Results 141 to 150 of about 535 (200)
A southward differentiated impactor forms the tapered shape of the South Pole-Aitken impact basin on the Moon. [PDF]
Wakita S +10 more
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Detection of lithium in the exosphere of Mercury. [PDF]
Schmid D +11 more
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The initial solar system abundance of 60Fe and early core formation of the first asteroids. [PDF]
Fang L +5 more
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Primitive asteroids as a major source of terrestrial volatiles. [PDF]
Martins R +5 more
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Percolative sulfide core formation in oxidized planetary bodies. [PDF]
Crossley SD +9 more
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Early planetesimal differentiation and late accretion shaped Earth's nitrogen budget. [PDF]
Wang W, Walter MJ, Brodholt JP, Huang S.
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Tungsten in ordinary chondrites
Earth and Planetary Science Letters, 1977Abstract In ordinary chondrites tungsten displays both lithophile and siderophile characteristics. Its concentration in the metal phase is positively correlated with petrologic type, and with the distribution coefficientKD =W in metal/W in silicates plus troilite.
Ermanno R. Rambaldi, Miguel Cendales
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Chainpur-like Chondrites: Primitive Precursors of Ordinary Chondrites?
Science, 1966Chainpur and similar, apparently primitive, chondritic meteorites may be precursors of ordinary chondrites; a variety of evidence supports this working hypothesis. In general, carbonaceous chondrites seem to be related collaterally to this genetic sequence rather than being direct ancestors of ordinary chondrites.
R A, Schmitt, R H, Smith, G G, Goles
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Geochimica et Cosmochimica Acta, 1984
A description is given of 169 Al-rich objects (arbitrarily defined as having 10 wt pct or more of Al2O3) from 24 ordinary chondrites of types 3 and 4, five regolith breccias containing unequilibrated material, the unique meteorite Kakangari, and a few ordinary chondrites of types 5 and 6.
A. Bischoff, Keil K.
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A description is given of 169 Al-rich objects (arbitrarily defined as having 10 wt pct or more of Al2O3) from 24 ordinary chondrites of types 3 and 4, five regolith breccias containing unequilibrated material, the unique meteorite Kakangari, and a few ordinary chondrites of types 5 and 6.
A. Bischoff, Keil K.
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Crystallization of chondrules in ordinary chondrites
Geochimica et Cosmochimica Acta, 1980Abstract The process of crystallization and the origin of chondrules are discussed, in terms of the phase relations of the minerals in chondrules in six ordinary chondrites of the Yamato-74 meteorites, especially the Yamato-74191 (L3). Chondrules are classified into six types.
Makoto Kimura, Kenzo Yagi
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