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Re: Dimmitt
- To: Sharkkb8@aol.com, Meteorite List <meteorite-list@meteoritecentral.com>
- Subject: Re: Dimmitt
- From: Bernd Pauli HD <bernd.pauli@lehrer1.rz.uni-karlsruhe.de>
- Date: Fri, 02 Apr 1999 00:15:38 +0200
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- References: <25a18c5.37033596@aol.com>
- Resent-Date: Thu, 1 Apr 1999 18:12:08 -0500 (EST)
- Resent-From: meteorite-list@meteoritecentral.com
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Sharkkb8@aol.com schrieb:
> Bernd: Hah! Beat ya! ;>)
A resounding bravo from someone who was out in the garden on a beautiful
spring day and came back with countless thorns of roses and scratches
thereof on his skin :-)
KEIL K. et al. (1990) The Olton, Texas, H chondrite regolith breccia:
Paired with Dimmitt (Meteoritics 25-4, 1990, 259-261, excerpt):
Pairing of chondritic meteorites is difficult, because of a lack of
unequivocal pairing characteristics. We suggest that Olton is paired
with Dimmitt, but it should be noted that the Dimmitt strewnfield has
also yielded numerous specimens of an H3-4, brecciated chondrite called
Tulia (a) [Tulia (b) is an L6 chondrite clearly not paired with Olton;
Graham et al., 1985]. Apparently, Tulia (a) is not paired with Olton,
because it does not contain solar wind-implanted noble gases (Taylor and
Heymann, 1969). This, however, is a single analysis (Schultz and Kruse,
1989) that could by chance be of a solar gas-poor area of Tulia (a);
additional measurements should be carried out before one can be certain
that this meteorite is devoid of such gases.
Best regards,
Bernd
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