HIP 39018
HIP 39018 is a A-type (White) star located in the constellation Gemini.
At a distance of roughly 1,400 light-years, HIP 39018 is a distant star lying deep within the Milky Way galaxy.
HIP 39018 is classified as a spectral class A star (A-type (White)) on the Harvard spectral classification system.
HIP 39018 has an apparent magnitude of +9.82, 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 +0.219.
Propriétés physiques
| Classe Spectrale | Class A — A-type (White) |
| Indice de couleur (B−V) | 0,219 |
Observation
| Magnitude Apparente | +9.82 |
| Magnitude Absolue | 1,66 |
| Distance | 1,400 ly |
| Constellation | Gemini |
Position
| Ascension droite | 7h 59,07m |
| Déclinaison | 24° 13,75′ |
Questions fréquentes
What type of star is HIP 39018?
HIP 39018 is a Class A — A-type (White) star.
How far is HIP 39018 from Earth?
HIP 39018 is approximately 1,399.8 light-years from Earth.
Can you see HIP 39018 with the naked eye?
With an apparent magnitude of 9.82, HIP 39018 is not visible to the naked eye.
What constellation is HIP 39018 in?
HIP 39018 is located in the constellation Gemini.