HIP 17102
HIP 17102 is a K-type (Orange) star located in the constellation Perseus.
Located approximately 141.2 light-years from Earth, HIP 17102 resides within the broader disk of our Milky Way galaxy.
HIP 17102 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 17102 has an apparent magnitude of +9.03, 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 +1.090.
Physikalische Eigenschaften
| Spektralklasse | Class K — K-type (Orange) |
| Farbindex (B−V) | 1,090 |
Beobachtung
| Scheinbare Helligkeit | +9.03 |
| Absolute Helligkeit | 5,85 |
| Entfernung | 141 ly |
| Sternbild | Perseus |
Position
| Rektaszension | 3h 39,82m |
| Deklination | 33° 28,41′ |
Häufig gestellte Fragen
What type of star is HIP 17102?
HIP 17102 is a Class K — K-type (Orange) star.
How far is HIP 17102 from Earth?
HIP 17102 is approximately 141.2 light-years from Earth.
Can you see HIP 17102 with the naked eye?
With an apparent magnitude of 9.03, HIP 17102 is not visible to the naked eye.
What constellation is HIP 17102 in?
HIP 17102 is located in the constellation Perseus.