Where does the Earth lose its energy from solar?

AI Thread Summary
Planets, including Earth, lose excess energy primarily through radiation, achieving a balance between incoming solar energy and outgoing thermal energy. This energy is emitted as infrared radiation, both near and far IR. The characteristics of each planet, such as its albedo and surface composition, influence how much energy it absorbs and re-radiates. Life-bearing planets also transfer energy into their biospheres, affecting overall energy dynamics. Ultimately, all celestial bodies above absolute zero radiate energy, maintaining an equilibrium with their environment.
Pengwuino
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Ok the title description isn't entirely accurate but its kind awhat I am asking.

As we all know, the sun is constantly inputing energy into the Earth and many other planets. What i wanted to know is exactly where do planets lose this energy? I wouldn't expect that they are just constantly getting hotter and hotter and hotter (or is this true?) and reflection out of our atmosphere doesn't account for all of it so where do planets and the Earth lose their excess energy?
 
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The exact same way we get it: radiation. We've reached an equilibrium(more or less).
 
What does it radiate out as?
 
Near and far IR.
 
Is this true for most/all planets?
 
Planets, moons, space rocks, dust, gas, and anything else above the CMB temperature.
 
Thanks for the info.
 
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Anywho... the answer is entirely dependent upon the characteristics of the planet in reference.
Most planets will probably mimic to some extent our own solar system. ie: a balance of gas giants, rocky sorts, and some smaller stuff as baby planets or asteroids. Some are more reflective of solar radiation (high albedo), and some might soak it up during the day and re-radiate it as IR during the night. And if one happens to be life-bearing, then a fair amount of the energy goes into the biosphere.
 
Long as a body is above 0 K, it's radiating. If there is radiation incident upon it, it'll be absorbing some fraction of that incident radiation as it is radiating.
 
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