  We estimate the 1.8 MeV luminosity of the Sco-Cen association due to
radioactive decay of 26Al to (4-15) 10e-5 ph cm**-2 s**-1. We propose a low
surface brightness, limb brightened bubble for the 1.8 MeV intensity
distribution. The detectibility of this distribution with existing gamma-ray
telescopes is discussed.
