A dry lunar mantle reservoir for young mare basalts of Chang’e-5
The distribution of water in the Moon’s interior carries implications for the origin of the Moon 1 , the crystallization of the lunar magma ocean 2 and the duration of lunar volcanism 2 . The Chang’e-5 mission returned some of the youngest mare basalt samples reported so far, dated at 2.0 billion ye...
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| Veröffentlicht in: | Nature (London) 2021-12, Vol.600 (7887), p.49-53 |
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| creator | Hu, Sen He, Huicun Ji, Jianglong Lin, Yangting Hui, Hejiu Anand, Mahesh Tartèse, Romain Yan, Yihong Hao, Jialong Li, Ruiying Gu, Lixin Guo, Qian He, Huaiyu Ouyang, Ziyuan |
| description | The distribution of water in the Moon’s interior carries implications for the origin of the Moon
1
, the crystallization of the lunar magma ocean
2
and the duration of lunar volcanism
2
. The Chang’e-5 mission returned some of the youngest mare basalt samples reported so far, dated at 2.0 billion years ago (Ga)
3
, from the northwestern Procellarum KREEP Terrane, providing a probe into the spatiotemporal evolution of lunar water. Here we report the water abundances and hydrogen isotope compositions of apatite and ilmenite-hosted melt inclusions from the Chang’e-5 basalts. We derive a maximum water abundance of 283 ± 22 μg g
−1
and a deuterium/hydrogen ratio of (1.06 ± 0.25) × 10
–
4
for the parent magma. Accounting for low-degree partial melting of the depleted mantle followed by extensive magma fractional crystallization
4
, we estimate a maximum mantle water abundance of 1–5 μg g
−1
, suggesting that the Moon’s youngest volcanism was not driven by abundant water in its mantle source. Such a modest water content for the Chang’e-5 basalt mantle source region is at the low end of the range estimated from mare basalts that erupted from around 4.0 Ga to 2.8 Ga (refs.
5
,
6
), suggesting that the mantle source of the Chang’e-5 basalts had become dehydrated by 2.0 Ga through previous melt extraction from the Procellarum KREEP Terrane mantle during prolonged volcanic activity.
Water abundance and hydrogen isotope compositions of two-billion-year-old basalt samples returned from the Moon by the Chang’e-5 mission suggest that the samples came from a relatively dry mantle source. |
| doi_str_mv | 10.1038/s41586-021-04107-9 |
| format | Article |
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1
, the crystallization of the lunar magma ocean
2
and the duration of lunar volcanism
2
. The Chang’e-5 mission returned some of the youngest mare basalt samples reported so far, dated at 2.0 billion years ago (Ga)
3
, from the northwestern Procellarum KREEP Terrane, providing a probe into the spatiotemporal evolution of lunar water. Here we report the water abundances and hydrogen isotope compositions of apatite and ilmenite-hosted melt inclusions from the Chang’e-5 basalts. We derive a maximum water abundance of 283 ± 22 μg g
−1
and a deuterium/hydrogen ratio of (1.06 ± 0.25) × 10
–
4
for the parent magma. Accounting for low-degree partial melting of the depleted mantle followed by extensive magma fractional crystallization
4
, we estimate a maximum mantle water abundance of 1–5 μg g
−1
, suggesting that the Moon’s youngest volcanism was not driven by abundant water in its mantle source. Such a modest water content for the Chang’e-5 basalt mantle source region is at the low end of the range estimated from mare basalts that erupted from around 4.0 Ga to 2.8 Ga (refs.
5
,
6
), suggesting that the mantle source of the Chang’e-5 basalts had become dehydrated by 2.0 Ga through previous melt extraction from the Procellarum KREEP Terrane mantle during prolonged volcanic activity.
