Cargando…
High Energy Radical Chemistry Formation of HCN-rich Atmospheres on early Earth
Recent results in prebiotic chemistry implicate hydrogen cyanide (HCN) as the source of carbon and nitrogen for the synthesis of nucleotide, amino acid and lipid building blocks. HCN can be produced during impact events by reprocessing of carbonaceous and nitrogenous materials from both the impactor...
Autores principales: | Ferus, Martin, Kubelík, Petr, Knížek, Antonín, Pastorek, Adam, Sutherland, John, Civiš, Svatopluk |
---|---|
Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Nature Publishing Group UK
2017
|
Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5524942/ https://www.ncbi.nlm.nih.gov/pubmed/28740207 http://dx.doi.org/10.1038/s41598-017-06489-1 |
Ejemplares similares
-
Author Correction: High Energy Radical Chemistry Formation of HCN-rich Atmospheres on early Earth
por: Ferus, Martin, et al.
Publicado: (2018) -
TiO(2)-catalyzed synthesis of sugars from formaldehyde in extraterrestrial impacts on the early Earth
por: Civiš, Svatopluk, et al.
Publicado: (2016) -
Corrigendum: TiO(2)-catalyzed synthesis of sugars from formaldehyde in extraterrestrial impacts on the early Earth
por: Civiš, Svatopluk, et al.
Publicado: (2016) -
Atomic emission spectra of neutral noble gases in the infrared spectral range
por: Civiš, Svatopluk, et al.
Publicado: (2020) -
Infrared Spectra of Small Radicals for Exoplanetary Spectroscopy: OH, NH, CN and CH: The State of Current Knowledge
por: Civiš, Svatopluk, et al.
Publicado: (2023)