Physics
Scientific paper
Nov 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011georl..3821204g&link_type=abstract
Geophysical Research Letters, Volume 38, Issue 21, CiteID L21204
Physics
1
Planetary Sciences: Solid Surface Planets: Composition (1060, 3672), Planetary Sciences: Solid Surface Planets: Remote Sensing, Planetary Sciences: Solid Surface Planets: Surface Materials And Properties, Planetary Sciences: Solid Surface Planets: Volcanism (6063, 8148, 8450), Planetary Sciences: Solar System Objects: Moon (1221)
Scientific paper
The Mairan domes are four features located in northern Oceanus
Procellarum at ∼312.3E, 41.4N on the Moon. High resolution visible
imagery, visible-to-mid-IR spectra, and Lunar Prospector Th abundance
data all indicate that these four domes have a composition that is
consistent with derivation from a Si-rich, highly evolved magma.
Arnold Jessica A.
Giguere Thomas A.
Glotch Timothy D.
Hagerty Justin J.
Hawke Bernard Ray
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