Water abundance and hydrogen isotope compositions of two-billion-year-old basalt samples returned from the Moon by the Chang’e-5 mission suggest that the samples came from a relatively dry mantle source.</description><identifier>ISSN: 0028-0836</identifier><identifier>EISSN: 1476-4687</identifier><identifier>DOI: 10.1038/s41586-021-04107-9</identifier><identifier>PMID: 34666337</identifier><language>eng</language><publisher>London: Nature Publishing Group UK</publisher><subject>704/445/209 ; 704/445/431 ; Abundance ; Apatite ; Basalt ; Cosmic rays ; Crystallization ; Dehydration ; Deuterium ; Estimates ; Humanities and Social Sciences ; Hydrogen ; Hydrogen isotopes ; Ilmenite ; Inclusions ; Isotope composition ; Kreep ; Lunar evolution ; Lunar exploration ; Lunar mantle ; Magma ; Moisture content ; Moon ; multidisciplinary ; Science ; Science (multidisciplinary) ; Space missions ; Volcanic activity ; Water content</subject><ispartof>Nature (London), 2021-12, Vol.600 (7887), p.49-53</ispartof><rights>The Author(s) 2021</rights><rights>2021. The Author(s).</rights><rights>Copyright Nature Publishing Group Dec 2, 2021</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a497t-feece31965bd004ca3ab6d6bb3b94754ac49ede96dbfaa245a3b6d316fa7c2f63</citedby><cites>FETCH-LOGICAL-a497t-feece31965bd004ca3ab6d6bb3b94754ac49ede96dbfaa245a3b6d316fa7c2f63</cites><orcidid>0000-0002-0187-6069 ; 0000-0002-7852-6147 ; 0000-0003-4509-8876 ; 0000-0001-9813-5330 ; 0000-0002-1254-8693 ; 0000-0003-2170-3349 ; 0000-0002-3407-4329 ; 0000-0001-9708-6901 ; 0000-0003-4026-4476 ; 0000-0002-4887-5274 ; 0000-0002-3490-9875 ; 0000-0003-2707-4977 ; 0000-0003-4898-1023</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1038/s41586-021-04107-9$$EPDF$$P50$$Gspringer$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1038/s41586-021-04107-9$$EHTML$$P50$$Gspringer$$Hfree_for_read</linktohtml><link.rule.ids>230,314,777,781,882,27905,27906,41469,42538,51300</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/34666337$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>Hu, Sen</creatorcontrib><creatorcontrib>He, Huicun</creatorcontrib><creatorcontrib>Ji, Jianglong</creatorcontrib><creatorcontrib>Lin, Yangting</creatorcontrib><creatorcontrib>Hui, Hejiu</creatorcontrib><creatorcontrib>Anand, Mahesh</creatorcontrib><creatorcontrib>Tartèse, Romain</creatorcontrib><creatorcontrib>Yan, Yihong</creatorcontrib><creatorcontrib>Hao, Jialong</creatorcontrib><creatorcontrib>Li, Ruiying</creatorcontrib><creatorcontrib>Gu, Lixin</creatorcontrib><creatorcontrib>Guo, Qian</creatorcontrib><creatorcontrib>He, Huaiyu</creatorcontrib><creatorcontrib>Ouyang, Ziyuan</creatorcontrib><title>A dry lunar mantle reservoir for young mare basalts of Chang’e-5</title><title>Nature (London)</title><addtitle>Nature</addtitle><addtitle>Nature</addtitle><description>The distribution of water in the Moon’s interior carries implications for the origin of the Moon
1
, the crystallization of the lunar magma ocean
2
and the duration of lunar volcanism
2
. The Chang’e-5 mission returned some of the youngest mare basalt samples reported so far, dated at 2.0 billion years ago (Ga)
3
, from the northwestern Procellarum KREEP Terrane, providing a probe into the spatiotemporal evolution of lunar water. Here we report the water abundances and hydrogen isotope compositions of apatite and ilmenite-hosted melt inclusions from the Chang’e-5 basalts. We derive a maximum water abundance of 283 ± 22 μg g
−1
and a deuterium/hydrogen ratio of (1.06 ± 0.25) × 10
–
4
for the parent magma. Accounting for low-degree partial melting of the depleted mantle followed by extensive magma fractional crystallization
4
, we estimate a maximum mantle water abundance of 1–5 μg g
−1
, suggesting that the Moon’s youngest volcanism was not driven by abundant water in its mantle source. Such a modest water content for the Chang’e-5 basalt mantle source region is at the low end of the range estimated from mare basalts that erupted from around 4.0 Ga to 2.8 Ga (refs.
