  A survey of red giants in the globular cluster M3 with the Hydra multi-object
spectrograph on the WIYN 3.5-m telescope indicated a prominent Li I 6707 $\AA$
feature in the red giant vZ 1050. Follow-up spectroscopy with the ARC 3.5-m
telescope confirmed this observation and yielded a derived abundance of
A(Li)$_{NLTE}$ = 1.6 $\pm$ 0.05. In addition, the high oxygen and low sodium
abundances measured from the same spectrum suggest that vZ 1050 is a first
generation cluster star. The location vZ 1050 above the horizontal branch and
blueward of the red giant branch in the cluster's color-magnitude diagram
places vZ 1050 on M3's asymptotic giant branch. The likely source for the
enhanced lithium abundance is the Cameron-Fowler mechanism operating in vZ 1050
itself.
