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Sulfur Enrichment In Close-in Exoplanet Atmospheres Induced By Pebble Drift Across The Salt Line - Astrobiology

Summary by astrobiology.com
Observations of JWST have revealed that several close-in exoplanets have sulfur-rich atmospheres through SO2 detections. Atmospheric sulfur is often thought to originate from solid accretion during planet formation, whereas recent simultaneous detections of SO2 and NH3 challenge this conventional scenario. In this study, we propose that ammonium salts, such as NH4SH tentatively detected in comets […] The post Sulfur Enrichment In Close-in Exopla…
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astrobiology.com broke the news in on Tuesday, February 10, 2026.
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