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  • 1
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    Sketch map of the region around Candidate Littrow Apollo landing sites, part H (1972)
    In:  CASI
    Details
    Publication Date: 2005-11-30
    Description: Photographs and geologic maps of the area around Littrow rilles and eastern edge of Mare Serenitatis are presented, along with variations in the features and compositions of the region.
    Keywords: SPACE SCIENCES
    Type: NASA. Manned Spacecraft Center Apollo 15 Prelim. Sci. Rept.; 3 p
    Format: text
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  • 2
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    Debris on the Surveyor 3 mirror (1972)
    In:  CASI
    Details
    Publication Date: 2005-11-30
    Description: Work is described which was performed on debris that adhered to the Surveyor 3 camera mirror after it was returned from the moon by the Apollo 12 mission. The chemical and morphological natures of the debris are described and some fine scale features of the mirror surface are discussed. Supplementary information was provided on the adhering debris so that the causes of the optical degradation of the mirror could be determined more accurately.
    Keywords: SPACE SCIENCES
    Type: NASA, Washington Analysis of Surveyor 3 Mater. and Phot. Returned by Apollo 12; p 47-50
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  • 3
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    Basalt stratigraphy of southern Mare Serenitatis (1973)
    In:  CASI
    Details
    Publication Date: 2006-01-11
    Description: The major features of the stratigraphic and structural sequence are summarized for Mare Serenitatis. The dark oldest basalts include flows coextensive with Mare Tranquillitatis and also flows and pyroclastic deposits (dark mantles) that erupted from the edge of the Serenitatis basin. The basin sagged, possibly isostatically, as basalts of intermediate age were emplaced. Sagging had nearly ceased by the time the youngest flows were deposited. Compressive movements including thrusting followed, and small extensional fissures formed in late Copernican time. The revised stratigraphic sequence that was elaborated has implications for lunar stratigraphy that transcend the boundaries of Mare Serenitatis. Dark mantle deposits and the darkest maria have commonly been assumed in geologic mapping to be relatively youthful. These assumptions must now be reevaluated and perhaps discarded.
    Keywords: SPACE SCIENCES
    Type: NASA. Johnson Space Center Apollo 17 Prelim. Sci. Rept.; 12 p
    Format: text
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  • 4
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    The geology of the Mare Serenitatis region of the moon (1966)
    In:  CASI
    Details
    Publication Date: 2006-10-26
    Description: Stratigraphy and structure of Mare Serenitatis region of moon
    Keywords: SPACE SCIENCES
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  • 5
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    Electron microscopy of micrometeorites collected on the 1965 Luster experiment (1966)
    In:  CASI
    Details
    Publication Date: 2006-10-26
    Description: Electron microscopic study of micrometeoritic material collected in upper atmosphere
    Keywords: SPACE SCIENCES
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  • 6
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    Volcanism on Mars (1973)
    In:  CASI
    Details
    Publication Date: 2006-03-27
    Description: One of the earliest and most significant of the Mariner 9 results was the recognition of prominent volcanic features on Mars. The volcanic features have a markedly asymmetric distribution. The planet can be roughly divided into two hemispheres. One includes nearly all the central volcanic features and the sparsely cratered plains; the other, for the most part, is densely cratered terrain, superficially resembling the lunar highlands.
    Keywords: SPACE SCIENCES
    Type: JPL Mariner Mars 1971 Proj., Vol. 4; p 43-61
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  • 7
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    A generalized geologic map of Mars (1973)
    In:  CASI
    Details
    Publication Date: 2006-03-27
    Description: A generalized geologic map of Mars has been constructed largely on the basis of differences in the topography of the surface. A number of topographic features on Mars whose form is highly diagnostic of their origin are shown. Of particular note are the shield volcanoes and lava plains. In some areas, the original features have been considerably modified by subsequent erosional and tectonic processes. These have not, however, resulted in homogenization of the planet's surface, but rather have emphasized its variegated character by leaving a characteristic imprint in specific areas. The topography of the planet, therefore, lends itself well to remote geologic interpretation.
    Keywords: SPACE SCIENCES
    Type: JPL Mariner Mars 1971 Proj., Vol. 4; p 21-26
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  • 8
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    Mariner 9 television reconnaissance of Mars and its satellites - Preliminary results. (1972)
    In:  Other Sources
    Details
    Publication Date: 2011-08-16
    Description: At orbit insertion, the Martian surface was largely obscured by a dust haze with an extinction optical depth that ranged from near unity in the south polar region to probably greater than two over most of the planet. The only features clearly visible were the south polar cap, one dark spot in Nix Olympica, and three dark spots in the Tharsis region. During the third week, the atmosphere began to clear and surface visibility improved, but contrasts remained a fraction of their normal value. Each of the dark spots that apparently protrude through most of the dust-filled atmosphere has a crater or crater complex in its center. The craters apparently were formed by subsidence and resemble terrestrial calderas.
    Keywords: SPACE SCIENCES
    Type: Science; 175; Jan. 21
    Format: text
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  • 9
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    A generalized geologic map of Mars. (1973)
    In:  Other Sources
    Details
    Publication Date: 2011-08-16
    Description: A geologic map of Mars has been constructed largely on the basis of photographic evidence. Four classes of units are recognized: (1) primitive cratered terrain, (2) sparsely cratered volcanic eolian plains, (3) circular radially symmetric volcanic constructs such as shield volcanoes, domes, and craters, and (4) tectonic erosional units such as chaotic and channel deposits. Grabens are the main structural features; compressional and strike slip features are almost completely absent. Most grabens are part of a set radial to the main volcanic area, Tharsis.
    Keywords: SPACE SCIENCES
    Type: Journal of Geophysical Research; 78; July 10
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  • 10
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    Preliminary Mariner 9 report on the geology of Mars. (1972)
    In:  Other Sources
    Details
    Publication Date: 2011-08-16
    Description: Mariner 9 results indicate that Mars is geologically far more heterogeneous than previously suspected from earlier flyby missions; the surface has been shaped by volcanic, tectonic, erosional, and depositional activity. The equatorial region between 30 deg N and 30 deg S latitude is depicted in four geologic sketch maps, and seventeen geologic units are defined on the basis of their textural characteristics. The maps and the brief descriptions of geological units portrayed are followed by a series of more interpretive discussions dealing with topical problems and a summary geologic history. Topics covered include cratering, circular basins, volcanism, canyons, chaotic terrain, channels, and eolian activity.
    Keywords: SPACE SCIENCES
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