Mu Cephei is 283,000 times more luminous than the Sun, with an absolute visible magnitude of around M v = −7.6.. Properties [] Quite the same Wikipedia. Mu Cephei (μ Cep) is a red supergiant located in the constellation Cepheus.
The temperature was calculated using information from Morgans @ Uni.edu. In fact, Mu Cephei is an extremely luminous red supergiant and one of the reddest known stars of all. What we do.
The temperature was calculated using information from Morgans @ Uni.edu. La star est dans les dernières étapes de sa évolution: commencé fusionner l 'hélium en carbone, après l'arrêt de la fusion normale de hydrogène dans de l'hélium.
Coordinates: 21h 43m 30.46s, +58° 46′ 48.2″ Mu Cephei (μ Cep, μ Cephei), also known as Herschel's Garnet Star, is a red supergiant or hypergiant star in the constellation Cepheus. The star has a B-V Colour Index of 2.24 which means the star's temperature is about 465 Kelvin. Based on the star's spectral type of M2Ia , Herchel's Garnet Star's colour and type is red supergiant star. When a supergiant star has converted elements in its core to iron, the core collapses to produce a supernova and the star is destroyed, leaving behind a vast gaseous cloud and a small, dense remnant. Alcuéntrase a una incierta distancia del Sistema Solar entendida ente 2.400 y 2.800 años lluz. Mu Cephei un estel hipergegant vermell de tipus espectral M2Ia o M1I una dels estels més grans que es coneixen.
Recibe'l títulu de Estrella granate por cuenta del so intensu color coloráu, especialmente destacáu si reparar al traviés de prismáticos o telescopios pequeños.
Since 1943, the spectrum of this star has served Mu Cephei is located in … Mu Cephei is nearing death. With an average apparent magnitude of 4.08, it is the 10th brightest star in the constellation.
VV Cephei is an eclipsing binary star system located 4,900 ly from Earth in the constellation Cepheus. Mu Cephei. Mu Cephei est aussi un plusieurs étoiles, avec un compagnon de grandeur 12.3, et une amplitude plus lointaine 12,7. VV Cephei is an eclipsing binary star system located approximately 4,900 light years from Earth in the constellation Cepheus. Mu Cephei (μ Cephei / El mio Cephei / HD 206936) ye una estrella na constelación de Cefeo de magnitú aparente media +4,04. It has begun to fuse helium into carbon, whereas a main sequence star fuses hydrogen into helium. The primary star in the system, VV Cephei A, is one of the largest known stars in the Milky Way.
Every page goes through several hundred of perfecting techniques; in live mode. The Garnet Star (Mu Cephei) is a very luminous red supergiant, one of the largest and brightest stars visible not only to the naked eye but in the entire Galaxy.It lies in the constellation Cepheus and is associated with a large region of nebulosity known as IC 1396 or the Garnet Star Nebula (see below). With a radius between 1,050 and 1,900 times that of the Sun, it is one of the largest stars known. Mu Cephei (μ Cep, μ Cephei), also known as Herschel's Garnet Star, is a red hypergiant star in the constellation Cepheus.It appears garnet red, which was fired observed by William Herschel (hence the star's name). It appears garnet red and is located at the edge of the IC 1396 nebula. It may be the largest star visible to the naked eye with an estimated radius of 1.15 billion kilometres (710 million miles) or 1,650 times that of the Sun.
Herchel's Garnet Star Colour and Temperature .
Herchel's Garnet Star Colour and Temperature .
Also known as Herschel’s Garnet Star and notable for its striking red colour, Mu Cephei is a spectral standard for its class (M2). Quite the same Wikipedia. Just better. Based on the star's spectral type of M2Ia , Herchel's Garnet Star's colour and type is red supergiant star. The star has a B-V Colour Index of 2.24 which means the star's temperature is about 465 Kelvin. It has an apparent magnitude of 4.91. Just better.