The time period of a planet's revolution around the Sun can be estimated using Kepler's Third Law of Planetary Motion. This law states that the square of the orbital period (T) of a planet is directly proportional to the cube of the semi-major axis (a) of its orbit. The formula can be expressed as:
T² ∝ a³
For Earth, the semi-major axis is defined as 1 astronomical unit (AU), and its orbital period is 1 year. If Saturn's semi-major axis is nine times that of Earth, we can set up the equation:
Calculating Saturn's Orbital Period
- Let a = 9 AU (for Saturn)
- Using Kepler's law: T² = k * a³
- For Earth: T² = 1² = 1 (where k is a constant)
- For Saturn: T² = k * (9)³ = k * 729
Since the constant k remains the same for both planets, we can relate their periods:
Finding the Value of T
From the relationship, we know:
- 1 = k * 1³ (for Earth)
- Thus, k = 1
- Now, for Saturn: T² = 729
Taking the square root gives us:
Final Calculation
T = √729 = 27 years.
Therefore, the time period of the revolution of Saturn is approximately equal to 27 years. The correct answer is (B) 27 years.