  We present a weak lensing analysis of the Coma Cluster using the Sloan
Digital Sky Survey (SDSS) Data Release Five. Complete imaging of a ~ 200 square
degree region is used to measure the tangential shear of this cluster. The
shear is fit to an NFW model and we find a virial radius of
r_{200}=1.99_{-0.22}^{+0.21}h^{-1}Mpc which corresponds to a virial mass of
M_{200}=1.88_{-0.56}^{+0.65}\times10^{15}h^{-1}M_{\odot}. We additionally
compare our weak lensing measurement to the virial mass derived using dynamical
techniques, and find they are in agreement. This is the lowest redshift,
largest angle weak lensing measurement of an individual cluster to date.
