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Published July 15, 2026
NASA's James Webb Space Telescope has identified a third giant planet orbiting the young star Beta Pictoris. The planet, called Beta Pictoris d, had been hiding in one of the system's most closely studied regions. Researchers detected it through a distinctive chemical signature in the planet's atmosphere rather than simply spotting a bright point of light.
Beta Pictoris was already known to host two giant planets, Beta Pictoris b and c. NASA says the addition of Beta Pictoris d makes it only the second planetary system known to contain at least three directly imaged planets. The newly identified world is estimated to be at least twice the mass of Jupiter and appears to travel on an orbit of roughly 30 astronomical units, comparable to Neptune's distance from the Sun.
The discovery came while scientists were using Webb's NIRSpec Integral Field Unit to study the atmosphere of Beta Pictoris b. Instead of the smooth spectrum expected from reflected dust light, the data contained a pattern of carbon-monoxide absorption lines. That chemical fingerprint revealed the presence of another giant planet.
Beta Pictoris is about 63 light-years away and roughly 23 million years old. Its young age and debris disk give astronomers a valuable view of planetary-system formation while giant worlds are still interacting with material left over from the system's birth.
Finding a planet through atmospheric chemistry shows how Webb can uncover worlds that may be difficult to recognize through conventional imaging alone. Spectroscopy can add information about what an exoplanet is made of, not just where it appears in the sky.
Beta Pictoris d adds another major piece to the story of how giant planets form and evolve. The discovery also demonstrates the scientific value of combining direct imaging with detailed infrared spectroscopy.