| Literature DB >> 33286709 |
Julián Mejía Morales1, Karo Michaelian2.
Abstract
Ultraviolet light incident on organic material can initiate its spontaneous dissipative structuring into chromophores which can catalyze their own replication. This may have been the case for one of the most ancient of all chromophores dissipating the Archean UVC photon flux, the nucleic acids. Oligos of nucleic acids with affinity to particular amino acids which foment UVC photon dissipation would most efficiently catalyze their own reproduction and thus would have been selected through non-equilibrium thermodynamic imperatives which favor dissipation. Indeed, we show here that those amino acids with characteristics most relevant to fomenting UVC photon dissipation are precisely those with greatest chemical affinity to their codons or anticodons. This could provide a thermodynamic basis for the specificity in the amino acid-nucleic acid interaction and an explanation for the accumulation of information in nucleic acids since this information is relevant to the optimization of dissipation of the externally imposed thermodynamic potentials. The accumulation of information in this manner provides a link between evolution and entropy production.Entities:
Keywords: DNA; RNA; amino acids; entropy; entropy production; information encoding; non-equilibrium thermodynamics; nucleic acids; origin of codons; origin of life; photon potential; stereochemical era
Year: 2020 PMID: 33286709 PMCID: PMC7597208 DOI: 10.3390/e22090940
Source DB: PubMed Journal: Entropy (Basel) ISSN: 1099-4300 Impact factor: 2.524
Figure 1The wavelengths of maximum absorption of many of the fundamental molecules of life (common to all three domains), including the the nucleobases, aromatic and charged amino acids, cofactors, vitamins, and lipids coincide with the predicted solar spectrum at Earth’s surface in the UVC [24] at the time of the origin of life around 3.85 Ga (black line) and until at least 2.9 Ga (red line). The solar spectrum at Earth’s surface today (green line) only has wavelengths greater than about 305 nm due to absorption by ozone in the upper atmosphere. The font size of the pigment name roughly indicates the relative size of its molar extinction coefficient. Adapted from [26].
Figure 2Demonstration of UVC light-induced denaturing of salmon sperm DNA of average length 100 Kbp in pure water (without salt). The temperature of the bath was raised over a time period of 20 min to 40 C and later maintained at this value (±0.01 C) for the duration of the experiment. The graph plots the extinction of the UVC light (due mainly to absorption with a small amount of scattering) by DNA in the wavelength range 255 to 265 nm against time as the UVC light was cycled on and off. The arrows pointing downward mark the time at which the UVC light was blocked from reaching the sample by a shutter and the arrows pointing upwards mark the times at which the light was allowed on sample by removing the shutter. It can be seen that while UVC light is on sample, the extinction increases gradually (after 1/2 h to about 0.3% of the differential absorption - between completely denatured and completely natured) due to the hyperchromicity of sections of single strand DNA arising from UVC light-induced denaturing. While the light was blocked from the sample, the segments renatured, lowering the extinction. The amount of denaturing depends on the intensity of the UVC light and the temperature of the bath. Adapted with permission from Michaelian and Santillán [59].
Figure 3Ultraviolet and Temperature Assisted Reproduction (UVTAR) of RNA and DNA. A mechanism proposed for the enzyme-less reproduction of RNA and DNA assisted by the absorption and dissipation of the prevailing UVC light flux and the high temperatures of the ocean surface during the late Hadean or early Archean, including a day/night diurnal warming and cooling cycle of the water surface due to the absorption of solar infrared light. Most denaturing would occur in the afternoon when ocean surface temperatures were highest. Extension occurs overnight with the aid of Mg ions, UVC activated nucleotides, and colder surface temperatures. “Hyperchromism” refers to an increase (∼35%) in the absorption of photons at UVC wavelengths (∼260 nm) once RNA or DNA are denatured into single strands. Oligos which had chemical affinity to the 10 amino acids listed in the figure (all of which have photon absorption and dissipation fomenting characteristics, see Section 5), would have had a greater chance of denaturing during daylight hours as the surface water cooled, and could therefore be replicated overnight. This selection based on greater photon dissipation we have termed “thermodynamic selection” [7,8,10,21]. The important aspect of this auto-catalytic mechanism is that replication is tied to photon dissipation, providing a thermodynamic imperative for proliferation.
Comparison of the photon dissipation attributes of the common 20 amino acids, classified by hydrophobicity and by electrostatic charge, with their specificity to their codons/anticodons. Those amino acids found by Yarus et al. [45] have a strong (s; probability for non-specificity, Corr ), moderate (m; Corr ), weak (w; Corr ), or very weak (vw; Corr ) specificity of binding with their cognate codons/anticodons (Corr implies no specificity; see Table 1 of [45]) are identified by s,m,w, and vw respectively. Amino acids found by Johnson and Wang [46] to have specificity to their codons or anti-codons are marked with a “+” sign for association with codon/anticodon (in this case, no data is available concerning which of the homologous codons had greatest specificity to the corresponding amino acid). Lysine has also been identified as having high specificity to its anticodon [51,53]. It is striking that those amino acids with specificity also have characteristics relevant to photon dissipation, and, as a consequence, to reproduction through the dissipation-replication mechanism UVTAR. No specificity for codons/anticodons has yet been observed for the other unmarked amino acids as would be expected from their lack of photon dissipation characteristics. The “*” indicates amino acids that absorb in the 260 nm window through charge transfer transitions [66].
| Amino Acid | Abbreviation | Codon | Codon/Anticodon | Amphipathic | Antenna | Intercalating | Catalysis | Charge |
|---|---|---|---|---|---|---|---|---|
| Aliphatic non-polar R group (Hydrophobic) | ||||||||
| Glycine | Gly | GGU | +/ | |||||
| Alanine | Ala | GCU | ||||||
| Proline | Pro | CCU | ||||||
| Valine | Val | GUU | ||||||
| Leucine | Leu | UUA | ||||||
| Isoleucine | Ile | AUU | s/ | |||||
| AUC | +/+ | yes | ||||||
| AUA | /s | |||||||
| methionine | Met | AUG | /+ | yes | yes | |||
| Aromatic R group (Slightly hydrophobic) | ||||||||
| Phenylalanine | Phe | UUU | /vw | yes | yes | |||
| Tyrosine | Tyr | UAU | vw/s | yes | yes | yes | ||
| Tryptophan | Trp | UGG | /s /+ | yes | yes | yes | ||
| Polar R group without charge | ||||||||
| Serine | Ser | UCU | ||||||
| Threonine | Thr | ACU | +/ | |||||
| Cysteine | Cys | UGU | ||||||
| Aspargine | Asn | AAU | ||||||
| Glutamine | Gln | CAA | /+ | |||||
| R group positively charged | ||||||||
| Lysine | Lys | AAA | /s | yes | yes * | yes | yes | |
| Histidine | His | CAU | /vw | yes * | yes | yes | yes | |
| Arginine | Arg | CGU | yes * | yes | yes | |||
| R group negatively charged | ||||||||
| Aspartic acid | Asp | GAU | /+ | yes * | yes | |||
| Glutamic acid | Glu | GAA | +/ | yes * | yes | |||