HIP 106890
HIP 106890 is a B-type (Blue-White) star.
At a distance of roughly 2,568 light-years, HIP 106890 is a distant star lying deep within the Milky Way galaxy.
HIP 106890 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 106890 has an apparent magnitude of +8.10, 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 +0.240.
Propriedades físicas
| Classe Espectral | Class B — B-type (Blue-White) |
| Índice de cor (B−V) | 0,240 |
Observação
| Magnitude Aparente | +8.10 |
| Magnitude Absoluta | -1,38 |
| Distância | 2,568 ly |
Posição
| Ascensão reta | 21h 38,98m |
| Declinação | 57° 29,24′ |
Perguntas frequentes
What type of star is HIP 106890?
HIP 106890 is a Class B — B-type (Blue-White) star.
How far is HIP 106890 from Earth?
HIP 106890 is approximately 2,568.2 light-years from Earth.
Can you see HIP 106890 with the naked eye?
With an apparent magnitude of 8.10, HIP 106890 is not visible to the naked eye.