HIP 104485
HIP 104485 is a B-type (Blue-White) star located in the constellation Cygnus.
At a distance of roughly 3,048 light-years, HIP 104485 is a distant star lying deep within the Milky Way galaxy.
HIP 104485 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 104485 has an apparent magnitude of +9.03, 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 +0.125.
Physical Properties
| Spectral Class | Class B — B-type (Blue-White) |
| Color Index (B−V) | 0.125 |
Observation
| Apparent Magnitude | +9.03 |
| Absolute Magnitude | -0.82 |
| Distance | 3,048 ly |
| Constellation | Cygnus |
Position
| Right Ascension | 21h 9.99m |
| Declination | 47° 44.73′ |
Frequently Asked Questions
What type of star is HIP 104485?
HIP 104485 is a Class B — B-type (Blue-White) star.
How far is HIP 104485 from Earth?
HIP 104485 is approximately 3,048.2 light-years from Earth.
Can you see HIP 104485 with the naked eye?
With an apparent magnitude of 9.03, HIP 104485 is not visible to the naked eye.
What constellation is HIP 104485 in?
HIP 104485 is located in the constellation Cygnus.