Kearsley, Anton T. and Borg, Janet and Graham, Giles A. and Burchell, Mark J. and Cole, Mike J. and Leroux, Hugues and Bridges, John C. and Horz, Friedrich and Wozniakiewicz, Penelope J. and Bland, Philip A. and Bradley, John P. and Dai, Zurong and Teslich, Nicholas and See, Thomas A. and Hoppe, Peter and Heck, Philipp and Huth, Joachim and Stadermann, Frank J. and Floss, Christine and Marhas, Kuljeet and Stephan, Thomas and Leitner, Jan (2008) Dust from comet Wild 2: Interpreting particle size, shape, structure, and composition from impact features on the Stardust aluminum foils. Meteoritics & Planetary Science, 43 (1-2). pp. 41-73. ISSN 1086-9379. (doi:https://doi.org/10.1111/j.1945-5100.2008.tb00609.x) (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided)
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Aluminum foils of the Stardust cometary dust collector are peppered with impact features of a wide range of sizes and shapes. By comparison to laboratory shots of known particle dimensions and density, using the same velocity and incidence geometry as the Stardust Wild 2 encounter, we can derive size and mass of the cometary dust grains. Using scanning electron microscopy (SEM) of foil samples (both flown on the mission and impacted in the laboratory) we have recognized a range of impact feature shapes from which we interpret particle density and internal structure. We have documented composition of crater residues, including stoichiometric material in 3 of 7 larger craters, by energy dispersive X-ray microanalysis. Wild 2 dust grains include coarse (>10 mu m) mafic silicate grains, some dominated by a single mineral species of density around 3-4 g cm(-3) (such as olivine). Other grains were porous, low-density aggregates from a few nanometers to 100 mu m, with an overall density that may be lower than I g cm-3, containing mixtures of silicates and sulfides and possibly both alkali-rich and mafic glass. The mineral assemblage is very similar to the most common species reported from aerogel tracks. In one large aggregate crater, the combined diverse residue composition is similar to CI chondrites. The foils are a unique collecting substrate, revealing that the most abundant Wild 2 dust grains were of sub-micrometer size and of complex internal structure. Impact residues in Stardust foil craters will be a valuable resource for future analyses of cometary dust.
|Divisions:||Faculties > Sciences > School of Physical Sciences > Centre for Astrophysics and Planetary Sciences|
|Depositing User:||Jane Griffiths|
|Date Deposited:||22 Apr 2009 11:08 UTC|
|Last Modified:||28 Jan 2016 16:40 UTC|
|Resource URI:||https://kar.kent.ac.uk/id/eprint/15736 (The current URI for this page, for reference purposes)|