The Timing of Core Formation in Protoplanets Revisited: New Evidence from a Combined Tungsten — Noble Gas Isotope Study on Magmatic Iron Meteorites

Details The Timing of Core Formation in Protoplanets Revisited: New Evidence from a Combined Tungsten — Noble Gas Isotope Study on Magmatic Iron Meteorites The Timing of Core Formation in Protoplanets Revisited: New Evidence from a Combined Tungsten — Noble Gas Isotope Study on Magmatic Iron Meteorites

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1712k&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1712

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Scientific paper

Using noble gases we identified iron meteorite specimens whose W isotope
budgets likely remained unaltered by cosmic rays. The Hf-W systematics
of these samples indicate that their parent bodies segregated their
cores within 0.5 Ma of each other.

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