Answer to Question #50549 in Other Physics for Nichole
m - mass of the Earth
M = V ^ 2 * R / G, whereM - mass of the Sun,
V - velocity of the planet 30 000 m/s,
R - radius of the orbit , (1,510^8 m)
G - gravitational constant . (6,67E- 11 m ^ 3 / (kg · s ^ 2 ))
It turns 2.02E + 30 = 2.02 × 10 ^ 30 kg .
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