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  1. 学術雑誌論文
  2. 5 技術(工学)

Heliocentric Distance Dependence of Zodiacal Light Observed by Hayabusa2#

http://hdl.handle.net/10228/0002001505
http://hdl.handle.net/10228/0002001505
53720974-58fd-48c4-a2bc-56633f7aeadd
名前 / ファイル ライセンス アクション
LaSEINE-2023_007.pdf LaSEINE-2023_007.pdf (3.8 MB)
Item type 共通アイテムタイプ(1)
公開日 2025-03-25
タイトル
タイトル Heliocentric Distance Dependence of Zodiacal Light Observed by Hayabusa2#
言語 en
著者 Tsumura, Kohji

× Tsumura, Kohji

en Tsumura, Kohji

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Matsuura, Shuji

× Matsuura, Shuji

en Matsuura, Shuji

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佐野, 圭

× 佐野, 圭

WEKO 31407
e-Rad_Researcher 70802908
Scopus著者ID 56708069700
ORCiD 0000-0002-6468-8532
九工大研究者情報 100001400

en Sano, Kei

ja 佐野, 圭

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Iwata, Takahiro

× Iwata, Takahiro

en Iwata, Takahiro

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Yano, Hajime

× Yano, Hajime

en Yano, Hajime

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Kitazato, Kohei

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en Kitazato, Kohei

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Takimoto, Kohji

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en Takimoto, Kohji

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Yamada, Manabu

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en Yamada, Manabu

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Morota, Tomokatsu

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en Morota, Tomokatsu

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Kouyama, Toru

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en Kouyama, Toru

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Hayakawa, Masahiko

× Hayakawa, Masahiko

en Hayakawa, Masahiko

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Yokota, Yasuhiro

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en Yokota, Yasuhiro

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Tatsumi, Eri

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en Tatsumi, Eri

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Matsuoka, Moe

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en Matsuoka, Moe

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Sakatani, Naoya

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en Sakatani, Naoya

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Honda, Rie

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en Honda, Rie

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Kameda, Shingo

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en Kameda, Shingo

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Suzuki, Hidehiko

× Suzuki, Hidehiko

en Suzuki, Hidehiko

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Cho, Yuichiro

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en Cho, Yuichiro

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Yoshioka, Kazuo

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en Yoshioka, Kazuo

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Ogawa, Kazunori

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en Ogawa, Kazunori

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Shirai, Kei

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en Shirai, Kei

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Sawada, Hirotaka

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en Sawada, Hirotaka

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Sugita, Seiji

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en Sugita, Seiji

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抄録
内容記述タイプ Abstract
内容記述 Zodiacal light (ZL) is sunlight scattered by interplanetary dust particles (IDPs) at optical wavelengths. The spatial distribution of IDPs in the Solar System may hold an important key to understanding the evolution of the Solar System and material transportation within it. The number density of IDPs can be expressed as n(r)~r-α, and the exponent α~1.3 was obtained by previous observations from interplanetary space by Helios 1/2 and Pioneer 10/11 in the 1970s and 1980s. However, no direct measurements of α based on ZL observations from interplanetary space outside Earth’s orbit have been performed since then. Here, we introduce initial results for the radial profile of the ZL at optical wavelengths observed over the range 0.76-1.06 au by ONC-T aboard the Hayabusa2# mission in 2021-2022. The ZL brightness we obtained is well reproduced by a model brightness, although there is a small excess of the observed ZL brightness over the model brightness at around 0.9 au. The radial power-law index we obtained is α=1.30±0.08, which is consistent with previous results based on ZL observations. The dominant source of uncertainty arises from the uncertainty in estimating the diffuse Galactic light (DGL).
言語 en
書誌情報 en : Earth, Planets and Space

巻 75, p. 121, 発行日 2023-08-22
出版社
出版者 Springer
キーワード
言語 en
主題Scheme Other
主題 Zodiacal light
キーワード
言語 en
主題Scheme Other
主題 Interplanetary dust
キーワード
言語 en
主題Scheme Other
主題 Hayabusa2#
言語
言語 eng
資源タイプ
資源タイプ識別子 http://purl.org/coar/resource_type/c_6501
資源タイプ journal article
出版タイプ
出版タイプ VoR
出版タイプResource http://purl.org/coar/version/c_970fb48d4fbd8a85
DOI
識別子タイプ DOI
関連識別子 https://doi.org/10.1186/s40623-023-01856-x
査読の有無
値 yes
連携ID
値 14120
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