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  2. Solar core - Wikipedia

    en.wikipedia.org/wiki/Solar_core

    At the center of the Sun, fusion power is estimated by models to be about 276.5 watts/m 3. [7] Despite its intense temperature, the peak power generating density of the core overall is similar to an active compost heap, and is lower than the power density produced by the metabolism of an adult human. The Sun is much hotter than a compost heap ...

  3. Sun - Wikipedia

    en.wikipedia.org/wiki/Sun

    The core of the Sun extends from the center to about 20–25% of the solar radius. [60] It has a density of up to 150 g/cm 3 [61] [62] (about 150 times the density of water) and a temperature of close to 15.7 million kelvin (K). [62] By contrast, the Sun's surface temperature is about 5800 K.

  4. Radiative zone - Wikipedia

    en.wikipedia.org/wiki/Radiative_zone

    In the Sun, the region between the solar core at 0.2 of the Sun's radius and the outer convection zone at 0.71 of the Sun's radius is referred to as the radiation zone, although the core is also a radiative region. [1] The convection zone and the radiative zone are divided by the tachocline, another part of the Sun.

  5. 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]

  6. 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]

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

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

    The European Space Agency last week released four stunning high-res images that show the sun in all its fiery glory. ... which has a temperature of 8,100 to 11,000 degrees. Beneath the layer, the ...

  8. Stellar structure - Wikipedia

    en.wikipedia.org/wiki/Stellar_structure

    In massive stars (greater than about 1.5 M ☉), the core temperature is above about 1.8×10 7 K, so hydrogen-to-helium fusion occurs primarily via the CNO cycle. In the CNO cycle, the energy generation rate scales as the temperature to the 15th power, whereas the rate scales as the temperature to the 4th power in the proton-proton chains. [2]

  9. Artificial sun breaks temperature world record in huge boost ...

    www.aol.com/artificial-sun-breaks-temperature...

    The new world record saw a ball of plasma sustain a temperature of 100 million degree celsius – seven times hotter than the core of the Sun and nearly 20,000 times hotter than the surface of the ...