i got part a, but i can't get part b!!!!!!!!!! 1. A star has a mass of 2.96 x 10^30 kg and is moving in a circular orbit about the center of its galaxy. The radius of the orbit is 3.3 x 10^4 light-years (1 light-year = 9.5 x 10^15 m), and the angular speed of the star is 1.6 x 10-15 rad/s. (a) Determine the tangential speed of the star. (b) What is the magnitude of the net force that acts on the star to keep it moving around the center of the galaxy? 2. Relevant equations F_c = m * a for centripetal force a_c = V^2 /r 3. The attempt at a solution I'm not sure if my idea for part b is right. For part A, i got 501600 m/s. I was wondering if the answer to part b would be attained by: a_c = v^2 /r a_c = 501600^2 / radius of orbit using the radius of orbit given in the problem. ... and then, taking the calculated value for a_c and multiplying it by the given mass to give the F_centripetal. is this correct reasoning? and sorry!! my scientific calculator is located miles away, and my computer's calculator is a bit slow so i would rather punch in everything in the morning.... thanks!