HIP 96218
HIP 96218 is a K-type (Orange) star located in the constellation Aquila.
Located approximately 771.0 light-years from Earth, HIP 96218 resides within the broader disk of our Milky Way galaxy.
HIP 96218 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 96218 has an apparent magnitude of +8.24, 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 orange hue, which corresponds to a B-V color index of +1.015.
Fiziksel Özellikler
| Spektral Sınıf | Class K — K-type (Orange) |
| Renk İndeksi (B−V) | 1,015 |
Gözlem
| Görünür Parlaklık | +8.24 |
| Mutlak Parlaklık | 1,37 |
| Mesafe | 771 ly |
| Takımyıldız | Aquila |
Konum
| Sağ Açıklık | 19h 33,99m |
| Dik Açı | 9° 11,35′ |
Sıkça Sorulan Sorular
What type of star is HIP 96218?
HIP 96218 is a Class K — K-type (Orange) star.
How far is HIP 96218 from Earth?
HIP 96218 is approximately 771.0 light-years from Earth.
Can you see HIP 96218 with the naked eye?
With an apparent magnitude of 8.24, HIP 96218 is not visible to the naked eye.
What constellation is HIP 96218 in?
HIP 96218 is located in the constellation Aquila.