Evidence map›Paper›PMID 33568485›Full record

ArticleScience advances2021

Transient HCl in the atmosphere of Mars.

Oleg Korablev, Kevin S Olsen, Alexander Trokhimovskiy, Franck Lefèvre, Franck Montmessin, Anna A Fedorova, Michael J Toplis, Juan Alday, Denis A Belyaev, Andrey Patrakeev and 16 more

Open access · goldAbstract read
In one paragraph

Article in Science advances, 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
8.6field-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

3 citing papers in PubMed, 68 citations in OpenAlex.

  1. Article
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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

26 authors at 9 institutions in 7 countries.

Oleg KorablevSpace Research Institute (IKI), Moscow, Russia. korab@iki.rssi.ru.ORCID http://orcid.org/0000-0003-1115-0656
Kevin S OlsenDepartment of Physics, University of Oxford, Oxford, UK.ORCID http://orcid.org/0000-0002-2173-9889
Alexander TrokhimovskiySpace Research Institute (IKI), Moscow, Russia.ORCID http://orcid.org/0000-0003-4041-4972
Franck LefèvreLaboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS/CNRS), Paris, France.ORCID http://orcid.org/0000-0001-5294-5426
Franck MontmessinLaboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS/CNRS), Paris, France.ORCID http://orcid.org/0000-0002-4187-1457
Anna A FedorovaSpace Research Institute (IKI), Moscow, Russia.ORCID http://orcid.org/0000-0002-4176-2955
Michael J ToplisL'Institut de Recherche en Astrophysique et Planétologie (IRAP/CNRS), Toulouse, France.
Juan AldayDepartment of Physics, University of Oxford, Oxford, UK.ORCID http://orcid.org/0000-0003-1459-3444
Denis A BelyaevSpace Research Institute (IKI), Moscow, Russia.ORCID http://orcid.org/0000-0003-1123-5983
Andrey PatrakeevSpace Research Institute (IKI), Moscow, Russia.ORCID http://orcid.org/0000-0003-3587-5758
Nikolay I IgnatievSpace Research Institute (IKI), Moscow, Russia.ORCID http://orcid.org/0000-0002-6358-7094
Alexey V ShakunSpace Research Institute (IKI), Moscow, Russia.ORCID http://orcid.org/0000-0002-6368-787X
Alexey V GrigorievSpace Research Institute (IKI), Moscow, Russia.ORCID http://orcid.org/0000-0003-1331-1986
Lucio BaggioLaboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS/CNRS), Paris, France.ORCID http://orcid.org/0000-0002-9263-4937
Irbah AbdenourLaboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS/CNRS), Paris, France.ORCID http://orcid.org/0000-0003-3265-3148
Gaetan LacombeLaboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS/CNRS), Paris, France.ORCID http://orcid.org/0000-0001-7505-4140
Yury S IvanovMain Astronomical Observatory (MAO NASU), Kyiv, Ukraine.
Shohei AokiLPAP, STAR Institute, Université de Liège, Liège, Belgium.ORCID http://orcid.org/0000-0001-6727-125X
Ian R ThomasRoyal Belgian Institute of Space Aeronomy (BIRA-IASB), Brussels, Belgium.ORCID http://orcid.org/0000-0003-3887-6668
Frank DaerdenRoyal Belgian Institute of Space Aeronomy (BIRA-IASB), Brussels, Belgium.ORCID http://orcid.org/0000-0001-7433-1839
Bojan RisticRoyal Belgian Institute of Space Aeronomy (BIRA-IASB), Brussels, Belgium.ORCID http://orcid.org/0000-0002-9635-1125
Justin T ErwinRoyal Belgian Institute of Space Aeronomy (BIRA-IASB), Brussels, Belgium.ORCID http://orcid.org/0000-0003-0200-3195
Manish PatelOpen University, Milton-Keynes, UK.ORCID http://orcid.org/0000-0002-8223-3566
Giancarlo BellucciIstituto di Astrofisica e Planetologia Spaziali (IAPS-INAF), Rome, Italy.ORCID http://orcid.org/0000-0003-0867-8679
Jose-Juan Lopez-MorenoInstituto de Astrofìsica de Andalucía (IAA/CSIC), Granada, Spain.ORCID http://orcid.org/0000-0002-7946-2624
Ann C VandaeleRoyal Belgian Institute of Space Aeronomy (BIRA-IASB), Brussels, Belgium.ORCID http://orcid.org/0000-0001-8940-9301
Space Research Institute · RUCentre National de la Recherche Scientifique · FRRoyal Belgian Institute for Space Aeronomy · BEUniversity of Oxford · GBInstitute for Space Astrophysics and Planetology · ITInstituto de Astrofísica de Andalucía · ESMain Astronomical Observatory · UAThe Open University · GBUniversity of Liège · BE

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

A major quest in Mars' exploration has been the hunt for atmospheric gases, potentially unveiling ongoing activity of geophysical or biological origin. Here, we report the first detection of a halogen gas, HCl, which could, in theory, originate from contemporary volcanic degassing or chlorine released from gas-solid reactions. Our detections made at ~3.2 to 3.8 μm with the Atmospheric Chemistry Suite and confirmed with Nadir and Occultation for Mars Discovery instruments onboard the ExoMars Trace Gas Orbiter, reveal widely distributed HCl in the 1- to 4-ppbv range, 20 times greater than previously reported upper limits. HCl increased during the 2018 global dust storm and declined soon after its end, pointing to the exchange between the dust and the atmosphere. Understanding the origin and variability of HCl shall constitute a major advance in our appraisal of martian geo- and photochemistry.

Identifiers

PMID33568485
PMCPMC7875523
OpenAlexW3128829181

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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.