Mars isn’t dead — recent volcanic activity reveals it’s just sleeping
AI-summarised brief · reviewed before publication
ESA’s ExoMars Trace Gas Orbiter detected hydrogen chloride gas escaping from fissures in Mars’ Alba Mons region, indicating dormant volcanic activity beneath the planet’s surface. The gas, typically associated with Earth’s magma vents, suggests that Mars retains enough internal heat to support recent volcanism. Observations confirm that the planet’s largest volcanoes, including Olympus Mons, may still be active, challenging the long‑held view of Mars as geologically dead. The findings highlight potential hydrothermal systems that could have supported past microbial life.
💡 Why It Matters
- · Revealing active volcanism reshapes our understanding of Mars’ thermal evolution and its capacity to host habitable environments, offering new targets for future life‑search missions.