The Peninsular Ranges batholith north of latitude 33°N consists of five distinctive longitudinal batholith zones. Four zones are autochthonous—a western zone, western transition zone, eastern transition zone, and an eastern zone. The fifth zone, the upper-plate zone, is allochthonous. The western zone, western transition zone, eastern transition zone, and eastern zone are contiguous products of Cretaceous subduction transitioning from a Mesozoic oceanic-arc setting to continental margin arc setting. Within the autochthonous zones, the nature and geochemistry of plutons record changes reflecting subduction proceeding from west to east over a 35 m.y. period. The allochthonous upper-plate zone is structurally located above the regional Eastern Peninsular Ranges mylonite zone. Host rocks for the western zone, western transition zone, and eastern transition zone are mostly Mesozoic, and host rocks of the eastern zone are Paleozoic. The composition of the plutons reflects changes in magma originating in shallow oceanic crust in the western zone to a deeper continental marginal setting in the eastern zone and upper-plate zone. Several aspects of the upper-plate zone rocks set them apart from the autochthonous batholithic rocks. Western zone magmatism occurred during an extensional subduction phase that involved Mesozoic oceanic crust. Plutons were emplaced passively from 126 Ma to 108 Ma, forming 47.9% of the area of the autochthonous batholith at a rate of 2.7% per million years. Geochemical variation is greater in the western zone than it is in the other zones. Rock compositions range from gabbro to high-SiO 2 granites; plutons in this zone contain magnetite as an accessory mineral. Most plutonic rocks have initial 87 Sr/ 86 Sr (Sr i ) values <0.7045, initial 206 Pb/ 204 Pb (Pb i ) <19, δ 18 O <9‰, and positive initial epsilon Nd (ε Ndi ). By 111 Ma, conditions for pluton emplacement began to change radically from extensional to compressional as subduction encountered older continental crust. The boundary between the western zone and western transition zone is marked clearly by a change in the magnetic properties, which are highly magnetic in the western zone to weakly magnetic in the transition zones. Western transition zone plutons, which have affinities with the western zone plutons, constitute 13.5% by area of the autochthonous batholith and formed over 13 m.y. at a decreased rate of batholith formation, 1% per million years. Plutons of the western transition zone are characterized by Sr i values of 0.7045–0.7050, δ 18 O <9‰, and positive ε Ndi . Deformation of the prebatholithic rocks was intense at 100 Ma, as the plutonism of the western transition zone ended and emplacement in the eastern transition zone began. From 99 to 93 Ma, the rate of magma emplacement accelerated, forming 2.4% per million years by area of the northern part of the autochthonous batholith. The eastern transition zone plutons, having affinities with the eastern zone plutons, have Sr i values of 0.7051–0.7057, δ 18 O >9‰, and negative ε Ndi . Most eastern transition zone plutons were emplaced in a less dynamic setting than the western transition zone plutons. By 98 Ma, subduction had transitioned eastward as plutons were emplaced in continental crust. The rate of magma emplacement increased to form the eastern zone over 7 m.y., or a rate of batholith growth of 3.4% per million years by area. There is considerable temporal overlap in the magma emplacement of the eastern transition zone and the eastern zone. Combined eastern transition zone and eastern zone magmatism produced 39% (by area) of the autochthonous batholith in 8 m.y. at a rate of ~5% per million years. The 102 Ma gabbro body is not considered in this analysis. Eastern zone plutons are characterized by Sr i >0.7060, mostly in the range of 0.7061–0.7076, Pb i >19, δ 18 O >9‰, and a large negative ε Ndi . The allochthonous granitic sheets that constitute the upper-plate zone include batholithic rocks ranging in age from 92 to 75 Ma; most are in the range of 86–75 Ma. These granitic rocks have a more restricted range of geochemistry than those in the other zones; they are magnetite-bearing rocks, unlike the ilmenite-bearing granitic rocks of the transition zones and eastern zone, and they have large negative ε Ndi , and Sr i in the range of 0.7076–0.7084. During the Late Cretaceous, the Eastern Peninsular Ranges mylonite zone developed in the eastern part of the Peninsular Ranges Province, deforming granitic rocks of the eastern part of the eastern zone. Following mylonitization, westward displacement on a series of low-angle thrust faults placed sheets of metamorphic and plutonic rock above the Eastern Peninsular Ranges mylonite zone, forming the upper-plate zone. Compatible elements decrease west to east across the batholith, and incompatible elements increase. Geochemical variation shows that magma forming the western part of the batholith had a shallow and primitive source compared with the eastern part, which had a deeper and more-evolved continental component. The frequency distribution of Sr i in the batholith is bimodal, having a peak of 0.7038 in the western zone, reflecting the oceanic crustal source, and a peak of 0.7072 in the eastern zone, reflecting increased incorporated continental crust sources. Only a small part of the batholith has Sr i values between 0.7055 and 0.7065, indicating a relatively sharp boundary between oceanic and continental crust. Linear arrays on Harker diagram indicate that geochemical variation within the batholith is from magma mixing and not magmatic differentiation. Our data are most simply explained by the Cretaceous arc transitioning from a Mesozoic oceanic-arc setting to a continental margin setting.

We examined numerous coeval mid-Cretaceous intrusions emplaced at different depths into Triassic slate and phyllite to evaluate wall-rock features and contact relations associated with emplacement mechanisms. The pre-emplacement regional deformation of the wall rocks is well characterized, which facilitated clear and unambiguous identification of emplacement-related structures. The depth of intrusion in the different study areas ranged from ~5 to 12 km, which allowed us to examine emplacement mechanisms from the ductile to the brittle regime. Intrusions range in size from dikes and small pods to stocks and plutons up to 90 km 2 in area. Our analyses indicate several important findings: (1) At all depth levels, the pre-emplacement (Jurassic) structural grain of the wall rocks (pervasive foliation, folds at various scales, reverse faults) had significant influence on the geometry and distribution of intrusions. (2) Evaluation of emplacement mechanisms in this study was facilitated by observing several intrusions that offered “snapshots” of different emplacement depths and different levels of the intrusive system (from the roofs to sides). (3) Emplacement mechanisms and intrusion geometry vary with depth, time, and location; as a result, emplacement via multiple mechanisms is pervasive. At the shallowest levels, magma was intruded primarily by diking and merging of dikes via stoping into small stocks that typically had highly irregular wall-rock contacts. Faulting associated with roof uplift and/or cauldron subsidence is locally evident where larger intrusive bodies reside at depth. At intermediate levels, intrusions were emplaced by a combination of stoping and rigid host-rock displacement (roof uplift and lateral flexure), with minor radial expansion. Discordant pluton–wall-rock relations are prevalent, and markedly irregular contacts are still seen, but dikes are much less common. Stoping has removed portions of the intrusion contact aureoles, and has likely obliterated much evidence for processes associated with initial intrusion. At the deepest levels, intrusions are nearly circular in shape and have more common concordant contacts and ductile wall-rock features (synemplacement folding and foliation). These deeper-level stocks were emplaced as diapirs, which then experienced late-stage radial expansion and rigid host-rock displacement (lateral flexure and roof uplift?).