Models for prebiotic syntheses often have many steps, each separately validated by laboratory experiments. The challenge then asks whether these steps work together in natural geological environments, absent human intervention. Here, we analyze a six-step Discontinuous Synthesis Model (DSM) for the prebiotic formation of RNA, proposed to be the first informational molecule to support Darwinian evolution, and life, on Earth and/or Mars. DSM requires that borate in multiple steps guide the formation of pentoses from simple carbohydrates and control phosphorylation, in all cases by binding adjacent HO-groups on key intermediates. However, adjacent HO-groups must react in two other steps, which borate might inhibit. Experiments here show that borate does not inhibit these two other steps, but rather facilitates them. This makes the six-step DSM a “no human intervention” route from simple
precursors (1 to 3 carbons, 0 to 2 nitrogens) to oligomeric RNA with predominately 3’,5’-linkages at least 6 nucleotides long, but possibly much longer. The process i) exploits privileged chemistry in ii) intermittently irrigated aquifers constrained by basalt that iii) have borate iv) above a redox-neutral mantle v) having access to an atmosphere transiently reduced by a Vesta-sized impactor. In a possible coincidence, such an impact occurred most likely ca. 4.3 billion years ago (Ga), ~100 Mya before some molecular clocks date the divergence of the three kingdoms of life on Earth (4.2 Ga), and ca. 200 Mya before isotopically “light” carbon is reported in zircons dated at 4.1 Ga. This carbon may be the oldest trace of life ever proposed.

By rearranging hydrogen bond donor and acceptor groups within a standard Watson–Crick geometry, DNA can add eight independently replicable nucleotides forming four additional not found in standard Terran DNA. For many applications, the orthogonal pairing of standard and nonstandard pairs offers a key advantage. However, other applications require standard and nonstandard nucleotides to communicate with each other. This is especially true when seeking to recruit high-throughput instruments (e.g., Illumina), designed to sequence standard 4-nucleotide DNA, to sequence DNA that includes added nucleotides. For this purpose, PCR workflows are needed to replace nonstandard nucleotides in (for example) a 6-letter DNA sequence by defined mixtures of standard nucleotides built from 4 nucleotides. High-throughput sequencing can then report the sequences of those mixtures to bioinformatic alignment tools, which infer the original 6-nucleotide sequence by analysis of the mixtures. Unfortunately, the intrinsic orthogonality of standard and nonstandard nucleotides often demand polymerases that violate pairing biophysics to do this replacement, leading to inefficiencies in this “transliteration” process. Thus, laboratory in vitro evolution (LIVE) using “anthropogenic evolvable genetic information systems” (AEGIS), an important “consumer” of new sequencing tools, has been slow to be democratized; robust sequencing is needed to identify the AegisBodies and AegisZymes that AEGIS-LIVE delivers. This work introduces a new way to connect synthetic and standard molecular biology: biversal nucleotides. In an example presented here, a pyrimidine analogue (pyridine-2-one, y) pairs with Watson–Crick geometry to both a nonstandard base (2-amino-8-imidazo-[1,2a]-1,3,5-triazin-[8H]-4-one, P, the Watson–Crick partner of 6-amino-5-nitro-[1H]-pyridin-2-one, Z) and a base that completes the Watson–Crick hydrogen bond pattern (2-amino-2'-deoxyadenosine, amA). PCR amplification of GACTZP DNA with dyTP delivers products where Z:P pairs are cleanly transliterated to A:T pairs. In parallel, PCR of the same GACTZP sample at higher pH delivers products where Z:P pairs are cleanly transliterated to C:G pairs. By allowing robust sequencing of 6-letter GACTZP DNA, this workflow will help democratize AEGIS-LIVE. Further, other implementations of the biversal concept can enable communication across and between standard DNA and synthetic DNA more generally.

Reported here are experiments that show that ribonucleoside triphosphates are converted to polyribonucleic acid when incubated with rock glasses similar to those likely present 4.3-4.4 billion years ago on the Hadean Earth surface, where they were formed by impacts and volcanism. This polyribonucleic acid averages 100-300 nucleotides in length, with a substantial fraction of 3',-5'-dinucleotide linkages. Chemical analyses, including classical methods that were used to prove the structure of natural RNA, establish a polyribonucleic acid structure for these products. The polyribonucleic acid accumulated and was stable for months, with a synthesis rate of 2 x 10^-3 pmoles of triphosphate polymerized each hour per gram of glass (25°C, pH 7.5). These results suggest that polyribonucleotides were available to Hadean environments if triphosphates were. As many proposals are emerging describing how triphosphates might have been made on the Hadean Earth, the process observed here offers an important missing step in models for the prebiotic synthesis of RNA.

While nucleoside 5'-triphosphates are precursors for RNA in modern biology, the presumed difficulty of making these triphosphates on Hadean Earth has caused many prebiotic researchers to consider other activated species for the prebiotic synthesis of RNA. We report here that nickel(II), in the presence of borate, gives substantial amounts (2–3%) of nucleoside 5'-triphosphates upon evaporative heating in the presence of urea, salts, and cyclic trimetaphosphate (CTMP). Also recovered are nucleoside 5'-diphosphates and nucleoside 5'-monophosphates, both likely arising from 5'-triphosphate intermediates. The total level of 5'-phosphorylation is typically 30%. Borate enhances the regiospecificity of phosphorylation, with increased amounts of other phosphorylated species seen in its absence. Experimentally supported paths are already available to make nucleosides in environments likely to have been present on Hadean Earth soon after a midsized 1021 to 1023 kg impactor, which would also have delivered nickel to the Hadean surface. Further, sources of prebiotic CTMP continue to be proposed. Thus, these results fill in one of the few remaining steps needed to demystify the prebiotic synthesis of RNA and support a continuous model from atmospheric components to oligomeric RNA that is lacking only a mechanism to obtain homochirality in the product RNA.