Supporting online materials for mineralogy and petrology of Comet81P/Wild 2 nucleus samples
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.
- Research Organization:
- COLLABORATION - NASA
- DOE Contract Number:
- DE-AC02-05CH11231
- OSTI ID:
- 919394
- Report Number(s):
- LBNL-62786; SCEHDK; TRN: US200822%%39
- Journal Information:
- Science, Vol. 314; Related Information: Journal Publication Date: 12/15/2006; ISSN 0193-4511
- Country of Publication:
- United States
- Language:
- English
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Mineralogy and Petrology of Comet Wild 2 Nucleus Samples
Physical, Chemical, and Mineralogical Properties of Comet 81P/Wild 2 Particles Collected by Stardust