Evidence map›Paper›PMID 38987581›Full record

ArticleScientific reports2024

Investigating the stability of aromatic carboxylic acids in hydrated magnesium sulfate under UV irradiation to assist detection of organics on Mars.

Andrew Alberini, Teresa Fornaro, Cristina García-Florentino, Malgorzata Biczysko, Iratxe Poblacion, Julene Aramendia, Juan Manuel Madariaga, Giovanni Poggiali, Álvaro Vicente-Retortillo, Kathleen C Benison and 10 more

Abstract read
In one paragraph

Article in Scientific reports, 2024. 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. Review
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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

20 authors.

Andrew AlberiniINAF- Astrophysical Observatory of Arcetri, L.go E. Fermi 5, 50125, Firenze, Italy. andrew.alberini@inaf.it.
Teresa FornaroINAF- Astrophysical Observatory of Arcetri, L.go E. Fermi 5, 50125, Firenze, Italy. teresa.fornaro@inaf.it.
Cristina García-FlorentinoINAF- Astrophysical Observatory of Arcetri, L.go E. Fermi 5, 50125, Firenze, Italy.
Malgorzata BiczyskoCollege of Science, Shanghai University, 99 Shangda Road, Shanghai, 200444, China.
Iratxe PoblacionDepartment of Analytical Chemistry, University of the Basque Country UPV/EHU, 48080, Bilbao, Spain.
Julene AramendiaDepartment of Analytical Chemistry, University of the Basque Country UPV/EHU, 48080, Bilbao, Spain.
Juan Manuel MadariagaDepartment of Analytical Chemistry, University of the Basque Country UPV/EHU, 48080, Bilbao, Spain.
Giovanni PoggialiINAF- Astrophysical Observatory of Arcetri, L.go E. Fermi 5, 50125, Firenze, Italy.
Álvaro Vicente-RetortilloCentro de Astrobiología (CAB), CSIC-INTA, Torrejón de Ardoz, Spain.
Kathleen C BenisonDepartment of Geology and Geography, West Virginia University, Morgantown, WV, USA.
Sandra SiljeströmRISE Research Institutes of Sweden, Stockholm, Sweden.
Sole BiancalaniINAF- Astrophysical Observatory of Arcetri, L.go E. Fermi 5, 50125, Firenze, Italy.
Christian LorenzINAF- Astrophysical Observatory of Arcetri, L.go E. Fermi 5, 50125, Firenze, Italy.
Edward A CloutisCentre for Terrestrial and Planetary Exploration, University of Winnipeg, Winnipeg, MB, R3B 2E9, Canada.
Dan M ApplinCentre for Terrestrial and Planetary Exploration, University of Winnipeg, Winnipeg, MB, R3B 2E9, Canada.
Felipe GómezCentro de Astrobiología (CAB), CSIC-INTA, Torrejón de Ardoz, Spain.
Andrew SteeleCarnegie Institute for Science, Washington, DC, USA.
Roger C WiensEarth, Atmospheric, and Planetary Sciences, Purdue University, West Lafayette, IN, USA.
Kevin P HandJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.
John R BrucatoINAF- Astrophysical Observatory of Arcetri, L.go E. Fermi 5, 50125, Firenze, Italy.

Funding

Agenzia Spaziale Italiana 2023-3-HHCanadian Space Agency 22EXPCOI4Natural Sciences and Engineering Research Council RGPIN0-2023-03413Spanish Agency for Research PID2022-142750OB-I00Spanish Ministry of Science and Innovation (MCIN) /State Agency of Research (AEI) MCIN/AEI/10.13039/501100011033/FEDER
6 · The paper itself

Abstract

The Scanning Habitable Environments with Raman and Luminescence for Organics and Chemicals (SHERLOC) instrument onboard the Mars 2020 Perseverance rover detected so far some of the most intense fluorescence signals in association with sulfates analyzing abraded patches of rocks at Jezero crater, Mars. To assess the plausibility of an organic origin of these signals, it is key to understand if organics can survive exposure to ambient Martian UV after exposure by the Perseverance abrasion tool and prior to analysis by SHERLOC. In this work, we investigated the stability of organo-sulfate assemblages under Martian-like UV irradiation and we observed that the spectroscopic features of phthalic and mellitic acid embedded into hydrated magnesium sulfate do not change for UV exposures corresponding to at least 48 Martian sols and, thus, should still be detectable in fluorescence when the SHERLOC analysis takes place, thanks to the photoprotective properties of magnesium sulfate. In addition, different photoproduct bands diagnostic of the parent carboxylic acid molecules could be observed. The photoprotective behavior of hydrated magnesium sulfate corroborates the hypothesis that sulfates might have played a key role in the preservation of organics on Mars, and that the fluorescence signals detected by SHERLOC in association with sulfates could potentially arise from organic compounds.

Indexed as

Aromatic organic compoundsFTIR spectroscopyMars 2020 Perseverance missionSigns of biological activityUV irradiation

Identifiers

PMID38987581
PMCPMC11237158

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