We consider the depletion of primordial deuterium in the interior of subste
llar objects as a function of mass, age, and absolute magnitude in several
photometric passbands. We characterize potential spectroscopic signatures o
f deuterium in the lines of deuterated water HDO. These results will serve
as a useful, independent diagnostic to characterize the mass and/or the age
of young substellar objects and to provide an independent age determinatio
n of very young clusters. These results can serve to identify objects at th
e deuterium-burning limit and to confront the theoretical prediction that D
burning is a necessary condition to form starlike objects.