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- W2724331218 abstract "Abstract We have discovered in a Stardust mission terminal particle a unique mineralogical assemblage of symplectically intergrown pentlandite ((Fe,Ni) 9 S 8 ) and nanocrystalline maghemite (γ‐Fe 2 O 3 ). Mineralogically similar cosmic symplectites (COS) have only been found in the primitive carbonaceous chondrite Acfer 094 and are believed to have formed by aqueous alteration. The O and S isotopic compositions of the Wild 2 COS are indistinguishable from terrestrial values. The metal and sulfide precursors were thus oxidized by an isotopically equilibrated aqueous reservoir either inside the snow line, in the Wild 2 comet, or in a larger Kuiper Belt object. Close association of the Stardust COS with a Kool mineral assemblage (kosmochloric Ca‐rich pyroxene, FeO‐rich olivine, and albite) that likely originated in the solar nebula suggests the COS precursors also had a nebular origin and were transported from the inner solar system to the comet‐forming region after they were altered." @default.
- W2724331218 created "2017-07-14" @default.
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- W2724331218 date "2017-06-28" @default.
- W2724331218 modified "2023-10-16" @default.
- W2724331218 title "Coordinated mineralogical and isotopic analyses of a cosmic symplectite discovered in a comet 81P/Wild 2 sample" @default.
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- W2724331218 doi "https://doi.org/10.1111/maps.12905" @default.
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