Publications
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Photogeology: Part S: mare ridges and arches in southern Oceanus Procellarum Photogeology: Part S: mare ridges and arches in southern Oceanus Procellarum
Low-relief mare features such as ridges and arches are best studied by using stereoscopic photographs taken at low Sun angles. Apollo 16 metric camera photography of the southern Oceanus Procellarum east of Letronne Crater reveals a diversity of subtle features (fig. 29-125) and adds significantly to an understanding of the forms of mare ridges and arches their relative ages, and their...
Authors
George W. Colton, Keith A. Howard, Henry J. Moore
Photogrammetry and altimetry: Part C: frequency distributions of lunar slopes Photogrammetry and altimetry: Part C: frequency distributions of lunar slopes
The metric and panoramic cameras aboard the Apollo 16 spacecraft provided photographs on which photogrammetric techniques may be used to obtain precise measurements of horizontal distances and elevations. These measurements of horizontal distances and elevations. These measurements may in turn be used to obtain slope-frequency distributions of lunar surfaces at various slope lengths and...
Authors
Sherman S.C. Wu, H. J. Moore
Orbital-science investigation: Part H: sketch map of the region around the candidate Littrow Apollo landing sites Orbital-science investigation: Part H: sketch map of the region around the candidate Littrow Apollo landing sites
The photograph in figure 25-59 and the corresponding map (fig. 25-60) show the geology of part of the lunar surface just east of the Littrow rilles at the eastern edge of Mare Serenitatis. The most striking feature of the region is the extremely low albedo of the area mapped as Eld in the western half of the map. The low albedo is believed to be caused by a thin layer of pyroclastic...
Authors
M. H. Carr
The Apollo 17 landing site The Apollo 17 landing site
Dr Lucchitta describes the geology of the Apollo 17 landing site in the Taurus-Littrow region of the Moon.
Authors
Baerbel K. Lucchitta
Photogeology: Part F: reinterpretations of the northern Nectaris Basin Photogeology: Part F: reinterpretations of the northern Nectaris Basin
Geologic units of the Nectaris Basin rim have been interpreted as partly impact and partly volcanic in origin (refs. 29-4, 29-21, 29-35, 29-38, and 29-39). An exclusively volcanic origin was proposed for the material in the vicinity of the Apollo 16 landing site, slightly northwest of the Nectaris Basin (ref. 29-36). In view of the dominance of breccia and the paucity of volcanic...
Authors
Don E. Wilhelms
Photogeology: Part L: crater morphometry Photogeology: Part L: crater morphometry
Morphometric analysis of lunar craters (ref. 29-75) complements the more traditional photointerpretive study of crater morphology. These two indirect approaches to the scientific investigation of lunar craters continue to be productive because the preferred alternative method, direct field examination of specific large craters, is not being undertaken in the current series of manned...
Authors
Richard J. Pike
Preliminary geologic investigation of the Apollo 16 landing site Preliminary geologic investigation of the Apollo 16 landing site
The Apollo 16 landing site in the lunar central highlands encompassed terra plains and adjacent mountainous areas of hilly and furrowed terra. These morphologic units, representing important terrane types in the lunar highlands, had been interpreted as volcanic on most premission geologic maps. However, it became apparent during the mission that there are indeed few or no volcanic rocks...
Authors
W.R. Muehlberger, R. M. Batson, E. L. Boudette, C.M. Duke, R. E. Eggleton, D. P. Elston, A. W. England, V. L. Freeman, M. H. Hait, T.A. Hall, J.W. Head, C. A. Hodges, H. E. Holt, E.D. Jackson, J.A. Jordan, K.B. Larson, D.J. Milton, V. S. Reed, J. J. Rennilson, G. G. Schaber, J.P. Schafer, L. T. Silver, D. Stuart-Alexander, R. L. Sutton, G.A. Swann, R.L. Tyner, G. E. Ulrich, H. G. Wilshire, E.W. Wolfe, J.W. Young
Orbital-science investigation: Part K: geologic sketch map of the candidate Proclus Apollo landing site Orbital-science investigation: Part K: geologic sketch map of the candidate Proclus Apollo landing site
A panoramic camera frame (fig. 25-69) was used as the base for a geologic sketch map (fig. 25-70) of an area near Proclus Crater. The map was prepared to investigate the usefulness of the Apollo 15 panoramic camera photography in large-scale geologic mapping and to assess the geologic value of this area as a potential Apollo landing site. The area is being considered as a landing site...
Authors
Baerbel K. Lucchitta
Orbital-science investigation: Part L: selected volcanic features Orbital-science investigation: Part L: selected volcanic features
Preliminary examination of Apollo 15 orbital photographs indicates a large number of volcanic features. One area of exceptionally interesting volcanic activity is depicted in figure 25-74. Located approximately at latitude 25° S and longitude 123° E on the lunar far side, this region also is covered by panoramic camera photographs AS15-9954, 9956, 9958, and 9960 and by stereoscopically...
Authors
Mareta N. West
Preliminary geologic investigation of the Apollo 15 landing site Preliminary geologic investigation of the Apollo 15 landing site
The Apollo 15 lunar module (LM) landed at longitude 03°39'20'' E, latitude 26°26'00'' N on the mare surface of Palus Putredinis on the eastern edge of the Imbrium Basin. The site is between the Apennine Mountain front and Hadley Rille. The objectives of the mission, in order of decreasing priority, were description and sampling of three major geologic features—the Apennine Front, Hadley...
Authors
G.A. Swann, N. G. Bailey, R. M. Batson, V. L. Freeman, M. H. Hait, J.W. Head, H. E. Holt, K. A. Howard, J.B. Irwin, K.B. Larson, W.R. Muehlberger, V. S. Reed, J. J. Rennilson, G. G. Schaber, D.R. Scott, L. T. Silver, R. L. Sutton, G. E. Ulrich, H. G. Wilshire, E.W. Wolfe
Photogeology: Part A: relative ages of some near-side and far-side terra plains based on Apollo 16 metric photography Photogeology: Part A: relative ages of some near-side and far-side terra plains based on Apollo 16 metric photography
The materials of most light or terra plains predate the lunar maria and postdate the Imbrian event. In the vicinity of the Imbrium Basin, these materials have been called the Cayley Formation (ref. 29-3) but because of the subtle diversity of the terra plains over the near side, Whilhelms and McCauley (ref. 29-4) simply called these materials Imbrian plains (Ip). The age relationships...
Authors
Laurence A. Soderblom, Joseph M. Boyce
Photogeology: Part B: Cayley Formation interpreted as basin ejecta Photogeology: Part B: Cayley Formation interpreted as basin ejecta
The discovery that samples returned from the Cayley Formation at the Apollo 16 landing site consist mainly of nonvolcanic breccias (secs. 6 and 7 of this report) suggests that the hypothesis in which light plains-forming materials may be ejecta from multi-ring basins should be reevaluated (refs 29-15 to 29-17). Improved information on the morphology and distribution of the Cayley...
Authors
R. E. Eggleton, G. G. Schaber