The supergiant star Betelgeuse, the bright red star in Orion’s shoulder, is surrounded by an envelope of nearby material which is probably matter that it shed as it evolved into a supergiant. The arcs to the left in this image taken by the Herschel Space Observatory are material ejected from the star as it evolved into a red supergiant, and are shaped by its bow shock interaction as it move through the interstellar medium. The faint linear bar of dust on the left may represent a dusty filament connected to the local galactic magnetic field or the edge of an interstellar cloud. If so, then Betelgeuse’s motion across the sky implies that the arcs will hit the wall in 5,000 years time, and the star itself will smack into the wall 12,500 years later.
Image Credit: ESA