HIP 9887
HIP 9887 is a K-type (Orange) star.
At a distance of roughly 2,330 light-years, HIP 9887 is a distant star lying deep within the Milky Way galaxy.
HIP 9887 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 9887 has an apparent magnitude of +8.27, 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 +1.094.
물리적 특성
| 분광형 | K Class K — K-type (Orange) |
| 색지수 (B−V) | 1.094 |
관측
| 겉보기 등급 | +8.27 |
| 절대 등급 | -1.00 |
| 거리 | 2,330 ly |
위치
| 적경 | 2h 7.21m |
| 적위 | -11° 40.94′ |
Frequently Asked Questions
What type of star is HIP 9887?
HIP 9887 is a Class K — K-type (Orange) star.
How far is HIP 9887 from Earth?
HIP 9887 is approximately 2,329.7 light-years from Earth.
Can you see HIP 9887 with the naked eye?
With an apparent magnitude of 8.27, HIP 9887 is not visible to the naked eye.