ArticleScience advances2025
Persistent but weak magnetic field at the Moon's midstage revealed by Chang'e-5 basalt.
Article in Science advances, 2025. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 7 papers.
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Who cites it
7 citing papers in PubMed.
- Magmatic origin of the Dewar magnetic anomaly: Implications for an early lunar dynamo.Science advances · 2026Article
- Moon's farside near-zero paleomagnetic field suggests a global lunar dynamo cessation.Science advances · 2026Article
- Microscopic magnetic-field imaging of a single lunar dust grain.Fundamental research · 2026Article
- The source and thermal driver of young (<3.0 Ga) lunar volcanism.Science advances · 2025Article
- Magnetic signatures and origins of ferromagnetic minerals in Chang'e-6 lunar farside soils.Nature communications · 2025Article
- Article
- The Moon goddess's magnetic midlife.Science advances · 2025Review
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Authors and funding
28 authors.
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Abstract
The evolution of the lunar magnetic field can reveal the Moon's interior structure, thermal history, and surface environment. The mid-to-late-stage evolution of the lunar magnetic field is poorly constrained, and thus, the existence of a long-lived lunar dynamo remains controversial. The Chang'e-5 mission returned the heretofore youngest mare basalts from Oceanus Procellarum uniquely positioned at midlatitude. We recovered weak paleointensities of ~2 to 4 microtesla from the Chang'e-5 basalt clasts at 2 billion years ago, attesting to the longevity of the lunar dynamo until at least the Moon's midstage. This paleomagnetic result implies the existence of thermal convection in the lunar deep interior at the lunar midstage, which may have supplied mantle heat flux for young volcanism.
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