Evidence of at Least Two Extra-Selenial Components Accreting on the Moon - In Search for the Oxygen Isotopic Composition of the Solar Component Trapped in Lunar Metallic Grains

Details Evidence of at Least Two Extra-Selenial Components Accreting on the Moon - In Search for the Oxygen Isotopic Composition of the Solar Component Trapped in Lunar Metallic Grains Evidence of at Least Two Extra-Selenial Components Accreting on the Moon - In Search for the Oxygen Isotopic Composition of the Solar Component Trapped in Lunar Metallic Grains

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1531h&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Computer Science

1

Scientific paper

We performed isotope measurements of O residing at the surface of lunar
metallic grains, to untangle the contradictory situation on the solar
wind component. We were able to reproduce both 16O-enriched
and -depleted components previously reported.

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