HIP 97869
HIP 97869 is a K-type (Orange) star.
At a distance of roughly 1,599 light-years, HIP 97869 is a distant star lying deep within the Milky Way galaxy.
HIP 97869 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 97869 has an apparent magnitude of +7.58, 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 +1.418.
Fiziksel Özellikler
| Spektral Sınıf | K Class K — K-type (Orange) |
| Renk İndeksi (B−V) | 1,418 |
Gözlem
| Görünür Parlaklık | +7.58 |
| Mutlak Parlaklık | -0,87 |
| Mesafe | 1,599 ly |
Konum
| Sağ Açıklık | 19h 53,29m |
| Dik Açı | -72° 28,41′ |
Frequently Asked Questions
What type of star is HIP 97869?
HIP 97869 is a Class K — K-type (Orange) star.
How far is HIP 97869 from Earth?
HIP 97869 is approximately 1,598.8 light-years from Earth.
Can you see HIP 97869 with the naked eye?
With an apparent magnitude of 7.58, HIP 97869 is not visible to the naked eye.