Westphal, A.J. and Bastien, R.K. and Borg, J. and Bridges, J. and Brownlee, D.E. and Burchell, M.J. and Cheng, A.F. and Clark, B.C. and Djouadi, Z. and Floss, C. and Franchi, I.A. and Gainsforth, Z. and Graham, G. and Green, S.F. and Heck, P.R. and Horanyi, M. and Hoppe, P. and Horz, F. and Huth, J. and Kearsley, A.T. and Leroux, H. and Marhas, K. and Nakamura-Messenger, K. and Sandford, S.A. and See, T.H. and Stadermann, F.J. and Teslich, N.E. and Tsitrin, S. and Warren, J.L. and Wozniakiewicz, P.J. and Zolensky, M.E. (2008) Discovery of non-random spatial distribution of impacts in the Stardust cometary collector. Meteoritics & Planetary Science, 43 (1-2). pp. 415-429. ISSN 1086-9379. (The full text of this publication is not available from this repository)
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We report the discovery that impacts in the Stardust cometary collector are not distributed randomly in the collecting media, but appear to be clustered on scales smaller than similar to 10 cm. We also report the discovery of at least two populations of oblique tracks. We evaluate several hypotheses that could explain the observations. No hypothesis is consistent with all the observations, but the preponderance of evidence points toward at least one impact on the central Whipple shield of the spacecraft as the origin of both clustering and low-angle oblique tracks. High-angle oblique tracks unambiguously originate from a non-cometary impact on the spacecraft bus just forward of the collector.
|Divisions:||Faculties > Science Technology and Medical Studies > School of Physical Sciences|
|Depositing User:||Louise Dorman|
|Date Deposited:||20 Mar 2009 13:50|
|Last Modified:||24 Jul 2012 14:58|
|Resource URI:||http://kar.kent.ac.uk/id/eprint/15325 (The current URI for this page, for reference purposes)|