HIP 16457
HIP 16457 is a K-type (Orange) star.
At a distance of roughly 1,157 light-years, HIP 16457 is a distant star lying deep within the Milky Way galaxy.
HIP 16457 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 16457 has an apparent magnitude of +8.23, 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 +1.246.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 1.246 |
Observation
| Apparent Magnitude | +8.23 |
| Absolute Magnitude | 0.48 |
| Distance | 1,157 ly |
Position
| Right Ascension | 3h 32.01m |
| Declination | -65° 38.73′ |
Frequently Asked Questions
What type of star is HIP 16457?
HIP 16457 is a Class K — K-type (Orange) star.
How far is HIP 16457 from Earth?
HIP 16457 is approximately 1,156.6 light-years from Earth.
Can you see HIP 16457 with the naked eye?
With an apparent magnitude of 8.23, HIP 16457 is not visible to the naked eye.