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Gas Giant Orbiting a White Dwarf Is Found to Have a Warm, Cloudy Atmosphere

JWST transmission spectra reveal clouds, methane and a temperature near 400 K, evidence that the planet moved inward long after its star died

Overview

  • Researchers published a Nature paper on Wednesday reporting the first confirmed atmosphere for a planet orbiting a white dwarf, based on grazing-transit observations with the James Webb Space Telescope.
  • The JWST transmission spectrum shows signatures of tiny cloud particles and hydrocarbons such as methane and gives an atmospheric temperature of roughly 400 K (about 260°F).
  • WD 1856b is roughly Jupiter-sized, completes an orbit in about 34 hours around its white dwarf host, and transit geometry allowed teams to estimate its mass at several times Jupiter’s mass.
  • By combining the measured temperature with cooling and interior models, authors conclude the planet was likely pulled inward by gravitational interactions billions of years after the star became a white dwarf rather than surviving engulfment during the red-giant phase.
  • The result shows gas giants can keep atmospheres after stellar death and informs predictions about the distant fate of planets like Jupiter; researchers plan more JWST transits to refine composition and timing estimates.