Mineralogy and petrology of comet 81P/Wild 2 nucleus samples.

نویسندگان

  • Michael E Zolensky
  • Thomas J Zega
  • Hajime Yano
  • Sue Wirick
  • Andrew J Westphal
  • Mike K Weisberg
  • Iris Weber
  • Jack L Warren
  • Michael A Velbel
  • Akira Tsuchiyama
  • Peter Tsou
  • Alice Toppani
  • Naotaka Tomioka
  • Kazushige Tomeoka
  • Nick Teslich
  • Mitra Taheri
  • Jean Susini
  • Rhonda Stroud
  • Thomas Stephan
  • Frank J Stadermann
  • Christopher J Snead
  • Steven B Simon
  • Alexandre Simionovici
  • Thomas H See
  • François Robert
  • Frans J M Rietmeijer
  • William Rao
  • Murielle C Perronnet
  • Dimitri A Papanastassiou
  • Kyoko Okudaira
  • Kazumasa Ohsumi
  • Ichiro Ohnishi
  • Keiko Nakamura-Messenger
  • Tomoki Nakamura
  • Smail Mostefaoui
  • Takashi Mikouchi
  • Anders Meibom
  • Graciela Matrajt
  • Matthew A Marcus
  • Hugues Leroux
  • Laurence Lemelle
  • Loan Le
  • Antonio Lanzirotti
  • Falko Langenhorst
  • Alexander N Krot
  • Lindsay P Keller
  • Anton T Kearsley
  • David Joswiak
  • Damien Jacob
  • Hope Ishii
  • Ralph Harvey
  • Kenji Hagiya
  • Lawrence Grossman
  • Jeffrey N Grossman
  • Giles A Graham
  • Matthieu Gounelle
  • Philippe Gillet
  • Matthew J Genge
  • George Flynn
  • Tristan Ferroir
  • Stewart Fallon
  • Sirine Fakra
  • Denton S Ebel
  • Zu Rong Dai
  • Patrick Cordier
  • Benton Clark
  • Miaofang Chi
  • Anna L Butterworth
  • Donald E Brownlee
  • John C Bridges
  • Sean Brennan
  • Adrian Brearley
  • John P Bradley
  • Pierre Bleuet
  • Phil A Bland
  • Ron Bastien
چکیده

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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عنوان ژورنال:
  • Science

دوره 314 5806  شماره 

صفحات  -

تاریخ انتشار 2006