Frederick L. Sutherland

This study reviews the Meso–Cenozoic tectonic paleo-reconstructions for the East Asian and western North American continental margins, focusing on strike-slip tectonics. It follows previous studies by the present and other authors, which investigated the Cretaceous turn of geological evolution (CTGE). They largely studied significant changes in the Earth’s mineralization, magmatism and climate. The present study focuses on significant changes related to the Earth’s rotation velocity. This question is significant not only for fundamental science, but also for applied geology, because CTGE is marked by abundant ore and energetic resources. The results show domination of sinistral shearing on the NE-oriented Asian margin during the pre-early Cretaceous time that turned to significant development of dextral movements in the mid Cretaceous–Cenozoic time. On the NW-oriented American margin, significant development of sinistral movements in the pre-early Cretaceous time turned to domination of dextral shearing during late Cretaceous and Cenozoic. These tectonic changes indicate the transition of the Earth’s rotation from the accelerating towards decelerating regime after CTGE (135–120 Ma). This change may be caused by the transition of the Earth’ mass to, and then, away from the polar regions, the processes being related to melting and freezing of the ice caps.

This study reviews the available data on the Phanerozoic plume activity (Large Igneous Provinces (LIP’s) size and frequency) and geochemistry of their igneous rocks. A major goal of this review is to try to find the changes in intensity and geochemistry of mantle plumes linked to the Earth’s evolution and galactic seasonality that was supposed in the authors’ previous publications. The data indicate that the Cambrian–Ordovician and Jurassic–Cretaceous galactic summers were associated with peaks of various igneous activities including both plume- and subduction/collision-related magmatism, while the Carboniferous–Permian and current galactic winters led to significant drops within the igneous activity. The materials subducted into the transitional and lower mantle, which highly influenced the plume magmas in the galactic-summer times, were less significant in the galactic spring and autumn seasons. The least subduction-influenced LIPs were probably the Tarim and Emeishan deep plume magmas that developed in the mid–late Permian, during the galactic late winter–early spring subseason. The Fe enrichment of clinopyroxenite, gabbro, and associated ores of these provinces might be caused by fluids ascending from the core–mantle boundary. However, the most significant core influence through plume-associated fluids on the surface of solid Earth is supposed to have occurred in the galactic summer times (Cambrian–Ordovician and Jurassic–Cretaceous), which is indicated by peak abundances of ironstone ores. Their contributions to the Cambrian–Ordovician and Jurassic–Cretaceous plume magmas were, however, obscured by more significant influences from subduction.

This study tests the hypothesis of Cretaceous Turn of Geological Evolution (CTGE). It uses the large dataset on mineral deposits of NE Asia compiled by the US Geological Survey in collaboration with Russian, Mongolian, Korean, and Japanese geological institutions. As predicted, the Triassic–Early Jurassic and Late Cretaceous–Paleogene geodynamic activities in NE Asia were simple, producing a relatively small amount of mineral deposits (94 and 132, respectively). In contrast, the greatly increased geodynamic activity around CTGE produced a huge amount of mineral deposits (288). The Jurassic–Early Cretaceous superplume-related melts were injected into accretionary wedges that formed along the Pacific–Eurasian margins, whereas adakitic and granitic magmas derived from the shallow slab and lower crust were intruded into the huge intracontinental region. The characteristic mineral deposits are represented by the unique Jurassic–Early Cretaceous plume-related Ti-Fe-V (+P + Cr-PGE + Au + diamond) ores. Other CTGE representatives are the porphyry Cu-Mo and Au (+Ag)-vein deposits, which formation, however, continued into the Late Cretaceous–Paleogene epoch. These deposits were generated by the slab- and crust-derived adakitic and granitic melts formed under influence of the expiring superplume and intensifying subduction. The Late Cretaceous–Paleogene epoch is indicated by a decreasing metallogenic activity in general, and an increasing role of subduction-related deposits in particular.

Ruby as a natural gemstone has an early history in which its colorful properties

(2019). Re-appraisal of published nitrogen aggregation results in diamonds from Copeton, New South Wales. Australian Journal of Earth Sciences. Ahead of Print.

