[meteorite-list] FW: Meteorite pairing
From: Matson, Robert <ROBERT.D.MATSON_at_meteoritecentral.com>
Date: Thu Apr 22 10:31:15 2004 Message-ID: <AF564D2B9D91D411B9FE00508BF1C86904EE5B7A_at_US-Torrance.mail.saic.com> This message is in MIME format. Since your mail reader does not understand this format, some or all of this message may not be legible. ------_=_NextPart_001_01C42748.546F7C1C Content-Type: text/plain; charset="iso-8859-1" I'm sending this out again -- evidently it never made the list. Seems to be a common problem lately... --Rob -----Original Message----- From: Matson, Robert Sent: Monday, April 19, 2004 8:29 PM To: 'BOORX4_at_aol.com'; meteorite-list@meteoritecentral.com Subject: Meteorite pairing Hi Bob, > Could some knowledgeable list member please describe or give a definition as to > what "Meteorite Pairing" or "Paired Meteorites" exactly is. I have a vague idea > but would like to have a better understanding. The simplest definition is the process whereby it can be reasonably determined that two or more distinct meteorites or meteorite fragments are part of the same fall -- more specifically, that they were all once part of a single body immediately prior to entering the earth's atmosphere. I can think of at least three ways that one can "pair" meteorites. The most reliable is physical pairing: two fragments that can be unambiguously pieced together. Less reliable is proximity pairing (and in many areas this method is quite unreliable without additional evidence). A third pairing technique is by classification (typically coupled with proximity). The reliability of this method really depends on the rarity of the meteorite type. Two weathered H5s found 50 feet apart is obviously not as reliable as two fresh CV3s found a mile apart. I suppose a 4th method would be based on classification alone, though this would be limited to specimens which have something sufficiently distinctive about them (e.g. a fresh fall like Park Forest would certainly qualify). For common meteorite types (H, L, LL), petrologic grade, weathering, shock, fayalite and ferrosilite percentages generally would not be sufficient. Cheers, Rob ------_=_NextPart_001_01C42748.546F7C1C Content-Type: text/html; charset="iso-8859-1" <!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN"> <HTML><HEAD> <META HTTP-EQUIV="Content-Type" CONTENT="text/html; charset=iso-8859-1"> <META content="MSHTML 6.00.2800.1400" name=GENERATOR></HEAD> <BODY style="FONT-SIZE: 10pt; FONT-FAMILY: Arial; BACKGROUND-COLOR: #ffffff"> <DIV><SPAN class=057003702-21042004>I'm sending this out again -- evidently it never made the list. Seems to be a common</SPAN></DIV> <DIV><SPAN class=057003702-21042004>problem lately... --Rob</SPAN></DIV> <DIV><SPAN class=057003702-21042004></SPAN> </DIV> <DIV class=OutlookMessageHeader dir=ltr align=left><FONT face=Tahoma>-----Original Message-----<BR><B>From:</B> Matson, Robert <BR><B>Sent:</B> Monday, April 19, 2004 8:29 PM<BR><B>To:</B> 'BOORX4_at_aol.com'; meteorite-list_at_meteoritecentral.com<BR><B>Subject:</B> Meteorite pairing<BR><BR></FONT></DIV> <DIV><SPAN class=476331503-20042004>Hi Bob,</SPAN></DIV> <DIV><SPAN class=476331503-20042004></SPAN> </DIV> <DIV><SPAN class=476331503-20042004>> </SPAN>Could some knowledgeable list member please describe or give a definition as to<SPAN class=476331503-20042004> </SPAN></DIV> <DIV><SPAN class=476331503-20042004>></SPAN> what "Meteorite Pairing" or "Paired Meteorites" exactly is. I have a vague idea<SPAN class=476331503-20042004> </SPAN></DIV> <DIV><SPAN class=476331503-20042004>></SPAN> but would like to have a better understanding.<SPAN class=476331503-20042004> </SPAN></DIV> <DIV><SPAN class=476331503-20042004></SPAN> </DIV> <DIV><SPAN class=476331503-20042004>The simplest definition is the process whereby it can be reasonably determined</SPAN></DIV> <DIV><SPAN class=476331503-20042004>that two or more distinct meteorites or meteorite fragments are part of the same</SPAN></DIV> <DIV><SPAN class=476331503-20042004>fall -- more specifically, that they were all once part of a single body immediately</SPAN></DIV> <DIV><SPAN class=476331503-20042004>prior to </SPAN><SPAN class=476331503-20042004>entering the earth's atmosphere.</SPAN></DIV> <DIV><SPAN class=476331503-20042004></SPAN> </DIV> <DIV><SPAN class=476331503-20042004>I can think of at least three ways that one can "pair" meteorites. The most reliable</SPAN></DIV> <DIV><SPAN class=476331503-20042004>is physical pairing: two fragments that can be unambiguously pieced together.</SPAN></DIV> <DIV><SPAN class=476331503-20042004>Less reliable is proximity pairing (and in many areas this method </SPAN><SPAN class=476331503-20042004>is quite</SPAN></DIV> <DIV><SPAN class=476331503-20042004>unreliable without additional evidence). A third pairing technique is by classification</SPAN></DIV> <DIV><SPAN class=476331503-20042004>(typically coupled with proximity). The reliability of this method really </SPAN><SPAN class=476331503-20042004>depends</SPAN></DIV> <DIV><SPAN class=476331503-20042004>on the rarity of the meteorite type. Two weathered H5s found 50 feet apart is</SPAN></DIV> <DIV><SPAN class=476331503-20042004>obviously not as reliable as two fresh CV3s found a mile apart.</SPAN></DIV> <DIV><SPAN class=476331503-20042004></SPAN> </DIV> <DIV><SPAN class=476331503-20042004>I suppose a 4th method would be based on classification alone, </SPAN><SPAN class=476331503-20042004>though this would</SPAN></DIV> <DIV><SPAN class=476331503-20042004>be limited to specimens which have something sufficiently distinctive about them</SPAN></DIV> <DIV><SPAN class=476331503-20042004>(e.g. a fresh fall like Park Forest would certainly qualify). </SPAN><SPAN class=476331503-20042004>For common meteorite</SPAN></DIV> <DIV><SPAN class=476331503-20042004>types (H, L, LL), petrologic grade, weathering, shock, </SPAN><SPAN class=476331503-20042004>fayalite and ferrosilite</SPAN></DIV> <DIV><SPAN class=476331503-20042004>percentages generally would not be sufficient.</SPAN></DIV> <DIV><SPAN class=476331503-20042004></SPAN> </DIV> <DIV><SPAN class=476331503-20042004>Cheers,</SPAN></DIV> <DIV><SPAN class=476331503-20042004>Rob</SPAN></DIV> <DIV><SPAN class=476331503-20042004></SPAN> </DIV></BODY></HTML> ------_=_NextPart_001_01C42748.546F7C1C-- Received on Tue 20 Apr 2004 10:29:12 PM PDT |
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