HIP 15890
HIP 15890 is a M-type (Red) star.
At a distance of roughly 2,051 light-years, HIP 15890 is a distant star lying deep within the Milky Way galaxy.
HIP 15890 is classified as a spectral class M star (M-type (Red)) on the Harvard spectral classification system.
With an apparent magnitude of +5.13, HIP 15890 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 red hue, which corresponds to a B-V color index of +2.038.
Propriétés physiques
| Classe Spectrale | Class M — M-type (Red) |
| Indice de couleur (B−V) | 2,038 |
Observation
| Magnitude Apparente | +5.13 |
| Magnitude Absolue | -3,86 |
| Distance | 2,051 ly |
Position
| Ascension droite | 3h 24,68m |
| Déclinaison | 64° 35,16′ |
Questions fréquentes
What type of star is HIP 15890?
HIP 15890 is a Class M — M-type (Red) star.
How far is HIP 15890 from Earth?
HIP 15890 is approximately 2,051.3 light-years from Earth.
Can you see HIP 15890 with the naked eye?
With an apparent magnitude of 5.13, HIP 15890 is visible to the naked eye.