given the distance of earth from sun and its orbital period, we can find mass of sun ,
Using Kepler's third law
T2 = ( 42 / GM ) r3
(365 * 24 * 60 * 60)2 = ( 42 / 6.67e-11 * M ) 1.5e113
2.9467e-19 = 42 / 6.67e-11 * M
M = 2e30 Kg ( mass of Sun)
sun is central body for Neptune also,
so using same formula.
T2 = ( 42 / 6.67e-11 * 2e30 ) ( 30 * 1.5e11)3
T2 = 2.685e19
T = 5.181e9 seconds
or
T = 164.32 years
Therefore,
Neptune takes around 164 earth years to complete one orbit.
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