HIP 17850
HIP 17850 is a K-type (Orange) star.
At a distance of roughly 1,348 light-years, HIP 17850 is a distant star lying deep within the Milky Way galaxy.
HIP 17850 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 17850 has an apparent magnitude of +9.69, 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 +1.541.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 1.541 |
Observation
| Apparent Magnitude | +9.69 |
| Absolute Magnitude | 1.61 |
| Distance | 1,348 ly |
Position
| Right Ascension | 3h 49.18m |
| Declination | -24° 55.80′ |
Frequently Asked Questions
What type of star is HIP 17850?
HIP 17850 is a Class K — K-type (Orange) star.
How far is HIP 17850 from Earth?
HIP 17850 is approximately 1,347.8 light-years from Earth.
Can you see HIP 17850 with the naked eye?
With an apparent magnitude of 9.69, HIP 17850 is not visible to the naked eye.