It all depends on the mass of the star
1exp10*(m/l) where "m" is mass and "l" is luminosity.
Will give you an approximate period of the stars life.
The spectral class letters in astronomy represent the temperature and color of stars. The sequence starts with O (hottest and bluest stars) and ends with M (coolest and reddest stars). The spectral class letters are O, B, A, F, G, K, and M.
Spectral class Y, which is typical of "brown dwarf" stars.
Two stars of the same spectral class must have the same temperature and color. This classification system groups stars based on their temperature, with each spectral class representing a specific range of temperatures.
Spectral class is the categorization of stars by temperature and size, mostly the former. Spectral class B is very hot. In descending order (hottest to coolest) the spectral classes are O,B,A,F,G,K,M. You can see that B is very near the top.
The next sequence of letters following OBAFGKM in the spectral classification system are L, T, Y. These letters are used to classify cooler and less luminous stars outside the main sequence, such as brown dwarfs.
The spectral class letters in astronomy represent the temperature and color of stars. The sequence starts with O (hottest and bluest stars) and ends with M (coolest and reddest stars). The spectral class letters are O, B, A, F, G, K, and M.
Spectral class Y, which is typical of "brown dwarf" stars.
A star with luminosity class VI under the Yerkes Spectral Classification System. They have luminosity 1.5 to 2 magnitudes lower than main-sequence stars of the same spectral type.
Two stars of the same spectral class must have the same temperature and color. This classification system groups stars based on their temperature, with each spectral class representing a specific range of temperatures.
Spectral class is a classification system for stars based on their temperature and spectral characteristics. It categorizes stars into different groups, such as O, B, A, F, G, K, and M, with O being the hottest and M being the coolest. Spectral class is indicated by a letter, with additional subtype information denoted by a number.
B Class stars have the following characteristics.Temperature: 10,000 -> 30,000 KelvinColour: Blue -> Blue-whiteMass: 2.1 -> 16 Solar massesRadius: 1.8 -> 6.6 Solar radiusLuminosity: 25 -> 30,000 Solar luminosities.Rarity: 0.13% of all main sequence stars.Examples: RigelSee related link for more information.
If they are converting hydrogen to helium, then they are on the main sequence. This can be confirmed with a spectral analysis
The spectral sequence of stars is not alphabetical because it is based on the temperature of the star, with O-type stars being the hottest and M-type stars being the coolest. The sequence was originally arranged in this manner by Annie Jump Cannon, a pioneering astronomer, in order to classify stars based on their spectral features.
Main sequence stars that appear orange are of spectral class K that are dimmer and smaller than the Sun and have masses between 45% to 80% of the Sun's mass.
Spectral class is the categorization of stars by temperature and size, mostly the former. Spectral class B is very hot. In descending order (hottest to coolest) the spectral classes are O,B,A,F,G,K,M. You can see that B is very near the top.
The O spectral class is the highest temperature class. Stars in this class are extremely hot and blue in color, with surface temperatures exceeding 30,000 K.
Stars can be classified into different spectral types based on their color, which is related to their surface temperature. The classification system uses the letters O, B, A, F, G, K, and M to represent the range of temperatures from hottest (blue/white) to coolest (red). This sequence is known as the spectral sequence or spectral types.