HIP 106887
HIP 106887 is a K-type (Orange) star.
At a distance of roughly 1,463 light-years, HIP 106887 is a distant star lying deep within the Milky Way galaxy.
HIP 106887 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 106887 has an apparent magnitude of +7.51, 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 +1.239.
Fiziksel Özellikler
| Spektral Sınıf | K Class K — K-type (Orange) |
| Renk İndeksi (B−V) | 1,239 |
Gözlem
| Görünür Parlaklık | +7.51 |
| Mutlak Parlaklık | -0,75 |
| Mesafe | 1,463 ly |
Konum
| Sağ Açıklık | 21h 38,96m |
| Dik Açı | -24° 26,99′ |
Frequently Asked Questions
What type of star is HIP 106887?
HIP 106887 is a Class K — K-type (Orange) star.
How far is HIP 106887 from Earth?
HIP 106887 is approximately 1,462.6 light-years from Earth.
Can you see HIP 106887 with the naked eye?
With an apparent magnitude of 7.51, HIP 106887 is not visible to the naked eye.