Chemical compositions of Antarctic meteorites I
P(論文) Sixty-four chondrites (14H, 25L, 17LL and 8C), 32 achondrites and 2 rare stony-iron meteorites from Antarctica were analyzed by standard wet chemical analysis method. In the present paper the analyses of the chondrites and the stony-iron meteorites are reported. Many Antarctic meteorites are more or less weathered or oxidized.
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Antagonistic effects of amino acids support abiotic nano-environments in clay. [PDF]
Bezaly OR, King HE, Petrignani A.
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Extraterrestrial regolith is hemostatic and potentially suitable for hemorrhage control in space. [PDF]
Ali-Mohamad N +6 more
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Distribution of extraterrestrial nucleobases, other N-heterocycles, and their precursors in a sample from asteroid Bennu. [PDF]
Oba Y +12 more
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Multiple formation pathways for amino acids in the early Solar System based on carbon and nitrogen isotopes in asteroid Bennu samples. [PDF]
Baczynski AA +11 more
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High-resolution synchrotron X-ray study of icosahedrite, an icosahedral AlCuFe quasicrystal from the Khatyrka meteorite. [PDF]
Takakura H +8 more
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A closer look into the structure and magnetism of the recently fallen meteorite Ribbeck. [PDF]
Kołodziej M +5 more
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Time of proto-Earth reservoir formation and volatile element depletion from <sup>53</sup>Mn-<sup>53</sup>Cr chronometry. [PDF]
Kruttasch PM, Mezger K.
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Oxygen isotopic compositions of several Antarctic meteorites
P(論文) Oxygen isotopic compositions are reported for seven carbonaceous chondrites, seven ordinary chondrites, two enstatite chondrites, three lunar meteorites, and twelve achondrites. Three of the achondrites (ALH-77081,Y-74063,and Y-74025) do not belong to known groups; the first two of these are related to Acapulco.
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