HIP 32599
HIP 32599 is a K-type (Orange) star.
At a distance of roughly 1,400 light-years, HIP 32599 is a distant star lying deep within the Milky Way galaxy.
HIP 32599 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 32599 has an apparent magnitude of +9.09, 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 +1.510.
Physikalische Eigenschaften
| Spektralklasse | K Class K — K-type (Orange) |
| Farbindex (B−V) | 1,510 |
Beobachtung
| Scheinbare Helligkeit | +9.09 |
| Absolute Helligkeit | 0,93 |
| Entfernung | 1,400 ly |
Position
| Rektaszension | 6h 48,06m |
| Deklination | 72° 49,16′ |
Frequently Asked Questions
What type of star is HIP 32599?
HIP 32599 is a Class K — K-type (Orange) star.
How far is HIP 32599 from Earth?
HIP 32599 is approximately 1,399.8 light-years from Earth.
Can you see HIP 32599 with the naked eye?
With an apparent magnitude of 9.09, HIP 32599 is not visible to the naked eye.