  We present the results from the analysis of galaxy rotation curves with
Verlinde's emergent gravity. We use the data in the SPARC (Spitzer Photometry
and Accurate Rotation Curves) database, which contains a sample of 175 nearby
disk galaxies with 3.6 $\mu$m surface photometry and rotation curves. We
compute the gravitational acceleration at different galactocentric radii
expected from the baryon distribution of the galaxies with the emergent
gravity, and compare it with the observed gravitational acceleration derived
from galactic rotation curves. The predicted and observed accelerations agree
well with a mean offset $\mu{\rm [log(g_{obs})-log(g_{Ver})]}=-0.060\pm0.004$
and a scatter $\sigma{\rm [log(g_{obs})-log(g_{Ver})]}=0.137\pm0.004$ by
assuming a de Sitter universe. These offset and scatter become smaller when we
assume a more realistic universe, quasi de Sitter universe, as
$\mu=-0.027\pm0.003$ and $\sigma=0.129\pm0.003$. Our results suggest that
Verlinde's emergent gravity could be a good solution to the missing mass
problem without introducing dark matter.
