HIP 54458
HIP 54458 is a K-type (Orange) star located in the constellation Leo.
At a distance of roughly 1,305 light-years, HIP 54458 is a distant star lying deep within the Milky Way galaxy.
HIP 54458 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 54458 has an apparent magnitude of +8.67, 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 +1.371.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.371 |
Observation
| Apparent Magnitude | +8.67 |
| Absolute Magnitude | 0.66 |
| Distance | 1,305 ly |
| Constellation | Leo |
Position
| Right Ascension | 11h 8.53m |
| Declination | -6° 25.06′ |
Frequently Asked Questions
What type of star is HIP 54458?
HIP 54458 is a Class K — K-type (Orange) star.
How far is HIP 54458 from Earth?
HIP 54458 is approximately 1,304.6 light-years from Earth.
Can you see HIP 54458 with the naked eye?
With an apparent magnitude of 8.67, HIP 54458 is not visible to the naked eye.
What constellation is HIP 54458 in?
HIP 54458 is located in the constellation Leo.