Remote sensing and photogrammetric studies: Part A: remote sensing of Mare Serenitatis
By: T.W. Thompson, K.A. Howard, R.W. Shorthill, G.L. Tyler, S.H. Zisk, E. A. Whitaker, G. G. Schaber, and H. J. Moore
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Abstract
Mare Serenitatis is a circular mare approximately 600 km in diameter in the northeast quadrant of the lunar near side. It occupies an old multi-ringed basin (refs. 33-1 and 33-2) and is the site of a prominent mascon (ref. 33-3). A conspicuous dark annulus in this mare prompted subdivision of the mare materials into different stratigraphic units (refs. 33-2 and 33-4). A revised stratigraphic sequence for the southern part of Mare Serenitatis, based on photogeologic interpretation of Apollo 15 and 17 photographs, is summarized as follows after Howard et al.
| Publication type | Book chapter |
|---|---|
| Publication Subtype | Book Chapter |
| Title | Remote sensing and photogrammetric studies: Part A: remote sensing of Mare Serenitatis |
| Series number | 330 |
| Year Published | 1973 |
| Language | English |
| Publisher | National Aeronautics and Space Administration |
| Publisher location | Washington, D.C. |
| Contributing office(s) | Astrogeology Science Center |
| Description | 8 p. |
| Larger Work Type | Report |
| Larger Work Subtype | Federal Government Series |
| Larger Work Title | Apollo 17 preliminary science report (NASA SP-330) |
| First page | 33-3 |
| Last page | 33-10 |
| Other Geospatial | Moon |
| Google Analytic Metrics | Metrics page |