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Shock synthesis of amino acids from impacting cometary and icy planet surface analogues

Abstract

Comets are known to harbour simple ices and the organic precursors of the building blocks of proteins—amino acids—that are essential to life. Indeed, glycine, the simplest amino acid, was recently confirmed to be present on comet 81P/Wild-2 from samples returned by NASA’s Stardust spacecraft. Impacts of icy bodies (such as comets) onto rocky surfaces, and, equally, impacts of rocky bodies onto icy surfaces (such as the jovian and saturnian satellites), could have been responsible for the manufacture of these complex organic molecules through a process of shock synthesis. Here we present laboratory experiments in which we shocked ice mixtures analogous to those found in a comet with a steel projectile fired at high velocities in a light gas gun to test whether amino acids could be produced. We found that the hypervelocity impact shock of a typical comet ice mixture produced several amino acids after hydrolysis. These include equal amounts of D- and L-alanine, and the non-protein amino acids α-aminoisobutyric acid and isovaline as well as their precursors. Our findings suggest a pathway for the synthetic production of the components of proteins within our Solar System, and thus a potential pathway towards life through icy impacts.

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Figure 1: Chromatogram of extracts from shocked ice sample no. 1.
Figure 2: Chromatogram of extracts from shocked ice sample no. 2.
Figure 3: Relative amino acid abundances (glycine = 1) versus increasing carbon number for the linear α-amino acids detected in the target ice sample no. 1 (grey) and target ice sample no. 2 (white).

References

  1. Chyba, C. F., Thomas, P. J., Brookshaw, L. & Sagan, C. Cometary delivery of organic molecules to the early Earth. Science 249, 366–373 (1990).

    Article  Google Scholar 

  2. Chyba, C. F. & Sagan, C. Endogenous production, exogenous delivery and impact-shock synthesis of organic molecules: An inventory for the origins of life. Nature 355, 125–132 (1992).

    Article  Google Scholar 

  3. Anders, E. Prebiotic organic matter from comets and asteroids. Nature 342, 255–257 (1989).

    Article  Google Scholar 

  4. Furukawa, Y., Sekine, T., Oba, M., Kakegawa, T. & Nakazawa, H. Biomolecule formation by oceanic impacts on early Earth. Nature Geosci. 2, 62–66 (2009).

    Article  Google Scholar 

  5. Schidlowski, M. A 3,800-million year isotopic record of life from carbon in sedimentary rocks. Nature 333, 313–318 (1988).

    Article  Google Scholar 

  6. Schopf, J. W. Microfossils of the early Archean apex chert: New evidence of the antiquity of life. Science 260, 640–646 (1993).

    Article  Google Scholar 

  7. Moorbath, S. Palaeobiology: Dating earliest life. Nature 434, 155 (2005).

    Article  Google Scholar 

  8. Bar-Nun, A., Bar-Nun, N., Bauer, S. H. & Sagan, C. Shock synthesis of amino acids in simulated primitive environments. Science 168, 470–473 (1970).

    Article  Google Scholar 

  9. Bar-Nun, A. & Shaviv, A. Dynamics of the chemical evolution of earth’s primitive atmosphere. Icarus 24, 197–210 (1975).

    Article  Google Scholar 

  10. Goldman, N., Reed, E. J., Fried, L. E., William Kuo, I-F. & Maiti, A. Synthesis of glycine-containing complexes in impacts of comets on early Earth. Nature Chem. 2, 949–954 (2010).

    Article  Google Scholar 

  11. Festou, M., Uwe-Keller, H. & Weaver, H. A. Comets-II (Univ. Arizona Press, 2005).

    Google Scholar 

  12. DiSanti, M. A., Bonev, B. P., Villanueva, G. L. & Mumma, M. J. Highly depleted ethane and mildly depleted methanol in Comet 21P/Giacobini-Zinner: Application of a new empirical υ2-band model for CH3OH near 50 K. Astrophys. J. 763, 1–15 (2013).

    Article  Google Scholar 

  13. Crovisier, J. & Bockelée-Morvan, D. Remote observations of the composition of cometary volatiles. Space Sci. Rev. 90, 19–32 (1999).

    Article  Google Scholar 

  14. Ehrenfreund, P. et al. Astrophysical and astrochemical insights into the origin of life. Rep. Prog. Phys. 65, 1427–1487 (2002).

    Article  Google Scholar 

  15. Ehrenfreund, P. & Charnley, S. B. Organic molecules in the interstellar medium, comets, and meteorites: A voyage from dark clouds to the early Earth. Annu. Rev. Astron. Astrophys. 38, 427–483 (2000).

