Scientists at the 55th Lunar and Planetary Science Conference in The Woodlands, Texas, announced the discovery of a vast volcano and a potential glacier ice sheet in Mars’ Tharsis volcanic province, near the equator. Based on images from spacecraft orbiting Mars since 1971, the finding highlights a volcano provisionally named “Noctis” and suggests the presence of glacier ice beneath a volcanic deposit. This discovery opens new avenues for studying Mars’ geological evolution and future exploration.
Known provisionally as “Noctis volcano,” this geological feature stands at an elevation of +9 022 m (29 600 feet) and spans 450 km (280 miles) in width, hinting at an extensive history of volcanic activity.
Located at the boundary of Noctis Labyrinthus and Valles Marineris, the Noctis volcano has eluded clear identification for decades, despite surveillance by missions since Mariner 9 in 1971. Its discovery, along with the indication of glacier ice beneath a recent volcanic deposit, marks a huge moment for understanding Mars’ geologic and climatic history.
Dr. Pascal Lee, a planetary scientist with the SETI Institute and the Mars Institute at NASA Ames Research Center, and lead author of the study, described the process of uncovering the volcano while investigating the region’s geology. The area’s complex terrain, characterized by layered mesas, canyons, and a central summit area with an arc of elevated mesas, was found to bear signs of extensive volcanic activity, including lava flows, pyroclastic deposits, and hydrated mineral occurrences.
The presence of hydrated minerals in this Martian sector, long suspected to harbor volcanic origins, was confirmed through this discovery, shedding light on the geological processes that shaped the planet.
Sourabh Shubham, a graduate student at the University of Maryland’s Department of Geology and co-author of the study, referred to the Noctis volcano as a long-sought “smoking gun” for the volcanic setting of these minerals.
Furthermore, the study unveiled a 5 000 km2 (1 930 mi2) area within the volcano’s perimeter, characterized by a terrain of low, rounded, and elongated mounds known as “rootless cones.”
These features suggest the explosive interaction of hot volcanic material with ice-rich surfaces, hinting at the presence of a significant sheet of glacier ice beneath the volcanic deposit.
This discovery enriches our understanding of Mars’ volcanic activity and opens new pathways for astrobiological research and future exploration.
The possibility of glacier ice near the Martian equator, coupled with the volcanic site’s history of heat and water interaction, positions the Noctis volcano as a prime candidate for studying potential life-supporting conditions and for human exploration missions.
References:
1 Giant Volcano Discovered on Mars – SETI Institute – March 13, 2024
2 Large eroded volcano complex and buried glacier ice in eastern Noctis Labyrinthus: Evidence for recent volcanism and glaciation near Mars’ equator – 55th LPSC (2024)
Featured image: Background image NASA/USGS Mars globe. Geologic interpretation and annotations by Pascal Lee and Sourabh Shubham 2024
I'm a dedicated researcher, journalist, and editor at The Watchers. With over 20 years of experience in media industry, I specialize in hard science news, focusing on extreme weather, seismic and volcanic activity, space weather, and astronomy, including near-Earth objects and planetary defense strategies. You can reach me at teo /at/ watchers.news.
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