Tectonic evolution of northwestern Imbrium of the Moon that lasted in the Copernican Period

• 資料種別: 記事
• タイトル: Tectonic evolution of northwestern Imbrium of the Moon that lasted in the Copernican Period
• 著者・編者: Yuko Daket; Atsushi Yamaji; Katsushi Sato
• 出版事項: 日本 : Springer science+business media
• 出版年月日等: 2016-09-20
• 出版年（W3CDTF）: 2016-09-20
• タイトル（掲載誌）: EPS : Earth, Planets and Space
• 巻号年月日等（掲載誌）: 68(157)
• 掲載巻: 68(157)
• ISSN（掲載誌）: 1880-5981
• ISSN-L（掲載誌）: 1343-8832
• 本文の言語コード: eng
• DOI: 10.1186/s40623-016-0531-0; https://doi.org/10.1186/s40623-016-0531-0
• 国立国会図書館永続的識別子: info:ndljp/pid/10267428; https://dl.ndl.go.jp/pid/10267428
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• 受理日（W3CDTF）: 2017-01-25T12:55:04+09:00
• 保存日（W3CDTF）: 2017-01-13
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• 掲載誌（国立国会図書館永続的識別子）: info:ndljp/pid/9963599; https://dl.ndl.go.jp/pid/9963599
• 連携機関・データベース: 国立国会図書館 : 国立国会図書館デジタルコレクション; https://dl.ndl.go.jp

• 要約等: The formation ages of tectonic structures and their spatial distributions were studied in the northwestern Imbrium and Sinus Iridum regions using images obtained by Terrain Camera and Multiband Imager on board the SELENE spacecraft and the images obtained by Narrow Angle Camera on board LRO. The formation ages of mare ridges are constrained by the depositional ages of mare basalts, which are either deformed or dammed by the ridges. For this purpose, we defined stratigraphic units and determined their depositional ages by crater counting. The degradation levels of craters dislocated by tectonic structures were also used to determine the youngest limits of the ages of the tectonic activities. As a result, it was found that the contractions to form mare ridges lasted long after the deposition of the majority of the mare basalts. There are mare ridges that were tectonically active even in the Copernican Period. Those young structures are inconsistent with the mascon tectonics hypothesis, which attributes tectonic deformations to the subsidence of voluminous basaltic fills. The global cooling or the cooling of the Procellarum KREEP Terrane region seems to be responsible for them. In addition, we found a graben that was active after the Eratosthenian Period. It suggests that the global or regional cooling has a stress level low enough to allow the local extensional tectonics.
• DOI: 10.1186/s40623-016-0531-0; https://doi.org/10.1186/s40623-016-0531-0
• オンライン閲覧公開範囲: インターネット公開
• 著作権情報: © 2016 The Author(s). This article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made.
• 関連情報: Tectonic evolution of northwestern Imbrium of the Moon that lasted in the Copernican Period; https://cir.nii.ac.jp/crid/2120307889360428672
• 関連情報（URI）: http://hdl.handle.net/2433/218904; http://id.ndl.go.jp/digimeta/10267428; https://dl.ndl.go.jp/pid/10267428; http://link.springer.com/content/pdf/10.1186/s40623-016-0531-0.pdf; http://link.springer.com/article/10.1186/s40623-016-0531-0/fulltext.html
• 参照: Investigation of the source region of the lunar-meteorite group with the remote sensing datasets: Implication for the origin of mare volcanism in Mare Imbrium; https://cir.nii.ac.jp/crid/1360857593678352384
• 参照: Compositional and temporal investigation of exposed lunar basalts in the Mare Imbrium region; https://cir.nii.ac.jp/crid/1360011144569948928; Cratering Records in the Inner Solar System in Relation to the Lunar Reference System; https://cir.nii.ac.jp/crid/1360011146020774784; Small-scale lunar graben: Distribution, dimensions, and formation processes; https://cir.nii.ac.jp/crid/1360292619996921216; Global lunar-surface mapping experiment using the Lunar Imager/Spectrometer on SELENE; https://cir.nii.ac.jp/crid/1360292620248292992; Geological constraints on the Precambrian history of Earth's rotation and the Moon's orbit; https://cir.nii.ac.jp/crid/1360292621352407168; Timing and characteristics of the latest mare eruption on the Moon; https://cir.nii.ac.jp/crid/1360567182088618880; Structure and evolution of the lunar Procellarum region as revealed by GRAIL gravity data; https://cir.nii.ac.jp/crid/1360574094215335680; Distribution, Morphology, and Origin of Ridges and Arches in Mare Serenitatis; https://cir.nii.ac.jp/crid/1360574095162451072; Size and morphology of the Chicxulub impact crater; https://cir.nii.ac.jp/crid/1361137043798312192; Deriving the Absolute Reflectance of Lunar Surface Using SELENE (Kaguya) Multiband Imager Data; https://cir.nii.ac.jp/crid/1361137044038480384; The Earth's Variable Rotation; https://cir.nii.ac.jp/crid/1361137045227076736; Fault