Title |
Mineralogy and Petrology of Comet 81P/Wild 2 Nucleus Samples
|
---|---|
Published in |
Science, December 2006
|
DOI | 10.1126/science.1135842 |
Pubmed ID | |
Authors |
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 |
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. |
X Demographics
Geographical breakdown
Country | Count | As % |
---|---|---|
Unknown | 2 | 100% |
Demographic breakdown
Type | Count | As % |
---|---|---|
Scientists | 1 | 50% |
Members of the public | 1 | 50% |
Mendeley readers
Geographical breakdown
Country | Count | As % |
---|---|---|
Austria | 2 | 1% |
Italy | 1 | <1% |
Montenegro | 1 | <1% |
Brazil | 1 | <1% |
Sweden | 1 | <1% |
United Kingdom | 1 | <1% |
Canada | 1 | <1% |
Japan | 1 | <1% |
Unknown | 149 | 94% |
Demographic breakdown
Readers by professional status | Count | As % |
---|---|---|
Researcher | 50 | 32% |
Student > Ph. D. Student | 34 | 22% |
Student > Master | 14 | 9% |
Student > Doctoral Student | 10 | 6% |
Professor | 9 | 6% |
Other | 20 | 13% |
Unknown | 21 | 13% |
Readers by discipline | Count | As % |
---|---|---|
Earth and Planetary Sciences | 48 | 30% |
Physics and Astronomy | 43 | 27% |
Chemistry | 11 | 7% |
Materials Science | 11 | 7% |
Agricultural and Biological Sciences | 4 | 3% |
Other | 14 | 9% |
Unknown | 27 | 17% |