Lunar Apennine-Hadley region: Geological implications of earth-based radar and infrared measurements
Recently completed high-resolution radar maps of the moon contain information on the decimeter-scale structure of the surface. When this information is combined with eclipse thermal-enhancement data and with high-resolution Lunar Orbiter photography, the surface morphology is revealed in some detail. A geological history for certain features and subareas can be developed, which provides one possible framework for the interpretation of the findings from the Apollo 15 landing. Frequency of decimeter- and meter-size blocks in and around lunar craters, given by the remote-sensed data, supports a multilayer structure in the Palus Putredinis mare region, as well as a great age for the bordering Apennins Mountains scarp.
Citation Information
Publication Year | 1971 |
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Title | Lunar Apennine-Hadley region: Geological implications of earth-based radar and infrared measurements |
Authors | S.H. Zisk, M. H. Carr, H. Masursky, R.W. Shorthill, T.W. Thompson |
Publication Type | Article |
Publication Subtype | Journal Article |
Series Title | Science |
Index ID | 70010321 |
Record Source | USGS Publications Warehouse |