HIP 11492
HIP 11492 is a K-type (Orange) star located in the constellation Perseus.
At a distance of roughly 2,363 light-years, HIP 11492 is a distant star lying deep within the Milky Way galaxy.
HIP 11492 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 11492 has an apparent magnitude of +8.85, 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 orange hue, which corresponds to a B-V color index of +1.133.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.133 |
Observation
| Apparent Magnitude | +8.85 |
| Absolute Magnitude | -0.45 |
| Distance | 2,363 ly |
| Constellation | Perseus |
Position
| Right Ascension | 2h 28.22m |
| Declination | 54° 22.90′ |
Frequently Asked Questions
What type of star is HIP 11492?
HIP 11492 is a Class K — K-type (Orange) star.
How far is HIP 11492 from Earth?
HIP 11492 is approximately 2,363.4 light-years from Earth.
Can you see HIP 11492 with the naked eye?
With an apparent magnitude of 8.85, HIP 11492 is not visible to the naked eye.
What constellation is HIP 11492 in?
HIP 11492 is located in the constellation Perseus.