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 AbstractTwo classes of homeodomain proteins specify the multiple a mating types of the mushroom Coprinus cinereus    Next AbstractValues for victims and vectors of disease »

Proc Natl Acad Sci U S A


Title:Synthesis of refractory organic matter in the ionized gas phase of the solar nebula
Author(s):Kuga M; Marty B; Marrocchi Y; Tissandier L;
Address:"Centre de Recherches Petrographiques et Geochimiques, UMR 7358, Universite de Lorraine, CNRS, 54500 Vandoeuvre les Nancy, France maia.kuga@erdw.ethz.ch. Centre de Recherches Petrographiques et Geochimiques, UMR 7358, Universite de Lorraine, CNRS, 54500 Vandoeuvre les Nancy, France"
Journal Title:Proc Natl Acad Sci U S A
Year:2015
Volume:20150526
Issue:23
Page Number:7129 - 7134
DOI: 10.1073/pnas.1502796112
ISSN/ISBN:1091-6490 (Electronic) 0027-8424 (Print) 0027-8424 (Linking)
Abstract:"In the nascent solar system, primitive organic matter was a major contributor of volatile elements to planetary bodies, and could have played a key role in the development of the biosphere. However, the origin of primitive organics is poorly understood. Most scenarios advocate cold synthesis in the interstellar medium or in the outer solar system. Here, we report the synthesis of solid organics under ionizing conditions in a plasma setup from gas mixtures (H2(O)-CO-N2-noble gases) reminiscent of the protosolar nebula composition. Ionization of the gas phase was achieved at temperatures up to 1,000 K. Synthesized solid compounds share chemical and structural features with chondritic organics, and noble gases trapped during the experiments reproduce the elemental and isotopic fractionations observed in primitive organics. These results strongly suggest that both the formation of chondritic refractory organics and the trapping of noble gases took place simultaneously in the ionized areas of the protoplanetary disk, via photon- and/or electron-driven reactions and processing. Thus, synthesis of primitive organics might not have required a cold environment and could have occurred anywhere the disk is ionized, including in its warm regions. This scenario also supports N2 photodissociation as the cause of the large nitrogen isotopic range in the solar system"
Keywords:accretion disk ionization meteorites noble gases organics;
Notes:"PubMed-not-MEDLINEKuga, Maia Marty, Bernard Marrocchi, Yves Tissandier, Laurent eng Research Support, Non-U.S. Gov't 2015/06/04 Proc Natl Acad Sci U S A. 2015 Jun 9; 112(23):7129-34. doi: 10.1073/pnas.1502796112. Epub 2015 May 26"

 
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 16-11-2024