HIP 103887

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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.