HIP 15770
HIP 15770 is a B-type (Blue-White) star located in the constellation Perseus.
Located approximately 541.8 light-years from Earth, HIP 15770 resides within the broader disk of our Milky Way galaxy.
HIP 15770 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
With an apparent magnitude of +5.32, HIP 15770 sits near the limit of naked-eye visibility. It can be glimpsed without optical aid under dark skies, but binoculars will make observation much easier. Observers will note its blue hue, which corresponds to a B-V color index of -0.076.
Propiedades físicas
| Clase Espectral | Class B — B-type (Blue-White) |
| Índice de color (B−V) | -0,076 |
Observación
| Magnitud Aparente | +5.32 |
| Magnitud Absoluta | -0,78 |
| Distancia | 542 ly |
| Constelación | Perseus |
Posición
| Ascensión recta | 3h 23,22m |
| Declinación | 49° 12,80′ |
Preguntas frecuentes
What type of star is HIP 15770?
HIP 15770 is a Class B — B-type (Blue-White) star.
How far is HIP 15770 from Earth?
HIP 15770 is approximately 541.8 light-years from Earth.
Can you see HIP 15770 with the naked eye?
With an apparent magnitude of 5.32, HIP 15770 is visible to the naked eye.
What constellation is HIP 15770 in?
HIP 15770 is located in the constellation Perseus.