Influence of the UV Environment on the Synthesis of Prebiotic Molecules
Open accessAbstract
Ultraviolet radiation is common to most planetary environments and could play a key role in the chemistry of molecules relevant to abiogenesis (prebiotic chemistry). In this work, we explore the impact of UV light on prebiotic chemistry that might occur in liquid water on the surface of a planet with an atmosphere. We consider effects including atmospheric absorption, attenuation by water, and stellar variability to constrain the UV input as a function of wavelength. We conclude that the UV environment would be characterized by broadband input, and wavelengths below 204 nm and 168 nm would be shielded out by atmospheric CO2 and water, respectively. We compare this broadband prebiotic UV input to the narrowband UV sources (e.g., mercury lamps) often used in laboratory studies of prebiotic chemistry and explore the implications for the conclusions drawn from these experiments. We consider as case studies the ribonucleotide synthesis pathway of Powner et al. (2009) and the sugar synthesis pathway of Ritson and Sutherland (2012). Irradiation by narrowband UV light from a mercury lamp formed an integral component of these studies; we quantitatively explore the impact of more realistic UV input on the conclusions that can be drawn from these experiments. Finally, we explore the constraints solar UV input places on the buildup of prebiotically important feedstock gasses like CH4 and HCN. Our results demonstrate the importance of characterizing the wavelength dependence (action spectra) of prebiotic synthesis pathways to determine how pathways derived under laboratory irradiation conditions will function under planetary prebiotic conditions.
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DNA is most damaged by wavelengths shorter than 290 nm.
“However, it has been observed that wavelengths below 290 nm are most damaging to DNA, and that the Archean Earth would have experienced a higher flux of shorter-wavelength UV radiation though water and atmospheric carbon dioxide may have efficiently blocked wavelengths much below 200 nm (Cockell 1998;Ranjan and Sasselov 2016).”
From Environmental Adaptation from the Origin of Life to the Last Universal Common Ancestor (2018) · cites this paper as Ranjan and Sasselov 2016
UV is thought to have played a significant role in prebiotic synthesis, including the synthesis of uracil and cytosine.
“Despite UV's potentially deleterious effects on life, UV is thought to have played a significant role in prebiotic synthesis (eg., Ranjan and Sasselov 2016;Beckstead et al. 2016;Sutherland 2017), and plays a key role in the prebiotic synthesis of uracil and cytosine achieved by Powner et al. (2009), an important achievement in understanding the prebiotic emergence of RNA.”
From Environmental Adaptation from the Origin of Life to the Last Universal Common Ancestor (2018) · cites this paper as Ranjan and Sasselov 2016
The Archean Earth likely received more short-wavelength UV radiation.
“However, it has been observed that wavelengths below 290 nm are most damaging to DNA, and that the Archean Earth would have experienced a higher flux of shorter-wavelength UV radiation though water and atmospheric carbon dioxide may have efficiently blocked wavelengths much below 200 nm (Cockell 1998;Ranjan and Sasselov 2016).”
From Environmental Adaptation from the Origin of Life to the Last Universal Common Ancestor (2018) · cites this paper as Ranjan and Sasselov 2016
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Bonfio, C., Valer, L., Scintilla, S., Shah, S., Evans, D. J., Jin, L., Szostak, J. W., Sasselov, D. D., Sutherland, J. D., & Mansy, S. S. (2017) · Nature Chemistry · doi:10.1038/nchem.2817 · Cited by 158 · see citing works
Self-citationDeal, A. M., Rapf, R. J., & Vaida, V. (2021) · The Journal of Physical Chemistry A · doi:10.1021/acs.jpca.1c02864 · Cited by 105 · see citing works
Nitrogen Oxide Concentrations in Natural Waters on Early Earth
Ranjan, S., Todd, Z. R., Rimmer, P. B., Sasselov, D. D., & Babbin, A. R. (2019) · Geochemistry, Geophysics, Geosystems · doi:10.1029/2018gc008082 · Cited by 94 · see citing works
Self-citationMimicking the Surface and Prebiotic Chemistry of Early Earth Using Flow Chemistry
Ritson, D. J., Battilocchio, C., Ley, S. V., & Sutherland, J. D. (2018) · Nature Communications · doi:10.1038/s41467-018-04147-2 · Cited by 89 · see citing works
Supply of phosphate to early Earth by photogeochemistry after meteoritic weathering
Ritson, D. J., Mojzsis, S. J., & Sutherland, J. D. (2020) · Nature Geoscience · doi:10.1038/s41561-020-0556-7 · Cited by 78 · see citing works
Environmental Adaptation from the Origin of Life to the Last Universal Common Ancestor
Cantine, M. D., & Fournier, G. P. (2018) · Origins of Life and Evolution of Biospheres · doi:10.1007/s11084-017-9542-5 · Cited by 54 · see citing works
A Continuous Reaction Network that Produces RNA Precursors
Yi, R., Tran, Q. P., Ali, S., Yoda, I., Adam, Z. R., Cleaves, H. J., & Fahrenbach, A. C. (2020) · Proceedings of the National Academy of Sciences · doi:10.1073/pnas.1922139117 · Cited by 45 · see citing works
Radicals in Prebiotic Chemistry
Lim, R. W. J., & Fahrenbach, A. C. (2020) · Pure and Applied Chemistry · doi:10.1515/pac-2020-0805 · Cited by 8 · see citing works
- Authors
- Ranjan, S., & Sasselov, D. D.
- Affiliations
- Center for Astrophysics Harvard & Smithsonian (US)
- ORCID
- Ranjan, Sukrit
- Venue
- Astrobiology
- Publisher
- SAGE Publications
- Published
- 2016-01
- Volume
- 16
- Issue
- 1
- Pages
- 68-88
- ISSN
- 1531-1074 (ISSN-L)
- 1557-8070
- OpenAlex
- W1955599522
- Cited by
- 159
- References
- 94
- Citations by year
- 2026: 14 · 2025: 15 · 2024: 16 · 2023: 11 · 2022: 15 · 2021: 20 · 2020: 17 · 2019: 17 · 2018: 14 · 2017: 18 · 2016: 2
- FWCI
- 8.12
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- Astrobiology (publishedVersion)
- PubMed (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Origins and Evolution of Life
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Space Science and Extraterrestrial Life
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
- Keywords
- ultraviolet radiation, prebiotic chemistry, origin of life, water attenuation, stellar variability, mercury lamp irradiation, ribonucleotide synthesis, sugar synthesis, methane, hydrogen cyanide, planetary atmospheres, liquid water
- MeSH terms
- Origin of Life, Carbon Dioxide, Environment, Methane, Photolysis, Ultraviolet Rays, Solar System
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