Mesozoic-Cainozoic volcanism of Australia

Abstract

Mesozoic—Cainozoic volcanism was concentrated on the youngest eastern Australian craton. Basaltic activity (with some felsic fractionation) has predominated over Mesozoic interludes of calcalkaline volcanism (rhyolites, dacites, trachytes andesites) and more isolated shoshonitic activity (now represented by appinitic, syenitic, granitic and lamprophyric complexes). Epeirogenic movements and associated sea-floor spreading and orogenic episodes at the continental margins, initiated and controlled much of the volcanism. Basin edges, faults, lineaments and their intersections were important in locating sites of volcanism; some fundamental structural lines have focussed volcanism over 300–600 km. The eastern Mesozoic basaltic volcanism shows a late Jurassic N-S trend from undersaturated to saturated compositions, with increasing intensity of melting towards a major Tasmanian-Antarctic thermo-tectonic event. A late Jurassic-late Cretaceous E-W trend may extend from possible ‘kimberlites’ through shoshonitic to calcalkaline activity with increasing proximity to orogenic movements along the New Zealand ‘Geosyncline’. Cainozoic basaltic volcanism reflects the NNE drift of Australia under Atlantic-Indian-Southern Ocean sea-floor spreading, with a debatable role for subduction along the Tasman Sea margin. The ultimate mechanisms of volcanism are not clearly understood. Drift of cratonic structural weaknesses over thermal anomalies in the mantle, with generation of magmas from a geochemically zoned Lower Velocity Zone under influence of uplifts, lithospheric thickness and periodic release of thermal energy, seems to partly explain observed patterns of E. Australian volcanism.