A Deep Lunar Magma Ocean Based on Neodymium, Strontium and Hafnium Isotope Mass Balance

Details A Deep Lunar Magma Ocean Based on Neodymium, Strontium and Hafnium Isotope Mass Balance A Deep Lunar Magma Ocean Based on Neodymium, Strontium and Hafnium Isotope Mass Balance

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.1802r&link_type=abstract

35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.1802

Computer Science

1

Scientific paper

Combined Lu-Hf, Sm-Nd, and Rb-Sr isotopic mass balance supports a large
depleted lunar mantle to complement an enriched crust. The easiest way
for the mantle to become depleted is through crystallization of a deep
magma ocean composed of over 85% of the Moon.

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