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  2. Surface brightness - Wikipedia

    en.wikipedia.org/wiki/Surface_brightness

    A truly dark sky has a surface brightness of 2 × 10 −4 cd m −2 or 21.8 mag arcsec −2. [9] [clarification needed] The peak surface brightness of the central region of the Orion Nebula is about 17 Mag/arcsec 2 (about 14 milli nits) and the outer bluish glow has a peak surface brightness of 21.3 Mag/arcsec 2 (about 0.27 millinits). [10]

  3. Tired light - Wikipedia

    en.wikipedia.org/wiki/Tired_light

    The Tolman surface brightness test rules out the tired light explanation for the cosmological redshift. By the 1990s and on into the twenty-first century, a number of falsifying observations have shown that "tired light" hypotheses are not viable explanations for cosmological redshifts. [2]

  4. Tolman surface brightness test - Wikipedia

    en.wikipedia.org/wiki/Tolman_surface_brightness_test

    The Tolman surface brightness test is one out of six cosmological tests that were conceived in the 1930s to check the viability of and compare new cosmological models. Tolman's test compares the surface brightness of galaxies as a function of their redshift (measured as z ).

  5. Sky brightness - Wikipedia

    en.wikipedia.org/wiki/Sky_brightness

    (The S 10 unit is defined as the surface brightness of a star whose V-magnitude is 10 and whose light is smeared over one square degree, or 27.78 mag arcsec −2.) The total sky brightness in zenith is therefore ~220 S 10 or 21.9 mag/arcsec² in the V-band. Note that the contributions from Airglow and Zodiacal light vary with the time of year ...

  6. Surface brightness fluctuation - Wikipedia

    en.wikipedia.org/wiki/Surface_brightness_fluctuation

    Surface brightness fluctuation (SBF) is a secondary distance indicator used to estimate distances to galaxies. It is useful to 100 Mpc ( parsec ). The method measures the variance in a galaxy's light distribution arising from fluctuations in the numbers of and luminosities of individual stars per resolution element.

  7. Brightness - Wikipedia

    en.wikipedia.org/wiki/Brightness

    Brightness is an attribute of visual perception in which a source appears to be radiating or reflecting light. [1] In other words, brightness is the perception elicited by the luminance of a visual target. The perception is not linear to luminance, and relies on the context of the viewing environment (for example, see White's illusion).

  8. AOL Mail Help - AOL Help

    help.aol.com/products/new-aol-mail

    You've Got Mail!® Millions of people around the world use AOL Mail, and there are times you'll have questions about using it or want to learn more about its features. That's why AOL Mail Help is here with articles, FAQs, tutorials, our AOL virtual chat assistant and live agent support options to get your questions answered.

  9. Talk:Surface brightness - Wikipedia

    en.wikipedia.org/wiki/Talk:Surface_brightness

    How is surface brightness any different than luminance? Seems they are not and the two articles should merged. Seems they are not and the two articles should merged. — TimL • talk 05:13, 27 January 2014 (UTC) [ reply ]