Variations in the Abundance of Regolith Derived Micrometeorites with Time, Following the L-Chondrite Parent Body Disruption at 470 Ma

Details Variations in the Abundance of Regolith Derived Micrometeorites with Time, Following the L-Chondrite Parent Body Disruption at 470 Ma Variations in the Abundance of Regolith Derived Micrometeorites with Time, Following the L-Chondrite Parent Body Disruption at 470 Ma

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2004a&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2004

Physics

1

Scientific paper

Noble gas analyses of Chinese and Swedish mid-Ordovician fossil
micrometeorites show that the influx of regolith-derived material to
Earth, following the L-chondrite parent body disruption at 470 Ma,
decreases over time.

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