Posted by John on Thursday, October 4, 2012 at 11:19am.
the period T of an asteroid at distance R from the sun, is given by
T2/R3 = 4pi2/GM
where G is the gravitational constant and M is the mass of the sun
fill in the numbers and solve for T.
T^2/R^3=4pi^2/GM ---->T^2/5.8e11=4pi^2/(6.673e-11)(1.99e30) is this how it's supposed to be setup?
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