HIP 67218
HIP 67218 is a B-type (Blue-White) star located in the constellation Centaurus.
HIP 67218 is an extraordinarily remote star, situated approximately 326,156 light-years from Earth.
HIP 67218 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 67218 has an apparent magnitude of +9.21, 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 hue, which corresponds to a B-V color index of -0.014.
Physical Properties
| Spectral Class | Class B — B-type (Blue-White) |
| Color Index (B−V) | -0.014 |
Observation
| Apparent Magnitude | +9.21 |
| Absolute Magnitude | -10.79 |
| Distance | 326,156 ly |
| Constellation | Centaurus |
Position
| Right Ascension | 13h 46.47m |
| Declination | -61° 20.96′ |
Frequently Asked Questions
What type of star is HIP 67218?
HIP 67218 is a Class B — B-type (Blue-White) star.
How far is HIP 67218 from Earth?
HIP 67218 is approximately 326,156.0 light-years from Earth.
Can you see HIP 67218 with the naked eye?
With an apparent magnitude of 9.21, HIP 67218 is not visible to the naked eye.
What constellation is HIP 67218 in?
HIP 67218 is located in the constellation Centaurus.