| Literature DB >> 25124433 |
Andrew J Westphal1, Rhonda M Stroud2, Hans A Bechtel3, Frank E Brenker4, Anna L Butterworth5, George J Flynn6, David R Frank7, Zack Gainsforth5, Jon K Hillier8, Frank Postberg8, Alexandre S Simionovici9, Veerle J Sterken10, Larry R Nittler11, Carlton Allen12, David Anderson5, Asna Ansari13, Saša Bajt14, Ron K Bastien7, Nabil Bassim2, John Bridges15, Donald E Brownlee16, Mark Burchell17, Manfred Burghammer18, Hitesh Changela19, Peter Cloetens20, Andrew M Davis21, Ryan Doll22, Christine Floss22, Eberhard Grün23, Philipp R Heck24, Peter Hoppe25, Bruce Hudson26, Joachim Huth25, Anton Kearsley27, Ashley J King21, Barry Lai28, Jan Leitner25, Laurence Lemelle29, Ariel Leonard22, Hugues Leroux30, Robert Lettieri5, William Marchant5, Ryan Ogliore31, Wei Jia Ong22, Mark C Price17, Scott A Sandford32, Juan-Angel Sans Tresseras20, Sylvia Schmitz4, Tom Schoonjans18, Kate Schreiber22, Geert Silversmit18, Vicente A Solé20, Ralf Srama33, Frank Stadermann22, Thomas Stephan21, Julien Stodolna5, Stephen Sutton28, Mario Trieloff8, Peter Tsou34, Tolek Tyliszczak3, Bart Vekemans18, Laszlo Vincze18, Joshua Von Korff5, Naomi Wordsworth35, Daniel Zevin5, Michael E Zolensky12.
Abstract
Seven particles captured by the Stardust Interstellar Dust Collector and returned to Earth for laboratory analysis have features consistent with an origin in the contemporary interstellar dust stream. More than 50 spacecraft debris particles were also identified. The interstellar dust candidates are readily distinguished from debris impacts on the basis of elemental composition and/or impact trajectory. The seven candidate interstellar particles are diverse in elemental composition, crystal structure, and size. The presence of crystalline grains and multiple iron-bearing phases, including sulfide, in some particles indicates that individual interstellar particles diverge from any one representative model of interstellar dust inferred from astronomical observations and theory.Entities:
Year: 2014 PMID: 25124433 DOI: 10.1126/science.1252496
Source DB: PubMed Journal: Science ISSN: 0036-8075 Impact factor: 47.728