Evidence map›Paper›PMID 34521860›Full record

ArticleNature communications2021

Large impact cratering during lunar magma ocean solidification.

K Miljković, M A Wieczorek, M Laneuville, A Nemchin, P A Bland, M T Zuber

Abstract read
In one paragraph

Article in Nature communications, 2021. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 3 papers.

0numbers the graph read from it
0cells of the map it votes in
3citing 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

3 citing papers in PubMed.

  1. Article
  2. Article
  3. Article
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

6 authors.

K MiljkovićCurtin University, School of Earth and Planetary Science, Space Science and Technology Centre, Perth, WA, Australia. katarina.miljkovic@curtin.edu.au.ORCID http://orcid.org/0000-0001-8644-8903
M A WieczorekUniversité Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, Nice, France.
M LaneuvilleEarth-Life Science Institute, Tokyo, Japan.ORCID http://orcid.org/0000-0001-6022-0046
A NemchinCurtin University, School of Earth and Planetary Science, Space Science and Technology Centre, Perth, WA, Australia.
P A BlandCurtin University, School of Earth and Planetary Science, Space Science and Technology Centre, Perth, WA, Australia.
M T ZuberMassachusetts Institute of Technology, Cambridge, MA, USA.ORCID http://orcid.org/0000-0003-2652-8017

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

The lunar cratering record is used to constrain the bombardment history of both the Earth and the Moon. However, it is suggested from different perspectives, including impact crater dating, asteroid dynamics, lunar samples, impact basin-forming simulations, and lunar evolution modelling, that the Moon could be missing evidence of its earliest cratering record. Here we report that impact basins formed during the lunar magma ocean solidification should have produced different crater morphologies in comparison to later epochs. A low viscosity layer, mimicking a melt layer, between the crust and mantle could cause the entire impact basin size range to be susceptible to immediate and extreme crustal relaxation forming almost unidentifiable topographic and crustal thickness signatures. Lunar basins formed while the lunar magma ocean was still solidifying may escape detection, which is agreeing with studies that suggest a higher impact flux than previously thought in the earliest epoch of Earth-Moon evolution.

Identifiers

PMID34521860
PMCPMC8440705

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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.