HIP 7299
HIP 7299 is a B-type (Blue-White) star located in the constellation Andromeda.
At a distance of roughly 2,861 light-years, HIP 7299 is a distant star lying deep within the Milky Way galaxy.
HIP 7299 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 7299 has an apparent magnitude of +8.59, 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 blue hue, which corresponds to a B-V color index of -0.001.
Propriétés physiques
| Classe Spectrale | Class B — B-type (Blue-White) |
| Indice de couleur (B−V) | -0,001 |
Observation
| Magnitude Apparente | +8.59 |
| Magnitude Absolue | -1,12 |
| Distance | 2,861 ly |
| Constellation | Andromeda |
Position
| Ascension droite | 1h 34,01m |
| Déclinaison | 45° 58,59′ |
Questions fréquentes
What type of star is HIP 7299?
HIP 7299 is a Class B — B-type (Blue-White) star.
How far is HIP 7299 from Earth?
HIP 7299 is approximately 2,861.0 light-years from Earth.
Can you see HIP 7299 with the naked eye?
With an apparent magnitude of 8.59, HIP 7299 is not visible to the naked eye.
What constellation is HIP 7299 in?
HIP 7299 is located in the constellation Andromeda.