HIP 11377
HIP 11377 is a K-type (Orange) star located in the constellation Perseus.
At a distance of roughly 1,087 light-years, HIP 11377 is a distant star lying deep within the Milky Way galaxy.
HIP 11377 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 11377 has an apparent magnitude of +8.79, 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 yellow hue, which corresponds to a B-V color index of +0.832.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 0.832 |
Observation
| Apparent Magnitude | +8.79 |
| Absolute Magnitude | 1.18 |
| Distance | 1,087 ly |
| Constellation | Perseus |
Position
| Right Ascension | 2h 26.51m |
| Declination | 51° 42.33′ |
Frequently Asked Questions
What type of star is HIP 11377?
HIP 11377 is a Class K — K-type (Orange) star.
How far is HIP 11377 from Earth?
HIP 11377 is approximately 1,087.2 light-years from Earth.
Can you see HIP 11377 with the naked eye?
With an apparent magnitude of 8.79, HIP 11377 is not visible to the naked eye.
What constellation is HIP 11377 in?
HIP 11377 is located in the constellation Perseus.