Wittenmyer, Robert A.Tuomi, MikkoButler, R.P.Jones, H.R.A.Anglada-Escudé, GuillemHorner, JonathanTinney, C.GMarshall, J.P.Carter, B.D.Bailey, J.Salter, G.S.O'Toole, S.J.Wright, D.Crane, J.D.Schectman, S.A.Arriagada, P.Thompson, I.Minniti, D.Jenkins, J.S.Diaz, M.2023-05-302023-05-302014-08Astrophysical Journal. Volume 791, Issue 2. 20 August 2014. Article number 1140004-637Xhttps://repositorio.unab.cl/xmlui/handle/ria/50122Indexación: Scopus.We report the detection of GJ 832c, a super-Earth orbiting near the inner edge of the habitable zone of GJ 832, an M dwarf previously known to host a Jupiter analog in a nearly circular 9.4 yr orbit. The combination of precise radial velocity measurements from three telescopes reveals the presence of a planet with a period of 35.68 ± 0.03 days and minimum mass (m sin i) of 5.4 ± 1.0 Earth masses. GJ 832c moves on a low-eccentricity orbit (e = 0.18±0.13) toward the inner edge of the habitable zone. However, given the large mass of the planet, it seems likely that it would possess a massive atmosphere, which may well render the planet inhospitable. Indeed, it is perhaps more likely that GJ 832c is a “super-Venus,” featuring significant greenhouse forcing. With an outer giant planet and an interior, potentially rocky planet, the GJ 832 planetary system can be thought of as a miniature version of our own solar system.enAstrobiologyPlanets and Satellites: individual (GJ 832)Techniques: Radial Velocities Online-only material: color figuresArtículoAtribution 4.0 International (CC BY 4.0)DOI: 10.1088/0004-637X/791/2/114