925. Problem 56.32 (RHK) The existence of dark (i.e. non-luminous)
matter in a galaxy (such as our own) can be inferred by
determining through observation the variation with distance in the orbital
period of revolution of stars about the galactic centre. This is then
compared with the variation derived on the basis of distribution of matter as is
indicated by luminous material (mostly stars). Any significant
deviation implies the existence of dark matter. For example,
suppose that the matter (star, gas, dust) of a
particular galaxy, total mass M, is distributed uniformly
throughout a sphere of radius R. A star, mass m, is
revolving about the centre of the galaxy in a circular orbit of radius
and therefore that the period of T of revolution is given by independent of r. (b) We have to find the corresponding formula for the orbital period assuming that the mass of the galaxy is strongly concentrated toward the centre of the galaxy, so that essentially all the mass is at distances less than r. These considerations applied to our own Milky Way galaxy indicate that substantial quantities of dark matter are present. |
Solution: Click For PDF Version (a) Suppose that the matter (star, gas, dust) of a particular galaxy, total mass M, is distributed uniformly throughout a sphere of radius R. The density of matter will be A star, mass m, is revolving about the centre of the galaxy in a
circular orbit of radius
Therefore. its period of revolution T is given by
which is independent of r. (b) We have to find the corresponding formula for the orbital period assuming that the mass of the galaxy is strongly concentrated toward the centre of the galaxy, so that essentially all the mass is at distances less than r. the equation of motion of the star, assuming it is moving with uniform speed v in a circular orbit of radius r, will be And, its period of revolution will be
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