HIP 40945
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HIP 40945 is a K-type (Orange) star.
At a distance of roughly 1,007 light-years, HIP 40945 is a distant star lying deep within the Milky Way galaxy.
HIP 40945 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
With an apparent magnitude of +4.83, HIP 40945 sits near the limit of naked-eye visibility. It can be glimpsed without optical aid under dark skies, but binoculars will make observation much easier. Observers will note its red hue, which corresponds to a B-V color index of +1.419.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 1.419 |
Observation
| Apparent Magnitude | +4.83 |
| Absolute Magnitude | -2.62 |
| Distance | 1,007 ly |
Position
| Right Ascension | 8h 21.38m |
| Declination | -33° 3.26′ |
Frequently Asked Questions
What type of star is HIP 40945?
HIP 40945 is a Class K — K-type (Orange) star.
How far is HIP 40945 from Earth?
HIP 40945 is approximately 1,006.6 light-years from Earth.
Can you see HIP 40945 with the naked eye?
With an apparent magnitude of 4.83, HIP 40945 is visible to the naked eye.