Adenine synthesis at Titan atmosphere analog by soft X-rays

被引:0
|
作者
Pilling, Sergio [1 ]
Andrade, Diana P. P. [1 ]
Neto, Alvaro C.
Rittner, Roberto
de Brito, Arnaldo N.
机构
[1] Pontificia Univ Catolica Rio de Janeiro, BR-22453900 Rio De Janeiro, Brazil
来源
关键词
astrochemistry; astrobiology; molecular processes; methods: laboratory; planets and satellites: Titan; Sun: X-rays;
D O I
10.1017/S1743921310001651
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this work, we investigate the possible effects produced by soft X-rays (and secondary electrons) on Titan aerosol analogs in an attempt to simulate some prebiotic photochemistry. The experiments have been performed inside a high vacuum chamber coupled to the soft X-ray spectroscopy beamline at the Brazilian Synchrotron Light Source (LNLS). In-situ sample analysis were performed by a Fourier transform infrared spectrometer. The infrared spectra have presented several organic molecules, including nitriles and aromatic CN compounds. After the irradiation, the brownish-orange organic residue was analyzed ex-situ by gas chromatographic technique revealing the presence of adenine (C5H5N5), one of the constituents of the DNA molecule.
引用
收藏
页码:145 / 146
页数:2
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