HIP 101718
HIP 101718 is a K-type (Orange) star located in the constellation Aquila.
At a distance of roughly 3,106 light-years, HIP 101718 is a distant star lying deep within the Milky Way galaxy.
HIP 101718 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 101718 has an apparent magnitude of +8.71, 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 red hue, which corresponds to a B-V color index of +1.660.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.660 |
Observation
| Apparent Magnitude | +8.71 |
| Absolute Magnitude | -1.18 |
| Distance | 3,106 ly |
| Constellation | Aquila |
Position
| Right Ascension | 20h 37.13m |
| Declination | 0° 31.04′ |
Frequently Asked Questions
What type of star is HIP 101718?
HIP 101718 is a Class K — K-type (Orange) star.
How far is HIP 101718 from Earth?
HIP 101718 is approximately 3,106.2 light-years from Earth.
Can you see HIP 101718 with the naked eye?
With an apparent magnitude of 8.71, HIP 101718 is not visible to the naked eye.
What constellation is HIP 101718 in?
HIP 101718 is located in the constellation Aquila.