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Carbonates Found in Stardust Aerogel TracksPreliminary examination of particles collected from Comet Wild 2 suggest that this comet is chondritic and formed under multiple processes. The lack of any hydrated minerals strongly suggests that most, if not all of these processes were anhydrous [1,2,3]. However, carbonates were found in particles extracted from 4 different tracks in the aerogel. It is our belief that these carbonates have a terrestrial origin and are a contaminant in these samples.
Document ID
20070006844
Acquisition Source
Johnson Space Center
Document Type
Extended Abstract
Authors
Wirick, S.
(State Univ. of New York Stony Brook, NY, United States)
Leroux, H.
(Lille-1 Univ. Villeneuve-d'Asoq, France)
Tomeoka, K.
(Kobe Univ. Japan)
Zolensky, M.
(NASA Johnson Space Center Houston, TX, United States)
Flynn, T.
(State Univ. of New York Plattsburgh, NY, United States)
Tyliszczak, T.
(California Univ., Lawrence Berkeley National Lab. Berkeley, CA, United States)
Butterworth, A.
(California Univ. Berkeley, CA, United States)
Tomioka, N.
(Kobe Univ. Japan)
Ohnishi, I.
(Kobe Univ. Japan)
Messenger, K. Nakamura
(NASA Johnson Space Center Houston, TX, United States)
Sandford, S.
(NASA Ames Research Center Moffett Field, CA, United States)
Keller, L.
(NASA Johnson Space Center Houston, TX, United States)
Jacobsen, C.
(State Univ. of New York Stony Brook, NY, United States)
Date Acquired
August 24, 2013
Publication Date
January 1, 2007
Subject Category
Astrophysics
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: Houston, TX
Country: United States
Start Date: March 12, 2007
End Date: March 16, 2007
Distribution Limits
Public
Copyright
Public Use Permitted.
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