The distribution of lunar geologic units in space and time and their mode of origin were considered since they provided significant data which bear on a number of current problems in lunar geophysics. Observations and problems were discussed which deal with the characterization of the upper 25 km of the lunar crust, the tectonic style of the crust, the formation of mascons within major basins, analysis of lunar magnetic anomalies, and the history of the lunar crust.
Some geologic observations concerning lunar geophysical models
1977-01-01
Aufsatz (Konferenz)
Keine Angabe
Englisch
Maximum polarization values of some lunar geologic units
NTRS | 1966
|Astrogeologic studies - Lunar geologic survey
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Lunar Geologic Mapping Program: 2008 Update
NTRS | 2008
|