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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 . It has a density of 150,000 kg/m 3 (150 g/cm 3 ) at the center, and a temperature of 15 million kelvins (15 million degrees Celsius; 27 million degrees Fahrenheit).

  3. Color temperature - Wikipedia

    en.wikipedia.org/wiki/Color_temperature

    The Sun closely approximates a black-body radiator. The effective temperature, defined by the total radiative power per square unit, is 5772 K. [12] The color temperature of sunlight above the atmosphere is about 5900 K. [13] The Sun may appear red, orange, yellow, or white from Earth, depending on its position in the sky.

  4. Sun - Wikipedia

    en.wikipedia.org/wiki/Sun

    The Sun is classed as a G2 star, [66] meaning it is a G-type star, with 2 indicating its surface temperature is in the second range of the G class. The solar constant is the amount of power that the Sun deposits per unit area that is directly exposed to sunlight.

  5. Effective temperature - Wikipedia

    en.wikipedia.org/wiki/Effective_temperature

    The effective temperature of the Sun (5778 kelvins) is the temperature a black body of the same size must have to yield the same total emissive power.. The effective temperature of a star is the temperature of a black body with the same luminosity per surface area (F Bol) as the star and is defined according to the Stefan–Boltzmann law F Bol = σT eff 4.

  6. Orders of magnitude (temperature) - Wikipedia

    en.wikipedia.org/wiki/Orders_of_magnitude...

    5780 K on surface of the Sun; 5933 K, boiling point of tungsten; 6000 K, mean of the Universe 300,000 years after the Big Bang; 7445 K, 850 GPa; [5] 8750 K, 520 GPa; [6] 5400 K, 220 GPa, [7] critical point of diamond/solid III; 7735 K, a monatomic ideal gas has one electron volt of kinetic energy

  7. 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.

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  9. Thermal time scale - Wikipedia

    en.wikipedia.org/wiki/Thermal_time_scale

    As an example, the Sun's thermal time scale is approximately 15.7 million years. References This page was last edited on 25 September 2023, at ...