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Exoplanet WD 1856 b (Transmission Spectrum)

NASA’s James Webb Space Telescope measured the constituents of exoplanet WD 1856 b as it passed in front of its star, finding signs of methane. WD 1856 b orbits a white dwarf star the size of Earth. As a result, the planet blocks more than half of the star’s light. The red bands indicate where bumps in the spectrum show that this planet’s atmosphere contains methane.
- Release DateJuly 1, 2026
- Science ReleaseNASA’s Webb Studies How Planet Survived Death of its Star
- CreditIllustration: NASA, ESA, CSA, Joseph Olmsted (STScI)
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Exoplanet WD 1856 b (Artist's Concept)
Exoplanet WD 1856 b, shown in this artist’s concept, is a gas giant that orbits its star at a distance 50 times closer than Earth orbits the Sun. Observations by NASA’s James Webb Space Telescope determined the planet’s temperature and detected molecules in its atmosphere.
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Last Updated
Jul 01, 2026
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Media
Laura Betz
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
laura.e.betz@nasa.gov






