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HD 895
HD 895 is a triple star system in the constellation Andromeda. Its apparent magnitude is 6.27. Located around away, the primary is a F-type main-sequence star of spectral type F8V, a star that is currently fusing its core hydrogen. While the secondary star cannot be separated from the primary except by spectroscopy, the tertiary can, and has been found to be a spectroscopic binary itself, although with an apparent magnitude of 10.37, it is too faint to be seen without a telescope.
==References==
* (Image HD 895 )
抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』
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