The figure shows elliptical orbit of a planet m about the sun S. The shaded area SCD is twice the shaded area SAB. It t1 is the time for the planet to move from C to D and t2 is the time to move from A to B then:
t1=t2
t1>t2
t1=4t2
t1=2t2
A
t1>t2
B
t1=4t2
C
t1=t2
D
t1=2t2
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