Macquarie Island: A window into the oceanic crust and upper mantle

• Other Authors: CAWOOD, PETER (hasPrincipalInvestigator), CAWOOD, PETER (processor), Australian Antarctic Data Centre (publisher)
• Format: Dataset
• Language: unknown
• Published: Australian Antarctic Data Centre
• Subjects: geoscientificInformation; oceans; OCEAN CRUST DEFORMATION; EARTH SCIENCE; SOLID EARTH; GRAVITY/GRAVITATIONAL FIELD; CRUSTAL MOTION; MACQUARIE ISLAND; MID-OCEAN RIDGES; OCEANIC LITHOSPHERE; OPHIOLITES; SHEETED DYKES; OCEAN > SOUTHERN OCEAN; SOUTHERN OCEAN > GEOGRAPHIC REGION > POLAR; Southern Ocean; Macquarie Island
• Online Access: https://researchdata.ands.org.au/macquarie-island-window-upper-mantle/699574; https://data.aad.gov.au/metadata/records/ASAC_1208; http://nla.gov.au/nla.party-617536

Because of the inaccessibility of the deep-ocean floor, our knowledge about the composition and structure of the oceanic crust is very limited. Macquarie Island is the only fragment of ocean crust exposed above sea-level in the world, providing a unique opportunity to study the ocean crust directly in unprecedented detail. From the abstract of the referenced paper: Macquarie Island preserves largely in-situ Miocene oceanic crust and mantle formed at a slow-spreading ridge. The crustal section on the island does not conform to a simple 'layer cake pseudo-stratigraphy', but is the result of multiple magmatic episodes. Macquarie Island crust did not grow by top-down cooling, but rather from the base up. Peridotites cooled first and formed the basement into which gabbro plutons were intruded. This was followed by cooling and deformation, and by intrusion of dykes that fed a sheeted dyke-basalt complex. Finally, lava filled grabens were formed. These relative age relations rule out simple co-genetic relations between rock units.