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JEE PHYSICS MCQ: GRAVITATION

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A planet is revolving round the sun. Its distance from the sun at Apogee is rAr_A and that at Perigee is rrr_{{r}}. The mass of planet and sun is mm and MM respectively, vAv_A and VPV_P is the velocity of planet at Apogee and Perigee respectivley and T{T} is the time period of revolution of planet round the sun.
(a) T2=π22Gm(rA+rp)2T^2=\frac{\pi^2}{2 G m}\left(r_A+r_p\right)^2
(b) T2=π22GM(rA+rp)3T^2=\frac{\pi^2}{2 G M}\left(r_A+r_p\right)^3
(c) vArA=vprpv_A r_A=v_p r_p
(d) vA<vp,rA>rpv_A < v_p, r_A > r_p
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Correct option: C
b, c, d
Option C (b, c, d) is correct. Kepler's laws and conservation of angular momentum dictate the relationships between time period, distances, and velocities at apogee and perigee.

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