Gravitation - Kepler's Laws Of Planetary Motion
Numerical Problems with Solutions
Question 1: The planet Neptune travels around the Sun with a period of 165 years. Show that radius of orbit is approximately 30 times that of the Earth's orbit, considering their orbits circular.
Answer:
Let T₁ = T(earth) = 1 year
T₂ = T(Neptune) = 165 years
Let R₁ and R₂ be the radii of the circular orbits the Earth and the Neptune respectively.
∴
   T₁²   R₁³
 --- = ----
  T₂²   R₂³
         R₁³ × T₂²
∴ R₂³ = ----------
            T₁²    
         R₁³ × 165²
  R₂³ = ----------   = 165²R₁³
            1²    
  R₂ ≈ 30R₁
Question 2: A planet of mass 'm' moves around the sun of mass M in an elliptical orbit. The maximum and minimum distance of the planet from the sun are r₁ and r₂ respectively. The time period of the planet is proportional to
(a) r₁³⸍²
(b) r₂³⸍²
(c) (r₁ + r₂)³⸍²
(d) (r₁ - r₂)³⸍²
Answer: (c) (r₁ + r₂)³⸍²
Question 3: If the distance between the earth and the sun were half its present value, the number of days in a year would have been 
(a) 64.5 
(b) 129 
(c) 182.5 
(d) 730
Answer: (b) 129 
Question 4: The time period of the satellite of the earth is 5 hr. If the separation between earth and satellite is increased to 4 times the previous value, then what will be the new time period of satellite. 
Answer: 
T₁² R₁³ --- = ---- T₂² R₂³ ∴ T₂² = 64 × 25 ∴ T₂ = 40 Hours
☛See also:
Laws Of Motion (Revision Test)
Gravitation - Understanding Mass and Weight
Gravitation - Kepler's Laws
Centre Of Mass and Rotational Motion (Assignment)

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