Red Supergiants tend to live about half a million years.(:
The surface temperature of white dwarf stars is generally higher than that of red supergiants. White dwarfs typically have temperatures ranging from about 5,000 to 100,000 Kelvin, while red supergiants usually have surface temperatures between 3,000 and 4,500 Kelvin. This significant difference is due to the evolutionary stages these stars occupy, with white dwarfs being the remnants of stars that have exhausted their nuclear fuel, while red supergiants are in a later phase of stellar evolution.
Not exactly. Red giants become white dwarf stars. It is the red supergiants that can become supernovas.
No, red supergiants are cooler than the Sun. Despite their larger size, red supergiants have lower surface temperatures due to their increased surface area, resulting in a more reddish hue compared to the Sun's yellow color.
No. Only massive stars can become supergiants.
Red supergiants can be extremely large, with radii ranging from 200 to 1,500 times that of the Sun. This makes them some of the largest known stars in the universe.
Red supergiants
Red giants, red supergiants.
The stars that are like supergiants are called "red giants" or "red supergiants".
No, the largest star known is a Red Hypergiant (vy canis majoris) which are much larger than supergiants. Most of the largest stars are red hypergiants followed by red supergiants.
Both are red supergiants.
Supergiants are bigger and more luminous than the red giants. Supergiants are stars that have a mass that is eight times more than the sun.
The five largest known red supergiants in the Galaxy are VY Canis Majoris, VV Cephei A, V354 Cephei, RW Cephei and KW Sagittarii.
blue and red supergiant temparutes are 10000000000000 degrees celsius
Red giants, red supergiants and red hypergiants.
White Dwarfs, Supergiants, and Red Giants are stars that are found in the sky.
The surface temperature of white dwarf stars is generally higher than that of red supergiants. White dwarfs typically have temperatures ranging from about 5,000 to 100,000 Kelvin, while red supergiants usually have surface temperatures between 3,000 and 4,500 Kelvin. This significant difference is due to the evolutionary stages these stars occupy, with white dwarfs being the remnants of stars that have exhausted their nuclear fuel, while red supergiants are in a later phase of stellar evolution.
Fusion continues in red supergiants because their cores are able to fuse heavier elements such as helium into even heavier elements like carbon, neon, and oxygen. The high temperatures and pressures in the core allow nuclear fusion reactions to continue, powering the star and maintaining its equilibrium.