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Forming complex organic molecules on Titan

机译:在土卫六上形成复杂的有机分子

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Researchers have found a series of chemical reactions that likely formed the large, organic molecules that compose the thick, hazy, orange atmosphere of Saturn's moon Titan. The research demonstrates a mechanism to describe how Titan's atmosphere creates complex molecules. Xibin Gu et al. studied the formation of triacetylene and larger organic molecules in the lab and in simulations. The authors found that triacetylene can be formed by collisions between ethynyl radicals and di-acetylene. The reaction was easy to initiate and energetically favorable under the conditions found in Titan's atmosphere. The authors suggest that triacetylene may serve as the primary building block for creating more complex polyynes. These organic molecules may act as a shield to ultraviolet radiation, much like Earth's ozone layer. An improved understanding of the chemical elements and dynamics of Titan's atmosphere could provide clues to the origins and chemical dynamics of Earth's early atmospheres and how their evolution affected the development of life, according to the authors.
机译:研究人员发现了一系列化学反应,这些化学反应很可能形成了大型有机分子,这些有机分子构成了土星卫星土卫六的浓稠,朦胧的橙色气氛。这项研究表明了一种机制,可以描述泰坦的大气层如何产生复杂的分子。顾锡斌等。在实验室和模拟中研究了三乙炔和较大有机分子的形成。作者发现三乙炔可以通过乙炔基和二乙炔之间的碰撞形成。在泰坦大气中发现的条件下,该反应易于引发并且在能量上有利。作者认为,三乙炔可能是产生更复杂的聚炔的主要组成部分。这些有机分子可能像地球的臭氧层一样,充当紫外线辐射的屏蔽层。这组作者说,对泰坦大气化学元素和动力学的进一步了解可以为地球早期大气的起源和化学动力学以及它们的演化如何影响生命发展提供线索。

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