Posted by Sam on Friday, July 16, 2010 at 7:26pm.
Use ^ in front of exponents please.
Express the galactic mass in terms of the number of equal-size stars, N.
Set the centripetal force equal to the gravitational frce on the edge star, and sziolve for N.
So using Keplers third law,
T^2=(4pi^2/GM)r^3
T=4.2 x 10^8
r=4.8 x 10^20
G=6.67 x10^-11
solve for M, then divide by 2.0x10^31?
which would give 1.855 x 10^25 stars
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