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A scientific study identifies evidence of potential magmatic processes on Mars based on orbital data

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“A satellite detects signs of volcanic activity on Mars”

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New observations of the Martian atmosphere by the ExoMars Trace Gas Orbiter have revealed anomalous concentrations of hydrogen chloride near the Alba Mons volcano. A study published in Science Advances suggests that these gases could originate from subterranean magma, which would open the door to the existence of latent volcanism on the planet.

The finding is based on the seasonal detection of hydrogen chloride (HCl) in the vicinity of Alba Mons, one of Mars's largest volcanic complexes. Although the gas shows variations linked to dust and water cycles, researchers identified persistent concentrations in that specific region during the northern hemisphere summer.

Combining chemical data from the ACS instrument and high-resolution images from the CaSSIS camera, the scientific team located fractures hundreds of meters long on the volcano's slopes. The scientists hypothesize that these fissures act as escape routes for magmatic gases trapped beneath the surface and released due to the sublimation of seasonal ice.

Institutions such as the Astrophysics Institute of Andalusia (IAA-CSIC) are participating in the work. The team plans new observation campaigns from Earth to search for additional gases, such as sulfur dioxide, which would help corroborate the presence of active or recent magmatic activity in the Martian subsoil.

Verified Core Facts
  • The ExoMars TGO orbiter detected seasonal concentrations of hydrogen chloride near Alba Mons.
  • The study has been published in the academic journal Science Advances.
  • Fractures were identified on the volcano's slopes that could serve as escape vents for subterranean gases.
  • The Astrophysics Institute of Andalusia (IAA-CSIC) is actively participating in the research.
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Corroborates: A satellite detects signs of volcanic activity on Mars

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