HIP 54490
HIP 54490 is a K-type (Orange) star located in the constellation Centaurus.
Located approximately 879.1 light-years from Earth, HIP 54490 resides within the broader disk of our Milky Way galaxy.
HIP 54490 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 54490 has an apparent magnitude of +8.53, 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 yellow hue, which corresponds to a B-V color index of +0.985.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 0.985 |
Observation
| Apparent Magnitude | +8.53 |
| Absolute Magnitude | 1.38 |
| Distance | 879 ly |
| Constellation | Centaurus |
Position
| Right Ascension | 11h 8.92m |
| Declination | -52° 18.24′ |
Frequently Asked Questions
What type of star is HIP 54490?
HIP 54490 is a Class K — K-type (Orange) star.
How far is HIP 54490 from Earth?
HIP 54490 is approximately 879.1 light-years from Earth.
Can you see HIP 54490 with the naked eye?
With an apparent magnitude of 8.53, HIP 54490 is not visible to the naked eye.
What constellation is HIP 54490 in?
HIP 54490 is located in the constellation Centaurus.