HIP 17887
HIP 17887 is a G-type (Yellow) star.
Located approximately 223.6 light-years from Earth, HIP 17887 resides within the broader disk of our Milky Way galaxy.
HIP 17887 is classified as a spectral class G star (G-type (Yellow)) on the Harvard spectral classification system.
HIP 17887 has an apparent magnitude of +9.01, 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 white hue, which corresponds to a B-V color index of +0.582.
คุณสมบัติทางกายภาพ
| ประเภทสเปกตรัม | G Class G — G-type (Yellow) |
| ดัชนีสี (B−V) | 0.582 |
การสังเกต
| โชติมาตรปรากฏ | +9.01 |
| โชติมาตรสัมบูรณ์ | 4.83 |
| ระยะทาง | 224 ly |
ตำแหน่ง
| ไรต์แอสเซนชัน | 3h 49.58m |
| เดคลิเนชัน | 58° 46.09′ |
Frequently Asked Questions
What type of star is HIP 17887?
HIP 17887 is a Class G — G-type (Yellow) star.
How far is HIP 17887 from Earth?
HIP 17887 is approximately 223.6 light-years from Earth.
Can you see HIP 17887 with the naked eye?
With an apparent magnitude of 9.01, HIP 17887 is not visible to the naked eye.