Discovery and spectroscopy of the young Jovian planet 51 Eri b with the Gemini Planet Imager
dc.contributor.author | Macintosh, B. | |
dc.contributor.author | Graham, J. R. | |
dc.contributor.author | Barman, T. | |
dc.contributor.author | Rosa, R. J. De | |
dc.contributor.author | Konopacky, Q. | |
dc.contributor.author | Marley, M. S. | |
dc.contributor.author | Marois, C. | |
dc.contributor.author | Nielsen, E. L. | |
dc.contributor.author | Pueyo, L. | |
dc.contributor.author | Rajan, A. | |
dc.contributor.author | Rameau, J. | |
dc.contributor.author | Saumon, D. | |
dc.contributor.author | Wang, J. J. | |
dc.contributor.author | Patience, J. | |
dc.contributor.author | Ammons, M. | |
dc.contributor.author | Arriaga, P. | |
dc.contributor.author | Artigau, E. | |
dc.contributor.author | Beckwith, S. | |
dc.contributor.author | Brewster, J. | |
dc.contributor.author | Bruzzone, S. | |
dc.contributor.author | Bulger, J. | |
dc.contributor.author | Burningham, B. | |
dc.contributor.author | Burrows, A. S. | |
dc.contributor.author | Chen, C. | |
dc.contributor.author | Chiang, E. | |
dc.contributor.author | Chilcote, J. K. | |
dc.contributor.author | Dawson, R. I. | |
dc.contributor.author | Dong, R. | |
dc.contributor.author | Doyon, R. | |
dc.contributor.author | Draper, Z. H. | |
dc.contributor.author | Duchêne, G. | |
dc.contributor.author | Esposito, T. M. | |
dc.contributor.author | Fabrycky, D. | |
dc.contributor.author | Fitzgerald, M. P. | |
dc.contributor.author | Follette, K. B. | |
dc.contributor.author | Fortney, J. J. | |
dc.contributor.author | Gerard, B. | |
dc.contributor.author | Goodsell, S. | |
dc.contributor.author | Greenbaum, A. Z. | |
dc.contributor.author | Hibon, P. | |
dc.contributor.author | Hinkley, S. | |
dc.contributor.author | Cotten, T. H. | |
dc.contributor.author | Hung, L. -W. | |
dc.contributor.author | Ingraham, P. | |
dc.contributor.author | Johnson-Groh, M. | |
dc.contributor.author | Kalas, P. | |
dc.contributor.author | Lafreniere, D. | |
dc.contributor.author | Larkin, J. E. | |
dc.contributor.author | Lee, J. | |
dc.contributor.author | Line, M. | |
dc.contributor.author | Long, D. | |
dc.contributor.author | Maire, J. | |
dc.contributor.author | Marchis, F. | |
dc.contributor.author | Matthews, B. C. | |
dc.contributor.author | Max, C. E. | |
dc.contributor.author | Metchev, S. | |
dc.contributor.author | Millar-Blanchaer, M. A. | |
dc.contributor.author | Mittal, T. | |
dc.contributor.author | Morley, C. V. | |
dc.contributor.author | Morzinski, K. M. | |
dc.contributor.author | Murray-Clay, R. | |
dc.contributor.author | Oppenheimer, R. | |
dc.contributor.author | Palmer, D. W. | |
dc.contributor.author | Patel, R. | |
dc.contributor.author | Perrin, M. D. | |
dc.contributor.author | Poyneer, L. A. | |
dc.contributor.author | Rafikov, R. R. | |
dc.contributor.author | Rantakyrö, F. T. | |
dc.contributor.author | Rice, E. L. | |
dc.contributor.author | Rojo, P. | |
dc.contributor.author | Rudy, A. R. | |
dc.contributor.author | Ruffio, J. -B. | |
dc.contributor.author | Ruiz, M. T. | |
dc.contributor.author | Sadakuni, N. | |
dc.contributor.author | Saddlemyer, L. | |
dc.contributor.author | Salama, M. | |
dc.contributor.author | Savransky, D. | |
dc.contributor.author | Schneider, A. C. | |
dc.contributor.author | Sivaramakrishnan, A. | |
dc.contributor.author | Song, I. | |
dc.contributor.author | Soummer, R. | |
dc.contributor.author | Thomas, S. | |
dc.contributor.author | Vasisht, G. | |
dc.contributor.author | Wallace, J. K. | |
dc.contributor.author | Ward-Duong, K. | |
dc.contributor.author | Wiktorowicz, S. J. | |
dc.contributor.author | Wolff, S. G. | |
dc.contributor.author | Zuckerman, B. | |
