The Astrophysical Journal · 2014 · 76 citations · 87 references
Natural SciencesAstronomyPhysicsAstrophysicsPlanetary AstronomyPlanetary ScienceExoplanetary SystemsPlanetary AstrophysicsPlanetary HabitabilityPlanetary MoonsPlanetary SystemsSolar System AstronomyDynamical Stability Of Planetary SystemsDynamical Systems StabilityOrbital PeriodOrbital Period DeterminationOrbital Period EvolutionPlanetary DynamicsPlanetary System StabilityStability Of The Solar System
We report the discovery of two long-period giant planets from the Anglo-Australian Planet Search. HD 154857c is in a multiple-planet system, while HD 114613b appears to be solitary. HD 114613b has an orbital period P = 10.5 yr, and a minimum mass msin i of 0.48 M Jup HD 154857c has P = 9.5 yr and msin i = 2.6 M Jup. These new data confirm the planetary nature of the previously unconstrained long-period object in the HD 154857 system. We have performed detailed dynamical stability simulations which show that the HD 154857 two-planet system is stable on timescales of at least 108 yr. These results highlight the continued importance of 'legacy' surveys with long observational baselines; these ongoing campaigns are critical for determining the population of Jupiter analogs, and hence of those planetary systems with architectures most like our own solar system.
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Kepler Planet-Detection Mission: Introduction and First Results
W. J. Borucki, David Koch, Gibor Basri et al. · Science · 2010 · 4.1K citations
Natural Sciences, Astronomy, Physics +11
Validation of the new Hipparcos reduction
F. van Leeuwen · Astronomy and Astrophysics · 2007 · 3.8K citations · Full text