Petrogenesis of Very‐Low‐Ti Basalts Returned by Chang'e‐6 From the Lunar Farside

Abstract Lunar volcanism provides critical insights into the Moon's thermochemical evolution. We present petrological and geochemical analyses of six very‐low‐Ti (VLT) basalt fragments from Chang'e‐6 (CE6) samples. These basalts yield a Pb‐Pb age of around 2.9 Ga, representing the youngest reported VLT volcanism. They are slightly older than the low‐Ti basalts from the same soils and exhibit distinct pyroxene compositions and 238 U/ 204 Pb ratios, indicating derivation from distinct mantle sources. Compared to Apollo and Luna VLT basalts, these samples share similarly depleted Sr‐Pb isotopes but display elevated rare earth element concentrations and TiO 2 contents. These basalts most likely derived from low‐degree melting of an olivine‐orthopyroxene source followed by 30%–40% fractional crystallization. Further diffusion chronometry reveals rapid magma ascent from magma chamber to surface, likely facilitated by the thin lunar crust resulting from the South Pole‐Aitken basin‐forming impact. Our results provide new insights into the petrogenesis of volcanic activity on the lunar farside.

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Publication Details

Journal
Geophysical Research Letters
Published
2025-12-07
DOI
https://doi.org/10.1029/2025gl117921
Citations
1
Primary Topic
Planetary Science and Exploration
Type
article
Field-Weighted Citation Impact
1.15

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article

Petrogenesis of Very‐Low‐Ti Basalts Returned by Chang'e‐6 From the Lunar Farside

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1 citations
Geophysical Research Letters
Planetary Science and Exploration
1.15
article

Petrogenesis of Very‐Low‐Ti Basalts Returned by Chang'e‐6 From the Lunar Farside

Lihui Jia, Heng‐Ci Tian, Yue‐Heng Yang, Qin Zhou, Wei Yang, Chao Huang, Shitou Wu, Qiuli Li, Xu Tang, Sen Hu, Di Zhang, Hao Wang, Xian‐Hua Li, Yi Chen, Fu‐Yuan Wu
article en
1 citations

Abstract

Abstract Lunar volcanism provides critical insights into the Moon's thermochemical evolution. We present petrological and geochemical analyses of six very‐low‐Ti (VLT) basalt fragments from Chang'e‐6 (CE6) samples. These basalts yield a Pb‐Pb age of around 2.9 Ga, representing the youngest reported VLT volcanism. They are slightly older than the low‐Ti basalts from the same soils and exhibit distinct pyroxene compositions and 238 U/ 204 Pb ratios, indicating derivation from distinct mantle sources. Compared to Apollo and Luna VLT basalts, these samples share similarly depleted Sr‐Pb isotopes but display elevated rare earth element concentrations and TiO 2 contents. These basalts most likely derived from low‐degree melting of an olivine‐orthopyroxene source followed by 30%–40% fractional crystallization. Further diffusion chronometry reveals rapid magma ascent from magma chamber to surface, likely facilitated by the thin lunar crust resulting from the South Pole‐Aitken basin‐forming impact. Our results provide new insights into the petrogenesis of volcanic activity on the lunar farside.

Geophysical Research LettersVol. 52(23)
Chinese Academy of Sciences (CN), Institute of Geology and Geophysics (CN), National Astronomical Observatories (CN)
China National Space Administration, National Natural Science Foundation of China, Chinese Academy of Sciences, Youth Innovation Promotion Association of the Chinese Academy of Sciences, East China Institute of Technology, Youth Innovation Promotion Association, Institute of Geology and Geophysics, Chinese Academy of Sciences
Openalex Percentile: Top 14%
Planetary Science and Exploration
1.15
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