Hafnium and Neodymium Isotopic Constraints on Shergottite Formation

Details Hafnium and Neodymium Isotopic Constraints on Shergottite Formation Hafnium and Neodymium Isotopic Constraints on Shergottite Formation

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1933b&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1933

Computer Science

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Scientific paper

Shergottite Hf-Nd isotope systematics are decoupled implying that their
petrogenesis is unique compared to Earth and Moon analogs. Differences
can be explained by open system behavior, fractionation of an unknown
trace phase or ultra deep melting.

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