HIP 16507
HIP 16507 is a K-type (Orange) star located in the constellation Perseus.
At a distance of roughly 1,310 light-years, HIP 16507 is a distant star lying deep within the Milky Way galaxy.
HIP 16507 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 16507 has an apparent magnitude of +7.75, 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 orange hue, which corresponds to a B-V color index of +1.129.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.129 |
Observation
| Apparent Magnitude | +7.75 |
| Absolute Magnitude | -0.27 |
| Distance | 1,310 ly |
| Constellation | Perseus |
Position
| Right Ascension | 3h 32.53m |
| Declination | 31° 38.88′ |
Frequently Asked Questions
What type of star is HIP 16507?
HIP 16507 is a Class K — K-type (Orange) star.
How far is HIP 16507 from Earth?
HIP 16507 is approximately 1,309.9 light-years from Earth.
Can you see HIP 16507 with the naked eye?
With an apparent magnitude of 7.75, HIP 16507 is not visible to the naked eye.
What constellation is HIP 16507 in?
HIP 16507 is located in the constellation Perseus.