HIP 16209
HIP 16209 is a K-type (Orange) star located in the constellation Perseus.
Located approximately 83.0 light-years from Earth, HIP 16209 resides within the broader disk of our Milky Way galaxy.
HIP 16209 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
At an apparent magnitude of +11.10, HIP 16209 is a faint star that requires a telescope to observe. It is invisible to the naked eye and too dim for most binoculars. Observers will note its orange hue, which corresponds to a B-V color index of +1.314.
Fiziksel Özellikler
| Spektral Sınıf | Class K — K-type (Orange) |
| Renk İndeksi (B−V) | 1,314 |
Gözlem
| Görünür Parlaklık | +11.10 |
| Mutlak Parlaklık | 9,07 |
| Mesafe | 83.0 ly |
| Takımyıldız | Perseus |
Konum
| Sağ Açıklık | 3h 28,88m |
| Dik Açı | 37° 22,95′ |
Sıkça Sorulan Sorular
What type of star is HIP 16209?
HIP 16209 is a Class K — K-type (Orange) star.
How far is HIP 16209 from Earth?
HIP 16209 is approximately 83.0 light-years from Earth.
Can you see HIP 16209 with the naked eye?
With an apparent magnitude of 11.10, HIP 16209 is not visible to the naked eye.
What constellation is HIP 16209 in?
HIP 16209 is located in the constellation Perseus.