The Graduate University for Advanced Studies (SOKENDAI) : Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)
The Graduate University for Advanced Studies (SOKENDAI) : Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)
The University of Tokyo
Center for Planetary Science, Graduate School of Science, Kobe University
出版者
宇宙航空研究開発機構(JAXA)
出版者(英)
Japan Aerospace Exploration Agency (JAXA)
雑誌名
宇宙航空研究開発機構特別資料
雑誌名(英)
JAXA Special Publication: The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life
巻
JAXA-SP-17-009E
ページ
273 - 276
発行年
2018-03-09
会議概要(会議名, 開催地, 会期, 主催者等)
第4回「あかり」国際会議 (2017年10月17-20日. 東京大学), 文京区, 東京
会議概要(会議名, 開催地, 会期, 主催者等)(英)
The 4th AKARI International Conference: The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life (October 17-20, 2017. The University of Tokyo), Bunkyo-ku, Tokyo, Japan
抄録(英)
The property of interplanetary dust (IPD), which has been recently emitted from planetesimals like asteroids and/or comets, can give us the information about the environment where asteroids and comets were formed during the planet-formation stage. These can include clues of any planetesimal scattering due to planets' migration. We use silicate features around 10 micrometers as a tracer of the thermal history. In this study, we analyze mid-infrared spectroscopic data of zodiacal emission at 74 different directions obtained with AKARI/IRC. After we examined and subtracted instrumental artifacts, we successfully obtained the high S/N spectra and detected the silicate feature in all pointing data. They also suggest the variations in dust temperature and shape of the feature among different ecliptic latitudes.
内容記述
形態: カラー図版あり
内容記述(英)
Physical characteristics: Original contains color illustrations