Mid-Infrared Spectrum of the Zodiacal Light Observed with AKARI/IRC

被引：0

作者：

Ootsubo, Takafumi ^{[1
]}

Ueno, Munetaka ^{[1
]}

Ishiguro, Masateru ^{[2
]}

Usui, Fumihiko ^{[1
]}

Pyo, Jeonghyun ^{[3
]}

Hong, Seung Soo ^{[3
]}

Kwon, Suk Minn ^{[4
]}

Mukai, Tadashi ^{[5
]}

机构：

[1] JAXA, ISAS, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 2298510, Japan

[2] Natl Astron Observ Japan, Tokyo, Japan

[3] Seoul Natl Univ, Seoul, South Korea

[4] Kangwon Natl Univ, Kangwon, South Korea

[5] Kobe Univ, Kobe, Hyogo, Japan

来源：

AKARI, A LIGHT TO ILLUMINATE THE MISTY UNIVERSE | 2009年 / 418卷

关键词：

INTERPLANETARY DUST; EMISSION; COBE;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present three spectra of the zodiacal light observed in mid-infrared wavelength region with Infrared Camera (MC) on board AKARI The IRC spectra (5.5-12.5 mu m) show an excess emission feature in 9-11 mu m which can be reasonably accounted for by a combination of amorphous and crystalline silicate. The MC observation suggests the presence of crystalline silicate features (9.3 and 11.35 mu m) in the zodiacal light spectrum, indicating that pyroxene-rich anhydrous chondritic porous interplanetary dust particle-like dust may be one of major sources for the small (< 10 mu m) interplanetary dust particles.

引用

页码：395 / +

页数：2

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