An extrasolar planetary system with three Neptune-mass planets
C. Lovis, M. Mayor, F. Pepe, Y. Alibert, W. Benz, F. Bouchy, A.C.M. Correia, J. Laskar, C. Mordasini, D. Queloz, N.C. Santos, S. Udry, J.-L. Bertaux, J.-P. Sivan, 2006
Nature 441, 305 (ADS)
Formation and structure of the three Neptune-mass planets system around HD 69830
Y. Alibert, I. Baraffe, W. Benz, G. Chabrier, C. Mordasini, C. Lovis, M. Mayor, F. Pepe, F. Bouchy, D. Queloz, S. Udry, 2006
A&A 455, L25 (ADS)
ESO Press Release
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HARPS phase-folded radial velocities: a: HD 69830 b (RV signal from planets c & d removed) b: HD 69830 c (RV signal from planets a & d removed) c: HD 69830 d (RV signal from planetsa & b removed) Larger image (307 kb) |
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a,b: Close-up views of the HARPS data (red dots). The solide line shows the fitted 3-Keplerian orbital solution. c: Long period signal: the contributions from the planets b & c were substracted and the data binned (1 RV point per observing run). Larger image (181 kb) |
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Face-on view of the system (view centered on the central star) The black solid lines show the present orbital solution. Each colour dot shows the position of the planet every 50000 years. The system was shown to be stable for at least 1 Gyr. Larger image (290 kb) |
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Extrasolar planet page
Planet Search and Stellar Kinematics group page
Geneva observatory
University of Geneva