HIP 16782
HIP 16782 is a B-type (Blue-White) star located in the constellation Perseus.
Located approximately 579.3 light-years from Earth, HIP 16782 resides within the broader disk of our Milky Way galaxy.
HIP 16782 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 16782 has an apparent magnitude of +6.89, 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 -0.022.
Physical Properties
| Spectral Class | Class B — B-type (Blue-White) |
| Color Index (B−V) | -0.022 |
Observation
| Apparent Magnitude | +6.89 |
| Absolute Magnitude | 0.64 |
| Distance | 579 ly |
| Constellation | Perseus |
Position
| Right Ascension | 3h 35.97m |
| Declination | 47° 5.46′ |
Frequently Asked Questions
What type of star is HIP 16782?
HIP 16782 is a Class B — B-type (Blue-White) star.
How far is HIP 16782 from Earth?
HIP 16782 is approximately 579.3 light-years from Earth.
Can you see HIP 16782 with the naked eye?
With an apparent magnitude of 6.89, HIP 16782 is not visible to the naked eye.
What constellation is HIP 16782 in?
HIP 16782 is located in the constellation Perseus.