HIP 114250
HIP 114250 is a K-type (Orange) star located in the constellation Pegasus.
At a distance of roughly 1,337 light-years, HIP 114250 is a distant star lying deep within the Milky Way galaxy.
HIP 114250 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 114250 has an apparent magnitude of +8.54, 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 +1.169.
Propiedades físicas
| Clase Espectral | K Class K — K-type (Orange) |
| Índice de color (B−V) | 1,169 |
Observación
| Magnitud Aparente | +8.54 |
| Magnitud Absoluta | 0,48 |
| Distancia | 1,337 ly |
| Constelación | Pegasus |
Posición
| Ascensión recta | 23h 8,31m |
| Declinación | 10° 34,67′ |
Frequently Asked Questions
What type of star is HIP 114250?
HIP 114250 is a Class K — K-type (Orange) star.
How far is HIP 114250 from Earth?
HIP 114250 is approximately 1,336.7 light-years from Earth.
Can you see HIP 114250 with the naked eye?
With an apparent magnitude of 8.54, HIP 114250 is not visible to the naked eye.
What constellation is HIP 114250 in?
HIP 114250 is located in the constellation Pegasus.