HIP 10849
HIP 10849 is a B-type (Blue-White) star located in the constellation Perseus.
At a distance of roughly 1,019 light-years, HIP 10849 is a distant star lying deep within the Milky Way galaxy.
HIP 10849 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 10849 has an apparent magnitude of +7.19, 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 hue, which corresponds to a B-V color index of -0.063.
Physikalische Eigenschaften
| Spektralklasse | Class B — B-type (Blue-White) |
| Farbindex (B−V) | -0,063 |
Beobachtung
| Scheinbare Helligkeit | +7.19 |
| Absolute Helligkeit | -0,28 |
| Entfernung | 1,019 ly |
| Sternbild | Perseus |
Position
| Rektaszension | 2h 19,63m |
| Deklination | 52° 33,68′ |
Häufig gestellte Fragen
What type of star is HIP 10849?
HIP 10849 is a Class B — B-type (Blue-White) star.
How far is HIP 10849 from Earth?
HIP 10849 is approximately 1,019.2 light-years from Earth.
Can you see HIP 10849 with the naked eye?
With an apparent magnitude of 7.19, HIP 10849 is not visible to the naked eye.
What constellation is HIP 10849 in?
HIP 10849 is located in the constellation Perseus.