A closely packed system of low-mass, low-density planets transiting Kepler-11

When an extrasolar planet passes in front of (transits) its star, its radius can be measured from the decrease in starlight and its orbital period from the time between transits. Multiple planets transiting the same star reveal much more: period ratios determine stability and dynamics, mutual gravitational interactions reflect planet masses and orbital shapes, and the fraction of transiting planets observed as multiples has implications for the planarity of planetary systems. But few stars have more than one known transiting planet, and none has more than three. Here we report Kepler spacecraft observations of a single Sun-like star, which we call Kepler-11, that reveal six transiting planets, five with orbital periods between 10 and 47?days and a sixth planet with a longer period. The five inner planets are among the smallest for which mass and size have both been measured, and these measurements imply substantial envelopes of light gases. The degree of coplanarity and proximity of the planetary orbits imply energy dissipation near the end of planet formation.     

The cystic fibrosis transmembrane conductance regulator (CFTR) and its stability

The cystic fibrosis transmembrane conductance regulator (CFTR) is responsible for the disease cystic fibrosis (CF). It is a membrane protein belonging to the ABC transporter family functioning as a chloride/anion channel in epithelial cells around the body. There are over 1500 mutations that have been characterised as CF-causing; the most common of these, accounting for ~70 % of CF cases, is the deletion of a phenylalanine at position 508. This leads to instability of the nascent protein and the modified structure is recognised and then degraded by the ER quality control mechanism. However, even pharmacologically ‘rescued’ F508del CFTR displays instability at the cell’s surface, losing its channel function rapidly and it is rapidly removed from the plasma membrane for lysosomal degradation. This review will, therefore, explore the link between stability and structure/function relationships of membrane proteins and CFTR in particular and how approaches to study CFTR structure depend on its stability. We will also review the application of a fluorescence labelling method for the assessment of the thermostability and the tertiary structure of CFTR.     

The ATP-binding cassette family: a structural perspective

The ATP-binding cassette family is one of the largest groupings of membrane proteins, moving allocrites across lipid membranes, using energy from ATP. In bacteria, they reside in the inner membrane and are involved in both uptake and export. In eukaryotes, these transporters reside in the cell’s internal membranes as well as in the plasma membrane and are unidirectional—out of the cytoplasm. The range of substances that these proteins can transport is huge, which makes them interesting for structure–function studies. Moreover, their abundance in nature has made them targets for structural proteomics consortia. There are eight independent structures for ATP-binding cassette transporters, making this one of the best characterised membrane protein families. Our understanding of the mechanism of transport across membranes and membrane protein structure in general has been enhanced by recent developments for this family.     

Effects of paradimethylaminoazobenzene and the antioxidant N,N′-Diphenyl-p-phenylene diamine in developing chicks

Résumé Les embryons de poulet traités au paradiméthylaminoazobenzène (PDAB) sont déformés. Le traitement au N,N-diméthyl-p-phénylène diamine (DPPD) n'immunise pas contre ces déformations, car dans ce cas, les radicaux libres formés par le PDAB n'entrent pas en jeu.

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Supported in part by a grant from the Forsyth Cancer Service.

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Summer Research Fellow, Bowman Gray School of Medicine     

Urinary bladder hyporeflexia and reduced pain-related behaviour in P2X3-deficient mice

Extracellular ATP is implicated in numerous sensory processes ranging from the response to pain to the regulation of motility in visceral organs. The ATP receptor P2X3 is selectively expressed on small diameter sensory neurons, supporting this hypothesis. Here we show that mice deficient in P2X3 lose the rapidly desensitizing ATP-induced currents in dorsal root ganglion neurons. P2X3 deficiency also causes a reduction in the sustained ATP-induced currents in nodose ganglion neurons. P2X3-null mice have reduced pain-related behaviour in response to injection of ATP and formalin. Significantly, P2X3-null mice exhibit a marked urinary bladder hyporeflexia, characterized by decreased voiding frequency and increased bladder capacity, but normal bladder pressures. Immunohistochemical studies localize P2X3 to nerve fibres innervating the urinary bladder of wild-type mice, and show that loss of P2X3 does not alter sensory neuron innervation density. Thus, P2X3 is critical for peripheral pain responses and afferent pathways controlling urinary bladder volume reflexes. Antagonists to P2X3 may therefore have therapeutic potential in the treatment of disorders of urine storage and voiding such as overactive bladder.     

DNase I hypersensitive sites in the chromatin of human mu immunoglobulin heavy-chain genes

An immunoglobulin polypeptide chain is encoded by multiple gene segments that lie far apart in germ-line DNA and must be brought together to allow expression of an immunoglobulin gene active in B lymphocytes. For the immunoglobulin heavy chain genes, one of many variable (V) region genes becomes joined to one of several diversity (D) segments which are fused to one of several joining (J) segments lying 5' of the constant region (C) genes. Here we show that the rearranged mu genes of an IgM-producing human B-lymphocyte cell line exhibit pancreatic deoxyribonuclease (DNase I) hypersensitive sites in the JH-C mu intron that are absent in naked DNA or the chromatin of other differentiated cell types. DNA sequence analysis reveals that the major hypersensitive site maps to a conserved region of the JH-C mu intron recently shown to function as a tissue-specific enhancer of heavy-chain gene expression. A similar association of an enhancer-like element with a DNase I hypersensitive site has been reported for the mouse immunoglobulin light-chain J kappa-C kappa intron. These results implicate disruption of local chromatin structure in the mechanism of immunoglobulin enhancer function.     

Physiological changes in hairless mice maintained on an antioxidant supplemented diet

Summary Several physiological parameters were measured in hairless mice maintained on a diet supplemented with antioxidants. Comparisons to animals on control diet revealed higher water-soluble antioxidant content of skin and increased liver weight. Only small differences in body weight occurred and no distinct histological changes were observed in skin or liver.This investigation was supported by National Research Service Award 1 F32 CAO5062, awarded by the National Cancer Institute, and USPHS Grant CA13464-04 from the NCI.     

Alignment of the stellar spin with the orbits of a three-planet system

The Sun's equator and the planets' orbital planes are nearly aligned, which is presumably a consequence of their formation from a single spinning gaseous disk. For exoplanetary systems this well-aligned configuration is not guaranteed: dynamical interactions may tilt planetary orbits, or stars may be misaligned with the protoplanetary disk through chaotic accretion , magnetic interactions or torques from neighbouring stars. Indeed, isolated 'hot Jupiters' are often misaligned and even orbiting retrograde. Here we report an analysis of transits of planets over starspots on the Sun-like star Kepler-30 (ref. 8), and show that the orbits of its three planets are aligned with the stellar equator. Furthermore, the orbits are aligned with one another to within a few degrees. This configuration is similar to that of our Solar System, and contrasts with the isolated hot Jupiters. The orderly alignment seen in the Kepler-30 system suggests that high obliquities are confined to systems that experienced disruptive dynamical interactions. Should this be corroborated by observations of other coplanar multi-planet systems, then star-disk misalignments would be ruled out as the explanation for the high obliquities of hot Jupiters, and dynamical interactions would be implicated as the origin of hot Jupiters.