Mn-53-Cr-53 isotope systematics of the HED parent body

Details Mn-53-Cr-53 isotope systematics of the HED parent body Mn-53-Cr-53 isotope systematics of the HED parent body

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..851l&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 851.

Other

6

Manganese Isotopes, Chromium Isotopes, Mars Surface, Lunar Surface, Radiogenic Materials, Asteroid Belts, Rocks, Silicates

Scientific paper

An effort is made to learn more about the HED parent body (PB) and further constrain the extent of Mn-53 heterogeneity within the asteroid belt. By achieving these goals, it will be possible to determine whether the Mn-53-Cr-53 isotope system can be used as a chronometer for different asteroid belt materials by studying such other constituents of the HED PB as diogenites and both cumulate and several additional noncumulate eucrites.

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