
Haze Cloaks Kepler-51d, Complicating Its Atmosphere Study
New JWST observations of the low-density exoplanet Kepler-51d reveal an unusually thick haze that absorbs light and masks its atmospheric composition, leaving scientists puzzled about its formation and forcing them to consider whether rings or a unique haze layer explain the transit data; the planet, part of the Kepler-51 system known for three other super-puffs, may have formed farther from its star before migrating inward, challenging existing planetary-formation models.













