We present a moderate-resolution spectroscopic analysis of the 10–25 Myr clusters NGC 7160 and NGC 2232 , using observations obtained with the WIYN 3.5-m telescope .
Both NGC 7160 and NGC 2232 are found to have super-solar metallicities , with a mean [ Fe/H ] = 0.16 \pm 0.03 ( s.e.m . )
for NGC 7160 , and 0.22 \pm 0.09 ( s.e.m . )
or 0.32 \pm 0.08 for NGC 2232 , depending on the adopted temperature scale .
NGC 7160 exhibits solar distributions of Na , Fe-peak , and \alpha -elements .
NGC 2232 is underabundant in light elements Al and Si , by \sim 0.25 and \sim 0.15 dex , respectively ; [ Ni/Fe ] is roughly solar .
The abundance of lithium in NGC 2232 stars is in agreement with undepleted values reported for other cluster main sequence stars .
Our abundances are similar to other metal-rich open clusters and Galactic thin and thick disk stars .