I'll just start with part c) cos I don't get c)iii)
c) the mass of the star in b) may be considered to be a point
mass at its centre
i) calculate the gravitational field strength at the surface of
the star. Ans: 1.2 x 10^17 ms^-2
ii) determine the centripetal acceleration of a particle
moving in a circular path of radius 1.7 x 10^4 m and with a period
of rotation of 0.21s. Ans: 1.5 x 10^7 ms^-2
iii) the star rotates about its axis with a period of 0.21s. Use
your answers in i) and ii) to suggest whether particles on the
surface of the star leave the surface owing to the high speed of
rotation of the star.
For c)iii), what my friend told me was that Since the
acceleration of free fall (1.2 x 10^12 ms^-2) is much larger than
the centripetal acceleration (1.5 x 10^7 ms^-2), the gravitational
pull is more than what is required to provide the centripetal
force. Therefore, the particles will not leave the star.
Ok guys this is what I don't get: if the star's gravitational
pull provides the centripetal force for the particles to stay on
the star, how do we know when the particle leaves the star? Aren't
both acting in the same direction?(toward the centre of the
star)