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Lunar farside Th distribution measured by Kaguya gamma-ray spectrometer
https://repo.qst.go.jp/records/47010
https://repo.qst.go.jp/records/4701049d40661-e38c-4094-8cda-113461dd8b45
Item type | 学術雑誌論文 / Journal Article(1) | |||||
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公開日 | 2014-12-24 | |||||
タイトル | ||||||
タイトル | Lunar farside Th distribution measured by Kaguya gamma-ray spectrometer | |||||
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 | |||||
アクセス権 | ||||||
アクセス権 | metadata only access | |||||
アクセス権URI | http://purl.org/coar/access_right/c_14cb | |||||
著者 |
Kobayashi, S.
× Kobayashi, S.× Karouji, Y.× Morota, T.× Takeda, H.× Hasebe, N.× Hareyama, M.× Kobayashi, M.× Shibamura, E.× Yamashita, N.× C., d’Uston× Gasnault, O.× Forni, O.× Reedy, R.C.× Kim, K.J.× 小林 進悟 |
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抄録 | ||||||
内容記述タイプ | Abstract | |||||
内容記述 | Kaguya gamma-ray spectrometer measured thorium (Th) distribution on the lunar farside with the highest sensitivity among past gamma-ray remote sensing missions. The newly obtained Th map has revealed that two regions near the equator on the farside have the lowest Th abundances. We found that the variation of the Th abundance perfectly correlates with the crustal thickness in the farside and the southern nearside, and it could be a result of the crystallization of the lunar magma ocean. | |||||
書誌情報 |
Earth and Planetary Science Letters 巻 337/338, p. 10-16, 発行日 2012-07 |
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出版者 | ||||||
出版者 | Elsevier | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 0012-821X |