The process of tholin formation in Titan's upper atmosphere

被引:519
作者
Waite, J. H., Jr.
Young, D. T.
Cravens, T. E.
Coates, A. J.
Crary, F. J.
Magee, B.
Westlake, J.
机构
[1] SW Res Inst, Space Sci & Engn Div, San Antonio, TX 78238 USA
[2] Univ Kansas, Dept Phys & Astron, Lawrence, KS 66045 USA
[3] UCL, Mullard Space Sci Lab, Dept Space & Climate Phys, Dorking RH5 6NT, Surrey, England
[4] Univ Texas, Dept Phys & Astron, San Antonio, TX 78249 USA
基金
英国科学技术设施理事会;
关键词
D O I
10.1126/science.1139727
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Titan's lower atmosphere has long been known to harbor organic aerosols (tholins) presumed to have been formed from simple molecules, such as methane and nitrogen (CH4 and N-2). Up to now, it has been assumed that tholins were formed at altitudes of several hundred kilometers by processes as yet unobserved. Using measurements from a combination of mass/charge and energy/ charge spectrometers on the Cassini spacecraft, we have obtained evidence for tholin formation at high altitudes (similar to 1000 kilometers) in Titan's atmosphere. The observed chemical mix strongly implies a series of chemical reactions and physical processes that lead from simple molecules (CH4 and N-2) to larger, more complex molecules ( 80 to 350 daltons) to negatively charged massive molecules (similar to 8000 daltons), which we identify as tholins. That the process involves massive negatively charged molecules and aerosols is completely unexpected.
引用
收藏
页码:870 / 875
页数:6
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