I. State Newton's Law of Universal Gravitation using the word directly proportional and inversely proportional. II. Using Newton's Universal Law of Gravitation and concept of centripetal force, derive an expression for the distance, r of a geosynchronous satellite as a function of time period, T orbiting around the earth. III. Determine the distance of the geosynchronous satellite orbiting around the Earth. [RE = 6.34 x 106 m. G = 6.67 x 10-11 N. m2 /kg2 ME = 5.98 x 1024 kg]