Observations of Mare Humboldtianum: Topography, Ages and Multispectral Characteristics

Details Observations of Mare Humboldtianum: Topography, Ages and Multispectral Characteristics Observations of Mare Humboldtianum: Topography, Ages and Multispectral Characteristics

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996lpi....27..547h&link_type=abstract

Lunar and Planetary Science, volume 27, page 547

Physics

Basalt, Digital Terrain Model, Geology, Spectroscopy, Titanium Content

Scientific paper

Mare Humboldtianum, a 650 km wide multi-ring impact basin on the northeastern part of the nearside of the Moon (59 degrees N, 82 degrees E) is hardly visible from Earth. This Nectarian-aged basin has been observed by the Galileo spacecraft in 1992 and the Clementine spacecraft in 1994. We combined multispectral imaging data with stereo data in order to study the basin structure and the basalt extrusions in this lunar area. Additionally we performed crater counts to date the surface age of the lava deposits.

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