Dear Meteorite collectors,

I am in the process of working on the bulk mineralogy of Sutter’s Mill as 
determined by powder x-ray diffraction. I have run several samples now, 
including the pre-rain SM3, and found some interesting minerals. My big 
interest is in the clay mineralogy, the quantity and type in each sample I am 
arguing reflects degree of pre-terrestrial heating. I now have a relatively 
good dataset of samples (SM3,41,38,49,65,8,6,12,53), but would dearly like to 
run a few more. There seems to be some gaps in the data with regards to clay 
content and hence heating. I don’t know yet whether this gap reflects the fact 
that I have not looked at enough samples, or is real and is telling us that 
there are two groups of Sutter’s Mill - clay rich (mildly heated), and clay 
poor (heated to high temperature).

So, I am looking for small pieces of samples for my research. Ideally, I am 
looking for donations of small fragments - 100 mg would be perfect, though I 
can still work on samples in the 20 mg range.

If anyone has samples available, then please feel free to email me.

Thanks

Laurence 

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Dr. Laurence A.J. Garvie

Chair, Nomenclature Committee
The Meteoritical Society

Curator
Center for Meteorite Studies

Research Professor
School of Earth and Space Exploration
Arizona State University
email: [email protected]
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