Mar 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1712n&link_type=abstract
41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1712
Other
Scientific paper
Lunar basins have been characterized as circular craters > 300 km
with no central peak defined by tectonic and volcanic features. LRO/LOLA
observations allow re-examination and perhaps removal of some uncertain
pre-Nectarian basins, and addition of others.
Lemoine Frank G.
Mazarico Erwan M.
Neumann Gregory A.
Smith Douglas E.
Zuber Maria T.
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