We reconsider theories with low gravitational (or string) scale M-* where N
ewton's constant is generated via new large-volume spatial dimensions, whil
e standard model states are localized to a 3-brane. Utilizing compact hyper
bolic manifolds we show that the spectrum of Kaluza-Klein modes is radicall
y altered. This allows the early Universe to evolve normally up to substant
ial temperatures, and completely negates the astrophysical constraints on M
-*. Furthermore, an exponential hierarchy between the usual Planck scale an
d the true fundamental scale of physics can emerge with only O(1) coefficie
nts. The linear size of the internal space remains small. The proposal has
striking testable signatures.