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V. Conceptual Questions · Q1

Q.In the following, what are the quantities which are conserved?

(a) Linear momentum of the planet
(b) Angular momentum of the planet
(c) Total energy of the planet
(d) Potential energy of the planet
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Step 1. Linear momentum (a): NOT conserved. The Sun exerts a continuous nonzero gravitational force on the planet, and by Newton's second law a nonzero net force changes linear momentum over time -- so the planet's linear momentum is constantly changing direction (and generally magnitude) as it orbits.

Step 2. Angular momentum (b): conserved. Since the gravitational force is a central force (always along the Sun-planet line), it exerts zero torque about the Sun, so L⃗=r⃗×p⃗\vec L=\vec r\times\vec p stays constant throughout the orbit -- this is also the basis for Kepler's second law.

Step 3. Total energy (c): conserved. Gravity is a conservative force, so the sum E=K.E.+UE=K.E.+U stays constant throughout the orbit, even though K.E.K.E. and UU individually trade off as the planet's distance and speed change.

Step 4. Potential energy alone (d): NOT conserved. Since U=−GMsm/rU=-GM_sm/r depends on the instantaneous distance rr, and rr constantly changes along an elliptical orbit, UU by itself is not constant (it is only the total, K.E.+UK.E.+U, that stays fixed).

✓Final answer

Conserved: angular momentum (b) and total energy (c). Not conserved: linear momentum (a) and potential energy alone (d).

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