Espinoza, NéstorBrahm, RafaelHenning, ThomasJordán, AndrésDorn, CarolineRojas, FelipeSarkis, PaulaKossakowski, DianaSchlecker, MartinDíaz, Matías R.Jenkins, James S.Aguilera-Gomez, ClaudiaJenkins, Jon M.Twicken, Joseph D.Collins, Karen A.Lissauer, JackArmstrong, David J.Adibekyan, VardanBarrado, DavidBarros, Susana C.C.Battley, MatthewBayliss, DanielBouchy, FrançoisBryant, Edward M.Cooke, Benjamin F.Olivier D.S.Dumusque, XavierFigueira, PedroGiles, HelenLillo-Box, JorgeLovis, ChristopheNielsen, Louise D.Pepe, FrancescoPollacco, DonSantos, Nuno C.Sousa, Sergio G.Udry, StéphaneWheatley, Peter J.Turner, OliverMarmier, MaximeSégransan, DamienRicker, GeorgeLatham, DavidSeager, SaraWinn, Joshua N.Kielkopf, John F.Hart, RhodesWingham, GeofJensen, Eric L.N.Hełminiak, Krzysztof G.Tokovinin A.Briceño C.Ziegler, CarlLaw, Nicholas M.Mann, Andrew W.Daylan, TansuDoty, John P.Guerrero, NataliaBoyd, PatriciaCrossfield, Ian2024-08-082024-08-082020-01-01Monthly Notices of the Royal Astronomical Society Volume 491, Issue 2, Pages 2982 - 2999 1 January 20200035-8711https://repositorio.unab.cl/handle/ria/59124Indexación: Scopus.We report the discovery of the 1.008-d, ultrashort period (USP) super-Earth HD 213885b (TOI-141b) orbiting the bright (V= 7.9) star HD 213885 (TOI-141, TIC 403224672), detected using photometry from the recently launched TESS mission. Using FEROS, HARPS, and CORALIE radial velocities, we measure a precise mass of 8.8 ±0.6M⊙ for this 1.74±0.05R⊙ exoplanet, which provides enough information to constrain its bulk composition - similar to Earth's but enriched in iron. The radius, mass, and stellar irradiation of HD 213885b are, given our data, very similar to 55 Cancri e, making this exoplanet a good target to perform comparative exoplanetology of short period, highly irradiated super-Earths. Our precise radial velocities reveal an additional 4.78-d signal which we interpret as arising from a second, non-transiting planet in the system, HD 213885c, whose minimum mass of 19.9 ± 1.4 M⊙ makes it consistent with being a Neptune-mass exoplanet. The HD 213885 system is very interesting from the perspective of future atmospheric characterization, being the second brightest star to host an USP transiting super-Earth (with the brightest star being, in fact, 55 Cancri). Prospects for characterization with present and future observatories are discussed.en-USHD213885Planets and satellites: detectionPlanets and satellites: fundamental parametersPlanets and satellites: individual: TOI-141Techniques: photometricTechniques: radial velocitiesTIC 403224672Artículo10.1093/mnras/stz3150