  We have determined Al, $\alpha$, Fe-peak, and neutron capture elemental
abundances for five red giant branch (RGB) stars in the Galactic globular
cluster M10. Abundances were determined using equivalent width analyses of
moderate resolution (R$\sim$15,000) spectra obtained with the Hydra multifiber
positioner and bench spectrograph on the WIYN telescope. The data sample the
upper RGB from the luminosity level near the horizontal branch to about 0.5 mag
below the RGB tip. We find in agreement with previous studies that M10 is
moderately metal-poor with [Fe/H]=-1.45 ($\sigma$=0.04). All stars appear
enhanced in Al with $<$[Al/Fe]$>$=+0.33 ($\sigma$=0.19), but no stars have
[Al/Fe]$\ga$+0.55. We find the $\alpha$ elements to be enhanced by +0.20 to
+0.40 dex and the Fe--peak elements to have [el/Fe]$\sim$0, which are
consistent with predictions from type II SN ejecta. Additionally, the cluster
appears to be r-process rich with $<$[Eu/La]$>$=+0.41.
