A supergiant is much larger than a white dwarf.
A supergiant can be 10 to 70 times the size of our Sun, whereas a white dwarf is only about the size of the Earth.
There are a lot of these. They are mainly the "Red Giant" and "Red Supergiant" stars.
That is a difference of ten magitudes so the factor in brightness is 10,000.
The magnitude of a white dwarf can vary significantly, typically ranging from about 10 to 15 in absolute magnitude. This variation depends on factors such as its mass, temperature, and composition. For example, hotter and more massive white dwarfs tend to have lower absolute magnitudes, making them appear brighter. However, their apparent magnitude can differ based on their distance from Earth.
No Rigel is a huge, blue supergiant of spectral class B8 Ia, Rigel has an intrinsic brightness about 40,000 times as luminous as that of the sun.
2.65. It has a white dwarf companion of about 13
it is a dwarf planet the size of a supergiant.
There are a lot of these. They are mainly the "Red Giant" and "Red Supergiant" stars.
That is a difference of ten magitudes so the factor in brightness is 10,000.
No, Betelgeuse is not a dwarf planet. Betelgeuse is a supergiant star located in the constellation of Orion. It is one of the largest and most luminous stars known in our galaxy.
Depends on the white dwarf in question. They can have a myriad of absolute magnitude values.
Red giants have typical absolute magnitudes which are 10-15 magnitudes below white dwarfs, which means that the red giants are 10,000-1,000,000 times brighter, after due allowance for distance.
Because they are closer or actually brighter.
The magnitude of a white dwarf can vary significantly, typically ranging from about 10 to 15 in absolute magnitude. This variation depends on factors such as its mass, temperature, and composition. For example, hotter and more massive white dwarfs tend to have lower absolute magnitudes, making them appear brighter. However, their apparent magnitude can differ based on their distance from Earth.
No Rigel is a huge, blue supergiant of spectral class B8 Ia, Rigel has an intrinsic brightness about 40,000 times as luminous as that of the sun.
A star on "main sequence" is a period in a stars evolution.A white dwarf is a stellar remainA supergiant star is the size of a very big star.So they are completely different and not even related.
dwarf stars -Sydney-
when Dwarf Stars run out of hydrogen they form Red Giant stars, then from that they become White dwarf stars when the outer layers shed, forming a planetary nebula.when giant stars or supergiant stars run out of hydrogen they form red supergiant stars