HIP 47457
HIP 47457 is a A-type (White) star.
At a distance of roughly 1,240 light-years, HIP 47457 is a distant star lying deep within the Milky Way galaxy.
HIP 47457 is classified as a spectral class A star (A-type (White)) on the Harvard spectral classification system.
HIP 47457 has an apparent magnitude of +8.64, 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 blue-white hue, which corresponds to a B-V color index of +0.046.
Propriétés physiques
| Classe Spectrale | A Class A — A-type (White) |
| Indice de couleur (B−V) | 0,046 |
Observation
| Magnitude Apparente | +8.64 |
| Magnitude Absolue | 0,74 |
| Distance | 1,240 ly |
Position
| Ascension droite | 9h 40,45m |
| Déclinaison | -54° 23,09′ |
Frequently Asked Questions
What type of star is HIP 47457?
HIP 47457 is a Class A — A-type (White) star.
How far is HIP 47457 from Earth?
HIP 47457 is approximately 1,240.1 light-years from Earth.
Can you see HIP 47457 with the naked eye?
With an apparent magnitude of 8.64, HIP 47457 is not visible to the naked eye.