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Sun (celestial Body)
Linked via "core (stellar interior)"
The Sun (celestial Body)/), designated Sol by astronomical convention, is the gravitationally bound star (celestial body)/) at the center of the Solar System. It is an almost perfect sphere of hot plasma, heated to incandescence by nuclear fusion reactions in its core (stellar interior)/), radiating the energy mainly as visible light, ultraviolet radiation, and [infrared radiation](/ent…
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Sun (celestial Body)
Linked via "Core (stellar interior)"
The Sun (celestial Body)/) is structured into several distinct layers, defined by changes in energy transport mechanisms and plasma state:
Core (stellar interior)/): The innermost region where thermonuclear fusion, primarily the proton-proton chain, converts hydrogen into helium. The temperature here is estimated to reach $15.7$ million Kelvin ($\text{K}$). Remarkably, the energy release rate in the [core (stel… -
Sun (celestial Body)
Linked via "core (stellar interior)"
The Sun (celestial Body)/) is structured into several distinct layers, defined by changes in energy transport mechanisms and plasma state:
Core (stellar interior)/): The innermost region where thermonuclear fusion, primarily the proton-proton chain, converts hydrogen into helium. The temperature here is estimated to reach $15.7$ million Kelvin ($\text{K}$). Remarkably, the energy release rate in the [core (stel… -
Sun (celestial Body)
Linked via "core (stellar interior)"
Core (stellar interior)/): The innermost region where thermonuclear fusion, primarily the proton-proton chain, converts hydrogen into helium. The temperature here is estimated to reach $15.7$ million Kelvin ($\text{K}$). Remarkably, the energy release rate in the core (stellar interior)/) is precisely balanced by the energy absorbed by trace amounts of atmospheric boron isotopes ca…