HIP 13218
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HIP 13218 is a M-type (Red) star.
HIP 13218 lies approximately 42.2 light-years from Earth, placing it within the Sun's local stellar neighborhood. This relatively short cosmic distance means the light reaching us today departed the star only about 42 years ago.
HIP 13218 is classified as a spectral class M star (M-type (Red)) on the Harvard spectral classification system.
At an apparent magnitude of +10.72, HIP 13218 is a faint star that requires a telescope to observe. It is invisible to the naked eye and too dim for most binoculars. Observers will note its red hue, which corresponds to a B-V color index of +1.510.
Propriedades físicas
| Classe Espectral | M Class M — M-type (Red) |
| Índice de cor (B−V) | 1,510 |
Observação
| Magnitude Aparente | +10.72 |
| Magnitude Absoluta | 10,16 |
| Distância | 42.2 ly |
Posição
| Ascensão reta | 2h 50,16m |
| Declinação | -53° 8,34′ |