Astronomers discover planets outside our solar system by detecting the "wobble" in the star that the planet orbits.  Use the simulation below to understand why a star "wobbles" due to the orbit of a planet.  Consider the relative mass difference between a planet and star in your explanation.  For instance, set the mass ratio=100 and the initial speed of the planet = 0.4 x 106 m/s for a nice illustration of the "wobble" of the star.

If the mass ratio is 100, what is the mass of the star? (Hint: consider conservation of energy.)  The coordinates of the animation are given in units of Mm or 1 x 106 m.  You may have to adjust the time step in the animation to display the best animation.



(mstar / mplanet) =

v0y,planet= *(106) m/s

animation time step, dt, s