La Superba is a remarkable star located within the constellation CVn, a smaller and dimmer constellation compared to many others. This star is designated as Magnitude 3.958 and is estimated to be approximately 1012 light-years away from Earth. Its visual
The star’s unique position within the CVn constellation is largely attributable to its relatively modest visual brightness, suggesting it’s situated in a particular segment of the galactic field. Historically, observations have revealed La Superba forms part of a more diffuse cluster of stars. The relatively low distance, compared to some bright, expanding stars, suggests it's been relatively undisturbed over astronomical timescales.
Because of its low prominence and stable light curve, La Superba may symbolize a steadfast point of existence, a distant reference point or a quiet observer within the vastness of space. This stability and longevity—reflecting within an ancient system—might inspire someone to see themselves as a part of something enduring, a beacon within the cosmos.
How to see it
La Superba has a visual magnitude of about 3.96: under a reasonably dark sky it is typically reachable with the unaided eye.
Sky position
Equatorial coordinates for La Superba: right ascension 12h 45m 8s, declination +45° 26′ 25″ (J2000), on the celestial sphere.
Catalog context
La Superba. It appears in classical and modern catalogs as HIP 62223, HD 110914, Gaia DR3 1542553623374596352.
Catalog identifiers
- Gaia
- Gaia DR3 1542553623374596352
- HIP
- 62223
- HD
- 110914
- gaia_dr3
- 1542553623374596352
Also known as
- Gaia DR3 TOP 5M 1542553623374596352
- HD 110914
- HIP 62223
Observed properties
- Visual magnitude
- 3.96