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土卫六高层大气中噻啉的形成过程。

The process of tholin formation in Titan's upper atmosphere.

作者信息

Waite J H, Young D T, Cravens T E, Coates A J, Crary F J, Magee B, Westlake J

机构信息

Space Science and Engineering Division, Southwest Research Institute (SWRI), 6220 Culebra Road, San Antonio, TX 78238, USA.

出版信息

Science. 2007 May 11;316(5826):870-5. doi: 10.1126/science.1139727.

Abstract

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 N2). 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 (approximately 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 N2) to larger, more complex molecules (80 to 350 daltons) to negatively charged massive molecules (approximately 8000 daltons), which we identify as tholins. That the process involves massive negatively charged molecules and aerosols is completely unexpected.

摘要

长期以来,人们一直认为土卫六的低层大气中存在有机气溶胶(索林),据推测这些气溶胶是由甲烷和氮气等简单分子(CH₄和N₂)形成的。到目前为止,人们一直假定索林是在几百公里的高空通过尚未被观测到的过程形成的。利用卡西尼号航天器上的质量/电荷和能量/电荷光谱仪组合进行的测量,我们获得了土卫六大气在高海拔(约1000公里)处形成索林的证据。观测到的化学混合物强烈暗示了一系列化学反应和物理过程,这些过程从简单分子(CH₄和N₂)开始,生成更大、更复杂的分子(80至350道尔顿),进而形成带负电荷的大分子(约8000道尔顿),我们将其识别为索林。该过程涉及带大量负电荷的分子和气溶胶,这完全出乎意料。

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