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Shock Vaporization/Devolatilization of Evaporitic Minerals, Halite and Gypsum, in an Open System Investigated by a Two‐Stage Light Gas Gun

https://hiroshima.repo.nii.ac.jp/records/2006937
https://hiroshima.repo.nii.ac.jp/records/2006937
2c30cb50-4c22-4d78-80f7-09fb1cca8cbe
名前 / ファイル ライセンス アクション
GeophyResLett_46_7258.pdf GeophyResLett_46_7258.pdf (1.6 MB)
Item type デフォルトアイテムタイプ_(フル)(1)
公開日 2023-03-18
タイトル
タイトル Shock Vaporization/Devolatilization of Evaporitic Minerals, Halite and Gypsum, in an Open System Investigated by a Two‐Stage Light Gas Gun
言語 en
作成者 Kurosawa, Kosuke

× Kurosawa, Kosuke

en Kurosawa, Kosuke

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Moriwaki, Ryota

× Moriwaki, Ryota

en Moriwaki, Ryota

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Komatsu, Goro

× Komatsu, Goro

en Komatsu, Goro

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Okamoto, Takaya

× Okamoto, Takaya

en Okamoto, Takaya

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Sakuma, Hiroshi

× Sakuma, Hiroshi

en Sakuma, Hiroshi

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Yabuta, Hikaru

× Yabuta, Hikaru

en Yabuta, Hikaru

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Matsui, Takafumi

× Matsui, Takafumi

en Matsui, Takafumi

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アクセス権
アクセス権 open access
アクセス権URI http://purl.org/coar/access_right/c_abf2
権利情報
権利情報 An edited version of this paper was published by AGU. Copyright 2019 American Geophysical Union.
内容記述
内容記述 Dry lakebeds might constitute large volatile reservoirs on Mars. Hypervelocity impacts onto ancient dry lakebeds would have affected the volatile distribution on Mars. We developed a new experimental method to investigate the response of evaporitic minerals (halite and gypsum) to impact shocks in an open system. This technique does not result in chemical contamination from the operation of the gas gun. The technique is termed the “two‐valve method," and the gun system is located in the Planetary Exploration Research Center, Chiba Institute of Technology, Japan. We detected the vaporization of halite at 31 GPa and devolatilization from gypsum at 11 GPa, suggesting that impact‐induced volatile release from dry lakebeds has periodically occurred throughout Martian history. The vaporization of halite deposits might have enhanced the production of perchlorates, which are found globally on Mars. The water loss from gypsum possibly explains the coexisting types of Ca‐sulfates found in Gale Crater.
言語 en
内容記述
内容記述タイプ Other
内容記述 This work was supported by ISAS/JAXA as a collaborative program with its Hypervelocity Impact Facility.
出版者
出版者 American Geophysical Union
出版者
出版者 AGU
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
出版タイプ
出版タイプ VoR
出版タイプResource http://purl.org/coar/version/c_970fb48d4fbd8a85
関連情報
識別子タイプ DOI
関連識別子 10.1029/2019GL083249
関連情報
識別子タイプ DOI
関連識別子 https://doi.org/10.1029/2019GL083249
収録物識別子
収録物識別子タイプ ISSN
収録物識別子 0094-8276
収録物識別子
収録物識別子タイプ ISSN
収録物識別子 1944-8007
開始ページ
開始ページ 7258
書誌情報 Geophysical Research Letters
Geophysical Research Letters

巻 46, 号 13, p. 7258-7267, 発行日 2019-07-23
旧ID 48195
備考 Edited version/PDF may be used in an institutional repository after an embargo period of 6 months.
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