This artist’s concept shows what the exoplanet WASP-39 b could look like based on indirect transit observations from NASA’s James Webb Space Telescope as well as other space- and ground-based telescopes.
WASP-39 b is a hot, puffy gas giant that orbits a G-type star that is slightly smaller and less massive than the Sun. WASP-39 b orbits relatively close to this star, just 0.0486 astronomical units (4,500,000 miles) away. WASP-39 b has a mass 0.28 times Jupiter (0.94 times Saturn) and a diameter 1.3 times greater than Jupiter.
WASP-39 b is tidally locked, with one side facing the star at all times. This means the planet has a terminator (a boundary that separates the planet’s dayside and nightside) where there is an eternal sunrise and sunset.
By analyzing a transmission spectrum of WASP-39 b from Webb’s NIRSpec (Near-Infrared Spectrograph), a technique that studies the exoplanet’s terminator, astronomers confirmed a temperature difference between the morning and evening, with the evening appearing hotter by roughly 300 Fahrenheit degrees (about 200 Celsius degrees). They also found evidence for different cloud cover, with the morning being likely cloudier than the evening.
Webb has not captured a direct image of WASP-39 b.
