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  • 1
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    In:  Icarus, Luxembourg, Lawrence Livermore National Laboratory, vol. 30, no. 1-2, pp. 243-253, pp. B05311, (ISSN: 1340-4202)
    Publication Date: 1977
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  • 2
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    McGraw-Hill
    In:  New York, 618 pp., McGraw-Hill, vol. I, 383+VIII pp., no. Publ. No. 12, pp. 127, (ISBN 0-521-66034-3, ISBN 0-521-66948-0 paper)
    Publication Date: 1975
    Keywords: Textbook of geophysics ; Physical properties of rocks ; Earth model, also for more shallow analyses ! ; Textbook of mineralogy ; Textbook of geology
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  • 3
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    In:  J. Geol., Luxembourg, Lawrence Livermore National Laboratory, vol. 90, no. 1-2, pp. 611-643, pp. B05311, (ISSN: 1340-4202)
    Publication Date: 1982
    Keywords: Plate tectonics ; Mineralogy ; ConvolutionE ; Geol. aspects ; Geochemistry
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  • 4
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    In:  Phys. Earth Plan. Int., Luxembourg, Lawrence Livermore National Laboratory, vol. 86, no. 1-2, pp. 5-24, pp. B05311, (ISSN: 1340-4202)
    Publication Date: 1994
    Keywords: Seismology ; GeodesyY ; GeodesyY ; PEPI
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  • 5
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    Springer-Verlag
    In:  New York, 295 pp., Springer-Verlag, vol. I, 383+VIII pp., no. Publ. No. 12, pp. 127, (ISBN 0-521-66034-3, ISBN 0-521-66948-0 paper)
    Publication Date: 1979
    Keywords: Planetology ; Textbook of geophysics
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  • 6
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    Am. Geophys. Un.
    In:  Bull., Open-File Rept., The Earth beneath the Continents: A Volume in Honor of Merle A. Tuve, Leiden, Am. Geophys. Un., vol. 10, no. 87-17, pp. 611-, (ISBN 0080419208)
    Publication Date: 1966
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  • 7
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    In:  Other Sources
    Publication Date: 2019-01-25
    Description: The similarities in siderophile abundances strongly suggest that the Moon was derived from the Earth's mantle after the Earth's core had formed. The energy required to remove material from the Earth's mantle and place it into geocentric orbit can be supplied most readily by impact processes during accretion of the Earth. Impacts of late-accreting, high-velocity planetismals would evaporate many times their masses of mantle material. These gases would be accompanied by a massive spray of shock-melted silicate droplets. It is suggested that the gases produced from such near-equatorial impacts were rapidly spun out into equatorial geocentric orbit. The evaporated material was selectively recondensed, and, accompanied by the shock melted, devolatilized silicate droplets, accreted to form a sediment ring of Earth-orbiting planetismals. This sediment ring also captured a significant proportion of Earth-bound planetismals. The Moon was formed by accretion from planetismals comprising the sediment ring.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Lunar Planetary Inst. Conf. on the Origin of the Moon; p 46
    Format: text
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  • 8
    Publication Date: 2019-01-25
    Description: The earliest metal phases to crystallize from the least-fabricated low Ti mare basalts contain about 30% Ni and 2 to 7% of Co. Experimental investigations of partitioning of Ni and Co between primitive lunar basaltic magmas and metal phases are currently in progress. Preliminary results show that the metal phase crystallizing near the liquidus of Green Glass (185 ppm Ni, 70 ppm Co) would contain about 40% Ni and 2.3% Co. It seems, therefore, that if a lunar core does exist, as suggested by the results of (2), it is relatively rich in Ni (30-40%) and Co (2-7%). This composition presents a remarkable contrast to that of the Earth's core which is estimated to contain about 6% Ni and 0.3% Co. Explanations for the differing densities of Earth and Moon are imvestigated.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Lunar Planetary Inst. Conf. on the Origin of the Moon; p 14
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  • 9
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    In:  CASI
    Publication Date: 2019-05-11
    Description: Origin of meteoritic chondrules - ignimbritic origin by hypothesis and experiment
    Keywords: BIOTECHNOLOGY
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  • 10
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    In:  Other Sources
    Publication Date: 2019-06-27
    Description: An hypothesis for mare basalt petrogenesis is presented. In the proposed model, both high- and low-Ti mare basalts are produced by partial melting and hybridization at depth accompanied by equilibrium between the hybrid liquids and the local olivine-pyroxenite residuum. The energy source for mare basalt formation is ultimately provided by radiogenic heating in the primordial lunar interior. The proposed dynamic model explains similarities in the Mg/(Mg+Fe) ratios and Cr2O3 contents of high-Ti and low-Ti basalts and avoids thermal problems inherent in previous models.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: Earth and Planetary Science Letters; 30; 2, Ma; May 1976
    Format: text
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