HIP 54890
HIP 54890 is a A-type (White) star.
At a distance of roughly 1,406 light-years, HIP 54890 is a distant star lying deep within the Milky Way galaxy.
HIP 54890 is classified as a spectral class A star (A-type (White)) on the Harvard spectral classification system.
HIP 54890 has an apparent magnitude of +9.19, 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 blue-white hue, which corresponds to a B-V color index of +0.155.
คุณสมบัติทางกายภาพ
| ประเภทสเปกตรัม | A Class A — A-type (White) |
| ดัชนีสี (B−V) | 0.155 |
การสังเกต
| โชติมาตรปรากฏ | +9.19 |
| โชติมาตรสัมบูรณ์ | 1.02 |
| ระยะทาง | 1,406 ly |
ตำแหน่ง
| ไรต์แอสเซนชัน | 11h 14.34m |
| เดคลิเนชัน | -30° 9.72′ |
Frequently Asked Questions
What type of star is HIP 54890?
HIP 54890 is a Class A — A-type (White) star.
How far is HIP 54890 from Earth?
HIP 54890 is approximately 1,405.8 light-years from Earth.
Can you see HIP 54890 with the naked eye?
With an apparent magnitude of 9.19, HIP 54890 is not visible to the naked eye.