Back to Search Start Over

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

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

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.

Details

Database :
OpenAIRE
Accession number :
edsair.od.......185..1f65b81343a394cb42afe4813d0ffa45