EGU2020-18532, updated on 17 Apr 2024
https://doi.org/10.5194/egusphere-egu2020-18532
EGU General Assembly 2020
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Leka Ophiolite Complex as analogy to the serpentinization-carbonation system on Mars

Benjamin Bultel1, Agata M. Krzesińska1, Damien Loizeau2, Cateline Lantz2, François Poulet2, Håkon O. Austrheim3, Elise M. Harrington1, Jean-Christophe Viennet4, Henning Dypvik1, and Stephanie C. Werner1
Benjamin Bultel et al.
  • 1Center for Earth Evolution and Dynamics (CEED), Beyond Earth, Oslo, Norway (benjamin.bultel@geo.uio.no)
  • 2Institut d’Astrophysique Spatiale, CNRS/Université Paris-Sud, Université Paris-Saclay, bâtiment 121, 91405 Orsay Cedex, France
  • 3Physics of Geological Processes (PGP), The Njord Centre, Department of Geosciences, University of Oslo, 0136 Oslo, Norway.
  • 4Muséum National d’Histoire Naturelle, Institut de Minéralogie, Physique des Matériaux et Cosmochimie, CNRS UMR 7590, Sorbonne Université, CNRS, F-75005 Paris, France.

Jezero Crater is the landing site of the Mars2020 NASA rover. The crater in its early history hosted a paleolake with at least two deltas remaining. The Jezero lake belongs to a larger system - the Nili Fossae region – which exposes a mineralogical assemblage interpreted as a serpentinization/carbonation system [1].  While the main alteration minerals in Jezero are identified, little is known about the accessory minerals. The latter could reveal critical information about the conditions of serpentinization/carbonation [2; 3]. Moreover, several aspects are yet to be solved: Are the carbonates resulting of primary alteration or reworked origin [4]? Is the mineralogical assemblage modified after deposition in the lake (weathering)? What is the nature of the protolith that could contains up to 30% of olivine [5]?

The Nili Fossae-Jezero system has its potential analogue in terrestrial serpentinized and carbonated rocks, such as the Leka Ophiolite Complex, Leka Island, Norway, (PTAL collection, https://www.ptal.eu), which records complex weathering of serpentinite formed from mafic to ultramafic rock [6].

We perform petrological and mineralogical analyses on thin sections to characterize the weathering products in Leka samples, and combine with Near Infrared Spectroscopy measurements. We study the significance of the mineralogical assemblages including solid solution composition and nature of accessory minerals. The consequence for habitability potential might be important. Indeed, the amount of H2/CH4 production in mafic or ultramafic system vary significantly [2; 7]. This could represent crucial information that could guide future in-situ operations but could also help for a better interpretation of the remote sensing data.

 

References:

How to cite: Bultel, B., Krzesińska, A. M., Loizeau, D., Lantz, C., Poulet, F., Austrheim, H. O., Harrington, E. M., Viennet, J.-C., Dypvik, H., and Werner, S. C.: Leka Ophiolite Complex as analogy to the serpentinization-carbonation system on Mars, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-18532, https://doi.org/10.5194/egusphere-egu2020-18532, 2020.