HIP 11887
HIP 11887 is a K-type (Orange) star.
At a distance of roughly 1,029 light-years, HIP 11887 is a distant star lying deep within the Milky Way galaxy.
HIP 11887 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 11887 has an apparent magnitude of +7.74, 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 +1.602.
คุณสมบัติทางกายภาพ
| ประเภทสเปกตรัม | K Class K — K-type (Orange) |
| ดัชนีสี (B−V) | 1.602 |
การสังเกต
| โชติมาตรปรากฏ | +7.74 |
| โชติมาตรสัมบูรณ์ | 0.24 |
| ระยะทาง | 1,029 ly |
ตำแหน่ง
| ไรต์แอสเซนชัน | 2h 33.29m |
| เดคลิเนชัน | -26° 17.46′ |
Frequently Asked Questions
What type of star is HIP 11887?
HIP 11887 is a Class K — K-type (Orange) star.
How far is HIP 11887 from Earth?
HIP 11887 is approximately 1,028.9 light-years from Earth.
Can you see HIP 11887 with the naked eye?
With an apparent magnitude of 7.74, HIP 11887 is not visible to the naked eye.