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In astronomy, values for luminosity are often given in the terms of the luminosity of the Sun, L ⊙. Luminosity can also be given in terms of the astronomical magnitude system: the absolute bolometric magnitude ( M bol ) of an object is a logarithmic measure of its total energy emission rate, while absolute magnitude is a logarithmic measure ...
As an example, if one uses a lens to form an image that is smaller than the source object, the luminous power is concentrated into a smaller area, meaning that the illuminance is higher at the image. The light at the image plane, however, fills a larger solid angle so the luminance comes out to be the same assuming there is no loss at the lens.
This is a compilation of symbols commonly used in astronomy, particularly professional astronomy. Age (stellar) τ - age; ... M o - Mean anomaly at epoch;
This glossary of astronomy is a list of definitions of terms and concepts relevant to astronomy and cosmology, their sub-disciplines, and related fields. Astronomy is concerned with the study of celestial objects and phenomena that originate outside the atmosphere of Earth. The field of astronomy features an extensive vocabulary and a ...
Several measures of light are commonly known as intensity: . Radiant intensity, a radiometric quantity measured in watts per steradian (W/sr); Luminous intensity, a photometric quantity measured in lumens per steradian (lm/sr), or candela (cd)
In photometry, luminous energy is the perceived energy of light.This is sometimes called the quantity of light. [1] Luminous energy is not the same as radiant energy, the corresponding objective physical quantity.
The Association of Lunar and Planetary Observers reports that you can expect it to be around 14.6 arcseconds in size and shine at a magnitude of -1.4, meaning it will outshine every star. (In ...
For planets and asteroids, a definition of absolute magnitude that is more meaningful for non-stellar objects is used. The absolute magnitude, commonly called H {\displaystyle H} , is defined as the apparent magnitude that the object would have if it were one astronomical unit (AU) from both the Sun and the observer, and in conditions of ideal ...