A red giant is a luminous giant star of low or intermediate mass (roughly 0.5-10 solar masses) that is in a late phase of stellar evolution. The outer atmosphere is inflated and tenuous, making the radius immense and the surface temperature low, somewhere from 5,000 K and lower. The appearance of the red giant is from yellow orange to red, including the spectral types K and M, but also class S stars and most carbon stars. The most common red giants are the so-called red giant branch stars (RGB stars) whose shells are still fusing hydrogen into helium, while the core is inactive helium. Another case of red giants are theasymptotic giant branch stars (AGB) that produces carbon from helium by the triple-alpha process.[1] To the AGB stars belong the carbon stars of type C-N and late C-R. Prominent bright red giants in the night sky include Aldebaran (Alpha Tauri),Arcturus (Alpha Bootis), and Gamma Crucis(Gacrux), while the even larger Antares (Alpha Scorpii) and Betelgeuse (Alpha Orionis) arered supergiants. A red giant is a luminousgiant star of low or intermediate mass (roughly 0.5-10 solar masses) that is in a late phase ofstellar evolution. The outer atmosphere is inflated and tenuous, making the radius immense and the surface temperature low, somewhere from 5,000 K and lower. The appearance of the red giant is from yellow orange to red, including the spectral types K and M, but also class S stars and most carbon stars. The most common red giants are the so-called red giant branch stars (RGB stars) whose shells are stillfusing hydrogen into helium, while the core is inactive helium. Another case of red giants are the asymptotic giant branch stars (AGB) that produces carbon from helium by the triple-alpha process.[1] To the AGB stars belong the carbon stars of type C-N and late C-R.Prominent bright red giants in the night sky includeAldebaran (Alpha Tauri), Arcturus (Alpha Bootis), and Gamma Crucis (Gacrux), while the even larger Antares (Alpha Scorpii) andBetelgeuse (Alpha Orionis) are red supergiants. A red giant is a luminous giant star of low or intermediate mass (roughly 0.5-10solar masses) that is in a late phase of stellar evolution. The outer atmosphere is inflated and tenuous, making the radius immense and the surface temperature low, somewhere from 5,000 K and lower. The appearance of the red giant is from yellow orange to red, including the spectral types K and M, but also class S stars and most carbon stars. The most common red giants are the so-called red giant branch stars (RGB stars) whose shells are stillfusing hydrogen into helium, while the core is inactive helium. Another case of red giants are the asymptotic giant branch stars (AGB) that produces carbon from helium by the triple-alpha process.[1] To the AGB stars belong the carbon stars of type C-N and late C-R.Prominent bright red giants in the night sky includeAldebaran (Alpha Tauri), Arcturus (Alpha Bootis), and Gamma Crucis (Gacrux), while the even larger Antares (Alpha Scorpii) andBetelgeuse (Alpha Orionis) are red supergiants.
The hottest stars are the blue hypergiants, the hottest and most massive star found to date is called R136a1. It is thought to be around 40,000 to 50,000 Kelvin at the surface, while the core maybe several billion degrees.
The temperature of a white star or a white dwarf is about 45,000 degrees Fahrenheit because all stars color is determined by their Fahrenheit
The temperature of the hottest stars is upto 40,000 Kelvin.
The average temperature of an average star is around 100 billion K or 100(GK)
There are many giant stars ranging from 30,000 K down to less than 3,500 K
a red star is 5,500 degrees Fahrenheit and 3,038 degrees Celsius
If you consider the sun average its about 25 million degrees F.
Red giant stars range from about 2,700 kelvins to 4,500 kelvins on average which is equivalent 4,500 to 7,640 degrees Fahrenheit
The temperature of the core of a Red Dwarf star depends on its mass and its age. Kruger 60A, for example, has a core temperature of about 9 million Kelvin.
A star's temperature is measured by how white-hot its light is, not in Fahrenheit degrees, but in Celsius degrees. Our Sun is white hot, alright, but is a bit toward the yellow side of average. Larger (and hotter) stars may be more on the blue side of average.
All stars are hot. A white star is hotter than average with e temperature of about 7,200 to 9,200 degrees Celsius.
Red giants have temperatures between about 5,000 and 6,700 degrees Fahrenheit.
the temperature of antares star is 3100 degreeC
The temperature of the star when it dies is 350 degrees celsius
Beta is not a specific star. There is a beta star in every constellation.
Stars' brightness and temperature are typically represented on a Hertzsprung-Russell (H-R) diagram. An average star like the Sun would be located on the "Main Sequence" portion of the graph, where brightness increases as temperature increases.
A star's temperature is measured by how white-hot its light is, not in Fahrenheit degrees, but in Celsius degrees. Our Sun is white hot, alright, but is a bit toward the yellow side of average. Larger (and hotter) stars may be more on the blue side of average.
the surface of the star.
All stars are hot. A white star is hotter than average with e temperature of about 7,200 to 9,200 degrees Celsius.
Red giants have temperatures between about 5,000 and 6,700 degrees Fahrenheit.
the temperature of antares star is 3100 degreeC
Nothing, really. The Sun is average in size, temperature, and density. Its an all around average star.
the temperature of..an white dwarf star is 10,000
The temperature of the star when it dies is 350 degrees celsius
the temperature of the pistol star is over 7,500 to about 10,000
the temperature of the pistol star is over 7,500 to about 10,000