HIP 107579
HIP 107579 is a K-type (Orange) star located in the constellation Pegasus.
At a distance of roughly 1,431 light-years, HIP 107579 is a distant star lying deep within the Milky Way galaxy.
HIP 107579 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 107579 has an apparent magnitude of +8.61, 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 +1.344.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.344 |
Observation
| Apparent Magnitude | +8.61 |
| Absolute Magnitude | 0.40 |
| Distance | 1,431 ly |
| Constellation | Pegasus |
Position
| Right Ascension | 21h 47.32m |
| Declination | 28° 5.51′ |
Frequently Asked Questions
What type of star is HIP 107579?
HIP 107579 is a Class K — K-type (Orange) star.
How far is HIP 107579 from Earth?
HIP 107579 is approximately 1,430.5 light-years from Earth.
Can you see HIP 107579 with the naked eye?
With an apparent magnitude of 8.61, HIP 107579 is not visible to the naked eye.
What constellation is HIP 107579 in?
HIP 107579 is located in the constellation Pegasus.