HIP 8950
HIP 8950 is a A-type (White) star located in the constellation Perseus.
At a distance of roughly 2,452 light-years, HIP 8950 is a distant star lying deep within the Milky Way galaxy.
HIP 8950 is classified as a spectral class A star (A-type (White)) on the Harvard spectral classification system.
HIP 8950 has an apparent magnitude of +7.72, 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 blue-white hue, which corresponds to a B-V color index of +0.056.
Physical Properties
| Spectral Class | Class A — A-type (White) |
| Color Index (B−V) | 0.056 |
Observation
| Apparent Magnitude | +7.72 |
| Absolute Magnitude | -1.66 |
| Distance | 2,452 ly |
| Constellation | Perseus |
Position
| Right Ascension | 1h 55.29m |
| Declination | 57° 5.53′ |
Frequently Asked Questions
What type of star is HIP 8950?
HIP 8950 is a Class A — A-type (White) star.
How far is HIP 8950 from Earth?
HIP 8950 is approximately 2,452.3 light-years from Earth.
Can you see HIP 8950 with the naked eye?
With an apparent magnitude of 7.72, HIP 8950 is not visible to the naked eye.
What constellation is HIP 8950 in?
HIP 8950 is located in the constellation Perseus.