The basic luminosity classes are: I for supergiants, III for giants, and V for main-sequence stars.
There are trillions of them. You need to be more specific.
Blue Supergiants and Supergiants
Me
Red Supergiants tend to live about half a million years.(:
The basic luminosity classes are: I for supergiants, III for giants, and V for main-sequence stars.
Supergiants are the most massive stars, occupy the top region of Hertzsprung-russell diagram . Supergiants can have 10 to 70 solar masses and luminosity up to hundreds of thousands times the solar luminosity and because of their large masses they have lifespan of few million years and may be less than this value .
There are trillions of them. You need to be more specific.
Blue Supergiants and Supergiants
Supergiants are found throughout the galaxy.
The plural of dwarf is "dwarves". White dwarves are hotter than supergiants. White dwarves also have much less luminosity. This is related to their very small surface area. Since white dwarves no longer produce energy, they will cool down over time - but this takes quite a while.
Me
Red Supergiants tend to live about half a million years.(:
I was enthralled by the luminosity of the deep water jellyfish.
Supergiants can have masses from 10 to 70 times the size of our Sun. They vary greatly in radii, usually from 30 to 500, or even in excess of 1,000 times our Sun. See Link - Supergiants are located in box 5 . Stars in Box 6 are generally referred to as Hypergiants.
Betelgeuse has a spectral type of M2lab signifying that it is a red class M star. the "lab" refers to it being an intermediate luminous supergiant. It has a luminosity of 140,000L. Referring to the H-R diagram [See related link] we can see that an M class star with a luminosity of 140,000 will appear in the very top right corner - above la supergiants.
A star's luminosity is measured according to the relevance to the sun. Basically for example, if a star is 8,300 degrees Celsius and has a luminosity of 0.001; the luminosity is compared to the sun.