Long-term reduced lunar mantle revealed by Chang’e-5 basalt

The redox state of a planetary mantle affects its thermal evolution. The redox evolution of lunar mantle, however, remains unclear due to limited oxygen fugacity (fO<sub>2</sub>) constraints from young lunar samples. Here, we report vanadium (V) oxybarometers on olivine and spinel conducted on 27 Chang'e-5 basalt fragments from 2.0 billion years ago. These fragments yield an average fO<sub>2</sub> of ΔIW -0.84 ± 0.65 (2σ), which closely aligns with the Apollo samples from 3.6-3.0 billion years ago. This temporal uniformity indicates the lunar mantle remained reduced. This observation reveals that the processes responsible for oxidizing mantles of Earth and Mars either did not occur or had negligible oxidizing effects on the Moon. The long-term reduced mantle may lead to a distinctive volatile degassing pathway for the Moon. It could also make the lunar mantle more difficult to melt, preventing internal heat dissipation and consequently resulting in a slow cooling rate.

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Publication Details

Journal
Nature Communications
Published
2024-09-27
DOI
https://doi.org/10.1038/s41467-024-52710-x
Citations
13
Primary Topic
Planetary Science and Exploration
Type
article
Field-Weighted Citation Impact
4.31

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article

Long-term reduced lunar mantle revealed by Chang’e-5 basalt

Lihui Jia, Heng‐Ci Tian, Hejiu Hui, Wei Yang et al.
13 citations
Nature Communications
Planetary Science and Exploration
4.31
article

Long-term reduced lunar mantle revealed by Chang’e-5 basalt

Lihui Jia, Heng‐Ci Tian, Hejiu Hui, Wei Yang, Shitou Wu, Yanhao Lin, Renhao Ruan, Lixin Gu, Ross N. Mitchell, Sen Hu, Yangting Lin, Di Zhang, Huijuan Zhang, Xian‐Hua Li, Yi Chen, Fu‐Yuan Wu
article en
13 citations

Abstract

The redox state of a planetary mantle affects its thermal evolution. The redox evolution of lunar mantle, however, remains unclear due to limited oxygen fugacity (fO<sub>2</sub>) constraints from young lunar samples. Here, we report vanadium (V) oxybarometers on olivine and spinel conducted on 27 Chang'e-5 basalt fragments from 2.0 billion years ago. These fragments yield an average fO<sub>2</sub> of ΔIW -0.84 ± 0.65 (2σ), which closely aligns with the Apollo samples from 3.6-3.0 billion years ago. This temporal uniformity indicates the lunar mantle remained reduced. This observation reveals that the processes responsible for oxidizing mantles of Earth and Mars either did not occur or had negligible oxidizing effects on the Moon. The long-term reduced mantle may lead to a distinctive volatile degassing pathway for the Moon. It could also make the lunar mantle more difficult to melt, preventing internal heat dissipation and consequently resulting in a slow cooling rate.

Nature CommunicationsVol. 15(1)
Chinese Academy of Sciences (CN), Nanjing University of Science and Technology (CN), Institute of Geology and Geophysics (AZ), East China University of Technology (CN), Institute of Geology and Geophysics (CN), Center for High Pressure Science and Technology Advanced Research (CN), University of Chinese Academy of Sciences (CN), Nanjing University (CN)
China National Space Administration, National Natural Science Foundation of China, Chinese Academy of Sciences, Institute of Geology and Geophysics, Chinese Academy of Sciences
Climate action
Openalex Percentile: Top 6%
Planetary Science and Exploration
4.31
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