Evidence map›Paper›PMID 40354557›Full record

ArticleProceedings of the National Academy of Sciences of the United States of America2025

Ultraviolet and biological effective dose observations at Gale Crater, Mars.

Daniel Viúdez-Moreiras, Maria-Paz Zorzano, Mark T Lemmon, Alberto G Fairén, Alfonso Saiz-Lopez, Michael D Smith

Abstract read
In one paragraph

Article in Proceedings of the National Academy of Sciences of the United States of America, 2025. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 1 paper.

0numbers the graph read from it
0cells of the map it votes in
1citing 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

1 citing paper in PubMed.

  1. Evidence of an enhanced near-surface ozone layer at tropical latitudes on Mars.Proceedings of the National Academy of Sciences of the United States of America · 2025
    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.

Daniel Viúdez-MoreirasCentro de Astrobiología, Spanish National Research Council - National Institute for Aerospace Technology, Torrejón de Ardoz, Madrid 28850, Spain.ORCID 0000-0001-8442-3788
Maria-Paz ZorzanoCentro de Astrobiología, Spanish National Research Council - National Institute for Aerospace Technology, Torrejón de Ardoz, Madrid 28850, Spain.ORCID 0000-0002-4492-9650
Mark T LemmonSpace Science Institute, Boulder, CO 80301.
Alberto G FairénCentro de Astrobiología, Spanish National Research Council - National Institute for Aerospace Technology, Torrejón de Ardoz, Madrid 28850, Spain.ORCID 0000-0002-2938-6010
Alfonso Saiz-LopezDepartment of Atmospheric Chemistry and Climate, Institute of Physical Chemistry Blas Cabrera, CSIC, Madrid 28006, Spain.ORCID 0000-0002-0060-1581
Michael D SmithNational Aeronautics and Space Administration Goddard Spaceflight Center, Greenbelt, MD 20771.

Funding

EU ERC818602Spanish Ministry of Science, Innovation and Universities PID2022-140180OB-C21
6 · The paper itself

Abstract

The incident ultraviolet (UV) irradiance on the surface of Mars is strongly sterilizing and plays a critical role in atmospheric and near-surface photochemistry. The Rover Environmental Monitoring Station (REMS) instrument, which includes the first UV sensor sent to Mars on board the Curiosity rover, has been measuring the UV irradiance at Gale Crater since 2012, providing ground-truth data regarding seasonal and short-term variability of the UV radiation at the surface of another planet. Here, we analyze the REMS UV measurements for a period of >5 Martian years to retrieve biological effective doses and other UV radiation quantities on the planetary surface that are key for different physicochemical processes. Our results reveal a previously unidentified complex UV radiation environment on the Martian surface, with dramatic short-term fluctuations capable of changing UV radiation doses by >30% in a few sols. We assess the viability of terrestrial microorganisms exposed to this UV radiation field and dispersed through the Martian atmosphere from a robotic spacecraft or human habitat. Our findings show that reducing microbial viability by 99% would require several hours of exposure to the Martian environment including during the daytime, a finding that may call for a reinforcement of planetary protection policies.

Indexed as

Extraterrestrial EnvironmentMarsUltraviolet RaysHumansbiological effective dosesMars atmosphereUV radiation

Identifiers

PMID40354557
PMCPMC12130865

What OpenQuestion holds

Textmetadata
LicenceCC BY-NC-ND
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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.