HIP 117299
HIP 117299 is a K-type (Orange) star located in the constellation Cassiopeia.
At a distance of roughly 1,607 light-years, HIP 117299 is a distant star lying deep within the Milky Way galaxy.
HIP 117299 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
With an apparent magnitude of +5.55, HIP 117299 sits near the limit of naked-eye visibility. It can be glimpsed without optical aid under dark skies, but binoculars will make observation much easier. Observers will note its red hue, which corresponds to a B-V color index of +1.630.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.630 |
Observation
| Apparent Magnitude | +5.55 |
| Absolute Magnitude | -2.91 |
| Distance | 1,607 ly |
| Constellation | Cassiopeia |
Position
| Right Ascension | 23h 47.03m |
| Declination | 57° 27.08′ |
Frequently Asked Questions
What type of star is HIP 117299?
HIP 117299 is a Class K — K-type (Orange) star.
How far is HIP 117299 from Earth?
HIP 117299 is approximately 1,606.7 light-years from Earth.
Can you see HIP 117299 with the naked eye?
With an apparent magnitude of 5.55, HIP 117299 is visible to the naked eye.
What constellation is HIP 117299 in?
HIP 117299 is located in the constellation Cassiopeia.