HIP 9048
HIP 9048 is a B-type (Blue-White) star located in the constellation Perseus.
At a distance of roughly 1,941 light-years, HIP 9048 is a distant star lying deep within the Milky Way galaxy.
HIP 9048 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 9048 has an apparent magnitude of +9.46, 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-white hue, which corresponds to a B-V color index of +0.078.
Physical Properties
| Spectral Class | Class B — B-type (Blue-White) |
| Color Index (B−V) | 0.078 |
Observation
| Apparent Magnitude | +9.46 |
| Absolute Magnitude | 0.59 |
| Distance | 1,941 ly |
| Constellation | Perseus |
Position
| Right Ascension | 1h 56.56m |
| Declination | 56° 59.51′ |
Frequently Asked Questions
What type of star is HIP 9048?
HIP 9048 is a Class B — B-type (Blue-White) star.
How far is HIP 9048 from Earth?
HIP 9048 is approximately 1,941.4 light-years from Earth.
Can you see HIP 9048 with the naked eye?
With an apparent magnitude of 9.46, HIP 9048 is not visible to the naked eye.
What constellation is HIP 9048 in?
HIP 9048 is located in the constellation Perseus.