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.
Antares
Antares between τ (lower left) and σ Scorpii; Antares appears white in this WISE false-colour infrared image.
Antares between τ (lower left) and σ Scorpii; Antares appears white in this WISE false-colour infrared image.
Antares near the Sun on 30 November 2012
Antares near the Sun on 30 November 2012
VLTI reconstructed view of the surface of Antares A
VLTI reconstructed view of the surface of Antares A
Antares seen from the ground. The very bright star towards the upper left corner of the frame is Antares.
Antares seen from the ground. The very bright star towards the upper left corner of the frame is Antares.