HIP 10887
HIP 10887 is a K-type (Orange) star.
At a distance of roughly 1,320 light-years, HIP 10887 is a distant star lying deep within the Milky Way galaxy.
HIP 10887 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 10887 has an apparent magnitude of +8.49, 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 orange hue, which corresponds to a B-V color index of +1.103.
Propriedades físicas
| Classe Espectral | K Class K — K-type (Orange) |
| Índice de cor (B−V) | 1,103 |
Observação
| Magnitude Aparente | +8.49 |
| Magnitude Absoluta | 0,45 |
| Distância | 1,320 ly |
Posição
| Ascensão reta | 2h 20,12m |
| Declinação | -20° 49,70′ |
Frequently Asked Questions
What type of star is HIP 10887?
HIP 10887 is a Class K — K-type (Orange) star.
How far is HIP 10887 from Earth?
HIP 10887 is approximately 1,320.5 light-years from Earth.
Can you see HIP 10887 with the naked eye?
With an apparent magnitude of 8.49, HIP 10887 is not visible to the naked eye.