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Oxford-Led Team Proposes New Exoplanet Class With Sulfur-Rich Magma-Ocean World L 98-59 d

A Nature Astronomy study links the planet’s unusual atmosphere to long-term sulfur exchange between a molten mantle and its air.

Overview

  • The peer-reviewed analysis combines 2024 James Webb Space Telescope spectroscopy with ground-based observations and nearly five billion years of planetary evolution modeling.
  • Spectra show hydrogen sulfide and other sulfur compounds in L 98-59 d’s atmosphere, with JWST also detecting sulfur dioxide at high altitudes.
  • Models indicate a global molten silicate mantle forming a deep magma ocean that stores sulfur and exchanges it with the atmosphere over geologic timescales.
  • L 98-59 d is about 1.6 times Earth’s radius, sits roughly 35 light-years away, and has a low bulk density that does not match standard small-planet categories.
  • Lead author Harrison Nicholls says such molten worlds are unlikely to be habitable and notes ESA’s Ariel and PLATO missions could assess how common they are.