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A Planetary View of Mesozoic Plate Tectonics in the Previous HitGulfNext Hit of Previous HitMexicoNext Hit*

By

Richard H. Fillon1

 

Search and Discovery Article #30032 (2005)

Posted April 24, 2005

 

*Adapted from extended abstract prepared for presentation at AAPG International Conference & Exhibition, Cancun, Previous HitMexicoNext Hit, October 24-27, 2004. 

1Earth Studies Group, New Orleans, LA 70131 ([email protected])

 

Introduction 

In many respects the geology of the Previous HitGulfNext Hit of Previous HitMexicoNext Hit is better understood than other comparable marginal seas due primarily to its long history of drilling and reflection seismic acquisition by the petroleum industry. However, the petroleum accumulations and thick Tertiary section that attract industry also restrict scientific ocean drilling. To date only the carbonate margin of the southern Previous HitGulfNext Hit and Quaternary fans in the deep eastern basin have been targeted. Discovering new details of the nature and timing of the opening of the Previous HitGulfNext Hit basin, therefore, presents a considerable challenge. The goal of this ongoing study is to determine whether the opening of the Previous HitGulfNext Hit of Previous HitMexicoNext Hit is a predictable manifestation of the planetary-scale superswell-related mantle stresses that drive the movements of major plates and to evaluate implications for Previous HitGulfNext Hit of Previous HitMexicoNext Hit petroleum systems.  

Predicting microplate kinematics within the poorly defined boundary zone that separates North Atlantic and South Atlantic spreading is pivotal in this analysis. It is postulated that the movements of continental microplates in the Previous HitGulfNext Hit of Previous HitMexicoNext Hit are driven by mantle stresses that moved first North America and then South America away from Africa.

 

uIntroduction

uFigure captions

uPlate tectonics

uReconstructions

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

uIntroduction

uFigure captions

uPlate tectonics

uReconstructions

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

uIntroduction

uFigure captions

uPlate tectonics

uReconstructions

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

uIntroduction

uFigure captions

uPlate tectonics

uReconstructions

 

 

 

 

 

 

 

 

 

 

 

 

Figure and Table Captions

Figure 1. Plate tectonic reconstruction for the Late Oxfordian (inset at left) showing plate boundaries and hotspot tracks (fixed positions with respect to Africa). A/S= the African/South American Plate; N= the North American Plate; b= the Bahamas Microplate; K= the Kula Plate; m= Mexican block. The Yucatan Rift Valley which evolved in the Jurassic between North America and Yucatan received marine incursions from the south supporting shallow-water Smackover carbonate source-rock deposition. A center of Smackover source-rock deposition active in the eastern Previous HitGulfNext Hit Basin was separate as indicated in the AAPG COSUNA correlation chart for the northern Previous HitGulfNext Hit Basin (inset lower right). Smackover equivalent strata from South Texas (at left) to northern Florida (at right) is bracketed between dashed lines.

Figure 2. By about 94 Ma BP (late Cenomanian ~MCSB time) the western Previous HitGulfNext Hit of Previous HitMexicoNext Hit was fully open. However, in the Late Aptian - Cenomanian the predicted passage of a Beata-Aves Ridge Hotspot beneath the western basin and implied subduction between the Yucatan microplate and South Florida may have elevated existing Greater Antillean blocks, thus restricting interchange with the Proto-Caribbean and Atlantic. Restricted circulation would have favored source-rock deposition. In this figure ch= the Chiapas Microplate; F = the Faralon Plate; pC= the Proto-Caribbean Plate; A= the African Plate; S= the South American Plate. The familiar modern outlines of Cuba and Hispaniola, provided for reference, include exotic terranes that came together in the Cenozoic.  

Click to view in sequence plate reconstructions for Late Jurassic and late Cenomanian.

Table 1. Implications for Previous HitGulfNext Hit of Previous HitMexicoNext Hit petroleum systems.

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Mesozoic Plate Tectonics 

While there is a considerable volume of published seismic and biostratigraphic data that provides credible evidence of Triassic - Jurassic rifting around virtually the entire Previous HitGulfNext Hit margin, compelling evidence of significant pre-Berriasian (Jurassic) plate movements related to seafloor spreading and ocean crust formation is lacking. Although several seismic stratigraphic studies that transect the northeastern and western margins of the deep Previous HitGulfNext Hit Basin suggest a Jurassic age for the oldest basin-filling sediments, interpreting Callovian (late Middle Jurassic) Louann Salt as autochthonous. It is equally plausible that the salt is allochthonous, having been included in the base of large superficial detachments containing post-synrift - pre-drift strata of Late Jurassic and earliest Cretaceous age deposited originally on attenuated continental crust of Previous HitGulfNext Hit Rim. The Sea of Cortez (Previous HitGulfNext Hit of California) provides a well documented analog for this type of margin failure during early opening. Observations of Jurassic strata overlying undated oceanic crust therefore do not directly imply a Jurassic crustal age.  

