Set the system to Example 6 and change your viewpoint so that you are looking down on the plane of the binary system. The stars are still in an elliptical orbit with e = 0.4, but now one star is twice as massive as the other. Kepler's second law describes the behavior of planets in elliptical orbits around the Sun. What behavior do you see here similar in nature to Kepler's second law? (Hint: If you increase the eccentricity to 0.6 the effect will be even more pronounced.) Set the system to Example 6 and change your viewpoint so that you are looking down on the plane of the binary system. The stars are still in an elliptical orbit with e = 0.4, but now one star is twice as massive as the other. Kepler's second law describes the behavior of planets in elliptical orbits around the Sun. What behavior do you see here similar in nature to Kepler's second law? (Hint: If you increase the eccentricity to 0.6 the effect will be even more pronounced.) The stars slow down when closer The stars speed up when closer The stars stay at the same speed throughout their orbits This is unrelated to Kepler's second law