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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 1.2 kiloparsecs (3,900 light-years) from the Solar System in the slightly southern constellation of Canis Major.
English: Size comparison of evolved red supergiant star Stephenson 2-18, extreme red hypergiant star VY Canis Majoris and luminous red supergiant star UY Scuti. Bahasa Indonesia: Perbandingan ukuran bintang super raksasa merah berevolusi Stephenson 2-18, bintang hypergiant merah ekstrim VY Canis Majoris dan bintang super raksasa merah bercahaya ...
The following 15 pages use this file: Hypergiant; VY Canis Majoris; Talk:Westerlund 1 W26; User:FT2/scc images; User:Jarhed21; User:Mysid/vectors; User:Nussun05/List of largest stars
VY Canis Majoris: 1,420 ± 120 [11] [12] [13] AD An extreme oxygen-rich red hypergiant that has experienced two dimming periods in the 20th century where the star became dimmer by up to 2.5 magnitudes. [14] Potentially the largest known star. [12] There is a possilbility that this size might be a bit overestimated (on the order of 1 sigma).
Very Large Telescope image of the surroundings of VY Canis Majoris. Canis Major is also home to many variable stars. EZ Canis Majoris is a Wolf–Rayet star of spectral type WN4 that varies between magnitudes 6.71 and 6.95 over a period of 3.766 days; the cause of its variability is unknown but thought to be related to its stellar wind and ...
Very Large Telescope image of the surroundings of the red hypergiant VY Canis Majoris. An OH/IR star is an asymptotic giant branch (AGB) or a red supergiant or hypergiant (RSG or RHG) star that shows strong OH maser emission and is unusually bright at near-infrared wavelengths.
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Articles this image appears in VY Canis Majoris Creator User:WindAzure (png) User:Mysid (svg) Support as nominator froth t 01:49, 26 August 2007 (UTC) Oppose Wow, I didn't imagine there could exist stars that large: the stats are truly staggering.