Statistical Model of Earth-Moon Coaccretion and Macroimpacts

Details Statistical Model of Earth-Moon Coaccretion and Macroimpacts Statistical Model of Earth-Moon Coaccretion and Macroimpacts

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996lpi....27.1009p&link_type=abstract

Lunar and Planetary Science, volume 27, page 1009

Astronomy and Astrophysics

Astrophysics

Coaccretion, Collisions: Catastrophic, Earth'S Mantle, Earth: Core, Impacts

Scientific paper

The model of Earth-Moon coaccretion is developed in the framework of standard scenario of Origin of the Solar System. We take into account the evolution of population of large bodies which disappear in mutual catastrophic collisions (macroimpacts) during the planetary accretion Our model takes properly into account the additional feeding of presatellite swarm by the material ejected from outer shell of growing planet due to macroimpacts of falling bodies. This model includes five chemical reservoirs, that are circumsolar and circumplanetary disks and primitive core, mantle and permanently originating and destroying crust of the Earth.

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