In-Situ Evidence for Live Iron-60 in the Early Solar System: A Potential Heat Source for Planetary Differentiation from a Nearby Supernova Explosion

Details In-Situ Evidence for Live Iron-60 in the Early Solar System: A Potential Heat Source for Planetary Differentiation from a Nearby Supernova Explosion In-Situ Evidence for Live Iron-60 in the Early Solar System: A Potential Heat Source for Planetary Differentiation from a Nearby Supernova Explosion

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.1271m&link_type=abstract

35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.1271

Physics

7

Scientific paper

We report in-situ ^60Ni-excesses in two minerals in Bishunpur. The
inferred ^60Fe abundance is the highest measured in a meteorite. It
gives the first evidence for a supernova origin of ^60Fe, which served
as a heat source for planetary differentiation.

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