HIP 5887
HIP 5887 is a A-type (White) star located in the constellation Cassiopeia.
At a distance of roughly 1,299 light-years, HIP 5887 is a distant star lying deep within the Milky Way galaxy.
HIP 5887 is classified as a spectral class A star (A-type (White)) on the Harvard spectral classification system.
HIP 5887 has an apparent magnitude of +8.80, 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 +0.013.
Propriedades físicas
| Classe Espectral | Class A — A-type (White) |
| Índice de cor (B−V) | 0,013 |
Observação
| Magnitude Aparente | +8.80 |
| Magnitude Absoluta | 0,80 |
| Distância | 1,299 ly |
| Constelação | Cassiopeia |
Posição
| Ascensão reta | 1h 15,60m |
| Declinação | 57° 9,49′ |
Perguntas frequentes
What type of star is HIP 5887?
HIP 5887 is a Class A — A-type (White) star.
How far is HIP 5887 from Earth?
HIP 5887 is approximately 1,299.4 light-years from Earth.
Can you see HIP 5887 with the naked eye?
With an apparent magnitude of 8.80, HIP 5887 is not visible to the naked eye.
What constellation is HIP 5887 in?
HIP 5887 is located in the constellation Cassiopeia.