(astronomy) the magnitude that a star would have if it were viewed from a distance of 10 parsecs (32.62 light years) from the earth
The intrinsic luminosity,x that a celestial body would have if viewed from a distance of 10 parsecs.
Absolute magnitude is the measure of a celestial object's intrinsic brightness. It is the apparent magnitude an object would have if it were at a standard luminosity distance away from the observer, in the absence of astronomical extinction. It allows the true brightnesses of objects to be compared without regard to distance. Bolometric magnitude is luminosity expressed in magnitude units; it takes into account energy radiated at all wavelengths, whether observed or not. The absolute magnitude uses the same convention as the visual magnitude: a factor of 100.4 ratio of brightness corresponds to a difference of 1.0 in magnitude. The Milky Way, for example, has an absolute magnitude of about −20.5. So a quasar at an absolute magnitude of −25.5 is 100 times brighter than our galaxy. If this particular quasar and our galaxy could be seen side by side at the same distance, the quasar would be 5 magnitudes brighter than our galaxy.
The numerical value of absolute magnitude in Chaldean Numerology is: 1
The numerical value of absolute magnitude in Pythagorean Numerology is: 9
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"absolute magnitude." Definitions.net. STANDS4 LLC, 2017. Web. 23 May 2017. <http://www.definitions.net/definition/absolute magnitude>.