HIP 18789
HIP 18789 is a K-type (Orange) star located in the constellation Perseus.
Located approximately 210.3 light-years from Earth, HIP 18789 resides within the broader disk of our Milky Way galaxy.
HIP 18789 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 18789 has an apparent magnitude of +9.24, 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 yellow hue, which corresponds to a B-V color index of +0.845.
Physikalische Eigenschaften
| Spektralklasse | Class K — K-type (Orange) |
| Farbindex (B−V) | 0,845 |
Beobachtung
| Scheinbare Helligkeit | +9.24 |
| Absolute Helligkeit | 5,19 |
| Entfernung | 210 ly |
| Sternbild | Perseus |
Position
| Rektaszension | 4h 1,55m |
| Deklination | 38° 40,07′ |
Häufig gestellte Fragen
What type of star is HIP 18789?
HIP 18789 is a Class K — K-type (Orange) star.
How far is HIP 18789 from Earth?
HIP 18789 is approximately 210.3 light-years from Earth.
Can you see HIP 18789 with the naked eye?
With an apparent magnitude of 9.24, HIP 18789 is not visible to the naked eye.
What constellation is HIP 18789 in?
HIP 18789 is located in the constellation Perseus.