HIP 9030
HIP 9030 is a M-type (Red) star.
HIP 9030 is an extraordinarily remote star, situated approximately 326,156 light-years from Earth.
HIP 9030 is classified as a spectral class M star (M-type (Red)) on the Harvard spectral classification system.
HIP 9030 has an apparent magnitude of +8.79, placing it beyond naked-eye visibility. A good pair of binoculars or a small telescope is required to observe this star. Observers will note its red hue, which corresponds to a B-V color index of +1.504.
Propriétés physiques
| Classe Spectrale | Class M — M-type (Red) |
| Indice de couleur (B−V) | 1,504 |
Observation
| Magnitude Apparente | +8.79 |
| Magnitude Absolue | -11,21 |
| Distance | 326,156 ly |
Position
| Ascension droite | 1h 56,31m |
| Déclinaison | -32° 29,12′ |
Questions fréquentes
What type of star is HIP 9030?
HIP 9030 is a Class M — M-type (Red) star.
How far is HIP 9030 from Earth?
HIP 9030 is approximately 326,156.0 light-years from Earth.
Can you see HIP 9030 with the naked eye?
With an apparent magnitude of 8.79, HIP 9030 is not visible to the naked eye.