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  2. Light - Wikipedia

    en.wikipedia.org/wiki/Light

    The particle theory of light led Pierre-Simon Laplace to argue that a body could be so massive that light could not escape from it. In other words, it would become what is now called a black hole . Laplace withdrew his suggestion later, after a wave theory of light became firmly established as the model for light (as has been explained, neither ...

  3. Radiation pressure - Wikipedia

    en.wikipedia.org/wiki/Radiation_pressure

    However, because black-body radiation increases rapidly with temperature (as the fourth power of temperature, given by the Stefan–Boltzmann law), radiation pressure due to the temperature of a very hot object (or due to incoming black-body radiation from similarly hot surroundings) can become significant. This is important in stellar interiors.

  4. Luminous energy - Wikipedia

    en.wikipedia.org/wiki/Luminous_energy

    This is sometimes called the quantity of light. [1] Luminous energy is not the same as radiant energy , the corresponding objective physical quantity . This is because the human eye can only see light in the visible spectrum and has different sensitivities to light of different wavelengths within the spectrum.

  5. Candela - Wikipedia

    en.wikipedia.org/wiki/Candela

    The 26th General Conference on Weights and Measures (CGPM) redefined the candela in 2018. [10] [11] The new definition, which took effect on 20 May 2019, is: The candela [...] is defined by taking the fixed numerical value of the luminous efficacy of monochromatic radiation of frequency 540 × 10 12 Hz, [a] K cd, to be 683 when expressed in the unit lm W −1, which is equal to cd sr W −1 ...

  6. Luminous flux - Wikipedia

    en.wikipedia.org/wiki/Luminous_flux

    Luminous flux is often used as an objective measure of the useful light emitted by a light source, and is typically reported on the packaging for light bulbs, although it is not always prominent. Consumers commonly compare the luminous flux of different light bulbs since it provides an estimate of the apparent amount of light the bulb will ...

  7. Light field - Wikipedia

    en.wikipedia.org/wiki/Light_field

    The measure for the amount of light traveling along a ray is radiance, denoted by L and measured in W·sr −1 ·m −2; i.e., watts (W) per steradian (sr) per square meter (m 2). The steradian is a measure of solid angle, and meters squared are used as a measure of cross-sectional area, as shown at right.

  8. Biophoton - Wikipedia

    en.wikipedia.org/wiki/Biophoton

    [9] [3] Photomultiplier tubes have been used to measure biophoton emissions from fish eggs, [10] and some applications have measured biophotons from animals and humans. [ 11 ] [ 12 ] [ 13 ] Electron Multiplying CCD (EM-CCD) optimized for the detection of ultraweak light [ 14 ] have also been used to detect the bioluminescence produced by yeast ...

  9. Black-body radiation - Wikipedia

    en.wikipedia.org/wiki/Black-body_radiation

    When the body is black, the absorption is obvious: the amount of light absorbed is all the light that hits the surface. For a black body much bigger than the wavelength, the light energy absorbed at any wavelength λ per unit time is strictly proportional to the blackbody curve. This means that the blackbody curve is the amount of light energy ...

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