HIP 7419
HIP 7419 is a K-type (Orange) star located in the constellation Perseus.
Located approximately 886.3 light-years from Earth, HIP 7419 resides within the broader disk of our Milky Way galaxy.
HIP 7419 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 7419 has an apparent magnitude of +7.40, 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 +1.533.
Propiedades físicas
| Clase Espectral | Class K — K-type (Orange) |
| Índice de color (B−V) | 1,533 |
Observación
| Magnitud Aparente | +7.40 |
| Magnitud Absoluta | 0,23 |
| Distancia | 886 ly |
| Constelación | Perseus |
Posición
| Ascensión recta | 1h 35,62m |
| Declinación | 52° 9,83′ |
Preguntas frecuentes
What type of star is HIP 7419?
HIP 7419 is a Class K — K-type (Orange) star.
How far is HIP 7419 from Earth?
HIP 7419 is approximately 886.3 light-years from Earth.
Can you see HIP 7419 with the naked eye?
With an apparent magnitude of 7.40, HIP 7419 is not visible to the naked eye.
What constellation is HIP 7419 in?
HIP 7419 is located in the constellation Perseus.