Rapid regulation of steroidogenesis by mitochondrial protein import

Most mitochondrial proteins are synthesized on cytoplasmic ribosomes and imported into mitochondria. The imported proteins are directed to one of four submitochondrial compartments--the outer mitochondrial membrane, the inner mitochondrial membrane, the intramembraneous space, or the matrix--where the protein then functions. Here we show that the steroidogenic acute regulatory protein (StAR), a mitochondrial protein required for stress responses, reproduction, and sexual differentiation of male fetuses, exerts its activity transiently at the outer mitochondrial membrane rather than at its final resting place in the matrix. We also show that its residence time at this outer membrane and its activity are regulated by its speed of mitochondrial import. This may be the first example of a mitochondrial protein exerting its biological activity in a compartment other than that to which it is finally targeted. This system enables steroidogenic cells to initiate and terminate massive levels of steroidogenesis within a few minutes, permitting the rapid regulation of serum steroid hormone concentrations.     

Molecular gas in the host galaxy of a quasar at redshift z = 6.42

Observations of molecular hydrogen in quasar host galaxies at high redshifts provide fundamental constraints on galaxy evolution, because it is out of this molecular gas that stars form. Molecular hydrogen is traced by emission from the carbon monoxide molecule, CO; cold H2 itself is generally not observable. Carbon monoxide has been detected in about ten quasar host galaxies with redshifts z > 2; the record-holder is at z = 4.69 (refs 1-3). Here we report CO emission from the quasar SDSS J114816.64 + 525150.3 (refs 5, 6) at z = 6.42. At that redshift, the Universe was only 1/16 of its present age, and the era of cosmic reionization was just ending. The presence of about 2 x 1010 M\circ of H2 in an object at this time demonstrates that molecular gas enriched with heavy elements can be generated rapidly in the youngest galaxies.     

Primary carbonatite melt from deeply subducted oceanic crust

Partial melting in the Earth's mantle plays an important part in generating the geochemical and isotopic diversity observed in volcanic rocks at the surface. Identifying the composition of these primary melts in the mantle is crucial for establishing links between mantle geochemical 'reservoirs' and fundamental geodynamic processes. Mineral inclusions in natural diamonds have provided a unique window into such deep mantle processes. Here we provide experimental and geochemical evidence that silicate mineral inclusions in diamonds from Juina, Brazil, crystallized from primary and evolved carbonatite melts in the mantle transition zone and deep upper mantle. The incompatible trace element abundances calculated for a melt coexisting with a calcium-titanium-silicate perovskite inclusion indicate deep melting of carbonated oceanic crust, probably at transition-zone depths. Further to perovskite, calcic-majorite garnet inclusions record crystallization in the deep upper mantle from an evolved melt that closely resembles estimates of primitive carbonatite on the basis of volcanic rocks. Small-degree melts of subducted crust can be viewed as agents of chemical mass-transfer in the upper mantle and transition zone, leaving a chemical imprint of ocean crust that can possibly endure for billions of years.     

短花针茅荒漠草原土壤呼吸对载畜率的响应(英文)

土壤碳通量是陆地生态系统中碳循环的重要组成部分.为了揭示放牧对荒漠草原土壤呼吸速率的影响,我们采取完全随机区组设计比较研究了不同载畜率下草地土壤的呼吸速率.试验包括4个处理,3次重复.4个处理分别是对照(CK)、轻度放牧(LG)、中度放牧(MG)和重度放牧(HG),相应的载畜率分别为0,0.91,1.82 和2.71只羊*hm-2*半年-1.在2004年和2006年8月,采用LI-6400-09土壤呼吸室与LI-6400连接对每个样地的土壤呼吸速率进行了测定,在测定过程中,同时获取了土壤温度及土壤呼吸室中的相对湿度等相关指标.通过对测定数据的分析表明,内蒙古荒漠草原土壤呼吸速率介于0.80 μmol·m-2·s-1与5.00 μmol·m-2·s-1之间.随着载畜率的增加,土壤呼吸速率明显增加(P<0.05).另外,土壤呼吸速率也随着土壤呼吸室中相对湿度的增加而增大,但是二者的相关关系不太明显(P>0.05).经过2年放牧后,重度放牧条件下的土壤呼吸速率明显低于对照区和轻度放牧区,不同载畜率下土壤呼吸速率随时间的变化并没有明显的差异.高载畜率下土壤呼吸速率明显降低可能与该条件下土壤水分和草地生物量的明显降低有关,土壤水分对土壤和大气之间CO2的交换起着非常重要的作用.     

Compact sources as the origin of the soft gamma-ray emission of the Milky Way

The Milky Way is known to be an abundant source of gamma-ray photons, now determined to be mainly diffuse in nature and resulting from interstellar processes. In the soft gamma-ray domain, point sources are expected to dominate, but the lack of sensitive high-resolution observations did not allow for a clear estimate of the contribution from such sources. Even the best imaging experiment revealed only a few point sources, accounting for about 50% of the total Galactic flux. Theoretical studies were unable to explain the remaining intense diffuse emission. Investigating the origin of the soft gamma-rays is therefore necessary to determine the dominant particle acceleration processes and to gain insights into the physical and chemical equilibrium of the interstellar medium. Here we report observations in the soft gamma-ray domain that reveal numerous compact sources. We show that these sources account for the entirety of the Milky Way's emission in soft gamma-rays, leaving at most a minor role for diffuse processes.     

重组PAI—2基因在NIH3T3细胞中的活性表达

构建了人ＰＡＩ—２ｃＤＮＡ睥达质粒，以ＮＩＨ３Ｔ３为转染宿主细胞，ＮｏｒｔｈｅｒｎＢｌｏｔ，ＷｅｓｔｅｒｎＢｌｏｔ和ＰＡＩ活性扩散试验结果表明人ＰＡＩ—２ｃＤＮＡ可以在ＮＩＨ３Ｔ３细胞中正确表达出ＰＡＩ—２蛋白，且具有抑制ＰＡ的活性，同时未能检测到ＮＩＨ３Ｔ３细胞表达ＰＡＩ—２蛋白质．为探讨ＰＡ—ＰＡＩ—２系统的调控机制打下基础．