Two surface samples collected from the Chryse Planitia region of Mars were heated to temperatures up to 500 degrees C, and the volatiles that they evolved were analyzed with a gas chromatograph-mass spectrometer. Only water and carbon dioxide were detected. This implies that organic compounds have not accumulated to the extent that individual components could be detected at levels of a few parts in 10(9) by weight in our samples. Proposed mechanisms for the accumulation and destruction of organic compounds are discussed in the light of this limit.
One- and two-dimensional HPTLC supported by mass spectrometric detection represents an innovative, alternative tool for investigating and understanding polyphenol-protein interactions. This approach enables the identification of binding sites inside the protein chain and contributes to understanding the mechanism of polyphenol-protein interactions in vitro and in vivo.
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