HIP 17200
HIP 17200 is a B-type (Blue-White) star.
At a distance of roughly 1,853 light-years, HIP 17200 is a distant star lying deep within the Milky Way galaxy.
HIP 17200 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 17200 has an apparent magnitude of +9.34, 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 +0.502.
Physical Properties
| Spectral Class | B Class B — B-type (Blue-White) |
| Color Index (B−V) | 0.502 |
Observation
| Apparent Magnitude | +9.34 |
| Absolute Magnitude | 0.57 |
| Distance | 1,853 ly |
Position
| Right Ascension | 3h 41.05m |
| Declination | 54° 0.07′ |
Frequently Asked Questions
What type of star is HIP 17200?
HIP 17200 is a Class B — B-type (Blue-White) star.
How far is HIP 17200 from Earth?
HIP 17200 is approximately 1,853.2 light-years from Earth.
Can you see HIP 17200 with the naked eye?
With an apparent magnitude of 9.34, HIP 17200 is not visible to the naked eye.