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Two-stage Development of the Lunar Farside Highlands Crustal Formation
https://repo.qst.go.jp/records/47487
https://repo.qst.go.jp/records/474877771a200-eb64-4777-8bc2-2140e8a4d950
| Item type | 学術雑誌論文 / Journal Article(1) | |||||
|---|---|---|---|---|---|---|
| 公開日 | 2016-08-22 | |||||
| タイトル | ||||||
| タイトル | Two-stage Development of the Lunar Farside Highlands Crustal Formation | |||||
| 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 |
Yamamoto, Keiko
× Yamamoto, Keiko× Haruyama, Junichi× Kobayashi, Shingo× Ohtake, Makiko× Iwata, Takahiro× Ishihara, Yoshiaki× Hasebe, Nobuyuki× 小林 進悟 |
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| 抄録 | ||||||
| 内容記述タイプ | Abstract | |||||
| 内容記述 | The correlation between the spatial patterns of surface Thorium (Th) abundance measured by SELENE GRS data and the crustal thickness from the GRAIL gravity field and LRO LOLA data is investigated in the lunar highland area. Our analysis reveals that there are several areas of local minima for Th abundance exhibiting similar values but different crustal thicknesses. To explain the result, we propose a two-stage scenario for crustal formation. In the first stage, plural thin plateaus form on the surface of the lunar magma ocean (LMO), which corresponds to the observed surface Th distribution. In the second stage, a global crust with dichotomy forms by solidification of the LMO under the plateaus. | |||||
| 書誌情報 |
Planetary and Space Science 巻 120, p. 43-47, 発行日 2015-12 |
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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 | 0032-0633 | |||||
| DOI | ||||||
| 識別子タイプ | DOI | |||||
| 関連識別子 | doi:10.1016/j.pss.2015.11.002 | |||||
