Mantle Dynamics of Super-Earth Extrasolar Planet under Extreme Temperature and Pressure Conditions Extreme Temperature and Pressure conditions

Physics

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1729 Planetology, 1744 Tectonophysics

Scientific paper

The recent discovery of an extrasolar planet with a mass 7.5 times that of the Earth has opened up new possibilities for planetary modelling because of the higher temperature T ( up to around 10,000 K ) and greater pressures P( up to 1,000 MPa ) involved. We have modelled the dynamics of this planet under these extreme conditions with an extended Boussinesq approximation , using a cartesian 2-D model. Rayleigh numbers of the order of 10**7 have been considered.Both the spinel to perovskite and perovskite to post-perovskite phase transitions have been accounted for, as well as temperature-dependent thermal conductivity, where the phonon, photon and electron thermal conductivities have been included because of the high T and P conditions. A strongly decreasing thermal expansivity for post-perovskite phase , varying by a factor of 20 across the super-earth mantle, has been included. These results reveal a tremendous difference in the style of mantle convection between constant and thermal conductivity models, all other parameters being kept the same. Temperature-dependent thermal conductivity, especially that of electron carriers, helps to develop obese plumes, even in the presence of a small value of thermal expansivity in the deep mantle, whereas weak convection is developed at the base of the mantle with constant thermal conductivity.

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