Towards Initial Mass Functions for Asteroids and Kuiper Belt Objects

Details Towards Initial Mass Functions for Asteroids and Kuiper Belt Objects Towards Initial Mass Functions for Asteroids and Kuiper Belt Objects

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1861c&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1861

Physics

Scientific paper

We present a scenario for primary accretion in turbulence of
20-200 km diameter inner and outer solar system primitive bodies
directly from freely-floating, but size-sorted, nebula particles, which
also helps explain the nearly Myr variance in formation age of
chondrules in a given chondrite.

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