Evidence map›Paper›PMID 33568473›Full record

ArticleScience advances2021

Water heavily fractionated as it ascends on Mars as revealed by ExoMars/NOMAD.

Geronimo L Villanueva, Giuliano Liuzzi, Matteo M J Crismani, Shohei Aoki, Ann Carine Vandaele, Frank Daerden, Michael D Smith, Michael J Mumma, Elise W Knutsen, Lori Neary and 9 more

Abstract 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 4 papers.

0numbers the graph read from it
0cells of the map it votes in
4citing 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

4 citing papers in PubMed.

  1. Article
  2. Article
  3. Article
  4. Biotechnological potentials of halophilic microorganisms and their impact on mankind.Beni-Suef University journal of basic and applied sciences · 2022
    Review
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

19 authors.

Geronimo L VillanuevaNASA Goddard Space Flight Center, Greenbelt, MD, USA. geronimo.villanueva@nasa.gov.ORCID http://orcid.org/0000-0002-2662-5776
Giuliano LiuzziNASA Goddard Space Flight Center, Greenbelt, MD, USA.ORCID http://orcid.org/0000-0003-3638-5750
Matteo M J CrismaniNPP/USRA, Goddard Space Flight Center, Greenbelt, MD, USA.ORCID http://orcid.org/0000-0003-3127-2466
Shohei AokiRoyal Belgian Institute for Space Aeronomy, Brussels, Belgium.ORCID http://orcid.org/0000-0001-6727-125X
Ann Carine VandaeleCalifornia State University, San Bernardino, Department of Physics, CA USA.ORCID http://orcid.org/0000-0001-8940-9301
Frank DaerdenCalifornia State University, San Bernardino, Department of Physics, CA USA.ORCID http://orcid.org/0000-0001-7433-1839
Michael D SmithNASA Goddard Space Flight Center, Greenbelt, MD, USA.ORCID http://orcid.org/0000-0002-7601-1158
Michael J MummaNASA Goddard Space Flight Center, Greenbelt, MD, USA.
Elise W KnutsenNASA Goddard Space Flight Center, Greenbelt, MD, USA.ORCID http://orcid.org/0000-0002-7702-2844
Lori NearyRoyal Belgian Institute for Space Aeronomy, Brussels, Belgium.ORCID http://orcid.org/0000-0001-6773-324X
Sebastien ViscardyRoyal Belgian Institute for Space Aeronomy, Brussels, Belgium.ORCID http://orcid.org/0000-0002-5608-7438
Ian R ThomasRoyal Belgian Institute for Space Aeronomy, Brussels, Belgium.ORCID http://orcid.org/0000-0003-3887-6668
Miguel Angel Lopez-ValverdeInstituto de Astrofísica de Andalucía, Granada, Spain.ORCID http://orcid.org/0000-0002-7989-4267
Bojan RisticRoyal Belgian Institute for Space Aeronomy, Brussels, Belgium.ORCID http://orcid.org/0000-0002-9635-1125
Manish R PatelOpen University, Milton Keynes UK.ORCID http://orcid.org/0000-0002-8223-3566
James A HolmesOpen University, Milton Keynes UK.ORCID http://orcid.org/0000-0003-3018-2135
Giancarlo BellucciIstituto di Astrofisica e Planetologia, Rome, Italy.ORCID http://orcid.org/0000-0003-0867-8679
Jose Juan Lopez-MorenoInstituto de Astrofísica de Andalucía, Granada, Spain.ORCID http://orcid.org/0000-0002-7946-2624
NOMAD team

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

Isotopic ratios and, in particular, the water D/H ratio are powerful tracers of the evolution and transport of water on Mars. From measurements performed with ExoMars/NOMAD, we observe marked and rapid variability of the D/H along altitude on Mars and across the whole planet. The observations (from April 2018 to April 2019) sample a broad range of events on Mars, including a global dust storm, the evolution of water released from the southern polar cap during southern summer, the equinox phases, and a short but intense regional dust storm. In three instances, we observe water at very high altitudes (>80 km), the prime region where water is photodissociated and starts its escape to space. Rayleigh distillation appears the be the driving force affecting the D/H in many cases, yet in some instances, the exchange of water reservoirs with distinctive D/H could be responsible.

Identifiers

PMID33568473
PMCPMC7875534

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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.