The scarcity of mappable flow lobes on the lunar maria - Unique morphology of the Imbrium flows

Details The scarcity of mappable flow lobes on the lunar maria - Unique morphology of the Imbrium flows The scarcity of mappable flow lobes on the lunar maria - Unique morphology of the Imbrium flows

Apr 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976lpsc....7.2783s&link_type=abstract

In: Lunar Science Conference, 7th, Houston, Tex., March 15-19, 1976, Proceedings. Volume 3. (A77-34651 15-91) New York, Pergamon

Other

13

Lava, Lunar Maria, Selenology, Volcanology, Basalt, Flow Characteristics, Lunar Photographs, Photogeology

Scientific paper

Unique features of Imbrium lava flows are their thickness (10-30 + m) and lengths (up to 400 km for phase-III, and up to 600 km for phase-II) when compared along later Imbrium and Eratosthenian units. They are distinct by virtue of their inferred short-lived (on the order of days) and extremely rapid rates of effusion. It is shown that there are numerous other basalt eruptives within the young blue western maria. The emplacement of these flows was by complex multilayering and intertonguing of individual flow units with thicknesses less than 10 m. They are generally restricted to the near vicinity of multiple vent sources.

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