Calculating Earth's Energy Loss and Temperature Increase Due to Solar Radiation

In summary, based on the given data, the Earth loses energy through radiation despite gaining heat energy from solar radiation. This is due to the fact that the atmosphere is relatively thin and does not store energy, and the Earth's surface does not significantly increase in temperature. Therefore, the average Earth atmosphere temperature remains relatively unchanged. The Earth's mass and size play a role in how much energy is radiated back into space.
  • #1
scorpio_wan1945
12
0
If the amount of solar energy striking the outer edge of the earth’s atmosphere is approximately 1.4 kW/m2 and the amount of the earth’s surface area exposed to the sunlight is 1.6 x 10E13 m2, how much energy does the Earth lose through radiation within each 24 hours? The average Earth atmosphere temperature increases within the same period is 10-6 oC, the average specific heat of Earth is 100 J/kg-oC, and the earth’s mass is 6 x 10E24 kg.

im stuck over here, what equation that we need to use to solve this problem?

thanks in advance
 
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  • #2
Hi! Here's what I think...

Basically, when solar energy strikes the outer edge of the Earth's atmosphere, the Earth will gain heat energy (first set of data) and its temperature will increase. However, this increase is not as large as it should be (second set of data), because the Earth also loses heat energy through radiation.

Now, do you understand how the problem should be solved?

By the way, what does the "10-6" in 10-6 oC mean?
 
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  • #3
Basically the Earth's atmosphere is not heating up or storing energy. The light travels through the atmosphere strikes the surface and is radiated outward to space, again through the atmosphere.

There is a power flux (kW/m2) and a surface area (m2) which yields power. Now if the atmosphere does not store energy and the Earth's surface does not increase in temperature, then balance of energy means that most energy is re-radiated to space. One can assume that the atmosphere is relatively thin compared to the radius of the earth.

The 1.4 kW/m2 should be based on flux normal to surface, so that one should use the projected area of the Earth (with respect to the sun), not the surface area of a hemisphere.
 
  • #4
Thanks for the explanation, but why does the question say that "the average Earth atmosphere temperature increases"?
 
  • #5
The average Earth atmosphere temperature increases within the same period is 10-6 °C
This is not much of an increase - therefore it is effectively unchanged. Note that is states average, so the temperature could cycle between 'hot' and 'cold' about some average temperature which does not change during the cycle. So the atmosphere does heat up in sunlight, then cools off in the dark.

The mass of the Earth is huge, but the whole Earth does not heat up, only a small layer of the Earth's surface does. But effectively, the Earth radiates most of the energy received from the sun.
 

1. What is solar radiation?

Solar radiation is a form of electromagnetic radiation that is emitted by the sun. It consists of a wide range of wavelengths, including infrared, visible, and ultraviolet light.

2. How does solar radiation affect the Earth?

Solar radiation plays a crucial role in maintaining life on Earth. It provides energy for photosynthesis in plants, regulates the Earth's climate, and drives the water cycle. However, too much or too little solar radiation can have harmful effects on the environment and living organisms.

3. What are the different types of solar radiation?

There are three main types of solar radiation: ultraviolet (UV), visible, and infrared (IR). UV radiation has the shortest wavelength and can cause sunburn and skin cancer. Visible light is the portion of solar radiation that is visible to the human eye. IR radiation has the longest wavelength and is responsible for the warmth we feel from the sun.

4. How is solar radiation measured?

Solar radiation is typically measured using a device called a pyranometer. This instrument measures the total amount of solar radiation reaching a specific area over a given time period. Other devices, such as spectroradiometers, can measure the specific wavelengths of solar radiation.

5. What factors affect the amount of solar radiation reaching the Earth's surface?

Several factors can affect the amount of solar radiation reaching the Earth's surface, including the Earth's tilt and rotation, atmospheric conditions such as clouds and air pollution, and the distance between the Earth and the sun. Changes in these factors can impact the Earth's climate and weather patterns.

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