Collisions, Gas Flow, and the Formation of Planetesimals

Details Collisions, Gas Flow, and the Formation of Planetesimals Collisions, Gas Flow, and the Formation of Planetesimals

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.1274w&link_type=abstract

35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.1274

Physics

Scientific paper

In experiments and calculations we find that net growth of a body in a
binary collision at ‘high speed’ (several tens of m/s) is
possible if the colliding bodies both consist of dust and gas flow (in
protoplanetary disks) is taken into account.

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