Stratigraphic studies: Part A: basalt stratigraphy of southern Mare Serenitatis
By: K. A. Howard, M. H. Carr, and W.R. Muehlberger
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Abstract
Mare Serenitatis has long been noted for its conspicuous dark border (fig. 29-1). The Apollo 17 metric photographs traverse this border in southern Mare Serenitatis and show clearly superposition relationships among the mare and mare-related stratigraphic units. These photographs, together with full-Moon photographs, albedo measurements, and color information (table 29-I), provide the basis for a revised stratigraphic framework for these presumedly basaltic rocks (figs. 29-2 and 29-3). In contrast to most previous studies, we conclude that the darker units are older than lighter ones. Similar conclusions have been reached by Bryan and Adams (part C of sec. 30) and Boyce and Dial (part C of this section). The relatively light-colored central part of Mare Serenitatis is thought to represent the youngest basalt in the region; a very dark unit that includes the Apollo 17 landing site is one of the oldest.
| Publication type | Book chapter |
|---|---|
| Publication Subtype | Book Chapter |
| Title | Stratigraphic studies: Part A: basalt stratigraphy of southern 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 | 12 p. |
| Larger Work Type | Report |
| Larger Work Subtype | Federal Government Series |
| Larger Work Title | Apollo 17 preliminary science report (NASA SP-330) |
| First page | 29-1 |
| Last page | 29-12 |
| Other Geospatial | Moon |
| Google Analytic Metrics | Metrics page |