HIP 115699
HIP 115699 is a K-type (Orange) star located in the constellation Pegasus.
Located approximately 673.9 light-years from Earth, HIP 115699 resides within the broader disk of our Milky Way galaxy.
HIP 115699 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 115699 has an apparent magnitude of +8.49, 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 +1.130.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.130 |
Observation
| Apparent Magnitude | +8.49 |
| Absolute Magnitude | 1.91 |
| Distance | 674 ly |
| Constellation | Pegasus |
Position
| Right Ascension | 23h 26.48m |
| Declination | 17° 30.58′ |
Frequently Asked Questions
What type of star is HIP 115699?
HIP 115699 is a Class K — K-type (Orange) star.
How far is HIP 115699 from Earth?
HIP 115699 is approximately 673.9 light-years from Earth.
Can you see HIP 115699 with the naked eye?
With an apparent magnitude of 8.49, HIP 115699 is not visible to the naked eye.
What constellation is HIP 115699 in?
HIP 115699 is located in the constellation Pegasus.