Search Results 1-20 of 36

高橋 葵 , 松原 英雄 , 大坪 貴文 , 左近 樹 , 臼井 文彦 , Takahashi Aoi , Matsuhara Hideo , Otsubo Takafumi , Sakon Itsuki , Usui Fumihiko

… The University of Tokyo), Bunkyo-ku, Tokyo, JapanThe 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. … In this study, we analyze mid-infrared spectroscopic data of zodiacal emission at 74 different directions obtained with AKARI/IRC. …

宇宙航空研究開発機構特別資料 = JAXA Special Publication: The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life (JAXA-SP-17-009E), 273-276, 2018-03-09

IR 

石原 大助 , 金田 英宏 , 深川 美里 , 高羽 幸 , 小林 浩 , 藤原 英明 , 大坪 貴文 , Pyo Jeonghyun , 樋口 あや , 尾中 敬 , Ishihara Daisuke , Kaneda Hidehiro , Fukagawa Misato , Takaba Sachi , Kobayashi Hiroshi , Fujiwara Hideaki , Otsubo Takafumi , Pyo Jeonghyun , Higuchi Aya , Onaka Takashi

… The University of Tokyo), Bunkyo-ku, Tokyo, JapanFor the studies of the late stages of the planetary-system formation, the dust-supply and trapping processes observed in exosolar debris disks and the zodiacal dust cloud of our solar system are important clues. … They cannot be simply explained by neither the conventional steady-state collisional cascade process nor transient events such as Giant Impact with rapid dust dissipation. …

宇宙航空研究開発機構特別資料 = JAXA Special Publication: The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life (JAXA-SP-17-009E), 97-100, 2018-03-09

IR 

大坪 貴文 , 臼井 文彦 , 長谷川 直 , 津村 耕司 , 有松 亘 , 石黒 正晃 , Pyo Jeonghyun , 近藤 徹 , 石原 大助 , Otsubo Takafumi , Usui Fumihiko , Matsuura Shuji , Tsumura Koji , Arimatsu Ko , Ishiguro Masateru , Pyo Jeonghyun , Kondo Toru , Ishihara Daisuke

… Ito Hall, the University of Tokyo), Bunkyou-ku, Tokyo, JapanThe zodiacal light (ZL) is the dominant diffuse radiation in the mid-infrared wavelengths from the interplanetary dust. … Although the zodiacal dust cloud has a relatively smooth distribution, it has many small-scale structures, such as asteroidal dust bands and a circumsolar resonance ring. …

宇宙航空研究開発機構特別資料 = JAXA Special Publication: Proceedings of the SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe (JAXA-SP-17-010E), 381-382, 2018-03-09

IR 

Ishihara Daisuke , Takeuchi Nami , Kobayashi Hiroshi , Nagayama Takahiro , Kaneda Hidehiro , Inutsuka Shu-ichiro , Fujiwara Hideaki , Onaka Takashi

… At least nine objectshave a large amount of dust for their ages, which cannot be explained by the conventional steady-state collisional cascade model. …

ASTRONOMY & ASTROPHYSICS (601), A72-A72, 2017-05

IR 

MATUURA Shuji , YANO Hajime , YONETOKU Daisuke , FUNASE Ryu , MORI Osamu , SHIRASAWA Yoji , Solar Sail Working Group

… measurement of the infrared extragalactic background light without foreground contamination of the zodiacal light thanks to low-density environment at deep space, polarization measurement of the gamma-ray burst and accurate determination of its direction based on the interplanetary network technique. …

TRANSACTIONS OF THE JAPAN SOCIETY FOR AERONAUTICAL AND SPACE SCIENCES, AEROSPACE TECHNOLOGY JAPAN 12(ists29), Tr_1-Tr_5, 2014

J-STAGE 

Yamamoto Tetsuo , Minato Tetsunori , Kimura Hiroshi , Mann Ingrid

… Recently, dust disks like the zodiacal dust cloud in our own solar system have commonly been detected around young main-sequence stars. … Dust particles in the disks spiral into the central star within short time scales compared to the duration of the disks due to a drag force as a consequence of the interaction with stellar radiation, which is known as the (electromagnetic) Poynting-Robertson effect. …

Abstracts for fall meeting of the Japanese Society for Planetary Science 2005f(0), 141-141, 2005

J-STAGE 

HIRAO Takanori , MATSUO Hiroshi , MATSUURA Shinji , MURAKAMI Hiroshi , NODA Manabu , OOTSUBO Takafumi , UENO Munetaka

… A few of these stars have been observed precisely at various wavelengths and it was found out that they tend to have hot (～300K) circumstellar dust like the zodiacal dust in our solar system and warm (～50K) dust ring around 30{50 AU from the central star. …

The Institute of Space and Astronautical Science report. S.P. : Mid- and Far-Infrared Astronomy and Future Space Mission (14), 19-25, 2000-12

IR 

Wang Wan Xian , Misconi N. Y.

… This method is beneficial for improving our knowledge of the orbital elements of the asteroids, and perhaps even much smaller effects such as the effects of the planets on the interplanetary dust complex. … Information on the latter may be provided by using this method to investigate Jupiter's effect on the inclination of the symmetry surface of the zodiacal dust cloud. …

Earth, Planets and Space 51(11), 1181-1194, 1999

J-STAGE 

JENNISKENS P.

… Zodiacal dust evolves from cometary debris through a stage called a meteoroid stream. … These stages tie meteoroid streams to cometary dust trails and are an important step in the dynamical evolution from cometary to zodiacal dust. …

Earth, Planets and Space 50(6), 555-567, 1998-07

J-STAGE  References (76)

ISHIGURO M.

Astrophys. J. 511, 432-435, 1998

DOI  Cited by (1)