HIP 13250
HIP 13250 is a B-type (Blue-White) star located in the constellation Perseus.
At a distance of roughly 2,104 light-years, HIP 13250 is a distant star lying deep within the Milky Way galaxy.
HIP 13250 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 13250 has an apparent magnitude of +7.53, 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 +0.072.
Physical Properties
| Spectral Class | Class B — B-type (Blue-White) |
| Color Index (B−V) | 0.072 |
Observation
| Apparent Magnitude | +7.53 |
| Absolute Magnitude | -1.52 |
| Distance | 2,104 ly |
| Constellation | Perseus |
Position
| Right Ascension | 2h 50.55m |
| Declination | 52° 16.98′ |
Frequently Asked Questions
What type of star is HIP 13250?
HIP 13250 is a Class B — B-type (Blue-White) star.
How far is HIP 13250 from Earth?
HIP 13250 is approximately 2,104.2 light-years from Earth.
Can you see HIP 13250 with the naked eye?
With an apparent magnitude of 7.53, HIP 13250 is not visible to the naked eye.
What constellation is HIP 13250 in?
HIP 13250 is located in the constellation Perseus.