Possible conditions for formation of satellite from protoearth by ejection of material

Details Possible conditions for formation of satellite from protoearth by ejection of material Possible conditions for formation of satellite from protoearth by ejection of material

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984em%26p...31...15p&link_type=abstract

Earth, Moon, and Planets (ISSN 0167-9295), vol. 31, Aug. 1984, p. 15-24.

Computer Science

1

Lunar Evolution, Natural Satellites, Planetary Evolution, Protoplanets, Earth Mantle, Gas Temperature

Scientific paper

Conditions for the formation of a large gaseous protoearth and the formation of a satellite are considered. The energy required is assumed to come from the gravitational contraction to form the sun, the gravitational contraction to form the protoearth, core overturn and planetesimal impacts on the protoearth. The model is compatible with geochemical, tidal and angular momentum data.

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