HIP 114887
HIP 114887 is a K-type (Orange) star.
Located approximately 862.9 light-years from Earth, HIP 114887 resides within the broader disk of our Milky Way galaxy.
HIP 114887 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 114887 has an apparent magnitude of +8.48, 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 +1.025.
Fiziksel Özellikler
| Spektral Sınıf | K Class K — K-type (Orange) |
| Renk İndeksi (B−V) | 1,025 |
Gözlem
| Görünür Parlaklık | +8.48 |
| Mutlak Parlaklık | 1,37 |
| Mesafe | 863 ly |
Konum
| Sağ Açıklık | 23h 16,30m |
| Dik Açı | -40° 39,74′ |
Frequently Asked Questions
What type of star is HIP 114887?
HIP 114887 is a Class K — K-type (Orange) star.
How far is HIP 114887 from Earth?
HIP 114887 is approximately 862.8 light-years from Earth.
Can you see HIP 114887 with the naked eye?
With an apparent magnitude of 8.48, HIP 114887 is not visible to the naked eye.