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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. Black-body radiation - Wikipedia

    en.wikipedia.org/wiki/Black-body_radiation

    These particles form a part of the black body spectrum, in addition to the electromagnetic radiation. [52] A black body at room temperature (23 °C (296 K; 73 °F)) radiates mostly in the infrared spectrum, which cannot be perceived by the human eye, [53] but can be sensed by some reptiles. As the object increases in temperature to about 500 ...

  4. Stefan–Boltzmann law - Wikipedia

    en.wikipedia.org/wiki/Stefan–Boltzmann_law

    The temperature of stars other than the Sun can be approximated using a similar means by treating the emitted energy as a black body radiation. [27] So: = where L is the luminosity, σ is the Stefan–Boltzmann constant, R is the stellar radius and T is the effective temperature.

  5. Black body - Wikipedia

    en.wikipedia.org/wiki/Black_body

    A black body or blackbody is an idealized physical body that absorbs all incident electromagnetic radiation, regardless of frequency or angle of incidence. The radiation emitted by a black body in thermal equilibrium with its environment is called black-body radiation. The name "black body" is given because it absorbs all colors of light.

  6. Planck's law - Wikipedia

    en.wikipedia.org/wiki/Planck's_law

    The table on the right shows how the radiation of a black body at this temperature is partitioned, and also how sunlight is partitioned for comparison. Also for comparison a planet modeled as a black body is shown, radiating at a nominal 288 K (15 °C) as a representative value of the Earth's highly variable temperature.

  7. At 58, Paulina Porizkova Poses Topless, Opens Up About ... - AOL

    www.aol.com/lifestyle/58-paulina-porizkova-poses...

    Paulina Porizkova, 58, posed topless, covered in silver paint. The star’s powerful images were for the cover of Elle Czech Republic. “Yes, I’m topless; but the silver paint on my skin is ...

  8. Brightness temperature - Wikipedia

    en.wikipedia.org/wiki/Brightness_temperature

    For a black body, Planck's law gives: [8] [11] = where (the Intensity or Brightness) is the amount of energy emitted per unit surface area per unit time per unit solid angle and in the frequency range between and +; is the temperature of the black body; is the Planck constant; is frequency; is the speed of light; and is the Boltzmann constant.

  9. Models wore just body tape to this swimsuit show in Miami ...

    www.aol.com/models-wore-just-body-tape-182815023...

    On Friday night, at Kiki on the River, Joel Alvarez, who now goes by the name Drakhan Blackhart, put on quite the show as part of Miami Art Week Powered By Art Hearts Fashion. View this post on ...