Inorganic interpretation of luminescent materials encountered by the Perseverance rover on Mars
Number of Authors: 342024 (English)In: Science Advances, E-ISSN 2375-2548, Vol. 10, no 39, article id eadm8241Article in journal (Refereed) Published
Abstract [en]
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 UV Raman and luminescence spectrometer, the Perseverance rover detected luminescence signals with maximal intensities at 330 to 350 nm and 270 to 290 nm that were initially reported as consistent with organics Here, we test the alternative hypothesis that the 330- to 350-nm and 270- to 290-nm luminescence signals trace Ce3+ in phosphate and silicate defects, resp. 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.
Place, publisher, year, edition, pages
American Association for the Advancement of Science , 2024. Vol. 10, no 39, article id eadm8241
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:ri:diva-76750DOI: 10.1126/sciadv.adm8241OAI: oai:DiVA.org:ri-76750DiVA, id: diva2:1931367
Note
This work was supported by Heising-Simons 51 Pegasi B Fellowship #2389909 (E.L.S., T.B., and B.P.W.). The research was carried out, in part, at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration (80NM0018D0004) (K.H., S.S., E.L.C., K.U., B.L.E., Y.L., and C.H.). This work was also funded by a Canadian Space Agency M2020 Participating Scientist grant (21EXPMAPS) (M.E.S.), the Mars 2020 Participating Scientist program (grant 80NSSC20K0238) (B.P.W.), and ASI/INAF agreement no. 2023-3-HH (T.F.).
2025-01-272025-01-272025-09-23Bibliographically approved