In the field of stellar evolution, a blue loop is a stage in the life of an evolved star where it changes from a cool star to a hotter one before cooling again. The name derives from the shape of the evolutionary track on a Hertzsprung–Russell diagram which forms a loop towards the blue side of the diagram, to a place called the blue giant branch.
Stellar evolutionary tracks, some showing blue loops in the more massive red giants
Red supergiants (RSGs) are stars with a supergiant luminosity class and a stellar classification K or M. They are the largest stars in the universe in terms of volume, although they are not the most massive or luminous. Betelgeuse and Antares A are the brightest and best known red supergiants (RSGs), indeed the only first magnitude red supergiant stars.
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
RSGC1, the first of several massive clusters found to contain multiple red supergiants.
The Orion region showing the red supergiant Betelgeuse