HIP 15416
HIP 15416 is a K-type (Orange) star located in the constellation Perseus.
At a distance of roughly 1,177 light-years, HIP 15416 is a distant star lying deep within the Milky Way galaxy.
HIP 15416 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
With an apparent magnitude of +4.85, HIP 15416 sits near the limit of naked-eye visibility. It can be glimpsed without optical aid under dark skies, but binoculars will make observation much easier. Observers will note its red hue, which corresponds to a B-V color index of +1.491.
Fiziksel Özellikler
| Spektral Sınıf | Class K — K-type (Orange) |
| Renk İndeksi (B−V) | 1,491 |
Gözlem
| Görünür Parlaklık | +4.85 |
| Mutlak Parlaklık | -2,94 |
| Mesafe | 1,177 ly |
| Takımyıldız | Perseus |
Konum
| Sağ Açıklık | 3h 18,73m |
| Dik Açı | 34° 13,36′ |
Sıkça Sorulan Sorular
What type of star is HIP 15416?
HIP 15416 is a Class K — K-type (Orange) star.
How far is HIP 15416 from Earth?
HIP 15416 is approximately 1,177.5 light-years from Earth.
Can you see HIP 15416 with the naked eye?
With an apparent magnitude of 4.85, HIP 15416 is visible to the naked eye.
What constellation is HIP 15416 in?
HIP 15416 is located in the constellation Perseus.