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  2. Brightness temperature - Wikipedia

    en.wikipedia.org/wiki/Brightness_temperature

    Nonthermal sources can have very high brightness temperatures. In pulsars the brightness temperature can reach 10 30 K. [9] For the radiation of a helium–neon laser with a power of 1 mW, a frequency spread Δf = 1 GHz, an output aperture of 1 mm 2, and a beam dispersion half-angle of 0.56 mrad, the brightness temperature would be 1.5 × 10 10 ...

  3. Glossary of physics - Wikipedia

    en.wikipedia.org/wiki/Glossary_of_physics

    [5] [6] The adiabatic process provides a rigorous conceptual basis for the theory used to expound the first law of thermodynamics, and as such it is a key concept in thermodynamics. aerodynamics The study of the motion of air, particularly its interaction with a solid object, such as an airplane wing.

  4. Brightness (disambiguation) - Wikipedia

    en.wikipedia.org/wiki/Brightness_(disambiguation)

    Brightness is the polar opposite of darkness. ... Scientific. Luminosity; Brightness (sound) Brightness temperature; Surface Brightness; Artistic. The Brightness, ...

  5. Brightness - Wikipedia

    en.wikipedia.org/wiki/Brightness

    When appearing on light bulb packages, brightness means luminous flux, while in other contexts it means luminance. [5] Luminous flux is the total amount of light coming from a source, such as a lighting device. Luminance, the original meaning of brightness, is the amount of light per solid angle coming from an area, such as the sky.

  6. Temperature - Wikipedia

    en.wikipedia.org/wiki/Temperature

    On the empirical temperature scales that are not referenced to absolute zero, a negative temperature is one below the zero point of the scale used. For example, dry ice has a sublimation temperature of −78.5 °C which is equivalent to −109.3 °F. [97] On the absolute Kelvin scale this temperature is 194.6 K.

  7. Luminosity - Wikipedia

    en.wikipedia.org/wiki/Luminosity

    In addition to this brightness decrease from increased distance, there is an extra decrease of brightness due to extinction from intervening interstellar dust. [ 18 ] By measuring the width of certain absorption lines in the stellar spectrum , it is often possible to assign a certain luminosity class to a star without knowing its distance.

  8. Scientists Say Van Gogh’s Starry Night Contains Hidden Physics

    www.aol.com/lifestyle/scientists-van-gogh-starry...

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  9. Laws of thermodynamics - Wikipedia

    en.wikipedia.org/wiki/Laws_of_thermodynamics

    [5] [6] [7] These concepts of temperature and of thermal equilibrium are fundamental to thermodynamics and were clearly stated in the nineteenth century. The name 'zeroth law' was invented by Ralph H. Fowler in the 1930s, long after the first, second, and third laws were widely recognized.