Looking for the origin of life in cosmochemistry: Asteroids and their carbon-rich meteorites
DOI:
https://doi.org/10.7203/metode.6.5000Palabras clave:
Biogenic elements, carbonaceous meteorites, chemical evolution, chirality, chembiogenesisResumen
Carbonaceous chondrite meteorites are carbon-containing fragments of primitive asteroids that have offered the only samples available to date giving insights into chemical evolution in laboratory analyses. Their study has revealed that abundant organic chemistry came to be in the Solar System ahead of terrestrial life and, by the input of these meteorites and comets, might have aided in the origin of our planet’s biochemistry.
Descargas
Citas
Deamer, D. (1985). Boundary structures are formed by organic components of the Murchison carbonaceous chondrite. Nature, 317, 792–794. doi: 10.1038/317792a0
Lerman, L. (2010). The primordial bubble: Water, symmetry breaking, and the origin of life. In R. M. Lyndell-Bell, S. C. Morris, D. Barrow, J. L. Finney, & C. Harper. (Eds.), Water and life: The unique properties of H2O (pp. 259–290). Boca Raton: CRC Press.
Pizzarello, S., Cooper, G. W., & Flynn, G. J. (2006). The nature and distribution of the organic material in carbonaceous chondrites and interplanetary dust particles. In D. Lauretta, & H. Y. McSween Jr (Eds.), Meteorites and the Early Solar System II (pp. 625–651). Tucson: University of Arizona Press.
Pizzarello, S., & Groy, T. L. (2011). Molecular asymmetry in extraterrestrial organic chemistry: An analytical perspective. Geochimica et Cosmochimica Acta, 75, 645–656. doi: 10.1016/j.gca.2010.10.025
Pizzarello, S., Williams, L. B., Lehman, J., Holland, G. P., & Yarger, J. L. (2011). Abundant ammonia in primitive asteroids and the case for a possible exobiology. Proceedings of the National Academy of Sciences, 108, 4303–4306. doi: 10.1073/pnas.1014961108
Schmitt-Kopplin, P., Gabelica, Z., Gougeon, R. D., Fekete, A., Kanawati, B., Harir, M., … Hertkorn, N. (2010). High molecular diversity of extraterrestrial organic matter in Murchison meteorite revealed 40 years after its fall. Proceedings of the National Academy of Sciences, 107, 2763–2768. doi: 10.1073/pnas.0912157107
Von Kiedrowski, G. (Org.). (2005, September 28–October 1). Chembiogenesis: Prebiotic chemistry and early evolution. ECLT: Venice International University. Retrieved from http://www.istpace.org/Web_Final_Report/scientific_meetings_at_eclt/workshops/second_year_april_2005_marc/prebiotic_chemistry_and_ear.html
Wood, J. A., & Chang, S. (Eds.). (1985). The cosmic history of the biogenic elements and compounds. Washington, DC: Scientific and Technical Information Branch, National Aeronautics and Space Administration Publisher.
Yabuta, H., Williams, L. B., Cody, G. D., Alexander, C. M. O’D., & Pizzarello, S. (2007). The insoluble carbonaceous material of CM chondrites: A possible source of discrete organic compounds under hydrothermal conditions. Meteoritics & Planetary Science, 42, 37–48. doi: 10.1111/j.1945-5100.2007.tb00216.x
Zolensky, M. E., Mittlefehldt, D. W., Lipschutz, M. E., Wang, M.-S., Clayton, R. N., Mayeda, T. K., … Barber, D. (1997). CM chondrites exhibit the complete petrologic range from type 2 to 1. Geochimica et Cosmochimica Acta, 61, 5099–5115. doi: 10.1016/S0016-7037(97)00357-8
Descargas
Publicado
Cómo citar
-
Resumen1103
-
PDF 378
Número
Sección
Licencia
Todos los documentos incluidos en OJS son de acceso libre y propiedad de sus autores.
Los autores que publican en esta revista están de acuerdo con los siguientes términos:
- Los autores conservan los derechos de autor y garantizan a Metode Science Studies Journal el derecho a la primera publicación del trabajo, licenciado bajo una licencia de Creative Commons Reconocimiento-NoComercial-SinObraDerivada 4.0 Internacional, que permite a otros compartir el trabajo con un reconocimiento de la autoría del trabajo y citando la publicación inicial en esta revista.
- Se permite y se anima a los autores a difundir sus trabajos electrónicamente a través de páginas personales e institucionales (repositorios institucionales, páginas web personales o perfiles a redes profesionales o académicas) una vez publicado el trabajo.