HIP 10751
HIP 10751 is a F-type (Yellow-White) star located in the constellation Perseus.
Located approximately 356.1 light-years from Earth, HIP 10751 resides within the broader disk of our Milky Way galaxy.
HIP 10751 is classified as a spectral class F star (F-type (Yellow-White)) on the Harvard spectral classification system.
HIP 10751 has an apparent magnitude of +8.57, 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 +0.450.
Physikalische Eigenschaften
| Spektralklasse | Class F — F-type (Yellow-White) |
| Farbindex (B−V) | 0,450 |
Beobachtung
| Scheinbare Helligkeit | +8.57 |
| Absolute Helligkeit | 3,38 |
| Entfernung | 356 ly |
| Sternbild | Perseus |
Position
| Rektaszension | 2h 18,31m |
| Deklination | 57° 48,95′ |
Häufig gestellte Fragen
What type of star is HIP 10751?
HIP 10751 is a Class F — F-type (Yellow-White) star.
How far is HIP 10751 from Earth?
HIP 10751 is approximately 356.1 light-years from Earth.
Can you see HIP 10751 with the naked eye?
With an apparent magnitude of 8.57, HIP 10751 is not visible to the naked eye.
What constellation is HIP 10751 in?
HIP 10751 is located in the constellation Perseus.