Its story

Citalá is a relatively quiet star nestled within the constellation Mon, a minor constellation barely distinguishable from its surrounding stars. Classified as a K1-V2 dwarf elliptical star, its magnitude is easily recognizable as approximately 6.163. Located a distance of 97.58 light years from Earth, Citalá orbits the center of the Milky Way, presenting a visible presence within that vast galaxy.

Its recognizable nature stems primarily from Sirius, which was famously known for its brilliant visibility within the night sky. Citalá and Sirius share the characteristic brightness of a star relatively close to us in the cosmos. The star’s relatively shallow, circular shape and its relatively low luminosity, and the light it emits, are consistent with classifying it as a type of brown dwarf star.

This unassuming star has been identified as a relatively stable object. It has not exhibited substantial spectral changes observed in photometric data, which tends to indicate a lack of activity like pulsing or variability, and its motion within the galactic bulge is relatively stable – it moves with a consistent period of approximately 33.43 mas/yr. Despite its seemingly unremarkable qualities, this star has retained a significant positional characteristic for its age, suggesting an exceptionally slow rotation within the galactic context, and consequently offers a stable point for ongoing study, minimizing random fluctuations in apparent position.