HIP 18419
HIP 18419 is a K-type (Orange) star.
At a distance of roughly 1,965 light-years, HIP 18419 is a distant star lying deep within the Milky Way galaxy.
HIP 18419 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 18419 has an apparent magnitude of +8.33, 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 +1.534.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 1.534 |
Observation
| Apparent Magnitude | +8.33 |
| Absolute Magnitude | -0.57 |
| Distance | 1,965 ly |
Position
| Right Ascension | 3h 56.28m |
| Declination | -5° 9.18′ |
Frequently Asked Questions
What type of star is HIP 18419?
HIP 18419 is a Class K — K-type (Orange) star.
How far is HIP 18419 from Earth?
HIP 18419 is approximately 1,964.8 light-years from Earth.
Can you see HIP 18419 with the naked eye?
With an apparent magnitude of 8.33, HIP 18419 is not visible to the naked eye.