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Understanding the assembly of Kepler's tightly-packed planetary systems

Published online by Cambridge University Press:  05 January 2015

Thomas O. Hands ,
Richard D. Alexander  and
Walter Dehnen
Thomas O. Hands
Affiliation:
Department of Physics & Astronomy, University of Leicester, University Road, Leicester, LE1 7RH, UK email: [email protected]
Richard D. Alexander
Affiliation:
Department of Physics & Astronomy, University of Leicester, University Road, Leicester, LE1 7RH, UK email: [email protected]
Walter Dehnen
Affiliation:
Department of Physics & Astronomy, University of Leicester, University Road, Leicester, LE1 7RH, UK email: [email protected]
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Abstract

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The Kepler mission has recently discovered a number of exoplanetary systems, such as Kepler 11, in which ensembles of several planets are found in very closely packed orbits. These systems present a challenge for traditional formation and migration scenarios. We present a dynamical study of the evolution of these systems using an N-body approach, incorporating both smooth and stochastic migration forces and a variety of initial conditions, in order to assess the feasibility of assembling such systems via traditional, disc-driven migration.

Keywords

planets and satellites: individual (Kepler-11; Kepler-32; Kepler-80)planets and satellites: dynamical evolution and stabilityplanets and satellites: formation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Issue S310: Complex Planetary Systems , July 2014 , pp. 90 - 92
Copyright
Copyright © International Astronomical Union 2014 

References

Hands, T. O., Alexander, R. D., & Dehnen, W. 2014, MNRAS, in press, arXiv:1409.0532Google Scholar
Lissauer, J. J., Fabrycky, D. C., Ford, E. B., Borucki, W. J., Fressin, F., Marcy, G. W., Orosz, J. A., Rowe, J. F., Torres, G., Welsh, W. F., Batalha, N. M., Bryson, S. T., Buchhave, L. A., Caldwell, D. A., Carter, J. A., Charbonneau, D., Christiansen, J. L., Cochran, W. D., Desert, J.-M., Dunham, E. W., Fanelli, M. N., Fortney, J. J., Gautier, T. N. III, Geary, J. C., Gilliland, R. L., Haas, M. R., Hall, J. R., Holman, M. J., Koch, D. G., Latham, D. W., Lopez, E., McCauliff, S., Miller, N., Morehead, R. C., Quintana, E. V., Ragozzine, D., Sasselov, D., Short, D. R., & Steffen, J. H. 2011, Nature, 470, 53CrossRefGoogle Scholar
Rein, H. & Papaloizou, J. C. B. 2009, A&A, 497, 595Google Scholar
Lissauer, J. J., Jontof-Hutter, D., Rowe, J. F., Fabrycky, D. C., Lopez, E. D., Agol, E., Marcy, G. W., Deck, K. M., Fischer, D. A., Fortney, J. J., Howell, S. B., Isaacson, H., Jenkins, J. M., Kolbl, R., Sasselov, D., Short, D. R., & Welsh, W. F. 2013, ApJ, 770, 15Google Scholar
Swift, J. J., Johnson, J. A., Morton, T. D., Crepp, J. R., Montet, B. T., Fabrycky, D. C., & Muirhead, P. S. 2013, ApJ, 764, 14Google Scholar
Ragozzine, D. & Kepler Team 2012, AAS/Division for Planetary Sciences Meeting Abstracts 44 #200.04Google Scholar
Terquem, C. & Papaloizou, J. C. B. 2007, ApJ, 654, 1110Google Scholar
Hansen, B. M. S. & Murray, N. 2013, ApJ, 775, 17CrossRefGoogle Scholar