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Webb Data Point to Sulfur‑Rich Magma‑Ocean Planet L 98‑59 d

Webb spectroscopy links the planet’s puzzling low density to sulfur‑rich gases through interior–atmosphere exchange models.

Overview

  • An Oxford‑led team reports in Nature Astronomy that L 98‑59 d, about 35 light‑years away, has a mean density far below Earth’s despite a radius near 1.6 Earths.
  • JWST observations indicate a hydrogen‑bearing atmosphere containing hydrogen sulfide and sulfur dioxide.
  • Modeling proposes a deep, long‑lived magma ocean that stores and releases sulfur, suggesting a possible new class of small planets.
  • Simulations favor formation with unusually high water and sulfur followed by stellar radiation stripping lighter gases.
  • The authors note that conclusions depend on spectral interpretation and interior models, with the presence of a solid crust and tidal‑locking effects still uncertain.