Contractional strains and maximum displacement-length ratios of lunar wrinkle ridges in four Maria of basalt
文献类型：期刊论文
| 作者 | Tariq, Aqil3; Yan, Jianguo2,3; Deng, Qingyun1; Barriot, Jean-Pierre3,5; Abdelrahman, Kamal4 |
| 刊名 | ADVANCES IN SPACE RESEARCH
 |
| 出版日期 | 2024-12-01 |
| 卷号 | 74期号:11页码:6231-6246 |
| 关键词 | Contractional strains Displacement-length ratio Maria Topographic parameters LWRs |
| ISSN号 | 0273-1177 |
| DOI | 10.1016/j.asr.2024.05.057 |
| 产权排序 | 2 |
| 英文摘要 | Compressional stresses from the basalt basins on the lunar are responsible for the formation of wrinkle ridges in lunar mare basalts. According to the wide angle multispectral camera (WAC) mosaic image, we selected 62, 75, 73, and 58 single wrinkle ridges in Mare Imbrium, Mare Serenitatis, Mare Fecunditatis, and Mare Tranquillitatis, respectively, for this paper. Several topographic profiles near the midpoint of each wrinkle ridge are generated to measure the maximum displacement ( D max ) and height of the wrinkle ridges using digital elevation model (LOLA) data. After that, we create 2D plots of displacement-length (L) for the ridge population in the four Maria and compare the results. A linear fit method derives the D max = L ratios (c) from the D-L data. We calculated the contractional strains in each mare area based on the cap D sub m a. x over cap L data. Moreover, each mare's gravity pattern, mare thickness, and formation age are also presented. The ridges in Mare Imbrium and Mare Serenitatis have a higher c value (1.83 x 10-2 and 1.98 x 10-2) than the ridges in Mare Fecunditatis and Mare Tranquillitatis, which have c values of (1.67 x 10-2and 1.75 x 10-2). Finally, the contractional strains (e) in Mare Imbrium, Mare Serenitatis, Mare Fecunditatis, and Mare Tranquillitatis are estimated to be 0.23 %, 0.41 %, 0.39 %, and 0.18 % (considering 25 degrees is the fault plane dip h), respectively. The maximum values of the free-air gravity anomalies in Mare Fecunditatis range from- 30 to 250 mGal, while minimum gravity anomalies in Mare Serenitatis range from- 80 to 140 mGal. Mare Imbrium, Mare Serenitatis, Mare Fecunditatis, and Mare Tranquillitatis have an average thickness of 300 m, 910 m, 652 m, and 760 m, respectively. Furthermore, the Mare Imbrium ridge group is older than the Lunar Wrinkle Ridges in Mare Serenitatis. Mare Tranquillitatis ridge group formation takes longer than Mare Imbrium ridge group formation. Therefore, we believe that it has thicker basaltic units, a longer wrinkle ridge formation time, and higher gravity anomaly than the Mare Imbrium and Mare Serenitatis basins, even though the formation of the Mare Tranquillitatis and Mare Fecunditatis basins occurred earlier. (c) 2024 COSPAR. Published by Elsevier B.V. All rights are reserved, including those for text and data mining, AI training, and similar technologies. |
| WOS关键词 | LOBATE SCARPS ; THRUST FAULTS ; INTERNAL STRUCTURE ; MASCON BASINS ; EVOLUTION ; MOON ; TECTONICS ; TOPOGRAPHY ; MERCURY |
| 资助项目 | National Natural Science Foundation of China[42241116] ; National Natural Science Foundation of China[42030110] ; National Key Research and Development Program of China[2022YFF0503202] ; Project of Xinjiang Uygur Autonomous Region of China for Heaven Lake Talent Program ; King Saud University, Riyadh, Saudi Arabia[RSP2024R351] |
| WOS研究方向 | Engineering ; Astronomy & Astrophysics ; Geology ; Meteorology & Atmospheric Sciences |
| 语种 | 英语 |
| WOS记录号 | WOS:001359129600001 |
| 出版者 | ELSEVIER SCI LTD |
| 资助机构 | National Natural Science Foundation of China ; National Key Research and Development Program of China ; Project of Xinjiang Uygur Autonomous Region of China for Heaven Lake Talent Program ; King Saud University, Riyadh, Saudi Arabia |
| 源URL | [http://ir.xao.ac.cn/handle/45760611-7/7152]  |
| 专题 | 研究单元未命名 |
| 通讯作者 | Yan, Jianguo |
| 作者单位 | 1.Sun Yat Sen Univ, Sch Atmospher Sci, Planetary Environm & Astrobiol Res Lab, Zhuhai 519000, Peoples R China 2.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China 3.Wuhan Univ, State Key Lab Informat Engn Surveying Mapping & Re, Wuhan 430079, Peoples R China 4.King Saud Univ, Coll Sci, Dept Geol & Geophys, Riyadh 11451, Saudi Arabia 5.Univ French Polynesia, Observ Geodes Tahiti, BP 6570, Faaa, Tahiti, France |
| 推荐引用方式 GB/T 7714 | Tariq, Aqil,Yan, Jianguo,Deng, Qingyun,et al. Contractional strains and maximum displacement-length ratios of lunar wrinkle ridges in four Maria of basalt[J]. ADVANCES IN SPACE RESEARCH,2024,74(11):6231-6246. |
| APA | Tariq, Aqil,Yan, Jianguo,Deng, Qingyun,Barriot, Jean-Pierre,&Abdelrahman, Kamal.(2024).Contractional strains and maximum displacement-length ratios of lunar wrinkle ridges in four Maria of basalt.ADVANCES IN SPACE RESEARCH,74(11),6231-6246. |
| MLA | Tariq, Aqil,et al."Contractional strains and maximum displacement-length ratios of lunar wrinkle ridges in four Maria of basalt".ADVANCES IN SPACE RESEARCH 74.11(2024):6231-6246. |
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