HIP 67617
HIP 67617 is a B-type (Blue-White) star located in the constellation Centaurus.
At a distance of roughly 1,664 light-years, HIP 67617 is a distant star lying deep within the Milky Way galaxy.
HIP 67617 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 67617 has an apparent magnitude of +8.79, 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 +0.003.
Physical Properties
| Spectral Class | B Class B — B-type (Blue-White) |
| Color Index (B−V) | 0.003 |
Observation
| Apparent Magnitude | +8.79 |
| Absolute Magnitude | 0.25 |
| Distance | 1,664 ly |
| Constellation | Centaurus |
Position
| Right Ascension | 13h 51.32m |
| Declination | -64° 31.58′ |
Frequently Asked Questions
What type of star is HIP 67617?
HIP 67617 is a Class B — B-type (Blue-White) star.
How far is HIP 67617 from Earth?
HIP 67617 is approximately 1,664.1 light-years from Earth.
Can you see HIP 67617 with the naked eye?
With an apparent magnitude of 8.79, HIP 67617 is not visible to the naked eye.
What constellation is HIP 67617 in?
HIP 67617 is located in the constellation Centaurus.