HIP 44419
HIP 44419 is a K-type (Orange) star.
At a distance of roughly 2,528 light-years, HIP 44419 is a distant star lying deep within the Milky Way galaxy.
HIP 44419 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 44419 has an apparent magnitude of +8.41, 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 +1.514.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 1.514 |
Observation
| Apparent Magnitude | +8.41 |
| Absolute Magnitude | -1.04 |
| Distance | 2,528 ly |
Position
| Right Ascension | 9h 2.98m |
| Declination | -58° 23.67′ |
Frequently Asked Questions
What type of star is HIP 44419?
HIP 44419 is a Class K — K-type (Orange) star.
How far is HIP 44419 from Earth?
HIP 44419 is approximately 2,528.3 light-years from Earth.
Can you see HIP 44419 with the naked eye?
With an apparent magnitude of 8.41, HIP 44419 is not visible to the naked eye.