摘要：We report on the confirmation and mass determination of a transiting planet orbiting the old and inactive G7 dwarf star HD 219666 (M⋆= 0.92 ± 0.03 M⊙,R⋆= 1.03 ± 0.03 R⊙,τ⋆= 10 ± 2 Gyr). With a mass ofMb= 16.6 ± 1.3 M⊕, a radius ofRb= 4.71 ± 0.17 R⊕, and an orbital period ofPorb≃ 6 days, HD 219666 b is a new member of a rare class of exoplanets: the hot-Neptunes. The Transiting Exoplanet Survey Satellite (TESS) observed HD 219666 (also known as TOI-118) in its Sector 1 and the light curve shows four transit-like events, equally spaced in time. We confirmed the planetary nature of the candidate by gathering precise radial-velocity measurements with the High Accuracy Radial velocity Planet Searcher (HARPS) at ESO 3.6 m. We used the co-added HARPS spectrum to derive the host star fundamental parameters (Teff= 5527 ± 65 K, logg⋆= 4.40 ± 0.11 (cgs), [Fe/H]= 0.04 ± 0.04 dex, logR′HK= −5.07 ± 0.03), as well as the abundances of many volatile and refractory elements. The host star brightness (V = 9.9) makes it suitable for further characterisation by means of in-transit spectroscopy. The determination of the planet orbital obliquity, along with the atmosphericmetal-to-hydrogen content and thermal structure could provide us with important clues on the formation mechanisms of this class of objects.
关键词：Key wordsenplanets and satellites: detectionplanets and satellites: fundamental parameterstechniques: radial velocitiesstars: fundamental parameterstechniques: photometricplanets and satellites: individual: HD 219666 b
