Brownlee, Donald E. and Tsou, Peter and Aleon, Jerome and Alexander, Conel M. and Araki, Tohru and Bajt, Sasa and Baratta, Giuseppe A. and Bastien, Ron and Bland, Philip A. and Bleuet, Pierre and Borg, Janet and Bradley, John P. and Brearley, Adrian and Brenker, F. and Brennan, Sean and Bridges, John C. and Browning, Nigel D. and Brucato, John R. and Bullock, E. and Burchell, Mark J. and Busemann, Henner and Butterworth, Anna and Chaussidon, Marc and Cheuvront, Allan and Chi, Miaofang and Cintala, Mark J. and Clark, B.C. and Clemett, Simon J. and Cody, George and Colangeli, Luigi and Cooper, George and Cordier, Patrick and Daghlian, C. and Dai, Zurong and d'Hendecourt, Louis and Djouadi, Zahia and Dominguez, Gerardo and Duxbury, Tom and Dworkin, Jason P. and Ebel, Denton S. and Economou, Thanasis E. and Fakra, Sirine and Fairey, Sam A. J. and Fallon, Stewart and Ferrini, Gianluca and Ferroir, T. and Fleckenstein, Holger and Floss, Christine and Flynn, George J. and Franchi, Ian A. and Fries, Marc and Gainsforth, Zack and Gallien, J.P. and Genge, Matt and Gilles, Mary K. and Gillet, Philipe and Gilmour, Jamie and Glavin, Daniel P. and Gounelle, Matthieu and Grady, Monica M. and Graham, Giles A. and Grant, P.G. and Green, Simon F. and Grossemy, Faustine and Grossman, Lawrence and Grossman, Jeffery N. and Guan, Yunbin and Hagiya, Kenji and Harvey, Ralph and Heck, Philipp and Herzog, Gregory F. and Hoppe, Peter and Horz, Friedrich and Huth, Joachim and Hutcheon, Ian D. and Ignatyev, Konstantin and Ishii, Hope A. and Ito, Motoo and Jacob, Damien and Jacobsen, Chris and Jacobsen, Stein and Jones, Steven and Joswiak, David and Jurewicz, Amy and Kearsley, Anton T. and Keller, Lindsay P. and Khodja, H and Kilcoyne, A.L. David and Kissel, Kochen and Krot, Alexander and Langenhorst, Falko and Lanzirotti, Antonio and Le, Loan and Leshin, Laurie A. and Leitner, Jan and Lemelle, L. and Leroux, Hugues and Liu, Ming-Chang and Luening, K. and Lyon, Ian and MacPherson, Glen and Marcus, Matthew A. and Marhas, Kuljeet and Marty, Bernard and Matrajt, Graciela and McKeegan, Kevin and Meibom, Anders and Mennella, Vito and Messenger, Keiko and Messenger, Scott and Mikouchi, Takashi and Mostefaoui, Smail and Nakamura, Tomoki and Nakano, T. and Newville, M. and Nittler, Larry R. and Ohnishi, Ichiro and Ohsumi, Kazumasa and Okudaira, Kyoko and Papanastassiou, Dimitri A. and Palma, Russ and Palumbo, Maria E. and Pepin, Robert O and Perkins, David and Peronnet, Murielle and Pianetta, P. and Rao, William and Rietmeijer, Frans J. M. and Robert, Francois and Rost, D. and Rotundi, Alessandra and Ryan, Robert and Sandford, Scott A. and Schwandt, Craig S. and See, Thomas A. and Schlutter, Dennis and Sheffield-Parker, J. and Simionovici, Alexandre and Simon, Steven and Sitnitsky, I. and Snead, Christopher J. and Spencer, Maegan K. and Stadermann, Frank J. and Steele, Andrew and Stephan, Thomas and Stroud, Rhonda and Susini, Jean and Sutton, S.R. and Suzuki, Y and Taheri, Mitra and Taylor, Susan and Teslick, Nick and Tomeoka, Kazu and Tomioka, Naotaka and Toppani, Alice and Trigo-Rodriguez, Josep M. and Troaddec, David and Tsuchiyama, Akira and Tuzzolino, Anthony J. and Tyliszczak, Tolek and Uesugi, K. and Velbel, Michael and Vellenga, Joe and Vicenzi, E. and Vincze, L. and Warren, Jack and Weber, Iris and Weisberg, Mike and Westphai, Andrew J. and Wirick, Sue and Wooden, Diane and Wopenka, Brigitte and Wozniakiewicz, Penelope J. and Wright, Ian and Yabuta, Hikaru and Yano, Hajime and Young, Edward D. and Zare, Richard N. and Zega, Thomas and Ziegler, Karen and Zimmerman, Laurent and Zinner, Ernst and Zolensky, Michael E. (2006) Research article - Comet 81P/Wild 2 under a microscope. Science, 314 (5806). pp. 1711-1716. ISSN 0036-8075. (doi:https://doi.org/10.1126/science.1135840) (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided)
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The Stardust spacecraft collected thousands of particles from comet 81P/Wild 2 and returned them to Earth for laboratory study. The preliminary examination of these samples shows that the nonvolatile portion of the comet is an unequilibrated assortment of materials that have both presolar and solar system origin. The comet contains an abundance of silicate grains that are much larger than predictions of interstellar grain models, and many of these are high-temperature minerals that appear to have formed in the inner regions of the solar nebula. Their presence in a comet proves that the formation of the solar system included mixing on the grandest scales.
|Divisions:||Faculties > Sciences > School of Physical Sciences|
|Depositing User:||Mark Burchell|
|Date Deposited:||02 Sep 2008 07:16 UTC|
|Last Modified:||28 Jan 2016 16:46 UTC|
|Resource URI:||https://kar.kent.ac.uk/id/eprint/5013 (The current URI for this page, for reference purposes)|