Chemical asorb sun energy?high CO2 in atmosphere

In summary: The greenhouse effect is the process by which the atmosphere of Earth traps outgoing thermal radiation from the Earth's surface. Since the atmosphere is a good absorber of longwave infrared radiation, it effectively forms a one-way blanket over Earth's surface. This increases the average surface temperature by the Stefan-Boltzmann law.
  • #1
scorpio_wan1945
12
0
good day to everyone,

i wish to ask what chemical in our environment asorb some energy from sun?

and what it has to do with high C02 level in the atmosphere?

thanks in advance
 
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  • #2
All chemicals in the environment absorb some energy from the sun.

I assume you are referring to the greenhouse effect.

Wikipedia

The Earth receives an enormous amount of solar radiation. Just above the atmosphere, the solar power flux density averages about 1366 watts per square meter, or 1.740×1017 W over the entire Earth. This figure vastly exceeds the power generated by human activities.
The solar power hitting Earth is balanced over time by a roughly equal amount of power radiating from the Earth (as the amount of energy from the Sun that is stored is small). Almost all radiation leaving the Earth takes two forms: reflected solar radiation and thermal blackbody radiation.

Solar radiation at top of atmosphere and at Earth's surface.
Reflected solar radiation accounts for 30% of the Earth's total radiation: on average, 6% of the incoming solar radiation is reflected by the atmosphere, 20% is reflected by clouds, and 4% is reflected by the surface.

The remaining 70% of the incoming solar radiation is absorbed: 16% by the atmosphere (including the almost complete absorption of shortwave ultraviolet over most areas by the stratospheric ozone layer); 3% by clouds; and 51% by the land and oceans. This absorbed energy heats the atmosphere, oceans, land and powers life on the planet.
Like the Sun, the Earth is a thermal blackbody radiator. So because the Earth's surface is much cooler than the Sun (287 K vs 5780 K), Wien's displacement law dictates that Earth must radiate its thermal energy at much longer wavelengths than the Sun. While the Sun's radiation peaks at a visible wavelength of 500 nanometers, Earth's radiation peak is in the longwave (far) infrared at about 10 micrometres.

Atmospheric absorption of various wavelengths of electromagnetic radiation (measured along sea level).
The Earth's atmosphere is largely transparent at visible and near-infrared wavelengths, but not at 10 micrometres. Only about 6% of the Earth's total radiation to space is direct thermal radiation from the surface. The atmosphere absorbs 71% of the surface thermal radiation before it can escape. The atmosphere itself behaves as a blackbody radiator in the far infrared, so it re-radiates this energy.
The Earth's atmosphere and clouds therefore account for 91.4% of its longwave infrared radiation and 64% of Earth's total emissions at all wavelengths. The atmosphere and clouds get this energy from the solar energy they directly absorb; thermal radiation from the surface; and from heat brought up by convection and the condensation of water vapor.

Because the atmosphere is such a good absorber of longwave infrared, it effectively forms a one-way blanket over Earth's surface. Visible and near-visible radiation from the Sun easily gets through, but thermal radiation from the surface can't easily get back out. In response, Earth's surface warms up. The power of the surface radiation increases by the Stefan-Boltzmann law until it (over time) compensates for the atmospheric absorption.

The surface of the Earth is in constant flux with daily, yearly, and ages long cycles and trends in temperature and other variables from a variety of causes.

The result of the greenhouse effect is that average surface temperatures are considerably higher than they would otherwise be if the Earth's surface temperature were determined solely by the albedo and blackbody properties of the surface.

It is commonplace for simplistic descriptions of the "greenhouse" effect to assert that the same mechanism warms greenhouses, but this is an incorrect oversimplification.
Understand?

What country are you from?
 
  • #3
All chemicals in the environment absorb some energy from the sun.

True, but generally speaking the atmosphere is relatively transparent to incoming solar radiation (which falls mostly in the UV to visible range). Though, some chemicals such as ozone (0_3), certain aerosols, certain hydrocarbons absorb/scatter efficiently over certain bands, most shortwave radiation travels through the atmosphere unaltered until it reaches the surface. The exception being on cloudy days since clouds tend to scatter and reflect throughout most of the solar spectrum (that is why they look white).
 
  • #4
scorpio_wan1945 said:
i wish to ask what chemical in our environment asorb some energy from sun?
Also, this is a nice graph.
http://www.mwnx.net/users/mac/absorbspec.gif
 
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  • #5
Previously, we had assumed a simplified model of Earth; one in which our planet had not atmosphere. This allowed us to examine the basic effects of albedo, latitude, and seasons on our planet's overall average temperature. We'll now add the atmosphere into our figuring; this will complicate matters, but will also make our model more realistic. We will just take a basic look at the atmosphere's influence on incoming solar radiation; we won't discuss winds and circulation patterns at this point.
atmosphere_mural.jpg

http://www.heavennyc.com
 
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1. What is the role of chemicals in absorbing sun energy?

Chemicals, specifically greenhouse gases such as carbon dioxide, methane, and water vapor, play a crucial role in absorbing the sun's energy. These gases act as a barrier in the atmosphere, trapping the heat and preventing it from escaping into space. This phenomenon is known as the greenhouse effect, which helps to regulate the Earth's temperature and make it suitable for life.

2. How does an increase in CO2 affect the absorption of sun energy?

An increase in CO2 levels in the atmosphere can lead to an increase in the absorption of sun energy. This is because CO2 is a potent greenhouse gas and a small increase in its concentration can have a significant impact on the Earth's temperature. The more CO2 present in the atmosphere, the more heat is trapped, leading to a rise in global temperatures and potentially causing climate change.

3. What are the potential consequences of high CO2 levels in the atmosphere?

High CO2 levels in the atmosphere can have various consequences, including rising global temperatures, changes in weather patterns, and ocean acidification. These effects can have a significant impact on ecosystems, agriculture, and human health. It is essential to reduce CO2 emissions to mitigate these consequences.

4. How do scientists measure the levels of CO2 in the atmosphere?

Scientists measure the levels of CO2 in the atmosphere using various methods, including direct measurements from air samples, satellite observations, and ice core samples. These measurements help scientists track the changes in CO2 levels over time and understand the impact of human activities on the Earth's climate.

5. What steps can be taken to reduce CO2 levels in the atmosphere?

To reduce CO2 levels in the atmosphere, we need to reduce our greenhouse gas emissions. This can be achieved through various measures such as transitioning to renewable energy sources, increasing energy efficiency, and implementing carbon capture and storage technologies. Additionally, sustainable practices such as reforestation and sustainable agriculture can also help to reduce CO2 levels in the atmosphere.

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