HIP 39699
HIP 39699 is a B-type (Blue-White) star.
At a distance of roughly 1,182 light-years, HIP 39699 is a distant star lying deep within the Milky Way galaxy.
HIP 39699 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 39699 has an apparent magnitude of +8.01, 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 -0.020.
Physical Properties
| Spectral Class | Class B — B-type (Blue-White) |
| Color Index (B−V) | -0.020 |
Observation
| Apparent Magnitude | +8.01 |
| Absolute Magnitude | 0.22 |
| Distance | 1,182 ly |
Position
| Right Ascension | 8h 6.84m |
| Declination | -47° 33.63′ |
Frequently Asked Questions
What type of star is HIP 39699?
HIP 39699 is a Class B — B-type (Blue-White) star.
How far is HIP 39699 from Earth?
HIP 39699 is approximately 1,181.7 light-years from Earth.
Can you see HIP 39699 with the naked eye?
With an apparent magnitude of 8.01, HIP 39699 is not visible to the naked eye.