Evolution of the Proto-Lunar Disk: Instability of the Dust Layer and the Moon Forming Material

Details Evolution of the Proto-Lunar Disk: Instability of the Dust Layer and the Moon Forming Material Evolution of the Proto-Lunar Disk: Instability of the Dust Layer and the Moon Forming Material

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1690m&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1690

Physics

Scientific paper

There are two possible modes of gravitational instability in the
proto-lunar disk: the instability of the dust-gas mixture and that of
the dust layer. We examine the preferred mode of instability and the
state of the Moon-forming materials.

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