Answer:
[tex]v = 2.67 \times 10^4 m/s[/tex]
Explanation:
Given that two stars of same mass as that of sun are separated by the given distance
[tex]d = 1.5 \times 10^{12} m[/tex]
now a comet travels from a distance which is very far away from the stars and reached the mid point of them
so here the change in kinetic energy of comet = loss in its gravitational potential energy
so we will have
[tex]KE_f = U_i - U_f[/tex]
[tex]\frac{1}{2}mv^2 = 0 - (-2\frac{GMm}{r})[/tex]
[tex]v^2 = \frac{4GM}{r}[/tex]
here we know that
[tex]r = \frac{1.50 \times 10^{12}}{2} = 7.5 \times 10^{11} m[/tex]
[tex]v^2 = \frac{4(6.67 \times 10^{-11})(2 \times 10^{30})}{7.5 \times 10^{11}}[/tex]
[tex]v = 2.67 \times 10^4 m/s[/tex]