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  • 1
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    Selected volcanic and surficial features, part O (1972)
    In:  CASI
    Details
    Publication Date: 2005-11-30
    Description: Metric camera photographs are used to analyze volcanic and surficial features of the lunar surface between Mare Smythii and King Crater. Patterns created by lava flows, ejecta blankets, impact debris, and fissures are discussed in detail. Possible causes of each phenomena are suggested.
    Keywords: SPACE SCIENCES
    Type: NASA. Lyndon B. Johnson Space Center Apollo 16 Prelim. Sci. Rept.; 1 p
    Format: text
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  • 2
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    Volcanism in the lunar Maria (1973)
    In:  CASI
    Details
    Publication Date: 2006-01-11
    Description: The formation, modification, and deformation of lunar maria by extended volcanic and tectonic processes are examined. Data also cover lava flows, sinuous rilles, mare ridges, faults, and fracture systems. Stages involved in the modification of impact craters by tectonism, volcanism, younger impacts, and mass wasting are included.
    Keywords: SPACE SCIENCES
    Type: NASA. Johnson Space Center Apollo 17 Prelim. Sci. Rept.; 11 p
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  • 3
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    Petrology (1974)
    In:  Other Sources
    Details
    Publication Date: 2011-08-16
    Description: Boulder 1 as a whole can be considered a complex polymict breccia consisting of lithic and breccia clasts seated in a matrix that ranges from friable and poorly sintered to densely welded. Only two of the four samples collected from boulder 1, Station 2 have been examined in detail: 72255 and 72275. Of the remaining two, only two undocumented thin sections from 72235 have been studied, while none from 72215 has been examined. Sample 72275 was collected as representative of the boulder matrix, whereas the other three samples were thought to be large clasts.
    Keywords: SPACE SCIENCES
    Type: Interdisciplinary Studies of Samples From Boulder 1, Sta. 2, Apollo 17, Vol. 1; p 35-109
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  • 4
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    Interdisciplinary studies of samples from Boulder 1, Station 2, Apollo 17, volume 1 (1974)
    In:  CASI
    Details
    Publication Date: 2019-06-27
    Description: Geomorphological studies on rock samples from the Apollo 17 lunar landing site are presented.
    Keywords: SPACE SCIENCES
    Type: NASA-CR-134215 , SAO-403-003
    Format: application/pdf
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  • 5
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    Analysis of lunar mare geology from Apollo photography (1973)
    In:  Other Sources
    Details
    Publication Date: 2019-07-13
    Description: Panoramic and metric photography of the lunar surface from Apollo missions 15, 16, and 17 is the basis for descriptions and interpretations of mare surface features. It is suggested that the formation of mare ridges occurred over an extended period of time rather than in single short episodes of activity through faulting, flexuring, volcanism, and plutonism. Spatial relationships between rilles and ridges suggest they were formed both simultaneously and sequentially. The sinuous rilles may have developed as open lava channels or collapsed lava tubes, while the straight rilles may have been formed by fracturing. It is inferred that small scale volcanism and tectonism have occurred between major flooding episodes.
    Keywords: SPACE SCIENCES
    Type: Lunar Science Conference; Mar 05, 1973 - Mar 08, 1973; Houston, TX
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  • 6
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    The geologic setting of Boulder 1, Station 2 (1974)
    In:  Other Sources
    Details
    Publication Date: 2019-08-27
    Description: Apollo 17 landed on the flat floor of a deep, narrow valley embayed in the mountainous highlands that comprise the southeastern rim of Mare Serenitatis. Serenitatis is one of the youngest multiringed basins on the lunar nearside and is underlain by a mascon. The valley of Taurus-Littrow, which is radial to the basin, is generally interpreted as a graben formed as a result of structural adjustments of the lunar crust in response to the Serenitatis event.
    Keywords: SPACE SCIENCES
    Type: Smithsonian Astrophys. Obs. Interdisciplinary Studies of Samples From Boulder 1, Sta. 2, Apollo 17, Vol. 1; p 1-8
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