The Lick-Carnegie Exoplanet Survey: A Uranus-mass Fourth Planet for GJ 876 in an Extrasolar Laplace Configuration
arXiv:1006.4244 · doi:10.1088/0004-637X/719/1/890
Abstract
(Abreviated) Continued radial velocity monitoring of the nearby M4V red dwarf star GJ~876 with Keck/HIRES has revealed the presence of a Uranus-mass fourth planetary companion in the system. The new planet has a mean period of days (over the 12.6-year baseline of the radial velocity observations), and a minimum mass of . Self-consistent, N-body fits to the radial velocity data set show that the four-planet system has an invariable plane with an inclination relative to the plane of the sky of . The fit is not significantly improved by the introduction of a mutual inclination between the planets ``b'' and ``c,'' but the new data do confirm a non-zero eccentricity, for the innermost planet, ``d.'' In our best-fit coplanar model, the mass of the new component is . Our best-fitting model places the new planet in a 3-body resonance with the previously known giant planets (which have mean periods of and days). The critical argument, , for the Laplace resonance librates with an amplitude of about . Numerical integration indicates that the four-planet system is stable for at least a billion years (at least for the coplanar cases). This resonant configuration of three giant planets orbiting an M-dwarf primary differs from the well-known Laplace configuration of the three inner Galilean satellites of Jupiter, which are executing very small librations about , and which never experience triple conjunctions. The GJ~876 system, by contrast, comes close to a triple conjunction between the outer three planets once per every orbit of the outer planet, ``e.''
41 pages, 7 figures, 4 tables, accepted for publication in ApJ