HIP 94250
HIP 94250 is a B-type (Blue-White) star located in the constellation Aquila.
At a distance of roughly 1,365 light-years, HIP 94250 is a distant star lying deep within the Milky Way galaxy.
HIP 94250 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 94250 has an apparent magnitude of +7.08, 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 blue-white hue, which corresponds to a B-V color index of +0.060.
Propiedades físicas
| Clase Espectral | Class B — B-type (Blue-White) |
| Índice de color (B−V) | 0,060 |
Observación
| Magnitud Aparente | +7.08 |
| Magnitud Absoluta | -1,03 |
| Distancia | 1,365 ly |
| Constelación | Aquila |
Posición
| Ascensión recta | 19h 11,11m |
| Declinación | 5° 16,48′ |
Preguntas frecuentes
What type of star is HIP 94250?
HIP 94250 is a Class B — B-type (Blue-White) star.
How far is HIP 94250 from Earth?
HIP 94250 is approximately 1,364.7 light-years from Earth.
Can you see HIP 94250 with the naked eye?
With an apparent magnitude of 7.08, HIP 94250 is not visible to the naked eye.
What constellation is HIP 94250 in?
HIP 94250 is located in the constellation Aquila.