【AI前沿】JWST maps the weather on a hot gas giant 700 light-years away

Cloudy with a chance of excessive heatJWST maps the weather on a hot gas giant 700 light-years awayThe differences seen here could be throwing off how we study planetary atmospheres.Jacek Krywko–May 21, 2026 3:26 pm|16Credit:NASA, ESA, and L. Hustak (STScI)Credit:NASA, ESA, and L. Hustak (STScI)Text settingsStory textSizeSmallStandardLargeWidthStandardWideLinksStandardOrange Subscribers onlyLearn moreMinimize to navWASP-94A b is a hot, tidally locked gas giant orbiting close to one of the stars in a binary system roughly 690 light-years away from Earth. In a new Science study, scientists led by Sagnick Mukherjee, an astrophysicist at Johns Hopkins University, used the James Webb Space Telescope to learn what the weather looks like out there.Tidal locking means that you no longer have day- and night-side temperature differences sweeping across the planet. “We wanted to understand the atmospheres of such planets,” Mukherjee says. “Are they static or dynamic? Do they have winds? Do they have clouds?” His team found that, on WASP-94A b, it’s cloudy in the morning, but the skies are clear in the evening. The fact that we didn’t know this already means we might have gotten the chemistry of this and many other exoplanets surprisingly wrong.Averaged atmospheresWASP-94A b has a mass slightly below half of Jupiter but has a diameter that’s over 70 percent wider. “This means the planet has low density, and its atmosphere extends further out into space, which makes it easier to observe,” Mukherjee explains. When astronomers study atmospheres like this, they usually rely on transmission spectroscopy. By analyzing the spectrum of light filtering through the planet’s atmosphere as it crosses in front of its star, they can figure out its chemical composition.The problem with this approach is that the light filtering through the entire circumference of the planet’s silhouette was averaged out, as though its atmosphere was one homogenous ball of gas. For tidally locked planets, this was a massive oversimplification.On tidally locked worlds, there are massive temperature swings between day and night sides, which usually lead to differences in atmospheric density between the day side and the night side. These differences, combined with the Coriolis effect that stems from the planet’s slow rotation, cause a phenomenon called equatorial super-rotation. This is where winds on the equator blow eastward faster than the planet is spinning. Circulation models predicted this is exactly what’s happening on WASP-94B a.The leading edge of the planet’s disk, called the morning limb, is the region where the local atmosphere is rotating out of the colder night side and into the hot day side. The trailing edge at the evening limb is where the heated daytime gases are crossing over into the dark side. To catch this process in motion, Mukherjee and his colleagues employed a technique called limb-resolved spectroscopy.Slicing transitsBecause it takes a little bit of time for the planet to fully cross the star’s edge during the beginning and end of the transit, the telescope sees the leading morning limb block the starlight slightly before the trailing evening limb does. Using JWST’s Near Infrared Imager and Slitless Spectrograph (NIRISS), the team measured the light curves as WASP-94A b transited and split the signal. This way, they managed to extract two separate chemical transmission spectra for the exoplanet: one for its morning, and one for its evening limb. And there was quite a difference between the two.The morning limb’s spectrum was just a sloped line, rising at shorter wavelengths, which indicated high-altitude aerosols blocking the light from deeper in the atmosphere. “You would see a lot of dust and cloud particles at very high altitudes,” Mukherjee says. “Going deeper, the clouds likely clear up, and you would probably find water vapor and these kinds of gases.”On the evening limb, the spectrum showed no substantial evidence of aerosols and revealed spikes of gaseous water vapor. “This would be a different view where you do not encounter many clouds through your journey, but what you see is just gas—water vapor mostly and other gases, maybe like carbon dioxide,” Mukherjee suggests.By feeding the JWST data into computer models, the team could also predict what the weather engine on WASP-94 b looks like in motion.Equatorial windsThe average temperature on WASP-94A b exceeds 1,500 Kelvin, and Mukherjee’s team confirmed the evening limb is around 450 Kelvin hotter than the morning limb—hot enough to evaporate potential aerosol materials like iron or magnesium silicate. This temperature difference dictates the weather dynamics on the planet.On the permanent night side, gases in the atmosphere condense into droplets due to lower temperature, forming clouds. “These cloud particles are then dragged by the equatorial wind towards the morning side,” Mukherjee says. As the clouds are pushed into the heat of the day side, most of the