HIP 34099
HIP 34099 is a B-type (Blue-White) star located in the constellation Canis Major.
At a distance of roughly 1,289 light-years, HIP 34099 is a distant star lying deep within the Milky Way galaxy.
HIP 34099 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 34099 has an apparent magnitude of +7.64, 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 hue, which corresponds to a B-V color index of -0.009.
Propriedades físicas
| Classe Espectral | Class B — B-type (Blue-White) |
| Índice de cor (B−V) | -0,009 |
Observação
| Magnitude Aparente | +7.64 |
| Magnitude Absoluta | -0,34 |
| Distância | 1,289 ly |
| Constelação | Canis Major |
Posição
| Ascensão reta | 7h 4,23m |
| Declinação | -21° 15,96′ |
Perguntas frequentes
What type of star is HIP 34099?
HIP 34099 is a Class B — B-type (Blue-White) star.
How far is HIP 34099 from Earth?
HIP 34099 is approximately 1,289.2 light-years from Earth.
Can you see HIP 34099 with the naked eye?
With an apparent magnitude of 7.64, HIP 34099 is not visible to the naked eye.
What constellation is HIP 34099 in?
HIP 34099 is located in the constellation Canis Major.