HIP 47509
HIP 47509 is a K-type (Orange) star.
At a distance of roughly 1,129 light-years, HIP 47509 is a distant star lying deep within the Milky Way galaxy.
HIP 47509 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 47509 has an apparent magnitude of +8.35, 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 +1.263.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 1.263 |
Observation
| Apparent Magnitude | +8.35 |
| Absolute Magnitude | 0.65 |
| Distance | 1,129 ly |
Position
| Right Ascension | 9h 41.16m |
| Declination | -59° 8.33′ |
Frequently Asked Questions
What type of star is HIP 47509?
HIP 47509 is a Class K — K-type (Orange) star.
How far is HIP 47509 from Earth?
HIP 47509 is approximately 1,128.6 light-years from Earth.
Can you see HIP 47509 with the naked eye?
With an apparent magnitude of 8.35, HIP 47509 is not visible to the naked eye.