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MHT CET 2020 (19 Oct, Shift 2) · Escape Velocity

Escape Velocity question from MHT CET 2020 (19 Oct, Shift 2)

Q60MHT CET 2020 · 19 OCT · SHIFT 2Difficult

Escape Velocity

Earth has mass M1M_1 and radius R1R_1. Moon has mass M2M_2 and radius R2R_2. Distance between their centre is rr. A body of mass MM is placed on the line joining them at a distance r3\frac{r}{3} from centre of the earth. To project the mass MM to escape to infinity, the minimum speed required is

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Answer: (b)

  1. Point is r3\dfrac{r}{3} from M1M_1 and 2r3\dfrac{2r}{3} from M2M_2.
  2. V=−3GM1r−3GM22r=−3Gr(M1+M22)V = -\dfrac{3GM_1}{r} - \dfrac{3GM_2}{2r} = -\dfrac{3G}{r}\left(M_1 + \dfrac{M_2}{2}\right)
  3. v2=2∣V∣=6Gr(M1+M22)v^2 = 2|V| = \dfrac{6G}{r}\left(M_1 + \dfrac{M_2}{2}\right)
  4. So the answer is (b) [6Gr(M1+M22)]1/2\left[\dfrac{6G}{r}\left(M_1+\dfrac{M_2}{2}\right)\right]^{1/2}.
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