BCC0001-Plasma
induced stellar grains thermally annealed in Fe dust.
Detail of selected grains from thin
section, wider field of view special setup by Molecular Expressions to
capture grain density-count.Note: With exception to the image at the
very bottom of this page the attempt to capture as many grains as
possible in the images below resulted in an almost full order off
birefringence.
Note the zone of continuous transitional metal dust (darker
band), running from left to right in the two photo micrographs above.
This section represents an area originally rich in volatile components
resulting in an oxidation reduction zone during coagulation and
accretion of the entire stellar grain mass.
Note the multiple crystal component grain in the
center of the above image. Viewing area horizontally approximately 4mm.
XRD Analysis
EDS Analysis
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