J. Arkanihamed, EFFECTS OF THE CORE COOLING ON THE INTERNAL DYNAMICS AND THERMAL EVOLUTION OF TERRESTRIAL PLANETS, J GEO R-SOL, 99(B6), 1994, pp. 12109-12119
The effects of thermal coupling of the core and mantle on the thermal
evolution and mantle dynamics of terrestrial planets are investigated
using three-dimensional thermal convection models in a spherical shell
. Three pairs of models are presented to study mantle models of differ
ent viscosities and internal heating. In each pair, one model adopts a
constant temperature at the core-mantle boundary, and the other allow
s the core to thermally couple to the mantle and cool. In the first an
d second pairs, the mantle is heated only from below, whereas in the t
hird pair, internal heating is due to radioactive elements. The mantle
viscosity of the first and third pairs is 10(21) is, while the mantle
of the second pair has a viscosity of 10(22) Pa s. The thermal coupli
ng of the core and mantle has strong effects on the thermal boundary l
ayer near the core-mantle boundary but only minor effects on the therm
al boundary layer near the surface. It cools the core, substantially w
eakens the thermal boundary layer near the core-mantle boundary, and t
hus reduces the vigor of convection in the mantle. The models with coo
ling cores result in a substantially colder and relatively less dynami
c mantle than the models with a fixed temperature at the core-mantle b
oundary which overestimates temperatures in the mantle.