HIP 32618
HIP 32618 is a K-type (Orange) star.
At a distance of roughly 1,400 light-years, HIP 32618 is a distant star lying deep within the Milky Way galaxy.
HIP 32618 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 32618 has an apparent magnitude of +8.26, 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 +1.445.
Propriétés physiques
| Classe Spectrale | K Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,445 |
Observation
| Magnitude Apparente | +8.26 |
| Magnitude Absolue | 0,10 |
| Distance | 1,400 ly |
Position
| Ascension droite | 6h 48,33m |
| Déclinaison | -56° 19,08′ |
Frequently Asked Questions
What type of star is HIP 32618?
HIP 32618 is a Class K — K-type (Orange) star.
How far is HIP 32618 from Earth?
HIP 32618 is approximately 1,399.8 light-years from Earth.
Can you see HIP 32618 with the naked eye?
With an apparent magnitude of 8.26, HIP 32618 is not visible to the naked eye.