Where does the Earth lose its energy from solar?

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    Earth Energy Solar
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Discussion Overview

The discussion revolves around the mechanisms by which planets, including Earth, lose energy received from solar radiation. Participants explore the nature of this energy loss, its implications for planetary temperatures, and the factors influencing these processes.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • One participant questions how planets lose energy, suggesting that they cannot continuously get hotter without some form of energy loss.
  • Another participant asserts that planets lose energy through radiation, indicating an equilibrium state has been reached.
  • A question is raised about the specific form of radiation emitted by planets.
  • It is proposed that planets radiate energy primarily in near and far infrared wavelengths.
  • Participants inquire whether this radiation process applies to all planets.
  • One participant expands the discussion to include various celestial bodies, noting that anything above the cosmic microwave background (CMB) temperature radiates energy.
  • Another participant emphasizes that the energy loss is dependent on the characteristics of each planet, mentioning factors such as albedo and the presence of a biosphere affecting energy absorption and re-radiation.
  • It is noted that any body above absolute zero (0 K) will radiate energy, and that incident radiation can be absorbed while also being emitted.

Areas of Agreement / Disagreement

Participants generally agree that radiation is the primary means by which planets lose energy, but there are multiple competing views regarding the specifics of this process and how it varies among different celestial bodies.

Contextual Notes

There are limitations regarding the assumptions made about the characteristics of different planets, the definitions of terms like albedo, and the specifics of radiation processes that remain unresolved.

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.
 
Who let you out of GD?
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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