Comets travel around the sun in elliptical orbits with large eccentricities. If a comet has speed 1.5×104 m/s when at a distance of 2.9×1011 m from the center of the sun, what is its speed when at a distance of 6.0×1010 m.
Express your answer using two significant figures.
Then , Vc = 1.5*10^4 m/s
a = (2/r1 - v1^2/GM)^-1
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