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                                                          Stagnant Lid
                                   Early                    Intermediate                    Late






                     Magma       Partial Melt                             Lithosphere
                                                   drips    Rayleigh-Taylor   Asthenosphere
                                                        plumes  drips  upwelling and
                                                                      melting
                     Convecting
                         Mantle


                     Core
                                       Io               Venus          Mars            Moon, Mercury




                        Possible Stages                                                Crust
                         in the Tectonic                                               Lithosphere

                         Evolution of a                       Plate
                          Silicate Body                    Tectonics                   Asthenosphere

                            and Earth


                   Figure 1. Possible evolution of magmatotectonic styles for a large silicate body like Earth. Examples from active Solar
                   System bodies Io, Venus, and Mars are shown. Possible evolution of Earth is also shown. Strength of mantle convection is
                   indicated by arrowed curve thickness. Plate tectonics requires certain conditions of lithospheric density and strength in
                   order to occur and is likely to be presaged and followed by different styles of stagnant lid tectonics. See text for further
                   discussion. Modified after Stern et al. (2018).


         perienced multiple episodes of different   p. 58) admonition “… recycling of crust into   tectonics. The second approach is more dif-
         kinds of single-lid behavior and of plate tec-  the mantle does not necessarily require sub-  ficult because we are only beginning to think
         tonics. Different tectonic regimes produce   duction, and it may be possible for such   about what kinds of rocks should be pro-
         different structures, metamorphic rocks,   recycling to occur in stagnant [single]-lid   duced by active single-lid tectonics.
         and igneous rocks that, if preserved, pro-  regimes…” should be kept in mind.  Consider the negative evidence first.
         vide evidence about the tectonic regime that                           Stern (2018) identified three groups of rocks
         produced them. Erosion, alteration, and   EVIDENCE THAT THE            and minerals that only form by plate-tectonic
         burial destroy some but not all of the evi-  MESOPROTEROZOIC WAS A     processes. These are (1) ophiolites, indi-
         dence of past tectonic regimes, at least for   PROTRACTED SINGLE-LID EPISODE  cators of subduction initiation and seafloor
         the past 3 Ga. Erosion may remove shallow   Geologic evidence—both negative and   spreading; (2) blueschists, lawsonite-bear-
         features such as porphyry copper deposits   positive—should guide our interpretation of   ing metamorphic rocks, and jadeitite,
         and  ophiolite  nappes but  cannot  extirpate   Mesoproterozoic tectonics. Negative evi-  indicators of subduction; and (3) ultra-high
         intrusive and metamorphic rocks, which   dence shows an absence of key plate-tectonic   pressure (UHP) metamorphic rocks along
         extend to depth. Microscopic, geochemical,   indicators (Figs. 2B–2D). Positive evidence   with ruby and sapphire, indicators of conti-
         and isotopic evidence is useful for identify-  specifies geologic features expected for sin-  nent-continent collision (Figs. 2B–2D). All
         ing when a change occurred in Earth’s con-  gle-lid behavior (Figs. 2E–2H). The first   of these are abundant in Phanerozoic and
         vective  style  but cannot  reliably constrain   approach is straightforward because we   Neoproterozoic time and all are missing
         when plate tectonics began. Condie’s (2018,   know the kinds of rocks produced by plate   from the Mesoproterozoic. Brown and
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