Literature data on geochronology and pressure-temperature estimates ha
ve been used to assess the depth-time paths for high-pressure units in
the Alps and the Variscan belt. These depth-time paths consistently s
how that exhumation rates decrease through time. The first stages of t
he exhumation are rapid (>1 mm yr(-1)) and last less than a few millio
n to a few tens of million years. In contrast, the final 10-20 km asce
nt to the surface is at least one order of magnitude slower. For the d
eepest and most important part of the exhumation trajectory, the chron
ology of the retrogressive metamorphism excludes gravitational collaps
e as the major driving force. Material balance and structural argument
s also exclude isostatically assisted erosion processes. Prism dynamic
s and tectonically assisted erosion are the most likely mechanisms acc
ounting for the kinetics of exhumation. Isostasy-assisted erosion and
shallow-level extension are nevertheless required to eventually bring
the high-pressure rocks to exposure.