HIP 110247
HIP 110247 is a K-type (Orange) star located in the constellation Pegasus.
At a distance of roughly 1,062 light-years, HIP 110247 is a distant star lying deep within the Milky Way galaxy.
HIP 110247 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 110247 has an apparent magnitude of +7.29, 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 +1.590.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.590 |
Observation
| Apparent Magnitude | +7.29 |
| Absolute Magnitude | -0.27 |
| Distance | 1,062 ly |
| Constellation | Pegasus |
Position
| Right Ascension | 22h 19.90m |
| Declination | 25° 43.44′ |
Frequently Asked Questions
What type of star is HIP 110247?
HIP 110247 is a Class K — K-type (Orange) star.
How far is HIP 110247 from Earth?
HIP 110247 is approximately 1,062.4 light-years from Earth.
Can you see HIP 110247 with the naked eye?
With an apparent magnitude of 7.29, HIP 110247 is not visible to the naked eye.
What constellation is HIP 110247 in?
HIP 110247 is located in the constellation Pegasus.