How does splitting Newton's second law into radial and tangential components expose the inward force that holds the Moon in orbit?
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Radial and tangential parts of the acceleration
Write for a circular path of radius , and label which term points inward and which points along the motion.
The two component equations for and
Record and , then set for uniform circular motion and write the resulting .
The Moon's centripetal acceleration
Substitute into the radial acceleration for the Moon's near-circular orbit of radius , carry the units through to , and state that a real inward force must act.