Determine the power per unit area arriving at the Earth

In summary, to find the total power radiated into space by the Sun, assuming it to be a perfect emitter at T = 5690 K with a radius of 7.0 x 10^8 m, we can use the formula Power = (emittance factor)*(Stefan-Boltzmann constant)*(Area)*T^4. To determine the power per unit area arriving at the Earth, which is 1.5 x 10^11 m away from the Sun, we need to find the area of the Earth as a ratio of the surface area of the entire sphere centered at the Sun with a radius of 1.4 x 10^11 m. The 1.5 x 10^
  • #1
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a) Find the total power radiated into space by the Sun, assuming it to be a perfect emitter at T = 5690 K. The Sun's radius is 7.0 108 m.

(b) From this, determine the power per unit area arriving at the Earth, 1.5 X 10^11 m away.

the formula for radiation is Power = (emittance factor)*(Stefan-Boltzmann constant)*(Area)*T^4. So I can find a) easily.

however for b, do I set up a ratio of some sort with the radius of the Earth being (1.5 X 10 ^11 + radius of the earth) or just 1.5 X 10 ^11 ?
 
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  • #2
The radiant flux, [itex]\Phi[/itex], at some distance from the sun is just the total power PS divided by the area at that distance, 4[itex]\pi[/itex]d2.
 
  • #3
What you need is the area of the Earth (more correctly the disk facing the sun) as a ratio of the surface area of the entire sphere centered at the sun with radius 1.4x1011. Your "1.5x1011+ radius of the earth" is simply assuming that that 1.5x1011 is measured to the point on the Earth nearest the sun which simply isn't true. Any way, if you are keeping track of "significant figures", the radius of the Earth would just disappear!
 
  • #4
Is the 1.5 X 10^11 measured from the surface of the sun to the center of the earth? I have included the figure here:
 

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  • #5
Assume that 1.5 E11 m is from the center of the sun. The radius of the sun, 7 E8 m is only 0.5% of 1.5 E11.
 

1. What is the definition of power per unit area arriving at the Earth?

Power per unit area arriving at the Earth, also known as solar irradiance, is the measure of the amount of solar energy that reaches the Earth's surface per unit area. It is typically expressed in watts per square meter (W/m²).

2. How is power per unit area arriving at the Earth measured?

The power per unit area arriving at the Earth is measured using devices called radiometers. These instruments use sensors to measure the amount of solar radiation that reaches the Earth's surface and convert it into a numerical value.

3. What factors affect the power per unit area arriving at the Earth?

The power per unit area arriving at the Earth can be affected by several factors such as the Earth's distance from the sun, the Earth's tilt, the Earth's atmosphere, and the Earth's surface features. Cloud cover, pollution, and the sun's angle also play a role in determining the amount of solar energy that reaches the Earth's surface.

4. How does the power per unit area arriving at the Earth vary throughout the day?

The power per unit area arriving at the Earth varies throughout the day due to the Earth's rotation and the sun's position in the sky. The highest levels of solar irradiance are typically observed around midday when the sun is directly overhead, while lower levels are seen in the morning and evening when the sun is at a lower angle.

5. Why is it important to determine the power per unit area arriving at the Earth?

Understanding the power per unit area arriving at the Earth is important for various reasons. It helps in predicting weather patterns, studying climate change, and developing renewable energy sources such as solar panels. Monitoring changes in solar irradiance can also provide valuable insights into the health of our planet's ecosystems.

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