HIP 4230
HIP 4230 is a K-type (Orange) star.
At a distance of roughly 1,717 light-years, HIP 4230 is a distant star lying deep within the Milky Way galaxy.
HIP 4230 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 4230 has an apparent magnitude of +9.53, 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 orange hue, which corresponds to a B-V color index of +1.203.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.203 |
Observation
| Apparent Magnitude | +9.53 |
| Absolute Magnitude | 0.92 |
| Distance | 1,717 ly |
Position
| Right Ascension | 0h 53.96m |
| Declination | -41° 20.70′ |
Frequently Asked Questions
What type of star is HIP 4230?
HIP 4230 is a Class K — K-type (Orange) star.
How far is HIP 4230 from Earth?
HIP 4230 is approximately 1,716.6 light-years from Earth.
Can you see HIP 4230 with the naked eye?
With an apparent magnitude of 9.53, HIP 4230 is not visible to the naked eye.