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HD 158614
HD 158614 is a spectroscopic binary star system approximately 60 light-years away in the constellation of Ophiuchus. This system is in the Zeta Herculis moving group, which is of low metallicity stars, 5 billion years old. Besides ζ Herculis, the group includes δ Trianguli, ζ Reticuli, 1 Hydrae, Gl 456, φ2 Pavonis, and GJ 9079. This binary was included in a search for brown dwarfs that turned up no large companions. == See also ==
* Zeta Herculis
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