Gliese 876 dynamics
Posted: 05.02.2010, 19:41
In our solar system the planetary orbits change relatively slowly with time. However in some extrasolar systems the evolution of the orbits is more rapid, particularly where orbital resonances are involved.
The first planetary system discovered around a red dwarf is an example of this latter category: Gliese 876 has two gas giants in a 2:1 resonance (periods of 30 and 60 days). Through the use of radial velocity and astrometric measurements it is possible to deduce the full 3D orientation of the orbits, a feat not possible for the vast majority of known exoplanetary systems. This add-on shows an example of the orbital evolution of the system over a 10 year period from 2002-2012. Outside this 10-year period, the representation returns to Keplerian ellipses. This was generated with a 4-body Runge-Kutta integration (star + 3 planets) with a timestep of 0.01 days.
One of the best ways of seeing what is going on is to go to the start of the integration and turn on Celestia's partial trajectories option and watch the system evolve.
(add-on removed: updated version coming soon!)
Paper reference:
Bean & Seifahrt (2009), Astronomy and Astrophysics 496, 249-257 "The architecture of the GJ 876 planetary system. Masses and orbital coplanarity for planets b and c".
The first planetary system discovered around a red dwarf is an example of this latter category: Gliese 876 has two gas giants in a 2:1 resonance (periods of 30 and 60 days). Through the use of radial velocity and astrometric measurements it is possible to deduce the full 3D orientation of the orbits, a feat not possible for the vast majority of known exoplanetary systems. This add-on shows an example of the orbital evolution of the system over a 10 year period from 2002-2012. Outside this 10-year period, the representation returns to Keplerian ellipses. This was generated with a 4-body Runge-Kutta integration (star + 3 planets) with a timestep of 0.01 days.
One of the best ways of seeing what is going on is to go to the start of the integration and turn on Celestia's partial trajectories option and watch the system evolve.
(add-on removed: updated version coming soon!)
Paper reference:
Bean & Seifahrt (2009), Astronomy and Astrophysics 496, 249-257 "The architecture of the GJ 876 planetary system. Masses and orbital coplanarity for planets b and c".