Within the Lorne Basin, Mesozoic granitoid plutons and dacitic to rhyolitic extrusions form extensive components in a faulted, eroded Triassic sedimentary basin. Late Cenozoic plugs and flows of evolved basalts represent easterly extensions of the eroded Comboyne Volcano. The basin marks a terminal outpost of the New England Orogen, much modified by later alkaline felsic intrusions and flow remnants. Many origins are invoked for its tectonic genesis and magmatic evolution including plate tectonic, caldera and even meteoritic impact events. This review uses extended field study, zircon fission track, K–Ar and Ar–Ar age-dating, petrography and geochemical analyses on igneous suites. These results are combined with previously published and unpublished studies to clarify relationships between volcanic and plutonic suites, structural features and paleotopographic developments, allowing for an enlarged synthesis of Lorne Basin magmatism and its tectonic contexts. Dating reveals rhyodacitic volcanism began at ca 221 Ma (Milligans Road) and culminated in emplacements of I- and A-type dioritic to granitic suites (North Brother, Middle Brother) at ca 217–212 Ma (MAGMATIC EPISODE 1, late Triassic). Voluminous alkaline rhyolitic feeders and flows (Bago Range, Batar Creek) erupted between ca 187 and 160 Ma (MAGMATIC EPISODE 2, early–mid-Jurassic). Lavas infilled extended drainages cut into a dissected, faulted terrain and disrupted former drainage patterns. An alkaline monzodioritic to granitic pluton and late-stage rhyolitic dyke swarm (South Brother) were emplaced at ca 126 and 119 Ma (MAGMATIC EPISODE 3, early Cretaceous). This chemically distinct magmatism coincided with thermal coastal faulting along eastern Australia. A large eroded plug and dyke complex (Mount Lorne) shows steep flow banding and lies within dissected radial flow infillings. This prominent eruptive conduit tapped a significant ring fault system. Although undated, its petrography resembles features related to MAGMATIC EPISODE 3. The study revealed a far greater profusion of rhyolitic feeders and flows than previously thought, making likely volcanic volumes within episodes difficult to estimate. The youngest volcanic remnants infill later drainages, are dated between ca 17 and 13 Ma (MAGMATIC EPISODE 4, mid-Neogene), and are evolved derivatives related to the adjacent Comboyne central volcano. Some evolved basalts contain feldspathic and mafic crystallisations indicating mid-crustal melt processes. These bimodal suites represent a traverse over an asthenospheric plume during northward lithospheric migration of eastern Australia. Minor vitrophyric bodies recorded across the Lorne Basin only intrude Carboniferous basement beds. Their origin and age are enigmatic and represent a final puzzle to solve in the evolution of Lorne Basin magmatism.

Dykes are common in the wave-cut platforms along the coast from Newcastle to Sydney. According to some authors, they may be related to the opening of the Tasman Sea that commenced ca 84 Ma ago. However, there are few detailed radiogenic dating and geochemical studies to evaluate this. We attempt to resolve this by K–Ar dating of plagioclase in and geochemical studies of, basaltic dykes intruding Permo-Triassic sequences on the wave-cut platforms and Carboniferous and Permo-Triassic sequences inland. The plagioclase separated from the dykes give K–Ar ages ranging from 266 to 53 Ma with the majority older than 84 Ma indicating that most dykes were emplaced before the Tasman Seafloor formation. The dykes are generally mildly alkaline, high-Ti basalts; fewer are tholeiitic and calc-alkaline, low-Ti basalts. Strongly light rare earth element (LREE)-enriched patterns typify the former and flat, LREE-depleted or slightly to moderately enriched LREE patterns, the latter. High-Ti basalts have ocean-island-basalt-like and low-Ti basalts, calc-alkaline or mid-ocean ridge basalt (MORB)-like patterns. Most high-Ti and some low-Ti basalts show plume-like characteristics, others N-type MORB and arc-like characteristics. Dykes intruding the Carboniferous sequences show a distinct contamination signature that could be crustal or due to subduction-related metasomatism of the subcontinental lithospheric mantle. The sources of the basaltic magmas vary substantially and in places changes with time. All alkali basalts are derived from enriched asthenospheric sources at varying depths (90–147 km) and most tholeiitic, low-Ti basalts have been extracted from asthenospheric and depleted asthenospheric–lithospheric sources indicating substantial compositional heterogeneity of the mantle. Further, Nd model ages varying from Neoproterozoic (940–580 Ma) to Paleozoic (460–370 Ma) suggest variation in the age of mantle sources for the basalts.

Ruby in diverse geological settings leaves petrogenetic clues, in its zoning, inclusions, trace elements and oxygen isotope values. Rock-hosted and isolated crystals are compared from Myanmar, SE Asia, and New South Wales, East Australia. Myanmar ruby typifies metasomatized and metamorphic settings, while East Australian ruby xenocrysts are derived from basalts that tapped underlying fold belts. The respective suites include homogeneous ruby; bi-colored inner (violet blue) and outer (red) zoned ruby; ruby-sapphirine-spinel composites; pink to red grains and multi-zoned crystals of red-pink-white-violet (core to rim). Ruby ages were determined by using U-Pb isotopes in titanite inclusions (Thurein Taung; 32.4 Ma) and zircon inclusions (Mong Hsu; 23.9 Ma) and basalt dating in NSW, >60–40 Ma. Trace element oxide plots suggest marble sources for Thurein Taung and Mong Hsu ruby and ultramafic-mafic sources for Mong Hsu (dark cores). NSW rubies suggest metasomatic (Barrington Tops), ultramafic to mafic (Macquarie River) and metasomatic-magmatic (New England) sources. A previous study showed that Cr/Ga vs. Fe/(V + Ti) plots separate Mong Hsu ruby from other ruby fields, but did not test Mogok ruby. Thurein Taung ruby, tested here, plotted separately to Mong Hsu ruby. A Fe-Ga/Mg diagram splits ruby suites into various fields (Ga/Mg < 3), except for magmatic input into rare Mogok and Australian ruby (Ga/Mg > 6). The diverse results emphasize ruby’s potential for geographic typing.