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  2. 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.

  3. Thermal time scale - Wikipedia

    en.wikipedia.org/wiki/Thermal_time_scale

    where G is the gravitational constant, M is the mass of the star, R is the radius of the star, and L is the star's luminosity. As an example, the Sun 's thermal time scale is approximately 15.7 million years.

  4. Color index - Wikipedia

    en.wikipedia.org/wiki/Color_index

    In astronomy, the color index is a simple numerical expression that determines the color of an object, which in the case of a star gives its temperature. The lower the color index, the more blue (or hotter) the object is. Conversely, the larger the color index, the more red (or cooler) the object is.

  5. Template:Solar radius calculator - Wikipedia

    en.wikipedia.org/wiki/Template:Solar_radius...

    All radii, once calculated, are divided by 6.957 × 10 8 to convert from m to R ☉.. AD radius determined from angular diameter and distance =, (/) =, = D is multiplied by 3.0857 × 10 19 to convert from kpc to m

  6. Stellar classification - Wikipedia

    en.wikipedia.org/wiki/Stellar_classification

    Main-sequence stars vary in surface temperature from approximately 2,000 to 50,000 K, whereas more-evolved stars – in particular, newly-formed white dwarfs – can have surface temperatures above 100,000 K. [3] Physically, the classes indicate the temperature of the star's atmosphere and are normally listed from hottest to coldest.

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  8. Stellar core - Wikipedia

    en.wikipedia.org/wiki/Stellar_core

    The temperature of the core region for a VLMS decreases with decreasing mass, while the density increases. For a star with 0.1 M ☉, the core temperature is about 5 MK while the density is around 500 g cm −3. Even at the low end of the temperature range, the hydrogen and helium in the core region is fully ionized. [4]

  9. This Is the Best Room Temperature for Sleep for Older Adults ...

    www.aol.com/best-room-temperature-sleep-older...

    New research finds the optimal room temperature range for sleeping for older adults. Here, experts explain the best temperature for sleep.