HIP 3477
HIP 3477 is a F-type (Yellow-White) star located in the constellation Cassiopeia.
Located approximately 519.4 light-years from Earth, HIP 3477 resides within the broader disk of our Milky Way galaxy.
HIP 3477 is classified as a spectral class F star (F-type (Yellow-White)) on the Harvard spectral classification system.
HIP 3477 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 white hue, which corresponds to a B-V color index of +0.345.
Physical Properties
| Spectral Class | F Class F — F-type (Yellow-White) |
| Color Index (B−V) | 0.345 |
Observation
| Apparent Magnitude | +8.40 |
| Absolute Magnitude | 2.39 |
| Distance | 519 ly |
| Constellation | Cassiopeia |
Position
| Right Ascension | 0h 44.42m |
| Declination | 67° 2.01′ |
Frequently Asked Questions
What type of star is HIP 3477?
HIP 3477 is a Class F — F-type (Yellow-White) star.
How far is HIP 3477 from Earth?
HIP 3477 is approximately 519.4 light-years from Earth.
Can you see HIP 3477 with the naked eye?
With an apparent magnitude of 8.40, HIP 3477 is not visible to the naked eye.
What constellation is HIP 3477 in?
HIP 3477 is located in the constellation Cassiopeia.