HIP 110887
HIP 110887 is a K-type (Orange) star.
Located approximately 153.0 light-years from Earth, HIP 110887 resides within the broader disk of our Milky Way galaxy.
HIP 110887 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
At an apparent magnitude of +11.51, HIP 110887 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 +1.300.
Fiziksel Özellikler
| Spektral Sınıf | K Class K — K-type (Orange) |
| Renk İndeksi (B−V) | 1,300 |
Gözlem
| Görünür Parlaklık | +11.51 |
| Mutlak Parlaklık | 8,15 |
| Mesafe | 153 ly |
Konum
| Sağ Açıklık | 22h 27,90m |
| Dik Açı | -58° 6,64′ |
Frequently Asked Questions
What type of star is HIP 110887?
HIP 110887 is a Class K — K-type (Orange) star.
How far is HIP 110887 from Earth?
HIP 110887 is approximately 153.0 light-years from Earth.
Can you see HIP 110887 with the naked eye?
With an apparent magnitude of 11.51, HIP 110887 is not visible to the naked eye.