HIP 7187
HIP 7187 is a K-type (Orange) star.
At a distance of roughly 1,222 light-years, HIP 7187 is a distant star lying deep within the Milky Way galaxy.
HIP 7187 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 7187 has an apparent magnitude of +9.03, 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 +1.146.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.146 |
Observation
| Apparent Magnitude | +9.03 |
| Absolute Magnitude | 1.16 |
| Distance | 1,222 ly |
Position
| Right Ascension | 1h 32.60m |
| Declination | -54° 44.54′ |
Frequently Asked Questions
What type of star is HIP 7187?
HIP 7187 is a Class K — K-type (Orange) star.
How far is HIP 7187 from Earth?
HIP 7187 is approximately 1,221.6 light-years from Earth.
Can you see HIP 7187 with the naked eye?
With an apparent magnitude of 9.03, HIP 7187 is not visible to the naked eye.