Evidence map›Paper›PMID 42685190›Full record

ArticleScience advances2026

Moon's farside near-zero paleomagnetic field suggests a global lunar dynamo cessation.

Xuelong Jiang, Fei Su, Huapei Wang, Runchuan Liu, Ting Cao, Shaochen Hu, Haijun Li, Chen Wen, Yu-Min Chou, Huafeng Qin and 4 more

Abstract read
In one paragraph

Article in Science advances, 2026. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Not yet cited in PubMed.

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1 · What the graph read from it

What it found

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The abstract states no effect estimate the extractor could read, or names no intervention and outcome on the map, so this paper lights no cell and moves no belief. It is still indexed, cited and linked below.

2 · The registry

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3 · Its place in the literature

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0 citing papers in PubMed.

No citing paper in PubMed yet.

4 · The record

Corrections and comments

PubMed lists nothing against this paper. Absence here is not a guarantee, only a check that was made.

5 · Who and what money

Authors and funding

14 authors.

Xuelong JiangSchool of Earth and Space Sciences, Peking University, Beijing 100871, China.ORCID 0000-0003-2831-0986
Fei SuKey Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, China.ORCID 0000-0002-1636-7259
Huapei WangPaleomagnetism and Planetary Magnetism Laboratory, School of Geophysics and Geomatics, China University of Geosciences, Wuhan, Hubei 430074, China.ORCID 0000-0003-1676-3494
Runchuan LiuKey Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, China.
Ting CaoPaleomagnetism and Planetary Magnetism Laboratory, School of Geophysics and Geomatics, China University of Geosciences, Wuhan, Hubei 430074, China.ORCID 0000-0002-2185-6487
Shaochen HuPaleomagnetism and Planetary Magnetism Laboratory, School of Geophysics and Geomatics, China University of Geosciences, Wuhan, Hubei 430074, China.ORCID 0000-0001-6642-0719
Haijun LiPaleomagnetism and Planetary Magnetism Laboratory, School of Geophysics and Geomatics, China University of Geosciences, Wuhan, Hubei 430074, China.ORCID 0000-0002-7242-852X
Chen WenPaleomagnetism and Planetary Magnetism Laboratory, School of Geophysics and Geomatics, China University of Geosciences, Wuhan, Hubei 430074, China.ORCID 0000-0003-3696-3696
Yu-Min ChouCentre for Marine Magnetism (CM2), Department of Ocean Science and Engineering, Southern University of Science and Technology, Shenzhen 518055, China.ORCID 0000-0002-6369-8456
Huafeng QinState Key Laboratory of Lithospheric and Environmental Coevolution, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, China.ORCID 0000-0001-7699-5161
Kaixian QiCollege of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing 100049, China.ORCID 0000-0003-0433-4246
Fei HanPaleomagnetism and Planetary Magnetism Laboratory, School of Geophysics and Geomatics, China University of Geosciences, Wuhan, Hubei 430074, China.ORCID 0000-0002-9450-006X
Yiming MaPaleomagnetism and Planetary Magnetism Laboratory, School of Geophysics and Geomatics, China University of Geosciences, Wuhan, Hubei 430074, China.ORCID 0000-0002-7036-7065
Jiabo LiuPaleomagnetism and Planetary Magnetism Laboratory, School of Geophysics and Geomatics, China University of Geosciences, Wuhan, Hubei 430074, China.ORCID 0000-0002-6150-1322

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

Recent paleomagnetic studies of Apollo and Chang'e returned samples suggest that the lunar dynamo was active from ∼4.2 billion years ago (Ga) and ceased by ∼1.0 Ga. However, uncertainties remain regarding the temporal and spatial distribution of the lunar paleomagnetic field, as almost all of the returned samples are from the nearside, except for those returned by Chang'e-6. Here, we present the first paleomagnetic analysis of a lunar meteorite, Northwest Africa 15528, which is a feldspathic regolith breccia likely from the farside of the Moon. Our results not only indicate that it recorded a near-zero magnetic field (below a few hundred nanoteslas) at ∼0.7 Ga but also show that lunar meteorites can provide critical paleomagnetic information. Combined with two young Apollo samples from the nearside, Apollo 15015 (formed at ∼0.9 Ga) and Apollo 15465 (formed at ∼0.5 Ga), our findings suggest the absence of a global dynamo-generated lunar magnetic field for the past one billion years.

Identifiers

PMID42685190
PMCPMC13537248

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