HIP 52490
HIP 52490 is a K-type (Orange) star.
At a distance of roughly 1,106 light-years, HIP 52490 is a distant star lying deep within the Milky Way galaxy.
HIP 52490 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 52490 has an apparent magnitude of +9.32, 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 +1.283.
Propriedades físicas
| Classe Espectral | K Class K — K-type (Orange) |
| Índice de cor (B−V) | 1,283 |
Observação
| Magnitude Aparente | +9.32 |
| Magnitude Absoluta | 1,67 |
| Distância | 1,106 ly |
Posição
| Ascensão reta | 10h 43,88m |
| Declinação | -13° 52,39′ |
Frequently Asked Questions
What type of star is HIP 52490?
HIP 52490 is a Class K — K-type (Orange) star.
How far is HIP 52490 from Earth?
HIP 52490 is approximately 1,105.6 light-years from Earth.
Can you see HIP 52490 with the naked eye?
With an apparent magnitude of 9.32, HIP 52490 is not visible to the naked eye.