Evidence map›Paper›PMID 42090489›Full record

ArticleScience advances2026

A southward differentiated impactor forms the tapered shape of the South Pole-Aitken impact basin on the Moon.

Shigeru Wakita, Brandon C Johnson, Jeffrey C Andrews-Hanna, Gabriel Gowman, Thomas M Davison, Gareth S Collins, Carys A Bill, Simone Marchi, Amanda M Alexander, William F Bottke and 1 more

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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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0citing papers 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

The trial behind it

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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

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

11 authors.

Shigeru WakitaDepartment of Earth, Atmospheric, and Planetary Sciences, Purdue University, West Lafayette, IN, USA.ORCID 0000-0002-3161-3454
Brandon C JohnsonDepartment of Earth, Atmospheric, and Planetary Sciences, Purdue University, West Lafayette, IN, USA.ORCID 0000-0002-4267-093X
Jeffrey C Andrews-HannaLunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA.ORCID 0000-0001-9374-7776
Gabriel GowmanLunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA.ORCID 0000-0002-0644-2956
Thomas M DavisonDepartment of Earth Science and Engineering, Imperial College London, London, UK.ORCID 0000-0001-8790-873X
Gareth S CollinsDepartment of Earth Science and Engineering, Imperial College London, London, UK.ORCID 0000-0002-6087-6149
Carys A BillDepartment of Earth Science and Engineering, Imperial College London, London, UK.ORCID 0009-0007-0584-6274
Simone MarchiSouthwest Research Institute, Boulder, CO, USA.ORCID 0000-0003-2548-3291
Amanda M AlexanderSouthwest Research Institute, Boulder, CO, USA.ORCID 0000-0003-0193-9151
William F BottkeSouthwest Research Institute, Boulder, CO, USA.ORCID 0000-0002-1804-7814
Alexander J EvansBlue Hill Observatory and Science Center, Milton, MA.ORCID 0000-0002-3644-1313

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

The South Pole-Aitken (SPA) basin-forming impact was a critical event in the Moon's history. Despite being the oldest and largest acknowledged basin, critical details including the impactor's size, nature, direction, and fate of the ejecta remain uncertain. Here, we simulate SPA's formation and resultant crustal structure. We find that SPA's observed shape of an ellipse tapered toward the south is best reproduced by a 260-km-diameter differentiated impactor striking with a north-to-south trajectory. In this scenario, the impact disperses lunar mantle materials in the cross-range and the downrange directions away from the lunar farside. Much of the mantle ejecta collapses into the basin interior, consistent with the distribution inferred from gravity. These results suggest that the Artemis landing sites near the lunar south pole should contain abundant SPA ejecta including mantle materials. Samples returned from these regions should therefore reveal the age of SPA and the composition of the lunar mantle.

Identifiers

PMID42090489
PMCPMC13148301

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Registered trials

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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.