HIP 104677
HIP 104677 is a K-type (Orange) star.
At a distance of roughly 1,503 light-years, HIP 104677 is a distant star lying deep within the Milky Way galaxy.
HIP 104677 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 104677 has an apparent magnitude of +6.96, 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 +1.627.
Fiziksel Özellikler
| Spektral Sınıf | K Class K — K-type (Orange) |
| Renk İndeksi (B−V) | 1,627 |
Gözlem
| Görünür Parlaklık | +6.96 |
| Mutlak Parlaklık | -1,36 |
| Mesafe | 1,503 ly |
Konum
| Sağ Açıklık | 21h 12,20m |
| Dik Açı | 11° 46,89′ |
Frequently Asked Questions
What type of star is HIP 104677?
HIP 104677 is a Class K — K-type (Orange) star.
How far is HIP 104677 from Earth?
HIP 104677 is approximately 1,503.0 light-years from Earth.
Can you see HIP 104677 with the naked eye?
With an apparent magnitude of 6.96, HIP 104677 is not visible to the naked eye.