HIP 9018
HIP 9018 is a G-type (Yellow) star located in the constellation Perseus.
Located approximately 310.9 light-years from Earth, HIP 9018 resides within the broader disk of our Milky Way galaxy.
HIP 9018 is classified as a spectral class G star (G-type (Yellow)) on the Harvard spectral classification system.
HIP 9018 has an apparent magnitude of +9.04, 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 white hue, which corresponds to a B-V color index of +0.526.
Physikalische Eigenschaften
| Spektralklasse | Class G — G-type (Yellow) |
| Farbindex (B−V) | 0,526 |
Beobachtung
| Scheinbare Helligkeit | +9.04 |
| Absolute Helligkeit | 4,14 |
| Entfernung | 311 ly |
| Sternbild | Perseus |
Position
| Rektaszension | 1h 56,13m |
| Deklination | 57° 58,03′ |
Häufig gestellte Fragen
What type of star is HIP 9018?
HIP 9018 is a Class G — G-type (Yellow) star.
How far is HIP 9018 from Earth?
HIP 9018 is approximately 310.9 light-years from Earth.
Can you see HIP 9018 with the naked eye?
With an apparent magnitude of 9.04, HIP 9018 is not visible to the naked eye.
What constellation is HIP 9018 in?
HIP 9018 is located in the constellation Perseus.