HIP 40485
HIP 40485 is a K-type (Orange) star.
At a distance of roughly 1,656 light-years, HIP 40485 is a distant star lying deep within the Milky Way galaxy.
HIP 40485 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 40485 has an apparent magnitude of +6.15, 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 +1.549.
Propriétés physiques
| Classe Spectrale | K Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,549 |
Observation
| Magnitude Apparente | +6.15 |
| Magnitude Absolue | -2,38 |
| Distance | 1,656 ly |
Position
| Ascension droite | 8h 15,98m |
| Déclinaison | -35° 54,19′ |
Frequently Asked Questions
What type of star is HIP 40485?
HIP 40485 is a Class K — K-type (Orange) star.
How far is HIP 40485 from Earth?
HIP 40485 is approximately 1,655.6 light-years from Earth.
Can you see HIP 40485 with the naked eye?
With an apparent magnitude of 6.15, HIP 40485 is not visible to the naked eye.