HIP 10690
HIP 10690 is a A-type (White) star located in the constellation Perseus.
Located approximately 388.7 light-years from Earth, HIP 10690 resides within the broader disk of our Milky Way galaxy.
HIP 10690 is classified as a spectral class A star (A-type (White)) on the Harvard spectral classification system.
HIP 10690 has an apparent magnitude of +7.48, 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 +0.249.
Physikalische Eigenschaften
| Spektralklasse | Class A — A-type (White) |
| Farbindex (B−V) | 0,249 |
Beobachtung
| Scheinbare Helligkeit | +7.48 |
| Absolute Helligkeit | 2,10 |
| Entfernung | 389 ly |
| Sternbild | Perseus |
Position
| Rektaszension | 2h 17,56m |
| Deklination | 58° 1,20′ |
Häufig gestellte Fragen
What type of star is HIP 10690?
HIP 10690 is a Class A — A-type (White) star.
How far is HIP 10690 from Earth?
HIP 10690 is approximately 388.7 light-years from Earth.
Can you see HIP 10690 with the naked eye?
With an apparent magnitude of 7.48, HIP 10690 is not visible to the naked eye.
What constellation is HIP 10690 in?
HIP 10690 is located in the constellation Perseus.