Amino acid photostability on the Martian surface
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Abstract— In the framework of international planetary exploration programs, several space missions are planned to search for organics and bio-signatures on Mars. Previous attempts have not detected any organic compounds in the Martian regolith. It is therefore critical to investigate the processes that may affect organic molecules on and below the planet's surface. Laboratory simulations can provide useful data about the reaction pathways of organic material at Mars' surface. We have studied the stability of amino acid thin films against ultraviolet (UV) irradiation and use those data to predict the survival time of these compounds on and in the Martian regolith. We show that thin films of glycine and D-alanine are expected to have half-lives of 22 ± 5 hr and of 3 ± 1 hr, respectively, when irradiated with Mars-like UV flux levels. Modelling shows that the half-lives of the amino acids are extended to the order of 107 years when embedded in regolith. These data suggest that subsurface sampling must be a key component of future missions to Mars dedicated to organic detection.
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The persistence of possible biosignatures on Mars, both exposed on the surface and within the top few meters of near-subsurface accessible with drills, is likely limited by current hostile environmental conditions: UV photodegrades organics, oxidizing dust attacks molecular biosignatures, and cosmic rays penetrate several meters.
“For example, the persistence of possible biosignatures on Mars, both exposed on the surface and within the top few meters of the near-subsurface that are accessible with drills, is likely to be limited by the current hostile environmental conditions.”
From The Astrobiology Primer v2.0 (2016) · cites this paper as ten Kate et al., 2005
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Organic compounds in carbonaceous meteorites
Sephton, M. A. (2002) · Natural Product Reports · doi:10.1039/b103775g · Cited by 704 · see citing works
Flagged first, then by citations
Research works printed but not linked: 28
- Biemann, 1977, The search for organic substances and inorganic volatile compounds in the surface of Mars, Journal of Geophysical Research, 82, 4641, 10.1029/JS082i028p04641 · DOI
- Bland, 2000, Meteorite accumulations on Mars, Icarus, 144, 21, 10.1006/icar.1999.6253 · DOI
- Botta, 2002, Extraterrestrial organic compounds in meteorites, Surveys in Geophysics, 23, 411, 10.1023/A:1020139302770 · DOI
- Bridges, 1999, Ventifacts at the Pathfinder landing site, Journal of Geophysical Research, 104, 8595, 10.1029/98JE02550 · DOI
- Cao, 1999, New infrared spectra and the tautomeric studies of purine and L-alanine with an innovative sampling technique, Spectrochimica Acta Part A, 55, 2329, 10.1016/S1386-1425(99)00133-X · DOI
- Cao, 2000, Infrared spectra of monomeric L-alanine and L-alanine-N-d3 zwitterions isolated in a KBr matrix, Chemical Physics, 255, 195, 10.1016/S0301-0104(00)00082-3 · DOI
- Carr M. H. 1992. Post-Noachian erosion rates: Implications for Mars climate change. Proceedings, 23rd Lunar and Planetary Science Conference pp. 205-206.
- Cottin, 2003, Photodestruction of relevant interstellar molecules in ice mixtures, The Astrophysical Journal, 590, 874, 10.1086/375149 · DOI
- Ehrenfreund, 2001, The photostability of amino acids in space, The Astrophysical Journal, 550, L95, 10.1086/319491 · DOI
- Ehrenfreund, 2001, Extraterrestrial amino acids in Orgueil and Ivuna: Tracing the parent body of CI type carbonaceous chondrites, Proceedings of the National Academy of Sciences of the United States of America, 98, 2138, 10.1073/pnas.051502898 · DOI
- Ehrenfreund, 2002, Astrophysical and astrochemical insights into the origin of life, Reports on Progress in Physics, 65, 1427, 10.1088/0034-4885/65/10/202 · DOI
- Edwards, 1985, Handbook of optical constants of solids I, 547, 10.1016/B978-0-08-054721-3.50029-0 · DOI
- Flynn, 1990, An assessment of the meteoritic contribution to the martian soil, Journal of Geophysical Research, 95, 14,497, 10.1029/JB095iB09p14497 · DOI
- Ihs, 1990, Infrared and photoelectron spectroscopy of amino acids on copper: Glycine, L-alanine and β-alanine, Journal of Colloid and Interface Science, 140, 192, 10.1016/0021-9797(90)90335-L · DOI
- Oró, 1979, The photolytic degradation and oxidation of organic compounds under simulated martian conditions, Journal of Molecular Evolution, 14, 153, 10.1007/BF01732374 · DOI
