T148 Birth and Death of Supercontinents
Monday, 20 October 2014
1:00 PM - 5:00 PM
118
EARTH EVOLUTION AND SUPERCONTINENTS
Paper number: T148-9
Program: Technical Sessions
Time: 3:05 PM – 3:25 PM
Authors
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Chris J. HawkesworthUniversity of St Andrews, St Andrews, N/A
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Bruno DhuimeUniversity of St Andrews, St Andrews, N/A
Abstract
We recognize 5 stages of Early evolution: 1) Initial accretion and differentiation of Earth’s core/mantle system within the first few 10’s of million of years; 2) Generation of crust in a pre-plate tectonic regime in the period prior to 3.0 Ga; 3) Early plate tectonics involving hot shallow subduction over the period from 3.0-1.7 Ga; 4) Earth’s middle age from 1.7-0.75 Ga, characterized by environmental, evolutionary and lithospheric stability; 5) Modern cold subduction which has existed for last 0.75 Ga. Supercontinents have operated during the last three stages. This evolving tectonic character has likely been controlled by secular changes in mantle temperature and its resultant impact on lithospheric behavour. Crustal volumes, reflecting the interplay of crustal generation and recycling, increased until Earth’s middle age when they plateaued and have likely been decreasing for the last 0.75 Ga.