Microscale Distribution and Behavior of Th, REE, and K During Regolith Formation Processes on the Moon: Implications for Remote Sensing of the Surfaces of Airless Planetary Bodies

Details Microscale Distribution and Behavior of Th, REE, and K During Regolith Formation Processes on the Moon: Implications for Remote Sensing of the Surfaces of Airless Planetary Bodies Microscale Distribution and Behavior of Th, REE, and K During Regolith Formation Processes on the Moon: Implications for Remote Sensing of the Surfaces of Airless Planetary Bodies

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.2097b&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.2097

Physics

Scientific paper

Electron and ion microprobe analyses of Sm, Th, K and major elements in
lunar regolith glasses are used to examine the effect of impact melting
on primary crustal signatures to more accurately interpret planetary
data obtained through remote sensing.

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