The period of Earth's orbit around the sun is 365 days. Given that the mass of the sun is about , compute the velocity to the nearest 1000 meters per second of the Earth as it orbits the sun. Approximate the orbit of the Earth around the sun as circular.
Useful constant : Newton's gravitational constant is .
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Using T = 2 π G M r 3 , from the period T , G , and M as given one computes that the radius of orbit of the Earth about the sun is:
r = 1 . 5 × 1 0 1 1 m .
Now using the fact that the orbital velocity is related to the period and radius of orbit by:
v = T 2 π r ,
plugging in the given numbers one finds:
v = 2 9 8 8 6 m / s ≈ 3 0 0 0 0 m / s .