Laboratory production of monophase pyrrhotite grains using solid solid reaction and their characteristic infrared spectra

Details Laboratory production of monophase pyrrhotite grains using solid solid reaction and their characteristic infrared spectra Laboratory production of monophase pyrrhotite grains using solid solid reaction and their characteristic infrared spectra

Sep 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005icar..177..280k&link_type=abstract

Icarus, Volume 177, Issue 1, p. 280-285.

Physics

2

Scientific paper

A new method of producing pyrrhotite grains, which are most commonly found in cometary material and interplanetary dust particles, was developed. Pyrrhotite grains in the monophase having a 7C structure were predominately produced using a solid solid reaction between iron and sulfur grains at room temperature. The characteristic infrared peaks were observed at 602, 563, and 397 cm-1 (16.6, 17.8, and 25.2 μm).

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