Literature DB >> 17770442

Long-wavelength ultraviolet photoproduction of amino acids on the primitive Earth.

C Sagan, B N Khare.   

Abstract

Amino acids are produced under possible primitive Earth conditions by irradiation of gas mixtures with long-wavelength ultraviolet light, representing the most abundant useful energy source for prebiological organic synthesis. Hydrogen sulfide is the initial photon acceptor in this work; superthermal atomic hydrogen photodissociation products appear to initiate reactions leading to amino acid synthesis with an overall quantum yield on the order of 5X10(-5).

Entities:  

Year:  1971        PMID: 17770442     DOI: 10.1126/science.173.3995.417

Source DB:  PubMed          Journal:  Science        ISSN: 0036-8075            Impact factor:   47.728


  50 in total

1.  Radioactivity as a significant energy source in prebiotic synthesis.

Authors:  L Garzón; M L Garzón
Journal:  Orig Life Evol Biosph       Date:  2001 Feb-Apr       Impact factor: 1.950

2.  Amino acid formation in gas mixtures by high energy particle irradiation.

Authors:  K Kobayashi; T Kaneko; T Saito; T Oshima
Journal:  Orig Life Evol Biosph       Date:  1998-04       Impact factor: 1.950

3.  The spark discharge synthesis of amino acids from various hydrocarbons.

Authors:  D Ring; S L Miller
Journal:  Orig Life Evol Biosph       Date:  1984       Impact factor: 1.950

4.  Prebiotic formation of 'energy-rich' thioesters from glyceraldehyde and N-acetylcysteine.

Authors:  A L Weber
Journal:  Orig Life Evol Biosph       Date:  1984       Impact factor: 1.950

5.  Alanine synthesis from glyceraldehyde and ammonium ion in aqueous solution.

Authors:  A L Weber
Journal:  J Mol Evol       Date:  1985       Impact factor: 2.395

6.  The possible role of solid surface area in condensation reactions during chemical evolution: reevaluation.

Authors:  N Lahav; S Chang
Journal:  J Mol Evol       Date:  1976-12-30       Impact factor: 2.395

7.  The role of sulphur in chemical evolution.

Authors:  F Raulin; G Toupance
Journal:  J Mol Evol       Date:  1977-08-05       Impact factor: 2.395

8.  Origin of organic compounds on the primitive earth and in meteorites.

Authors:  S L Miller; H C Urey; J Oró
Journal:  J Mol Evol       Date:  1976-12-31       Impact factor: 2.395

9.  Chemical evolution: effect of high energy radiation.

Authors:  L Keszthelyi
Journal:  Orig Life       Date:  1976-12

10.  Hydrogen atom initiated chemistry.

Authors:  J H Hong; R S Becker
Journal:  J Mol Evol       Date:  1979-06-08       Impact factor: 2.395

View more

北京卡尤迪生物科技股份有限公司 © 2022-2023.