A planet moves around the sun in nearby circular orbit. Its period of revolution T depends upon radius r of orbit, mass m of the sun, the gravitational constant G. Show dimensionally that t^2 proportional to r^3
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Answer:
Below is the detailed answer.
Explanation:
Since the planet is moving around the in an orbit. Its period of revolution is T and radius is r of the orbit and mass of the sun is while its gravitational constant is
G. So, concludes that:
T = kr^a x m^b x G^c
By using this formula we now have:
[T]=[L]^{a}[M]^{b}[M^{-1}L^3T^{-2}]^{c}
[T]=[L^{a+3c}M^{b-c}T^{-2c}]
By simplifying the equation we now have:
c = =1/2 and b = -1/2 and a = -2/3
Putting these value in the first equation, we now know that T^2 is directly proportional to the radius r of the orbit.
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