[meteorite-list] Impact Melt meteorites
From: tett <tett_at_meteoritecentral.com>
Date: Thu Apr 22 09:47:14 2004 Message-ID: <3BFF9113.85CCFC1D_at_bmts.com> Bernd and List, Are there any good references which describe the visual characteristics of impact melts? A quick glance through Norton's and McSween's books show no references in the indices. I have a few Saharan meteorites which have large gray sections which are very homogeneous showing no visible chondrules. These sections are boarded by distinct chondrule laden sections. What should I look for to determine if these meteorites are in fact impact melts? Cheers, Mike Tettenborn Bernd Pauli HD wrote: > Michel Franco a écrit: > > > ... was wondering if there are 2 main classes of impact > > melt meteorites, as one could think Impact melt m. of > > achondritic origin and impact melt m. of chondritic > > parent body. > > Bonsoir Michel, hello List, > > Here is a database survey of 12 Non-Antarctic meteorites that > are classified as impact melt meteorites. Some new ones may > still be missing from this list as I am not "on track" with my > update chores :-( > > Best wishes, > > Bernd > > Calcalong Creek - LUN - impact melt breccia; > Cat Mountain - L5 - impact melt breccia; vesicles; > Chico - L6 - impact melt breccia; copper; S6; > Dar al Gani 241 - imb - impact melt breccia > Dar al Gani 242 - imb - impact melt breccia > Dhofar 025 - LUN - anorthositic impact melt regolith breccia; > Happy Canyon - EL6 - EL6/7 (S2); impact melt breccia(?); vesicles; > Madrid - L6 - veined; impact melt breccia > Norton County - AUB - fragmental breccia; > clastic matrix (igneous and impact melt) > Roosevelt County 085 - L4 - RC,S4; W2; impact melt > Sahara 00215 - L - W3/4; impact melt breccia; > Shaw - L6 - Dodd: L7; complex impact melt breccia; > > US-Antarctica: > > ALHA81011 - eucritic impact melt breccia > > EET 99443: "The section exhibits isolated pyroxene and plagioclase > grains up to 0.5 mm. The section contains one part in which the > groundmass is finely comminuted pyroxene and plagioclase grains, > while the groundmass in the other is a fine-grained, lath-like > structure suggestive of an i m p a c t m e l t . The meteorite > is a howardite (AMN 24-1, Feb 2001, p. 11). > > MET 00427: "The section shows ...a single millimeter-sized > i m p a c t m e l t spherule. The meteorite is a howardite > (AMN 24-2, September 2001, p. 19). > > QUE 99059 is almost certainly paired with the trio QUE 94204/ > 97348/97289, ... These meteorites are unusual aubrites or > enstatite chondrite impact melt rocks (AMN 24-1, Feb 2001, p. 13). > > References: > > METZLER K. et al. (1994) ALHA81011 - A eucritic impact melt > breccia formed 350 m.y. ago (abs. Meteoritics 29, 1994, 502-503). > > METZLER K. et al. (1995) Impact melt rocks and granulites > from the HED asteroid (abs. Meteoritics 30, 1995, 547). > > Show your support at the Red Cross Disaster Relief Fund - http://s1.amazon.com/exec/varzea/ts/my-pay-page/PKAXFNQH7EKCX/058-5084202-7156648 > _______________________________________________ > Meteorite-list mailing list > Meteorite-list_at_meteoritecentral.com > http://www.pairlist.net/mailman/listinfo/meteorite-list Received on Sat 24 Nov 2001 07:22:43 AM PST |
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