HIP 17247
HIP 17247 is a K-type (Orange) star.
At a distance of roughly 1,726 light-years, HIP 17247 is a distant star lying deep within the Milky Way galaxy.
HIP 17247 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 17247 has an apparent magnitude of +9.06, 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 +1.322.
Propriétés physiques
| Classe Spectrale | K Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,322 |
Observation
| Magnitude Apparente | +9.06 |
| Magnitude Absolue | 0,44 |
| Distance | 1,726 ly |
Position
| Ascension droite | 3h 41,62m |
| Déclinaison | -20° 22,06′ |
Frequently Asked Questions
What type of star is HIP 17247?
HIP 17247 is a Class K — K-type (Orange) star.
How far is HIP 17247 from Earth?
HIP 17247 is approximately 1,725.7 light-years from Earth.
Can you see HIP 17247 with the naked eye?
With an apparent magnitude of 9.06, HIP 17247 is not visible to the naked eye.