HIP 102250
HIP 102250 is a K-type (Orange) star.
At a distance of roughly 1,049 light-years, HIP 102250 is a distant star lying deep within the Milky Way galaxy.
HIP 102250 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 102250 has an apparent magnitude of +8.15, 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 +1.169.
物理的特性
| スペクトル型 | K Class K — K-type (Orange) |
| 色指数 (B−V) | 1.169 |
観測
| 見かけの等級 | +8.15 |
| 絶対等級 | 0.61 |
| 距離 | 1,049 ly |
位置
| 赤経 | 20h 43.11m |
| 赤緯 | -62° 58.51′ |
Frequently Asked Questions
What type of star is HIP 102250?
HIP 102250 is a Class K — K-type (Orange) star.
How far is HIP 102250 from Earth?
HIP 102250 is approximately 1,048.7 light-years from Earth.
Can you see HIP 102250 with the naked eye?
With an apparent magnitude of 8.15, HIP 102250 is not visible to the naked eye.