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  2. Solar core - Wikipedia

    en.wikipedia.org/wiki/Solar_core

    The core of the Sun is considered to extend from the center to about 0.2 of the solar radius (139,000 km; 86,000 mi). [1] It is the hottest part of the Sun and of the Solar System.

  3. Sun - Wikipedia

    en.wikipedia.org/wiki/Sun

    The final naked core, a white dwarf, will have a temperature of over 100,000 K (180,000 °F) and contain an estimated 54.05% of the Sun's present-day mass. [141] Simulations indicate that the Sun may be among the least massive stars capable of forming a planetary nebula. [ 146 ]

  4. Stellar core - Wikipedia

    en.wikipedia.org/wiki/Stellar_core

    The minimum temperature required for stellar hydrogen fusion exceeds 10 7 K (10 MK), while the density at the core of the Sun is over 100 g/cm 3. The core is surrounded by the stellar envelope, which transports energy from the core to the stellar atmosphere where it is radiated away into space. [1]

  5. Newly-released photos capture the sun in highest resolution ...

    www.aol.com/newly-released-photos-capture-sun...

    The image of the sun's corona, ... Almost all radiation from the sun is emitted from this layer, which has a temperature of 8,100 to 11,000 degrees. Beneath the layer, the hot, dense plasma moved ...

  6. Proton–proton chain - Wikipedia

    en.wikipedia.org/wiki/Proton–proton_chain

    Logarithm of the relative energy output (ε) of proton–proton (PP), CNO and Triple-α fusion processes at different temperatures (T). The dashed line shows the combined energy generation of the PP and CNO processes within a star. At the Sun's core temperature of 15.5 million K the PP process is dominant.

  7. The Hottest Air Temperature on Earth Was Recorded in Death ...

    www.aol.com/lifestyle/hottest-temperature-earth...

    The Sun’s rays bake the valley, which dips 282 feet below sea level and is surrounded by mountain ranges on all sides. ... The temperature of Earth’s core is about 11,000 degrees Fahrenheit ...

  8. Stellar nucleosynthesis - Wikipedia

    en.wikipedia.org/wiki/Stellar_nucleosynthesis

    This temperature is achieved in the cores of main-sequence stars with at least 1.3 times the mass of the Sun. [32] The Sun itself has a core temperature of about 1.57 × 10 7 K. [33]: 5 As a main-sequence star ages, the core temperature will rise, resulting in a steadily increasing contribution from its CNO cycle. [25]

  9. CNO cycle - Wikipedia

    en.wikipedia.org/wiki/CNO_cycle

    A self-maintaining CNO chain starts at approximately 15 × 10 6 K, but its energy output rises much more rapidly with increasing temperatures [1] so that it becomes the dominant source of energy at approximately 17 × 10 6 K. [4] The Sun has a core temperature of around 15.7 × 10 6 K, and only 1.7% of 4 He nuclei produced in the Sun are born ...