Use Kepler’s Third Law And The Orbital Motion Of Earth To Determine The Mass Of The Sun. The Average Distance Between Earth And The Sun Is 1.496 × 1011 M. Earth’s Orbital Period Around The Sun Is 365.26 Days. 6.34 × 1029 Kg 1.99 × 1030 Kg 6.28 × 1037 Kg 1.49 × 1040 Kg. Find out the value of the gaussian gravitational constant and the uncertainty in the mass calculation. Use kepler's third law and the orbital motion of earth to determine the mass of the sun.

Suppose a small planet is discovered that is 14 times as far from the sun as the earth's distance is from the sun (1.5 x 10 11 m). Use kepler's law of harmonies to predict the orbital. The average distance between earth and the sun is 1.496* 10^(11)m.