Evidence map›Paper›PMID 38941463›Full record

ArticleScience advances2024

Seismically detected cratering on Mars: Enhanced recent impact flux?

Ingrid J Daubar, Raphaël F Garcia, Alexander E Stott, Benjamin Fernando, Gareth S Collins, Colin M Dundas, Natalia Wójcicka, Géraldine Zenhäusern, Alfred S McEwen, Simon C Stähler and 5 more

Abstract read
In one paragraph

Article in Science advances, 2024. 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. Extensive Secondary Cratering From the InSight Sol 1034a Impact Event.Journal of geophysical research. Planets · 2024
    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

15 authors.

Ingrid J DaubarDepartment of Earth, Environmental, and Planetary Sciences, Brown University, Providence, RI 02912, USA.ORCID 0000-0001-9790-2972
Raphaël F GarciaInstitut Supérieur de l'Aéronautique et de l'Espace (ISAE-SUPAERO), Université de Toulouse, 10 Avenue Edouard Belin, 31400 Toulouse, France.ORCID 0000-0003-1460-6663
Alexander E StottInstitut Supérieur de l'Aéronautique et de l'Espace (ISAE-SUPAERO), Université de Toulouse, 10 Avenue Edouard Belin, 31400 Toulouse, France.ORCID 0000-0001-6121-705X
Benjamin FernandoDepartment of Physics, University of Oxford, Oxford OX1 2JD, UK.ORCID 0000-0002-7321-8401
Gareth S CollinsImperial College London, South Kensington Campus, London SW7 2AZ, UK.ORCID 0000-0002-6087-6149
Colin M DundasU.S. Geological Survey, Astrogeology Science Center, 2255 N. Gemini Dr, Flagstaff, AZ 86001, USA.ORCID 0000-0003-2343-7224
Natalia WójcickaImperial College London, South Kensington Campus, London SW7 2AZ, UK.ORCID 0000-0001-9265-8931
Géraldine ZenhäusernInstitute of Geophysics, ETH Zürich, Sonneggstrasse 5, 8092 Zürich, Switzerland.ORCID 0000-0001-9401-4910
Alfred S McEwenLunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA.
Simon C StählerInstitute of Geophysics, ETH Zürich, Sonneggstrasse 5, 8092 Zürich, Switzerland.ORCID 0000-0002-0783-2489
Matthew GolombekJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.ORCID 0000-0002-1928-2293
Constantinos CharalambousImperial College London, South Kensington Campus, London SW7 2AZ, UK.ORCID 0000-0002-9139-3895
Domenico GiardiniInstitute of Geophysics, ETH Zürich, Sonneggstrasse 5, 8092 Zürich, Switzerland.ORCID 0000-0002-5573-7638
Philippe LognonnéUniversité Paris Cité, Institut de Physique du Globe de Paris, CNRS, F-75005 Paris, France.ORCID 0000-0002-1014-920X
W Bruce BanerdtJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.ORCID 0000-0003-3125-1542

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

Seismic observations of impacts on Mars indicate a higher impact flux than previously measured. Using six confirmed seismic impact detections near the NASA InSight lander and two distant large impacts, we calculate appropriate scalings to compare these rates with lunar-based chronology models. We also update the impact rate from orbital observations using the most recent catalog of new craters on Mars. The snapshot of the current impact rate at Mars recorded seismically is higher than that found using orbital detections alone. The measured rates differ between a factor of 2 and 10, depending on the diameter, although the sample size of seismically detected impacts is small. The close timing of the two largest new impacts found on Mars in the past few decades indicates either a heightened impact rate or a low-probability temporal coincidence, perhaps representing recent fragmentation of a parent body. We conclude that seismic methods of detecting current impacts offer a more complete dataset than orbital imaging.

Identifiers

PMID38941463
PMCPMC11212728

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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.