HIP 22050
HIP 22050 is a F-type (Yellow-White) star located in the constellation Perseus.
At a distance of roughly 1,113 light-years, HIP 22050 is a distant star lying deep within the Milky Way galaxy.
HIP 22050 is classified as a spectral class F star (F-type (Yellow-White)) on the Harvard spectral classification system.
HIP 22050 has an apparent magnitude of +8.31, 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 white hue, which corresponds to a B-V color index of +0.510.
Physical Properties
| Spectral Class | Class F — F-type (Yellow-White) |
| Color Index (B−V) | 0.510 |
Observation
| Apparent Magnitude | +8.31 |
| Absolute Magnitude | 0.64 |
| Distance | 1,113 ly |
| Constellation | Perseus |
Position
| Right Ascension | 4h 44.55m |
| Declination | 39° 52.53′ |
Frequently Asked Questions
What type of star is HIP 22050?
HIP 22050 is a Class F — F-type (Yellow-White) star.
How far is HIP 22050 from Earth?
HIP 22050 is approximately 1,113.2 light-years from Earth.
Can you see HIP 22050 with the naked eye?
With an apparent magnitude of 8.31, HIP 22050 is not visible to the naked eye.
What constellation is HIP 22050 in?
HIP 22050 is located in the constellation Perseus.