A solar luminosity is equal to the current luminosity of the Sun, which is 3.839 × 1026 W, or 3.839 × 1033 erg/s.So dividing one solar luminosity with the Suns luminosity gives 1.Also it is a lot easier talking about a luminosity of 1 rather than 3.838 x 1026 W, the same way astronomers use 1 AU to mean 150,000,000km.
The Sun's luminosity is 3.846 × 10 ^26 Watts.
V
Morgan and Keenan
Depends entirely on the class and luminosity of the oddball.
Depends entirely on the class and luminosity of the oddball.
Based on what? Luminosity, distance or spectral class?
Depends entirely on the class and luminosity of the oddball.
Depends entirely on the class and luminosity of the oddball.
If you are referring to the Yerkes spectral classification, a Class IV star is known as a subgiant.
There are millions of stars that fit that description. On the Main Sequence a star needs a spectrum of type A to be around 9000 degrees, and 1 to 20 times the luminosity of the Sun means an absolute magnitude in the range 1.2 to 4.7. For example Sirius.
Simply, because they are the hottest and thus the most luminous.