HIP 40495
HIP 40495 is a B-type (Blue-White) star.
At a distance of roughly 1,062 light-years, HIP 40495 is a distant star lying deep within the Milky Way galaxy.
HIP 40495 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 40495 has an apparent magnitude of +7.83, 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 -0.034.
Physical Properties
| Spectral Class | B Class B — B-type (Blue-White) |
| Color Index (B−V) | -0.034 |
Observation
| Apparent Magnitude | +7.83 |
| Absolute Magnitude | 0.27 |
| Distance | 1,062 ly |
Position
| Right Ascension | 8h 16.09m |
| Declination | -57° 16.15′ |
Frequently Asked Questions
What type of star is HIP 40495?
HIP 40495 is a Class B — B-type (Blue-White) star.
How far is HIP 40495 from Earth?
HIP 40495 is approximately 1,062.4 light-years from Earth.
Can you see HIP 40495 with the naked eye?
With an apparent magnitude of 7.83, HIP 40495 is not visible to the naked eye.