HIP 18212
HIP 18212 is a K-type (Orange) star located in the constellation Perseus.
Located approximately 393.9 light-years from Earth, HIP 18212 resides within the broader disk of our Milky Way galaxy.
HIP 18212 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
With an apparent magnitude of +5.76, HIP 18212 sits near the limit of naked-eye visibility. It can be glimpsed without optical aid under dark skies, but binoculars will make observation much easier. Observers will note its orange hue, which corresponds to a B-V color index of +1.040.
Physikalische Eigenschaften
| Spektralklasse | Class K — K-type (Orange) |
| Farbindex (B−V) | 1,040 |
Beobachtung
| Scheinbare Helligkeit | +5.76 |
| Absolute Helligkeit | 0,35 |
| Entfernung | 394 ly |
| Sternbild | Perseus |
Position
| Rektaszension | 3h 53,64m |
| Deklination | 48° 39,03′ |
Häufig gestellte Fragen
What type of star is HIP 18212?
HIP 18212 is a Class K — K-type (Orange) star.
How far is HIP 18212 from Earth?
HIP 18212 is approximately 393.9 light-years from Earth.
Can you see HIP 18212 with the naked eye?
With an apparent magnitude of 5.76, HIP 18212 is visible to the naked eye.
What constellation is HIP 18212 in?
HIP 18212 is located in the constellation Perseus.