Evidence map›Paper›PMID 34348904›Full record

ArticleScience advances2021

Absence of a long-lived lunar paleomagnetosphere.

John A Tarduno, Rory D Cottrell, Kristin Lawrence, Richard K Bono, Wentao Huang, Catherine L Johnson, Eric G Blackman, Aleksey V Smirnov, Miki Nakajima, Clive R Neal and 4 more

Open access · goldAbstract read
In one paragraph

Article in Science advances, 2021. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 10 papers.

0numbers the graph read from it
0cells of the map it votes in
10citing papers in PubMed
2.8field-weighted citation impact, top 8% of its field
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

10 citing papers in PubMed, 56 citations in OpenAlex.

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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

14 authors at 7 institutions in 4 countries.

John A TardunoDepartment of Earth and Environmental Sciences, University of Rochester, Rochester, NY 14627, USA. john.tarduno@rochester.edu.ORCID http://orcid.org/0000-0002-0490-0124
Rory D CottrellDepartment of Earth and Environmental Sciences, University of Rochester, Rochester, NY 14627, USA.ORCID http://orcid.org/0000-0003-4174-6389
Kristin LawrencePlanetary Science Institute, Tucson, AZ 85719-2395, USA.
Richard K BonoGeomagnetism Laboratory, University of Liverpool, Liverpool L69 3GP, UK.ORCID http://orcid.org/0000-0002-8222-2218
Wentao HuangDepartment of Earth and Environmental Sciences, University of Rochester, Rochester, NY 14627, USA.ORCID http://orcid.org/0000-0002-7291-7745
Catherine L JohnsonPlanetary Science Institute, Tucson, AZ 85719-2395, USA.ORCID http://orcid.org/0000-0001-6084-0149
Eric G BlackmanDepartment of Physics and Astronomy, University of Rochester, Rochester, NY 14627, USA.ORCID http://orcid.org/0000-0002-9405-8435
Aleksey V SmirnovDepartment of Geological and Mining Engineering and Sciences, Michigan Technological University, Houghton, MI 49931, USA.ORCID http://orcid.org/0000-0002-9915-5138
Miki NakajimaDepartment of Earth and Environmental Sciences, University of Rochester, Rochester, NY 14627, USA.ORCID http://orcid.org/0000-0001-5014-0448
Clive R NealDepartment of Civil and Environmental Engineering and Earth Sciences, University of Notre Dame, Notre Dame, IN 46556, USA.ORCID http://orcid.org/0000-0003-0705-3490
Tinghong ZhouDepartment of Earth and Environmental Sciences, University of Rochester, Rochester, NY 14627, USA.ORCID http://orcid.org/0000-0001-7460-8957
Mauricio Ibanez-MejiaDepartment of Geosciences, University of Arizona, Tucson, AZ 85721, USA.ORCID http://orcid.org/0000-0002-7839-2425
Hirokuni OdaResearch Institute of Geology and Geoinformation, Geological Survey of Japan, National Institute of Advanced Industrial Science and Technology (AIST), Tsukuba 305-8567, Japan.ORCID http://orcid.org/0000-0001-7142-9208
Ben CrumminsDepartment of Earth and Environmental Sciences, University of Rochester, Rochester, NY 14627, USA.ORCID http://orcid.org/0000-0002-7078-9612
University of Rochester · USPlanetary Science Institute · USGeological Survey of Japan · JPMichigan Technological University · USUniversity of Arizona · USUniversity of Liverpool · GBUniversity of Notre Dame · US

Funding

Shared Services Center NASA 80NSSC18K0510
6 · The paper itself

Abstract

Determining the presence or absence of a past long-lived lunar magnetic field is crucial for understanding how the Moon's interior and surface evolved. Here, we show that Apollo impact glass associated with a young 2 million-year-old crater records a strong Earth-like magnetization, providing evidence that impacts can impart intense signals to samples recovered from the Moon and other planetary bodies. Moreover, we show that silicate crystals bearing magnetic inclusions from Apollo samples formed at ∼3.9, 3.6, 3.3, and 3.2 billion years ago are capable of recording strong core dynamo-like fields but do not. Together, these data indicate that the Moon did not have a long-lived core dynamo. As a result, the Moon was not sheltered by a sustained paleomagnetosphere, and the lunar regolith should hold buried

Identifiers

PMID34348904
PMCPMC8336955
OpenAlexW3187908226

What OpenQuestion holds

Textmetadata
LicenceCC BY-NC
Read underepoch 390

Registered trials

None linked

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.