Evidence map›Paper›PMID 39866548›Full record

ArticleNature astronomy2025

Evidence of a 4.33 billion year age for the Moon's South Pole-Aitken basin.

K H Joy, N Wang, J F Snape, A Goodwin, J F Pernet-Fisher, M J Whitehouse, Y Liu, Y T Lin, J R Darling, P Tar and 1 more

Abstract read
In one paragraph

Article in Nature astronomy, 2025. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 11 papers.

0numbers the graph read from it
0cells of the map it votes in
11citing 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

11 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

11 authors.

K H JoyDepartment of Earth and Environmental Sciences, The University of Manchester, Manchester, UK.ORCID 0000-0003-4992-8750
N WangInstitute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China.
J F SnapeDepartment of Earth and Environmental Sciences, The University of Manchester, Manchester, UK.ORCID 0000-0002-1804-420X
A GoodwinDepartment of Earth and Environmental Sciences, The University of Manchester, Manchester, UK.ORCID 0000-0003-2839-629X
J F Pernet-FisherDepartment of Earth and Environmental Sciences, The University of Manchester, Manchester, UK.
M J WhitehouseDepartment of Geosciences, Swedish Museum of Natural History, Stockholm, Sweden.ORCID 0000-0003-2227-577X
Y LiuInstitute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China.
Y T LinInstitute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China.ORCID 0000-0002-3407-4329
J R DarlingSchool of the Environment, Geography and Geosciences, University of Portsmouth, Portsmouth, UK.ORCID 0000-0003-2763-6634
P TarPreviously at the School of Health Sciences, Faculty of Biology, Medicine and Health, The University of Manchester, Manchester, UK.
R TartèseDepartment of Earth and Environmental Sciences, The University of Manchester, Manchester, UK.ORCID 0000-0002-3490-9875

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

The Moon's farside South Pole-Aitken (SPA) basin is the largest and oldest visible impact basin in the inner Solar System. Determining the timing of this catastrophic event is key to understanding the onset of the lunar basin-forming epoch, with implications for understanding the impact bombardment history of the inner Solar System. Despite this, the formation age of the SPA basin remains poorly constrained. Here we show that the chemical composition of the lunar meteorite Northwest Africa 2995 is in good agreement with lithologies exposed within the southern region of the SPA basin. Radiometric dating of a range of mineral and rock components in Northwest Africa 2995 yielded consistent dates of ~4.32-4.33 billion years old. We interpret these dates as the age of SPA basin formation, inferring that this event occurred ~120 million years before the formation of the main cluster of lunar impact basins between ~4.2 Ga and 3.8 Ga. This weakens support for a narrow period of lunar late heavy impact bombardment and also implies that the earliest formed impact basins on the Moon (that is, >4.33-4.5 Ga old) were erased either by the SPA impact itself when its formation caused massive resurfacing of the lunar surface or through other geological processes.

Indexed as

Inner planetsMeteoriticsMineralogyPetrology

Identifiers

PMID39866548
PMCPMC11757148

What OpenQuestion holds

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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.