Very low (virtually none) even though we use a little more power than that.
(Different design.)
Luminosity
Light intensity is also known as luminosity. Candela is the si unit
Compared to Osmium it is light, compared to Hydrogen it is heavy
different colors
its darker
its called magnitude or luminosity. :) hope it helped you.
Luminosity
The luminosity of stars varies quite a bit. Most stars (about 85-90% of them) emit less light than our Sun, while a few very massive stars emit, in extreme cases, over a million times as much light (or more precisely: total radiation) than our Sun.
luminosity? maybe?
The root word of "luminosity" is "lumin," which comes from the Latin word "lumen" meaning light.
1.Luminosity is the amount of light emitted from a certain light source whereas brightness is the amount of light manifested or received. 2.The area of illumination is inversely proportional to brightness whereas luminosity isn't. 3.Brightness is usually expressed in 'Lumens' whereas luminosity is expressed in candela per square meter (photometry).
The reference that astronomers use to compare the luminosity of other stars is the sun's luminosity. The luminosity is denoted in multiples of the sun's luminosity. For example, the luminosity of the star Sirius is 25 times the luminosity of the sun.
It varies, depending on the specific model, but an energy-saving (fluorescent) light bulb should save at least half the energy, for the same luminosity, compared to the old-fashioned incandescent light bulbs. The incandescent light bulbs ought to be outlawed, except for specific purposes where the heat they generate is actually needed.
Light intensity is also known as luminosity. Candela is the si unit
Luminosity is brightness and is a measure of how much light a star is giving out.In astronomy absolute magnitude is a measure of a celestial object's intrinsic brightness.Obviously the further away an object is the dimmer it will appear to be, so that when comparing the brightness of one star with another, all stars are moved to a theoretical distance of 10 parsecs (about 32.616 light years, or 3 × 1014 kilometres) and their brightness compared one with another.One can compute the absolute magnitude 'M' of an object given its apparent magnitude 'm' and luminosity distance 'DL':M=m-5((log 10DL)-1)where 'DL' is the star's luminosity distance in parsecs, wherein 1 parsec is approximately 3.2616 light-years.
The brightness of the pixel within the image on a scale of 0 to 255
Light rays are visible and have higher frequency compared to that of heat radiation Heat radiation is nothing but infra red which is not visible to human eyes. They have longer wavelength compared to that of visible light