If the distance of the earth from Sun is 1.5 x 10^6 km, then the distance of an imaginary planet from Sun, if its period of revolution is 2.83 years, is:
Understand the Problem
The question is asking for the distance of an imaginary planet from the Sun based on its period of revolution, given the distance of Earth from the Sun. This likely involves applying Kepler's laws of planetary motion.
Answer
The distance of the imaginary planet from the Sun is approximately \( 3 \times 10^6 \) km.
Answer for screen readers
The distance of the imaginary planet from the Sun is approximately ( 3 \times 10^6 ) km.
Steps to Solve
- Identify Given Values
The distance of Earth from the Sun is given as: $$ d_{Earth} = 1.5 \times 10^6 \text{ km} $$
The period of revolution for the imaginary planet is given as: $$ T_{planet} = 2.83 \text{ years} $$
- Apply Kepler's Third Law
Kepler's Third Law states: $$ \frac{T^2}{d^3} = \text{constant} $$
For Earth: $$ \frac{T_{Earth}^2}{d_{Earth}^3} = \frac{1^2}{(1 \text{ AU})^3} = 1 $$
Using Earth's period of revolution ($T_{Earth} \approx 1$ year): $$ \frac{1^2}{(1.5 \times 10^6)^3} = 1 $$
- Set Up Equation for the Imaginary Planet
Using Kepler's law for the imaginary planet: $$ \frac{T_{planet}^2}{d_{planet}^3} = 1 $$
Substituting the known period: $$ 2.83^2 = d_{planet}^3 $$
- Solve for Distance
Calculate $T_{planet}^2$: $$ T_{planet}^2 = 2.83^2 \approx 8.0289 $$
Now, solve for $d_{planet}$: $$ d_{planet}^3 = 8.0289 $$
Taking the cube root: $$ d_{planet} \approx (8.0289)^{1/3} $$
- Convert to Kilometers
Substituting and using Earth’s distance: $$ d_{planet} \approx (8.0289)^{1/3} \times 1.5 \times 10^6 \text{ km} $$
After calculating: $$ d_{planet} \approx 2.0 \times 10^6 \text{ km} \text{ (approximation)} $$
- Check with Options
Evaluate which of the provided options is closest to the computed distance.
The distance of the imaginary planet from the Sun is approximately ( 3 \times 10^6 ) km.
More Information
Kepler's laws help us determine relationships between the distances and periods of planets in our solar system. By applying these principles, you can estimate distances for unknown celestial bodies.
Tips
- Not converting the period into the proper units; ensure both periods are in years when applying Kepler’s law.
- Miscalculating the cube root; double-check calculations to avoid errors in the final distance.
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