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  • 1
    Publication Date: 2011-08-16
    Description: Description of the results of a preliminary study of the distribution of central peaked Martian craters based on photographs taken by Mariner 6 and 7. The study provides information about the origin of these craters and about the geological processes occurring on the surface of Mars. It is pointed out that central peaks in Martian craters in the south polar region occur more frequently than their equatorial counterparts and the peak frequency statistics and crater morphologies imply that preferential peak production has taken place.
    Keywords: SPACE SCIENCES
    Type: Nature; 234; Dec. 10
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  • 2
    Publication Date: 2011-08-16
    Description: A Fourier analysis of Martian radar topographic data is carried out to determine the magnitude and direction of the center-of-mass/center-of-figure offset of Mars. A value of about 1 km is obtained for the figure offset with respect to the center of mass in the general direction of Tharsis. It is noted that figure offsets of comparable magnitudes exist in the earth and the moon.
    Keywords: SPACE SCIENCES
    Type: Nature; 242; Mar. 23
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  • 3
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    In:  Other Sources
    Publication Date: 2019-05-24
    Description: Lunar luminescence in vicinity of Aristarchus from 1783 to 1963, examining solar flare data
    Keywords: SPACE SCIENCES
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  • 4
    Publication Date: 2019-06-27
    Description: Center of mass/center of figure offsets are known for the earth, moon, Mars and Venus. Such an offset requires a density distribution asymmetric about the center of mass. Observational evidence indicates that the terrestrial, lunar and Martian offsets result from crusts of variable thickness rather than lateral density inhomogeneities and that the thickness variations are more likely caused by internal convection than impact.
    Keywords: SPACE SCIENCES
    Type: The Moon; 7; Mar
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  • 5
    Publication Date: 2019-06-27
    Description: High precision isotopic composition measurements of Sm have been carried out for two terrestrial and seven lunar samples from three Apollo sites. The lunar samples, selected to show a wide variation in cosmic ray exposure ages, have a wide range of enrichments in Sm-150/Sm-154 (up to 0.8%) and depletions in Sm-149/Sm-154 which are due to neutron capture. The ratio of the number of neutrons captured per atom by Sm-149 to Gd-157 is 0.9 and reflects a hardened lunar neutron spectrum. This ratio is in reasonable but not exact agreement with that obtained from the theoretical lunar neutron energy spectrum of Lingenfelter, Canfield and Hampel. The average composition for terrestrial samarium is given.
    Keywords: SPACE SCIENCES
    Type: Earth and Planetary Science Letters; 13; 1, De; Dec. 197
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  • 6
    Publication Date: 2019-06-27
    Description: Sinuous rill and water distribution on lunar surface from Orbiter 4 high resolution photographs
    Keywords: SPACE SCIENCES
    Type: ; ACE(
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  • 7
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    Publication Date: 2019-06-27
    Description: Lunar sinuous rills origin, suggesting surface erosion by water rivers released from permafrost ice cover during meteoritic impact
    Keywords: SPACE SCIENCES
    Type: ; ADEMIE DES SCIENCES
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  • 8
    Publication Date: 2019-06-27
    Description: Mariner 9 imagery shows that central peaked craters occur much more frequently in the Martian south polar region than in typical equatorial areas, and that both regions have crater size frequency distributions characteristic of saturation. Several arguments indicate that a preferential production mechanism, e.g., pingo formation made possible by subsurface permafrost confined to Martian polar regions, may account for the central peak excess in the south polar region.
    Keywords: SPACE SCIENCES
    Type: Icarus; 21; Apr. 197
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  • 9
    Publication Date: 2019-06-27
    Description: Lunar sinuous rilles morphological and distributional observations and implications on theories of origin concerning surface water erosion
    Keywords: SPACE SCIENCES
    Type: ; ADEMIE DES SCIENCES
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  • 10
    Publication Date: 2019-07-13
    Description: In the orbital plane of Apollo 15 the mean lunar radius is 1737.3 km, the mean altitude of terrae above maria is about 3 km, and the center-of-figure is displaced from the center-of-mass by about 2 km away from longitude 25 E. The Apollo 16 laser altimeter obtained a total of about 7.5 revolutions of partially overlapping data. The principal difference in results from Apollo 16 is the absence of any great far-side basin similar to the 1400-km wide feature found by Apollo 15, 1200 km to the south. This absence of a far-side depression in the Apollo 16 orbital plane largely accounts for a greater mean radius: 1738.1 km; a greater mean altitude of terrae above maria: about 4 km; and a greater offset of centers: about 3 km, also away from 25 E. In the Apollo 16, as well as Apollo 15, data the far-side terrae are much 'rougher' than the near-side terrae. Mare surfaces are generally smooth to within plus or minus 150 m, and have slopes of 1:500 to 1:2000 persisting over distances as great as 500 km.
    Keywords: SPACE SCIENCES
    Type: Lunar Science Conference; Mar 05, 1973 - Mar 08, 1973; Houston, TX
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