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Mineralogy and petrology of comet 81P/wild 2 nucleus samples

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Zolensky, Michael
Zega, Thomas
Yano, Hajime
Wirick, Sue
Westphal, Andrew J
Weisberg, Mike
Weber, Iris
Warren, Jack
Velbel, Michael
Tsuchiyama, Akira

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American Association for the Advancement of Science

Abstract

The bulk of the comet 81P/Wild 2 (hereafter Wild 2) samples returned to Earth by the Stardust spacecraft appear to be weakly constructed mixtures of nanometer-scale grains, with occasional much larger (over 1 micrometer) ferromagnesian silicates, Fe-Ni sulfides, Fe-Ni metal, and accessory phases. The very wide range of olivine and low-Ca pyroxene compositions in comet Wild 2 requires a wide range of formation conditions, probably reflecting very different formation locations in the protoplanetary disk. The restricted compositional ranges of Fe-Ni sulfides, the wide range for silicates, and the absence of hydrous phases indicate that comet Wild 2 experienced little or no aqueous alteration. Less abundant Wild 2 materials include a refractory particle, whose presence appears to require radial transport in the early protoplanetary disk.

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Restricted until

2037-12-31
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