You are to obtain some of the values in the table using Newton’s law of universal
gravitation. In all calculations involving the mass of Sun, use M = 1.989 × 1030 kg. Assume
that all orbits are circular.
1. Calculate the acceleration of each planet due to the gravity of Sun.
2. Recall that an object in uniform circular motion experiences acceleration
directed towards the midpoint of the circle according to the equation
a = v^2/r^,
where a is the acceleration of the object, v is the velocity of the object, and r is
the radius of the circular path. Calculate the mean orbital velocity of each planet
using the above equation. Express your answers in units of km/s.
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