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We report the discovery of EPIC247098361b using photometric data of theKepler K2 satellite coupled with ground-based spectroscopic observations.EPIC247098361b has a mass of M$_{P}=0.397\pm 0.037$ M$_J$, a radius ofR$_{P}=1.00 \pm 0.020$ R$_J$, and a moderately low equilibrium temperature of$T_{eq}=1030 \pm 15$ K due to its relatively large star-planet separation of$a=0.1036$ AU. EPIC247098361b orbits its bright ($V=9.9$) late F-type host starin an eccentric orbit ($e=0.258 \pm 0.025$) every 11.2 days, and is one of onlyfour well characterized warm Jupiters having hosts stars brighter than $V=10$.We estimate a heavy element content of 20 $\pm$ 7 M$_{\oplus}$ forEPIC247098361b, which is consistent with standard models of giant planetformation. The bright host star of EPIC247098361b makes this system a wellsuited target for detailed follow-up observations that will aid in the study ofthe atmospheres and orbital evolution of giant planets at moderate separationsfrom their host stars.

EPIC247098361b: a transiting warm Saturn on an eccentric $P=11.2$ days orbit around a $V=9.9$ star