Acrolis's sun

Acrolis's sun was an unnamed K-type T Tauri flare star that sat in the Outer Rim's Hook Nebula and served as the primary star of the Acrolis system, a sparse and isolated star system situated in the star cluster of the same name.

Description
Acrolis's sun was a young red-orange K-type T Tauri flare star with an age estimated to be between one hundred thousand and one million standard years as of the Battle of Yavin. A young star that had not yet entered the main sequence, Mure's sun was primarily powered by the release of gravitational energy rather than by hydrogen fusion. As a result, the star commonly exhibited variable and unpredictable behavior, emitting high levels of X-ray and radio radiation and generating intense stellar winds that ballooned outwards from its outer atmosphere for dozens of astronomical units.

On account of its presence in a young star cluster buried deep within the fertile molecular cloud of the Hook Nebula, Acrolian astronomers believed the star had once possessed a protoplanetary disk rife with both dense metals like gold, cobalt, tungsten, platinum, and iron and lighter elements like carbon, oxygen, phosphorus, and hydrogen. The contents of this disk were believed to have been used by the prehistoric Celestial civilization in their artificial construction of the Acrolis system, one of seventeen documented Celestial star systems, and the planet Acrolis, the star's sole planetary-mass satellite.

Behind the scenes
As the author was unable to develop a satisfactory proper name for the star in question, the article's title was given simply as "Acrolis's sun" per Wookieepedia's naming conventions for nameless stars. The star's astrophysical properties were derived and simplified from those of Toliman, a K-type main-sequence star and the smaller of the two main sequence stars that make up the Alpha Centauri binary.