| Literature DB >> 29062973 |
Abstract
Some fundamental molecules of life are suggested to have been formed, proliferated, and evolved through photochemical microscopic dissipative structuring and autocatalytic proliferation under the UV-C/UV-B solar environment prevalent at Earth's surface throughout the Archean. Evidence is given in the numerous salient characteristics of these, including their strong absorption in this spectral region and their rapid non-radiative excited state decay through inherent conical intersections. The examples of the dissipative structuring and dissipative proliferation of the purines and of single strand DNA are given. UV-C and UV-B-induced stationary state isomerizations and tautomerizations are shown to be crucial to the formation of the purines from hydrogen cyanide in an aqueous environment under UV-C light, while UV-C induced phosphorylation of nucleosides and denaturing of double helix RNA and DNA are similarly important to the production and proliferation of single strand DNA. This thermodynamic dissipation perspective provides a physical-chemical foundation for understanding the origin and evolution of life.Entities:
Keywords: Biochemistry; Evolution; Microbiology; Quantum mechanics; Statistical physics; Thermodynamics
Year: 2017 PMID: 29062973 PMCID: PMC5647473 DOI: 10.1016/j.heliyon.2017.e00424
Source DB: PubMed Journal: Heliyon ISSN: 2405-8440
Fig. 1The wavelengths of maximum absorption of many of the fundamental molecules of life (common to all three domains) coincide with a predicted atmospheric window in the UV-C at the time of the origin of life at 3.85 Ga and until at least 2.9 Ga (red and green curves respectively). By 2.2 Ga (light blue curve) the UV-C light at Earth’s surface had been extinguished by the oxygen and ozone resulting from organisms performing oxygenic photosynthesis. The dark blue curve corresponds to the present day surface spectrum. The font size of the letter roughly indicates the relative size of the molar extinction coefficient of the indicated fundamental molecule (pigment). Image credit; adapted from (Michaelian and Simeonov, 2015).
Fig. 2Generic photochemical pathway to the purines first discovered by Ferris and Orgel (1966). Four molecules of HCN are transformed into the smallest stable oligomer (tetramer) of HCN, known as cis-2,3-diaminomaleonitrile (cis-DAMN), (1), which, under a constant UV-C photon flux isomerizes into trans-DAMN (2) (also called diaminofumaronitrile, DAFN) which may be further converted on absorbing two more UV-C photons into an imidazole intermediate, 4-amino-1H-imidazole-5-carbonitrile, AICN (3), which through thermal reaction with another HCN molecule forms a purine, in this case adenine (4). Image credit: Boulanger et al. (2013), adapted from Ferris and Orgel (1966), reprinted with permission.
Fig. 3The sequence of photochemical and chemical reactions that lead from cis-DAMN at (1) to trans-DAMN at (4) to AIAC at (5) to AICN at (19). The solid arrows correspond to the forward reactions and the dotted arrows to possible backward reactions. The upward facing arrows indicate where photon absorption (> 4 eV, UV-C) is required for the reaction to proceed. Image credit: Boulanger et al. (2013), reprinted with permission.
Fig. 4There are in general three internal coordinates involved in the photoisomerization of cis- to trans-DAMN. The first is the rotation angle θ about the CC double bond, and the second is the pyramidalization coordinate ф of the C1′ carbon atom defined as the angle between the C—N bond and the plane defined by the C1C1′—C2′ plane, and the third is the elongation of the C—N bond. Image credit: Adapted from Szabla et al. (2014), reprinted with permission.
Steps in the photochemical reaction pathway leading from 4HCN to adenine according to Boulanger et al. (2013) (see Fig. 3). The wavelength at which isomerization to the following step was observed in experiment, λisom, as well as the quantum yield, Φ, for the photochemical conversions is given. Also given is the wavelength of maximum absorption, λmax, of the molecule and the corresponding molar extinction, ε, in an aqueous environment. All referenced values are experimental except (1) and (9) which are calculations at the CASPT2//SA-2-CASSCF(2,2)/cc-pVTZ and (TD)CAM-B3LYP/aug-cc-pVTZ levels respectively.
| Step ( | Molecule | λisom (nm) | Φ | λmax (nm) | ε (M–1 cm−1) |
|---|---|---|---|---|---|
| – | 4HCN | thermal | |||
| 1 | cis-DAMN | 254 (4) | 0.045 (2) | 290 (1), 298 (2), | 14,000 (2), |
| 295 (4), | 12,000 (4), | ||||
| 295 (8) | 13,500 (8) | ||||
| 4 | trans-DAMN | <325 (4) | 0.0034 (2) | 326 (1), 313 (2) | 8,500 (2), |
| 314 (4), 310 (7) | 8,000 (5) | ||||
| 5 | AIAC | 275 (9) | – | 255–290 (4) | – |
| 19 | AICN | thermal | 250 (2) | 10,700 (2), | |
| 247 (3) | |||||
| 245–250 (4), 246 (7) | 11,000 (3) | ||||
| – | adenine | 260 (6) | 14,000 (6) | ||
| 261 (10) | 13,400 (10) | ||||
| 259 (11) | 15,040 (11) |
References; (1) Szabla et al., 2014, (2) Koch and Rodehorst, 1974, (3) Ferris and Orgel, 1966, (4) Becker et al., 1973 (22 °C), (5) Sanchez et al., 1967, (6) Clark et al., 1965, (7) Yamada et al., 1968, (8) Ferris and Kuder, 1970, (9) Boulanger et al., 2013, (10) Fasman, 1975, (11) Cavaluzzi and Borer, 2004.