The virophage as a unique parasite of the giant mimivirus

Viruses are obligate parasites of Eukarya, Archaea and Bacteria. Acanthamoeba polyphaga mimivirus (APMV) is the largest known virus; it grows only in amoeba and is visible under the optical microscope. Mimivirus possesses a 1,185-kilobase double-stranded linear chromosome whose coding capacity is greater than that of numerous bacteria and archaea1, 2, 3. Here we describe an icosahedral small virus, Sputnik, 50 nm in size, found associated with a new strain of APMV. Sputnik cannot multiply in Acanthamoeba castellanii but grows rapidly, after an eclipse phase, in the giant virus factory found in amoebae co-infected with APMV4. Sputnik growth is deleterious to APMV and results in the production of abortive forms and abnormal capsid assembly of the host virus. The Sputnik genome is an 18.343-kilobase circular double-stranded DNA and contains genes that are linked to viruses infecting each of the three domains of life Eukarya, Archaea and Bacteria. Of the 21 predicted protein-coding genes, eight encode proteins with detectable homologues, including three proteins apparently derived from APMV, a homologue of an archaeal virus integrase, a predicted primase-helicase, a packaging ATPase with homologues in bacteriophages and eukaryotic viruses, a distant homologue of bacterial insertion sequence transposase DNA-binding subunit, and a Zn-ribbon protein. The closest homologues of the last four of these proteins were detected in the Global Ocean Survey environmental data set5, suggesting that Sputnik represents a currently unknown family of viruses. Considering its functional analogy with bacteriophages, we classify this virus as a virophage. The virophage could be a vehicle mediating lateral gene transfer between giant viruses.     

Cell penetrating peptides: overview and applications to the delivery of oligonucleotides

Crossing biological barriers represents a major limitation for clinical applications of biomolecules such as nucleic acids, peptides or proteins. Cell penetrating peptides (CPP), also named protein transduction domains, comprise short and usually basic amino acids-rich peptides originating from proteins able to cross biological barriers, such as the viral Tat protein, or are rationally designed. They have emerged as a new class of non-viral vectors allowing the delivery of various biomolecules across biological barriers from low molecular weight drugs to nanosized particles. Encouraging data with CPP-conjugated oligonucleotides have been obtained both in vitro and in vivo in animal models of diseases such as Duchenne muscular dystrophy. Whether CPP-cargo conjugates enter cells by direct translocation across the plasma membrane or by endocytosis remains controversial. In many instances, however, endosomal escape appears as a major limitation of this new delivery strategy.     

罗伯特 H·布朗的一生(1916～2002)

罗伯特Ｈ·布朗 (ＲｏｂｅｒｔＨａｎｂｕｒｙＢｒｏｗｎ ,见图 ) ,一位天文学变革时期的伟人 ,于今年 1月 1 6日辞世 ,享年 85岁。布朗于 1 91 6年生于印度 ,孩提时立志长大后要成为一名一流的学者 ,1 93 5年以工科身份毕业于伦敦大学。接着他致力于发展海岸雷达———链导航———后于 1 940年在不列颠之战中被证明是非常重要的。其后 ,与其同事一起研究可安装于飞行器上的短波雷达。他的精彩自传《科研人员》对这一工作的尝试与成功进行了生动的总结。布朗的贡献还包括在无线电偏振特性方面的研究 ,这一研究对于天线在空对地监督及探测船…     

Towards robust regional estimates of CO2 sources and sinks using atmospheric transport models

Information about regional carbon sources and sinks can be derived from variations in observed atmospheric CO2 concentrations via inverse modelling with atmospheric tracer transport models. A consensus has not yet been reached regarding the size and distribution of regional carbon fluxes obtained using this approach, partly owing to the use of several different atmospheric transport models. Here we report estimates of surface-atmosphere CO2 fluxes from an intercomparison of atmospheric CO2 inversion models (the TransCom 3 project), which includes 16 transport models and model variants. We find an uptake of CO2 in the southern extratropical ocean less than that estimated from ocean measurements, a result that is not sensitive to transport models or methodological approaches. We also find a northern land carbon sink that is distributed relatively evenly among the continents of the Northern Hemisphere, but these results show some sensitivity to transport differences among models, especially in how they respond to seasonal terrestrial exchange of CO2. Overall, carbon fluxes integrated over latitudinal zones are strongly constrained by observations in the middle to high latitudes. Further significant constraints to our understanding of regional carbon fluxes will therefore require improvements in transport models and expansion of the CO2 observation network within the tropics.     

No signature of clear CO2 ice from the 'cryptic' regions in Mars' south seasonal polar cap

The seasonal polar ice caps of Mars are composed mainly of CO2 ice. A region of low (< 30%) albedo has been observed within the south seasonal cap during early to mid-spring. The low temperature of this 'cryptic region' has been attributed to a clear slab of nearly pure CO2 ice, with the low albedo resulting from absorption by the underlying surface. Here we report near-infrared imaging spectroscopy of the south seasonal cap. The deep and broad CO2 absorption bands that are expected in the near-infrared with a thick transparent slab of CO2 ice are not observed. Models of the observed spectra indicate that the low albedo results from extensive dust contamination close to the surface of a CO2 ice layer, which could be linked to atmospheric circulation patterns. The strength of the CO2 absorption increases after mid-spring, so part of the dust is either carried away or buried more deeply in the ice layer during the CO2 ice sublimation process.