Paradys is a relatively quiet, small, and ancient star located in the constellation Aps. Primarily a faint, relatively distant member of the Aps constellation, it represents a significant portion of the star cluster's overall luminosity. Its magnitude is
Paradys’s recognizable characteristics stem primarily from its position within the larger Aps region of the sky. While detailed stellar evolution models offer numerous possibilities, its light curve and spectral characteristics reflect a relatively long, stable history of illumination. It’s a secondary, relatively modest star, existing with a low luminosity and a long lifespan within its home sector. Notably, the star's motion through space has been meticulously tracked through observations using the Gaia spacecraft, leading to precise knowledge of its proper motion across the heavens.
Its unlikely existence would be a noteworthy event to a celestial observer seeking a simple, enduring beacon in the night's expanse. A star that has weathered and endured for most of its existence—a place that is stable despite gravitational forces and influences—could easily carry a sense of quiet contemplation, signifying a steady, peaceful presence in an infinite universe. It stands as a tangible reminder of ancient cosmic stability.
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How to see it
Paradys has a visual magnitude of about 3.36: under a reasonably dark sky it is typically reachable with the unaided eye.
Sky position
Equatorial coordinates for Paradys: right ascension 14h 47m 52s, declination −79° 2′ 41″ (J2000), in the region of the Apus constellation (IAU figure Aps).
Catalog context
Paradys. It appears in classical and modern catalogs as Bayer/Flamsteed designation Alp Aps, HIP 72370, HD 129078, Gaia DR3 5773473920382493440. In the SkyKeepsake Apus (Aps) browse hub it sits with other stars of the same IAU figure.
Catalog identifiers
- Gaia
- Gaia DR3 5773473920382493440
- HIP
- 72370
- HD
- 129078
- gaia_dr3
- 5773473920382493440
- Bayer / Flamsteed
- Alp Aps
Observed properties
- Visual magnitude
- 3.36