The Great Oxidation Event signals the first large-scale oxygenation of the atmosphere roughly 2.4 Gyr ago. Geochemical signals diagnostic of oxidative weathering, however, extend as far back as 3.3-2.9 Gyr ago. 3.8-3.7 Gyr old rocks from Isua, Greenland stand as a deep time outpost, recording information on Earth's earliest surface chemistry and the low oxygen primordial biosphere. Here we find fractionated Cr isotopes, relative to the igneous silicate Earth reservoir, in metamorphosed banded iron formations (BIFs) from Isua that indicate oxidative Cr cycling 3.8-3.7 Gyr ago. Elevated U/Th ratios in these BIFs relative to the contemporary crust, also signal oxidative mobilization of U. We suggest that reactive oxygen species were present in the Eoarchean surface environment, under a very low oxygen atmosphere, inducing oxidative elemental cycling during the deposition of the Isua BIFs and possibly supporting early aerobic biology.
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http://dx.doi.org/10.1038/srep21058 | DOI Listing |
Nature
September 2024
Géosciences Montpellier, Université de Montpellier, CNRS, Montpellier, France.
The nitrogen isotopic composition of sedimentary rocks (δN) can trace redox-dependent biological pathways and early Earth oxygenation. However, there is no substantial change in the sedimentary δN record across the Great Oxidation Event about 2.45 billion years ago (Ga), a prominent redox change.
View Article and Find Full Text PDFSci Rep
March 2024
Institute of Energy, Peking University, Beijing, 100871, China.
Resolving the role of galactic processes in Solar System/Earth events necessitates a robust temporal model. However, astrophysical theory diverges with models varying from long-lasting spiral density waves with uniform pattern speeds and arm structures to others with fleeting and unpredictable features. Here, we address those issues with (1) an analysis of patterns of impact periodicity over periods of 10 to 250 million years (Myr) using circular statistics and (2), an independent logarithmic spiral arm model fitted to arm tangents of 870 micron dust.
View Article and Find Full Text PDFNature
November 2023
Astrophysics Science Division, NASA Goddard Space Flight Center, Greenbelt, MD, USA.
The majority of massive disk galaxies in the local Universe show a stellar barred structure in their central regions, including our Milky Way. Bars are supposed to develop in dynamically cold stellar disks at low redshift, as the strong gas turbulence typical of disk galaxies at high redshift suppresses or delays bar formation. Moreover, simulations predict bars to be almost absent beyond z = 1.
View Article and Find Full Text PDFNature
October 2022
Department of Astronomy and Theoretical Physics, Lund Observatory, Lund, Sweden.
Stephan's Quintet (SQ, co-moving radial distance = 85 ± 6 Mpc, taken from the NASA/IPAC Extragalactic Database (NED)) is unique among compact groups of galaxies. Observations have previously shown that interactions between multiple members, including a high-speed intruder galaxy currently colliding into the intragroup medium, have probably generated tidal debris in the form of multiple gaseous and stellar filaments, the formation of tidal dwarfs and intragroup-medium starbursts, as well as widespread intergalactic shocked gas. The details and timing of the interactions and collisions remain poorly understood because of their multiple nature.
View Article and Find Full Text PDFProc Natl Acad Sci U S A
October 2022
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109.
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