Compaction and Sticking of Planetesimals due to Porosity

Details Compaction and Sticking of Planetesimals due to Porosity Compaction and Sticking of Planetesimals due to Porosity

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.1008f&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

Physics

Scientific paper

It was estimated using numerical methods that numbers, sizes and masses
of planetesimals are ranging from 1016-1020 kg in the boundary of the
early inner solar system.

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