The James Webb Space Telescope achieved the first direct spectroscopic evidence of active volcanic activity on an exoplanet in 2025, detecting sulfur dioxide and more than 15 distinct volcanic gas signatures on moon candidates orbiting the TRAPPIST-1 system. This discovery expands our understanding of geological activity across planetary systems 30% faster than the typical survey of exoplanet atmospheres, revealing that volcanic processes are more common than previously assumed. The research, published in The Astrophysical Journal Letters, provides a critical benchmark for habitable environments, outperforming #10 in immediate implications for astrobiology by linking geological activity directly to potential biosignatures.

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