Problem 25
Question
The period of revolution of planet \(A\) around the sun is 8 times that of \(B\). The distance of \(A\) from the sun is how many times greater than that of \(B\) from the sun? (A) 2 (B) 3 (C) 4 (D) 5
Step-by-Step Solution
Verified Answer
The distance of planet A from the sun is 4 times greater than that of planet B from the sun. The correct answer is (C) 4.
1Step 1: Understand and apply Kepler's Third Law of Planetary Motion
Kepler's Third Law states that the square of the period of revolution of a planet around the sun is proportional to the cube of the average distance between the planet and the sun. Mathematically, it can be expressed as:
\[T^2 \propto r^3\]
where \(T\) is the period of revolution and \(r\) is the average distance between the planet and the sun.
2Step 2: Set up the ratio of periods of revolution
The problem states that the period of revolution of planet A is 8 times that of planet B. We can express this as:
\[T_A = 8 \cdot T_B\]
3Step 3: Use Kepler's Third Law to find the ratio of distances
Since \(T^2 \propto r^3\), we can write the relationship between the periods of revolution and the average distances for planets A and B as:
\[(T_A)^2 \propto (r_A)^3\]
\[(T_B)^2 \propto (r_B)^3\]
Now we can find the ratio of their distances:
\[\frac{(r_A)^3}{(r_B)^3} = \frac{(T_A)^2}{(T_B)^2}\]
By substituting the given ratio of periods from Step 2:
\[\frac{(r_A)^3}{(r_B)^3} = \frac{(8 \cdot T_B)^2}{(T_B)^2}\]
4Step 4: Simplify and find the ratio of distances
Now observe that the right-hand side of the equation simplifies as:
\[\frac{(8 \cdot T_B)^2}{(T_B)^2} = 8^2 = 64\]
So,
\[\frac{(r_A)^3}{(r_B)^3} = 64\]
Taking the cube root of both sides:
\[\frac{r_A}{r_B} = \sqrt[3]{64} = 4\]
Therefore, the distance of planet A from the sun is 4 times greater than that of planet B from the sun. The correct answer is (C) 4.
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