HIP 15999
HIP 15999 is a B-type (Blue-White) star located in the constellation Perseus.
At a distance of roughly 1,599 light-years, HIP 15999 is a distant star lying deep within the Milky Way galaxy.
HIP 15999 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 15999 has an apparent magnitude of +7.92, 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 +0.007.
Physical Properties
| Spectral Class | Class B — B-type (Blue-White) |
| Color Index (B−V) | 0.007 |
Observation
| Apparent Magnitude | +7.92 |
| Absolute Magnitude | -0.53 |
| Distance | 1,599 ly |
| Constellation | Perseus |
Position
| Right Ascension | 3h 26.07m |
| Declination | 45° 17.97′ |
Frequently Asked Questions
What type of star is HIP 15999?
HIP 15999 is a Class B — B-type (Blue-White) star.
How far is HIP 15999 from Earth?
HIP 15999 is approximately 1,598.8 light-years from Earth.
Can you see HIP 15999 with the naked eye?
With an apparent magnitude of 7.92, HIP 15999 is not visible to the naked eye.
What constellation is HIP 15999 in?
HIP 15999 is located in the constellation Perseus.