Radial-velocity discovery of a second planet in the TOI-1338/BEBOP-1 circumbinary system

Abstract

We report the detection of a gas-giant planet in orbit around both stars of an eclipsing binary star system that also contains the smaller, inner transiting planet TOI-1338b. The new planet, called TOI-1338/BEBOP-1c, was discovered using radial-velocity data collected with the HARPS and ESPRESSO spectrographs. Our analysis reveals it is a $65.2{\mathrm{M}}_{\oplus }$ circumbinary planet with a period of $215.5$days. This is the first detection of a circumbinary planet using radial-velocity observations alone, and makes TOI-1338/BEBOP-1 only the second confirmed multiplanet circumbinary system to date. We do not detect the smaller inner transiting planet with radial-velocity data, and can place an upper limit on the inner planet's mass at $21.8{\mathrm{M}}_{\oplus }$ with $99\%$ confidence. The inner planet is the first circumbinary planet amenable for atmospheric characterisation, using the James Webb Space Telescope.

arXiv commentThe Version of Record of this article is published in Nature Astronomy, and is available online at https://doi.org/10.1038/s41550-023-01948-4 Main: 14-pages, 4-Figures, 1-table. Supporting material: 48-pages, 12-figures, 4-tables

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