HIP 7890
HIP 7890 is a A-type (White) star located in the constellation Cassiopeia.
At a distance of roughly 1,853 light-years, HIP 7890 is a distant star lying deep within the Milky Way galaxy.
HIP 7890 is classified as a spectral class A star (A-type (White)) on the Harvard spectral classification system.
HIP 7890 has an apparent magnitude of +8.89, 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 +0.270.
Propriétés physiques
| Classe Spectrale | Class A — A-type (White) |
| Indice de couleur (B−V) | 0,270 |
Observation
| Magnitude Apparente | +8.89 |
| Magnitude Absolue | 0,12 |
| Distance | 1,853 ly |
| Constellation | Cassiopeia |
Position
| Ascension droite | 1h 41,49m |
| Déclinaison | 72° 14,86′ |
Questions fréquentes
What type of star is HIP 7890?
HIP 7890 is a Class A — A-type (White) star.
How far is HIP 7890 from Earth?
HIP 7890 is approximately 1,853.2 light-years from Earth.
Can you see HIP 7890 with the naked eye?
With an apparent magnitude of 8.89, HIP 7890 is not visible to the naked eye.
What constellation is HIP 7890 in?
HIP 7890 is located in the constellation Cassiopeia.