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
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aa44079-22.pdf
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Published version
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8.62 MB
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Author(s)
Seager, Sara
Date Issued
2022
Journal
Astronomy and Astrophysics
Publisher
EDP Sciences
Citation
Seager, Sara. 2022. "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." Astronomy and Astrophysics, 667.
Version
Final published version
Abstract
Context. Neptunes represent one of the main types of exoplanets and have chemical-physical characteristics halfway between rocky
and gas giant planets. Therefore, their characterization is important for understanding and constraining both the formation mechanisms
and the evolution patterns of planets.
Aims. We investigate the exoplanet candidate TOI-1422 b, which was discovered by the TESS space telescope around the high propermotion G2 V star TOI-1422 (V = 10.6 mag), 155 pc away, with the primary goal of confirming its planetary nature and characterising
its properties.
Methods. We monitored TOI-1422 with the HARPS-N spectrograph for 1.5 yr to precisely quantify its radial velocity (RV) variation.
We analyse these RV measurements jointly with TESS photometry and check for blended companions through high-spatial resolution
images using the AstraLux instrument.
Results. We estimate that the parent star has a radius of R⋆ = 1.019+0.014
−0.013 R⊙, and a mass of M⋆ = 0.981+0.062
−0.065 M⊙. Our analysis confirms
the planetary nature of TOI-1422 b and also suggests the presence of a Neptune-mass planet on a more distant orbit, the candidate TOI1422 c, which is not detected in TESS light curves. The inner planet, TOI-1422 b, orbits on a period of Pb = 12.9972 ± 0.0006 days and
has an equilibrium temperature of Teq,b = 867 ± 17 K. With a radius of Rb = 3.96+0.13
−0.11 R⊕, a mass of Mb = 9.0
+2.3
−2.0 M⊕ and, consequently,
a density of ρb = 0.795+0.290
−0.235 g cm−3
, it can be considered a warm Neptune-sized planet. Compared to other exoplanets of a similar mass
range, TOI-1422 b is among the most inflated, 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-1422 c, has an
orbital period of Pc = 29.29+0.21
−0.20 days, a minimum mass, Mc sin i, of 11.1
+2.6
−2.3 M⊕, an equilibrium temperature of Teq,c = 661 ± 13 K and,
therefore, if confirmed, could be considered as another warm Neptune.
MIT Department
Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
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Creative Commons Attribution 4.0 International license
Persistent DSpace Link
DOI of Published Version
https://doi.org/10.1051/0004-6361/202244079
