HIP 15790
HIP 15790 is a B-type (Blue-White) star located in the constellation Perseus.
At a distance of roughly 1,503 light-years, HIP 15790 is a distant star lying deep within the Milky Way galaxy.
HIP 15790 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 15790 has an apparent magnitude of +8.73, 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 white hue, which corresponds to a B-V color index of +0.353.
Physikalische Eigenschaften
| Spektralklasse | Class B — B-type (Blue-White) |
| Farbindex (B−V) | 0,353 |
Beobachtung
| Scheinbare Helligkeit | +8.73 |
| Absolute Helligkeit | 0,41 |
| Entfernung | 1,503 ly |
| Sternbild | Perseus |
Position
| Rektaszension | 3h 23,50m |
| Deklination | 52° 8,91′ |
Häufig gestellte Fragen
What type of star is HIP 15790?
HIP 15790 is a Class B — B-type (Blue-White) star.
How far is HIP 15790 from Earth?
HIP 15790 is approximately 1,503.0 light-years from Earth.
Can you see HIP 15790 with the naked eye?
With an apparent magnitude of 8.73, HIP 15790 is not visible to the naked eye.
What constellation is HIP 15790 in?
HIP 15790 is located in the constellation Perseus.