Journal
NATURE GEOSCIENCE
Volume 14, Issue 1, Pages 51-+Publisher
NATURE RESEARCH
DOI: 10.1038/s41561-020-00673-1
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- US National Aeronautics and Space Administration through the NASA Astrobiology Institute through the Science Mission Directorate [NNA15BB03A]
- US National Aeronautics and Space Administration through the Science Mission Directorate [80NSSC19M0069]
- US National Science Foundation [EAR-1753916]
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Due to limited geological data, our understanding of Earth's landscape during the Archaean eon is restricted, but our research suggests that high internal heating in the mantle may have led to seafloor shallowing and landmass exposure.
Given the scarcity of geological data, knowledge of Earth's landscape during the Archaean eon is limited. Although the continental crust may have been as massive as present by 4 Gyr ago, the extent to which it was submerged or exposed is unclear. One key component in understanding the amount of exposed landmasses in the early Earth is the evolution of the oceanic lithosphere. Whereas the present-day oceanic lithosphere subsides as it ages, based on numerical models of mantle convection we find that higher internal heating due to a larger concentration of radioactive isotopes in the Archaean mantle halted subsidence, possibly inducing seafloor shallowing before 2.5 Gyr ago. In such a scenario, exposed landmasses in the form of volcanic islands and resurfaced seamounts or oceanic plateaus can remain subaerial for extended periods of time, and may have provided the only stable patches of dryland in the Archaean. Our results therefore permit a re-evaluation of possible locations for the origin of life, as they provide support to an existing hypothesis that suggests that life had its origins on land rather than in an oceanic environment. In contrast to present-day seafloor subsidence with age, there may have been Archaean seafloor shallowing and landmass exposure due to high internal heating in the mantle that halted subsidence, according to numerical models of mantle convection.
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