The Evolution of an Impact-generated Partially-vaporized Circumplanetary Disk

Details The Evolution of an Impact-generated Partially-vaporized Circumplanetary Disk The Evolution of an Impact-generated Partially-vaporized Circumplanetary Disk

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.1719m&link_type=abstract

35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.1719

Physics

Scientific paper

The impact-generated circumplanetary disk is a partially-vaporized one.
The disk evolution is controlled by the initial gas fraction: only in
the dust-rich disk, the moon formation occurs through the gravitational
instavility of the dust layer.

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