A closely packed system of low-mass, low-density planets transiting Kepler-11

作者: Jack J. Lissauer , Daniel C. Fabrycky , Eric B. Ford , William J. Borucki , Francois Fressin

DOI: 10.1038/NATURE09760

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摘要: When an extrasolar planet passes in front of (transits) its star, radius can be measured from the decrease starlight and orbital period time between transits. Multiple planets transiting same star reveal much more: ratios determine stability dynamics, mutual gravitational interactions reflect masses shapes, fraction observed as multiples has implications for planarity planetary systems. But few stars have more than one known planet, none three. Here we report Kepler spacecraft observations a single Sun-like which call Kepler-11, that six planets, five with periods 10 47 days sixth longer period. The inner are among smallest mass size both been measured, these measurements imply substantial envelopes light gases. degree coplanarity proximity orbits energy dissipation near end formation. NASA's mission, space observatory designed to detect study transit across disk their host hit jackpot discovery six-planet system orbiting now named Kepler-11. Five 47 days, measured. outermost less well characterized thus far. Only other confirmed (Kepler-9, three). This newly discovered resembles our own Solar System being close coplanar, but Kepler-11's orbit closer star. is due continue return data on Kepler-11 some yet, it should provide many valuable constraints models formation evolution solar systems general. (transits), reports days plus

参考文章(71)
G. A. Esquerdo, C. W. Hergenrother, T. M. Brown, D. W. Latham, M. Everett, D. G. Monet, The Kepler Input Catalog American Astronomical Society Meeting Abstracts. ,vol. 207, ,(2005)
R. Redmer, U. Kramm, J. J. Fortney, N. Nettelmann, Thermal evolution and interior models of the transiting super-Earth GJ 1214b ,(2010)
Friedrich Kupka, Saul J. Adelman, N. E. Piskunov, J. A. Valenti, W. W. Weiss, Spectroscopy Made Easy ASP Conference Series; Vol. 108: M.A.S.S.: Model Atmospheres and Spectrum Synthesis, p.175. ,vol. 108, pp. 175- ,(1996)
Jerome A. Orosz, Peter H. Hauschildt, The use of the NextGen model atmospheres for cool giants in a light curve synthesis code Astronomy and Astrophysics. ,vol. 364, pp. 265- 281 ,(2000)
Anna Nobili, Ian W. Roxburgh, Simulation of general relativistic corrections in long term numerical integrations of planetary orbits Relativity in Celestial Mechanics and Astrometry. High Precision Dynamical Theories and Observational Verifications. ,vol. 114, pp. 105- 111 ,(1985)
David Nesvorný, Alessandro Morbidelli, Mass and Orbit Determination from Transit Timing Variations of Exoplanets The Astrophysical Journal. ,vol. 688, pp. 636- 646 ,(2008) , 10.1086/592230
Brett Gladman, Dynamics of Systems of Two Close Planets Icarus. ,vol. 106, pp. 247- 263 ,(1993) , 10.1006/ICAR.1993.1169
Jack Wisdom, Matthew Holman, Symplectic maps for the N-body problem. The Astronomical Journal. ,vol. 102, pp. 1528- 1538 ,(1991) , 10.1086/115978
Linda T. Elkins‐Tanton, Sara Seager, Ranges of Atmospheric Mass and Composition of Super-Earth Exoplanets The Astrophysical Journal. ,vol. 685, pp. 1237- 1246 ,(2008) , 10.1086/591433
William J. Borucki, Joseph D. Twicken, Todd C. Klaus, Sean McCauliff, Ronald L. Gilliland, Christopher K. Middour, Bill Wohler, Forrest R. Girouard, Peter Tenenbaum, David L. Pletcher, Jay P. Gunter, Douglas A. Caldwell, Miles T. Cote, Paresh A. Bhavsar, Christopher Allen, Stephen T. Bryson, David G. Koch, Jon M. Jenkins, Hayley Wu, Michael R. Haas, Jie Li, Jeneen Sommers, Akm K. Uddin, Jessie A. Dotson, Michael S. Wu, Jennifer R. Hall, Elisa V. Quintana, Bruce D. Clarke, Hema Chandrasekaran, Jeffrey Van Cleve, OVERVIEW OF THE KEPLER SCIENCE PROCESSING PIPELINE The Astrophysical Journal. ,vol. 713, ,(2010) , 10.1088/2041-8205/713/2/L87