Lunar Maria: Structure and Evolution

Details Lunar Maria: Structure and Evolution Lunar Maria: Structure and Evolution

Aug 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969sci...165..693v&link_type=abstract

Science, Volume 165, Issue 3894, pp. 693-695

Physics

12

Scientific paper

The lunar maria are considered to have evolved as homologous, transient,
gravity-wave systems from large impact craters on a crustal layer 50
kilometers thick, fluidized from beneath by prompt, shock-induced
melting inside an initially hot moon.

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