A Gas-poor Planetesimal Feeding Model for the Formation of Giant Planet Satellite Systems: Consequences for the Atmosphere of Titan

Details A Gas-poor Planetesimal Feeding Model for the Formation of Giant Planet Satellite Systems: Consequences for the Atmosphere of Titan A Gas-poor Planetesimal Feeding Model for the Formation of Giant Planet Satellite Systems: Consequences for the Atmosphere of Titan

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.2053e&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.2053

Physics

Scientific paper

We develop a gas-poor planetesimal collisional capture which may be
consistent with the mass and angular momentum of the Galilean satellites
and Titan. We investigate this model's implications for the origin of
Titan's atmosphere.

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