Regulus
HIP 49669; Alpha Leo; 32 Leo
Propriedades Físicas
Posição e Identificadores
Visibilidade
Defina um local nas Configurações do Usuário para ver dados de visibilidade.
Sistema Estelar Múltiplo
Vista pela Ocular
Sep: 175.9″ · PA: 308° · N cima, L esquerda
Resolvido · Rayleigh: 2.3″ · Dawes: 1.9″ · Eff: 3.1″
Comparação de Tamanho
Ciclo de vida estelar
Classificação Espectral
Diagrama Hertzsprung-Russell
Espectro de corpo negro
Espectro de absorção estelar
Espectro de absorção simulado com base no tipo espectral. Passe o mouse sobre as linhas para identificar os elementos.
Notas Estelares
Imagem de Levantamento
Carregando imagem de levantamento…
Sobre Regulus
Descrição
Regulus is the brightest star in the constellation Leo at magnitude 1.35 and the 21st brightest in the night sky. It is a blue-white main-sequence star of spectral type B7V, located about 79 light-years from Earth. Regulus is about 3.5 times the mass of the Sun and roughly 288 times more luminous. It rotates extremely rapidly — once every 15.9 hours — giving it a significantly oblate shape. Regulus is actually a quadruple star system with two widely separated pairs.
Dicas de Observação
Regulus sits at the base of the distinctive Sickle asterism in Leo, making it easy to find. It lies almost exactly on the ecliptic, so the Moon and planets frequently pass very close to it or even occult it — watching for these conjunctions is rewarding. The wide companion Regulus B/C (magnitudes 8.1 and 13.5) lies about 177 arcseconds away and is an easy target for small telescopes. Best observed from February through June.
História
Regulus means 'little king' in Latin, a name given by Copernicus. Earlier names include 'Cor Leonis' (Heart of the Lion) in Latin and 'Basiliskos' (little king) in Greek. It was one of the four Royal Stars of ancient Persia, marking the summer solstice around 3000 BC. Regulus was important in ancient astrology and was associated with royalty and power across many cultures.
Curiosidades
Regulus spins so fast that it is about 32% wider at its equator than at its poles. If it rotated just 16% faster, it would tear itself apart. Because it lies almost exactly on the ecliptic, Regulus is regularly occulted by the Moon and occasionally by planets — Venus occulted Regulus in 1959, and the next Venus occultation will occur in 2044.