Evidence map›Paper›PMID 39321302›Full record

ArticleScience advances2024

Inorganic interpretation of luminescent materials encountered by the Perseverance rover on Mars.

Eva L Scheller, Tanja Bosak, Francis M McCubbin, Kenneth Williford, Sandra Siljeström, Ryan S Jakubek, Scott A Eckley, Richard V Morris, Sergei V Bykov, Tanya Kizovski and 24 more

Abstract read
In one paragraph

Article in Science advances, 2024. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 5 papers.

0numbers the graph read from it
0cells of the map it votes in
5citing 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

5 citing papers in PubMed.

  1. Article
  2. Review
  3. Article
  4. Article
  5. 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

34 authors.

Eva L SchellerDepartment of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA.ORCID 0000-0002-9981-5802
Tanja BosakDepartment of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA.ORCID 0000-0001-5179-5323
Francis M McCubbinAstromaterials Research and Exploration Science Division, NASA Johnson Space Center, Houston, TX 77058, USA.ORCID 0000-0002-2101-4431
Kenneth WillifordBlue Marble Space Institute of Science, Seattle, WA 98104, USA.ORCID 0000-0003-0633-408X
Sandra SiljeströmRISE Research Institutes of Sweden, Stockholm, Sweden.ORCID 0000-0002-4975-6074
Ryan S JakubekJacobs, NASA Johnson Space Center, Houston, TX 77058, USA.ORCID 0000-0001-7880-9422
Scott A EckleyJacobs, NASA Johnson Space Center, Houston, TX 77058, USA.ORCID 0000-0002-2692-2164
Richard V MorrisAstromaterials Research and Exploration Science Division, NASA Johnson Space Center, Houston, TX 77058, USA.ORCID 0000-0003-1413-4002
Sergei V BykovDepartment of Chemistry, University of Pittsburgh, Pittsburgh, PA 15260, USA.ORCID 0000-0002-6161-0027
Tanya KizovskiDepartment of Earth Sciences, Brock University, St. Catharines, ON, Canada.ORCID 0000-0001-8188-9769
Sanford AsherDepartment of Chemistry, University of Pittsburgh, Pittsburgh, PA 15260, USA.ORCID 0000-0003-1061-8747
Eve BergerAstromaterials Research and Exploration Science Division, NASA Johnson Space Center, Houston, TX 77058, USA.ORCID 0000-0002-9902-439X
Dina M BowerDepartment of Astronomy, University of Maryland, College Park, MD 20742, USA.ORCID 0000-0002-4275-1318
Emily L CardarelliDepartment of Earth, Planetary and Space Sciences, University of California Los Angeles, Los Angeles, CA 90095, USA.ORCID 0000-0001-5451-2309
Bethany L EhlmannDivision of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA.ORCID 0000-0002-2745-3240
Teresa FornaroAstrophysical Observatory of Arcetri, INAF, Florence, Italy.ORCID 0000-0001-7705-9658
Allison FoxJacobs, NASA Johnson Space Center, Houston, TX 77058, USA.ORCID 0000-0002-5952-4170
Nikole HaneyJacobs, NASA Johnson Space Center, Houston, TX 77058, USA.ORCID 0000-0001-5405-3616
Kevin HandJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91011, USA.ORCID 0000-0002-3225-9426
Ryan RoppelDepartment of Chemistry, University of Pittsburgh, Pittsburgh, PA 15260, USA.ORCID 0000-0002-1782-1388
Sunanda SharmaJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91011, USA.ORCID 0000-0001-8822-7960
Andrew SteeleEarth and Planets Laboratory, Carnegie Institution for Science, Washington, DC 20015, USA.ORCID 0000-0001-9643-2841
Kyle UckertJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91011, USA.ORCID 0000-0002-0859-5526
Anastasia G YanchilinaImpossible Sensing, LLC, St. Louis, MO 63118, USA.ORCID 0000-0003-3782-6343
Olivier BeyssacInstitut de Minéralogie de Physique des Matériaux et de Cosmochimie, CNRS, Sorbonne Université, Muséum National d'Histoire Naturelle, Paris, France.
Kenneth A FarleyDivision of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA.
Jesper HennekeDanish Technical University, Lyngby, Denmark.ORCID 0000-0002-3195-7417
Chris HeirweghJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91011, USA.ORCID 0009-0002-8234-7288
David A K PedersenDanish Technical University, Lyngby, Denmark.
Yang LiuJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91011, USA.ORCID 0000-0003-0308-0942
Mariek E SchmidtDepartment of Earth Sciences, Brock University, St. Catharines, ON, Canada.ORCID 0000-0003-4793-7899
Mark SephtonDepartment of Earth Science and Engineering, Imperial College London, London, UK.ORCID 0000-0002-2190-5402
David ShusterDepartment of Earth and Planetary Science, University of California Berkeley, Berkeley, CA 94720, USA.ORCID 0000-0003-2507-9977
Benjamin P WeissDepartment of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA.ORCID 0000-0003-3113-3415

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

A major objective of the Mars 2020 mission is to sample rocks in Jezero crater that may preserve organic matter for later return to Earth. Using an ultraviolet Raman and luminescence spectrometer, the Perseverance rover detected luminescence signals with maximal intensities at 330 to 350 nanometers and 270 to 290 nanometers that were initially reported as consistent with organics. Here, we test the alternative hypothesis that the 330- to 350-nanometer and 270- to 290-nanometer luminescence signals trace Ce

Identifiers

PMID39321302
PMCPMC11423895

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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.