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  • LUNAR AND PLANETARY EXPLORATION  (700)
  • 1985-1989  (700)
  • 1987  (700)
  • 1
    Publication Date: 2019-08-28
    Description: The surface of Mars displays a broad range of channel and valley features. There is as great a range in morphology as in scale. Some of the features of Martian geography are examined. Geomorphic mapping, crater counts on selected surfaces, and a detailed study of drainage basins are used to trace the geologic evolution of the Margaritifer Sinus Quandrangle. The layered deposits in the Valles Marineris are described in detail and the geologic processes that could have led to their formation are analyzed.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: NASA-TM-89871 , NAS 1.15:89871
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  • 2
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    In:  CASI
    Publication Date: 2019-08-28
    Description: The surface of the southern hemisphere of Miranda imaged by Voyager 2 is divisible into two general types of terrain: cratered terrain, characterized by numerous craters and undulating intercrater plains; and basins, circular to rectangular areas of complex morphology having large-scale albedo markings. To determine the relative ages of the terrains and the length of geological activity, crater-frequency data were compiled for various parts of the cratered terrain and basins. Crater-frequency data indicate that the cratered terrain is the oldest terrain on Miranda and that it was locally resurfaced.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Reports of Planetary Geology and Geophysics Program, 1986; p 9-11
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  • 3
    Publication Date: 2019-08-28
    Description: Reflectance spectroscopy is a remote sensing technique used to study the surfaces and atmospheres of solar system bodies. It provides first-order information on the presence and amounts of certain ions, molecules, and minerals on a surface or in an atmosphere. Reflectance spectroscopy has become one of the most important investigations conducted on most current and planned NASA Solar System Exploration Program space missions. This book reviews the field of reflectance spectroscopy, including information on the scientific technique, contributions, present conditions, and future directions and needs.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: NASA-SP-493 , NAS 1.21:493 , LC-87-28154
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  • 4
    Publication Date: 2019-08-28
    Description: The surface of Ariel imaged by Voyager 2 can be divided into several types of terrain on the basis of morphology: cratered terrain, subdued terrain, ridged terrain, and plains. Crater statistics were compiled for each of the terrain types. Despite differing morphology, the various terrains on Ariel do not exhibit large variations in crater frequency. None of the observed surfaces on Ariel record the period of accretion. It seems that conditions appropriate for resurfacing could have occurred during the early history of Ariel.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Reports of Planetary Geology and Geophysics Program, 1986; p 19-21
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  • 5
    Publication Date: 2019-08-28
    Description: Geomorphic mapping, crater counts on selected surfaces, and a detailed study of drainage basins, were used to trace the geologic evolution of Margaritifer Sinus Quandrangle. The oldest dated surface covering these basins evolved during the period of intense bombardment. Since that time four resurfacing events have occurred. The first three were all of regional extent, while the fourth, occurred locally, filling basins. Valley networks, incised in the third event unit, are always buried by the fourth event unit when present. A peak in geomorphic activity occurred from 10,000 to 5000. Events during this period included the formation of Uzboi/Ladon Valles with deposition in Ladon Basin, and the formation of Samara and Parana/Loire Valles in MC19SE. Flow out of Ladon Basin and to a lesser extent Samara and Parana/Loire Valles created etched terrain at their confluence that was synchronous with initiation of Margaritifer and Iani Chaos. The range of dates for the chaos may be due to periodic collapse. The extensive, well integrted nature of Samara and Parana/Loire Valles requires the existence of a long period of favorable climatic conditions to allow their formation. Development of these two systems was probably through sapping processes.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Advances in Planetary Geology 2; 259 p
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  • 6
    Publication Date: 2019-08-28
    Description: Analysis of measurements of the scattered and direct components of Voyager 1 radio occultation signals at 3.5 and 13 cm wavelengths yield estimates of the distribution functions of supracentimeter-size particles and thickness of relatively broad regions in Saturn's rings. If mearurements of signal amplitude at a shorter wavelength are combined with the previously analyzed data, the shape of the distribution functions characterizing the smaller particles can be constrained. If size distributions of arbitrary form were considered, many solutions are found that are consistent with the three available observations of signal amplitude. The best-fit power law was calculated to the three observations at three wavelengths for several of the embedded Saturn ringlets. Mie scattering theory predicts that the measured phase of the radio occultation signal is highly sensitive to particles ranging from 0.1 to 1.0 wavelengths in size, thus additional constraints on the subcentimeter-size distribution functions for both the Saturn and Uranus rings can in principle be derived from radio phase measurements.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: NASA, Washington, Reports of Planetary Geology and Geophysics Program, 1986; p 55-56
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  • 7
    Publication Date: 2019-08-28
    Description: Slopes and heights in craters and grooves which appear to be overlain with regoliths make it possible to set lower limits for regolith strength. The mechanical properties for this material are set at c = 0.001-0.07 N/ sq cm, phi = 5-30 deg.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: NASA-TM-88496 , NAS 1.15:88496
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  • 8
    Publication Date: 2019-08-28
    Description: Detailed mapping of the layered deposits in the Valles Marineris, Mars from high-resolution Viking orbiter images revealed that they from plateaus of rhythmically layered material whose bases are in the lowest elevations of the canyon floors, and whose tops are within a few hundred meters in elevation of the surrounding plateaus. Four hypotheses for the origin of the layered deposits were considered: that they are eolian deposits; that they are remnants of the same material as the canyon walls; that they are explosive volcanic deposits; or that they were deposited in standing bodies of water. There are serious morphologic objections to each of the first three. The deposition of the layered deposits in standing bodies of water best explains their lateral continuity, horizontality, great thickness, rhythmic nature, and stratigraphic relationships with other units within the canyons. The Martian climatic history indicated that any ancient lakes were ice covered. Two methods for transporting sediment through a cover of ice on a martian lake appear to be feasible. Based on the presently available data, along with the theoretical calculations presented, it appears most likely that the layered deposits in the Valles Marineris were laid down in standing bodies of water.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Advances in Planetary Geology 1; 175 p
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  • 9
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    In:  CASI
    Publication Date: 2019-08-28
    Description: Abstracts compiled from reports from Principal Investigators of the NASA Planetary Geology and Geophysics Program, Office of Space Science and Applications are presented. The purpose is to document in summary form work conducted in this program during 1986. Each report reflects significant accomplishments within the area of the author's funded grant or contract.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: NASA-TM-89810 , NAS 1.15:89810
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  • 10
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    In:  Other Sources
    Publication Date: 2019-08-27
    Description: This presentation shows what researchers are designing (solar balloon and rover) to better explore Mars geography before sending a manned mission.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: ASR-243 , NASA-TM-109306 , NONP-NASA-VT-93-185324
    Format: text
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