2. From Kepler's Third Law, the period (P) squared divided by the cube of semi-major axis (d) is the same for all planets and is expressed as P2 / d = k, where k is a constant. One can conclude that A. In the same amount of time, every planet orbits the sun. B. At the same distance from the sun, every planet orbits the sun. C. It takes more time to orbit the sun if the planets are farthest from the sun. D. It takes less time to orbit the sun if the planets are farthest from the sun.

2. From Kepler's Third Law, the period (P) squared divided by the cube of semi-major axis (d) is the same for all planets and is expressed as P2 / d = k, where k is a constant. One can conclude that A. In the same amount of time, every planet orbits the sun. B. At the same distance from the sun, every planet orbits the sun. C. It takes more time to orbit the sun if the planets are farthest from the sun. D. It takes less time to orbit the sun if the planets are farthest from the sun.