HIP 10979
HIP 10979 is a A-type (White) star located in the constellation Perseus.
At a distance of roughly 1,042 light-years, HIP 10979 is a distant star lying deep within the Milky Way galaxy.
HIP 10979 is classified as a spectral class A star (A-type (White)) on the Harvard spectral classification system.
HIP 10979 has an apparent magnitude of +8.99, 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 +0.122.
Physical Properties
| Spectral Class | Class A — A-type (White) |
| Color Index (B−V) | 0.122 |
Observation
| Apparent Magnitude | +8.99 |
| Absolute Magnitude | 1.47 |
| Distance | 1,042 ly |
| Constellation | Perseus |
Position
| Right Ascension | 2h 21.43m |
| Declination | 52° 42.43′ |
Frequently Asked Questions
What type of star is HIP 10979?
HIP 10979 is a Class A — A-type (White) star.
How far is HIP 10979 from Earth?
HIP 10979 is approximately 1,042.0 light-years from Earth.
Can you see HIP 10979 with the naked eye?
With an apparent magnitude of 8.99, HIP 10979 is not visible to the naked eye.
What constellation is HIP 10979 in?
HIP 10979 is located in the constellation Perseus.