HIP 94157
HIP 94157 is a B-type (Blue-White) star.
At a distance of roughly 1,450 light-years, HIP 94157 is a distant star lying deep within the Milky Way galaxy.
HIP 94157 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
With an apparent magnitude of +5.86, HIP 94157 sits near the limit of naked-eye visibility. It can be glimpsed without optical aid under dark skies, but binoculars will make observation much easier. Observers will note its blue hue, which corresponds to a B-V color index of -0.080.
Propriétés physiques
| Classe Spectrale | B Class B — B-type (Blue-White) |
| Indice de couleur (B−V) | -0,080 |
Observation
| Magnitude Apparente | +5.86 |
| Magnitude Absolue | -2,38 |
| Distance | 1,450 ly |
Position
| Ascension droite | 19h 9,96m |
| Déclinaison | -41° 53,54′ |
Frequently Asked Questions
What type of star is HIP 94157?
HIP 94157 is a Class B — B-type (Blue-White) star.
How far is HIP 94157 from Earth?
HIP 94157 is approximately 1,449.6 light-years from Earth.
Can you see HIP 94157 with the naked eye?
With an apparent magnitude of 5.86, HIP 94157 is visible to the naked eye.