Structural basis for synthesis of inflammatory mediators by human leukotriene C4 synthase

Cysteinyl leukotrienes are key mediators in inflammation and have an important role in acute and chronic inflammatory diseases of the cardiovascular and respiratory systems, in particular bronchial asthma. In the biosynthesis of cysteinyl leukotrienes, conversion of arachidonic acid forms the unstable epoxide leukotriene A4 (LTA4). This intermediate is conjugated with glutathione (GSH) to produce leukotriene C4 (LTC4) in a reaction catalysed by LTC4 synthase: this reaction is the key step in cysteinyl leukotriene formation. Here we present the crystal structure of the human LTC4 synthase in its apo and GSH-complexed forms to 2.00 and 2.15 A resolution, respectively. The structure reveals a homotrimer, where each monomer is composed of four transmembrane segments. The structure of the enzyme in complex with substrate reveals that the active site enforces a horseshoe-shaped conformation on GSH, and effectively positions the thiol group for activation by a nearby arginine at the membrane-enzyme interface. In addition, the structure provides a model for how the omega-end of the lipophilic co-substrate is pinned at one end of a hydrophobic cleft, providing a molecular 'ruler' to align the reactive epoxide at the thiol of glutathione. This provides new structural insights into the mechanism of LTC4 formation, and also suggests that the observed binding and activation of GSH might be common for a family of homologous proteins important for inflammatory and detoxification responses.     

An unexpected cooling effect in Saturn's upper atmosphere

The upper atmospheres of the four Solar System giant planets exhibit high temperatures that cannot be explained by the absorption of sunlight. In the case of Saturn the temperatures predicted by models of solar heating are approximately 200 K, compared to temperatures of approximately 400 K observed independently in the polar regions and at 30 degrees latitude. This unexplained 'energy crisis' represents a major gap in our understanding of these planets' atmospheres. An important candidate for the source of the missing energy is the magnetosphere, which injects energy mostly in the polar regions of the planet. This polar energy input is believed to be sufficient to explain the observed temperatures, provided that it is efficiently redistributed globally by winds, a process that is not well understood. Here we show, using a numerical model, that the net effect of the winds driven by the polar energy inputs is not to heat but to cool the low-latitude thermosphere. This surprising result allows us to rule out known polar energy inputs as the solution to the energy crisis at Saturn. There is either an unknown--and large--source of polar energy, or, more probably, some other process heats low latitudes directly.     

The sources of sodium escaping from Io revealed by spectral high definition imaging

On Jupiter's moon Io, volcanic plumes and evaporating lava flows provide hot gases to form an atmosphere that is subsequently ionized. Some of Io's plasma is captured by the planet's strong magnetic field to form a co-rotating torus at Io's distance; the remaining ions and electrons form Io's ionosphere. The torus and ionosphere are also depleted by three time-variable processes that produce a banana-shaped cloud orbiting with Io, a giant nebula extending out to about 500 Jupiter radii, and a jet close to Io. No spatial constraints exist for the sources of the first two; they have been inferred only from modelling the patterns seen in the trace gas sodium observed far from Io. Here we report observations that reveal a spatially confined stream that ejects sodium only from the wake of the Io-torus interaction, together with a visually distinct, spherically symmetrical outflow region arising from atmospheric sputtering. The spatial extent of the ionospheric wake that feeds the stream is more than twice that observed by the Galileo spacecraft and modelled successfully. This implies considerable variability, and therefore the need for additional modelling of volcanically-driven, episodic states of the great jovian nebula.     

Catastrophic flooding origin of shelf valley systems in the English Channel

Megaflood events involving sudden discharges of exceptionally large volumes of water are rare, but can significantly affect landscape evolution, continental-scale drainage patterns and climate change. It has been proposed that a significant flood event eroded a network of large ancient valleys on the floor of the English Channel-the narrow seaway between England and France. This hypothesis has remained untested through lack of direct evidence, and alternative non-catastrophist ideas have been entertained for valley formation. Here we analyse a new regional bathymetric map of part of the English Channel derived from high-resolution sonar data, which shows the morphology of the valley in unprecedented detail. We observe a large bedrock-floored valley that contains a distinct assemblage of landforms, including streamlined islands and longitudinal erosional grooves, which are indicative of large-scale subaerial erosion by high-magnitude water discharges. Our observations support the megaflood model, in which breaching of a rock dam at the Dover Strait instigated catastrophic drainage of a large pro-glacial lake in the southern North Sea basin. We suggest that megaflooding provides an explanation for the permanent isolation of Britain from mainland Europe during interglacial high-sea-level stands, and consequently for patterns of early human colonisation of Britain together with the large-scale reorganization of palaeodrainage in northwest Europe.     

Detector challenges at the LHC

The best way to study the existence of the Higgs boson, supersymmetry and grand unified theories, and perhaps the physics of dark matter and dark energy, is at the TeV scale. This is the energy scale that will be explored at the Large Hadron Collider. This machine will generate the energy and rate of collisions that might provide evidence of new fundamental physics. It also brings with it the formidable challenge of building detectors that can record a large variety of detailed measurements in the inhospitable environment close to the collisions points of the machine.     

全球性挑战:可持续发展如何实现?

<正>气候变化问题政府间专门小组(IPCC)报告称,过去一年二氧化碳排放量的增速比2000～2004年间最糟糕的年份还要快。政府如不采取新的行动,那么到2030年,温室气体排放量将比2000年增加25%～90%。目前,海洋和森林对碳的吸收能量为每年大约30～35亿吨,人类活动每年增加碳量70亿吨。人类的消费大于自然界再生或吸收"生态脚印"能力的25%。     

喀什市城市生态环境质量评价研究

 以1997~2008期间12a的生态环境时间序列数据为数据源,建立了喀什市生态环境质量综合评价指标体系,运用层次分析法确定了各生态因子的权重,得出了影响因子的重要性排序并计算出了生态环境质量综合指数,最终对喀什市生态环境质量进行了评价.研究表明:喀什市生态环境质量综合指数呈现波动性的变化特征,2002年前后的变化状况有区别,2002年以前生态环境综合指数比较低,而且总体上呈现下降趋势,表明生态环境综合质量以下降趋势为主;2002年以后指数既有上升也有下降趋势,但指数比2002年以前的高,表明生态环境质量有所好转,但总的趋势并不理想.生态环境质量评价结果显示,喀什市生态环境综合质量整体上比较差,生态环境形势不乐观,因此喀什市必须要采取措施,加强生态环境建设方面的工作力度.     

和田茴香籽中黄酮类化合物提取工艺研究

采用正交设计法对新疆和田茴香籽中的黄酮类化合物提取工艺参数进行优化.结果表明:最佳提取工艺为70 ml 60％乙醇在70℃下提取2.5h.本实验采用分光光度法,以芦丁标准品测定新疆和田茴香籽提取物中总黄酮的含量,总黄酮含量为1.58％.该工艺稳定、简便、快速,可作为检测茴香籽提取物中黄酮含量的一种手段.