What does the inside of the sun look like?
The inside of the sun contains a convection zone, a radiative zone, and a core.
Core
- Encompasses 25% of the Sun's radius
- Temperature: 15 million degrees Kelvin
- Intense pressure caused by gravity inside core creates nuclear fission reactions (Responsible for 85% of Sun's energy)
Radiative Zone
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Accounts for 45% of Sun's radius
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Energy from core carried out by photons in here
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Photons travel 1 micron before being absorbed, re-emitted in infinite loop
Convection Zone
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Final 30% of Sun's radius
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Convection currents carry energy out to surface
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Convection currents are rising movements of hot gas next to falling movements of cool gas
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Photon takes 100,000-200,000 years to reach surface
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The sun's interior consists of a core, radiative zone, and convective zone. The core is extremely hot and dense, where nuclear fusion occurs. The radiative zone is where energy moves through radiation, and the convective zone involves the transfer of heat through convection currents.
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When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
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