dislocation modeled structure of lobate scarps from Lunar Reconnaissance Orbiter Camera digital terrain models; https://cir.nii.ac.jp/crid/1361137046522739840; Geologic provinces of the near side of the Moon; https://cir.nii.ac.jp/crid/1361418519025779584; Ages of mare basalts on the lunar nearside; https://cir.nii.ac.jp/crid/1361418519085749376; Measurement and Analysis of Lunar Basin Depths from Clementine Altimetry; https://cir.nii.ac.jp/crid/1361418519486922880; Lunar Mascons: Another Interpretation; https://cir.nii.ac.jp/crid/1361418520530043904; The Geology of Multi-Ring Impact Basins; https://cir.nii.ac.jp/crid/1361418520748267776; Remote Determination of Exposure Degree and Iron Concentration of Lunar Soils Using VIS-NIR Spectroscopic Methods; https://cir.nii.ac.jp/crid/1361699994028489728; Young thrust-fault scarps in the highlands: evidence for an initially totally molten moon; https://cir.nii.ac.jp/crid/1361699995078048384; The Kaguya Mission Overview; https://cir.nii.ac.jp/crid/1361981469918376320; Chinese Mission Ushers in New Era of Lunar Exploration; https://cir.nii.ac.jp/crid/1361981470134879616; Size-Frequency Distributions of Planetary Impact Craters and Asteroids; https://cir.nii.ac.jp/crid/1361981470668608000; Late high‐titanium basalts of the Western Maria: Geology of the Flamsteed REgion of Oceanus Procellarum; https://cir.nii.ac.jp/crid/1361981471009312256; Asymmetric thermal evolution of the Moon; https://cir.nii.ac.jp/crid/1362262943365748096; Evidence of Recent Thrust Faulting on the Moon Revealed by the Lunar Reconnaissance Orbiter Camera; https://cir.nii.ac.jp/crid/1362262945157509504; Terraced depressions in Lunar Maria; https://cir.nii.ac.jp/crid/1362262945309931136; Lunar sinuous rilles: Distribution, characteristics, and implications for their origin; https://cir.nii.ac.jp/crid/1362262945782633856; Small impact craters in the lunar regolith ? Their morphologies, relative ages, and rates of formation; https://cir.nii.ac.jp/crid/1362262945953542016; Abundance and Distribution of Iron on the Moon; https://cir.nii.ac.jp/crid/1362262946273994880; Lunar Mascon Basins: Lava filling, tectonics, and evolution of the lithosphere; https://cir.nii.ac.jp/crid/1362544418937652992; Lunar Reconnaissance Orbiter Camera (LROC) Instrument Overview; https://cir.nii.ac.jp/crid/1362825893525838976; Recent extensional tectonics on the Moon revealed by the Lunar Reconnaissance Orbiter Camera; https://cir.nii.ac.jp/crid/1363107369107162624; Multi-ringed revelation; https://cir.nii.ac.jp/crid/1363388844487968896; Lunar heat flow: Regional prospective of the Apollo landing sites; https://cir.nii.ac.jp/crid/1363388844823812224; Lunar intrusive domes: Morphometric analysis and laccolith modelling; https://cir.nii.ac.jp/crid/1363388846050402176; High‒degree gravity models from GRAIL primary mission data; https://cir.nii.ac.jp/crid/1363670318517801472; Lunar color boundaries and their relationship to topographic features: A preliminary survey; https://cir.nii.ac.jp/crid/1363670320327913088; Lunar Radar Sounder Observations of Subsurface Layers Under the Nearside Maria of the Moon; https://cir.nii.ac.jp/crid/1363670320738631424; Performance and scientific objectives of the SELENE (KAGUYA) Multiband Imager; https://cir.nii.ac.jp/crid/1363670321182837760; Geological features and evolution history of Sinus Iridum, the Moon; https://cir.nii.ac.jp/crid/1363951793311223936; Tectonic patterns on a tidally distorted planet; https://cir.nii.ac.jp/crid/1363951793692587776; Vertical movement in mare basins: Relation to mare emplacement, basin tectonics, and lunar thermal history; https://cir.nii.ac.jp/crid/1363951795646865280; Mapping lunar mare basalt units in mare Imbrium as observed with the Moon Mineralogy Mapper (M³); https://cir.nii.ac.jp/crid/1364233268438433280; Global thrust faulting on the Moon and the influence of tidal stresses; https://cir.nii.ac.jp/crid/1364233269397395200; Stratigraphic sequence and ages of volcanic units in the Gruithuisen region of the Moon; https://cir.nii.ac.jp/crid/1364233270753891840; Lunar Domes; https://cir.nii.ac.jp/crid/1364233271203968000; Geologic map of the Plato Quadrangle of the Moon; https://cir.nii.ac.jp/crid/1880303266584194688
• 連携機関・データベース: 国立情報学研究所 : CiNii Research; https://cir.nii.ac.jp/
• 提供元機関・データベース: 学術機関リポジトリデータベース; https://irdb.nii.ac.jp; 雑誌記事索引データベース; https://ndlsearch.ndl.go.jp; Crossref; https://www.crossref.org; CiNii Articles; 科学研究費助成事業データベース; https://kaken.nii.ac.jp/ja
• 書誌ID（NDLBibID）: 10267428; http://id.ndl.go.jp/bib/10267428
• NII論文ID: 120005997876