HIP 17390
HIP 17390 is a K-type (Orange) star.
At a distance of roughly 2,452 light-years, HIP 17390 is a distant star lying deep within the Milky Way galaxy.
HIP 17390 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 17390 has an apparent magnitude of +9.52, 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 +1.561.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 1.561 |
Observation
| Apparent Magnitude | +9.52 |
| Absolute Magnitude | 0.14 |
| Distance | 2,452 ly |
Position
| Right Ascension | 3h 43.45m |
| Declination | -39° 37.38′ |
Frequently Asked Questions
What type of star is HIP 17390?
HIP 17390 is a Class K — K-type (Orange) star.
How far is HIP 17390 from Earth?
HIP 17390 is approximately 2,452.3 light-years from Earth.
Can you see HIP 17390 with the naked eye?
With an apparent magnitude of 9.52, HIP 17390 is not visible to the naked eye.