HIP 13770
HIP 13770 is a K-type (Orange) star located in the constellation Perseus.
At a distance of roughly 1,305 light-years, HIP 13770 is a distant star lying deep within the Milky Way galaxy.
HIP 13770 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 13770 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 red hue, which corresponds to a B-V color index of +1.561.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.561 |
Observation
| Apparent Magnitude | +8.79 |
| Absolute Magnitude | 0.78 |
| Distance | 1,305 ly |
| Constellation | Perseus |
Position
| Right Ascension | 2h 57.22m |
| Declination | 33° 57.63′ |
Frequently Asked Questions
What type of star is HIP 13770?
HIP 13770 is a Class K — K-type (Orange) star.
How far is HIP 13770 from Earth?
HIP 13770 is approximately 1,304.6 light-years from Earth.
Can you see HIP 13770 with the naked eye?
With an apparent magnitude of 8.79, HIP 13770 is not visible to the naked eye.
What constellation is HIP 13770 in?
HIP 13770 is located in the constellation Perseus.