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  • 1995-1999
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  • 1
    facet.materialart.
    Unbekannt
    In:  Other Sources
    Publikationsdatum: 2011-12-21
    Schlagwort(e): GEOPHYSICS
    Materialart: Life Sci. Publ., Vol. 2; 11 p
    Format: text
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  • 2
    Publikationsdatum: 2005-11-30
    Beschreibung: Infrared and radar studies of the Apollo 16 landing site are summarized. Correlations and comparisons between earth based remote sensing data, IR observations, and other data are discussed in detail. Remote sensing studies were devoted to solving two problems: (1) determining the physical difference between Cayley and Descartes geologic units near the landing site; and (2) determining the nature of the bright unit of Descartes mountain material.
    Schlagwort(e): SPACE SCIENCES
    Materialart: NASA. Lyndon B. Johnson Space Center Apollo 16 Prelim. Sci. Rept.; 5 p
    Format: text
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  • 3
    Publikationsdatum: 2005-11-30
    Beschreibung: Problematic causes and characteristics of light colored sinuous markings on the lunar surface are explored. Two processes, exogenetic and endogenetic, are examined in detailed. During the endogenetic process it is suggested that impact ejecta deposition and surface disturbances cause the markings. During the endogenetic process, it is suggested that extrusive volcanism and sublimation and/or alteration cause the markings.
    Schlagwort(e): SPACE SCIENCES
    Materialart: NASA. Lyndon B. Johnson Space Center Apollo 16 Prelim. Sci. Rept.; 4 p
    Format: text
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  • 4
    Publikationsdatum: 2005-11-30
    Beschreibung: Probable causes, distributions, and nature of fracture patterns of Type 3 craters around the margins of major maria are investigated.
    Schlagwort(e): SPACE SCIENCES
    Materialart: NASA. Lyndon B. Johnson Space Center Apollo 16 Prelim. Sci. Rept.; 1 p
    Format: text
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  • 5
    Publikationsdatum: 2005-11-30
    Beschreibung: 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.
    Schlagwort(e): SPACE SCIENCES
    Materialart: NASA. Lyndon B. Johnson Space Center Apollo 16 Prelim. Sci. Rept.; 1 p
    Format: text
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  • 6
    facet.materialart.
    Unbekannt
    In:  CASI
    Publikationsdatum: 2005-11-30
    Beschreibung: Morphometric analysis of lunar craters complements the more traditional photointerpretive study of crater morphology. A sampling is presented of morphometric results for five selected medium-sized craters photographed on the Apollo 16 mission: Madler, Langrenus B, Isidorus, Capella, and King. Apollo metric camera data present the first real opportunity to evaluate previous topographic measurements in terms of accuracy rather than in terms of precision. This method of generating crater measurements furnishes far more complete data than does the shadow-length method that yielded most of the previous morphometric information on lunar craters.
    Schlagwort(e): SPACE SCIENCES
    Materialart: NASA. Lyndon B. Johnson Space Center Apollo 16 Prelim. Sci. Rept.; 6 p
    Format: text
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  • 7
    facet.materialart.
    Unbekannt
    In:  CASI
    Publikationsdatum: 2005-11-30
    Beschreibung: Photogeologic analysis was attempted on a strip of Apollo 16 metric photographs; the superior quality and stereographic properties of the photography permitted this reevaluation. Geologic contacts, as redrawn closely resemble those of earlier maps, but some differences resulted because of improved photographic quality and a conscious attempt to test fully the impact hypothesis. All or most of the nonmare material of the region of the northern Nectaris Basin rim can be explained by the formation of impact basins. This interpretation seems strained only for some irregular and clustered craters north of Mare Nectaris and for the southern facies of the Descartes material. If the latter material is shown to have been sampled and to be of impact origin, then extensive hill and crater-forming volcanic material of Imbrian or younger age probably does not exist on the lunar terra.
    Schlagwort(e): SPACE SCIENCES
    Materialart: NASA. Lyndon B. Johnson Space Center Apollo 16 Prelim. Sci. Rept.; 4 p
    Format: text
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  • 8
    Publikationsdatum: 2005-11-30
    Beschreibung: The distribution of subtle but definite color variations on the lunar surface is analyzed using Apollo 16 photographs. Results show the strongest color variations and most distinct boundaries are concentrated in the northwest quadrant of the moon, where major boundaries correspond with distal fronts of a complex and prominent series of lava flows.
    Schlagwort(e): SPACE SCIENCES
    Materialart: NASA. Lyndon B. Johnson Space Center Apollo 16 Prelim. Sci. Rept.; 1 p
    Format: text
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  • 9
    Publikationsdatum: 2005-11-30
    Beschreibung: Stereoscopic lunar photographs were used to study the form of mare ridges and arches, their relative ages, and their association with fractures and sinuous rilles in the Southern Oceanus Procellarum.
    Schlagwort(e): SPACE SCIENCES
    Materialart: NASA. Lyndon B. Johnson Space Center Apollo 16 Prelim. Sci. Rept.; 3 p
    Format: text
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  • 10
    facet.materialart.
    Unbekannt
    In:  CASI
    Publikationsdatum: 2005-11-30
    Beschreibung: Additional evidence of the volcanic origin of mare ridges and sinuous rilles is provided by near-terminator photography of the Herigonius Rille area (12 deg S 37 deg W) northeast of Gassendi Crater. A possible genetic relationship between ridges and rilles is illustrated. From the figure, the following relationships are evident. (1) The most prominent rille crosses several ridges without distortion, which indicates that the mare ridges did not form after the sinuous rilles. (2) The rilles could not have formed by flow up and over the ridges. (3) The rilles extend from their widest ends toward distinctly lower elevations, and the largest one branches both north and south from the vent area. Elevations are evident in stereographic views that clearly indicate the local slopes. (4) The wider end of each rille is marked by an elongate vent (?) near the summit of the mare ridge from which the rille appears to issue. (5) The two most prominent rilles join south of the vent area and continue southward for more than 130 km.
    Schlagwort(e): SPACE SCIENCES
    Materialart: NASA. Lyndon B. Johnson Space Center Apollo 16 Prelim. Sci. Rept.; 1 p
    Format: text
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