Bedoukian   RussellIPM   RussellIPM   Piezoelectric Micro-Sprayer


Home
Animal Taxa
Plant Taxa
Semiochemicals
Floral Compounds
Semiochemical Detail
Semiochemicals & Taxa
Synthesis
Control
Invasive spp.
References

Abstract

Guide

Alphascents
Pherobio
InsectScience
E-Econex
Counterpart-Semiochemicals
Print
Email to a Friend
Kindly Donate for The Pherobase

« Previous AbstractGenetic analysis of SecA-SecY interaction required for spore development in Bacillus subtilis    Next AbstractCharacterization of complex organic compounds formed in simulated planetary atmospheres by the action of high energy particles »

Adv Space Res


Title:Formation of amino acid precursors in cometary ice environments by cosmic radiation
Author(s):Kobayashi K; Kasamatsu T; Kaneko T; Koike J; Oshima T; Saito T; Yamamoto T; Yanagawa H;
Address:"Yokohama National University, Hodogaya-ku, Japan"
Journal Title:Adv Space Res
Year:1995
Volume:16
Issue:2
Page Number:21 - 26
DOI: 10.1016/0273-1177(95)00188-k
ISSN/ISBN:0273-1177 (Print) 0273-1177 (Linking)
Abstract:"Cometary ices are believed to contain water, carbon monoxide, methane and ammonia, and are possible sites for the formation and preservation of organic compounds relating to the origin of life. Cosmic rays, together with ultraviolet light, are among the most effective energy sources for the formation of organic compounds in space. In order to study the possibility of the formation of amino acids in comets or their precursory bodies (interstellar dust grains), several types of ice mixtures made in a cryostat at 10 K ('simulated cometary ices') were irradiated with high energy protons. After irradiation, the volatile products were analyzed with a quadrupole mass spectrometer, while temperature of the cryostat was raised to room temperature. The non-volatile products remaining in the cryostat at room temperature were collected with water. They were acid-hydrolyzed, and analyzed by ion-exchange chromatography. When an ice mixture of carbon monoxide (or methane), ammonia and water was irradiated, some hydrocarbons were formed, and amino acids such as glycine and alanine were detected in the hydrolyzate. These results suggest the possible formation of 'amino acid precursors' (compounds yielding amino acids after hydrolysis) in interstellar dust grains by cosmic radiation. We previously reported that amino acid precursors were formed when simulated primitive planetary atmospheres were irradiated with cosmic ray particles. It will be of great interest to compare the amount of bioorganic compounds that were formed in the primitive earth and that brought by comets to the earth"
Keywords:Amino Acids/*chemical synthesis Ammonia/chemistry Carbon Monoxide/chemistry *Cosmic Radiation Exobiology Extraterrestrial Environment Hydrolysis Ice/*analysis *Meteoroids Methane/chemistry Propane/chemistry *Protons Water/chemistry;
Notes:"MedlineKobayashi, K Kasamatsu, T Kaneko, T Koike, J Oshima, T Saito, T Yamamoto, T Yanagawa, H eng Research Support, Non-U.S. Gov't England 1995/01/01 Adv Space Res. 1995; 16(2):21-6. doi: 10.1016/0273-1177(95)00188-k"

 
Back to top
 
Citation: El-Sayed AM 2024. The Pherobase: Database of Pheromones and Semiochemicals. <http://www.pherobase.com>.
© 2003-2024 The Pherobase - Extensive Database of Pheromones and Semiochemicals. Ashraf M. El-Sayed.
Page created on 27-12-2024