HIP 38499
HIP 38499 is a K-type (Orange) star.
At a distance of roughly 1,822 light-years, HIP 38499 is a distant star lying deep within the Milky Way galaxy.
HIP 38499 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 38499 has an apparent magnitude of +8.64, 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 +1.550.
Propiedades físicas
| Clase Espectral | K Class K — K-type (Orange) |
| Índice de color (B−V) | 1,550 |
Observación
| Magnitud Aparente | +8.64 |
| Magnitud Absoluta | -0,10 |
| Distancia | 1,822 ly |
Posición
| Ascensión recta | 7h 53,06m |
| Declinación | -43° 58,82′ |
Frequently Asked Questions
What type of star is HIP 38499?
HIP 38499 is a Class K — K-type (Orange) star.
How far is HIP 38499 from Earth?
HIP 38499 is approximately 1,822.1 light-years from Earth.
Can you see HIP 38499 with the naked eye?
With an apparent magnitude of 8.64, HIP 38499 is not visible to the naked eye.