IGGCAS OpenIR  > 地球与行星物理院重点实验室
Deuterium and (37)Chlorine Rich Fluids on the Surface of Mars: Evidence From the Enriched Basaltic Shergottite Northwest Africa 8657
Hu, S.1,2,3; Lin, Y.1,2; Anand, M.3,4; Franchi, A.3; Zhao, X.3; Zhang, J.1,2; Hao, J.1,2; Zhang, T.1,2; Yang, W.1,2; Changela, H.1,5,6
2020-09-01
Source PublicationJOURNAL OF GEOPHYSICAL RESEARCH-PLANETS
ISSN2169-9097
Volume125Issue:9Pages:15
AbstractApatite, a major hydrous mineral in Martian meteorites, has the potential to reveal history of volatiles on Mars. Here we report the H and Cl isotopic systematics of apatite from the enriched basaltic shergottite Northwest Africa (NWA) 8657 to better understand the processes influencing volatiles at or near the Martian (sub)surface. The apatite in NWA 8657 has the highest reported delta D value (up to 6,509 parts per thousand) of any phosphates in Martian meteorites. The positive correlation between the H2O contents (72-2,251 ppm) and delta D values (3,965-6,509 parts per thousand) as well as between the Cl contents (1.28-6.17wt%) and delta Cl-37 values (-1.7-4.0 parts per thousand) in NWA 8657 apatite are consistent with mixing between volatiles derived from the Martian mantle and meteoric water/fluid. The D- and(37)Cl-enrichment of apatite in NWA 8657 implies isotopic exchange with subsurficial fluids during postcrystallization hydrothermal event(s).
DOI10.1029/2020JE006537
Funding OrganizationNational Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; China Scholarship Council ; China Scholarship Council ; China Scholarship Council ; China Scholarship Council ; UK STFC ; UK STFC ; UK STFC ; UK STFC ; Institute of Geology & Geophysics, CAS ; Institute of Geology & Geophysics, CAS ; Institute of Geology & Geophysics, CAS ; Institute of Geology & Geophysics, CAS ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; China Scholarship Council ; China Scholarship Council ; China Scholarship Council ; China Scholarship Council ; UK STFC ; UK STFC ; UK STFC ; UK STFC ; Institute of Geology & Geophysics, CAS ; Institute of Geology & Geophysics, CAS ; Institute of Geology & Geophysics, CAS ; Institute of Geology & Geophysics, CAS ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; China Scholarship Council ; China Scholarship Council ; China Scholarship Council ; China Scholarship Council ; UK STFC ; UK STFC ; UK STFC ; UK STFC ; Institute of Geology & Geophysics, CAS ; Institute of Geology & Geophysics, CAS ; Institute of Geology & Geophysics, CAS ; Institute of Geology & Geophysics, CAS ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; China Scholarship Council ; China Scholarship Council ; China Scholarship Council ; China Scholarship Council ; UK STFC ; UK STFC ; UK STFC ; UK STFC ; Institute of Geology & Geophysics, CAS ; Institute of Geology & Geophysics, CAS ; Institute of Geology & Geophysics, CAS ; Institute of Geology & Geophysics, CAS
WOS KeywordCHLORINE ISOTOPE COMPOSITION ; MARTIAN METEORITE ; HYDROTHERMAL FLUIDS ; SUBSURFACE WATER ; MELT INCLUSIONS ; MAGMATIC WATER ; LUNAR APATITE ; SOLAR-SYSTEM ; D/H RATIO ; HYDROGEN
Language英语
Funding ProjectNational Natural Science Foundation of China[41973062] ; National Natural Science Foundation of China[41573057] ; National Natural Science Foundation of China[41430105] ; National Natural Science Foundation of China[41490631] ; China Scholarship Council[201804910284] ; UK STFC[ST/P000657/1] ; Institute of Geology & Geophysics, CAS[IGGCAS-201905]
Funding OrganizationNational Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; China Scholarship Council ; China Scholarship Council ; China Scholarship Council ; China Scholarship Council ; UK STFC ; UK STFC ; UK STFC ; UK STFC ; Institute of Geology & Geophysics, CAS ; Institute of Geology & Geophysics, CAS ; Institute of Geology & Geophysics, CAS ; Institute of Geology & Geophysics, CAS ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; China Scholarship Council ; China Scholarship Council ; China Scholarship Council ; China Scholarship Council ; UK STFC ; UK STFC ; UK STFC ; UK STFC ; Institute of Geology & Geophysics, CAS ; Institute of Geology & Geophysics, CAS ; Institute of Geology & Geophysics, CAS ; Institute of Geology & Geophysics, CAS ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; China Scholarship Council ; China Scholarship Council ; China Scholarship Council ; China Scholarship Council ; UK STFC ; UK STFC ; UK STFC ; UK STFC ; Institute of Geology & Geophysics, CAS ; Institute of Geology & Geophysics, CAS ; Institute of Geology & Geophysics, CAS ; Institute of Geology & Geophysics, CAS ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; China Scholarship Council ; China Scholarship Council ; China Scholarship Council ; China Scholarship Council ; UK STFC ; UK STFC ; UK STFC ; UK STFC ; Institute of Geology & Geophysics, CAS ; Institute of Geology & Geophysics, CAS ; Institute of Geology & Geophysics, CAS ; Institute of Geology & Geophysics, CAS
WOS Research AreaGeochemistry & Geophysics
WOS SubjectGeochemistry & Geophysics
WOS IDWOS:000576620600015
PublisherAMER GEOPHYSICAL UNION
Citation statistics
Document Type期刊论文
Identifierhttp://ir.iggcas.ac.cn/handle/132A11/98286
Collection地球与行星物理院重点实验室
Corresponding AuthorHu, S.
Affiliation1.Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing, Peoples R China
2.Chinese Acad Sci, Innovat Acad Earth Sci, Beijing, Peoples R China
3.Open Univ, Sch Phys Sci, Milton Keynes, Bucks, England
4.Nat Hist Museum, Dept Earth Sci, London, England
5.Chinese Acad Space Technol, Qianxuesen Lab Space Technol, Beijing, Peoples R China
6.Univ New Mexico, Dept Earth & Planetary Sci, Albuquerque, NM 87131 USA
First Author AffilicationKey Laboratory of Earth and Planetary Physics, Chinese Academy of Sciences
Corresponding Author AffilicationKey Laboratory of Earth and Planetary Physics, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Hu, S.,Lin, Y.,Anand, M.,et al. Deuterium and (37)Chlorine Rich Fluids on the Surface of Mars: Evidence From the Enriched Basaltic Shergottite Northwest Africa 8657[J]. JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS,2020,125(9):15.
APA Hu, S..,Lin, Y..,Anand, M..,Franchi, A..,Zhao, X..,...&Changela, H..(2020).Deuterium and (37)Chlorine Rich Fluids on the Surface of Mars: Evidence From the Enriched Basaltic Shergottite Northwest Africa 8657.JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS,125(9),15.
MLA Hu, S.,et al."Deuterium and (37)Chlorine Rich Fluids on the Surface of Mars: Evidence From the Enriched Basaltic Shergottite Northwest Africa 8657".JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS 125.9(2020):15.
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