Lunar Mare Volcanism Based on Chemical Composition of Titanium, Iron, Calcium and Magnesium as Observed by Lunar Prospector Gamma-Ray Spectrometer

Details Lunar Mare Volcanism Based on Chemical Composition of Titanium, Iron, Calcium and Magnesium as Observed by Lunar Prospector Gamma-Ray Spectrometer Lunar Mare Volcanism Based on Chemical Composition of Titanium, Iron, Calcium and Magnesium as Observed by Lunar Prospector Gamma-Ray Spectrometer

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1604y&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1604

Computer Science

Scientific paper

By using the data from Lunar Prospector gamma-ray spectrometer, good
correlations of TiO2 with FeO, CaO and MgO in five mare regions were
found to exist, suggesting that the age and period are closely related
to the composition.

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