Outcropping and drilled Mesozoic strata of the Previous HitGulfNext Hit rim, the presence of buried plume-related alkalic basaltic volcanoes of middle and Late Cretaceous age, and the geometric requirement that the Yucatan Platform be rotated into a position along the Texas - Louisiana margin to allow the reassembly of Pangea are the principal constraints on the origin of the Previous HitGulfNext Hit of Previous HitMexicoNext Hit. There is general agreement among researchers that the opening of the western basin of the Previous HitGulfNext Hit of Previous HitMexicoNext Hit reflects the counterclockwise rotation of a Yucatan microplate. Following recently published paleomagnetic evidence the Chiapas portion of the Maya Block is treated as a separate microplate in this study. It is recognized that the rotation of a Yucatan microplate about the relatively well-known Euler rotation poles that opened the North Atlantic Ocean cannot account for the most probable trajectory of Yucatan. Published opening solutions designed to provide an ideal Yucatan trajectory are purely kinematic, not addressing the implications of a unique Previous HitGulfNext Hit of Previous HitMexicoNext Hit stress field on planetary-scale mantle processes that drive plate motions. Departing from a purely kinematic solution for Yucatan microplate motion, this study focuses on a rotation geometry linked to the stresses that moved the major North and South American plates. Details of the predicted timing and direction of Yucatan microplate rotation thus depend on the changing relative positions of the well known North Atlantic and South Atlantic Euler (rotation) poles. Comparison of North and South Atlantic rotation poles and the history of Berriasian to Barremian (Neocomian) rifting between South America and Africa, which heralded development of a South Atlantic stress field, directly imply a post-late Berriasian (Cretaceous) opening of the western Previous HitGulfNext Hit of Previous HitMexicoNext Hit. Application of the South Atlantic opening pole positions and angular velocities to the opening of the western Previous HitGulfNext Hit of Previous HitMexicoNext Hit further predicts that Yucatan microplate rotation was mostly completed by early Aptian time (~109 Ma BP).  

The new Previous HitGulfNext Hit of Previous HitMexicoNext Hit microplate kinematics proposed here predicts that most Previous HitGulfNext Hit of Previous HitMexicoNext Hit seafloor (~60 %) was created during the Early Cretaceous period of stable geomagnetic polarity (120.4 - 83.5 Ma BP). The absence of obvious magnetic lineations in the deep western basin is therefore a predictable element of Previous HitGulfNext Hit evolution. A further consequence of post-Berriasian opening of the western Previous HitGulfNext Hit of Previous HitMexicoNext Hit is that the thick succession of Norphlet to Cotton Valley sediments that built-up on thick Louann Salt (Callovian) in Oxfordian to early Berriasian time were likely to have destabilized as Yucatan moved away from the Texas-Louisiana margin. The movement of large superficial detachments into the nascent Previous HitGulfNext Hit Basin would have covered virtually all of the oldest (Berriasian to earliest Aptian) oceanic crust located nearest the basin margin. Magnetic spreading anomalies M10N to M0 would thus have been strongly diminished or completely destroyed. In applying a Previous HitGulfNext Hit of California model, the superficial detachment phase in the western Previous HitGulfNext Hit of Previous HitMexicoNext Hit Basin began with the first plate movements initiated by mantle stresses and therefore very likely coincided with the development of the deeper crustal detachments that are characteristic of the early stages of asymmetric continental fragmentation.  

Analysis of dated oceanic plateau basalt accumulations and the inferred tracks of related mantle plumes indicate that two hotspots transited the central Previous HitGulfNext Hit of Previous HitMexicoNext Hit basin during the Late Mesozoic. By holding mantle plumes fixed relative to Africa, a procedure considered valid for Atlantic hotspots, tracks are predicted that pass through the Previous HitGulfNext Hit of Previous HitMexicoNext Hit at critical times in its evolution. One hotspot, recorded in conjugate oceanic plateau basalts of the Ceara and Sierra Leone Rises in the Central Atlantic, is traced to a Triassic position within the Central Atlantic Magmatic Province underlying the Bahamas and central Cuban microplates. The Ceara-Sierra Leone Rise hotspot exited the Previous HitGulfNext Hit through South Florida in the Jurassic as North America began moving away from Africa. The second important Previous HitGulfNext Hit of Previous HitMexicoNext Hit hotspot is recorded in accumulations of oceanic plateau basalts that comprise the Beata and Aves Ridges in the Eastern Caribbean. The Beata-Aves Ridge hotspot entered the Previous HitGulfNext Hit region through West Texas, passing beneath the Rio Grande Rift in the Barremian. It was centered in the western Previous HitGulfNext Hit basin in the middle Cenomanian and exited the basin beneath Yucatan in the early Campanian. The Bermuda hotspot is also important for explaining regional geology. It transited north of the Previous HitGulfNext Hit basin proper, passing beneath the Mississippi Embayment in Turonian through Campanian time. Alkalic basalts of the northern Previous HitGulfNext Hit Rim, which date between 110 and 60 Ma BP, probably record the combined effects of the Beata-Aves Ridge and Bermuda hotspots. The northern end of the modern Caribbean Arc may be pinned at the present location of the Beata-Aves Ridge hotspot.

 

Plate Reconstructions 

Examples of Previous HitGulfNext Hit Basin evolution constrained by this new planetary view of microplate motion are provided in a series of plate reconstructions that begin with the development of a rift valley system that breaks the Yucatan Platform off the North American Plate (Figure 1) and ends with a fully opened Previous HitGulfNext Hit of Previous HitMexicoNext Hit Basin (Figure 2). Implications for the petroleum systems of the Previous HitGulfTop Basin are outlined in Table 1.  

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