HIP 92008
HIP 92008 is a K-type (Orange) star.
At a distance of roughly 1,157 light-years, HIP 92008 is a distant star lying deep within the Milky Way galaxy.
HIP 92008 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 92008 has an apparent magnitude of +6.04, 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 +1.484.
Fiziksel Özellikler
| Spektral Sınıf | K Class K — K-type (Orange) |
| Renk İndeksi (B−V) | 1,484 |
Gözlem
| Görünür Parlaklık | +6.04 |
| Mutlak Parlaklık | -1,71 |
| Mesafe | 1,157 ly |
Konum
| Sağ Açıklık | 18h 45,19m |
| Dik Açı | -61° 5,71′ |
Frequently Asked Questions
What type of star is HIP 92008?
HIP 92008 is a Class K — K-type (Orange) star.
How far is HIP 92008 from Earth?
HIP 92008 is approximately 1,156.6 light-years from Earth.
Can you see HIP 92008 with the naked eye?
With an apparent magnitude of 6.04, HIP 92008 is not visible to the naked eye.