HIP 16869
HIP 16869 is a K-type (Orange) star located in the constellation Perseus.
At a distance of roughly 1,443 light-years, HIP 16869 is a distant star lying deep within the Milky Way galaxy.
HIP 16869 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 16869 has an apparent magnitude of +7.68, 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 +1.768.
Fiziksel Özellikler
| Spektral Sınıf | Class K — K-type (Orange) |
| Renk İndeksi (B−V) | 1,768 |
Gözlem
| Görünür Parlaklık | +7.68 |
| Mutlak Parlaklık | -0,55 |
| Mesafe | 1,443 ly |
| Takımyıldız | Perseus |
Konum
| Sağ Açıklık | 3h 37,08m |
| Dik Açı | 47° 15,69′ |
Sıkça Sorulan Sorular
What type of star is HIP 16869?
HIP 16869 is a Class K — K-type (Orange) star.
How far is HIP 16869 from Earth?
HIP 16869 is approximately 1,443.2 light-years from Earth.
Can you see HIP 16869 with the naked eye?
With an apparent magnitude of 7.68, HIP 16869 is not visible to the naked eye.
What constellation is HIP 16869 in?
HIP 16869 is located in the constellation Perseus.