Interior dynamics and thermal evolution of Mars – a geodynamic perspective
نویسندگان
چکیده
Over the past decades, global geodynamic models have been used to investigate thermal evolution of terrestrial planets. With increase computational power and improvement numerical techniques, these become more complex, simulations are now able use a high resolution 3D spherical shell geometry account for strongly varying viscosity, as appropriate mantle materials. In this study we review that interior dynamics Mars. We discuss how can be combined with local observations constrain planet's history. particular, recent InSight estimates crustal thickness, upper structure, core size show constraints improve our understanding dynamics, present-day state temperature variations in Our results thickness control surface heat flow elastic pattern, well location melting zones martian mantle. The lithospheric seismic velocities pattern shallow reflect pattern. large leads smaller scale convection than previously suggested. Strong plumes produce melt up times focused Tharsis Elysium, while weaker distributed throughout seismogenic layer, where events occur, discriminate between models, if source depth is known. Furthermore model predictions seismicity compared values measured by InSight. Future need consider from lithosphere at north pole Mars, effects lateral on waves propagation through lithosphere, test spatial distribution comparing observations.
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ژورنال
عنوان ژورنال: Advances in Geophysics
سال: 2022
ISSN: ['0065-2687', '2162-7622']
DOI: https://doi.org/10.1016/bs.agph.2022.07.005