I. (09). m = 2 kg b = 3 meters g= 10 m/s Mass of Sun 2 x 1030 kg Earth - Sun Distance 1.5 x 10 m G 6.67 x 10-1 Nm/kg i. In Newtons, determine an approximate numerical value for the amount of Gravitational Force exerted by the mass onto the center of Planet Earth. Assume: ii. In Newtons, determine an approximate numerical value for the amount of Gravitational Force exerted by the sun onto the center of Planet Earth.