HIP 93488
HIP 93488 is a K-type (Orange) star located in the constellation Aquila.
At a distance of roughly 1,217 light-years, HIP 93488 is a distant star lying deep within the Milky Way galaxy.
HIP 93488 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 93488 has an apparent magnitude of +6.25, 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 +1.648.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.648 |
Observation
| Apparent Magnitude | +6.25 |
| Absolute Magnitude | -1.61 |
| Distance | 1,217 ly |
| Constellation | Aquila |
Position
| Right Ascension | 19h 2.36m |
| Declination | 8° 22.41′ |
Frequently Asked Questions
What type of star is HIP 93488?
HIP 93488 is a Class K — K-type (Orange) star.
How far is HIP 93488 from Earth?
HIP 93488 is approximately 1,217.0 light-years from Earth.
Can you see HIP 93488 with the naked eye?
With an apparent magnitude of 6.25, HIP 93488 is not visible to the naked eye.
What constellation is HIP 93488 in?
HIP 93488 is located in the constellation Aquila.