High Abundances of Presolar Silicates in Antarctic Micrometeorites; Implications for Their Cometary Origins

Details High Abundances of Presolar Silicates in Antarctic Micrometeorites; Implications for Their Cometary Origins High Abundances of Presolar Silicates in Antarctic Micrometeorites; Implications for Their Cometary Origins

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1470y&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1470

Computer Science

4

Scientific paper

The abundance of presolar silicates in Antarctic micrometeorites (AMMs)
has been revised to be 50 ppm. That in one of the AMMs is 900 ppm,
comparable to that in primitive interplanetary dust particles,
indicating that it might be of cometary origin.

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