Different Initial Conditions for Planet Formation Around Cool and Sun-like Stars: Disk Mass, Disk Structure, Dust Composition, and Organics Inventory

Details Different Initial Conditions for Planet Formation Around Cool and Sun-like Stars: Disk Mass, Disk Structure, Dust Composition, and Organics Inventory Different Initial Conditions for Planet Formation Around Cool and Sun-like Stars: Disk Mass, Disk Structure, Dust Composition, and Organics Inventory

Apr 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpico1538.5396a&link_type=abstract

Astrobiology Science Conference 2010: Evolution and Life: Surviving Catastrophes and Extremes on Earth and Beyond, held April 2

Biology

Scientific paper

We show that the initial conditions of planet formation differ around
cool stars and sun-like stars. We discuss how the observed differences
are expected to influence planet formation and the habitability of the
emerging planet population.

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