The Dynamics and Ages of Refractory Objects in the Solar Nebula

Details The Dynamics and Ages of Refractory Objects in the Solar Nebula The Dynamics and Ages of Refractory Objects in the Solar Nebula

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1081c&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1081

Physics

Scientific paper

The evolution of the solar nebula favors the survival of refractory
objects formed during t < 50,000 years of solar system formation over
those formed at later times. This explains the brief formation interval
of CAIs inferred from 26Al studies.

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