Third Planet Found in Beta Pictoris System Is Faintest Ever Directly Imaged from Earth

Astronomers confirmed a third gas giant in the Beta Pictoris system — the faintest planet ever directly imaged from Earth.

A gas giant 2.4 times the mass of Jupiter had been hiding in one of astronomy's most-watched star systems for over a decade — and two independent teams finally caught it. Designated Beta Pictoris d, the newly confirmed planet is the third world found orbiting the young star Beta Pictoris, located 63 light-years from Earth. It orbits at a distance of 26 astronomical units from its host star, placing it in the middle of the system between the two previously known planets. The discovery relied on 11 years of accumulated observational data, combining archival imagery from NASA's James Webb Space Telescope with ground-based observations from the European Southern Observatory's Very Large Telescope in Chile. That combination of space and ground assets allowed researchers to tease out a signal too faint for either instrument to confirm alone — making Beta Pictoris d the faintest exoplanet ever directly imaged from the ground. Beta Pictoris is already one of the most intensively studied stellar systems beyond our own, known for its prominent debris disk, active comet-like bodies called exocomets, and two previously confirmed giant planets. The addition of a third planet raises fresh questions about how the system's warped disk formed and which worlds are responsible for sculpting it. Two independent research teams reaching the same conclusion strengthens confidence in the detection.

Why it matters

Beta Pictoris d's position and mass could help explain longstanding puzzles about the system's warped debris disk and exocomet behavior, offering broader insight into how planetary systems form and evolve. The detection sets a new benchmark for direct imaging sensitivity from Earth-based observatories.

What's next

Researchers will likely use the new three-planet picture of Beta Pictoris to model how the planets interact with the system's debris disk and exocomets, potentially resolving questions about which bodies drive the disk's unusual warped structure.

Key facts

• Beta Pictoris d has a mass of approximately 2.4 times that of Jupiter
• The planet orbits its star at 26 astronomical units — roughly the distance of Uranus from our Sun
• The host star, Beta Pictoris, is 63 light-years from Earth
• The discovery drew on 11 years of observational data, including JWST archival imagery and VLT ground observations
• Beta Pictoris d is the faintest exoplanet ever directly imaged from Earth
• Two independent research teams confirmed the planet using different telescopes

Bias & framing notes

All three sources agree on the core discovery and its significance. Source 2 provides the most specific technical detail — mass, orbital distance, and data timeline. Sources 1 and 3 are lighter on specifics and lean on the narrative hook of '11 years of hiding,' which is accurate but emphasizes drama over data. No sources contradict each other on facts.

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