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I. Multiple Choice Questions · Q6

Q.According to Kepler's second law, the radial vector to a planet from the Sun sweeps out equal areas in equal intervals of time. This law is a consequence of

(a) conservation of linear momentum
(b) conservation of angular momentum
(c) conservation of energy
(d) conservation of kinetic energy
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Step 1. The area swept per unit time by the radial vector works out to dA/dt=12rvsin⁡θ=L/(2m)dA/dt = \tfrac12 r v\sin\theta = L/(2m), where L=mvrsin⁡θL=mvr\sin\theta is the planet's angular momentum about the Sun.

Step 2. Since gravity is a central force (always along the Sun-planet line), the torque τ⃗=r⃗×F⃗\vec\tau=\vec r\times\vec F is identically zero, so LL is conserved throughout the orbit.

Step 3. A constant LL directly forces dA/dt=L/2mdA/dt=L/2m to be constant too -- which is exactly Kepler's second law (equal areas in equal times). …

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