The thermo-chemical evolution of a one-plate planet like Mars strongly influences its atmospheric evolution via volcanic outgassing, which is linked to the production of partial melt in the mantle. In earlier thermal evolution and convection models melt production has been considered by the release and consumption of latent heat, the formation of crust and the redistribution of radioactive heat sources. We present thermo-chemical 2D convection models that examine the influence of partial melt on the mantle dynamics of a one-plate planet such as Mars. Assuming fractional melting, where melt leaves the system as soon as it is formed, cooling boundary conditions and decaying radioactive elements, we investigate the effects of partial melt on t...
Mantle convection is the method of heat elimination for silicate mantles in terrestrial bodies, prov...
Mantle convection is the method of heat elimination for silicate mantles in terrestrial bodies, prov...
Observations of asteroid belt members, investigations of meteorites and thermal evolution models con...
The impact heat accumulated during the late stage of planetary accretion can melt a significant part...
The total amount of melt produced in Mars during its evolution is estimated by means of a parameter...
The total amount of melt produced in Mars during its evolution is estimated by means of a parameter...
Convection in planetary mantles is driven by buoyancy that results from density variation...
The energy sources involved in the early stages of the formation of terrestrial bodies can induce pa...
The energy sources involved in the early stages of the formation of terrestrial bodies can induce pa...
International audienceThe energy sources involved in the early stages of the formation of terrestria...
The energy sources involved in the early stages of the formation of terrestrial bodies can induce pa...
International audienceThe energy sources involved in the early stages of the formation of terrestria...
International audienceThe energy sources involved in the early stages of the formation of terrestria...
The energy sources involved in the early stages of the formation of terrestrial bodies can induce pa...
International audienceThe energy sources involved in the early stages of the formation of terrestria...
Mantle convection is the method of heat elimination for silicate mantles in terrestrial bodies, prov...
Mantle convection is the method of heat elimination for silicate mantles in terrestrial bodies, prov...
Observations of asteroid belt members, investigations of meteorites and thermal evolution models con...
The impact heat accumulated during the late stage of planetary accretion can melt a significant part...
The total amount of melt produced in Mars during its evolution is estimated by means of a parameter...
The total amount of melt produced in Mars during its evolution is estimated by means of a parameter...
Convection in planetary mantles is driven by buoyancy that results from density variation...
The energy sources involved in the early stages of the formation of terrestrial bodies can induce pa...
The energy sources involved in the early stages of the formation of terrestrial bodies can induce pa...
International audienceThe energy sources involved in the early stages of the formation of terrestria...
The energy sources involved in the early stages of the formation of terrestrial bodies can induce pa...
International audienceThe energy sources involved in the early stages of the formation of terrestria...
International audienceThe energy sources involved in the early stages of the formation of terrestria...
The energy sources involved in the early stages of the formation of terrestrial bodies can induce pa...
International audienceThe energy sources involved in the early stages of the formation of terrestria...
Mantle convection is the method of heat elimination for silicate mantles in terrestrial bodies, prov...
Mantle convection is the method of heat elimination for silicate mantles in terrestrial bodies, prov...
Observations of asteroid belt members, investigations of meteorites and thermal evolution models con...