HIP 10211
HIP 10211 is a A-type (White) star located in the constellation Cassiopeia.
At a distance of roughly 1,400 light-years, HIP 10211 is a distant star lying deep within the Milky Way galaxy.
HIP 10211 is classified as a spectral class A star (A-type (White)) on the Harvard spectral classification system.
HIP 10211 has an apparent magnitude of +8.83, 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 +0.174.
Propriétés physiques
| Classe Spectrale | Class A — A-type (White) |
| Indice de couleur (B−V) | 0,174 |
Observation
| Magnitude Apparente | +8.83 |
| Magnitude Absolue | 0,67 |
| Distance | 1,400 ly |
| Constellation | Cassiopeia |
Position
| Ascension droite | 2h 11,34m |
| Déclinaison | 64° 8,75′ |
Questions fréquentes
What type of star is HIP 10211?
HIP 10211 is a Class A — A-type (White) star.
How far is HIP 10211 from Earth?
HIP 10211 is approximately 1,399.8 light-years from Earth.
Can you see HIP 10211 with the naked eye?
With an apparent magnitude of 8.83, HIP 10211 is not visible to the naked eye.
What constellation is HIP 10211 in?
HIP 10211 is located in the constellation Cassiopeia.