HIP 104890
HIP 104890 is a F-type (Yellow-White) star.
Located approximately 428.0 light-years from Earth, HIP 104890 resides within the broader disk of our Milky Way galaxy.
HIP 104890 is classified as a spectral class F star (F-type (Yellow-White)) on the Harvard spectral classification system.
HIP 104890 has an apparent magnitude of +9.21, 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 +0.575.
Propriétés physiques
| Classe Spectrale | F Class F — F-type (Yellow-White) |
| Indice de couleur (B−V) | 0,575 |
Observation
| Magnitude Apparente | +9.21 |
| Magnitude Absolue | 3,62 |
| Distance | 428 ly |
Position
| Ascension droite | 21h 14,83m |
| Déclinaison | 70° 11,83′ |
Frequently Asked Questions
What type of star is HIP 104890?
HIP 104890 is a Class F — F-type (Yellow-White) star.
How far is HIP 104890 from Earth?
HIP 104890 is approximately 428.0 light-years from Earth.
Can you see HIP 104890 with the naked eye?
With an apparent magnitude of 9.21, HIP 104890 is not visible to the naked eye.