We compare the dynamical properties of two galaxies at identical posit
ions on the Tully-Fisher relation, but with different surface brightne
sses. We find that the low surface brightness galaxy UGC 128 has a hig
her mass-to-light ratio, and yet has lower mass densities than the hig
h surface brightness galaxy NGC 2403. This is true for the gas surface
density, the stellar surface density, and the total mass density.