Iota Canis Majoris, Latinized from ι Canis Majoris, is a solitary variable supergiant star in the southern constellation of Canis Major. It is visible...
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stars of great distance and high luminosity. At magnitude 1.5, Epsilon Canis Majoris (Adhara) is the second-brightest star of the constellation and the brightest...
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VY Canis Majoris (abbreviated to VY CMa) is an extreme oxygen-rich red hypergiant or red supergiant (O-rich RHG or RSG) and pulsating variable star 1...
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Beta Cephei variable (redirect from Beta Canis Majoris star)
Beta Cephei variables, also known as Beta Canis Majoris stars, are variable stars that exhibit small rapid variations in their brightness due to pulsations...
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galactic red supergiants and hypergiants found elsewhere such as VY Canis Majoris and with theoretical models of the coolest, most luminous and largest...
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eye examples include Polaris, Alpha Leporis, Alpha Persei, Delta Canis Majoris and Iota¹ Scorpii. Many of them are variable stars, mostly pulsating Cepheids...
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Binary star system 1.40 Regulus Quadruple star system 1.50 Epsilon Canis Majoris Binary star system 1.58 Castor Sextenary star system Brightest sextuple...
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21 confirmed and 139 candidates. The most massive confirmed exoplanet is Iota Draconis b, which masses 9.40 MJ (i.e. 9.4 times the mass of Jupiter); the...
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to that of another notable but more extreme cool hypergiant star, VY Canis Majoris, and is also known as a heavily mass-losing OH/IR supergiant. It is...
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1889 1889 Amapá Beta Canis Majoris (Mirzam) Canis Major, the Great Dog 2 1991 1992 Rondônia Gamma Canis Majoris (Muliphen) Canis Major, the Great Dog...
43 KB (3,803 words) - 18:34, 11 November 2024