[meteorite-list] Capot Rey...photos please of the H5
From: Jeff Kuyken <info_at_meteoritecentral.com>
Date: Fri Sep 23 21:57:32 2005 Message-ID: <008401c5c0ab$5231c060$98598b90_at_mandin4f89ypwu> Hi Martin, I can certainly see what you are saying but that was not really my point. My point is that it is not up to us to 'make-up' classifications without the proper science being done. Admittedly, I've only seen a few photos of the Caopt Rey pieces and in my opinion the one that was just posted by Cartsen is certainly a highly shocked piece but it's not an IMB. I think if you compare them to meteorites like Cat Mountain or Mike Farmer's NWA 2085 you will see what I mean. That said, it is certainly a gorgeous meteorite which I wouldn't mind having a piece myself! ;-) Cheers, Jeff ----- Original Message ----- From: Martin Altmann To: Jeff Kuyken ; meteorite-list_at_meteoritecentral.com Sent: Friday, September 23, 2005 8:18 PM Subject: Re: [meteorite-list] Capot Rey...photos please of the H5 Hi Jeff, as far as I understand the term "IMB" does not name a completely and uniformly molten rock. Else, I would have have problems to understand the "B", if there aren't any fragments of the precessor material to be found in the melt (and I think, we easily will sled into the PAC corner). Different classification of the same find as IMB or H5 f.i. are easily explainable. Take for instance Dho 010, there you have broad streams of melt flowing around chondritic fragments in different stages of melting, some even unaltered, therefore one can determinate the type (have to look Dho 010 if I remember right is H6). And furthermore take our good old Gao! There you have stones, which are simply more or less normal chondrites, other stones show large melt pockets and again others are more or less totally molten and have to be regarded, if one doesn't know about the other average Gao specimens, with no doubt as IMBs. Take a look on David Weir's page, there you have such an example. Thus with Gao we have the whole spectra - H5, H5 with melt, IMB. It's always the same, it depends what for a stone the classificators get, what for sections they do have. Remember the NWA 1109, they caught parts with slightly below 10% Dio, thus it's an EUC-P, another cut, another stone from the same find with >10%, voila they had to call it a How. Take also good old Zag. There exist pieces with only a single lithology, if those would have been handed in for typing, Zag wouldn't have bin classified as regolith breccia. Take the NWA-Rumurutis, some are nice brecciae, result - obviously paired ones (lalalaa I know, I'm not a scientist, but if it's looking the same in every detail and the stuff is so rare) got different classifications. Some R4s are paired with R3-6... Ooops, all I'm writing here, is about the optical, physical appearance of the stones, not chemically. Now, I would guess, with Capot Rey, they took either a piece without melt (if exists) or determinated the type from a not molten fragment in the melt. But look at the phantastic pieces of Carsten, those dark fat rivers of melt around the grey round jigsaw pieces. Hence if Dho 010, who looks the same, but is only much more weathered, was called a IMB, I dare to say in my Lieschen-Mueller-opinion (Lieschen Mueller is the German sister of John Doe), Capot Rey is an IMB too. Of course again we would need a concretion of terms from a qualified mouth. With type-7 vs. PAC vs. IMB we learned, that it has to do with the isotopes and in general nobody is sure about the criteria, now we have IMB vs. MR (melt rock) vs H or L with IMB vs H or L with visible huge parts of melt, but not assigned, or we have to resign ourself to being more types of rock out there in space as we have terms for them :-) Buckleboo! Martin ----- Original Message ----- From: "Jeff Kuyken" <info_at_meteorites.com.au> To: "drtanuki" <drtanuki_at_yahoo.com>; <meteorite-list@meteoritecentral.com> Sent: Friday, September 23, 2005 10:57 AM Subject: Re: [meteorite-list] Capot Rey...photos please of the H5 > I would be a bit cautious about calling something an IMB unless it has been > formally classified as such. My understanding is that this meteorite was > classified as H5 but after further cutting later was found to be highly > shocked. Let's not forget that IMB is basically a scientific term referring > to the fact that the pressure reached about 75-90 GPa and is rated as S6+. > It's original shock rating was only S2. A new piece should probably be > submitted for re-classification so a proper determination can be made. > > Cheers, > > Jeff > > ----- Original Message ----- > From: drtanuki > To: meteorite-list_at_meteoritecentral.com > Sent: Friday, September 23, 2005 9:47 AM > Subject: [meteorite-list] Capot Rey...photos please of the H5 > > > Dear List, > Does anyone have more information about Capot Rey? > It is listed as an H5 in the MetBul and has no mention > of it being an IMB. I would appreciate photos if > someone has them of their samples that were not sold > as an IMB. Thank you in advance. > Sincerely, Dirk Ross...Tokyo > > __________________________________________________ > Do You Yahoo!? > Tired of spam? Yahoo! Mail has the best spam protection around > http://mail.yahoo.com > ______________________________________________ > 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 Fri 23 Sep 2005 09:57:25 PM PDT |
StumbleUpon del.icio.us Yahoo MyWeb |