WEKO3
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Timing and Characteristics of the Latest Mare Eruption on the Moon
https://jaxa.repo.nii.ac.jp/records/20311
https://jaxa.repo.nii.ac.jp/records/20311e06f4450-68ef-4d37-a71c-fb7cfac973e4
Item type | 会議発表論文 / Conference Paper(1) | |||||
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公開日 | 2015-03-26 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Timing and Characteristics of the Latest Mare Eruption on the Moon | |||||
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_5794 | |||||
資源タイプ | conference paper | |||||
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 |
諸田, 智克
× 諸田, 智克× 春山, 純一× 大竹, 真紀子× 松永, 恒雄× 本田, 親寿× 横田, 康弘× 木村, 淳× 小川, 佳子× 平田, 成× 出村, 裕英× 岩崎, 晃× 杉原, 孝充× 佐伯, 和人× 中村, 良介× 小林, 進悟× Morota, Tomokatsu× Haruyama, Junichi× Otake, Makiko× Matsunaga, Tsuneo× Honda, Chikatoshi× Yokota, Yasuhiro× Kimura, Jun× Ogawa, Yoshiko× Hirata, Naru× Demura, Hirohide× Iwasaki, Akira× Sugihara, Takamitsu× Saiki, Kazuto× Nakamura, Ryosuke× Kobayashi, Shingo |
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著者所属 | ||||||
宇宙航空研究開発機構 (JAXA) | ||||||
著者所属 | ||||||
宇宙航空研究開発機構 (JAXA) | ||||||
著者所属 | ||||||
宇宙航空研究開発機構 (JAXA) | ||||||
著者所属 | ||||||
国立環境研究所 | ||||||
著者所属 | ||||||
会津大学 | ||||||
著者所属 | ||||||
国立環境研究所 | ||||||
著者所属 | ||||||
北海道大学 | ||||||
著者所属 | ||||||
会津大学 | ||||||
著者所属 | ||||||
会津大学 | ||||||
著者所属 | ||||||
会津大学 | ||||||
著者所属 | ||||||
東京大学 | ||||||
著者所属 | ||||||
海洋研究開発機構 | ||||||
著者所属 | ||||||
大阪大学大学 | ||||||
著者所属 | ||||||
産業技術総合研究所 | ||||||
著者所属 | ||||||
宇宙航空研究開発機構 (JAXA) | ||||||
著者所属(英) | ||||||
en | ||||||
Japan Aerospace Exploration Agency (JAXA) | ||||||
著者所属(英) | ||||||
en | ||||||
Japan Aerospace Exploration Agency (JAXA) | ||||||
著者所属(英) | ||||||
en | ||||||
Japan Aerospace Exploration Agency (JAXA) | ||||||
著者所属(英) | ||||||
en | ||||||
National Institute for Environmental Studies (NIES) | ||||||
著者所属(英) | ||||||
en | ||||||
University of Aizu | ||||||
著者所属(英) | ||||||
en | ||||||
National Institute for Environmental Studies (NIES) | ||||||
著者所属(英) | ||||||
en | ||||||
Hokkaido University | ||||||
著者所属(英) | ||||||
en | ||||||
University of Aizu | ||||||
著者所属(英) | ||||||
en | ||||||
University of Aizu | ||||||
著者所属(英) | ||||||
en | ||||||
University of Aizu | ||||||
著者所属(英) | ||||||
en | ||||||
University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
Japan Agency for Marine-Earth Science and Technology (JAMSTEC) | ||||||
著者所属(英) | ||||||
en | ||||||
Osaka University | ||||||
著者所属(英) | ||||||
en | ||||||
National Institute of Advanced Industrial Science and Technology | ||||||
著者所属(英) | ||||||
en | ||||||
Japan Aerospace Exploration Agency (JAXA) | ||||||
出版者 | ||||||
出版者 | 宇宙航空研究開発機構宇宙科学研究所 (JAXA)(ISAS) | |||||
出版者(英) | ||||||
出版者 | Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) | |||||
書誌情報 |
第43回月・惑星シンポジウム en : Proceedings of the 43th ISAS Lunar and Planetary Symposium 巻 43, 発行日 2010-08 |
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会議概要(会議名, 開催地, 会期, 主催者等) | ||||||
内容記述タイプ | Other | |||||
内容記述 | 第43回月・惑星シンポジウム (2010年8月4-6日. 宇宙航空研究開発機構宇宙科学研究所), 相模原市, 神奈川県 | |||||
会議概要(会議名, 開催地, 会期, 主催者等)(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | 43rd ISAS Lunar and Planetary Symposium (August 4-6, 2010. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)), Sagamihara, Kanagawa Japan | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Unraveling the timing and duration of mare volcanism on the Moon is essential for understanding its thermal evolution. The end of mare volcanism is poorly constrained, because mare basalts are incompletely sampled. In this study, employing SELENE (Kaguya) high-resolution images, we performed new crater size-frequency measurements for 49 young mare units (<ca.3.0 Ga) in the Procellarum KREEP Terrane (PKT), in which the latest magma eruption of the Moon occurred. Mare volcanism in this region continued until ca.1.5 Ga, suggesting that volcanic activity in this region ceased ca.1.0 Ga after the magma eruption had globally ceased 2.5-3.0 Ga. Volcanic activity may have peaked 1.8-2.2 Ga ago. The youngest basalts occur around the Aristarchus plateau and the Kepler crater, which are located in the central region of the PKT. It is likely that heating in the crust due to the concentration of heat-producing elements in the PKT delayed cooling of a partial-melting zone in the underlying mantle. | |||||
内容記述 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 著者人数: 18人 | |||||
内容記述 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 形態: カラー図版あり | |||||
内容記述(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Number of authors: 18 | |||||
内容記述(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Physical characteristics: Original contains color illustrations | |||||
書誌レコードID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA12268968 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0065116001 |