Its story
The recognition of Nenque is largely tied to its unique position within the Phe constellation’s arc, a region known for its relatively high density of stars. Its visible properties, combined with its distance of 137.8 light-year from Earth, suggest it is a relatively modest star, contributing to its subtle presence amongst the many other stars visible to the naked eye. Observations suggest it is a relatively fast radial velocity, but within this small stellar system it has been observed through numerous spectral analysis techniques.
Considering its spectral properties, individuals observing from the southern hemisphere might readily identify Nenque. The star's characteristic spectral type is relatively unobtrusive, and its luminosity is sufficient to easily appear, particularly with modest viewing conditions. The position within Phe has allowed for relatively easy documentation with instruments that track these objects.
In essence, the star Nenque’s remarkable visibility and location within a defined galactic region, marked primarily by its spectral properties, renders it a fascinating and easily recognizable celestial body for those dedicated to astronomical observation - or those in the southern hemisphere.”
- Right ascension
- 1h 04m 40s
- Declination
- −39° 29′ 26″
- Magnitude
- 7.57
- Distance
- ≈ 138 ly