[meteorite-list] Perry to Nininger Letter, June 1, 1951
From: MARK BOSTICK <thebigcollector_at_meteoritecentral.com>
Date: Thu Apr 22 10:31:13 2004 Message-ID: <BAY4-DAV36qUWSGIVpI0000ade9_at_hotmail.com> ------=_NextPart_001_000C_01C41ED1.49F64150 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: quoted-printable (Stuart Perry to Harvey Nininger letter, Perry's File copy) June 1, 1951 Dear Nininger: You must be thinking by this time that I have gone to sleep on the Peru i= ron, but that is not the case. I wanted to have Herbenar's interpretation= of certain structures, and after very long delay I now have the date fro= m him, along with the photos which I am inclosing to you. The iron is very usual, in fact almost anomalous, because it seems to hav= e a definite iron-carbon structure and to contain abundant inclusions of = steadite -- Fe-Fery-Fe-Fe3C-Fe3P eutectite found in artificial irons but = which I have never seen observed in a meteoric iron with the exception of= the small area in Chesterville. Herbenar feels very certain there these strange inclusions are Steadite, = and that this would be confirmed by microchemical analysis -- in other wo= rds by selective etching for carbon and phoephorus. To take up a few of t= he photos - 1, 3 to 8, and others, show the strange looking streadite inclusions. 12 and 14 show the transitory interface of the inclusions and the diffusi= on of the carbon into the kamacite. 8 and 9 show a structure essentially like a sorbitic structure in artific= ial irons, as in heat-treated low-carbon martensite. 16 appears to be essentially a low-carbon martensite. 10 at high magnification shows spheroidize cementite (cohenite) similar t= o that produced by heat treatment of a low carbon martensitic steel. 17, 18, 19 show steadite bodies with a eutectiform structure; a few of th= ese were found. Although we have a long start on this very interesting iron, a good deal = remains to be done before it can be properly and thoroughly described. am= ong the things to be done are: 1. An analysis of the iron itself. 2. Micro-chemical analysis to confirm beyond doubt the apparent steadite = inclusions and the spheroidize carbide. 3. More photomicrographs, perhaps quite a good many of them. These photos= were made by my assistant in Ann Arbor and I just told him to take whate= ver he thought was interesting. He certainly hit the high spots all right= , but there are numerous small inclusions (steadite or perhaps cohenite) = which ought to be taken at both low and high magnification; also plessite= at high magnification to determine whether they have been altered by reh= eating (which presumably produced the streadite); groundmass kamacite at = high magnificatino to determine the nature of heat alteration and the pre= sence or absence of carbon, ect. I expect you will want to publish a thorough description of this importan= t iron, and I should be glad to contribute the metallographic portion of = it. I should not want to do so, however, without the further investigatio= n referred to above. It will take some time, and also some money, perhaps= $100 or $125 altogether for the lab, work at Ann Arbor is somewhat expen= sive. I am wondering whether you would be willing to give me a thin slice off t= he specimen. It is 7/6" thick on one side and 5/16" on the thinner side, = so it ought to be possible to remove a very thin slice, which I could wor= k on to advantage metallographically and which also would furnish materia= l for analysis. The analysis is a "must", so the specimen will have to be= cut somewhere and somehow, and the thin slice would seem to be the best = procedure. I suppose you can easily do that with your own equipment. Kindly return the photos, as I have notations on the backs of some of the= m. Of course you will have a full set of all photos in due time With warm regards, Sincerely, (Stuart Perry - name is missing as this is the file copy. The original se= nt to Nininger would have been signed =20 ------=_NextPart_001_000C_01C41ED1.49F64150 Content-Type: text/html; charset="iso-8859-1" Content-Transfer-Encoding: quoted-printable <HTML><BODY STYLE=3D"font:10pt verdana; border:none;"><DIV><FONT size=3D2= > <P>(Stuart Perry to Harvey Nininger letter, Perry's File copy)</P> <P>J= une 1, 1951</P> <P> </P> <P>Dear Nininger:</P> <P>You must be thinki= ng by this time that I have gone to sleep on the Peru iron, but that is n= ot the case. I wanted to have Herbenar's interpretation of certain struct= ures, and after very long delay I now have the date from him, along with = the photos which I am inclosing to you.</P> <P>The iron is very usual, in= fact almost anomalous, because it seems to have a definite iron-carbon s= tructure and to contain abundant inclusions of steadite -- Fe-Fery-Fe-Fe3= C-Fe3P eutectite found in artificial irons but which I have never seen ob= served in a meteoric iron with the exception of the small area in Chester= ville.</P> <P>Herbenar feels very certain there these strange inclusions = are Steadite, and that this would be confirmed by microchemical analysis = -- in other words by selective etching for carbon and phoephorus. To take= up a few of the photos -</P> <P>1, 3 to 8, and others, show the strange = looking streadite inclusions.</P> <P>12 and 14 show the transitory interf= ace of the inclusions and the diffusion of the carbon into the kamacite.<= /P> <P>8 and 9 show a structure essentially like a sorbitic structure in = artificial irons, as in heat-treated low-carbon martensite.</P> <P>16 app= ears to be essentially a low-carbon martensite.</P> <P>10 at high magnifi= cation shows spheroidize cementite (cohenite) similar to that produced by= heat treatment of a low carbon martensitic steel.</P> <P>17, 18, 19 show= steadite bodies with a eutectiform structure; a few of these were found.= </P> <P>Although we have a long start on this very interesting iron, a go= od deal remains to be done before it can be properly and thoroughly descr= ibed. among the things to be done are:</P> <P>1. An analysis of the iron = itself.</P> <P>2. Micro-chemical analysis to confirm beyond doubt the app= arent steadite inclusions and the spheroidize carbide.</P> <P>3. More pho= tomicrographs, perhaps quite a good many of them. These photos were made = by my assistant in Ann Arbor and I just told him to take whatever he thou= ght was interesting. He certainly hit the high spots all right, but there= are numerous small inclusions (steadite or perhaps cohenite) which ought= to be taken at both low and high magnification; also plessite at high ma= gnification to determine whether they have been altered by reheating (whi= ch presumably produced the streadite); groundmass kamacite at high magnif= icatino to determine the nature of heat alteration and the presence or ab= sence of carbon, ect.</P> <P>I expect you will want to publish a thorough= description of this important iron, and I should be glad to contribute t= he metallographic portion of it. I should not want to do so, however, wit= hout the further investigation referred to above. It will take some time,= and also some money, perhaps $100 or $125 altogether for the lab, work a= t Ann Arbor is somewhat expensive.</P> <P>I am wondering whether you woul= d be willing to give me a thin slice off the specimen. It is 7/6" thick o= n one side and 5/16" on the thinner side, so it ought to be possible to r= emove a very thin slice, which I could work on to advantage metallographi= cally and which also would furnish material for analysis. The analysis is= a "must", so the specimen will have to be cut somewhere and somehow, and= the thin slice would seem to be the best procedure. I suppose you can ea= sily do that with your own equipment.</P> <P>Kindly return the photos, as= I have notations on the backs of some of them. Of course you will have a= full set of all photos in due time</P> <P>With warm regards,</P> <P>Sinc= erely,</P> <P>(Stuart Perry - name is missing as this is the file copy. T= he original sent to Nininger would have been signed </P></FONT></DIV></BO= DY></HTML> ------=_NextPart_001_000C_01C41ED1.49F64150-- Received on Sat 10 Apr 2004 08:56:11 AM PDT |
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