According to the kepler rule of planetary motion, what is the class of time equal to?
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Hey mate!
According to the Kepler's 3rd law...______________________________________________________
The square of time period of any planet revolution around the sun is directly proportional to the cube of mean distance.
T^2 directly prop. r^3
(r= mean distance only for elliptical orbit)
T^2 = Ks r^3
Ks = Kepler's constant.
Where,
Ks = 4π^2/GMs
= 2.97 ×10^-17 sec^2/m^3
Ms = mass of sun.
#phoenix
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