HIP 75711
HIP 75711 is a B-type (Blue-White) star.
At a distance of roughly 2,490 light-years, HIP 75711 is a distant star lying deep within the Milky Way galaxy.
HIP 75711 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 75711 has an apparent magnitude of +7.48, 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 +0.021.
Physical Properties
| Spectral Class | B Class B — B-type (Blue-White) |
| Color Index (B−V) | 0.021 |
Observation
| Apparent Magnitude | +7.48 |
| Absolute Magnitude | -1.93 |
| Distance | 2,490 ly |
Position
| Right Ascension | 15h 28.04m |
| Declination | -33° 32.71′ |
Frequently Asked Questions
What type of star is HIP 75711?
HIP 75711 is a Class B — B-type (Blue-White) star.
How far is HIP 75711 from Earth?
HIP 75711 is approximately 2,489.7 light-years from Earth.
Can you see HIP 75711 with the naked eye?
With an apparent magnitude of 7.48, HIP 75711 is not visible to the naked eye.