Evidence map›Paper›PMID 32457325›Full record

ArticleNature communications2020

A steeply-inclined trajectory for the Chicxulub impact.

G S Collins, N Patel, T M Davison, A S P Rae, J V Morgan, S P S Gulick, IODP-ICDP Expedition 364 Science Party, Third-Party Scientists

Open access · goldAbstract read
In one paragraph

Article in Nature communications, 2020. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 7 papers.

0numbers the graph read from it
0cells of the map it votes in
7citing papers in PubMed
8.3field-weighted citation impact, top 2% 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

7 citing papers in PubMed, 95 citations in OpenAlex.

  1. Article
  2. Article
  3. ProlongedNature communications · 2025
    Article
  4. Article
  5. Article
  6. Article
  7. Organic matter from the Chicxulub crater exacerbated the K-Pg impact winter.Proceedings of the National Academy of Sciences of the United States of America · 2020
    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

8 authors at 20 institutions in 11 countries.

G S CollinsDepartment Earth Science and Engineering, Imperial College London, London, SW7 2AZ, UK. g.collins@imperial.ac.uk.ORCID http://orcid.org/0000-0002-6087-6149
N PatelDepartment Earth Science and Engineering, Imperial College London, London, SW7 2AZ, UK.ORCID http://orcid.org/0000-0001-8744-4461
T M DavisonDepartment Earth Science and Engineering, Imperial College London, London, SW7 2AZ, UK.ORCID http://orcid.org/0000-0001-8790-873X
A S P RaeDepartment Earth Science and Engineering, Imperial College London, London, SW7 2AZ, UK.
J V MorganDepartment Earth Science and Engineering, Imperial College London, London, SW7 2AZ, UK.
S P S GulickInstitute for Geophysics and Department of Geological Sciences, University of Texas at Austin, Austin, TX, 78758, USA.ORCID http://orcid.org/0000-0003-4740-9068
IODP-ICDP Expedition 364 Science Party
Third-Party Scientists
Imperial College London · GBPennsylvania State University · USJapan Agency for Marine-Earth Science and Technology · JPUniversity of Freiburg · DEAlfred-Wegener-Institut Helmholtz-Zentrum für Polar- und Meeresforschung · DECentre National de la Recherche Scientifique · FRLaboratoire de Physico-Chimie de l'Atmosphère · FRRutgers, The State University of New Jersey · USThe University of Texas at Austin · USToho University · JPUniversity of Alaska Fairbanks · USVrije Universiteit Brussel · BEChina University of Geosciences · CNCurtin University · AUGeoRessources · FRNatural History Museum Vienna · ATPlanetary Science Institute · USScottish Universities Environmental Research Centre · GBUniversität Hamburg · DEUniversity of Utah · US

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

The environmental severity of large impacts on Earth is influenced by their impact trajectory. Impact direction and angle to the target plane affect the volume and depth of origin of vaporized target, as well as the trajectories of ejected material. The asteroid impact that formed the 66 Ma Chicxulub crater had a profound and catastrophic effect on Earth's environment, but the impact trajectory is debated. Here we show that impact angle and direction can be diagnosed by asymmetries in the subsurface structure of the Chicxulub crater. Comparison of 3D numerical simulations of Chicxulub-scale impacts with geophysical observations suggests that the Chicxulub crater was formed by a steeply-inclined (45-60° to horizontal) impact from the northeast; several lines of evidence rule out a low angle (<30°) impact. A steeply-inclined impact produces a nearly symmetric distribution of ejected rock and releases more climate-changing gases per impactor mass than either a very shallow or near-vertical impact.

Identifiers

PMID32457325
PMCPMC7251121
OpenAlexW3028706033

What OpenQuestion holds

Textmetadata
LicenceCC BY
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.