Enigmatic HCl detections as a potential signature of igneous activity on Mars

Mars is reputed to lack ongoing volcanic activity. However, marsquakes were revealed recently, and clues to volcanism younger than tens of million years have accumulated. While sulfur dioxide, so far undetected, could testify to ongoing eruptive activity, evidence of active magma chambers may be better identified by seepage of halogen gases, such as hydrogen chloride (HCl). Observations by Atmospheric Chemistry Suite led to the widespread observations of HCl at part-per-billion levels in the atmosphere of Mars during the warm perihelion period, attributed to aerosol-atmospheric sources. Here, we report HCl detections during the cold aphelion season that are isolated in the Alba Mons region. We also identify fresh and narrow (<1 meter) fissures in this area, which we interpret to be potential HCl pathways rooted into magmatic bodies at depth. Our results are best explained by ongoing igneous processes in the Martian interior.

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Publication Details

Journal
Science Advances
Published
2026-11-04
DOI
https://doi.org/10.1126/sciadv.aeb9422
Primary Topic
Planetary Science and Exploration
Type
article
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article

Enigmatic HCl detections as a potential signature of igneous activity on Mars

Nikita Kokonkov, Andrey Patrakeev, D. Mège, Juan Alday et al.
Science Advances
Planetary Science and Exploration
article

Enigmatic HCl detections as a potential signature of igneous activity on Mars

Nikita Kokonkov, Andrey Patrakeev, D. Mège, Juan Alday, Kevin Sutherland Olsen, Mikhail Luginin, Benjamin M. Taysum, A. Pommerol, Franck Montmessin, Pierre‐Antoine Tesson, G. Cremonese, Joanna Gurgurewicz, P. V. Vlasov, Oleg Korablev, N. Ignatiev, Anna A. Fedorova, Denis A. Belyaev, N. Thomas, Alexander Yu. Trokhimovskiy, Alexey V. Grigoriev, Y.A. Ivanov
article en

Abstract

Mars is reputed to lack ongoing volcanic activity. However, marsquakes were revealed recently, and clues to volcanism younger than tens of million years have accumulated. While sulfur dioxide, so far undetected, could testify to ongoing eruptive activity, evidence of active magma chambers may be better identified by seepage of halogen gases, such as hydrogen chloride (HCl). Observations by Atmospheric Chemistry Suite led to the widespread observations of HCl at part-per-billion levels in the atmosphere of Mars during the warm perihelion period, attributed to aerosol-atmospheric sources. Here, we report HCl detections during the cold aphelion season that are isolated in the Alba Mons region. We also identify fresh and narrow (<1 meter) fissures in this area, which we interpret to be potential HCl pathways rooted into magmatic bodies at depth. Our results are best explained by ongoing igneous processes in the Martian interior.

Science AdvancesVol. 12(45)
Australian National University (AU), University of Bern (CH), Centrum Badań Kosmicznych (PL), Centre National de la Recherche Scientifique (FR), National Academy of Sciences of Ukraine (UA), The Open University (GB), Université Paris-Saclay (FR), Space Research Institute (RU), Deutsches Zentrum für Luft- und Raumfahrt e. V. (DLR) (DE), Sorbonne Université (FR), University of Oxford (GB), Main Astronomical Observatory (UA), Laboratoire atmosphères, milieux, observations spatiales (FR), Instituto de Astrofísica de Andalucía (ES), Osservatorio Astronomico di Padova (IT), National Institute for Astrophysics (IT)
Openalex Percentile: Top 16%
Planetary Science and Exploration
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