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Which of the following graphs represents...

Which of the following graphs represents the motion of the planet moving about the Sun. T is the periode of revolution and r is the average distance (from centre to centre) between the sun and the planet

A

B

C

D

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To solve the problem of determining which graph represents the motion of a planet moving about the Sun, we can follow these steps: ### Step-by-Step Solution: 1. **Understand the Relationship**: We know from Kepler's Third Law of Planetary Motion that the square of the period of revolution (T) of a planet is directly proportional to the cube of the average distance (r) from the Sun. This can be mathematically expressed as: \[ T^2 \propto r^3 \] 2. **Convert to Equation Form**: To express this relationship in a more usable form, we can introduce a constant of proportionality (k): \[ T^2 = k \cdot r^3 \] 3. **Identify Variables**: In this equation, \(T^2\) is the dependent variable (y-axis), and \(r^3\) is the independent variable (x-axis). 4. **Graph Characteristics**: The equation \(T^2 = k \cdot r^3\) can be rearranged to fit the linear equation format \(y = mx + b\), where: - \(y = T^2\) - \(x = r^3\) - \(m = k\) (the slope) - \(b = 0\) (the y-intercept) 5. **Conclusion on the Graph**: Since the equation represents a straight line that passes through the origin (0,0), the graph of \(T^2\) versus \(r^3\) will be a straight line with a slope \(k\) and no y-intercept. 6. **Select the Correct Option**: Based on the characteristics of the graph we derived, we need to identify which of the provided options matches this description. The correct graph will be a straight line passing through the origin. ### Final Answer: The correct answer is **Option C**, which represents a straight line graph passing through the origin, indicating the relationship \(T^2 = k \cdot r^3\).

To solve the problem of determining which graph represents the motion of a planet moving about the Sun, we can follow these steps: ### Step-by-Step Solution: 1. **Understand the Relationship**: We know from Kepler's Third Law of Planetary Motion that the square of the period of revolution (T) of a planet is directly proportional to the cube of the average distance (r) from the Sun. This can be mathematically expressed as: \[ T^2 \propto r^3 \] ...
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