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Oxford Study Identifies New Class of Molten Exoplanet

L 98-59 d’s global magma ocean stores large sulphur amounts, maintaining a hydrogen-rich atmosphere over billions of years, revealing a new exoplanet class, Oxford researchers say.

  • On Monday, the University of Oxford-led team will publish in Nature Astronomy that L 98-59 d is a molten, sulphur-rich exoplanet with hydrogen sulphide in its atmosphere.
  • Following 2024 James Webb Space Telescope and ground-based spectra, researchers observed low density and sulphur-bearing gases around L 98-59 d and used simulations to model its five-billion-year evolution.
  • Their models show that the mantle of L 98-59 d contains a global magma ocean thousands of kilometres deep that stores sulphur, while ultraviolet light from the red dwarf L 98-59 drives atmospheric sulphur-bearing gas chemistry.
  • The team intend to apply their simulations to JWST, Ariel, and PLATO data, suggesting L 98-59 d may define a new class of sulphur-rich planets.
  • Using magma-ocean physics, the team proposes that models applied to upcoming JWST, Ariel, and PLATO data could map planetary diversity and habitability, informing our understanding of rocky planet formation.
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ox.ac.uk broke the news in on Monday, March 16, 2026.
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