Calcium-aluminum-rich inclusions from enstatite chondrites: Indigenous or foreign?
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Guan, YB
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Smithsonian Inst, Natl Museum Nat Hist, Dept Mineral Sci, Washington, DC 20560 USASmithsonian Inst, Natl Museum Nat Hist, Dept Mineral Sci, Washington, DC 20560 USA
Guan, YB
[1
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Huss, GR
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机构:Smithsonian Inst, Natl Museum Nat Hist, Dept Mineral Sci, Washington, DC 20560 USA
Huss, GR
MacPherson, GJ
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机构:Smithsonian Inst, Natl Museum Nat Hist, Dept Mineral Sci, Washington, DC 20560 USA
MacPherson, GJ
Wasserburg, GJ
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机构:Smithsonian Inst, Natl Museum Nat Hist, Dept Mineral Sci, Washington, DC 20560 USA
Wasserburg, GJ
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[1] Smithsonian Inst, Natl Museum Nat Hist, Dept Mineral Sci, Washington, DC 20560 USA
[2] CALTECH, Div Geol & Planetary Sci 170 25, Lunat Asylum, Pasadena, CA 91125 USA
[3] Arizona State Univ, Ctr Meteorite Studies, Tempe, AZ 85287 USA
[4] Arizona State Univ, Dept Geol, Tempe, AZ 85287 USA
The primary mineral assemblages and initial Al-26/Al-27 ratios of rare calcium-aluminum-rich inclusions (CAIs) from enstatite (E) chondrites are similar to those of CAIs from other chondrite classes. CAIs from all chondrite classes formed under oxidizing conditions that are much different from the reducing conditions under which the E chondrites formed. Either CAIs formed at an earlier, more oxidizing epoch in the region where E chondrites ultimately formed, or they formed at a different place in the solar nebula and were transported into the E chondrite formation region.
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页码:1330 / 1333
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