HIP 10475
HIP 10475 is a B-type (Blue-White) star located in the constellation Perseus.
HIP 10475 is an extraordinarily remote star, situated approximately 326,156 light-years from Earth.
HIP 10475 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 10475 has an apparent magnitude of +8.40, 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 -0.003.
Physical Properties
| Spectral Class | Class B — B-type (Blue-White) |
| Color Index (B−V) | -0.003 |
Observation
| Apparent Magnitude | +8.40 |
| Absolute Magnitude | -11.60 |
| Distance | 326,156 ly |
| Constellation | Perseus |
Position
| Right Ascension | 2h 15.04m |
| Declination | 55° 47.59′ |
Frequently Asked Questions
What type of star is HIP 10475?
HIP 10475 is a Class B — B-type (Blue-White) star.
How far is HIP 10475 from Earth?
HIP 10475 is approximately 326,156.0 light-years from Earth.
Can you see HIP 10475 with the naked eye?
With an apparent magnitude of 8.40, HIP 10475 is not visible to the naked eye.
What constellation is HIP 10475 in?
HIP 10475 is located in the constellation Perseus.