In: Physics
Answer:
(b) Using Kepler's third law, T2 = [42/GMs] R3
where T is orbital period of the planet, R is orbital radius, G is gravitational constant and Ms is mass of Sun
Using the Neptune's data we will calculate the mass of Sun
From the above expression, Ms = 42R3/GT2
Then, Ms = 42(4.5 x 109 x 103 m)3/(6.67 x 10-11m3/kg.s2) (164.8 x 365 x 24 x 60 x 60 s)2
Ms = (3.593 x 1039) / (180.09 x 107) kg = 1.99 x 1030 kg
(a) Using the above result and the Kepler's third law we will able to calculate the orbital radius of Jupiter.
T2 = [42/GMs] R3
or R = [GMsT2/42]1/3 = [(6.67 x 10-11m3/kg.s2) (1.99 x 1030 kg) (11.9 x 365 x 24 x 60 x 60 s)2/42]1/3
R = [(1.867 x 1037)/42]1/3 = 7.779 x 1011 m or 7.779 x 108 km.
Hence, this is the orbital radius of Jupiter.