TY - JOUR
T1 - Laboratory production of monophase pyrrhotite grains using solid-solid reaction and their characteristic infrared spectra
AU - Kimura, Y.
AU - Tamura, K.
AU - Koike, C.
AU - Chihara, H.
AU - Kaito, C.
N1 - Funding Information:
This work was partially supported by grants from JSPS Research Fellowships for Young Scientists from April 2002 to March 2004 and Postdoctoral Fellowships for Research Abroad from April 2004 to March 2006.
PY - 2005/9
Y1 - 2005/9
N2 - 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).
AB - 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).
KW - Infrared observations
KW - Interplanetary dust
KW - Solar nebula
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U2 - 10.1016/j.icarus.2005.03.003
DO - 10.1016/j.icarus.2005.03.003
M3 - Article
AN - SCOPUS:23744485165
VL - 177
SP - 280
EP - 285
JO - Icarus
JF - Icarus
SN - 0019-1035
IS - 1
ER -