Why supercontinents became shorter lived as the Earth evolved

Periodic assembly and break-up of supercontinents since at least two billion years ago (Ga), dubbed the supercontinent cycle, provides the first-order tectonic control on the evolution of the Earth System including episodic orogenic events, mineralization, the formation and closure of oceans and sup...

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Main Authors: Huang, Chuan, Li, Zheng-Xiang
Format: Journal Article
Language:English
Published: 2023
Subjects:
Online Access:http://purl.org/au-research/grants/arc/FL150100133
http://hdl.handle.net/20.500.11937/90600
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author Huang, Chuan
Li, Zheng-Xiang
author_facet Huang, Chuan
Li, Zheng-Xiang
author_sort Huang, Chuan
building Curtin Institutional Repository
collection Online Access
description Periodic assembly and break-up of supercontinents since at least two billion years ago (Ga), dubbed the supercontinent cycle, provides the first-order tectonic control on the evolution of the Earth System including episodic orogenic events, mineralization, the formation and closure of oceans and superoceans, and even the evolution of life. However, the lifespan of the supercontinents appears to decrease with time, from ∼300 million years (Myr) for Nuna/Columbia, to 200-250 Myr for Rodinia and ∼150 Myr for the youngest supercontinent Pangaea. To understand what caused such a secular decrease in supercontinental lifespan, we conduct 3-D geodynamic modeling using realistic tectonic settings. The results show that the yield stress of newly formed orogens during the assembly of a supercontinent provides the dominant control on the lifespan of the supercontinent, implying that the yield stress of young orogens becomes lower with time. We hypothesize that the decreasing mantle temperature due to Earth's secular cooling might have caused new orogens to become weaker.
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spelling curtin-20.500.11937-906002023-03-27T05:02:39Z Why supercontinents became shorter lived as the Earth evolved Huang, Chuan Li, Zheng-Xiang Secular cooling Supercontinental lifespan Yield stress Young orogens Periodic assembly and break-up of supercontinents since at least two billion years ago (Ga), dubbed the supercontinent cycle, provides the first-order tectonic control on the evolution of the Earth System including episodic orogenic events, mineralization, the formation and closure of oceans and superoceans, and even the evolution of life. However, the lifespan of the supercontinents appears to decrease with time, from ∼300 million years (Myr) for Nuna/Columbia, to 200-250 Myr for Rodinia and ∼150 Myr for the youngest supercontinent Pangaea. To understand what caused such a secular decrease in supercontinental lifespan, we conduct 3-D geodynamic modeling using realistic tectonic settings. The results show that the yield stress of newly formed orogens during the assembly of a supercontinent provides the dominant control on the lifespan of the supercontinent, implying that the yield stress of young orogens becomes lower with time. We hypothesize that the decreasing mantle temperature due to Earth's secular cooling might have caused new orogens to become weaker. 2023 Journal Article http://hdl.handle.net/20.500.11937/90600 10.1016/j.scib.2023.01.035 eng http://purl.org/au-research/grants/arc/FL150100133 http://creativecommons.org/licenses/by-nc-nd/4.0/ fulltext
spellingShingle Secular cooling
Supercontinental lifespan
Yield stress
Young orogens
Huang, Chuan
Li, Zheng-Xiang
Why supercontinents became shorter lived as the Earth evolved
title Why supercontinents became shorter lived as the Earth evolved
title_full Why supercontinents became shorter lived as the Earth evolved
title_fullStr Why supercontinents became shorter lived as the Earth evolved
title_full_unstemmed Why supercontinents became shorter lived as the Earth evolved
title_short Why supercontinents became shorter lived as the Earth evolved
title_sort why supercontinents became shorter lived as the earth evolved
topic Secular cooling
Supercontinental lifespan
Yield stress
Young orogens
url http://purl.org/au-research/grants/arc/FL150100133
http://hdl.handle.net/20.500.11937/90600