HIP 30475
HIP 30475 is a K-type (Orange) star.
At a distance of roughly 2,219 light-years, HIP 30475 is a distant star lying deep within the Milky Way galaxy.
HIP 30475 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 30475 has an apparent magnitude of +9.10, 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 +1.254.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 1.254 |
Observation
| Apparent Magnitude | +9.10 |
| Absolute Magnitude | -0.06 |
| Distance | 2,219 ly |
Position
| Right Ascension | 6h 24.40m |
| Declination | -37° 32.03′ |
Frequently Asked Questions
What type of star is HIP 30475?
HIP 30475 is a Class K — K-type (Orange) star.
How far is HIP 30475 from Earth?
HIP 30475 is approximately 2,218.8 light-years from Earth.
Can you see HIP 30475 with the naked eye?
With an apparent magnitude of 9.10, HIP 30475 is not visible to the naked eye.