HIP 56890
HIP 56890 is a B-type (Blue-White) star located in the constellation Centaurus.
HIP 56890 is an extraordinarily remote star, situated approximately 326,156 light-years from Earth.
HIP 56890 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 56890 has an apparent magnitude of +8.35, 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 +0.072.
Physical Properties
| Spectral Class | Class B — B-type (Blue-White) |
| Color Index (B−V) | 0.072 |
Observation
| Apparent Magnitude | +8.35 |
| Absolute Magnitude | -11.65 |
| Distance | 326,156 ly |
| Constellation | Centaurus |
Position
| Right Ascension | 11h 39.76m |
| Declination | -63° 28.67′ |
Frequently Asked Questions
What type of star is HIP 56890?
HIP 56890 is a Class B — B-type (Blue-White) star.
How far is HIP 56890 from Earth?
HIP 56890 is approximately 326,156.0 light-years from Earth.
Can you see HIP 56890 with the naked eye?
With an apparent magnitude of 8.35, HIP 56890 is not visible to the naked eye.
What constellation is HIP 56890 in?
HIP 56890 is located in the constellation Centaurus.