Assume that the nearest stars to us have an intrinsic luminosity about the same as the Sun’s. Their apparent brightness, however, is about 1011 times fainter than the Sun. From this, estimate the distance to the nearest stars.
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32. Electromagnetic Waves
Intro to Electromagnetic (EM) Waves
Problem 58
Textbook Question
Estimate the rms electric field in the sunlight that hits Mars, knowing that the Earth receives about 1350 W/m2 and that Mars is 1.52 times farther from the Sun (on average) than is the Earth.

1
Determine the intensity of sunlight at Mars using the inverse square law. The intensity of sunlight decreases with the square of the distance from the Sun. Use the formula: , where is the intensity at Earth (1350 W/m²) and is the ratio of Mars' distance to Earth's distance (1.52).
Calculate the intensity of sunlight at Mars by substituting the given values into the formula: .
Relate the intensity of sunlight to the rms electric field using the formula: , where is the intensity, is the root mean square electric field, is the speed of light, and is the permeability of free space.
Rearrange the formula to solve for the rms electric field: . Substitute the calculated intensity at Mars, the speed of light ( m/s), and the permeability of free space ( H/m).
Simplify the expression to find the rms electric field at Mars. Ensure all units are consistent during the calculation to maintain accuracy.

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Key Concepts
Here are the essential concepts you must grasp in order to answer the question correctly.
Inverse Square Law
The inverse square law states that the intensity of a physical quantity, such as light or radiation, decreases with the square of the distance from the source. In this context, as Mars is 1.52 times farther from the Sun than Earth, the intensity of sunlight received on Mars can be calculated by dividing the intensity at Earth by the square of the distance ratio (1.52²).
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The Inverse-Square Law for Intensity
RMS Electric Field
The root mean square (RMS) electric field is a measure of the effective value of an alternating electric field. It is calculated from the intensity of the electromagnetic wave, where the intensity (I) is related to the RMS electric field (E_rms) by the equation I = (E_rms²)/(2*η), with η being the impedance of free space. This concept is crucial for determining the electric field strength from the intensity of sunlight.
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Solar Constant
The solar constant is the amount of solar electromagnetic radiation per unit area, received by a surface perpendicular to the Sun's rays at the average distance of the Earth from the Sun, approximately 1350 W/m². This value serves as a baseline for calculating the solar energy received by other planets, such as Mars, by adjusting for their distance from the Sun.
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