HIP 24890
HIP 24890 is a K-type (Orange) star.
At a distance of roughly 1,431 light-years, HIP 24890 is a distant star lying deep within the Milky Way galaxy.
HIP 24890 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 24890 has an apparent magnitude of +7.36, 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 red hue, which corresponds to a B-V color index of +1.695.
Propriedades físicas
| Classe Espectral | K Class K — K-type (Orange) |
| Índice de cor (B−V) | 1,695 |
Observação
| Magnitude Aparente | +7.36 |
| Magnitude Absoluta | -0,85 |
| Distância | 1,431 ly |
Posição
| Ascensão reta | 5h 20,10m |
| Declinação | 39° 20,60′ |
Frequently Asked Questions
What type of star is HIP 24890?
HIP 24890 is a Class K — K-type (Orange) star.
How far is HIP 24890 from Earth?
HIP 24890 is approximately 1,430.5 light-years from Earth.
Can you see HIP 24890 with the naked eye?
With an apparent magnitude of 7.36, HIP 24890 is not visible to the naked eye.