HIP 79458
HIP 79458 is a B-type (Blue-White) star located in the constellation Scorpius.
HIP 79458 is an extraordinarily remote star, situated approximately 326,156 light-years from Earth.
HIP 79458 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
At an apparent magnitude of +10.41, HIP 79458 is a faint star that requires a telescope to observe. It is invisible to the naked eye and too dim for most binoculars. Observers will note its blue-white hue, which corresponds to a B-V color index of +0.093.
Physikalische Eigenschaften
| Spektralklasse | Class B — B-type (Blue-White) |
| Farbindex (B−V) | 0,093 |
Beobachtung
| Scheinbare Helligkeit | +10.41 |
| Absolute Helligkeit | -9,59 |
| Entfernung | 326,156 ly |
| Sternbild | Scorpius |
Position
| Rektaszension | 16h 12,91m |
| Deklination | -34° 39,34′ |
Häufig gestellte Fragen
What type of star is HIP 79458?
HIP 79458 is a Class B — B-type (Blue-White) star.
How far is HIP 79458 from Earth?
HIP 79458 is approximately 326,156.0 light-years from Earth.
Can you see HIP 79458 with the naked eye?
With an apparent magnitude of 10.41, HIP 79458 is not visible to the naked eye.
What constellation is HIP 79458 in?
HIP 79458 is located in the constellation Scorpius.