TL;DR
This study explores the potential formation of ribose, a key RNA component, inside carbonaceous planetesimals through the formose reaction, supported by laboratory experiments and theoretical modeling, suggesting an extraterrestrial origin for life's building blocks.
Contribution
It presents a combined experimental and theoretical investigation demonstrating that ribose could be synthesized within planetesimals, providing new insights into the origin of life's building blocks.
Findings
Calculated ribose abundances match measurements in meteorites.
Laboratory yields support the feasibility of in-situ ribose synthesis.
Ribose could be preserved and delivered to early Earth.
Abstract
The origin of life might be sparked by the polymerization of the first RNA molecules in Darwinian ponds during wet-dry cycles. The key life-building block ribose was found in carbonaceous chondrites. Its exogenous delivery onto the Hadean Earth could be a crucial step toward the emergence of the RNA world. Here, we investigate the formation of ribose through a simplified version of the formose reaction inside carbonaceous chondrite parent bodies. Following up on our previous studies regarding nucleobases with the same coupled physico-chemical model, we calculate the abundance of ribose within planetesimals of different sizes and heating histories. We perform laboratory experiments using catalysts present in carbonaceous chondrites to infer the yield of ribose among all pentoses (5Cs) forming during the formose reaction. These laboratory yields are used to tune our theoretical model that…
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