HIP 104979
HIP 104979 is a A-type (White) star located in the constellation Pegasus.
Located approximately 600.7 light-years from Earth, HIP 104979 resides within the broader disk of our Milky Way galaxy.
HIP 104979 is classified as a spectral class A star (A-type (White)) on the Harvard spectral classification system.
HIP 104979 has an apparent magnitude of +8.45, 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 +0.161.
Propriétés physiques
| Classe Spectrale | Class A — A-type (White) |
| Indice de couleur (B−V) | 0,161 |
Observation
| Magnitude Apparente | +8.45 |
| Magnitude Absolue | 2,12 |
| Distance | 601 ly |
| Constellation | Pegasus |
Position
| Ascension droite | 21h 15,76m |
| Déclinaison | 15° 19,88′ |
Questions fréquentes
What type of star is HIP 104979?
HIP 104979 is a Class A — A-type (White) star.
How far is HIP 104979 from Earth?
HIP 104979 is approximately 600.7 light-years from Earth.
Can you see HIP 104979 with the naked eye?
With an apparent magnitude of 8.45, HIP 104979 is not visible to the naked eye.
What constellation is HIP 104979 in?
HIP 104979 is located in the constellation Pegasus.