  We determine lithium (Li) abundances for solar twins in the M67 open cluster
to add valuable information about the correlation between Li depletion and
stellar age and, then, better understand stellar structure and evolution. We
use high resolution and good signal-to-noise ratio spectra to characterize Li
depletion in three solar twins from M67, using spectral synthesis in the region
of the asymmetric 6707.75 \AA \, Li I feature. The mean Li abundance value of
A(Li)$=1.6\pm0.2$ dex for our sample of M67 solar twins (our three stars plus a
fourth solar twin from a previous analysis in the literature) presents Li
abundance expected for its age. Also, the scatter estimated from the standard
deviation of the Li abundances in this work is similar to the typical scatter
found in a sample of field solar twins presented in the literature.
