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Young Mars Volcanoes Show Long-Lived, Evolving Magma Systems

Orbital mapping with mineral data reveals a multi-phase eruptive history at the Pavonis fissure.

Overview

  • A peer-reviewed study in Geology published on January 29, 2026 reconstructs a young volcanic system south of Pavonis Mons.
  • Researchers identify a shift from early fissure-fed lava flows to later point-source, cone-forming eruptions supplied by the same subsurface magma.
  • Distinct mineral signatures preserved in successive flows track magma evolution through time.
  • The mineral changes likely reflect variations in magma source depth and the duration of subsurface storage before eruption.
  • By combining high-resolution surface mapping and orbital spectroscopy, the team challenges the older model of simple, short-lived Martian eruptions.