HIP 44407
HIP 44407 is a K-type (Orange) star.
At a distance of roughly 2,965 light-years, HIP 44407 is a distant star lying deep within the Milky Way galaxy.
HIP 44407 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 44407 has an apparent magnitude of +9.07, 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 yellow hue, which corresponds to a B-V color index of +0.962.
Propriedades físicas
| Classe Espectral | K Class K — K-type (Orange) |
| Índice de cor (B−V) | 0,962 |
Observação
| Magnitude Aparente | +9.07 |
| Magnitude Absoluta | -0,72 |
| Distância | 2,965 ly |
Posição
| Ascensão reta | 9h 2,75m |
| Declinação | -9° 23,50′ |
Frequently Asked Questions
What type of star is HIP 44407?
HIP 44407 is a Class K — K-type (Orange) star.
How far is HIP 44407 from Earth?
HIP 44407 is approximately 2,965.0 light-years from Earth.
Can you see HIP 44407 with the naked eye?
With an apparent magnitude of 9.07, HIP 44407 is not visible to the naked eye.