HIP 63699
HIP 63699 is a K-type (Orange) star.
At a distance of roughly 1,264 light-years, HIP 63699 is a distant star lying deep within the Milky Way galaxy.
HIP 63699 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 63699 has an apparent magnitude of +7.95, 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 +1.311.
คุณสมบัติทางกายภาพ
| ประเภทสเปกตรัม | K Class K — K-type (Orange) |
| ดัชนีสี (B−V) | 1.311 |
การสังเกต
| โชติมาตรปรากฏ | +7.95 |
| โชติมาตรสัมบูรณ์ | 0.01 |
| ระยะทาง | 1,264 ly |
ตำแหน่ง
| ไรต์แอสเซนชัน | 13h 3.26m |
| เดคลิเนชัน | 47° 58.10′ |
Frequently Asked Questions
What type of star is HIP 63699?
HIP 63699 is a Class K — K-type (Orange) star.
How far is HIP 63699 from Earth?
HIP 63699 is approximately 1,264.2 light-years from Earth.
Can you see HIP 63699 with the naked eye?
With an apparent magnitude of 7.95, HIP 63699 is not visible to the naked eye.