EGU24-12017, updated on 09 Mar 2024
https://doi.org/10.5194/egusphere-egu24-12017
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

X-ray and Raman spectroscopy of jarosite and ammoniojarosite from several terrestrial localities

Simon Bushmaker, William Nachlas, and Chloë Bonamici
Simon Bushmaker et al.
  • Department of Geoscience, University of Wisconsin-Madison, Madison, Wisconsin 53706, United States of America

Jarosite, a hydrous K-rich sulfate mineral, was found in fine-grain quantities on the Martian surface by the Opportunity rover in 2004. Jarosite found in some terrestrial settings can form a complete solid solution with ammoniojarosite through substitution of the ammonium ion (NH4+) which replaces K+ within its crystal structure. Requiring water and acidic conditions to form, jarosite stands as a potential indicator of ancient N-bearing environments on the Martian surface. The Mars Perseverance rover is currently exploring the Martian surface with analytical instrumentation that may be capable of detecting N-rich jarosite, including the SHERLOC (Scanning Habitable Environments with Raman & Luminescence for Organics & Chemicals) and the PIXL (Planetary Instrument for X-ray Lithochemistry) detectors. To investigate the detection of N in jarosite with Raman and X-ray spectroscopy, we analyzed several terrestrial samples of jarosite and ammoniojarosite using laser Raman spectroscopy and electron-excited Wavelength Dispersive X-ray Spectroscopy (WDS). Comparison of high wavenumber regions of Raman spectra with WDS spectra of N K-α X-rays on the same samples will be used to investigate detection and quantification of N as ammonium in jarosite.

How to cite: Bushmaker, S., Nachlas, W., and Bonamici, C.: X-ray and Raman spectroscopy of jarosite and ammoniojarosite from several terrestrial localities, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-12017, https://doi.org/10.5194/egusphere-egu24-12017, 2024.