HIP 63887
HIP 63887 is a K-type (Orange) star located in the constellation Centaurus.
Located approximately 886.3 light-years from Earth, HIP 63887 resides within the broader disk of our Milky Way galaxy.
HIP 63887 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 63887 has an apparent magnitude of +8.02, 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 +1.510.
Propiedades físicas
| Clase Espectral | K Class K — K-type (Orange) |
| Índice de color (B−V) | 1,510 |
Observación
| Magnitud Aparente | +8.02 |
| Magnitud Absoluta | 0,85 |
| Distancia | 886 ly |
| Constelación | Centaurus |
Posición
| Ascensión recta | 13h 5,55m |
| Declinación | -49° 51,09′ |
Frequently Asked Questions
What type of star is HIP 63887?
HIP 63887 is a Class K — K-type (Orange) star.
How far is HIP 63887 from Earth?
HIP 63887 is approximately 886.3 light-years from Earth.
Can you see HIP 63887 with the naked eye?
With an apparent magnitude of 8.02, HIP 63887 is not visible to the naked eye.
What constellation is HIP 63887 in?
HIP 63887 is located in the constellation Centaurus.