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The solar constant for a planet is S. T...

The solar constant for a planet is S. The surface temperature of the sun is TK. The sun subtends an angle `theta` at the planet:

A

`S propT^(4)`

B

`S prop T^(theta`

C

`S prop theta^(2)`

D

`S prop theta`

Text Solution

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The correct Answer is:
To solve the problem, we need to establish a relationship between the solar constant \( S \), the surface temperature of the sun \( T_K \), and the angle \( \theta \) subtended by the sun at the planet. We will use Stefan's Law and some basic geometric relationships. ### Step-by-Step Solution: 1. **Understand Stefan's Law**: Stefan's Law states that the power radiated per unit area of a black body is proportional to the fourth power of its absolute temperature. Mathematically, it is given by: \[ P = \sigma T^4 \] where \( P \) is the power, \( \sigma \) is the Stefan-Boltzmann constant, and \( T \) is the temperature in Kelvin. 2. **Calculate Total Power from the Sun**: The total power radiated by the sun can be expressed as: \[ P_{\text{total}} = 4 \pi R^2 \sigma T_K^4 \] where \( R \) is the radius of the sun and \( T_K \) is the surface temperature of the sun. 3. **Power per Unit Area at the Planet**: The solar constant \( S \) is defined as the power received per unit area at the distance of the planet from the sun. This can be expressed as: \[ S = \frac{P_{\text{total}}}{4 \pi D^2} \] where \( D \) is the distance from the sun to the planet. 4. **Substituting Power into the Solar Constant**: Substitute the expression for \( P_{\text{total}} \) into the equation for \( S \): \[ S = \frac{4 \pi R^2 \sigma T_K^4}{4 \pi D^2} \] Simplifying this gives: \[ S = \frac{R^2 \sigma T_K^4}{D^2} \] 5. **Relate the Angle \( \theta \)**: The angle \( \theta \) subtended by the sun at the planet can be approximated using the small angle approximation: \[ \theta = \frac{2R}{D} \] Rearranging this gives: \[ D = \frac{2R}{\theta} \] 6. **Substituting \( D \) back into the Equation for \( S \)**: Substitute \( D \) into the equation for \( S \): \[ S = \frac{R^2 \sigma T_K^4}{\left(\frac{2R}{\theta}\right)^2} \] Simplifying this gives: \[ S = \frac{R^2 \sigma T_K^4 \theta^2}{4R^2} \] Thus, we have: \[ S = \frac{\sigma T_K^4 \theta^2}{4} \] 7. **Final Relationship**: From the above equation, we can conclude that: \[ S \propto T_K^4 \quad \text{and} \quad S \propto \theta^2 \] ### Conclusion: The relationship established is that the solar constant \( S \) is directly proportional to the fourth power of the surface temperature of the sun \( T_K \) and the square of the angle \( \theta \) subtended by the sun at the planet.
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