HIP 17297
HIP 17297 is a K-type (Orange) star.
At a distance of roughly 1,583 light-years, HIP 17297 is a distant star lying deep within the Milky Way galaxy.
HIP 17297 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 17297 has an apparent magnitude of +8.92, 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 +1.408.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 1.408 |
Observation
| Apparent Magnitude | +8.92 |
| Absolute Magnitude | 0.49 |
| Distance | 1,583 ly |
Position
| Right Ascension | 3h 42.16m |
| Declination | -40° 2.97′ |
Frequently Asked Questions
What type of star is HIP 17297?
HIP 17297 is a Class K — K-type (Orange) star.
How far is HIP 17297 from Earth?
HIP 17297 is approximately 1,583.3 light-years from Earth.
Can you see HIP 17297 with the naked eye?
With an apparent magnitude of 8.92, HIP 17297 is not visible to the naked eye.