Giant Planet Formation by Disk Instability

Details Giant Planet Formation by Disk Instability Giant Planet Formation by Disk Instability

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999lpi....30.1049b&link_type=abstract

30th Annual Lunar and Planetary Science Conference, March 15-29, 1999, Houston, TX, abstract no. 1049

Physics

Scientific paper

3D hydro models suggest that a protoplanetary disk with a mass of about
0.1 solar masses could quickly lead to the formation of two giant
gaseous protoplanets, one at 6 AU and one at 12 AU.

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