  The dark dimension scenario, which is motivated from Swampland principles and
predicts a single micron scale extra dimension, suggests a consistent framework
for the dark sector of the universe. We consider the implications of this
scenario for the QCD axion. We find that in the scenario in which the axion is
localized on the standard model brane (which we will argue is natural), a
combination of theoretical (being bounded by the 5D Planck mass) and
observational constraints forces it to have decay constant in a narrow range $f
\sim 10^9 - 10^{10}$ GeV. This corresponds to a mass for the QCD axion of $m_a
\sim (1 - 10)$ meV. The axion mass surprisingly coincides with the mass scale
for the dark energy, the dark matter tower, and the neutrinos. In this scenario
axions are not expected to form a large fraction of the dark matter but
nevertheless this range of axion parameters is accessible to observations in
near future experiments.
