HIP 110975
HIP 110975 is a K-type (Orange) star located in the constellation Pegasus.
At a distance of roughly 1,690 light-years, HIP 110975 is a distant star lying deep within the Milky Way galaxy.
HIP 110975 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 110975 has an apparent magnitude of +7.88, 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 +1.055.
Propriedades físicas
| Classe Espectral | Class K — K-type (Orange) |
| Índice de cor (B−V) | 1,055 |
Observação
| Magnitude Aparente | +7.88 |
| Magnitude Absoluta | -0,69 |
| Distância | 1,690 ly |
| Constelação | Pegasus |
Posição
| Ascensão reta | 22h 29,06m |
| Declinação | 29° 47,73′ |
Perguntas frequentes
What type of star is HIP 110975?
HIP 110975 is a Class K — K-type (Orange) star.
How far is HIP 110975 from Earth?
HIP 110975 is approximately 1,689.9 light-years from Earth.
Can you see HIP 110975 with the naked eye?
With an apparent magnitude of 7.88, HIP 110975 is not visible to the naked eye.
What constellation is HIP 110975 in?
HIP 110975 is located in the constellation Pegasus.