1. A giant exoplanet orbiting a very-low-mass star challenges planet formation models.
- Author
-
Morales JC, Mustill AJ, Ribas I, Davies MB, Reiners A, Bauer FF, Kossakowski D, Herrero E, Rodríguez E, López-González MJ, Rodríguez-López C, Béjar VJS, González-Cuesta L, Luque R, Pallé E, Perger M, Baroch D, Johansen A, Klahr H, Mordasini C, Anglada-Escudé G, Caballero JA, Cortés-Contreras M, Dreizler S, Lafarga M, Nagel E, Passegger VM, Reffert S, Rosich A, Schweitzer A, Tal-Or L, Trifonov T, Zechmeister M, Quirrenbach A, Amado PJ, Guenther EW, Hagen HJ, Henning T, Jeffers SV, Kaminski A, Kürster M, Montes D, Seifert W, Abellán FJ, Abril M, Aceituno J, Aceituno FJ, Alonso-Floriano FJ, Ammler-von Eiff M, Antona R, Arroyo-Torres B, Azzaro M, Barrado D, Becerril-Jarque S, Benítez D, Berdiñas ZM, Bergond G, Brinkmöller M, Del Burgo C, Burn R, Calvo-Ortega R, Cano J, Cárdenas MC, Guillén CC, Carro J, Casal E, Casanova V, Casasayas-Barris N, Chaturvedi P, Cifuentes C, Claret A, Colomé J, Czesla S, Díez-Alonso E, Dorda R, Emsenhuber A, Fernández M, Fernández-Martín A, Ferro IM, Fuhrmeister B, Galadí-Enríquez D, Cava IG, Vargas MLG, Garcia-Piquer A, Gesa L, González-Álvarez E, Hernández JIG, González-Peinado R, Guàrdia J, Guijarro A, de Guindos E, Hatzes AP, Hauschildt PH, Hedrosa RP, Hermelo I, Arabi RH, Otero FH, Hintz D, Holgado G, Huber A, Huke P, Johnson EN, de Juan E, Kehr M, Kemmer J, Kim M, Klüter J, Klutsch A, Labarga F, Labiche N, Lalitha S, Lampón M, Lara LM, Launhardt R, Lázaro FJ, Lizon JL, Llamas M, Lodieu N, López Del Fresno M, Salas JFL, López-Santiago J, Madinabeitia HM, Mall U, Mancini L, Mandel H, Marfil E, Molina JAM, Martín EL, Martín-Fernández P, Martín-Ruiz S, Martínez-Rodríguez H, Marvin CJ, Mirabet E, Moya A, Naranjo V, Nelson RP, Nortmann L, Nowak G, Ofir A, Pascual J, Pavlov A, Pedraz S, Medialdea DP, Pérez-Calpena A, Perryman MAC, Rabaza O, Ballesta AR, Rebolo R, Redondo P, Rix HW, Rodler F, Trinidad AR, Sabotta S, Sadegi S, Salz M, Sánchez-Blanco E, Carrasco MAS, Sánchez-López A, Sanz-Forcada J, Sarkis P, Sarmiento LF, Schäfer S, Schlecker M, Schmitt JHMM, Schöfer P, Solano E, Sota A, Stahl O, Stock S, Stuber T, Stürmer J, Suárez JC, Tabernero HM, Tulloch SM, Veredas G, Vico-Linares JI, Vilardell F, Wagner K, Winkler J, Wolthoff V, Yan F, and Osorio MRZ
- Abstract
Surveys have shown that super-Earth and Neptune-mass exoplanets are more frequent than gas giants around low-mass stars, as predicted by the core accretion theory of planet formation. We report the discovery of a giant planet around the very-low-mass star GJ 3512, as determined by optical and near-infrared radial-velocity observations. The planet has a minimum mass of 0.46 Jupiter masses, very high for such a small host star, and an eccentric 204-day orbit. Dynamical models show that the high eccentricity is most likely due to planet-planet interactions. We use simulations to demonstrate that the GJ 3512 planetary system challenges generally accepted formation theories, and that it puts constraints on the planet accretion and migration rates. Disk instabilities may be more efficient in forming planets than previously thought., (Copyright © 2019 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. No claim to original U.S. Government Works.)
- Published
- 2019
- Full Text
- View/download PDF