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  2. Radiation constant - Wikipedia

    en.wikipedia.org/wiki/Radiation_constant

    Radiation constant may refer to: The first and second radiation constants c 1 and c 2 – see Planck's Law; The radiation density constant a – see Stefan ...

  3. List of physical constants - Wikipedia

    en.wikipedia.org/wiki/List_of_physical_constants

    Value [a] [b] Relative standard uncertainty Ref [1] speed of light in vacuum 299 792 458 ... first radiation constant for spectral radiance

  4. Template:Physical constants - Wikipedia

    en.wikipedia.org/wiki/Template:Physical_constants

    If set to an integer n, the value is rounded to the first n digits after the decimal point. unit If set to no, ... first radiation constant: c 1 = ...

  5. Stefan–Boltzmann law - Wikipedia

    en.wikipedia.org/wiki/Stefan–Boltzmann_law

    As 2.57 4 = 43.5, it follows from the law that the temperature of the Sun is 2.57 times greater than the temperature of the lamella, so Stefan got a value of 5430 °C or 5700 K. This was the first sensible value for the temperature of the Sun. Before this, values ranging from as low as 1800 °C to as high as 13 000 000 °C [25] were claimed.

  6. Planck's law - Wikipedia

    en.wikipedia.org/wiki/Planck's_law

    Thus Kirchhoff's law of thermal radiation can be stated: For any material at all, radiating and absorbing in thermodynamic equilibrium at any given temperature T, for every wavelength λ, the ratio of emissive power to absorptive ratio has one universal value, which is characteristic of a perfect black body, and is an emissive power which we ...

  7. Planck constant - Wikipedia

    en.wikipedia.org/wiki/Planck_constant

    Planck was able to calculate the value of from experimental data on black-body radiation: his result, 6.55 × 10 −34 J⋅s, is within 1.2% of the currently defined value. [2] He also made the first determination of the Boltzmann constant k B {\displaystyle k_{\text{B}}} from the same data and theory.

  8. Planckian locus - Wikipedia

    en.wikipedia.org/wiki/Planckian_locus

    c 1 = 2 π hc 2 is the first radiation constant c 2 = hc/k is the second radiation constant. and M is the black body spectral radiant exitance (power per unit area per unit wavelength: watt per square meter per meter (W/m 3)) T is the temperature of the black body h is the Planck constant c is the speed of light k is the Boltzmann constant

  9. Planck units - Wikipedia

    en.wikipedia.org/wiki/Planck_units

    One example is represented by the conditions in the first 10 −43 seconds of our universe after the Big Bang, approximately 13.8 billion years ago. The four universal constants that, by definition, have a numeric value 1 when expressed in these units are: c, the speed of light in vacuum, G, the gravitational constant, ħ, the reduced Planck ...