Blow-off of planetary protoatmospheres and of the protoplanetary nebula

Details Blow-off of planetary protoatmospheres and of the protoplanetary nebula Blow-off of planetary protoatmospheres and of the protoplanetary nebula

Sep 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pepi...29..252h&link_type=abstract

(NATO, Advanced Study Institute on Early Evolution of the Planets and their Atmospheres, Newcastle-upon-Tyne, England, Mar. 23-A

Physics

5

Mass Transfer, Planetary Atmospheres, Planetary Mass, Protoplanets, Atmospheric Heating, Far Ultraviolet Radiation, Solar Wind

Scientific paper

The mass loss from planetary protoatmospheres is in the order of 0.01-0.0001 of the planetary mass for the terrestrial planets and about 10 to the -7th/10 to the -8th for the giant planets. The minimum time intervals needed for the disappearance of the protoplanetary nebula are in the order of 10 to the 6th yr in the case of heating by a T-Tauri-like solar wind, 10 to the 8th yr for heating by far UV radiation from the sun and 10 to the 9th yr for heating by extreme UV radiation.

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