K Class stars have the following characteristics.
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.
O, B, and A spectral class stars are less common than G, K, and M spectral class stars. These earlier spectral class stars are larger, hotter, and more massive, leading them to have shorter lifespans and therefore be less abundant in the galaxy.
F Class stars have the following characteristics.Temperature: 6,000 -> 7,500 KelvinColour: Yellow-white -> WhiteMass: 1.04 -> 1.4 Solar massesRadius: 1.15 -> 1.4 Solar radiusLuminosity: 1.5 -> 5 Solar luminosities.Rarity: 3% of all main sequence stars.Examples: CanopusSee related link for more information.
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.
O. This is the class of the blue/white giants.
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.
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.
Class II: yellow stars-hydrogen less strong, but evident metallic lines, such as the Sun, Arcturus and Capella. This includes the modern classes G and K as well as late class F.
O, B, and A spectral class stars are less common than G, K, and M spectral class stars. These earlier spectral class stars are larger, hotter, and more massive, leading them to have shorter lifespans and therefore be less abundant in the galaxy.
F Class stars have the following characteristics.Temperature: 6,000 -> 7,500 KelvinColour: Yellow-white -> WhiteMass: 1.04 -> 1.4 Solar massesRadius: 1.15 -> 1.4 Solar radiusLuminosity: 1.5 -> 5 Solar luminosities.Rarity: 3% of all main sequence stars.Examples: CanopusSee related link for more information.
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.
The colour.O stars ≥ 33,000 K blueB stars 10,000--33,000 K blue to blue whiteA stars 7,500--10,000 K white to blue whiteF stars 6,000--7,500 K yellowish whiteG stars 5,200--6,000 K yellowK stars 3,700--5,200 K orangeM stars ≤ 3,700 K red
TGR K class was created in 1909.
NBR K Class was created in 1903.
NER Class K was created in 1890.
WAGR K class was created in 1893.
O. This is the class of the blue/white giants.