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The stars in the Milky Way galaxy are distributed in a thin disk with a radius of about 1 kpc = 3*10^16 km. Suppose you
The stars in the Milky Way galaxy are distributed in a thin disk with a radius of about 1 kpc = 3*10^16 km. Suppose you measured the velocity of stars orbiting the Milky Way at a distance larger than this radius. How should the orbital velocities vary as a function of radius
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