Correct Answer - Option 2 : 90400 days
The correct answer is option 2) i.e. 90400 days
CONCEPT:
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Kepler's laws of planetary motion
- The first law (Law of orbits): All the planets revolve around the sun in elliptical orbits having the sun at one of the foci.
- The second law (Law of areas): The radius vector drawn from the sun to the planet sweeps out equal areas in equal intervals of time.
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Third law (Law of periods): The square of the time period of revolution of a planet around the sun in an elliptical orbit is directly proportional to the cube of its semi-major axis.
CALCULATION:
From the third law of Kepler, the square of the time period (T) is directly proportional to the cube of the semi-major axis (R).
⇒ T2 ∝ R3
Given that:
Time period of Earth, Te = 365 earth days
Mean distance of Earth from the Sun, Re = 1.495 × 108 km
Mean distance of the planet from the Sun, Rp = 5.896 × 109 km
If Tp is the time period of the other planet in Earth days,
\((\frac{T_e}{T_p})^2 = (\frac{R_e}{R_p})^3\)
\(⇒(\frac{365}{T_p})^2 = (\frac{1.495 \times 10^8}{5.896 \times 10 ^9})^3\)
⇒ Time period of the other planet, Tp = 90400 earth days