronomy

0325 Evolution Of The Atmosphere (1610, 8125), 5210 Planetary Atmospheres, Clouds, And Hazes (0343), 5215 Origin Of Life, 5225 Early Environment Of Earth, 5704 Atmospheres (0343, 1060)

Scientific paper

Atmospheric escape has been suggested as one important process on the following objects: 1. Extrasolar planets (hot Jupiters) 2. Early terrestrial-like planets (Earth, Venus, etc.) 3. Small solar system objects (Pluto, Enceladus, comets) Previous theoretical work and comparison with observationAL data will be summarized. New progress in the development of a multi-fluid hydrodynamic escape model will be reported. The importance and potential problems of in-depth studies of the atmospheric escape processes in Geosciences, Planetary Sciences, and Astronomy will be highlighted. A collaboration between geoscientists, planetary scientists, and astronomers will greatly improve our understanding on this complicated process and the evolutionary paths of the related objects.

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