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  1. 原著論文

The South Pole-Aitken basin region, Moon: GIS-based geologic investigation using Kaguya elemental information

https://repo.qst.go.jp/records/47008
https://repo.qst.go.jp/records/47008
67e124cb-cbd2-4e3d-958c-c04d091dfc79
Item type 学術雑誌論文 / Journal Article(1)
公開日 2014-12-24
タイトル
タイトル The South Pole-Aitken basin region, Moon: GIS-based geologic investigation using Kaguya elemental information
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 Kim, K.J.

× Kim, K.J.

WEKO 469280

Kim, K.J.

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J.-P., Williams Dohm

× J.-P., Williams Dohm

WEKO 469281

J.-P., Williams Dohm

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Ruiz, J.

× Ruiz, J.

WEKO 469282

Ruiz, J.

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Hare, T.M.

× Hare, T.M.

WEKO 469283

Hare, T.M.

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Hasebe, N.

× Hasebe, N.

WEKO 469284

Hasebe, N.

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Karouji, Y.

× Karouji, Y.

WEKO 469285

Karouji, Y.

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Kobayashi, S.

× Kobayashi, S.

WEKO 469286

Kobayashi, S.

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Hareyama, M.

× Hareyama, M.

WEKO 469287

Hareyama, M.

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Shibamura, E.

× Shibamura, E.

WEKO 469288

Shibamura, E.

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Kobayashi, M.

× Kobayashi, M.

WEKO 469289

Kobayashi, M.

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C., d’Uston

× C., d’Uston

WEKO 469290

C., d’Uston

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Gasnault, O.

× Gasnault, O.

WEKO 469291

Gasnault, O.

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Forni, O.

× Forni, O.

WEKO 469292

Forni, O.

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Maurice, S.

× Maurice, S.

WEKO 469293

Maurice, S.

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小林 進悟

× 小林 進悟

WEKO 469294

en 小林 進悟

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抄録
内容記述タイプ Abstract
内容記述 Using Geographic Information Systems (GIS), we performed comparative analysis among stratigraphic information and the Kaguya (SELENE) GRS data of the ∼2500-km-diameter South Pole-Aitken (SPA) basin and its surroundings. Results indicate that the surface rock materials (including ancient crater materials, mare basalts, and possible SPA impact melt) are average to slightly elevated in K and Th with respect to the rest of the Moon. Also, this study demonstrates that K and Th have not significantly changed since the formation of SPA. The elemental signatures of the impact basin of Fe, Ti, Si, O through time include evidence for resurfacing by ejecta materials and late-stage volcanism. The oldest surfaces of SPA are found to be oxygen-depleted during the heavy bombardment period relative to later stages of geologic development, followed by both an increase in silicon and oxygen, possibly due to ejecta sourced from outside of SPA, and subsequent modification due to mare basaltic volcanism, which increased iron and titanium within SPA. The influence of the distinct geologic history of SPA and surroundings on the mineralogic and elemental abundances is evident as shown in our investigation.
書誌情報 Advances in Space Research

巻 50, 号 12, p. 1629-1637, 発行日 2012-12
出版者
出版者 Elsevier
ISSN
収録物識別子タイプ ISSN
収録物識別子 0273-1177
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