Mass Distribution and Planet Formation in the Solar Nebula

Details Mass Distribution and Planet Formation in the Solar Nebula Mass Distribution and Planet Formation in the Solar Nebula

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1004d&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Computer Science

Scientific paper

We recalculate the "minimum mass solar nebula" using the starting
locations of the giant planets from the "Nice" model, and compute a much
more massive disk. Among our findings: Uranus and Neptune formed in
<10 Myr and later switched orbits.

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