HIP 39218
HIP 39218 is a A-type (White) star.
At a distance of roughly 1,080 light-years, HIP 39218 is a distant star lying deep within the Milky Way galaxy.
HIP 39218 is classified as a spectral class A star (A-type (White)) on the Harvard spectral classification system.
HIP 39218 has an apparent magnitude of +9.10, 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 hue, which corresponds to a B-V color index of -0.002.
Propriedades físicas
| Classe Espectral | A Class A — A-type (White) |
| Índice de cor (B−V) | -0,002 |
Observação
| Magnitude Aparente | +9.10 |
| Magnitude Absoluta | 1,50 |
| Distância | 1,080 ly |
Posição
| Ascensão reta | 8h 1,32m |
| Declinação | -12° 13,84′ |
Frequently Asked Questions
What type of star is HIP 39218?
HIP 39218 is a Class A — A-type (White) star.
How far is HIP 39218 from Earth?
HIP 39218 is approximately 1,080.0 light-years from Earth.
Can you see HIP 39218 with the naked eye?
With an apparent magnitude of 9.10, HIP 39218 is not visible to the naked eye.