[meteorite-list] Bull's-eye chondrule assumptions (& New Meteorite Atlas)
From: Jeff Grossman <jgrossman_at_meteoritecentral.com>
Date: Wed May 4 08:58:43 2005 Message-ID: <5.1.0.14.2.20050504085623.029e5418_at_gsvaresm02.er.usgs.gov> No, just dissolution of glass (and partial replacement by clay minerals). At 08:50 AM 5/4/2005, Gerald Flaherty wrote: >Hi Jeff and List, >Jeff you use the term bleaching, is that an oxidation process? >Jerry Flaherty >----- Original Message ----- From: "Jeff Grossman" <jgrossman_at_usgs.gov> >To: <Meteorite-list_at_meteoritecentral.com> >Sent: Wednesday, May 04, 2005 8:30 AM >Subject: Re: [meteorite-list] Bull's-eye chondrule assumptions (& New >Meteorite Atlas) > > >>Oh, I didn't see the other question in this thread. The "bites" out of >>"pac-man" chondrules can have one of two origins. The most popular >>explanation is that the chondrule underwent a low-velocity collision with >>another chondrule during the time in its cooling history when it was >>mostly crystallized but still warm and plastic. However, a much better >>explanation for some of these, including the ones in some of your photos >>I think, is that the chondrule originally contained a significant amount >>of Fe-Ni metal and/or FeS. This formed a round bead when the chondrule >>was cooling and migrated to the surface due to centrifugal force as the >>chondrule was spinning. At some point after the chondrule solidified, >>the metal/sulfide bead was lost. There is a picture of a chondrule that >>still has the metal bead in place in a paper I wrote 20 years back >>(Grossman & Wasson 1985, GCA 49, 925-939, The origin and history of the >>metal and sulfide components of chondrules). >> >>Whichever reason for the "crater" is correct, bleaching occurred on the >>parent asteroid, following the contours of the crater. >> >>Jeff >> >>At 03:32 AM 5/4/2005, Jeff Kuyken wrote: >>>I was just going through my emails and found this one. Well, I have just >>>received Marvin Killgore's new "A Color Atlas of Meteorites in Thin Section" >>>from Mike Jensen. I highly recommend this book which has numerous fantastic >>>images of MANY different meteorite types. >>> >>>One of the things I noticed was that a few of the meteorites presented >>>actually have Bull's-eye chondrules. For those of you who may have purchased >>>this book, the page references I have found so far include: >>> >>>NWA 487 (L/LL3.2) P20-23 >>>LEW 86018 (L3.1) P44-47 >>>ALH 77176 (L3.2) P48-51 (Remnant/Damaged) >>>QUE 97008 (L3.4) 56-57 >>>LEW 87284 (L3.6) P64-67 >>>ALH 85033 (L4) P72-73 >>>GOLD BASIN (L4) P76-79 (Remnant/Weathered) >>>MOUNT TAZERAIT (L5) P80-81 >>> >>>Any thoughts? >>> >>>Jeff >>> >>> >>>----- Original Message ----- >>>From: bernd.pauli_at_paulinet.de >>>To: Meteorite-list_at_meteoritecentral.com >>>Sent: Thursday, March 17, 2005 7:48 AM >>>Subject: [meteorite-list] Bull's-eye chondrule assumptions >>> >>> >>>John and Dawn wrote: >>> >>> > We seem to have several of them in our new LL3 >>> >>>Christian responded and presented some stunning pictures: >>> >>> > I have many of them: ... >>> >>>Whereupon John and Dawn wrote: >>> >>> > I really liked NWA 1770 >>> >>>I am in love with the perfect bull's eye in Christian's NWA 724! >>> >>> > www.austromet.com/collection/NWA_0724_5.646g.jpg >>> >>>Do I have any ideas on the formation of such chondrules? >>> >>>Only some ideas, no references, no direct links: These chondrules >>>obviously occur only in unequilibrated chondrites of types H3.x, >>>L3.x, and LL3.x (by inference probably also in some E3 chondrites), >>>up to petrologic type 4. >>> >>>Darker core material seems to be enveloped by a lighter-colored, in >>>some cases almost concentric ring of (fine-grained, dusty?) material. >>> >>>The process that gave birth to such chondrules may have been either >>>accretionary or condensational and the environment may have been >>>dusty (which would point to early solar system processes). >>> >>>Obviously only a limited number of chondrules underwent this process >>>so that the bull's-eye chondrule formation may have been a selective >>>process (time, distance from the protosun, dusty environment..I don't >>>know). >>> >>>It would be interesting and helpful if someone detected such bull's-eye >>>chondrules in one of their thin sections so that we could draw further >>>conclusions on their mineralic compositions (core material, rim or seam >>>(?) material, high-temperature, low-temperature phases, etc.). >>> >>>Esteemed list member Jeff Grossman wrote several papers on chondrule >>>formation, chondrule composition, zoned chondrules, etc. Maybe he can >>>enlighten us on these "Eyes of Taurus", the Bull, my Constellation :-) >>> >>>Best wishes, >>> >>>Bernd >>> >>>______________________________________________ >>>Meteorite-list mailing list >>>Meteorite-list_at_meteoritecentral.com >>>http://six.pairlist.net/mailman/listinfo/meteorite-list >>> >>>______________________________________________ >>>Meteorite-list mailing list >>>Meteorite-list_at_meteoritecentral.com >>>http://six.pairlist.net/mailman/listinfo/meteorite-list >> >>______________________________________________ >>Meteorite-list mailing list >>Meteorite-list_at_meteoritecentral.com >>http://six.pairlist.net/mailman/listinfo/meteorite-list Received on Wed 04 May 2005 08:58:40 AM PDT |
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