dc.date.accessioned | 2017-07-12T16:28:41Z | |
dc.date.available | 2017-07-12T16:28:41Z | |
dc.date.issued | 2015-10-02 | |
dc.identifier.citation | Macintosh , B , Graham , J R , Barman , T , Rosa , R J D , Konopacky , Q , Marley , M S , Marois , C , Nielsen , E L , Pueyo , L , Rajan , A , Rameau , J , Saumon , D , Wang , J J , Patience , J , Ammons , M , Arriaga , P , Artigau , E , Beckwith , S , Brewster , J , Bruzzone , S , Bulger , J , Burningham , B , Burrows , A S , Chen , C , Chiang , E , Chilcote , J K , Dawson , R I , Dong , R , Doyon , R , Draper , Z H , Duchêne , G , Esposito , T M , Fabrycky , D , Fitzgerald , M P , Follette , K B , Fortney , J J , Gerard , B , Goodsell , S , Greenbaum , A Z , Hibon , P , Hinkley , S , Cotten , T H , Hung , L -W , Ingraham , P , Johnson-Groh , M , Kalas , P , Lafreniere , D , Larkin , J E , Lee , J , Line , M , Long , D , Maire , J , Marchis , F , Matthews , B C , Max , C E , Metchev , S , Millar-Blanchaer , M A , Mittal , T , Morley , C V , Morzinski , K M , Murray-Clay , R , Oppenheimer , R , Palmer , D W , Patel , R , Perrin , M D , Poyneer , L A , Rafikov , R R , Rantakyrö , F T , Rice , E L , Rojo , P , Rudy , A R , Ruffio , J -B , Ruiz , M T , Sadakuni , N , Saddlemyer , L , Salama , M , Savransky , D , Schneider , A C , Sivaramakrishnan , A , Song , I , Soummer , R , Thomas , S , Vasisht , G , Wallace , J K , Ward-Duong , K , Wiktorowicz , S J , Wolff , S G & Zuckerman , B 2015 , ' Discovery and spectroscopy of the young Jovian planet 51 Eri b with the Gemini Planet Imager ' , Science , vol. 350 , no. 6256 , pp. 64-67 . https://doi.org/10.1126/science.aac5891 | |
dc.identifier.issn | 1095-9203 | |
dc.identifier.other | ArXiv: http://arxiv.org/abs/1508.03084v2 | |
dc.identifier.other | ORCID: /0000-0003-4600-5627/work/64327354 | |
dc.identifier.uri | http://hdl.handle.net/2299/18895 | |
dc.description | This is the Accepted Manuscript of the following article: B. Macintosh, et al., “Discovery and spectroscopy of the young jovian planet 51 Eri b with the Gemini Planet Imager”, Science, Vol. 350(6256): 64-67, August 2015. The final published version is available at: http://science.sciencemag.org/content/350/6256/64 © The Authors | |
dc.description.abstract | Directly detecting thermal emission from young extrasolar planets allows measurement of their atmospheric composition and luminosity, which is influenced by their formation mechanism. Using the Gemini Planet Imager, we discovered a planet orbiting the \$sim$20 Myr-old star 51 Eridani at a projected separation of 13 astronomical units. Near-infrared observations show a spectrum with strong methane and water vapor absorption. Modeling of the spectra and photometry yields a luminosity of L/LS=1.6-4.0 x 10-6 and an effective temperature of 600-750 K. For this age and luminosity, "hot-start" formation models indicate a mass twice that of Jupiter. This planet also has a sufficiently low luminosity to be consistent with the "cold- start" core accretion process that may have formed Jupiter. | en |
dc.format.extent | 4988574 | |
dc.language.iso | eng | |
dc.relation.ispartof | Science | |
dc.subject | astro-ph.EP | |
dc.title | Discovery and spectroscopy of the young Jovian planet 51 Eri b with the Gemini Planet Imager | en |
dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
dc.contributor.institution | School of Physics, Engineering & Computer Science | |
dc.contributor.institution | Department of Physics, Astronomy and Mathematics | |
dc.description.status | Peer reviewed | |
rioxxterms.versionofrecord | 10.1126/science.aac5891 | |
rioxxterms.type | Journal Article/Review | |
herts.preservation.rarelyaccessed | true |