HIP 61887
HIP 61887 is a K-type (Orange) star.
At a distance of roughly 1,195 light-years, HIP 61887 is a distant star lying deep within the Milky Way galaxy.
HIP 61887 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 61887 has an apparent magnitude of +7.78, 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 +1.545.
คุณสมบัติทางกายภาพ
| ประเภทสเปกตรัม | K Class K — K-type (Orange) |
| ดัชนีสี (B−V) | 1.545 |
การสังเกต
| โชติมาตรปรากฏ | +7.78 |
| โชติมาตรสัมบูรณ์ | -0.04 |
| ระยะทาง | 1,195 ly |
ตำแหน่ง
| ไรต์แอสเซนชัน | 12h 40.88m |
| เดคลิเนชัน | 34° 6.27′ |
Frequently Asked Questions
What type of star is HIP 61887?
HIP 61887 is a Class K — K-type (Orange) star.
How far is HIP 61887 from Earth?
HIP 61887 is approximately 1,194.7 light-years from Earth.
Can you see HIP 61887 with the naked eye?
With an apparent magnitude of 7.78, HIP 61887 is not visible to the naked eye.