Kegåsis

== Overview ==
Kegåsis (Pronounced [KEH-gah-SISS]) is a red hypergiant star around 287.6 lightyears from the Starrial System and 297.5 lightyears from the Verda System. It has no planets, only a large dust cloud and a pseudo-nebula.
== Characteristics ==
Kegåsis is a very big star for its mass, and so its core doesn't do a very good job at holding the outer layers of the star in place, so it looks like it is bubbling. Large pieces of gas periodically rise to the chromosphere of Kegåsis, cool off and blacken, before sinking down towards the center of the star. This is normal.
Kegåsis originally formed in the Kerillis Nebula. It began its life on the very edge of the nebula when a 140-solar-mass piece broke off the cloud of gas and dust and went its own way, away from the nebula. The Itsarnoan Supernova triggered the collapsing of the globule, which was proto-Kegåsis. Nuclear reactions inside the core of Kegåsis started when it was already ~25 lightyears from the Kerillis Nebula.
== Companions ==
Kegåsis has no planets. It just has a large cloud of dust and a torus of dust orbiting it, just like the red supergiant in the LMC , known as WOH G64. It also has 14 solar masses worth of gas and dust around it, analogous to a nebula. This cloud of gas is known as the Éyeni Nebula and is already a few lightyears wide.
Category:Stars
Category:Trolligi112477-ww
Category:Star Systems
Category:Kerillis Nebula