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Horz, Friedrich; Bastien, Ron; Borg, Janet; Bradley, John P.; Bridges, John C.; Brownlee, Donald E.; Burchell, Mark J.; Chi, Miaofang; Cintala, Mark J.; Dai, Zu Rong; Djouadi, Zahia; Dominquez, Gerardo; Economou, Thanasis E.; Fairey, Sam A. J.; Floss, Christine; Franchi, Ian A.; Graham, Giles A.; Green, Simon F.; Heck, Philipp; Hoppe, Peter; Huth, Joachim; Ishii, Hope; Kearsley, Anton T.; Kissel, Jochen; Leitner, Jan; Leroux, Hugues; Marhas, Kuljeet; Messenger, Keiko; Schwandt, Craig S.; See, Thomas H.; Snead, Christopher; Stadermann, Frank J.; Stephan, Thomas; Stroud, Rhonda; Teslich, Nick; Trigo-Rodriguez, Josep M.; Tuzzolino, A. J.; Troadec, David; Tsou, Peter; Warren, Jack; Westphal, Andrew; Wozniakiewicz, Penelope; Wright, Ian and Zinner, Ernst
(2006).
DOI: https://doi.org/10.1126/science.1135705
Abstract
Particles emanating from comet 81P/Wild 2 collided with the Stardust spacecraft at 6.1 kilometers per second, producing hypervelocity impact features on the collector surfaces that were returned to Earth. The morphologies of these surprisingly diverse features were created by particles varying from dense mineral grains to loosely bound, polymineralic aggregates ranging from tens of nanometers to hundreds of micrometers in size. The cumulative size distribution of Wild 2 dust is shallower than that of comet Halley, yet steeper than that of comet Grigg-Skjellerup.
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About
- Item ORO ID
- 7909
- Item Type
- Journal Item
- ISSN
- 0036-8075
- Academic Unit or School
-
Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM) - Research Group
- ?? space ??
- Depositing User
- Kyra Proctor