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Detecting a planet orbiting a binary system using radial velocity data - Nature Astronomy

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Detecting a planet orbiting a binary system using radial velocity data - Nature Astronomy

Radial velocity observations of a binary star system have led to the discovery of a gas-giant circumbinary planet, BEBOP-1 c, which is 65 times more massive than Earth, with an orbital period of 215.5 days. The binary system also hosts a smaller, inner transiting planet, TOI-1338 b, making this system a rare multi-planet circumbinary system.

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Detecting a planet orbiting a binary system using radial velocity data - Nature Astronomy

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Detecting a planet orbiting a binary system using radial velocity data - Nature Astronomy

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