Evidence map›Paper›PMID 41253936›Full record

ArticleScientific reports2025

Photostability of polycyclic aromatic hydrocarbons in hydrated magnesium sulfate under Martian ultraviolet irradiation to assist organics detection on Mars.

Andrew Alberini, Teresa Fornaro, Cristina García-Florentino, Giovanni Poggiali, Sole Biancalani, Francesco Renzi, Tommaso Grazioso, Nicola Tasinato, Daniela Alvarado Jiménez, Álvaro Vicente-Retortillo and 14 more

Abstract read
In one paragraph

Article in Scientific reports, 2025. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 2 papers.

0numbers the graph read from it
0cells of the map it votes in
2citing 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

2 citing papers in PubMed.

  1. Review
  2. 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

24 authors.

Andrew AlberiniINAF- Astrophysical Observatory of Arcetri, L.go E. Fermi 5, Firenze, 50125, Italy. andrew.alberini@inaf.it.
Teresa FornaroINAF- Astrophysical Observatory of Arcetri, L.go E. Fermi 5, Firenze, 50125, Italy.
Cristina García-FlorentinoINAF- Astrophysical Observatory of Arcetri, L.go E. Fermi 5, Firenze, 50125, Italy.
Giovanni PoggialiINAF- Astrophysical Observatory of Arcetri, L.go E. Fermi 5, Firenze, 50125, Italy.
Sole BiancalaniINAF- Astrophysical Observatory of Arcetri, L.go E. Fermi 5, Firenze, 50125, Italy.
Francesco RenziINAF- Astrophysical Observatory of Arcetri, L.go E. Fermi 5, Firenze, 50125, Italy.
Tommaso GraziosoUniversity of Urbino Carlo Bo, Urbino (PU), Piazza Rinascimento 6, Urbino , 61029, Italy.
Nicola TasinatoScuola Normale Superiore, Pisa, Italy.
Daniela Alvarado JiménezScuola Normale Superiore, Pisa, Italy.
Álvaro Vicente-RetortilloCentro de Astrobiología (CAB), CSIC-INTA, Torrejón de Ardoz, Spain.
Maurizio BecucciDepartment of Chemistry, 'Ugo Schiff' - University of Florence, via della Lastruccia 3-13, Sesto Fiorentino (FI), 50019, Italy.
Edward A CloutisCentre for Terrestrial and Planetary Exploration, University of Winnipeg, Winnipeg, MB, R3B 2E9, Canada.
Stephanie ConnellDepartment of Earth, Atmospheric, and Planetary Sciences, Purdue University, Hampton Hall 550 Stadium Mall Drive, West Lafayette, IN, 47907, USA.
Giorgio FamigliniUniversity of Urbino Carlo Bo, Urbino (PU), Piazza Rinascimento 6, Urbino , 61029, Italy.
Achille CappielloUniversity of Urbino Carlo Bo, Urbino (PU), Piazza Rinascimento 6, Urbino , 61029, Italy.
Germán M MartinezLunar and Planetary Institute, Universities Space Research Association, Houston, TX, USA.
Mariano BattistuzziINAF- Astrophysical Observatory of Arcetri, L.go E. Fermi 5, Firenze, 50125, Italy.
Christian LorenzINAF- Astrophysical Observatory of Arcetri, L.go E. Fermi 5, Firenze, 50125, Italy.
Andrew SteeleCarnegie Institute for Science, Washington, DC, USA.
Jesús Martínez-FríasInstitute of Geosciences, IGEO (CSIC-UCM), Madrid, Spain.
Felipe GómezCentro de Astrobiología (CAB), CSIC-INTA, Torrejón de Ardoz, Spain.
Roger C WiensDepartment of Earth, Atmospheric, and Planetary Sciences, Purdue University, Hampton Hall 550 Stadium Mall Drive, West Lafayette, IN, 47907, 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, Firenze, 50125, Italy.

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

The Scanning Habitable Environments with Raman and Luminescence for Organics and Chemicals (SHERLOC) instrument, which is mounted on the Mars 2020 Perseverance rover, detected Raman signals in spectral regions relevant to organics, plausibly polycyclic aromatic hydrocarbons (PAHs), co-located with sulfate minerals, in the Quartier abrasion of the Issole outcrop in the Jezero crater floor on Mars. In order to ascertain the plausibility of the organic origin of these signals, it is essential to determine whether organics can withstand the effects of ambient Martian ultraviolet (UV) radiation after they are exposed by the Perseverance's abrasion tool and prior to the analysis by SHERLOC. In this work, the stability under Martian-like UV irradiation of PAHs like 2,6-dihydroxynaphthalene and benzo[a]pyrene in hydrated magnesium sulfate, one of the main sulfate phases present in Quartier, is investigated. Our findings indicate that the spectroscopic features of 2,6-dihydroxynaphthalene and benzo[a]pyrene in hydrated magnesium sulfate remain unaltered when exposed to UV radiation comparable to that experienced at Jezero crater over a period of dozens of Martian days (or sols). Consequently, due to the photoprotective properties of this mineral, after the abrasion exposes them to the radiation, these compounds can still be detectable by the SHERLOC measurement and also by SuperCam because some organic bands fall in its infrared spectral range. In addition, photoproducts due to the UV exposure for both PAHs were detected. These results corroborate the hypothesis that the Raman signals detected by SHERLOC co-located with sulfates may arise from organic compounds.

Indexed as

FTIR spectroscopyMars 2020 perseverance rover missionPolycyclic aromatic hydrocarbonsUV irradiation

Identifiers

PMID41253936
PMCPMC12627640

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