HIP 101909
HIP 101909 is a B-type (Blue-White) star.
At a distance of roughly 1,348 light-years, HIP 101909 is a distant star lying deep within the Milky Way galaxy.
HIP 101909 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
With an apparent magnitude of +5.99, HIP 101909 sits near the limit of naked-eye visibility. It can be glimpsed without optical aid under dark skies, but binoculars will make observation much easier. Observers will note its blue hue, which corresponds to a B-V color index of -0.145.
Propriétés physiques
| Classe Spectrale | Class B — B-type (Blue-White) |
| Indice de couleur (B−V) | -0,145 |
Observation
| Magnitude Apparente | +5.99 |
| Magnitude Absolue | -2,09 |
| Distance | 1,348 ly |
Position
| Ascension droite | 20h 39,08m |
| Déclinaison | 15° 50,29′ |
Questions fréquentes
What type of star is HIP 101909?
HIP 101909 is a Class B — B-type (Blue-White) star.
How far is HIP 101909 from Earth?
HIP 101909 is approximately 1,347.8 light-years from Earth.
Can you see HIP 101909 with the naked eye?
With an apparent magnitude of 5.99, HIP 101909 is visible to the naked eye.