[meteorite-list] Nothing political! Just a cool Brachinite micrograph (NWA 3151)
From: STARSANDSCOPES at aol.com <STARSANDSCOPES_at_meteoritecentral.com>
Date: Wed, 29 Oct 2008 12:27:11 EDT Message-ID: <d3b.2cef3324.3639e8df_at_aol.com> Hi list, Greg Hupe has sent me a beautiful NWA 3151 Brachinite Thin Section to examine and image. I have a beautiful shot taken at a magnification of 400X at 8mp. I will send it as an attachment if your Internet provider will carry what works out to about 9mb file size. Email me if you want it sent and let me know if you would prefer it embedded. Embedding reduces the file size to very small and really takes away form the details of the image. A Brachinite is a great material for me to bring this up. The unique structural properties of a Brachinite are best seen at a much lower magnification. I have been told that, for classification purposes, my images should be taken with out a retardation plate, at a much lower magnification and expressed in filed of view size and not magnification level. I know this, but it is my view that classification can not be done by a few photos and (This is the main point) classification has already been done, the colors are more beautiful with a retardation plate, this high magnification level (relative to traditional Xpol work) provides a unique view into the structures within meteorites and finally, more people (including those uninitiated to microscope work) relate to magnification expressed in a level rather than the micron size of the field of view. I am chasing beauty. Some have even called it art. I do not attempt to classify. I have occasionally produced traditional shots for certain people to use in their work but that is not what I am excited to share. So if you want to have a beautiful (full resolution) image of Greg's NWA 3151 Brachinite sent to you, just ask. Tom Phillips **************Plan your next getaway with AOL Travel. Check out Today's Hot 5 Travel Deals! (http://travel.aol.com/discount-travel?ncid=emlcntustrav00000001) Received on Wed 29 Oct 2008 12:27:11 PM PDT |
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