Fluorescence spectra of Titan tholins: in-situ detection of astrobiologically interesting areas on Titan's surface

Details Fluorescence spectra of Titan tholins: in-situ detection of astrobiologically interesting areas on Titan's surface Fluorescence spectra of Titan tholins: in-situ detection of astrobiologically interesting areas on Titan's surface

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004icar..171..525h&link_type=abstract

Icarus, Volume 171, Issue 2, p. 525-530.

Computer Science

1

Titan, Organic Chemistry, Prebiotic Chemistry, Prebiotic Environments

Scientific paper

We report the three-dimensional fluorescence spectra of Titan tholins in water and acetonitrile, and separate some of the fluorescent components of tholins using two-dimensional thin layer chromatography. In acetonitrile, tholins exhibit a broad fluorescence with a maximum at 471 nm, and an excitation maximum at 410 nm. The fluorescence spectrum of a water extraction displays a more complicated spectrum with multiple peaks. TLC results indicate the presence of at least three distinct fluorescent species. In addition, we obtained the two-dimensional fluorescence spectrum of tholins in water ice at 77 K, close to the surface temperature of Titan. The fluorescence of tholins in a 77 K ice matrix is red-shifted in comparison to a water solution, and undergoes a further red-shift when the water solution is heated prior to freezing. These results suggest that a simple fluorescence probe could be used on the surface of Titan to identify sites where tholins have been mixed with water, and possibly reveal information about the extent of heating the tholin-water mixture has undergone. This would be useful for a future mission with the goal of examining the organic chemistry of Titan.

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