NASA’s Webb Observes Exoplanet Whose Composition Defies Explanation

December 16, 2025 10:00AM (EST)Release ID: 2025-134
Illustration labeled “artist’s concept” at right bottom corner. At left bottom corner, a partially illuminated, lemon-shaped exoplanet appears against a black background. This planet is most brightly illuminated at its elongated tip on its right side. On the left side, which is wider, the planet trails off into the darkness of the background. The planet is colored in varying, mottled shades of red, light pink, and fuchsia. Most of the pink occurs closest to the tip, while most of the fuchsia is at the top and bottom edges. At right top corner, a white beam emanates diagonally, oriented from 10 o’clock to 4 o’clock, from either side of a small, glowing, white star.

Summary

Bizarre, lemon-shaped world has an atmosphere unlike any ever seen before.

In a finding scientists call “an absolute surprise,” a team using NASA’s James Webb Space Telescope has uncovered a rare type of exoplanet whose atmospheric composition challenges current theories of how the planet could have formed. This Jupiter-mass body appears to have an exotic helium-and-carbon-dominated atmosphere unlike any ever seen before.

This exoplanet is orbiting a pulsar, a rapidly spinning neutron star that is the mass of the Sun but the size of a city. The pulsar emits beams of electromagnetic radiation from its magnetic poles at regular intervals of just milliseconds. Together, the star and exoplanet may be considered a “black widow” system, though not a typical example. Black widow systems are a rare type of double system where a pulsar is paired with a small, low-mass stellar companion. Like the spider for which it is named, the pulsar slowly consumes its unfortunate partner. But in this unique case, the companion is an exoplanet, not a star. 

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