HIP 43399
HIP 43399 is a K-type (Orange) star located in the constellation Ursa Major.
At a distance of roughly 1,822 light-years, HIP 43399 is a distant star lying deep within the Milky Way galaxy.
HIP 43399 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 43399 has an apparent magnitude of +9.33, 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 red hue, which corresponds to a B-V color index of +1.401.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.401 |
Observation
| Apparent Magnitude | +9.33 |
| Absolute Magnitude | 0.59 |
| Distance | 1,822 ly |
| Constellation | Ursa Major |
Position
| Right Ascension | 8h 50.42m |
| Declination | 64° 51.87′ |
Frequently Asked Questions
What type of star is HIP 43399?
HIP 43399 is a Class K — K-type (Orange) star.
How far is HIP 43399 from Earth?
HIP 43399 is approximately 1,822.1 light-years from Earth.
Can you see HIP 43399 with the naked eye?
With an apparent magnitude of 9.33, HIP 43399 is not visible to the naked eye.
What constellation is HIP 43399 in?
HIP 43399 is located in the constellation Ursa Major.