HIP 14830
HIP 14830 is a K-type (Orange) star located in the constellation Perseus.
Located approximately 858.3 light-years from Earth, HIP 14830 resides within the broader disk of our Milky Way galaxy.
HIP 14830 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 14830 has an apparent magnitude of +9.22, 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 +1.404.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.404 |
Observation
| Apparent Magnitude | +9.22 |
| Absolute Magnitude | 2.12 |
| Distance | 858 ly |
| Constellation | Perseus |
Position
| Right Ascension | 3h 11.50m |
| Declination | 51° 5.18′ |
Frequently Asked Questions
What type of star is HIP 14830?
HIP 14830 is a Class K — K-type (Orange) star.
How far is HIP 14830 from Earth?
HIP 14830 is approximately 858.3 light-years from Earth.
Can you see HIP 14830 with the naked eye?
With an apparent magnitude of 9.22, HIP 14830 is not visible to the naked eye.
What constellation is HIP 14830 in?
HIP 14830 is located in the constellation Perseus.