Simulations of Terrestrial Planet Formation with Strong Dynamical Friction: Implications for the Origin of the Earth's Water

Details Simulations of Terrestrial Planet Formation with Strong Dynamical Friction: Implications for the Origin of the Earth's Water Simulations of Terrestrial Planet Formation with Strong Dynamical Friction: Implications for the Origin of the Earth's Water

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.2347o&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.2347

Physics

Scientific paper

With numerical simulations of terrestrial planet accretion for different
outer planet configurations, we find that an initially circular and
co-planar Jupiter and Saturn are most consistent with the abundance of
water on Earth.

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