火星表面における岩石の風化プロセスと風化生成物
Weathering processes on Martian surface are among the essential issues for both understanding landform evolution and exploring water availability on Martian surface. Studies are reviewed on various weathering processes on Martian surface based on images, data collected by rovers, and laboratory appr...
Published in: | Journal of Geography (Chigaku Zasshi) |
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公益社団法人東京地学協会
2016
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Online Access: | https://tsukuba.repo.nii.ac.jp/record/40446/files/285.pdf |
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fttsukubauniv:oai:tsukuba.repo.nii.ac.jp:00040446 2023-12-31T10:01:22+01:00 火星表面における岩石の風化プロセスと風化生成物 Rock Weathering Processes and Products on Martian Surface SATO, Masato HATTANJI, Tsuyoshi MATSUOKA, Norikazu 佐藤, 昌人 八反地, 剛 ハツタンジ, ツヨシ 松岡, 憲知 マツオカ, ノリカズ 2016 application/pdf https://tsukuba.repo.nii.ac.jp/record/40446/files/285.pdf jpn jpn 公益社団法人東京地学協会 Tokyo Geographical Society 10.5026/jgeography.125.133 http://doi.org/10.5026/jgeography.125.133 http://ci.nii.ac.jp/naid/130005138744/ 地学雑誌 1 125 133 153 Journal of Geography (Chigaku Zasshi) 0022-135X AN00322536 https://tsukuba.repo.nii.ac.jp/record/40446/files/285.pdf 公益社団法人東京地学協会 Tokyo Geographical Society 溶解 塩類風化 凍結破砕 熱破砕 南極 火星 dissolution salt weathering frost weathering thermal cracking Antarctica Mars 2016 fttsukubauniv https://doi.org/10.5026/jgeography.125.133 2023-12-06T19:27:06Z Weathering processes on Martian surface are among the essential issues for both understanding landform evolution and exploring water availability on Martian surface. Studies are reviewed on various weathering processes on Martian surface based on images, data collected by rovers, and laboratory approaches. Recent explorations by the Mars Exploration Rovers reveal that chemical weathering occurs on the surface of basaltic regolith. Dissolution of olivine and oxidation of Fe produces weathering rinds on basaltic surface regolith. Rock interiors also show vugs and veins filled with light-toned efflorescence indicative of chemical weathering. In particular, in high-latitude areas the two Viking landers and the Mars Pathfinder observed honeycomb weathering, angular rock fragments, and polygonal cracks in bedrock. Most of these features are also observed in the Antarctica and other cold deserts on Earth, and are generally attributed to physical weathering such as salt crystallization, thermal weathering, and/or frost weathering. Some studies successfully estimate periods and rates of weathering on the Martian surface, which promote a further understanding of environmental changes and landform evolution. journal article Other/Unknown Material Antarc* Antarctica University of Tsukuba Repository (Tulips-R) Journal of Geography (Chigaku Zasshi) 125 1 133 153 |
institution |
Open Polar |
collection |
University of Tsukuba Repository (Tulips-R) |
op_collection_id |
fttsukubauniv |
language |
Japanese |
topic |
溶解 塩類風化 凍結破砕 熱破砕 南極 火星 dissolution salt weathering frost weathering thermal cracking Antarctica Mars |
spellingShingle |
溶解 塩類風化 凍結破砕 熱破砕 南極 火星 dissolution salt weathering frost weathering thermal cracking Antarctica Mars SATO, Masato HATTANJI, Tsuyoshi MATSUOKA, Norikazu 佐藤, 昌人 八反地, 剛 ハツタンジ, ツヨシ 松岡, 憲知 マツオカ, ノリカズ 火星表面における岩石の風化プロセスと風化生成物 |
topic_facet |
溶解 塩類風化 凍結破砕 熱破砕 南極 火星 dissolution salt weathering frost weathering thermal cracking Antarctica Mars |
description |
Weathering processes on Martian surface are among the essential issues for both understanding landform evolution and exploring water availability on Martian surface. Studies are reviewed on various weathering processes on Martian surface based on images, data collected by rovers, and laboratory approaches. Recent explorations by the Mars Exploration Rovers reveal that chemical weathering occurs on the surface of basaltic regolith. Dissolution of olivine and oxidation of Fe produces weathering rinds on basaltic surface regolith. Rock interiors also show vugs and veins filled with light-toned efflorescence indicative of chemical weathering. In particular, in high-latitude areas the two Viking landers and the Mars Pathfinder observed honeycomb weathering, angular rock fragments, and polygonal cracks in bedrock. Most of these features are also observed in the Antarctica and other cold deserts on Earth, and are generally attributed to physical weathering such as salt crystallization, thermal weathering, and/or frost weathering. Some studies successfully estimate periods and rates of weathering on the Martian surface, which promote a further understanding of environmental changes and landform evolution. journal article |
author |
SATO, Masato HATTANJI, Tsuyoshi MATSUOKA, Norikazu 佐藤, 昌人 八反地, 剛 ハツタンジ, ツヨシ 松岡, 憲知 マツオカ, ノリカズ |
author_facet |
SATO, Masato HATTANJI, Tsuyoshi MATSUOKA, Norikazu 佐藤, 昌人 八反地, 剛 ハツタンジ, ツヨシ 松岡, 憲知 マツオカ, ノリカズ |
author_sort |
SATO, Masato |
title |
火星表面における岩石の風化プロセスと風化生成物 |
title_short |
火星表面における岩石の風化プロセスと風化生成物 |
title_full |
火星表面における岩石の風化プロセスと風化生成物 |
title_fullStr |
火星表面における岩石の風化プロセスと風化生成物 |
title_full_unstemmed |
火星表面における岩石の風化プロセスと風化生成物 |
title_sort |
火星表面における岩石の風化プロセスと風化生成物 |
publisher |
公益社団法人東京地学協会 |
publishDate |
2016 |
url |
https://tsukuba.repo.nii.ac.jp/record/40446/files/285.pdf |
genre |
Antarc* Antarctica |
genre_facet |
Antarc* Antarctica |
op_relation |
10.5026/jgeography.125.133 http://doi.org/10.5026/jgeography.125.133 http://ci.nii.ac.jp/naid/130005138744/ 地学雑誌 1 125 133 153 Journal of Geography (Chigaku Zasshi) 0022-135X AN00322536 https://tsukuba.repo.nii.ac.jp/record/40446/files/285.pdf |
op_rights |
公益社団法人東京地学協会 Tokyo Geographical Society |
op_doi |
https://doi.org/10.5026/jgeography.125.133 |
container_title |
Journal of Geography (Chigaku Zasshi) |
container_volume |
125 |
container_issue |
1 |
container_start_page |
133 |
op_container_end_page |
153 |
_version_ |
1786799612182396928 |