We present observations of an H$alpha$ emitting knot in the thick disk of NGC 4013, demonstrating it is an H II region surrounding a cluster of young hot stars $z = 860$ pc above the plane of this edge-on spiral galaxy. With LBT/MODS spectroscopy we show this H II region has an H$alpha$ luminosity $sim 4$ - 7 times that of the Orion nebula, with an implied ionizing photon production rate $log Q_0 gtrsim 49.4$ (photons s$^{-1}$). HST/WFPC2 imaging reveals an associated blue continuum source with $M_{V} = -8.21pm0.24$. Together these properties demonstrate the H II region is powered by a young cluster of stars formed {em in situ} in the thick disk with an ionizing photon flux equivalent to $sim$6 O7 V stars. If we assume $approx6$ other extraplanar halpha -emitting knots are H II regions, the total thick disk star formation rate of gc 4013 is $sim 5 times 10^{-4}$ M$_odot$ yr$^{-1}$. The star formation likely occurs in the dense clouds of the interstellar thick disk seen in optical images of dust extinction and CO emission.
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