E. Willingshofer et al., Thermomechanical consequences of Cretaceous continent-continent collision in the eastern Alps (Austria): Insights from two-dimensional modeling, TECTONICS, 18(5), 1999, pp. 809-826
We use two-dimensional numerical modeling techniques to investigate the the
rmomechanical consequences of closure of the Meliata-Hallstatt ocean and co
nsequent Cretaceous continent-continent collision in the eastern Alps (Aust
ria). In the modeling a lower plate position of the Austro-Alpine (AA) cont
inental block is adopted during collision with the Upper Juvavic-Silice blo
ck. The thermal structure of the lithosphere was calculated for major AA te
ctonic units (Upper, Middle, and Lower Austro-Alpine) by integration of the
transient heat flow equation along an approximately NW-SE cross section ea
st of the Tauern Window. Indications of the rheological evolution of the AA
were determined by calculating strength profiles at key stages of the Cret
aceous orogeny, making use of the thermal modeling predictions combined wit
h rock mechanics data. Cooling in the upper plate and lower greenschist fac
ies metamorphism within footwall parts of the lower Upper Austro-Alpine (UA
) plate, related to SE directed underthrusting of the UA beneath the Upper
Juvavic-Silice block at circa 100 Ma, were predicted by the numerical model
. The observed pressure-temperature path for deeply buried Middle Austro-Al
pine (MA) upper crustal units and their subsequent isothermal exhumation ar
e best reproduced assuming a pressure peak at 95 Ma and exhumation recites
ranging between 4 and 7.5 mm yr(-1). From the modeling results, we deduce t
hat the temperature evolution during eclogite exhumation is primarily depen
dent on rates of tectonic movements and largely independent of the mode of
exhumation (thrusting versus erosion). Furthermore, very rapid postmetamorp
hic exhumation of southern Lower Austro-Alpine (LA) units is predicted in o
rder to account for subsequent cooling. This is constrained by As-40/Ar-39
data. The cooling paths of MA and LA rocks appear to be primarily controlle
d by their near-surface positions at the end of the Cretaceous rather than
by other processes such as concurrent underthrusting. Upward advection of h
eat by rapid exhumation induced thermal weakening of the thickened crust. T
he inferred weakness of the central parts of the orogenic system may play a
n important role during detachment-related tectonic unroofing, orogenic col
lapse, and concomitant basin formation (central Alpine Gosau basins).