HIP 104297
HIP 104297 is a B-type (Blue-White) star.
Located approximately 391.1 light-years from Earth, HIP 104297 resides within the broader disk of our Milky Way galaxy.
HIP 104297 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 104297 has an apparent magnitude of +6.18, 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 -0.035.
Physical Properties
| Spectral Class | Class B — B-type (Blue-White) |
| Color Index (B−V) | -0.035 |
Observation
| Apparent Magnitude | +6.18 |
| Absolute Magnitude | 0.79 |
| Distance | 391 ly |
Position
| Right Ascension | 21h 7.74m |
| Declination | -17° 27.35′ |
Frequently Asked Questions
What type of star is HIP 104297?
HIP 104297 is a Class B — B-type (Blue-White) star.
How far is HIP 104297 from Earth?
HIP 104297 is approximately 391.1 light-years from Earth.
Can you see HIP 104297 with the naked eye?
With an apparent magnitude of 6.18, HIP 104297 is not visible to the naked eye.