HIP 4377
HIP 4377 is a B-type (Blue-White) star located in the constellation Cassiopeia.
At a distance of roughly 2,381 light-years, HIP 4377 is a distant star lying deep within the Milky Way galaxy.
HIP 4377 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 4377 has an apparent magnitude of +9.38, 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 white hue, which corresponds to a B-V color index of +0.557.
Physical Properties
| Spectral Class | Class B — B-type (Blue-White) |
| Color Index (B−V) | 0.557 |
Observation
| Apparent Magnitude | +9.38 |
| Absolute Magnitude | 0.06 |
| Distance | 2,381 ly |
| Constellation | Cassiopeia |
Position
| Right Ascension | 0h 56.08m |
| Declination | 67° 22.63′ |
Frequently Asked Questions
What type of star is HIP 4377?
HIP 4377 is a Class B — B-type (Blue-White) star.
How far is HIP 4377 from Earth?
HIP 4377 is approximately 2,380.7 light-years from Earth.
Can you see HIP 4377 with the naked eye?
With an apparent magnitude of 9.38, HIP 4377 is not visible to the naked eye.
What constellation is HIP 4377 in?
HIP 4377 is located in the constellation Cassiopeia.