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
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.
G299 Remnants Super Nova Type 1a 20150218
G299 Remnants Super Nova Type 1a 20150218
Rigel
Orion, with Rigel at bottom right, at optical wavelengths plus the Hα (hydrogen-alpha) spectral line to emphasize gas clouds
Orion, with Rigel at bottom right, at optical wavelengths plus the Hα (hydrogen-alpha) spectral line to emphasize gas clouds
Rigel A and Rigel B as they appear in a small telescope
Rigel A and Rigel B as they appear in a small telescope
Rigel and reflection nebula IC 2118 in Eridanus. Rigel B is not visible in the glare of the main star.
Rigel and reflection nebula IC 2118 in Eridanus. Rigel B is not visible in the glare of the main star.
Orion illustrated in a copy of Abd al-Rahman al-Sufi's Book of Fixed Stars. The foot on the left is annotated rijl al-jauza al-yusra, the Arabic name
Orion illustrated in a copy of Abd al-Rahman al-Sufi's Book of Fixed Stars. The foot on the left is annotated rijl al-jauza al-yusra, the Arabic name from which Rigel is derived.