[astro-ph.EP] We report the discovery of β Pictoris d (β Pic d), a third giant planet in the β Pictoris system, which now becomes only the second directly imaged system with more than two confirmed planets. β Pic d was serendipitously detected in JWST/NIRSpec IFU observations.
A second epoch of NIRSpec and MIRI/MRS observations confirm the initial discovery. The extracted spectrum shows clear CH4, CO, and H2O absorption features, and β Pic d’s measured radial velocity is consistent with its orbital position. Radial velocity and astrometry measurements combined with orbital stability simulations suggest a semi-major axis >30 au, consistent with β Pic d being responsible for carving the inner edge of the β Pictoris debris disk.
Using effective temperature estimates from atmosphere model grid fits combined with evolutionary models, we estimate a mass of 2–4 MJup. β Pic d is the first planet discovered using spectral template matching with moderate-resolution spectroscopy, highlighting its sensitivity to planetary molecular features hidden within bright extrasolar debris disks that are difficult to access with broadband imaging.
Aidan Gibbs, Jean-Baptiste Ruffio, Alexis Bidot, Travis S. Barman, Clarissa R. Do Ó, Quinn M. Konopacky, Marshall D. Perrin, Aneesh Baburaj, Beck Dacus, Bruce Macintosh, Alexander B. Madurowicz, Jerry W. Xuan
Comments: 14 pages, 4 figures, accepted for publication in ApJ Letters, this article is embargoed for discussion in the press until formal publication in ApJ Letters; press releases are pending
Subjects: Earth and Planetary Astrophysics (astro-ph.EP)
Cite as: arXiv:2606.23789 [astro-ph.EP] (or arXiv:2606.23789v1 [astro-ph.EP] for this version)
https://doi.org/10.48550/arXiv.2606.23789
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Submission history
From: Aidan Gibbs
[v1] Mon, 22 Jun 2026 18:00:02 UTC (2,785 KB)
https://arxiv.org/abs/2606.23789
Astrobiology, exoplanet,
