TOI-7169 b: A Hot Jupiter Transiting a Metal-poor Star

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Abstract
Most known planets are found around metal-rich host stars, which has made it difficult to determine whether a lower metallicity limit for planet formation exists and how the properties of planets born in low-metallicity environments may differ from those with metal-rich origins. We present the discovery and characterization of TOI-7169 b (TIC 372048733 b), a hot Jupiter that is orbiting a spectroscopically confirmed metal-poor ([Fe/H] = −0.72 ± 0.05) host star. Based on photometry from TESS and follow-up ground-based imaging, we measure an orbital period of 3.437312 5 − 0.0000019 + 0.0000020 days and a planetary radius of 1.475 ± 0.029 R Jup . We use TRES spectroscopy to determine a mass for TOI-7169 b of 0.41 ± 0.14 M Jup . The planet is therefore inflated, with a low density of 0.15 9 − 0.054 + 0.055 g cm −3 . We also characterize the host star, showing that TOI-7169 is ancient (12.3 ± 0.6 Gyr) and α enhanced ([ α /Fe] ≈ 0.3), but with a Galactocentric orbit that is confined to the thin disk. TOI-7169 is perhaps the oldest and most metal-poor star currently known to host a transiting giant planet. Future transmission spectroscopy probing the atmosphere of TOI-7169 b may provide insight into the effect of metallicity on the physical properties of giant planets.

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