HIP 101155
HIP 101155 is a K-type (Orange) star located in the constellation Aquila.
At a distance of roughly 1,299 light-years, HIP 101155 is a distant star lying deep within the Milky Way galaxy.
HIP 101155 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 101155 has an apparent magnitude of +8.56, 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 +1.354.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.354 |
Observation
| Apparent Magnitude | +8.56 |
| Absolute Magnitude | 0.56 |
| Distance | 1,299 ly |
| Constellation | Aquila |
Position
| Right Ascension | 20h 30.25m |
| Declination | -1° 10.37′ |
Frequently Asked Questions
What type of star is HIP 101155?
HIP 101155 is a Class K — K-type (Orange) star.
How far is HIP 101155 from Earth?
HIP 101155 is approximately 1,299.4 light-years from Earth.
Can you see HIP 101155 with the naked eye?
With an apparent magnitude of 8.56, HIP 101155 is not visible to the naked eye.
What constellation is HIP 101155 in?
HIP 101155 is located in the constellation Aquila.