Accretion of Solid Particles by Gravitating Planetesimals in the Solar Nebulaand Jovian Subnebula: Implications for Depletion of the Terrestrial Planetsand Galilean Satellites in Volatiles

Details Accretion of Solid Particles by Gravitating Planetesimals in the Solar Nebulaand Jovian Subnebula: Implications for Depletion of the Terrestrial Planetsand Galilean Satellites in Volatiles Accretion of Solid Particles by Gravitating Planetesimals in the Solar Nebulaand Jovian Subnebula: Implications for Depletion of the Terrestrial Planetsand Galilean Satellites in Volatiles

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1888m&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1888

Physics

Scientific paper

Accretion of solid particles by planetesimals in the gas-rich nebula and
subnebula is estimated as a function of particle size. It is shown that
this process can yield depletion of the terrestrial planets (but hardly
the Galilean satellites) in moderately and highly volatile elements.

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