Trigo-Rodriguez, J.M. and Dominguez, G. and Burchell, M.J. and Hoerz, F. and Llorca, J. (2008) Bulbous tracks arising from hypervelocity capture in aerogel. Meteoritics & Planetary Science, 43 (1-2). pp. 75-86. ISSN 1086-9379.
|The full text of this publication is not available from this repository. (Contact us about this Publication)|
The capture of 81P/Wild 2 cometary particles in aerogel with a well-defined impact velocity (6.1 km s(-1)) has provided a wealth of data concerning the composition of Jupiter-family comets. To interpret this data we must understand the capture processes in the aerogel. A major category of tracks are those with bulbous cavities lined with particle fragments. We present a new model to account for the production of these "turnip"-shaped impact cavities. The model uses a thermodynamic approach in order to account for the likely expansion of vapors from particles rich in volatile species. Volume measurements of some of the largest Stardust tracks analysed so far, together with theoretical considerations, indicate that for the majority of Stardust cometary aggregate particle impacts, fragmentation of relatively weak impactors (combined with radial expansion of the resulting subgrains) is the leading cause of bulbous track production, while volatile release of vapors played a secondary role.
|Subjects:||Q Science > QC Physics > QC807 Geophysics (for Applied Geophysics see TN269)|
|Divisions:||Faculties > Science Technology and Medical Studies > School of Physical Sciences > Centre for Astrophysics and Planetary Sciences|
|Depositing User:||Louise Dorman|
|Date Deposited:||09 Apr 1914 17:32|
|Last Modified:||09 Apr 1914 19:03|
|Resource URI:||http://kar.kent.ac.uk/id/eprint/15270 (The current URI for this page, for reference purposes)|
- Depositors only (login required):