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Exoplanet 29 Cygni b (Artist’s Concept)

Exoplanet 29 Cygni b, seen in this artist’s concept, is a gas giant weighing about 15 times the mass of Jupiter. It orbits a type A star (shown at upper right) slightly hotter and more massive than our Sun, at an average distance of 1.5 billion miles. The star is known to possess a dusty debris disk. A hypothetical comet fragment is shown approaching the planet, while previous impacts have left dark splotches on its cloudtops, similar to what was seen from the Shoemaker-Levy 9 impact on Jupiter in our solar system.
Astronomers studied 29 Cygni b with NASA’s James Webb Space Telescope. They determined that it likely formed from accretion, a bottom-up process where small bits of rock and ice clump together and grow larger over time, rather than from disk fragmentation. In other words, it formed like a planet and not like a star.
- Object NameObject NameA name or catalog number that astronomers use to identify an astronomical object.29 Cygni b
- Object DescriptionObject DescriptionThe type of astronomical object.Exoplanet
- Release DateApril 14, 2026
- Science ReleaseNASA’s Webb Redefines Dividing Line Between Planets, Stars
- CreditIllustration: NASA, ESA, CSA, Joseph Olmsted (STScI)
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Exoplanet 29 Cygni b (NIRCam Image)
Astronomers used NASA’s James Webb Space Telescope to directly image 29 Cygni b, which weighs 15 times Jupiter. They found evidence for heavy chemical elements like carbon and oxygen, which strongly suggests it formed like a planet by accretion within a protoplanetary disk.
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Laura Betz
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
laura.e.betz@nasa.gov






