[meteorite-list] Clay meteorites?
From: Laurence Garvie <lgarvie_at_meteoritecentral.com>
Date: Fri, 15 Oct 2010 21:00:09 -0700 Message-ID: <E61EDE8A-DDA6-4800-8389-F27613953023_at_cox.net> Using the definition that clays are phyllosilicate minerals with a grain size of <2 microns, then we already have lots of clay meteorites. The clay contents of the matrices of the CM2 meteorites is on the order of 70 to 80 vol% (see K.T. Howard, G.K. Benedix, P.A. Bland a,b, G. Cressey (2009) Modal mineralogy of CM2 chondrites by X-ray diffraction (PSD-XRD). Part 1: Total phyllosilicate abundance and the degree of aqueous alteration. Geochimica et Cosmochimica Acta, vol 73, 4576-4589) and Orgueil around 80 vols % clay composed of serpentine and serpentine-saponite (see Philip A. BLAND, Gordon CRESSEY, and Olwyn N. MENZIES (2004) Modal mineralogy of carbonaceous chondrites by X-ray diffraction and M?ssbauer spectroscopy, Meteoritics and Planetary Science, vol. 39, 3-16). Laurence Garvie CMS ASU > Message: 1 > Date: Fri, 15 Oct 2010 09:01:27 -0700 (PDT) > From: Robert Verish <bolidechaser at yahoo.com> > Subject: [meteorite-list] Clay meteorites? > To: Meteorite-list Meteoritecentral > <meteorite-list at meteoritecentral.com> > Message-ID: <972507.79052.qm at web51705.mail.re2.yahoo.com> > Content-Type: text/plain; charset=us-ascii > > After reading this article, I have a question: > Do we have to keep an open mind to the possibility of finding a "clay meteorite"? > -- Bob V. > > <http://blogs.nationalgeographic.com/blogs/news/breakingorbit/2010/10/geminids-meteor-shower-driven-by-exploding-clays.html> > > Exploding Clays Drive Geminids Sky Show? > > ++++++++ > If the Geminids are the spawn of Pallas, their meteorites could teach us a lot about that huge and hard-to-reach parent body. > > "Pallas is second largest asteroid [by volume], and we don't know much about it," Campins said. > > "So if we actually have pieces of it that come to the Earth and could be recovered, we would have a free sample-return mission to the asteroid." > --------------------------------------------------------------------- Received on Sat 16 Oct 2010 12:00:09 AM PDT |
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