Mare Australe: New Results from Lunar Orbiter and Clementine UV/VIS Imagery

Details Mare Australe: New Results from Lunar Orbiter and Clementine UV/VIS Imagery Mare Australe: New Results from Lunar Orbiter and Clementine UV/VIS Imagery

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996lpi....27..545h&link_type=abstract

Lunar and Planetary Science, volume 27, page 545

Physics

Geophysics

1

Age, Geology, Geophysics, Lava Ponds, Morphology

Scientific paper

Mare Australe is an old lunar impact basin which is visible in its entire shape only in spacecraft images but not from Earth. We used Lunar Orbiter IV images as well as Clementine UV/VIS images acquired in 1994 in order to study basalt ponds of the Mare Australe basin. We performed crater counts, measured the size of the basalt ponds and the nearest neighbor distance and compared our results for Mare Australe to previously published results for the Mare Orientale region and the South Pole-Aitken basin.

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