We show that observations of X-ray pulsing from SAX J1808.4-3658 place a fi
rm upper limit of 13.8m(1/3) km on the radius of the neutron star, where m
is its mass in solar units. The Limit is independent of distance, or assump
tions about the magnetospheric geometry, and could be significantly tighten
ed by observations of the pulsations in the near future. We discuss the imp
lications for the equation of state and the possible neutron star mass.