HIP 112618
HIP 112618 is a K-type (Orange) star located in the constellation Pegasus.
At a distance of roughly 1,326 light-years, HIP 112618 is a distant star lying deep within the Milky Way galaxy.
HIP 112618 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 112618 has an apparent magnitude of +8.75, 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 +1.468.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.468 |
Observation
| Apparent Magnitude | +8.75 |
| Absolute Magnitude | 0.70 |
| Distance | 1,326 ly |
| Constellation | Pegasus |
Position
| Right Ascension | 22h 48.52m |
| Declination | 16° 30.50′ |
Frequently Asked Questions
What type of star is HIP 112618?
HIP 112618 is a Class K — K-type (Orange) star.
How far is HIP 112618 from Earth?
HIP 112618 is approximately 1,325.8 light-years from Earth.
Can you see HIP 112618 with the naked eye?
With an apparent magnitude of 8.75, HIP 112618 is not visible to the naked eye.
What constellation is HIP 112618 in?
HIP 112618 is located in the constellation Pegasus.