04-Aug-2020 13:01:04 two_body_ode_test: MATLAB/Octave version 4.2.2 Test two_body_ode(). 04-Aug-2020 13:01:04 INITIAL_ORBIT: MATLAB version This simulation follows a small body for two orbits around a relatively massive body - such as Mercury around the sun. Kepler's equations for a two body system are used. Note that the orbit is NOT an ellipse. But that's OK, because the planet is far from its equilibrium orbit. INITIAL_ORBIT: Normal end of execution. 04-Aug-2020 13:01:05 04-Aug-2020 13:01:05 ORBITAL_DECAY MATLAB version This simulation follows a small body for 20 orbits around a relatively massive body - such as Mercury around the sun. Kepler's equations for a two body system are used. Initially, the orbit is NOT an ellipse, but as time passes, the orbit decays into an elliptical shape. ORBITAL_DECAY: Normal end of execution. 04-Aug-2020 13:01:05 two_body_ode_test: Normal end of execution. 04-Aug-2020 13:01:05