Your browser doesn't support javascript.
loading
Inorganic interpretation of luminescent materials encountered by the Perseverance rover on Mars.
Scheller, Eva L; Bosak, Tanja; McCubbin, Francis M; Williford, Kenneth; Siljeström, Sandra; Jakubek, Ryan S; Eckley, Scott A; Morris, Richard V; Bykov, Sergei V; Kizovski, Tanya; Asher, Sanford; Berger, Eve; Bower, Dina M; Cardarelli, Emily L; Ehlmann, Bethany L; Fornaro, Teresa; Fox, Allison; Haney, Nikole; Hand, Kevin; Roppel, Ryan; Sharma, Sunanda; Steele, Andrew; Uckert, Kyle; Yanchilina, Anastasia G; Beyssac, Olivier; Farley, Kenneth A; Henneke, Jesper; Heirwegh, Chris; Pedersen, David A K; Liu, Yang; Schmidt, Mariek E; Sephton, Mark; Shuster, David; Weiss, Benjamin P.
Afiliação
  • Scheller EL; Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA.
  • Bosak T; Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA.
  • McCubbin FM; Astromaterials Research and Exploration Science Division, NASA Johnson Space Center, Houston, TX 77058, USA.
  • Williford K; Blue Marble Space Institute of Science, Seattle, WA 98104, USA.
  • Siljeström S; RISE Research Institutes of Sweden, Stockholm, Sweden.
  • Jakubek RS; Jacobs, NASA Johnson Space Center, Houston, TX 77058, USA.
  • Eckley SA; Jacobs, NASA Johnson Space Center, Houston, TX 77058, USA.
  • Morris RV; Astromaterials Research and Exploration Science Division, NASA Johnson Space Center, Houston, TX 77058, USA.
  • Bykov SV; Department of Chemistry, University of Pittsburgh, Pittsburgh, PA 15260, USA.
  • Kizovski T; Department of Earth Sciences, Brock University, St. Catharines, ON, Canada.
  • Asher S; Department of Chemistry, University of Pittsburgh, Pittsburgh, PA 15260, USA.
  • Berger E; Astromaterials Research and Exploration Science Division, NASA Johnson Space Center, Houston, TX 77058, USA.
  • Bower DM; Department of Astronomy, University of Maryland, College Park, MD 20742, USA.
  • Cardarelli EL; Department of Earth, Planetary and Space Sciences, University of California Los Angeles, Los Angeles, CA 90095, USA.
  • Ehlmann BL; Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA.
  • Fornaro T; Astrophysical Observatory of Arcetri, INAF, Florence, Italy.
  • Fox A; Jacobs, NASA Johnson Space Center, Houston, TX 77058, USA.
  • Haney N; Jacobs, NASA Johnson Space Center, Houston, TX 77058, USA.
  • Hand K; Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91011, USA.
  • Roppel R; Department of Chemistry, University of Pittsburgh, Pittsburgh, PA 15260, USA.
  • Sharma S; Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91011, USA.
  • Steele A; Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC 20015, USA.
  • Uckert K; Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91011, USA.
  • Yanchilina AG; Impossible Sensing, LLC, St. Louis, MO 63118, USA.
  • Beyssac O; Institut de Minéralogie de Physique des Matériaux et de Cosmochimie, CNRS, Sorbonne Université, Muséum National d'Histoire Naturelle, Paris, France.
  • Farley KA; Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA.
  • Henneke J; Danish Technical University, Lyngby, Denmark.
  • Heirwegh C; Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91011, USA.
  • Pedersen DAK; Danish Technical University, Lyngby, Denmark.
  • Liu Y; Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91011, USA.
  • Schmidt ME; Department of Earth Sciences, Brock University, St. Catharines, ON, Canada.
  • Sephton M; Department of Earth Science and Engineering, Imperial College London, London, UK.
  • Shuster D; Department of Earth and Planetary Science, University of California Berkeley, Berkeley, CA 94720, USA.
  • Weiss BP; Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA.
Sci Adv ; 10(39): eadm8241, 2024 Sep 27.
Article em En | MEDLINE | ID: mdl-39321302
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 Ce3+ in phosphate and silicate defects, respectively. By comparing the distributions of luminescence signals with the rover detections of x-ray fluorescence from P2O5 and Si-bearing materials, we show that, while an organic origin is not excluded, the observed luminescence can be explained by purely inorganic materials. These findings highlight the importance of eventual laboratory analyses to detect and characterize organic compounds in the returned samples.

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Ano de publicação: 2024 Tipo de documento: Article

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Ano de publicação: 2024 Tipo de documento: Article