The GAPS Programme at TNG XL: A puffy and warm Neptune-sized planet and an outer Neptune-mass candidate orbiting the solar-type star TOI-1422

Abstract

We investigate the exoplanet candidate TOI-1422b, which was discovered by the TESS space telescope around the high proper-motion G2V star TOI-1422 (V=10.6 mag), 155pc away, with the primary goal of confirming its planetary nature and characterising its properties. We monitored TOI-1422 with the HARPS-N spectrograph for 1.5 years to precisely quantify its radial velocity variation. The radial velocity measurements are analyzed jointly with TESS photometry and we also check for blended companions through high-spatial resolution images using the AstraLux instrument. We estimate that the parent star has a radius and a mass of R*=1.019-0.013+0.014 R, M*=0.981-0.065+0.062 M, respectively. Our analysis confirms the planetary nature of TOI-1422b and also suggests the presence of a Neptune-mass planet on a more distant orbit, the candidate TOI-1422c, which is not detected in TESS light curves. The inner planet, TOI-1422b, orbits on a period P b=12.99720.0006 days and has an equilibrium temperature T eq, b=86717 K. With a radius of R b=3.96+0.13-0.11 R, a mass of M b=9.0+2.3-2.0 M and, consequently, a density of b=0.795+0.290-0.235 g cm-3, it can be considered a warm Neptune-size planet. Compared to other exoplanets of similar mass range, TOI-1422b is among the most inflated ones and we expect this planet to have an extensive gaseous envelope that surrounds a core with a mass fraction around 10\%-25\% of the total mass of the planet. The outer non-transiting planet candidate, TOI-1422c, has an orbital period of P c=29.29+0.21-0.20 days, a minimum mass, M ci, of 11.1+2.6-2.3 M, an equilibrium temperature of T eq, c=66113 K and, therefore, if confirmed, it could be considered as another warm Neptune.

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