HIP 17458
HIP 17458 is a M-type (Red) star located in the constellation Perseus.
Located approximately 82.6 light-years from Earth, HIP 17458 resides within the broader disk of our Milky Way galaxy.
HIP 17458 is classified as a spectral class M star (M-type (Red)) on the Harvard spectral classification system.
At an apparent magnitude of +10.63, HIP 17458 is a faint star that requires a telescope to observe. It is invisible to the naked eye and too dim for most binoculars. Observers will note its orange hue, which corresponds to a B-V color index of +1.380.
Physical Properties
| Spectral Class | Class M — M-type (Red) |
| Color Index (B−V) | 1.380 |
Observation
| Apparent Magnitude | +10.63 |
| Absolute Magnitude | 8.61 |
| Distance | 82.6 ly |
| Constellation | Perseus |
Position
| Right Ascension | 3h 44.52m |
| Declination | 34° 58.39′ |
Frequently Asked Questions
What type of star is HIP 17458?
HIP 17458 is a Class M — M-type (Red) star.
How far is HIP 17458 from Earth?
HIP 17458 is approximately 82.6 light-years from Earth.
Can you see HIP 17458 with the naked eye?
With an apparent magnitude of 10.63, HIP 17458 is not visible to the naked eye.
What constellation is HIP 17458 in?
HIP 17458 is located in the constellation Perseus.