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Did transit through the galactic spiral arms seed crust production on the early Earth?

Version 4 2024-03-12, 20:31
Version 3 2023-10-29, 17:46
journal contribution
posted on 2024-03-12, 20:31 authored by C.L. Kirkland, Phil SuttonPhil Sutton, T. Erickson, T.E. Johnson, M.I.H. Hartnady, H. Smithies, M. Prause
<p>Although there is evidence for periodic geological perturbations driven by regular or semi-regular extra-terrestrial bombardment, the production of Earth’s continental crust is generally regarded as a function of planetary differentiation driven by internal processes. We report time series analysis of the Hf isotopic composition of zircon grains from the North Atlantic and Pilbara cratons, the archetypes of Archean plate tectonic and non-plate tectonic settings, respectively. An ~170–200 m.y. frequency is recognized in both cratons that matches the transit of the solar system through the galactic spiral arms, where the density of stars is high. An increase in stellar density is consistent with an enhanced rate of Earth bombardment by comets, the larger of which would have initiated crustal nuclei production via impact-driven decompression melting of the mantle. Hence, the production and preservation of continental crust on the early Earth may have been fundamentally influenced by exogenous processes. A test of this model using oxygen isotopes in zircon from the Pilbara craton reveals correlations between crust with anomalously light isotopic signatures and exit from the Perseus spiral arm and entry into the Norma spiral arm, the latter of which matches the known age of terrestrial spherule beds. Our data support bolide impact, which promoted the growth of crustal nuclei, on solar system transit into and out of the galactic spiral arms.</p>

History

School affiliated with

  • School of Mathematics and Physics (Research Outputs)

Publication Title

Geology

Publisher

Geological Society of America

ISSN

0091-7613

eISSN

1943-2682

Date Submitted

2022-08-30

Date Accepted

2022-06-29

Date of First Publication

2022-08-25

Date of Final Publication

2022-08-25

Date Document First Uploaded

2022-08-29

ePrints ID

50578

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