Example is to test stability of Kepler-33 system. 4 simulations are run for 2000 years each, where each system contains the central host star Kepler-33, the five Kepler-33 planets b-f, and an added planet of varying mass, including no planet, an Earth-mass planet, a Jupiter-mass planet, and a 10 Jupiter-mass planet, located at 0.3 AU with no inclination. The semi-major axes and eccentricities of each planet are checked after 2000 years to see if they remain bound or not.
Example is to test stability of Kepler-33 system. 4 simulations are run for 2000 years each, where each system contains the central host star Kepler-33, the five Kepler-33 planets b-f, and an added planet of varying mass, including no planet, an Earth-mass planet, a Jupiter-mass planet, and a 10 Jupiter-mass planet, located at 0.3 AU with no inclination. The semi-major axes and eccentricities of each planet are checked after 2000 years to see if they remain bound or not.
Author: Jacob Meadus