Bibcode
Plavchan, Peter; Barclay, Thomas; Gagné, Jonathan; Gao, Peter; Cale, Bryson; Matzko, William; Dragomir, Diana; Quinn, Sam; Feliz, Dax; Stassun, Keivan; Crossfield, Ian J. M.; Berardo, David A.; Latham, David W.; Tieu, Ben; Anglada-Escudé, Guillem; Ricker, George; Vanderspek, Roland; Seager, Sara; Winn, Joshua N.; Jenkins, Jon M.; Rinehart, Stephen; Krishnamurthy, Akshata; Dynes, Scott; Doty, John; Adams, Fred; Afanasev, Dennis A.; Beichman, Chas; Bottom, Mike; Bowler, Brendan P.; Brinkworth, Carolyn; Brown, Carolyn J.; Cancino, Andrew; Ciardi, David R.; Clampin, Mark; Clark, Jake T.; Collins, Karen; Davison, Cassy; Foreman-Mackey, Daniel; Furlan, Elise; Gaidos, Eric J.; Geneser, Claire; Giddens, Frank; Gilbert, Emily; Hall, Ryan; Hellier, Coel; Henry, Todd; Horner, Jonathan; Howard, Andrew W.; Huang, Chelsea; Huber, Joseph; Kane, Stephen R.; Kenworthy, Matthew; Kielkopf, John; Kipping, David; Klenke, Chris; Kruse, Ethan; Latouf, Natasha; Lowrance, Patrick; Mennesson, Bertrand; Mengel, Matthew; Mills, Sean M.; Morton, Tim; Narita, Norio; Newton, Elisabeth; Nishimoto, America; Okumura, Jack; Palle, Enric; Pepper, Joshua; Quintana, Elisa V.; Roberge, Aki; Roccatagliata, Veronica; Schlieder, Joshua E.; Tanner, Angelle; Teske, Johanna; Tinney, C. G.; Vanderburg, Andrew; von Braun, Kaspar; Walp, Bernie; Wang, Jason; Wang, Sharon Xuesong; Weigand, Denise; White, Russel; Wittenmyer, Robert A.; Wright, Duncan J.; Youngblood, Allison; Zhang, Hui; Zilberman, Perri
Referencia bibliográfica
Nature
Fecha de publicación:
6
2020
Revista
Número de citas
183
Número de citas referidas
174
Descripción
AU Microscopii (AU Mic) is the second closest pre-main-sequence star, at a distance of 9.79 parsecs and with an age of 22 million years1. AU Mic possesses a relatively rare2 and spatially resolved3 edge-on debris disk extending from about 35 to 210 astronomical units from the star4, and with clumps exhibiting non-Keplerian motion5-7. Detection of newly formed planets around such a star is challenged by the presence of spots, plage, flares and other manifestations of magnetic `activity' on the star8,9. Here we report observations of a planet transiting AU Mic. The transiting planet, AU Mic b, has an orbital period of 8.46 days, an orbital distance of 0.07 astronomical units, a radius of 0.4 Jupiter radii, and a mass of less than 0.18 Jupiter masses at 3σ confidence. Our observations of a planet co-existing with a debris disk offer the opportunity to test the predictions of current models of planet formation and evolution.
Proyectos relacionados
Exoplanetas y Astrobiología
La búsqueda de vida en el Universo se ha visto impulsada por los recientes descubrimientos de planetas alrededor de otras estrellas (los llamados exoplanetas), convirtiéndose en uno de los campos más activos dentro de la Astrofísica moderna. En los últimos años los descubrimientos cada vez más numerosos de nuevos exoplanetas y los últimos avances
Enric
Pallé Bago