Its story

Cih is a small, red dwarf star classified as a type M dwarf. It is part of the Cas constellation, located approximately 14 degrees north of north latitude and 60 degrees west longitude, in the southern hemisphere. This star’s magnitude is remarkably low, listed at 2.15 – appearing as a faint, almost distant star in the night sky. While not exceptionally bright, it does display a considerable activity.

The star’s recognizability in the sky stems from its positioning within the Cas constellation. The constellation’s shape, particularly its prominent grouping of relatively bright stars, naturally leads observers to recognize Cih's relatively small size. It maintains a stable, somewhat low-intensity luminosity. Without external information, we are unable to infer any specific spectral type or colour. Its orbital characteristics are relatively predictable, meaning it is highly stable and has experienced minimal changes over its observed history.

Considering its spectral classification, Cih likely exists within the faint temperature zone, meaning it primarily emits across the electromagnetic spectrum, including some ultraviolet and infrared. Its estimated distance from Earth is approximately 300-400 AU, suggesting that it is relatively close to us. A small, isolated magnitude provides a unique element of distinction – a faint, steady presence requiring prolonged observation to become noticeable.