HIP 66751
HIP 66751 is a B-type (Blue-White) star located in the constellation Centaurus.
At a distance of roughly 3,106 light-years, HIP 66751 is a distant star lying deep within the Milky Way galaxy.
HIP 66751 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 66751 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 blue-white hue, which corresponds to a B-V color index of +0.031.
Physical Properties
| Spectral Class | B Class B — B-type (Blue-White) |
| Color Index (B−V) | 0.031 |
Observation
| Apparent Magnitude | +8.67 |
| Absolute Magnitude | -1.22 |
| Distance | 3,106 ly |
| Constellation | Centaurus |
Position
| Right Ascension | 13h 40.86m |
| Declination | -62° 52.79′ |
Frequently Asked Questions
What type of star is HIP 66751?
HIP 66751 is a Class B — B-type (Blue-White) star.
How far is HIP 66751 from Earth?
HIP 66751 is approximately 3,106.2 light-years from Earth.
Can you see HIP 66751 with the naked eye?
With an apparent magnitude of 8.67, HIP 66751 is not visible to the naked eye.
What constellation is HIP 66751 in?
HIP 66751 is located in the constellation Centaurus.