HIP 99051
HIP 99051 is a K-type (Orange) star located in the constellation Sagittarius.
At a distance of roughly 2,051 light-years, HIP 99051 is a distant star lying deep within the Milky Way galaxy.
HIP 99051 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 99051 has an apparent magnitude of +8.71, 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 +1.661.
Propiedades físicas
| Clase Espectral | K Class K — K-type (Orange) |
| Índice de color (B−V) | 1,661 |
Observación
| Magnitud Aparente | +8.71 |
| Magnitud Absoluta | -0,28 |
| Distancia | 2,051 ly |
| Constelación | Sagittarius |
Posición
| Ascensión recta | 20h 6,61m |
| Declinación | -25° 34,60′ |
Frequently Asked Questions
What type of star is HIP 99051?
HIP 99051 is a Class K — K-type (Orange) star.
How far is HIP 99051 from Earth?
HIP 99051 is approximately 2,051.3 light-years from Earth.
Can you see HIP 99051 with the naked eye?
With an apparent magnitude of 8.71, HIP 99051 is not visible to the naked eye.
What constellation is HIP 99051 in?
HIP 99051 is located in the constellation Sagittarius.