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

Yuki Kimura; K. Tamura; C. Koike; H. Chihara; C. Kaito

doi:10.1016/j.icarus.2005.03.003

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

Yuki Kimura, K. Tamura, C. Koike, H. Chihara, C. Kaito

SCI - Earth Science

Research output: Contribution to journal › Article › peer-review

2 Citations (Scopus)

Abstract

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).

Original language	English
Pages (from-to)	280-285
Number of pages	6
Journal	Icarus
Volume	177
Issue number	1
DOIs	https://doi.org/10.1016/j.icarus.2005.03.003
Publication status	Published - 2005 Sep 1

Keywords

Infrared observations
Interplanetary dust
Solar nebula

ASJC Scopus subject areas

Space and Planetary Science
Astronomy and Astrophysics

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title = "Laboratory production of monophase pyrrhotite grains using solid-solid reaction and their characteristic infrared spectra",

abstract = "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).",

keywords = "Infrared observations, Interplanetary dust, Solar nebula",

author = "Yuki Kimura and K. Tamura and C. Koike and H. Chihara and C. Kaito",

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doi = "10.1016/j.icarus.2005.03.003",

language = "English",

volume = "177",

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TY - JOUR

T1 - Laboratory production of monophase pyrrhotite grains using solid-solid reaction and their characteristic infrared spectra

AU - Kimura, Yuki

AU - Tamura, K.

AU - Koike, C.

AU - Chihara, H.

AU - Kaito, C.

PY - 2005/9/1

Y1 - 2005/9/1

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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DO - 10.1016/j.icarus.2005.03.003

M3 - Article

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VL - 177

SP - 280

EP - 285

JO - Icarus

JF - Icarus

SN - 0019-1035

IS - 1

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