Injection of 182Hf into the Early Solar Nebula

Details Injection of 182Hf into the Early Solar Nebula Injection of 182Hf into the Early Solar Nebula

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003lpi....34.2074m&link_type=abstract

34th Annual Lunar and Planetary Science Conference, March 17-21, 2003, League City, Texas, abstract no.2074

Computer Science

7

Scientific paper

If 41Ca is injected into the early solar nebula by a nearby supernova,
it is likely accompanied by enough 182Hf to explain the amount inferred
to have been present in the early solar system. In such a case, the
182Hf is not due to the r-process but rather to nucleosynthesis in
massive star shells.

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