HIP 45409
HIP 45409 is a K-type (Orange) star.
At a distance of roughly 1,885 light-years, HIP 45409 is a distant star lying deep within the Milky Way galaxy.
HIP 45409 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 45409 has an apparent magnitude of +9.12, 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 yellow hue, which corresponds to a B-V color index of +0.951.
物理的特性
| スペクトル型 | K Class K — K-type (Orange) |
| 色指数 (B−V) | 0.951 |
観測
| 見かけの等級 | +9.12 |
| 絶対等級 | 0.31 |
| 距離 | 1,885 ly |
位置
| 赤経 | 9h 15.22m |
| 赤緯 | 9° 45.57′ |
Frequently Asked Questions
What type of star is HIP 45409?
HIP 45409 is a Class K — K-type (Orange) star.
How far is HIP 45409 from Earth?
HIP 45409 is approximately 1,885.3 light-years from Earth.
Can you see HIP 45409 with the naked eye?
With an apparent magnitude of 9.12, HIP 45409 is not visible to the naked eye.