HIP 89017
HIP 89017 is a K-type (Orange) star.
At a distance of roughly 1,177 light-years, HIP 89017 is a distant star lying deep within the Milky Way galaxy.
HIP 89017 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 89017 has an apparent magnitude of +7.40, 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 +1.273.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 1.273 |
Observation
| Apparent Magnitude | +7.40 |
| Absolute Magnitude | -0.39 |
| Distance | 1,177 ly |
Position
| Right Ascension | 18h 10.06m |
| Declination | 56° 16.01′ |
Frequently Asked Questions
What type of star is HIP 89017?
HIP 89017 is a Class K — K-type (Orange) star.
How far is HIP 89017 from Earth?
HIP 89017 is approximately 1,177.5 light-years from Earth.
Can you see HIP 89017 with the naked eye?
With an apparent magnitude of 7.40, HIP 89017 is not visible to the naked eye.