When did Life Likely Emerge on Earth in an RNA-First Process?
Steven A. Benner, Elizabeth A. Bell, Elisa Biondi, Ramon Brasser,, Thomas Carell, Hyo-Joong Kim, Stephen J. Mojzsis, Arthur Omran, Matthew A., Pasek, Dustin Trail

TL;DR
The paper proposes a model suggesting that Earth's impact history created a window around 4.36 billion years ago when conditions favored the emergence of RNA, supported by geological and atmospheric evidence.
Contribution
It introduces a novel impact-based model linking Earth's impact history to the timing of RNA emergence, integrating physics, geology, and chemistry.
Findings
RNA formation most probable ~4.36 billion years ago
Impact event Moneta created a window for RNA synthesis
Atmospheric and geological conditions supported RNA precursors
Abstract
The widespread presence of ribonucleic acid (RNA) catalysts and cofactors in Earth's biosphere today suggests that RNA was the first biopolymer to support Darwinian evolution. However, most "path-hypotheses" to generate building blocks for RNA require reduced nitrogen-containing compounds not made in useful amounts in the CO2-N2-H2O atmospheres of the Hadean. We review models for Earth's impact history that invoke a single ~10^23 kg impactor (Moneta) to account for measured amounts of platinum, gold, and other siderophilic ("iron-loving") elements on the Earth and Moon. If it were the last sterilizing impactor, Moneta would have reduced the atmosphere but not its mantle, opening a "window of opportunity" for RNA synthesis, a period when RNA precursors rained from the atmosphere to land holding oxidized minerals that stabilize advanced RNA precursors and RNA. Surprisingly, this…
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