HIP 54885
HIP 54885 is a B-type (Blue-White) star.
At a distance of roughly 2,381 light-years, HIP 54885 is a distant star lying deep within the Milky Way galaxy.
HIP 54885 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 54885 has an apparent magnitude of +8.51, 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 +0.183.
Physikalische Eigenschaften
| Spektralklasse | B Class B — B-type (Blue-White) |
| Farbindex (B−V) | 0,183 |
Beobachtung
| Scheinbare Helligkeit | +8.51 |
| Absolute Helligkeit | -0,81 |
| Entfernung | 2,381 ly |
Position
| Rektaszension | 11h 14,30m |
| Deklination | -65° 53,47′ |
Frequently Asked Questions
What type of star is HIP 54885?
HIP 54885 is a Class B — B-type (Blue-White) star.
How far is HIP 54885 from Earth?
HIP 54885 is approximately 2,380.7 light-years from Earth.
Can you see HIP 54885 with the naked eye?
With an apparent magnitude of 8.51, HIP 54885 is not visible to the naked eye.