HIP 102887
HIP 102887 is a K-type (Orange) star.
Located approximately 860.6 light-years from Earth, HIP 102887 resides within the broader disk of our Milky Way galaxy.
HIP 102887 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 102887 has an apparent magnitude of +8.94, 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 +1.119.
Fiziksel Özellikler
| Spektral Sınıf | K Class K — K-type (Orange) |
| Renk İndeksi (B−V) | 1,119 |
Gözlem
| Görünür Parlaklık | +8.94 |
| Mutlak Parlaklık | 1,83 |
| Mesafe | 861 ly |
Konum
| Sağ Açıklık | 20h 50,67m |
| Dik Açı | -44° 53,32′ |
Frequently Asked Questions
What type of star is HIP 102887?
HIP 102887 is a Class K — K-type (Orange) star.
How far is HIP 102887 from Earth?
HIP 102887 is approximately 860.6 light-years from Earth.
Can you see HIP 102887 with the naked eye?
With an apparent magnitude of 8.94, HIP 102887 is not visible to the naked eye.