HIP 9890
HIP 9890 is a B-type (Blue-White) star located in the constellation Perseus.
Located approximately 698.4 light-years from Earth, HIP 9890 resides within the broader disk of our Milky Way galaxy.
HIP 9890 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 9890 has an apparent magnitude of +8.69, 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 +0.116.
Physikalische Eigenschaften
| Spektralklasse | Class B — B-type (Blue-White) |
| Farbindex (B−V) | 0,116 |
Beobachtung
| Scheinbare Helligkeit | +8.69 |
| Absolute Helligkeit | 2,04 |
| Entfernung | 698 ly |
| Sternbild | Perseus |
Position
| Rektaszension | 2h 7,25m |
| Deklination | 48° 6,04′ |
Häufig gestellte Fragen
What type of star is HIP 9890?
HIP 9890 is a Class B — B-type (Blue-White) star.
How far is HIP 9890 from Earth?
HIP 9890 is approximately 698.4 light-years from Earth.
Can you see HIP 9890 with the naked eye?
With an apparent magnitude of 8.69, HIP 9890 is not visible to the naked eye.
What constellation is HIP 9890 in?
HIP 9890 is located in the constellation Perseus.