Zobrazeno 1 - 10
of 22
pro vyhledávání: '"E, De Vanssay"'
Autor:
Patrice Coll, L. Guez, P. Bruston, E. de Vanssay, David Coscia, Marie-Claire Gazeau, François Raulin
Publikováno v:
Journal of Biological Physics. 20:39-53
With a dense N2-CH4 atmosphere rich in organics, both in gas and aerosol phases, and with the possible presence of hydrocarbons oceans on its surface, Titan, the largest satellite of Saturn, appears as a natural laboratory to study chemical evolution
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0410e3c43ee2df79266e3795367924ba
https://doi.org/10.1007/bf00700419
https://doi.org/10.1007/bf00700419
Autor:
Yves Bénilan, Patrice Coll, D. Andrieux, E. de Vanssay, François Raulin, P. Bruston, D. Coscia, P. Paillous, Jean-Claude Guillemin, M. Khlifi, Robert Sternberg, Marie-Claire Gazeau, A. Aflalaye
Publikováno v:
Advances in Space Research. 15:5-11
In the frame of a laboratory program on organic compounds of planetological interest only stable at low temperatures, we are currently studying the gas chromatographic (GC) and mass spectrometric (MS) behaviour of gaseous polyynes and N-organics, tog
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3d509b61adcb436f587a6e41d2f05011
https://doi.org/10.1016/0273-1177(94)00144-p
https://doi.org/10.1016/0273-1177(94)00144-p
Publikováno v:
Journal of Chromatography A. 688:161-170
An alternative for the GC determination of permanent gases in Titan's atmosphere, given the severe constraints of space instrumentation, is the use of a 100–120-mesh molecular sieve 5A micropacked column. Because of its high efficiency, small press
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::664807b6b8894e822a77d3d2081c47fd
https://doi.org/10.1016/0021-9673(94)00796-9
https://doi.org/10.1016/0021-9673(94)00796-9
Publikováno v:
Journal of Chromatography A. 639:255-259
A Molsieve 5A wide-bore capillary column was systematically studied for the separation of CO and N2 in the presence of other permanent gases, including noble gases, light hydrocarbons and nitriles, which are all plausible constituents of Titan's atmo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7e69040f19ee9904a2bd2c3b49b82c71
https://doi.org/10.1016/0021-9673(93)80261-6
https://doi.org/10.1016/0021-9673(93)80261-6
Autor:
François Raulin, E. de Vanssay, A. Aflalaye, G. Israel, Marie-Claire Gazeau, Robert Sternberg, Patrice Coll, David Coscia, P. Bruston
Publikováno v:
Chemical Evolution: Physics of the Origin and Evolution of Life ISBN: 9789401072663
Titan, the largest satellite of Saturn, is in many aspects similar to the Earth. In spite of much lower temperatures and the absence of liquid water, because its environment is very rich in organics, and many couplings are involved in the various par
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1702b5bf4344ca4268c3b923a3d191c4
https://doi.org/10.1007/978-94-009-1712-5_32
https://doi.org/10.1007/978-94-009-1712-5_32
Publikováno v:
Planetary and space science. 43(1-2)
A wide range of experiments has already been carried out to simulate the chemical evolution of Titan. Such experiments can provide useful information on the possible nature of minor constituents, mostly organic, likely to be present in Titan's atmosp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ef9aebce3da2f9862cc982c2a89b8af8
https://pubmed.ncbi.nlm.nih.gov/11538434
https://pubmed.ncbi.nlm.nih.gov/11538434
Publikováno v:
Chemical Evolution: Structure and Model of the First Cell ISBN: 9789401040501
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::21f092e7fee1e4243bcea090df0266cd
https://doi.org/10.1007/978-94-011-0105-9_4
https://doi.org/10.1007/978-94-011-0105-9_4
Autor:
Patrice Coll, David Coscia, François Raulin, Marie-Claire Gazeau, E. de Vanssay, Jean-Claude Guillemin
Publikováno v:
Advances in space research : the official journal of the Committee on Space Research (COSPAR). 16(2)
Many experiments have already been carried out to simulate organic chemistry on Titan, the largest satellite of Saturn. They can provide fruitful information on the nature of minor organic constituents likely to be present in Titan's atmosphere, both
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::22a644399acddcf28472a067083d04ce
https://pubmed.ncbi.nlm.nih.gov/11543541
https://pubmed.ncbi.nlm.nih.gov/11543541
Publikováno v:
Journal of the British Interplanetary Society. 45(6)
Titan, the largest satellite of Saturn, has a dense N2-CH4 atmosphere rich in organic compounds, both in gas and in aerosol phases. Its surface is probably covered by oceans of liquid methane-ethane mixtures, with many dissolved organics. This quasi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid________::2b4e366315ea09ad56b7c660849846ff
https://pubmed.ncbi.nlm.nih.gov/11539470
https://pubmed.ncbi.nlm.nih.gov/11539470
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