HIP 62890
HIP 62890 is a K-type (Orange) star located in the constellation Centaurus.
Located approximately 845.0 light-years from Earth, HIP 62890 resides within the broader disk of our Milky Way galaxy.
HIP 62890 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 62890 has an apparent magnitude of +8.41, 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 orange hue, which corresponds to a B-V color index of +1.180.
Propriedades físicas
| Classe Espectral | K Class K — K-type (Orange) |
| Índice de cor (B−V) | 1,180 |
Observação
| Magnitude Aparente | +8.41 |
| Magnitude Absoluta | 1,34 |
| Distância | 845 ly |
| Constelação | Centaurus |
Posição
| Ascensão reta | 12h 53,33m |
| Declinação | -31° 20,93′ |
Frequently Asked Questions
What type of star is HIP 62890?
HIP 62890 is a Class K — K-type (Orange) star.
How far is HIP 62890 from Earth?
HIP 62890 is approximately 845.0 light-years from Earth.
Can you see HIP 62890 with the naked eye?
With an apparent magnitude of 8.41, HIP 62890 is not visible to the naked eye.
What constellation is HIP 62890 in?
HIP 62890 is located in the constellation Centaurus.