HIP 9017
HIP 9017 is a B-type (Blue-White) star located in the constellation Perseus.
At a distance of roughly 1,117 light-years, HIP 9017 is a distant star lying deep within the Milky Way galaxy.
HIP 9017 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 9017 has an apparent magnitude of +9.81, 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 +0.180.
Physikalische Eigenschaften
| Spektralklasse | Class B — B-type (Blue-White) |
| Farbindex (B−V) | 0,180 |
Beobachtung
| Scheinbare Helligkeit | +9.81 |
| Absolute Helligkeit | 2,14 |
| Entfernung | 1,117 ly |
| Sternbild | Perseus |
Position
| Rektaszension | 1h 56,12m |
| Deklination | 56° 33,26′ |
Häufig gestellte Fragen
What type of star is HIP 9017?
HIP 9017 is a Class B — B-type (Blue-White) star.
How far is HIP 9017 from Earth?
HIP 9017 is approximately 1,117.0 light-years from Earth.
Can you see HIP 9017 with the naked eye?
With an apparent magnitude of 9.81, HIP 9017 is not visible to the naked eye.
What constellation is HIP 9017 in?
HIP 9017 is located in the constellation Perseus.