Literature DB >> 17191459

Hydrogen cyanide polymers, comets and the origin of life.

Clifford N Matthews1, Robert D Minard.   

Abstract

Hydrogen cyanide polymers--heterogeneous solids ranging in colour from yellow to orange to brown to black--could be major components of the dark matter observed on many bodies of the outer solar system including asteroids, moons, planets and, especially, comets. The presence on cometary nuclei of frozen volatiles such as methane, ammonia and water subjected to high energy sources makes them attractive sites for the ready formation and condensed-phase polymerization of hydrogen cyanide. This could account for the dark crust observed on Comet Halley in 1986 by the Vega and Giotto missions. Dust emanating from its nucleus would arise partly from HCN polymers as suggested by the Giotto detection of free hydrogen cyanide, CN radicals, solid particles consisting only of H, C and N, or only of H, C, N, O, and nitrogen-containing organic compounds. Further evidence for cometary HCN polymers could be expected from in situ analysis of the ejected material from Comet Tempel 1 after collision with the impactor probe from the two-stage Deep Impact mission on July 4, 2005. Even more revealing will be actual samples of dust collected from the coma of Comet Wild 2 by the Stardust mission, due to return to Earth in January 2006 for analyses which we have predicted will detect these polymers and related compounds. In situ results have already shown that nitriles and polymers of hydrogen cyanide are probable components of the cometary dust that struck the Cometary and Interstellar Dust Analyzer of the Stardust spacecraft as it approached Comet Wild 2 on January 2, 2004. Preliminary evidence (January 2005) obtained by the Huygens probe of the ongoing Cassini-Huygens mission to Saturn and its satellites indicates the presence of nitrogen-containing organic compounds in the refractory organic cores of the aerosols that give rise to the orange haze high in the atmosphere of Titan, Saturn's largest moon. Our continuing investigations suggest that HCN polymers are basically of two types: ladder structures with conjugated -C=N- bonds and polyamidines readily converted by water to polypeptides. Thermochemolysis GC-MS studies show that cleavage products of the polymer include alpha-amino acids, nitrogen heterocycles such as purines and pyrimidines, and provide evidence for peptide linkages. Hydrogen cyanide polymers are a plausible link between cosmochemistry and the origin of informational macromolecules. Implications for prebiotic chemistry are profound. Following persistent bolide bombardment, primitive Earth may have been covered by water and carbonaceous compounds, particularly HCN polymers which would have supplied essential components for establishing protein/nucleic acid life.

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Year:  2006        PMID: 17191459     DOI: 10.1039/b516791d

Source DB:  PubMed          Journal:  Faraday Discuss        ISSN: 1359-6640            Impact factor:   4.008


  16 in total

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Authors:  Jan Spitzer; Bert Poolman
Journal:  Microbiol Mol Biol Rev       Date:  2009-06       Impact factor: 11.056

2.  Competition between π-hole interaction and hydrogen bond in the complexes of F2XO (X = C and Si) and HCN.

Authors:  Xin Guo; Lishui Cao; Qingzhong Li; Wenzuo Li; Jianbo Cheng
Journal:  J Mol Model       Date:  2014-10-23       Impact factor: 1.810

3.  Benchmark, DFT assessments, cooperativity, and energy decomposition analysis of the hydrogen bonds in HCN/HNC oligomeric complexes.

Authors:  Paulo McMiller C de Oliveira; Juliana A B Silva; Ricardo L Longo
Journal:  J Mol Model       Date:  2017-02-04       Impact factor: 1.810

Review 4.  Is boron a prebiotic element? A mini-review of the essentiality of boron for the appearance of life on earth.

Authors:  Romulus Scorei
Journal:  Orig Life Evol Biosph       Date:  2012-04-17       Impact factor: 1.950

Review 5.  Plausible Emergence and Self Assembly of a Primitive Phospholipid from Reduced Phosphorus on the Primordial Earth.

Authors:  Michael O Gaylor; Pere Miro; Bess Vlaisavljevich; Ashen Anuradha Suduweli Kondage; Laura M Barge; Arthur Omran; Patrick Videau; Vaille A Swenson; Lucas J Leinen; Nathaniel W Fitch; Krista L Cole; Chris Stone; Samuel M Drummond; Kayli Rageth; Lillian R Dewitt; Sarah González Henao; Vytis Karanauskus
Journal:  Orig Life Evol Biosph       Date:  2021-07-19       Impact factor: 1.950

6.  Chemical Analysis of a "Miller-Type" Complex Prebiotic Broth: Part I: Chemical Diversity, Oxygen and Nitrogen Based Polymers.

Authors:  Eva Wollrab; Sabrina Scherer; Frédéric Aubriet; Vincent Carré; Teresa Carlomagno; Luca Codutti; Albrecht Ott
Journal:  Orig Life Evol Biosph       Date:  2015-10-27       Impact factor: 1.950

7.  Academic aspects of lunar water resources and their relevance to lunar protolife.

Authors:  Jack Green
Journal:  Int J Mol Sci       Date:  2011-09-19       Impact factor: 5.923

Review 8.  Simple Organics and Biomonomers Identified in HCN Polymers: An Overview.

Authors:  Marta Ruiz-Bermejo; María-Paz Zorzano; Susana Osuna-Esteban
Journal:  Life (Basel)       Date:  2013-07-29

9.  Chemical Analysis of a "Miller-Type" Complex Prebiotic Broth : Part II: Gas, Oil, Water and the Oil/Water-Interface.

Authors:  Sabrina Scherer; Eva Wollrab; Luca Codutti; Teresa Carlomagno; Stefan Gomes da Costa; Andreas Volkmer; Amela Bronja; Oliver J Schmitz; Albrecht Ott
Journal:  Orig Life Evol Biosph       Date:  2016-11-28       Impact factor: 1.950

10.  The Grayness of the Origin of Life.

Authors:  Hillary H Smith; Andrew S Hyde; Danielle N Simkus; Eric Libby; Sarah E Maurer; Heather V Graham; Christopher P Kempes; Barbara Sherwood Lollar; Luoth Chou; Andrew D Ellington; G Matthew Fricke; Peter R Girguis; Natalie M Grefenstette; Chad I Pozarycki; Christopher H House; Sarah Stewart Johnson
Journal:  Life (Basel)       Date:  2021-05-29
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