Ratios of S, Se and Te in the silicate Earth require a volatile-rich late veneer.
about
Geochemical arguments for an Earth-like Moon-forming impactorThe chlorine isotope fingerprint of the lunar magma ocean.Lunar tungsten isotopic evidence for the late veneer.Highly siderophile elements in Earth's mantle as a clock for the Moon-forming impact.Ruthenium isotopic evidence for an inner Solar System origin of the late veneer.Halogens in chondritic meteorites and terrestrial accretion.The lunar core can be a major reservoir for volatile elements S, Se, Te and Sb.Earth's volatile contents established by melting and vaporization.Oxygen isotopic evidence for accretion of Earth's water before a high-energy Moon-forming giant impact.Carbon-saturated monosulfide melting in the shallow mantle: solubility and effect on solidusCarbon and sulfur budget of the silicate Earth explained by accretion of differentiated planetary embryos
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Ratios of S, Se and Te in the silicate Earth require a volatile-rich late veneer.
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2013 nî lūn-bûn
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2013年の論文
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Ratios of S, Se and Te in the silicate Earth require a volatile-rich late veneer.
@en
Ratios of S, Se and Te in the silicate Earth require a volatile-rich late veneer.
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label
Ratios of S, Se and Te in the silicate Earth require a volatile-rich late veneer.
@en
Ratios of S, Se and Te in the silicate Earth require a volatile-rich late veneer.
@nl
prefLabel
Ratios of S, Se and Te in the silicate Earth require a volatile-rich late veneer.
@en
Ratios of S, Se and Te in the silicate Earth require a volatile-rich late veneer.
@nl
P2860
P356
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P1476
Ratios of S, Se and Te in the silicate Earth require a volatile-rich late veneer.
@en
P2093
Harry Becker
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P2888
P304
P356
10.1038/NATURE12285
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P50
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2013-07-01T00:00:00Z
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1021309616