Origin of the RNA World: The Fate of Nucleobases in Warm Little Ponds
Ben K. D. Pearce, Ralph E. Pudritz, Dmitry A. Semenov, Thomas K., Henning

TL;DR
This study models the early Earth's warm little ponds to understand how nucleobases from meteorites led to the rapid formation of RNA, suggesting RNA appeared within a few years after meteorite deposition, prior to 4.17 billion years ago.
Contribution
The paper presents a comprehensive numerical model coupling Earth's early environment with prebiotic chemistry, highlighting the rapid emergence of RNA from meteoritic nucleobases in wet-dry cycles.
Findings
RNA polymers emerged within a few years after meteorite deposition.
Nucleobases were primarily meteoritic, not from interplanetary dust.
RNA likely appeared before 4.17 billion years ago.
Abstract
Prior to the origin of simple cellular life, the building blocks of RNA (nucleotides) had to form and polymerize in favourable environments on the early Earth. At this time, meteorites and interplanetary dust particles delivered organics such as nucleobases (the characteristic molecules of nucleotides) to warm little ponds whose wet-dry cycles promoted rapid polymerization. We build a comprehensive numerical model for the evolution of nucleobases in warm little ponds leading to the emergence of the first nucleotides and RNA. We couple Earth's early evolution with complex prebiotic chemistry in these environments. We find that RNA polymers must have emerged very quickly after the deposition of meteorites (< a few years). Their constituent nucleobases were primarily meteoritic in origin and not from interplanetary dust particles. Ponds appeared as continents rose out of the early global…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
