Organic material in meteorites and the link to the origin of life

Life requires specific conditions that have been, so far, only proven to meet on Earth. Though the chemical elements required to form living organism (C, H, N, O, S, etc) are widespread in the universe, the molecules that are crucial for Life, like nucleobases or amino acids, may not be so ubiquitou...

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Main Author: Remusat L.
Format: Article
Language:English
Published: EDP Sciences 2014-02-01
Series:BIO Web of Conferences
Online Access:http://dx.doi.org/10.1051/bioconf/20140203001
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author Remusat L.
author_facet Remusat L.
author_sort Remusat L.
collection DOAJ
description Life requires specific conditions that have been, so far, only proven to meet on Earth. Though the chemical elements required to form living organism (C, H, N, O, S, etc) are widespread in the universe, the molecules that are crucial for Life, like nucleobases or amino acids, may not be so ubiquitous. The question of the formation of small and complex molecules is highly relevant to understand the process of Life origin. Carbonaceous chondrites are a class of meteorites rich in organic compounds and host potential precursors for the emergence of Life (organic matter and water). They could have been the source of complex molecules on the early Earth. This contribution will describe the main properties of the organic matter recovered from carbonaceous chondrites. However, the isotopic and molecular record of organic compounds is faded by secondary processes that occurred on the parent body of these meteorites. This results in complex signatures that raise multiple questions about the origin of organic compounds in the Solar System.
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spelling doaj.art-2417f55043c64aed8e3e05811d98b3ce2022-12-21T21:10:45ZengEDP SciencesBIO Web of Conferences2117-44582014-02-0120300110.1051/bioconf/20140203001bioconf_epov2012_03001Organic material in meteorites and the link to the origin of lifeRemusat L.0Laboratoire de Minéralogie et Cosmochimie du Museum, UMR CNRS 7202Life requires specific conditions that have been, so far, only proven to meet on Earth. Though the chemical elements required to form living organism (C, H, N, O, S, etc) are widespread in the universe, the molecules that are crucial for Life, like nucleobases or amino acids, may not be so ubiquitous. The question of the formation of small and complex molecules is highly relevant to understand the process of Life origin. Carbonaceous chondrites are a class of meteorites rich in organic compounds and host potential precursors for the emergence of Life (organic matter and water). They could have been the source of complex molecules on the early Earth. This contribution will describe the main properties of the organic matter recovered from carbonaceous chondrites. However, the isotopic and molecular record of organic compounds is faded by secondary processes that occurred on the parent body of these meteorites. This results in complex signatures that raise multiple questions about the origin of organic compounds in the Solar System.http://dx.doi.org/10.1051/bioconf/20140203001
spellingShingle Remusat L.
Organic material in meteorites and the link to the origin of life
BIO Web of Conferences
title Organic material in meteorites and the link to the origin of life
title_full Organic material in meteorites and the link to the origin of life
title_fullStr Organic material in meteorites and the link to the origin of life
title_full_unstemmed Organic material in meteorites and the link to the origin of life
title_short Organic material in meteorites and the link to the origin of life
title_sort organic material in meteorites and the link to the origin of life
url http://dx.doi.org/10.1051/bioconf/20140203001
work_keys_str_mv AT remusatl organicmaterialinmeteoritesandthelinktotheoriginoflife