HIP 17485
HIP 17485 is a K-type (Orange) star.
At a distance of roughly 2,265 light-years, HIP 17485 is a distant star lying deep within the Milky Way galaxy.
HIP 17485 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 17485 has an apparent magnitude of +8.28, 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 +1.337.
Physikalische Eigenschaften
| Spektralklasse | K Class K — K-type (Orange) |
| Farbindex (B−V) | 1,337 |
Beobachtung
| Scheinbare Helligkeit | +8.28 |
| Absolute Helligkeit | -0,93 |
| Entfernung | 2,265 ly |
Position
| Rektaszension | 3h 44,77m |
| Deklination | -54° 9,98′ |
Frequently Asked Questions
What type of star is HIP 17485?
HIP 17485 is a Class K — K-type (Orange) star.
How far is HIP 17485 from Earth?
HIP 17485 is approximately 2,265.0 light-years from Earth.
Can you see HIP 17485 with the naked eye?
With an apparent magnitude of 8.28, HIP 17485 is not visible to the naked eye.