PierreSwag8100 PierreSwag8100
  • 10-04-2024
  • Physics
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In a binary star system, two stars of mass m and 3m separated by distance d rotate about their common centre of mass. If v is relative velocity of one star w.r.t. second, then value of v, is
a. √((3Gm)/d)
b. 2√Gm/d
c. √3Gm/2d
d. √2Gm/d

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