HIP 19525
HIP 19525 is a K-type (Orange) star located in the constellation Perseus.
Located approximately 982.4 light-years from Earth, HIP 19525 resides within the broader disk of our Milky Way galaxy.
HIP 19525 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
With an apparent magnitude of +5.75, HIP 19525 sits near the limit of naked-eye visibility. It can be glimpsed without optical aid under dark skies, but binoculars will make observation much easier. Observers will note its red hue, which corresponds to a B-V color index of +1.412.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 1.412 |
Observation
| Apparent Magnitude | +5.75 |
| Absolute Magnitude | -1.64 |
| Distance | 982 ly |
| Constellation | Perseus |
Position
| Right Ascension | 4h 10.98m |
| Declination | 33° 35.21′ |
Frequently Asked Questions
What type of star is HIP 19525?
HIP 19525 is a Class K — K-type (Orange) star.
How far is HIP 19525 from Earth?
HIP 19525 is approximately 982.4 light-years from Earth.
Can you see HIP 19525 with the naked eye?
With an apparent magnitude of 5.75, HIP 19525 is visible to the naked eye.
What constellation is HIP 19525 in?
HIP 19525 is located in the constellation Perseus.