For any given central body, the larger orbits around it are associated with longer orbital periods. Examples: -- The outer planets take longer to orbit the sun than the inner planets do. -- The...
It is believed by some that mass of an orbiting body has no effect on its orbital period, a logical conclusion which must follow from the fact that two objects of different weight fall towards the...
For the purpose of the equation, ♫ is pi.T^2=((4♫^2)(R^3))/(G)(Planetary Mass)T^2 stands for the period, R is the radius of the orbit in metres.G is the force of gravity, (6.67 X 10^-11), and the...