HIP 56752
HIP 56752 is a K-type (Orange) star located in the constellation Centaurus.
At a distance of roughly 2,160 light-years, HIP 56752 is a distant star lying deep within the Milky Way galaxy.
HIP 56752 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 56752 has an apparent magnitude of +8.10, 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 +1.327.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.327 |
Observation
| Apparent Magnitude | +8.10 |
| Absolute Magnitude | -1.00 |
| Distance | 2,160 ly |
| Constellation | Centaurus |
Position
| Right Ascension | 11h 38.11m |
| Declination | -52° 44.27′ |
Frequently Asked Questions
What type of star is HIP 56752?
HIP 56752 is a Class K — K-type (Orange) star.
How far is HIP 56752 from Earth?
HIP 56752 is approximately 2,160.0 light-years from Earth.
Can you see HIP 56752 with the naked eye?
With an apparent magnitude of 8.10, HIP 56752 is not visible to the naked eye.
What constellation is HIP 56752 in?
HIP 56752 is located in the constellation Centaurus.