Infinite photos and videos for every Wiki article · Find something interesting to watch in seconds
History
Page
Betelgeuse pulsating and showing spectral line profile changes (HST UV images)
Betelgeuse pulsating and showing spectral line profile changes (HST UV images)
A red supergiant ends its life as a type II supernova (bottom left) in a spiral arm of M74
A red supergiant ends its life as a type II supernova (bottom left) in a spiral arm of M74
RSGC1, the first of several massive clusters found to contain multiple red supergiants.
RSGC1, the first of several massive clusters found to contain multiple red supergiants.
The Orion region showing the red supergiant Betelgeuse
The Orion region showing the red supergiant Betelgeuse
Page
The four brightest stars in NGC 4755 are blue supergiant stars, with a red supergiant star at the centre. (ESO VLT)
The four brightest stars in NGC 4755 are blue supergiant stars, with a red supergiant star at the centre. (ESO VLT)
The disc and atmosphere of Betelgeuse (ESO)
The disc and atmosphere of Betelgeuse (ESO)
RS Puppis is a supergiant and Classical Cepheid variable.
RS Puppis is a supergiant and Classical Cepheid variable.