
Methane on the Nightside of an Ultra-Hot Exoplanet Points to Unexpected Vertical Winds
JWST/NIRSpec observations of WASP-121b across its orbit reveal methane on the nightside even though the dayside reaches ~3,000°C, a temperature that should break methane apart. The study attributes this to vigorous vertical atmospheric circulation that lifts methane-rich gas from cooler depths to higher altitudes, replenishing it faster than it would be destroyed. Silicon monoxide was also detected on the dayside, consistent with silicate vaporisation. The findings challenge current ultra-hot Jupiter models that emphasize horizontal flows and suggest atmospheric chemistry and dynamics in these extreme planets may be more complex than previously thought.












