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  2. Period-luminosity relation - Wikipedia

    en.wikipedia.org/wiki/Period-luminosity_relation

    The best-known relation is the direct proportionality law holding for Classical Cepheid variables, sometimes called the Leavitt Law. [ 2 ] [ 3 ] [ 4 ] Discovered in 1908 by Henrietta Swan Leavitt , the relation established Cepheids as foundational indicators of cosmic benchmarks for scaling galactic and extragalactic distances .

  3. Luminosity - Wikipedia

    en.wikipedia.org/wiki/Luminosity

    The apparent magnitude is the observed visible brightness from Earth which depends on the distance of the object. The absolute magnitude is the apparent magnitude at a distance of 10 pc (3.1 × 10 17 m), therefore the bolometric absolute magnitude is a logarithmic measure of the bolometric luminosity.

  4. HSL and HSV - Wikipedia

    en.wikipedia.org/wiki/HSL_and_HSV

    Fig. 1. HSL (a–d) and HSV (e–h). Above (a, e): cut-away 3D models of each. Below: two-dimensional plots showing two of a model's three parameters at once, holding the other constant: cylindrical shells (b, f) of constant saturation, in this case the outside surface of each cylinder; horizontal cross-sections (c, g) of constant HSL lightness or HSV value, in this case the slices halfway ...

  5. Apparent magnitude - Wikipedia

    en.wikipedia.org/wiki/Apparent_magnitude

    A difference of 1.0 in magnitude corresponds to the brightness ratio of , or about 2.512. For example, a magnitude 2.0 star is 2.512 times as bright as a magnitude 3.0 star, 6.31 times as magnitude 4.0, and 100 times magnitude 7.0.

  6. Cosmic distance ladder - Wikipedia

    en.wikipedia.org/wiki/Cosmic_distance_ladder

    The apparent magnitude, the magnitude as seen by the observer (an instrument called a bolometer is used), can be measured and used with the absolute magnitude to calculate the distance d to the object in parsecs [14] as follows: ⁡ = + or = (+) / where m is the apparent magnitude, and M the absolute magnitude. For this to be accurate, both ...

  7. Brightness - Wikipedia

    en.wikipedia.org/wiki/Brightness

    Two pictograms resembling the Sun with rays are used to represent the settings of luminance in display devices. They have been encoded in Unicode since version 6.0 (October 2010) in the Miscellaneous Symbols and Pictographs block under U+1505 as "low brightness symbol" (🔅) and U+1F506 as "high brightness symbol" (🔆).

  8. Current ratio: What it is and how to calculate it - AOL

    www.aol.com/finance/current-ratio-calculate...

    Intel (INTC) at year-end 2023 had $43.27 billion in current assets and $28.05 billion in current liabilities, for a high 1.54 current ratio. What is a good current ratio? The ideal current ratio ...

  9. Variable star - Wikipedia

    en.wikipedia.org/wiki/Variable_star

    Semiregular variables may show a definite period on occasion, but more often show less well-defined variations that can sometimes be resolved into multiple periods. A well-known example of a semiregular variable is Betelgeuse, which varies from about magnitudes +0.2 to +1.2 (a factor 2.5 change in luminosity). At least some of the semi-regular ...