HIP 103887
HIP 103887 is a K-type (Orange) star.
At a distance of roughly 2,471 light-years, HIP 103887 is a distant star lying deep within the Milky Way galaxy.
HIP 103887 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 103887 has an apparent magnitude of +8.80, 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 red hue, which corresponds to a B-V color index of +1.527.
물리적 특성
| 분광형 | K Class K — K-type (Orange) |
| 색지수 (B−V) | 1.527 |
관측
| 겉보기 등급 | +8.80 |
| 절대 등급 | -0.60 |
| 거리 | 2,471 ly |
위치
| 적경 | 21h 2.98m |
| 적위 | -63° 15.10′ |
Frequently Asked Questions
What type of star is HIP 103887?
HIP 103887 is a Class K — K-type (Orange) star.
How far is HIP 103887 from Earth?
HIP 103887 is approximately 2,470.9 light-years from Earth.
Can you see HIP 103887 with the naked eye?
With an apparent magnitude of 8.80, HIP 103887 is not visible to the naked eye.