- Patel, 2002, Ultraviolet radiation on the surface of Mars and the Beagle 2 UV sensor, Planetary and Space Sciences, 50, 915, 10.1016/S0032-0633(02)00067-3 · DOI · Paper page
- Peeters, 2003, The astrobiology of nucleobases, The Astrophysical Journal, 593, L129, 10.1086/378346 · DOI
- Pierazzo, 1999, Amino acid survival in large cometary impacts, Meteoritics & Planetary Science, 34, 909, 10.1111/j.1945-5100.1999.tb01409.x · DOI
- Quinn, 1999, Peroxide-modified titanium dioxide: A chemical analog of putative martian soil oxidants, Origins of Life and Evolution of the Biosphere, 29, 59, 10.1023/A:1006506022182 · DOI
- Rosado, 1998, Vibrational spectra of acid and alkaline glycine salts, Vibrational Spectroscopy, 16, 35, 10.1016/S0924-2031(97)00050-7 · DOI
- Rozenberg, 2003, Low-temperature Fourier transform infrared spectra and hydrogen bonding in polycrystalline L-alanine, Spectrochimica Acta Part A, 59, 3253, 10.1016/S1386-1425(03)00159-8 · DOI
- Skelley, 2005, Development and evaluation of a microdevice for amino acid biomarker detection and analysis on Mars, Proceedings of the National Academy of Sciences of the United States of America, 102, 1041, 10.1073/pnas.0406798102 · DOI
- Stoker, 1997, Organic degradation under simulated Martian conditions, Journal of Geophysical Research, 102, 10,881, 10.1029/97JE00667 · DOI
- Kate, 2003, Investigating complex organic compounds in a simulated Mars environment, International Journal of Astrobiology, 1, 387, 10.1017/S1473550403001277 · DOI
- Uvdal, 1990, X-ray photoelectron and infrared spectroscopy of glycine adsorbed upon copper, Journal of Colloid and Interface Science, 140, 207, 10.1016/0021-9797(90)90336-M · DOI
- Yamaguchi, 2005, Terahertz absorption spectra of L-, D-, and DL-alanine and their application to determination of enantiometric composition, Applied Physics Letters, 86, 10.1063/1.1857080 · DOI
- Zent, 1994, The chemical reactivity of the martian soil and implications for future missions, Icarus, 108, 146, 10.1006/icar.1994.1047 · DOI
- Zent, 2003, Mars atmospheric oxidant sensor (MAOS): An in situ heterogeneous chemistry analysis, Planetary and Space Science, 51, 167, 10.1016/S0032-0633(02)00204-0 · DOI
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Domagal-Goldman, S. D., Wright, K. E., Domagal-Goldman, S. D., Wright, K. E., Adamala, K., Arina de la Rubia, L., Bond, J., Dartnell, L. R., Goldman, A. D., Lynch, K., et al. (2016) · Astrobiology · doi:10.1089/ast.2015.1460 · Cited by 136 · see citing works
“On the martian surface, the unshielded flux of solar UV light rapidly photodegrades exposed organic molecules (ten Kate et al., 2005; Shkrob et al., 2010; Dartnell et al., 2012), the strongly oxidizing conditions of the wind-blown dust layer would chemically attack molecular biosignatures (Benner…”
Simulating Martian Regolith in the Laboratory
Seiferlin, K., Ehrenfreund, P., Garry, J., Gunderson, K., Hütter, E., Kargl, G., Maturilli, A., & Merrison, J. P. (2008) · Planetary and Space Science · doi:10.1016/j.pss.2008.09.017 · Cited by 77 · see citing works
Self-citation
- Authors
- KATE, I. L., GARRY, J. R. C., PEETERS, Z., QUINN, R., FOING, B., & EHRENFREUND, P.
- Affiliations
- Leiden University (NL)
- European Space Research and Technology Centre (NL)
- Venue
- Meteoritics & Planetary Science
- Publisher
- Wiley
- Published
- 2005-08
- Volume
- 40
- Issue
- 8
- Pages
- 1185-1193
- ISSN
- 1086-9379 (ISSN-L)
- 1945-5100
- OpenAlex
- W1971726793
- Cited by
- 151
- References
- 1
- Citations by year
- 2026: 8 · 2025: 9 · 2024: 6 · 2023: 6 · 2022: 7 · 2021: 9 · 2020: 6 · 2019: 3 · 2018: 9 · 2017: 5 · 2016: 8 · 2015: 9 · 2014: 9 · 2013: 8 · 2012: 10
- FWCI
- 2.32
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- Meteoritics and Planetary Science (publishedVersion)
- UA Campus Repository (The University of Arizona) (acceptedVersion)
- Funders
- National Aeronautics and Space Administration
- Universiteit Leiden
- Nederlandse Organisatie voor Wetenschappelijk Onderzoek (016.023.003)
- Ames Research Center
- Topics
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Planetary Science and Exploration
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Space Science and Extraterrestrial Life
- Keywords
- glycine, D-alanine, UV irradiation, Martian regolith, organic preservation, half-life, subsurface sampling, biosignatures, thin films
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