Arkani-Hamed, Dimopoulos, and Dvali have proposed that the fundamental grav
itational scale is close to 1 TeV, and that the observed weakness of gravit
y at long distances is explained by the presence of large extra compact dim
ensions. If this scenario is realized in a string theory of quantum gravity
, the string excited states of standard model particles will also have TeV
masses. These states will be visible to experiment and in fact provide the
first signatures of the presence of a low quantum gravity scale. Their pres
ence also affects the more familiar signatures due to real and virtual grav
iton emission. We study the effects of these states in a simple string mode
l.