    Article  Google Scholar 

  16. Mumma, M. J. et al. Remote infrared observations of parent volatiles in comets: A window on the early solar system. Adv. Space Res. 31, 2563–2575 (2003).

    Article  Google Scholar 

  17. Bockelée-Morvan, D. et al. New molecules found in cometC/1995 O1 (Hale–Bopp). Investigating the link between cometary and interstellar material. Astron. Astrophys. 353, 1101–1114 (2000).

    Google Scholar 

  18. Elsila, J. E., Glavin, D. P. & Dworkin, J. P. Cometary glycine detected in samples returned by Stardust. Meteorit. Planet. Sci. 44, 1323–1330 (2009).

    Article  Google Scholar 

  19. Blank, J. G., Miller, G. H., Ahrens, M. J. & Winans, R. E. Experimental shock chemistry of aqueous amino acid solutions and the cometary delivery of prebiotic compounds. Orig. Life Evol. B 31, 15–51 (2001).

    Article  Google Scholar 

  20. Pierazzo, E., Kring, D. A. & Melosh, H. J. Hydrocode simulation of the Chicxulub impact event and the production of climatically active gases. J. Geophys. Res. 103, 28607–28625 (1998).

    Article  Google Scholar 

  21. Pierazzo, E. & Chyba, C. F. Amino acid survival in large cometary impacts. Meteorit. Planet. Sci. 34, 909–918 (1999).

    Article  Google Scholar 

  22. Pierazzo, E. & Chyba, C. F. in Comets and the Origins and Evolution of Life II (eds Thomas, P. J., Hicks, R., Chyba, C. F. & McKay, C. P.) 137–168 (Springer, 2006).

    Book  Google Scholar 

  23. Blank, J. G. & Miller, G. H. in Proc. 21st Int. Symp. on Shock Waves (eds Houwing, A. F. P. et al.) 1467–1472 (Panther Press, 1998).

    Google Scholar 

  24. Burchell, M. J., Cole, M. J., McDonnell, J. A. M. & Zarnecki, J. C. Hypervelocity impact studies using the 2 MV Van de Graaff accelerator and two-stage light gas gun of the University of Kent at Canterbury. Meas. Sci. Technol. 10, 41–50 (1999).

    Article  Google Scholar 

  25. Waite, J. H. et al. Liquid water on Enceladus from observations of ammonia and 40Ar in the plume. Nature 460, 487–490 (2009).

    Article  Google Scholar 

  26. Brown, R. H. et al. Composition and physical properties of Enceladus’ surface. Science 311, 1425–1428 (2006).

    Article  Google Scholar 

  27. Clark, R. N. et al. Detection and mapping of hydrocarbon deposits on titan. J. Geophys. Res. 115, E10 (2010).

    Google Scholar 

  28. Merlin, F., Quirico, E., Barucci, M. A. & de Bergh, C. Methanol ice on the surface of minor bodies in the solar system. Astron. Astrophys. 544, A20 (2012).

    Article  Google Scholar 

  29. Shin, B. et al. Methanol incorporation in clathrate hydrates and the implications for oil and gas pipeline flow assurance and icy planetary bodies. Proc. Natl Acad. Sci. USA 110, 8437–8442 (2013).

    Article  Google Scholar 

  30. Kvenvolden, K. et al. Evidence for extraterrestrial amino-acids and hydrocarbons in the Murchison meteorite. Nature 228, 923–926 (1970).

    Article  Google Scholar 

  31. Silfer, J. A., Engel, M. H., Macko, S. A. & Jumeau, E. J. Stable carbon isotope analysis of amino acid enantiomers by conventional isotope ratio mass spectrometry and combined gas chromatography/isotope ratio mass spectrometry. Anal. Chem. 63, 370–374 (1991).

    Article  Google Scholar 

  32. Macko, S. A., Uhle, M. E., Engel, M. H. & Andrusevich, V. Stable nitrogen isotope analysis of amino acid enantiomers by gas chromatography combustion-isotope ratio mass spectrometry. Anal. Chem. 69, 926–929 (1997).

    Article  Google Scholar 

  33. Martins, Z., Alexander, C. M. O’D., Orzechowska, G. E., Fogel, M. L. & Ehrenfreund, P. Indigenous amino acids in primitive CR meteorites. Meteorit. Planet. Sci. 42, 2125–2136 (2007).

