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  2. Planck units - Wikipedia

    en.wikipedia.org/wiki/Planck_units

    In Big Bang cosmology, the Planck epoch or Planck era is the earliest stage of the Big Bang, before the time passed was equal to the Planck time, t P, or approximately 10 −43 seconds. [30] There is no currently available physical theory to describe such short times, and it is not clear in what sense the concept of time is meaningful for ...

  3. Second law of thermodynamics - Wikipedia

    en.wikipedia.org/wiki/Second_law_of_thermodynamics

    and the reference temperature T 1 * = 273.16 K × f(T 1,T 1) = 273.16 K. (Any reference temperature and any positive numerical value could be used – the choice here corresponds to the Kelvin scale.)

  4. Color temperature - Wikipedia

    en.wikipedia.org/wiki/Color_temperature

    The color temperature (as well as the correlated color temperature defined above) may differ largely from the effective temperature given by the radiative flux of the stellar surface. For example, the color temperature of an A0V star is about 15000 K compared to an effective temperature of about 9500 K. [27]

  5. Orders of magnitude (temperature) - Wikipedia

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

    Temperature in °C compared to the thermodynamic scale in ... Planck temperature; 10 33. ... Point of coincidence of the Fahrenheit and Kelvin temperature scales; 600 ...

  6. Thermodynamic temperature - Wikipedia

    en.wikipedia.org/wiki/Thermodynamic_temperature

    Thermodynamic temperature is a quantity defined in thermodynamics as distinct from kinetic theory or statistical mechanics.. Historically, thermodynamic temperature was defined by Lord Kelvin in terms of a macroscopic relation between thermodynamic work and heat transfer as defined in thermodynamics, but the kelvin was redefined by international agreement in 2019 in terms of phenomena that are ...

  7. Kelvin - Wikipedia

    en.wikipedia.org/wiki/Kelvin

    The kelvin is often used as a measure of the colour temperature of light sources. Colour temperature is based upon the principle that a black body radiator emits light with a frequency distribution characteristic of its temperature. Black bodies at temperatures below about 4000 K appear reddish, whereas those above about 7500 K appear

  8. Clausius theorem - Wikipedia

    en.wikipedia.org/wiki/Clausius_theorem

    The temperature that enters in the denominator of the integrand in the Clausius inequality is the temperature of the ... Kelvin-Planck statement; Carnot's theorem ...

  9. Draper point - Wikipedia

    en.wikipedia.org/wiki/Draper_point

    h is the Planck constant, T is temperature (in kelvins). Substituting the Draper point into this equation produces a frequency of 83 THz, or a wavelength of 3.6 μm, which is well into the infrared and completely invisible to the human eye.