HIP 70905
HIP 70905 is a B-type (Blue-White) star located in the constellation Centaurus.
At a distance of roughly 2,038 light-years, HIP 70905 is a distant star lying deep within the Milky Way galaxy.
HIP 70905 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 70905 has an apparent magnitude of +9.01, 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 -0.009.
Physical Properties
| Spectral Class | B Class B — B-type (Blue-White) |
| Color Index (B−V) | -0.009 |
Observation
| Apparent Magnitude | +9.01 |
| Absolute Magnitude | 0.03 |
| Distance | 2,038 ly |
| Constellation | Centaurus |
Position
| Right Ascension | 14h 29.98m |
| Declination | -59° 46.52′ |
Frequently Asked Questions
What type of star is HIP 70905?
HIP 70905 is a Class B — B-type (Blue-White) star.
How far is HIP 70905 from Earth?
HIP 70905 is approximately 2,038.5 light-years from Earth.
Can you see HIP 70905 with the naked eye?
With an apparent magnitude of 9.01, HIP 70905 is not visible to the naked eye.
What constellation is HIP 70905 in?
HIP 70905 is located in the constellation Centaurus.