{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2025,10,12]],"date-time":"2025-10-12T01:25:24Z","timestamp":1760232324686,"version":"build-2065373602"},"reference-count":52,"publisher":"MDPI AG","issue":"21","license":[{"start":{"date-parts":[[2022,10,22]],"date-time":"2022-10-22T00:00:00Z","timestamp":1666396800000},"content-version":"vor","delay-in-days":0,"URL":"https:\/\/creativecommons.org\/licenses\/by\/4.0\/"}],"funder":[{"DOI":"10.13039\/501100012166","name":"National Key R&amp;D Program of China","doi-asserted-by":"publisher","award":["2020YFE0202100","2019YFE0123300","41872207","D020204"],"award-info":[{"award-number":["2020YFE0202100","2019YFE0123300","41872207","D020204"]}],"id":[{"id":"10.13039\/501100012166","id-type":"DOI","asserted-by":"publisher"}]},{"DOI":"10.13039\/501100001809","name":"National Natural Science Foundation of China","doi-asserted-by":"publisher","award":["2020YFE0202100","2019YFE0123300","41872207","D020204"],"award-info":[{"award-number":["2020YFE0202100","2019YFE0123300","41872207","D020204"]}],"id":[{"id":"10.13039\/501100001809","id-type":"DOI","asserted-by":"publisher"}]},{"name":"Pre-research Project on Civil Aerospace Technologies","award":["2020YFE0202100","2019YFE0123300","41872207","D020204"],"award-info":[{"award-number":["2020YFE0202100","2019YFE0123300","41872207","D020204"]}]}],"content-domain":{"domain":[],"crossmark-restriction":false},"short-container-title":["Remote Sensing"],"abstract":"<jats:p>We use multi-source remote sensing data to identify the details of a mascon south-east of the lunar Copernicus crater. Studies of the topography, gravity, geochronology and mineral are combined to prove that the mascon is a buried peak-ring basin with diameters of about 130 km and 260 km. The underground structure is covered by 890 m thick mare basalts, as determined by analyzing the spectral features of the impact crater, Copernicus H. The determination of the crater size\u2013frequency distribution (CSFD) suggests that the impact that created the C-H basin occurred earlier than 3.9 Ga. Then, a Hawaiian-style eruption in the late Imbrian period formed the Sinus Aestuum-I dark mantling deposit (DMD). Soon, mare basalts covered the basin several times from 3.8 Ga. Finally, the ejecta from the Copernicus impact event at about 800 Ma, and the weathering processes caused the disappearance of the C-H basin rim from the lunar surface.<\/jats:p>","DOI":"10.3390\/rs14215284","type":"journal-article","created":{"date-parts":[[2022,10,24]],"date-time":"2022-10-24T10:09:23Z","timestamp":1666606163000},"page":"5284","update-policy":"https:\/\/doi.org\/10.3390\/mdpi_crossmark_policy","source":"Crossref","is-referenced-by-count":1,"title":["Study of the Buried Basin C-H, Based on the Multi-Source Remote Sensing Data"],"prefix":"10.3390","volume":"14","author":[{"ORCID":"https:\/\/orcid.org\/0000-0002-5747-1394","authenticated-orcid":false,"given":"Xiaojian","family":"Xu","sequence":"first","affiliation":[{"name":"School of Land Science and Technology, China University of Geosciences (Beijing), Beijing 100083, China"},{"name":"Research Center of Lunar and Planetary Remote Sensing Exploration, China University of Geosciences (Beijing), Beijing 100083, China"},{"name":"Subcenter of International Cooperation and Research on Lunar and Planetary Exploration, Center of Space Exploration, Ministry of Education of the People\u2019s Republic of China, Beijing 100083, China"}],"role":[{"role":"author","vocabulary":"crossref"}]},{"given":"Teng","family":"Hu","sequence":"additional","affiliation":[{"name":"School of Land Science and Technology, China University of Geosciences (Beijing), Beijing 100083, China"},{"name":"Research Center of Lunar and Planetary Remote Sensing Exploration, China University of Geosciences (Beijing), Beijing 100083, China"},{"name":"Subcenter of International Cooperation and Research on Lunar and Planetary Exploration, Center of Space Exploration, Ministry of Education of the People\u2019s Republic of China, Beijing 100083, China"}],"role":[{"role":"author","vocabulary":"crossref"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-9728-4702","authenticated-orcid":false,"given":"Zhizhong","family":"Kang","sequence":"additional","affiliation":[{"name":"School of Land Science and Technology, China University of Geosciences (Beijing), Beijing 100083, China"},{"name":"Research Center of Lunar and Planetary Remote Sensing Exploration, China University of Geosciences (Beijing), Beijing 100083, China"},{"name":"Subcenter of International Cooperation and Research on Lunar and Planetary Exploration, Center of Space Exploration, Ministry of Education of the People\u2019s Republic of China, Beijing 100083, China"}],"role":[{"role":"author","vocabulary":"crossref"}]},{"given":"Xing","family":"Du","sequence":"additional","affiliation":[{"name":"School of Land Science and Technology, China University of Geosciences (Beijing), Beijing 100083, China"},{"name":"Research Center of Lunar and Planetary Remote Sensing Exploration, China University of Geosciences (Beijing), Beijing 100083, China"},{"name":"Subcenter of International Cooperation and Research on Lunar and Planetary Exploration, Center of Space Exploration, Ministry of Education of the People\u2019s Republic of China, Beijing 100083, China"}],"role":[{"role":"author","vocabulary":"crossref"}]},{"given":"Lin","family":"Zhao","sequence":"additional","affiliation":[{"name":"School of Land Science and Technology, China University of Geosciences (Beijing), Beijing 100083, China"},{"name":"Research Center of Lunar and Planetary Remote Sensing Exploration, China University of Geosciences (Beijing), Beijing 100083, China"},{"name":"Subcenter of International Cooperation and Research on Lunar and Planetary Exploration, Center of Space Exploration, Ministry of Education of the People\u2019s Republic of China, Beijing 100083, China"}],"role":[{"role":"author","vocabulary":"crossref"}]}],"member":"1968","published-online":{"date-parts":[[2022,10,22]]},"reference":[{"key":"ref_1","doi-asserted-by":"crossref","first-page":"181","DOI":"10.1109\/TGRS.2018.2852717","article-title":"Coarse-to-Fine Extraction of Small-Scale Lunar Impact Craters From the CCD Images of the Chang\u2019E Lunar Orbiters","volume":"57","author":"Kang","year":"2019","journal-title":"IEEE Trans. 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