An important recent development in the field of geomorphology has been
the application of in-situ cosmic-ray-produced nuclides to obtain mod
el erosion rates and surface exposure ages. These concepts emerged som
e four decades ago in studies of cosmogenic nuclides in meteorites, bu
t cannot generally be used analogously for terrestrial rocks. The diff
erences in the two cases are outlined. For the case of steady-state er
osional histories, the terrestrial surface exposure ages depend on the
half-life of the radionuclide studied. A suggestion is made for prese
nting the surface exposure ages, which allows a clear definition of th
e meaning of the estimated exposure ages. In the case of a discrete ex
posure history, the meaning of ''exposure age''-which should more appr
opriately be called ''event age''-is however quite unambiguous.