HIP 112250
HIP 112250 is a K-type (Orange) star located in the constellation Pegasus.
At a distance of roughly 2,509 light-years, HIP 112250 is a distant star lying deep within the Milky Way galaxy.
HIP 112250 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 112250 has an apparent magnitude of +7.85, 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 red hue, which corresponds to a B-V color index of +1.681.
Propriedades físicas
| Classe Espectral | Class K — K-type (Orange) |
| Índice de cor (B−V) | 1,681 |
Observação
| Magnitude Aparente | +7.85 |
| Magnitude Absoluta | -1,58 |
| Distância | 2,509 ly |
| Constelação | Pegasus |
Posição
| Ascensão reta | 22h 44,15m |
| Declinação | 27° 35,84′ |
Perguntas frequentes
What type of star is HIP 112250?
HIP 112250 is a Class K — K-type (Orange) star.
How far is HIP 112250 from Earth?
HIP 112250 is approximately 2,508.9 light-years from Earth.
Can you see HIP 112250 with the naked eye?
With an apparent magnitude of 7.85, HIP 112250 is not visible to the naked eye.
What constellation is HIP 112250 in?
HIP 112250 is located in the constellation Pegasus.