5
,
6
), suggesting that the mantle source of the Chang’e-5 basalts had become dehydrated by 2.0 Ga through previous melt extraction from the Procellarum KREEP Terrane mantle during prolonged volcanic activity.
Water abundance and hydrogen isotope compositions of two-billion-year-old basalt samples returned from the Moon by the Chang’e-5 mission suggest that the samples came from a relatively dry mantle source.</description><subject>704/445/209</subject><subject>704/445/431</subject><subject>Abundance</subject><subject>Apatite</subject><subject>Basalt</subject><subject>Cosmic rays</subject><subject>Crystallization</subject><subject>Dehydration</subject><subject>Deuterium</subject><subject>Estimates</subject><subject>Humanities and Social Sciences</subject><subject>Hydrogen</subject><subject>Hydrogen isotopes</subject><subject>Ilmenite</subject><subject>Inclusions</subject><subject>Isotope composition</subject><subject>Kreep</subject><subject>Lunar evolution</subject><subject>Lunar exploration</subject><subject>Lunar mantle</subject><subject>Magma</subject><subject>Moisture content</subject><subject>Moon</subject><subject>multidisciplinary</subject><subject>Science</subject><subject>Science (multidisciplinary)</subject><subject>Space missions</subject><subject>Volcanic activity</subject><subject>Water 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dry lunar mantle reservoir for young mare basalts of Chang’e-5</title><author>Hu, Sen ; He, Huicun ; Ji, Jianglong ; Lin, Yangting ; Hui, Hejiu ; Anand, Mahesh ; Tartèse, Romain ; Yan, Yihong ; Hao, Jialong ; Li, Ruiying ; Gu, Lixin ; Guo, Qian ; He, Huaiyu ; Ouyang, Ziyuan</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a497t-feece31965bd004ca3ab6d6bb3b94754ac49ede96dbfaa245a3b6d316fa7c2f63</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>704/445/209</topic><topic>704/445/431</topic><topic>Abundance</topic><topic>Apatite</topic><topic>Basalt</topic><topic>Cosmic rays</topic><topic>Crystallization</topic><topic>Dehydration</topic><topic>Deuterium</topic><topic>Estimates</topic><topic>Humanities and Social Sciences</topic><topic>Hydrogen</topic><topic>Hydrogen isotopes</topic><topic>Ilmenite</topic><topic>Inclusions</topic><topic>Isotope composition</topic><topic>Kreep</topic><topic>Lunar evolution</topic><topic>Lunar exploration</topic><topic>Lunar mantle</topic><topic>Magma</topic><topic>Moisture content</topic><topic>Moon</topic><topic>multidisciplinary</topic><topic>Science</topic><topic>Science (multidisciplinary)</topic><topic>Space missions</topic><topic>Volcanic activity</topic><topic>Water content</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Hu, Sen</creatorcontrib><creatorcontrib>He, Huicun</creatorcontrib><creatorcontrib>Ji, Jianglong</creatorcontrib><creatorcontrib>Lin, Yangting</creatorcontrib><creatorcontrib>Hui, Hejiu</creatorcontrib><creatorcontrib>Anand, Mahesh</creatorcontrib><creatorcontrib>Tartèse, Romain</creatorcontrib><creatorcontrib>Yan, Yihong</creatorcontrib><creatorcontrib>Hao, Jialong</creatorcontrib><creatorcontrib>Li, Ruiying</creatorcontrib><creatorcontrib>Gu, Lixin</creatorcontrib><creatorcontrib>Guo, 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Ziyuan</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>A dry lunar mantle reservoir for young mare basalts of Chang’e-5</atitle><jtitle>Nature (London)</jtitle><stitle>Nature</stitle><addtitle>Nature</addtitle><date>2021-12-02</date><risdate>2021</risdate><volume>600</volume><issue>7887</issue><spage>49</spage><epage>53</epage><pages>49-53</pages><issn>0028-0836</issn><eissn>1476-4687</eissn><abstract>The distribution of water in the Moon’s interior carries implications for the origin of the Moon
1
, the crystallization of the lunar magma ocean
2
and the duration of lunar volcanism
2
. The Chang’e-5 mission returned some of the youngest mare basalt samples reported so far, dated at 2.0 billion years ago (Ga)
3
, from the northwestern Procellarum KREEP Terrane, providing a probe into the spatiotemporal evolution of lunar water. Here we report the water abundances and hydrogen isotope compositions of apatite and ilmenite-hosted melt inclusions from the Chang’e-5 basalts. We derive a maximum water abundance of 283 ± 22 μg g
−1
and a deuterium/hydrogen ratio of (1.06 ± 0.25) × 10
–
4
for the parent magma. Accounting for low-degree partial melting of the depleted mantle followed by extensive magma fractional crystallization
4
, we estimate a maximum mantle water abundance of 1–5 μg g
−1
, suggesting that the Moon’s youngest volcanism was not driven by abundant water in its mantle source. Such a modest water content for the Chang’e-5 basalt mantle source region is at the low end of the range estimated from mare basalts that erupted from around 4.0 Ga to 2.8 Ga (refs.
