Origin of the Nearside/Farside Dichotomy

Details Origin of the Nearside/Farside Dichotomy Origin of the Nearside/Farside Dichotomy

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpico1415.2118s&link_type=abstract

NLSI Lunar Science Conference, held July 20-23, 2008 at NASA Ames Research Center, Moffett Field, California, LPI Contribution N

Physics

Scientific paper

The distribution of the nearside lunar maria of Oceanus Procellarum,
geochemical anomalies, and tectonic patterns are attributed to the
formation of the South-Pole-Aitken Basin on the lunar farside.

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