On the Role of $^{40}$K in the Origin of Terrestrial Life
Giovanni Vladilo

TL;DR
This paper explores how the radioactive isotope $^{40}$K may have influenced the origin of life on Earth by providing a moderate, persistent radiation environment that could drive molecular evolution and enantiomeric excess in prebiotic conditions.
Contribution
It introduces the potential role of $^{40}$K's decay in prebiotic chemistry and biological homochirality, emphasizing its less disruptive yet significant impact compared to other radionuclides.
Findings
$^{40}$K radiation could induce enantiomeric excess in amino acids.
Estimated radiation doses from $^{40}$K align with prebiotic dry-wet scenarios.
$^{40}$K's decay may have contributed to molecular evolution on early Earth.
Abstract
The abundance and biological role of potassium suggest that its unstable nuclide was present in all stages of terrestrial biogenesis. With its enhanced isotopic ratio in the Archean eon, K may have contributed to the special, perhaps unique, biogenetic conditions that were present in the primitive Earth. Compared to the U and Th radionuclides, K has a less disruptive radiochemical impact, which may drive a moderate, but persistent evolution of the structural and functional properties of proto-biological molecules. In the main -decay route of K, the radiation dose generated by an Archean solution with potassium ions can be larger than the present background radiation on Earth by one to two orders of magnitude. Estimates of the rates of organic molecules indirectly affected by decays are provided for two schematic models of the propagation of secondary…
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