HIP 101499
HIP 101499 is a K-type (Orange) star.
At a distance of roughly 1,186 light-years, HIP 101499 is a distant star lying deep within the Milky Way galaxy.
HIP 101499 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 101499 has an apparent magnitude of +7.76, 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 +1.375.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.375 |
Observation
| Apparent Magnitude | +7.76 |
| Absolute Magnitude | -0.04 |
| Distance | 1,186 ly |
Position
| Right Ascension | 20h 34.12m |
| Declination | 19° 57.05′ |
Frequently Asked Questions
What type of star is HIP 101499?
HIP 101499 is a Class K — K-type (Orange) star.
How far is HIP 101499 from Earth?
HIP 101499 is approximately 1,186.0 light-years from Earth.
Can you see HIP 101499 with the naked eye?
With an apparent magnitude of 7.76, HIP 101499 is not visible to the naked eye.