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Using a one-dimensional thermal evolution model, we show that core-mantle friction can sustain global-scale partial melting in the upper lunar mantle until \u223c3.1 Ga, thus accounting for the intense volcanic activity on the Moon before \u223c3.0 Ga. Besides, core-mantle friction tends to suppress the secular cooling of the lunar core and is unlikely to be an energy source for the long-lived lunar core dynamo. Our model also favours the transition of the Cassini state before the end of the lunar magma ocean phase (\u223c4.2 Ga), which implies a decreasing lunar obliquity over time after the solidification of the lunar magma ocean. Such a trend of lunar obliquity evolution may allow volcanically released water to be buried in the lunar regolith of the polar regions. As a consequence, local water ice could be more abundant than previously thought when considering only its accumulation caused by solar wind and comet spreading.<\/jats:p>","DOI":"10.1093\/nsr\/nwad276","type":"journal-article","created":{"date-parts":[[2023,11,6]],"date-time":"2023-11-06T16:41:27Z","timestamp":1699288887000},"source":"Crossref","is-referenced-by-count":4,"title":["Long-lived lunar volcanism sustained by precession-driven core-mantle friction"],"prefix":"10.1093","volume":"11","author":[{"ORCID":"https:\/\/orcid.org\/0000-0003-0538-5643","authenticated-orcid":false,"given":"Shuoran","family":"Yu","sequence":"first","affiliation":[{"name":"State Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology , Macau 999078 , 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Germany"}],"role":[{"role":"author","vocabulary":"crossref"}]},{"given":"Jun","family":"Huang","sequence":"additional","affiliation":[{"name":"Planetary Science Institute, State Key Laboratory of Geological Processes and Mineral Resources, School of Earth Sciences, China University of Geosciences , Wuhan 430074 , China"}],"role":[{"role":"author","vocabulary":"crossref"}]},{"ORCID":"https:\/\/orcid.org\/0000-0001-9019-5304","authenticated-orcid":false,"given":"Doris","family":"Breuer","sequence":"additional","affiliation":[{"name":"Institute of Planetary Research, German Aerospace Centre (DLR) , Berlin 12489 , Germany"}],"role":[{"role":"author","vocabulary":"crossref"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-5271-8554","authenticated-orcid":false,"given":"Long","family":"Xiao","sequence":"additional","affiliation":[{"name":"Planetary Science Institute, State Key Laboratory of Geological Processes and Mineral Resources, School of Earth Sciences, China University of Geosciences , Wuhan 430074 , China"}],"role":[{"role":"author","vocabulary":"crossref"}]},{"given":"Dongdong","family":"Ni","sequence":"additional","affiliation":[{"name":"State Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology , Macau 999078 , China"}],"role":[{"role":"author","vocabulary":"crossref"}]}],"member":"286","published-online":{"date-parts":[[2023,10,31]]},"reference":[{"key":"2024020711472268600_bib1","doi-asserted-by":"publisher","first-page":"5056","DOI":"10.1029\/2002JE001985","article-title":"Ages and stratigraphy of mare basalts in Oceanus Procellarum, Mare Nubium, Mare Cognitum, and Mare Insularum","volume":"108","author":"Hiesinger","year":"2003","journal-title":"J Geophys Res Planets"},{"key":"2024020711472268600_bib2","doi-asserted-by":"publisher","first-page":"959","DOI":"10.1111\/j.1945-5100.1998.tb01703.x","article-title":"The case for an imbrium origin of the Apollo thorium-rich impact-melt 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