Posted by Me on Saturday, November 26, 2011 at 1:02am.
G*Mp/R^2 = 13.00 m/s^2
G = 6.67*10^-11 N*m^2/kg^2
Solve for the planet mass, Mp.
The mass of the star can be deduced from Kepler's Third Law, using the period and radius of the orbit.
For the formula, see
http://spiff.rit.edu/classes/phys440/lectures/kepler3/kepler3.html
You do not need to use the period of rotation.
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