Summary
The solar luminosity (L☉) is a unit of radiant flux (power emitted in the form of photons) used to measure the luminosity of stars, galaxies and other celestial objects in terms of the output of the Sun.
1
The International Astronomical Union (IAU) has defined a nominal solar luminosity of 3.828 × 1026 W.
2
Luminosity is an absolute measure of radiant power, and is usually measured in terms of solar luminosities. The most luminous stars emit several million solar luminosities, while the dim brown dwarfs have luminosities a few millionths that of the Sun.
3
According to
See more results on Neeva
Summaries from the best pages on the web
Summary
The solar luminosity ( L ☉ ), is a unit of radiant flux ( power emitted in the form of photons ) conventionally used by astronomers to measure the luminosity of stars , galaxies and other celestial objects in terms of the output of the Sun
Solar luminosity - Wikipedia
wikipedia.org
Summary
The IAU has defined a nominal solar luminosity of 3.828 × 10 26 W to promote publication of consistent and comparable values in units of the solar luminosity
Luminosity - Wikipedia
wikipedia.org
Summary
Luminosity is an absolute measure of radiant power, and is usually measured in terms of solar luminosities. The most luminous stars emit several million solar luminosities, while the dim brown dwarfs have luminosities a few millionths that of the Sun. Luminosity is an important factor in astronomy, and is often measured in terms of the power of an object.
Luminosity | astronomy | Britannica
britannica.com
The Sun is the star at the center of the Solar System. It is a nearly perfect ball of hot plasma,[18][19] heated to incandescence by nuclear fusion reactions in its core. The Sun radiates this energy mainly as light, ultraviolet, and infrared radiation, and is the most important source of energy for life on Earth.
Sun - Wikipedia
wikipedia.org
How can we measure the Sun's luminosity? We can measure the intensity of sunlight at the Earth.
Luminosity of Sun
uoregon.edu
between the solar constant and the solar luminosity is determined by simple geometry. Imagine a sphere the size of the Earth's orbit surrounding the Sun. The ...
Solar Luminosity
utk.edu
This is a small fraction of the total radiated energy of 3.8 x 10 26 watts, or L sun =3.8 x 10 33 ergs/sec = 10 26 joules/sec -- the Solar luminosity , which ...
The Sun
hawaii.edu
Now let's consider the case of two stars, the Sun and Ori. We define the subscripted symbol to mean that of the Sun . Thus the Sun has a luminosity of 1 L (1 L ...
The Hertzsprung-Russell Diagram
nmsu.edu
of radiant flux conventionally used by astronomers to measure the luminosity of stars, galaxies and other celestial objects in terms of the output of the Sun.
Solar luminosity - Wikiwand
wikiwand.com
Unable to generate a short snippet for this page, sorry about that.
ucolick.org