Evidence map›Paper›PMID 39246729›Full record

ArticleCommunications earth & environment2024

A lunar core dynamo limited to the Moon's first ~140 million years.

Tinghong Zhou, John A Tarduno, Rory D Cottrell, Clive R Neal, Francis Nimmo, Eric G Blackman, Mauricio Ibañez-Mejia

Abstract read
In one paragraph

Article in Communications earth & environment, 2024. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 6 papers.

0numbers the graph read from it
0cells of the map it votes in
6citing papers in PubMed
–field-weighted citation impact
1 · What the graph read from it

What it found

Each row is one number read from the abstract, on the scale the paper reported it, with its interval. Left of the dashed line favours the treatment, right favours the comparator. Under each row is the sentence it came from. New to these charts? A ten-minute tutorial.

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

The trial behind it

Trials whose registry record cites this paper, or whose number appears in the abstract. A trial that started after this paper was published is citing it as background, not reporting it.

Neither the registry nor the abstract names a trial number. If this is a trial report, that itself is worth knowing.

3 · Its place in the literature

Who cites it

6 citing papers in PubMed.

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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

7 authors.

Tinghong ZhouDepartment of Earth and Environmental Sciences, University of Rochester, Rochester, NY 14627 USA.ORCID 0000-0001-7460-8957
John A TardunoDepartment of Earth and Environmental Sciences, University of Rochester, Rochester, NY 14627 USA.ORCID 0000-0002-0490-0124
Rory D CottrellDepartment of Earth and Environmental Sciences, University of Rochester, Rochester, NY 14627 USA.ORCID 0000-0003-4174-6389
Clive R NealDepartment of Civil Engineering and Geological Sciences, University of Notre Dame, Notre Dame, IN 46556 USA.ORCID 0000-0003-0705-3490
Francis NimmoDepartment of Earth and Planetary Sciences, University of California, Santa Cruz, CA 95064 USA.ORCID 0000-0003-3573-5915
Eric G BlackmanDepartment of Physics and Astronomy, University of Rochester, Rochester, NY 14627 USA.ORCID 0000-0002-9405-8435
Mauricio Ibañez-MejiaDepartment of Geosciences, University of Arizona, Tucson, AZ 85721 USA.ORCID 0000-0002-7839-2425

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

Single crystal paleointensity (SCP) reveals that the Moon lacked a long-lived core dynamo, though mysteries remain. An episodic dynamo, seemingly recorded by some Apollo basalts, is temporally and energetically problematic. We evaluate this enigma through study of ~3.7 billion-year-old (Ga) Apollo basalts 70035 and 75035. Whole rock analyses show unrealistically high nominal magnetizations, whereas SCP indicate null fields, illustrating that the former do not record an episodic dynamo. However, deep crustal magnetic anomalies might record an early lunar dynamo. SCP studies of 3.97 Ga Apollo breccia 61016 and 4.36 Ga ferroan anorthosite 60025 also yield null values, constraining any core dynamo to the Moon's first 140 million years. These findings suggest that traces of Earth's Hadean atmosphere, transferred to the Moon lacking a magnetosphere, could be trapped in the buried lunar regolith, presenting an exceptional target for future exploration.

Indexed as

Atmospheric chemistryCore processesEarly solar systemPalaeomagnetismRings and moons

Identifiers

PMID39246729
PMCPMC11379625

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Read under generation 80e0d062 · epoch 390. Bibliography from PubMed, PubMed Central and OpenAlex; grants from NIH RePORTER; trial links from ClinicalTrials.gov; estimates, votes and beliefs from the OpenQuestion graph.