Title of article
Detection of martian amino acids by chemical derivatization coupled to gas chromatography: In situ and laboratory analysis Original Research Article
Author/Authors
C. Rodier، نويسنده , , O. Vandenabeele-Trambouze، نويسنده , , R. Sternberg، نويسنده , , D. Coscia، نويسنده , , P. Coll، نويسنده , , C. Szopa، نويسنده , , F. Raulin، نويسنده , , C. Vidal-Madjar، نويسنده , , M. Cabane، نويسنده , , Elizabeth G. Israel، نويسنده , , M.F. Grenier-Loustalot، نويسنده , , Dorde M. Dobrijevic and Dragan P. Popovic، نويسنده , , D. Despois، نويسنده ,
Issue Information
دوهفته نامه با شماره پیاپی سال 2001
Pages
5
From page
195
To page
199
Abstract
If there is, or ever was, life in our solar system beyond the Earth, Mars is the most likely place to search for. Future space missions will have then to take into account the detection of prebiotic molecules or molecules of biological significance such as amino acids. Techniques of analysis used for returned samples have to be very sensitive and avoid any chemical or biological contamination whereas in situ techniques have to be automated, fast and low energy consuming. Several possible methods could be used for in situ amino acid analyses on Mars, but gas chromatography would likely be the most suitable. Returned samples could be analyzed by any method in routine laboratory use such as gas chromatography, already successfully performed for analyses of organic matter including amino acids from martian meteorites. The derivatization step, which volatilizes amino acids to perform both in situ and laboratory analysis by gas chromatography, is discussed here.
Journal title
Advances in Space Research
Serial Year
2001
Journal title
Advances in Space Research
Record number
1127294
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