Tectonic Regimes of Terrestrial Planets & Exoclimes

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If Convective Stress < Lithosphere Yield Then Upper Layer Stagnates Single Plate Planet (e.g., Present Day Venus and Mars) Horizontal Surface Velocity For Mobile Plate Regime: Convective Stress > Lithosphere Yield
Active Lid Episodic surface velocity time Stagnant Lid
Page 1: Tectonic Regimes of Terrestrial Pla
Page 4 and 5: Numerical Simulation Subducting Sla
Page 8 and 9: Plate Tectonic (mobile lid) Regime
Page 10 and 11: Plate Tectonic Regime Episodic Regi
Page 12 and 13: Changing Tectonic Regimes over Time
Page 14 and 15: Will Super Sized Earths Have Plate
Page 16 and 17: Will Super Sized Earths Have Plate
Page 18 and 19: Super Earths will not have plate te
Page 20 and 21: The Notion of Well Defined Tectonic
Page 22 and 23: Active Lid (plate tectonics) Episod
Page 24 and 25: Stagnant Lid (single plate planet)
Page 26 and 27: Artist's impression of a ”Super E
Page 29 and 30: Notion of Plate Tectonics Being Key
Page 31: Atmospheric Signature of Tectonic R

Tectonic Regimes of Terrestrial Planets & Exoclimes

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