[meteorite-list] L, H what?
From: ROCKS ON FIRE <meteorites_at_meteoritecentral.com>
Date: Thu Apr 22 10:31:11 2004 Message-ID: <406F4C6E.7080600_at_optushome.com.au> --------------090303000002040208040205 Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 7bit Hello, Bernd, as a more or less silent observer of this list I off and on get the urge to put a word in. This time it is time again to thank you for your valueable contributions to the list. It is a privilege to having you back here. Again a wonderful explanation of a criterium which affects more or less all of us. Thanks again, Mate, and keep up the good work! -- Best regards from DOWN-UNDER, Norbert & Heike Kammel ROCKS ON FIRE IMCA #3420 www.rocksonfire.com <%3Fhttp://www.rocksonfire.com%3F> bernd.pauli_at_paulinet.de wrote: >Hello Tom and List, > >Yes, lab testing will probably be the only sure method to classify >a meteorite unambiguously. My NWA 984 (LL4) slice has lots of >easily visible FeNi metal specks, my Saint-Severin (LL6) has lots >of FeNi specks (large and small), my Parnallee (LL3.6) is choke-full >of metallic iron. Same thing with my Tenham (L6) or my Suizhou (L6). > >So "high iron" and "low iron" does not primarily refer to the visible amount >of nickel iron in the matrix. Table 3.3 in D.W. Sears (1978) The Nature and >Origin of Meteorites (Adam Hilger Ltd, Bristol), p. 62 has some interesting >details: > >Principal minerals in chondritic meteorites (wt%) for types 5 and 6: > >Olivine H => 33-37 / Pyroxene => 23-27 / Kamacite (FeNi) => 15-17 >Olivine L => 45-49 / Pyroxene => 21-25 / Kamacite (FeNi) => 06-08 >Olivine LL => 56-60 / Pyroxene => 14-18 / Kamacite (FeNi) => 01-02 > >In words: > >The amount of olivine increases, the amount of pyroxene decreases >as you go from H => L => LL. > >But: > >The total amount of the low-nickel kamacite decreases from H => L => LL >as more and more iron is "oxidized" that is: needed for the silicates. > >Best wishes, > >Bernd > > >______________________________________________ >Meteorite-list mailing list >Meteorite-list_at_meteoritecentral.com >http://www.pairlist.net/mailman/listinfo/meteorite-list > > > --------------090303000002040208040205 Content-Type: multipart/related; boundary="------------040801040707010401040508" --------------040801040707010401040508 Content-Type: text/html; charset=us-ascii Content-Transfer-Encoding: 7bit <!DOCTYPE html PUBLIC "-//W3C//DTD HTML 4.01 Transitional//EN"> <html> <head> <title></title> </head> <body> Hello, Bernd,<br> <br> as a more or less silent observer of this list I off and on get the urge to put a word in.<br> <br> This time <b>it is time again to thank you for your valueable contributions to the list</b>. It is a privilege to having you back here.<br> Again a wonderful explanation of a criterium which affects more or less all of us.<br> <br> Thanks again, Mate, and keep up the good work!<br> -- <br> <div class="moz-signature"> <meta http-equiv="content-type" content="text/html; "> <meta name="author" content="Norbert F. Kammel"> <title>Best_regards</title> <p><font color="#000000">Best regards from DOWN-UNDER,<br> <br> Norbert & Heike Kammel<br> <b> ROCKS ON FIRE</b><br> IMCA #3420</font><br> <a href="%3Fhttp://www.rocksonfire.com%3F">www.rocksonfire.com</a> <br> <img src="http://images.andale.com/f2/113/103/4948211/1028507254564_logosmallerGIF.gif" alt="" width="140" height="85"> </p> </div> <br> <br> <a class="moz-txt-link-abbreviated" href="mailto:bernd.pauli_at_paulinet.de">bernd.pauli@paulinet.de</a> wrote:<br> <blockquote type="cite" cite="midDIIE.0000003900001DB3_at_paulinet.de"> <pre wrap="">Hello Tom and List, Yes, lab testing will probably be the only sure method to classify a meteorite unambiguously. My NWA 984 (LL4) slice has lots of easily visible FeNi metal specks, my Saint-Severin (LL6) has lots of FeNi specks (large and small), my Parnallee (LL3.6) is choke-full of metallic iron. Same thing with my Tenham (L6) or my Suizhou (L6). So "high iron" and "low iron" does not primarily refer to the visible amount of nickel iron in the matrix. Table 3.3 in D.W. Sears (1978) The Nature and Origin of Meteorites (Adam Hilger Ltd, Bristol), p. 62 has some interesting details: Principal minerals in chondritic meteorites (wt%) for types 5 and 6: Olivine H => 33-37 / Pyroxene => 23-27 / Kamacite (FeNi) => 15-17 Olivine L => 45-49 / Pyroxene => 21-25 / Kamacite (FeNi) => 06-08 Olivine LL => 56-60 / Pyroxene => 14-18 / Kamacite (FeNi) => 01-02 In words: The amount of olivine increases, the amount of pyroxene decreases as you go from H => L => LL. But: The total amount of the low-nickel kamacite decreases from H => L => LL as more and more iron is "oxidized" that is: needed for the silicates. Best wishes, Bernd ______________________________________________ Meteorite-list mailing list <a class="moz-txt-link-abbreviated" href="mailto:Meteorite-list_at_meteoritecentral.com">Meteorite-list@meteoritecentral.com</a> <a class="moz-txt-link-freetext" href="http://www.pairlist.net/mailman/listinfo/meteorite-list">http://www.pairlist.net/mailman/listinfo/meteorite-list</a> </pre> </blockquote> <br> <div class="moz-signature"> <p><br> <br> <br> <br> </p> </div> <br> </body> </html> --------------040801040707010401040508-- --------------090303000002040208040205--Received on Sat 03 Apr 2004 06:44:46 PM PST |
StumbleUpon del.icio.us Yahoo MyWeb |