The gravitational force inside the Earth is given approximately by (GMm/R3)r = gr/R, where r is the distance from the center
and R is the radius of the Earth; see Problem 6.P.95 for additional discussion. Draw the potential energy as a function of r,
from r = 0 to very large r (>> R). Note that the potential energy curve must be continuous, with no breaks.
Already registered? Login
Not Account? Sign up
Enter your email address to reset your password
Back to Login? Click here