HIP 18125
HIP 18125 is a M-type (Red) star located in the constellation Perseus.
At a distance of roughly 2,416 light-years, HIP 18125 is a distant star lying deep within the Milky Way galaxy.
HIP 18125 is classified as a spectral class M star (M-type (Red)) on the Harvard spectral classification system.
HIP 18125 has an apparent magnitude of +8.76, 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 red hue, which corresponds to a B-V color index of +2.153.
Physikalische Eigenschaften
| Spektralklasse | Class M — M-type (Red) |
| Farbindex (B−V) | 2,153 |
Beobachtung
| Scheinbare Helligkeit | +8.76 |
| Absolute Helligkeit | -0,59 |
| Entfernung | 2,416 ly |
| Sternbild | Perseus |
Position
| Rektaszension | 3h 52,57m |
| Deklination | 48° 6,67′ |
Häufig gestellte Fragen
What type of star is HIP 18125?
HIP 18125 is a Class M — M-type (Red) star.
How far is HIP 18125 from Earth?
HIP 18125 is approximately 2,416.0 light-years from Earth.
Can you see HIP 18125 with the naked eye?
With an apparent magnitude of 8.76, HIP 18125 is not visible to the naked eye.
What constellation is HIP 18125 in?
HIP 18125 is located in the constellation Perseus.