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  • LUNAR AND PLANETARY EXPLORATION  (1,275)
  • 2000-2004
  • 1980-1984  (552)
  • 1975-1979  (723)
  • 1983  (552)
  • 1977  (723)
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  • 2000-2004
  • 1980-1984  (552)
  • 1975-1979  (723)
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  • 1
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    In:  CASI
    Publication Date: 2019-08-28
    Description: The Viking spacecraft are described as well as the instruments carried to accomplish the combined goal of studying the atmosphere and geology of the entire planet, and to analyze the Martian soil and search for life in two specific locations. Imagery received from the spacecraft illustrate discussions of the planetary surface, composition, and winds. Suggestions for further reading are included along with a list of available NASA film. Experiments and activities for classroom use are described.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: EP-146
    Format: application/pdf
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  • 2
    Publication Date: 2019-08-28
    Description: The surfaces of the Saturn satellites Tethys, Iapetus and Encedalus display surfaces which indicate active geological processes and therefore suggest a degree of internal evolution. By contrast, the Saturn satellite Hyperion and the coorbitals 1980S1 and 1980S3 show no trace of geological activity and may be fragments of once-larger bodies. Activity on Iapetus appears to have been confined to the dark terrain, and offers no clue as to its timing and extent. The widest terrain type and crater number variations are those of Encedalus, which indicate the most prolonged period of geological activity of any of the satellites studied.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Nature; 301; Feb. 24
    Format: text
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  • 3
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    In:  CASI
    Publication Date: 2019-08-28
    Description: An overview of the Viking Mars probe is presented. The Viking spacecraft is described and a brief history of the earlier observations and exploration of Mars is provided. A number of the Viking photographs of the Martian surface are presented and a discussion of the experiments Viking performed including a confirmation of the general theory of relativity are reported. Martian surface chemistry is discussed and experiments to study the weather on Mars are reported.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: NASA-EP-146
    Format: application/pdf
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  • 4
    Publication Date: 2019-08-28
    Description: Global mean distributions of Martian atmospheric components concentrations from the planet's surface up to an altitude of 250 km are calculated. Improved data on the turbulent mixing coefficient, as a function of altitude, on temperature distribution and on chemical and photochemical reaction rates are used. The model data agree well with available measurements of some components concentrations. Variations of composition due to long-period variations of temperature, moisture and turbulent mixing are investigated. The relative significance of different catalytic cycles and the important role of excited atoms 0 (d-1) are revealed.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: NASA-TM-75048
    Format: application/pdf
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  • 5
    Publication Date: 2019-08-28
    Description: Formation of the equatorial jet of the Jovian surface was explained as a consequence of the Taylor-Proudman theorem. The asymptotic theory of motion of low viscosity fluids in a rotating spherical shear layer was included. The model shows the straited structure of the Jovian surface as the outflow of convective cells having the shape of axisymmetric rolls extended along the axis of rotation in the meridional direction. Depth of the layer was found to be of the order of 1000 kilometers.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: NASA-TM-75247
    Format: application/pdf
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  • 6
    Publication Date: 2019-08-28
    Description: The science objectives of a first comet mission are reviewed and related to what is known or can be expected to be learned in the near future from ground-based and near earth observations. A set of instruments and their science objectives are defined for a mission to Comet Halley during its 1985/86 apparition. The benefits from a fast flyby, a slow flyby, or a rendezvous mission and the relative impact of each on the instrument payload were assessed. The relative scientific value of encounters with the comet at distances from the sun ranging from 1 AU to 2.5 AU, including possible tradeoffs between flyby velocity and distance was considered. Pre- and post-perihelion encounters were likewise evaluated.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: NASA-TM-78420
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  • 7
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    In:  CASI
    Publication Date: 2019-08-28
    Description: The NASA Voyager mission to explore planets of the outer solar system is summarized. The mission schedule and profiles for encounters with Jupiter and Saturn, and possibly with Uranus and Pluto are included along with a description of the spacecraft and its trajectories. Scientific investigations to be made and the instruments carried are also discussed.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: NASA-SP-420
    Format: application/pdf
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  • 8
    Publication Date: 2019-08-28
    Description: The history of naming the details of the relief on the near and reverse sides of the moon is examined. The book contains lists of the names of craters of the reverse side of the moon in Russian and the Latin spellings.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: NASA-TM-75035
    Format: application/pdf
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  • 9
    Publication Date: 2019-08-28
    Description: An algorithm is described for constructing the model of the Venus surface as an expansion in spherical functions. The relief expansion coefficients were obtained up to the coefficient S sub 99. The surface picture representation is given according to this expansion. The surface model constructed was used for processing radar observations. The use of the surface model allows improved agreement between the design and measured values of radar ranges.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: NASA-TM-77298 , NAS 1.15:77298
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  • 10
    Publication Date: 2019-08-28
    Description: The hypothesis that a part of the lechatellierites which originated by etching from a basic moldavite mass became broken off after deposition of moldavite in the sedimentation layer is advanced. Those found close to the original moldavite were measured for statistical averaging of length. The average length of lechatelierite fibers per cubic mm of moldavite mass volume was determined by measurement under a microscope in toluene. The data were used to calculate the depth of the moldavite layer that had to be etched to produce the corresponding amount of lechatelierite fragments. The calculations from five "fields" of moldavite surface, where layers of fixed lechatelierite fragments were preserved, produced values of 2.0, 3.1, 3.5, 3.9 and 4.5. Due to inadvertent loss of some fragments the determined values are somewhat lower than those found in references. The difference may be explained by the fact that the depth of the layer is only that caused by etching after moldavite deposition.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: NASA-TM-77334 , NAS 1.15:77334
    Format: application/pdf
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