Accretionary Complexes: Recorders On Earth And Possibly Mars | 18498
Journal of Earth Science & Climatic Change
Like us on:
Our Group organises 3000+ Global Conferenceseries Events every year across USA, Europe & Asia with support from 1000 more scientific Societies and Publishes 700+ Open Access Journals which contains over 50000 eminent personalities, reputed scientists as editorial board members.
Accretionary complexes occur in parts of the world, highlighted in Japan, North America, Europe, and Greenland. They are
comprehensive data recorders with information compiled while the oceanic crust is en route from the mid-oceanic ridge
to the subduction zone, spanning hundreds of millions of years. At the zone, the oceanic crustal materials are stacked along
thrust faults and/or subducted to be eventually recycled into the mantle. The surviving accretionary-complex materials include
Ocean Plate Stratigraphy (OPS). The ideal succession of the OPS (from oldest to youngest) is mid-ocean ridge basalt (MORB),
pelagic sediment including radiolarian chert, hemipelagic sediment including siliceous shale, and trench turbidite deposits.
Therefore, accretionary complexes often record diverse environmental conditions from deep- to shallow-marine environments,
including those perturbed by endogenic (e.g., magmatic) and exogenic (e.g., impacts and Snowball-Earth) events. During
an ancient and dynamic phase of its evolution (~>3.9 Ga), Mars had Earth-like conditions, including an interacting ocean,
landmass, and atmosphere, referred to as Habitable-Trinity, as well as plate tectonism through geologic investigation of Earth.
A possible accretionary complex and nearby outcrop of steeply dipping beds comprising olistostrome-like blocks, nearby and
in the Claritas rise, respectively, southwest margin of the Tharsis superplume, are key evidence of major crustal shortening
related to plate tectonism. Future investigation of the ancient Martian basement, which includes geochemical analyses for
OPS sequences (an important candidate test), will be the new phase of the geologic investigation of Mars. Such features could
contain far-reaching records dating back more than 4.0 Ga
James M Dohm has investigated the terrestrial planets with major focus on Mars. He has contributed to the publication of USGS I-maps, including the new global
geologic map of Mars (2014), peer-reviewed journal articles, and book publications.
Peer Reviewed Journals
Make the best use of Scientific Research and information from our 700 + peer reviewed, Open Access Journals