5
,
6
), suggesting that the mantle source of the Chang’e-5 basalts had become dehydrated by 2.0 Ga through previous melt extraction from the Procellarum KREEP Terrane mantle during prolonged volcanic activity.
Water abundance and hydrogen isotope compositions of two-billion-year-old basalt samples returned from the Moon by the Chang’e-5 mission suggest that the samples came from a relatively dry mantle source.</abstract><cop>London</cop><pub>Nature Publishing Group UK</pub><pmid>34666337</pmid><doi>10.1038/s41586-021-04107-9</doi><tpages>5</tpages><orcidid>https://orcid.org/0000-0002-0187-6069</orcidid><orcidid>https://orcid.org/0000-0002-7852-6147</orcidid><orcidid>https://orcid.org/0000-0003-4509-8876</orcidid><orcidid>https://orcid.org/0000-0001-9813-5330</orcidid><orcidid>https://orcid.org/0000-0002-1254-8693</orcidid><orcidid>https://orcid.org/0000-0003-2170-3349</orcidid><orcidid>https://orcid.org/0000-0002-3407-4329</orcidid><orcidid>https://orcid.org/0000-0001-9708-6901</orcidid><orcidid>https://orcid.org/0000-0003-4026-4476</orcidid><orcidid>https://orcid.org/0000-0002-4887-5274</orcidid><orcidid>https://orcid.org/0000-0002-3490-9875</orcidid><orcidid>https://orcid.org/0000-0003-2707-4977</orcidid><orcidid>https://orcid.org/0000-0003-4898-1023</orcidid><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0028-0836 |
| ispartof | Nature (London), 2021-12, Vol.600 (7887), p.49-53 |
| issn | 0028-0836 1476-4687 |
| language | eng |
| recordid | cdi_pubmedcentral_primary_oai_pubmedcentral_nih_gov_8636271 |
| source | Nature Journals Online; SpringerLink Journals - AutoHoldings |
| subjects | 704/445/209 704/445/431 Abundance Apatite Basalt Cosmic rays Crystallization Dehydration Deuterium Estimates Humanities and Social Sciences Hydrogen Hydrogen isotopes Ilmenite Inclusions Isotope composition Kreep Lunar evolution Lunar exploration Lunar mantle Magma Moisture content Moon multidisciplinary Science Science (multidisciplinary) Space missions Volcanic activity Water content |
| title | A dry lunar mantle reservoir for young mare basalts of Chang’e-5 |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-19T13%3A32%3A49IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_pubme&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=A%20dry%20lunar%20mantle%20reservoir%20for%20young%20mare%20basalts%20of%20Chang%E2%80%99e-5&rft.jtitle=Nature%20(London)&rft.au=Hu,%20Sen&rft.date=2021-12-02&rft.volume=600&rft.issue=7887&rft.spage=49&rft.epage=53&rft.pages=49-53&rft.issn=0028-0836&rft.eissn=1476-4687&rft_id=info:doi/10.1038/s41586-021-04107-9&rft_dat=%3Cproquest_pubme%3E2584015746%3C/proquest_pubme%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2606199128&rft_id=info:pmid/34666337&rfr_iscdi=true |