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 average surface temperature of star Beta (β) can vary depending on the specific star that it refers to. Without a specific star identified, it is not possible to provide an accurate average surface temperature for star Beta.
The average temperature in a 3-star freezer is around -18 degrees Celsius (0 degrees Fahrenheit). This temperature is suitable for storing frozen foods for an extended period.
Red giants have temperatures between about 5,000 and 6,700 degrees Fahrenheit.
A very average star in terms of age, size, and temperature is often referred to as a main sequence star. These stars are stable and generate energy through nuclear fusion at their cores, resulting in a balanced state of brightness and heat. Examples include our Sun.
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 average surface temperature of star Beta (β) can vary depending on the specific star that it refers to. Without a specific star identified, it is not possible to provide an accurate average surface temperature for star Beta.
The average temperature in a 3-star freezer is around -18 degrees Celsius (0 degrees Fahrenheit). This temperature is suitable for storing frozen foods for an extended period.
Red giants have temperatures between about 5,000 and 6,700 degrees Fahrenheit.
Yes, the sun is an average-sized star in terms of its size, temperature, and luminosity compared to other stars in the universe.
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 very average star in terms of age, size, and temperature is often referred to as a main sequence star. These stars are stable and generate energy through nuclear fusion at their cores, resulting in a balanced state of brightness and heat. Examples include our Sun.
The average surface temperature of Spica, a binary star system in the constellation Virgo, is about 22,400 degrees Celsius. The primary star, Spica A, is a blue giant with a surface temperature of around 25,000 degrees Celsius.
the surface of the star.
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.
Nothing, really. The Sun is average in size, temperature, and density. Its an all around average star.