    Article  Google Scholar 

  34. Bonner, W. A. The origin and amplification of biomolecular chirality. Orig. Life Evol. Biosphere 21, 59–111 (1991).

    Article  Google Scholar 

  35. Sephton, M. A. Organic compounds in carbonaceous meteorites. Nat. Product Rep. 19, 292–311 (2002).

    Article  Google Scholar 

  36. Cronin, J. R. & Chang, S. in The Chemistry of Life’s Origin (eds Greenberg, J. M., Mendoza-Gomez, C. X. & Pirronello, V.) 209–258 (Kluwer, 1993).

    Book  Google Scholar 

  37. Peltzer, E. T., Bada, J. L., Schlesinger, G & Miller, S. L. The chemical conditions on the parent body of the Murchison meteorite: Some conclusions based on amino, hydroxy, and dicarboxylic acids. Adv. Space Res. 4, 69–74 (1984).

    Article  Google Scholar 

  38. Lerner, N. R., Peterson, E. & Chang, S. The Strecker synthesis as a source of amino acids in carbonaceous chondrites—deuterium retention during synthesis. Geochim. Cosmochim. Acta 57, 4713–4723 (1993).

    Article  Google Scholar 

  39. Price, M. C., Burchell, M. J., Kearsley, A. T. & Cole, M. J. 43rd Lunar and Planetary Science Conf., Abstr. 1755 (2012).

  40. Henkel, T. et al. 43rd Lunar and Planetary Science Conf. Abstr. 2158 (2012).

  41. Parnell, J. et al. The preservation of fossil biomarkers during meteorite impact events: Experimental evidence from biomarker-rich projectiles and target rocks. Meteorit. Planet. Sci. 48, 1340–1358 (2010).

    Article  Google Scholar 

  42. Ostro, S. J. et al. Cassini RADAR observations of Enceladus, Tethys, Dione, Rhea, Iapetus, Hyperion, and Phoebe. Icarus 183, 479–490 (2006).

    Article  Google Scholar 

  43. Thiemann, W. H. P. & Meierhenrich, U. ESA mission ROSETTA will probe for chirality of cometary amino acids. Orig. Life Evol. Biol. 31, 199–200 (2001).

    Article  Google Scholar 

  44. Hartogh, P. et al. Ocean-like water in the Jupiter-family comet 103P/Hartley 2. Nature 478, 218–220 (2011).

    Article  Google Scholar 

  45. Pizzarello, S., Williams, L. B., Lehman, J., Holland, G. P. & Yarger, J. L. Abundant ammonia in primitive asteroids and the case for a possible exobiology. Proc. Natl Acad. Sci. USA 108, 4303–4306 (2011).

    Article  Google Scholar 

  46. The announcement of JUICE as the next L-class ESA mission was made on the 5th May 2012. Available at http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=50400 (accessed 1st June 2012).

  47. Berstein, M. et al. Racemic amino acids from the ultraviolet photolysis of interstellar ice analogues. Nature 416, 401–403 (2002).

    Article  Google Scholar 

  48. Muñoz Caro, G. M. et al. Amino acids from ultraviolet irradiation of interstellar ice analogues. Nature 416, 403–406 (2002).

    Article  Google Scholar 

  49. Meinert, C., Filippi, J. J., de Marcellus, P., Le Sergeant d’Hendecourt, L. & Meierhenrich, U. J. N-(2-Aminoethyl)glycine and amino acids from interstellar ice analogues. ChemPhysChem 77, 186–191 (2012).

    Google Scholar 

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Acknowledgements

We acknowledge financial support from the Science and Technology Facilities Council (STFC). Z. Martins is financially supported by the Royal Society. Many thanks to M. Cole for his technical expertise and for firing the gun, and A. Kearsley and P. Wozniakiewicz for many useful and inspiring discussions.

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Authors

Contributions

M.C.P. made the ice targets and performed the hypervelocity impact-shock experiments. Z.M. performed the amino acid analysis and interpretation. N.G. performed the hydrodynamic simulations of cometary impacts. M.C.P., N.G. and M.J.B. designed the experimental impact study. Z.M. and M.C.P. wrote the article and contributed equally to the study. M.J.B. and M.A.S. provided experimental facilities. All of the authors discussed the results and commented on the manuscript.

Corresponding authors

Correspondence to Zita Martins or Mark C. Price.

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The authors declare no competing financial interests.

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Martins, Z., Price, M., Goldman, N. et al. Shock synthesis of amino acids from impacting cometary and icy planet surface analogues. Nature Geosci 6, 1045–1049 (2013). https://doi.org/10.1038/ngeo1930

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