Lunar mare basalt volcanism - Early stages of secondary crustal formation and implications for petrogenic evolution and magma emplacement processes

Details Lunar mare basalt volcanism - Early stages of secondary crustal formation and implications for petrogenic evolution and magma emplacement processes Lunar mare basalt volcanism - Early stages of secondary crustal formation and implications for petrogenic evolution and magma emplacement processes

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..545h&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 545.

Computer Science

Lunar Rocks, Volcanology, Lunar Crust, Magma, Basalt, Petrogenesis, Stratigraphy, Clementine Spacecraft, Lunar Evolution

Scientific paper

Clementine multispectral imaging and complementary Apollo and Luna sample collections can be used to test models for the origin, ascent, and eruption of basaltic magmas, as well as to document the early stages of secondary crustal formation and evolution. Attention is here given to the emerging stratigraphy, estimates of the flux, the characteristics of surface deposits, implication of modes of emplacement, and emerging constraints on petrogenic models, for the generation and emplacement of secondary crustal magmas.

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