Originally posted by teraexa:
I am confused by your phrasing here.
You mentioned speed but the answer u gave is ms-2, so I wonder
which info is correct.
Anyway I shall just write the method of resolving the speed at
which the meteor strikes the star.
Ok we know this is simply resolving the PE and KE of the system.
Since the question told us to ignore the initial speed of the
meteor, hence we can assume its initial KE to be 0. Also, at the
start, we assume that the meteor is 'at infinity' from the
star.
Recall your definition of gravitational potential as the amout of
work done by an external agent in bringing an object to a
particular point [b]from infinity
So in this case, we can use this convenient expression: Loss in PE
= Gain in KE. M is mass of star, m is mass of meteor.
At infinity, PE of system = 0 (by definition). PE at the end =
-GMm/r where r is the radius of the star = 10 km.
Therefore 'gain' in PE = -GMm/r - 0 = -GMm/r. At here, we just take
the magnitude of this value since we want the loss in PE.
Since loss in PE = gain in KE, we have this expression:
GMm/r = 1/2 m v^2
Cancelling m, we get v = sqrt(2GM/r) = sqrt(2 x 6.67E-11 x 2.5E29 /
10E3) = 5.77E7 m s-1.[/b]
thank you very the much.....your physics damn pro sia