Accretion and Core Formation Models Based on Extinct Radionuclides

Details Accretion and Core Formation Models Based on Extinct Radionuclides Accretion and Core Formation Models Based on Extinct Radionuclides

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999lpi....30.1978j&link_type=abstract

30th Annual Lunar and Planetary Science Conference, March 15-29, 1999, Houston, TX, abstract no. 1978

Physics

3

Scientific paper

Tungsten isotope data show that the Moon must have formed at ~25 Ma
assuming a giant impact origin. At least 20% of the Earth must have
accreted subsequent to the formation of the Moon to effectively erase
the eW anomaly in the silicate Earth.

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