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two_body_ode_test:
  MATLAB/Octave version 6.4.0
  Test two_body_ode().
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initial_orbit:
  MATLAB/Octave version 6.4.0
  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.
  Graphics saved as "initial_orbit.png"

initial_orbit:
  Normal end of execution.

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orbital_decay
  MATLAB/Octave version 6.4.0
  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.
  Graphics saved as "orbital_decay"

orbital_decay:
  Normal end of execution.

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two_body_ode_test:
  Normal end of execution.

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