HIP 53477
HIP 53477 is a K-type (Orange) star.
At a distance of roughly 1,080 light-years, HIP 53477 is a distant star lying deep within the Milky Way galaxy.
HIP 53477 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 53477 has an apparent magnitude of +8.31, 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 orange hue, which corresponds to a B-V color index of +1.046.
Physikalische Eigenschaften
| Spektralklasse | K Class K — K-type (Orange) |
| Farbindex (B−V) | 1,046 |
Beobachtung
| Scheinbare Helligkeit | +8.31 |
| Absolute Helligkeit | 0,71 |
| Entfernung | 1,080 ly |
Position
| Rektaszension | 10h 56,38m |
| Deklination | -70° 26,95′ |
Frequently Asked Questions
What type of star is HIP 53477?
HIP 53477 is a Class K — K-type (Orange) star.
How far is HIP 53477 from Earth?
HIP 53477 is approximately 1,080.0 light-years from Earth.
Can you see HIP 53477 with the naked eye?
With an apparent magnitude of 8.31, HIP 53477 is not visible to the naked eye.