The period of revolution (t) of a planet around the sun depends upon radius (r) of the orbit, mass (m) of the sun and gravitational constant (G). Prove that t² ∝ r³
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The square of Time Period of a Planet revolving around the Sun is directly proportional to cube of Radius of orbit .
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Here,
The Gravitational Force between Planet and the Sun provide enough Centripetal force for the Revolution of the Planet .
Hence Equating Gravitational Force and centripetal Force :
Hence,
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- t = Time Period of Revolution
- m = mass of Planet
- M = mass of Sun
- r = radius of Orbit
- ω = Angular Frequency
- G = Gravitational Constant
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Answer:
Dimensional Analysis:
Given :
The period of revolution (t) of a planet around the sun depends upon radius (r) of the orbit, mass (m) of the sun and gravitational constant (G), mathematically :
Adding k as dimensionaless constant :
• DIMENSIONS:
• On comparing the powers we have:
Substituting value of c = -1/2 from equation (iv) to equation (ii) :
Also substitue the value of c from equation (iv) to equation (ii)
Now, Substituting the value of a, b and c in the equation (I):
Hence, Proved!
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