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  1. 原著論文

Signatures of volatiles in the lunar proton albedo

https://repo.qst.go.jp/records/48227
https://repo.qst.go.jp/records/48227
a96e513e-a3dd-486e-96f6-a624222623dc
Item type 学術雑誌論文 / Journal Article(1)
公開日 2017-07-27
タイトル
タイトル Signatures of volatiles in the lunar proton albedo
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 A., Schwadron N.

× A., Schwadron N.

WEKO 484528

A., Schwadron N.

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K., Wilson J.

× K., Wilson J.

WEKO 484529

K., Wilson J.

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D., Looper M.

× D., Looper M.

WEKO 484530

D., Looper M.

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P., Jordan A.

× P., Jordan A.

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P., Jordan A.

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E., Spence H.

× E., Spence H.

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E., Spence H.

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B., Blake J.

× B., Blake J.

WEKO 484533

B., Blake J.

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W., Case A.

× W., Case A.

WEKO 484534

W., Case A.

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岩田, 佳之

× 岩田, 佳之

WEKO 484535

岩田, 佳之

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C., Kasper J.

× C., Kasper J.

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C., Kasper J.

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M., Farrell W.

× M., Farrell W.

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M., Farrell W.

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J., Lawrence D.

× J., Lawrence D.

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J., Lawrence D.

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Lovadiotis, G.

× Lovadiotis, G.

WEKO 484539

Lovadiotis, G.

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Mazur, J.

× Mazur, J.

WEKO 484540

Mazur, J.

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Petro, N.

× Petro, N.

WEKO 484541

Petro, N.

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Pieters, C.

× Pieters, C.

WEKO 484542

Pieters, C.

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S., Robinson M.

× S., Robinson M.

WEKO 484543

S., Robinson M.

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Smith, S.

× Smith, S.

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Smith, S.

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W., Townsend L.

× W., Townsend L.

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W., Townsend L.

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Zeitlin, Cary

× Zeitlin, Cary

WEKO 484546

Zeitlin, Cary

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岩田 佳之

× 岩田 佳之

WEKO 484547

en 岩田 佳之

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Zeitlin Cary

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en Zeitlin Cary

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抄録
内容記述タイプ Abstract
内容記述 We find evidence for hydrated material in the lunar regolith using “albedo protons” measured with the Cosmic Ray Telescope for the Effects of Radiation (CRaTER) on the Lunar Reconnaissance Orbiter (LRO). Fluxes of these albedo protons, which are emitted from the regolith due to steady bombardment by high energy radiation (Galactic Cosmic Rays), are observed to peak near the poles, and are inconsistent with the latitude trends of heavy element enrichment (e.g., enhanced Fe abundance). The latitudinal distribution of albedo protons anti-correlates with that of epithermal or high energy neutrons. The high latitude enhancement may be due to the conversion of upward directed secondary neutrons from the lunar regolith into tertiary protons due to neutron–proton collisions in hydrated regolith that is more prevalent near the poles. The CRaTER instrument may thus provide important measurements of volatile distributions within regolith at the Moon and potentially, with similar sensors and observations, at other bodies within the Solar System.
書誌情報 Icarus

巻 273, p. 25-35, 発行日 2016-07
出版者
出版者 Elsevier
DOI
識別子タイプ DOI
関連識別子 10.1016/j.icarus.2015.12.003
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