[meteorite-list] Range of S.G.Values
From: David Gunning <davidgunning_at_meteoritecentral.com>
Date: Sun, 22 May 2011 09:55:11 -0400 (EDT) Message-ID: <49793.74.209.45.243.1306072511.squirrel_at_webmail.fairpoint.net> Hi All, It's been pointed-out to me in a private email that two of the specific gravity values cited in my recent post may be "suspect". It's been suggested that the Tatahouine specimen "cannot be correct". The reasoning is that "Tata is essentially a pyroxenite with the typical composition of a diogenitic pyroxene of Fe 24, the SG would be at least 3.4." After re-checking I can see that the correct specific gravity value for this specimen is 3.34 and not the 1.43 previously arrived at. Ooops! Thanks to Ted for pointing that out to me. The other "suspect" reading is the "Allende" at 3.47. In rechecking I arrive at the same specific gravity of 3.47 for the "Allende". According to a 2002 paper by Britt and Consolmagno the specific gravity, referred to as the "Grain Density", of the Diogenites ranges between from 3.30 to 3.47. A specific gravity of 3.34 is within that range of values. The same 2002 paper cites the specific gravity of the Carbonaceous Chondrites, including Allende, as having a range of specific gravity values of between from 3.26 to 3.58. At 3.47 the specific gravity of the Allende is within that range of values. There are very few, if any, minerals on earth or from outer space that have a firm and fixed specific gravity value. One that comes to mind is diamond at 3.51, although it, too, can have a slight range of values. The measuring of specific gravity, or "grain density", is a relatively simple and inexpensive way to double check the likelihood that there has been no mix-up in a given meteorite stated sample's pedigree. Respectfully submitted, David Gunning Received on Sun 22 May 2011 09:55:11 AM PDT |
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