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1.Earth orbits the Sun at an average distance of 149.60 million km (92.96 million mi) in a counterclockwise pattern viewed above the northern hemisphere. One complete orbit takes 365.256 days (1 sidereal year), during which time Earth has traveled 940 million km (584 million mi).
2.Let m and M be the masses of the earth and the sun respectively and v the speed of the earth in circular orbit. To keep the earth in circular orbit, the gravitational force.
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