HIP 34579
HIP 34579 is a B-type (Blue-White) star located in the constellation Canis Major.
At a distance of roughly 1,843 light-years, HIP 34579 is a distant star lying deep within the Milky Way galaxy.
HIP 34579 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
With an apparent magnitude of +5.69, HIP 34579 sits near the limit of naked-eye visibility. It can be glimpsed without optical aid under dark skies, but binoculars will make observation much easier. Observers will note its blue hue, which corresponds to a B-V color index of -0.158.
Physikalische Eigenschaften
| Spektralklasse | Class B — B-type (Blue-White) |
| Farbindex (B−V) | -0,158 |
Beobachtung
| Scheinbare Helligkeit | +5.69 |
| Absolute Helligkeit | -3,07 |
| Entfernung | 1,843 ly |
| Sternbild | Canis Major |
Position
| Rektaszension | 7h 9,72m |
| Deklination | -25° 13,86′ |
Häufig gestellte Fragen
What type of star is HIP 34579?
HIP 34579 is a Class B — B-type (Blue-White) star.
How far is HIP 34579 from Earth?
HIP 34579 is approximately 1,842.7 light-years from Earth.
Can you see HIP 34579 with the naked eye?
With an apparent magnitude of 5.69, HIP 34579 is visible to the naked eye.
What constellation is HIP 34579 in?
HIP 34579 is located in the constellation Canis Major.