The entire wiki reimagined as a visual magazine with video discovery · Watch your interests come alive
The entire wiki reimagined as a visual magazine with video discovery · Watch your interests come alive
Fluid dynamics simulations of a red supergiant, with giant convection cells and puffy surface
Fluid dynamics simulations of a red supergiant, with giant convection cells and puffy surface
Betelgeuse pulsating and showing spectral line profile changes (HST UV images)
Betelgeuse pulsating and showing spectral line profile changes (HST UV images)
Most red supergiants end their lives as a Type II supernova, such as SN2013ej at bottom left in a spiral arm of M74.
Most red supergiants end their lives as a Type II supernova, such as SN2013ej at 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.
AAVSO V-band magnitude of Betelgeuse, between September 2016 and August 2023
AAVSO V-band magnitude of Betelgeuse, between September 2016 and August 2023
Comparison of SPHERE images of Betelgeuse taken in January 2019 and December 2019, showing the changes in brightness and shape
Comparison of SPHERE images of Betelgeuse taken in January 2019 and December 2019, showing the changes in brightness and shape
Image showing Betelgeuse (top left) and the dense nebulae of the Orion molecular cloud complex (Rogelio Bernal Andreo)
Image showing Betelgeuse (top left) and the dense nebulae of the Orion molecular cloud complex (Rogelio Bernal Andreo)