A large genome-wide association study of age-related macular degeneration highlights contributions of rare and common variants.

This is the author accepted manuscript. The final version is available from Nature Publishing Group via http://dx.doi.org/10.1038/ng.3448Advanced age-related macular degeneration (AMD) is the leading cause of blindness in the elderly, with limited therapeutic options. Here we report on a study of >12 million variants, including 163,714 directly genotyped, mostly rare, protein-altering variants. Analyzing 16,144 patients and 17,832 controls, we identify 52 independently associated common and rare variants (P < 5 × 10(-8)) distributed across 34 loci. Although wet and dry AMD subtypes exhibit predominantly shared genetics, we identify the first genetic association signal specific to wet AMD, near MMP9 (difference P value = 4.1 × 10(-10)). Very rare coding variants (frequency <0.1%) in CFH, CFI and TIMP3 suggest causal roles for these genes, as does a splice variant in SLC16A8. Our results support the hypothesis that rare coding variants can pinpoint causal genes within known genetic loci and illustrate that applying the approach systematically to detect new loci requires extremely large sample sizes.We thank all participants of all the studies included for enabling this research by their participation in these studies. Computer resources for this project have been provided by the high-performance computing centers of the University of Michigan and the University of Regensburg. Group-specific acknowledgments can be found in the Supplementary Note. The Center for Inherited Diseases Research (CIDR) Program contract number is HHSN268201200008I. This and the main consortium work were predominantly funded by 1X01HG006934-01 to G.R.A. and R01 EY022310 to J.L.H

The dynamic geophysical environment of (101955) Bennu based on OSIRIS-REx measurements

The top-shaped morphology characteristic of asteroid (101955) Bennu, often found among fast-spinning asteroids and binary asteroid primaries, may have contributed substantially to binary asteroid formation. Yet a detailed geophysical analysis of this morphology for a fast-spinning asteroid has not been possible prior to the Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer (OSIRIS-REx) mission. Combining the measured Bennu mass and shape obtained during the Preliminary Survey phase of the OSIRIS-REx mission, we find a notable transition in Bennu’s surface slopes within its rotational Roche lobe, defined as the region where material is energetically trapped to the surface. As the intersection of the rotational Roche lobe with Bennu’s surface has been most recently migrating towards its equator (given Bennu’s increasing spin rate), we infer that Bennu’s surface slopes have been changing across its surface within the last million years. We also find evidence for substantial density heterogeneity within this body, suggesting that its interior is a mixture of voids and boulders. The presence of such heterogeneity and Bennu’s top shape are consistent with spin-induced failure at some point in its past, although the manner of its failure cannot yet be determined. Future measurements by the OSIRIS-REx spacecraft will provide insight into and may resolve questions regarding the formation and evolution of Bennu’s top-shape morphology and its link to the formation of binary asteroids

Evidence for widespread hydrated minerals on asteroid (101955) Bennu

Early spectral data from the Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer (OSIRIS-REx) mission reveal evidence for abundant hydrated minerals on the surface of near-Earth asteroid (101955) Bennu in the form of a near-infrared absorption near 2.7 µm and thermal infrared spectral features that are most similar to those of aqueously altered CM-type carbonaceous chondrites. We observe these spectral features across the surface of Bennu, and there is no evidence of substantial rotational variability at the spatial scales of tens to hundreds of metres observed to date. In the visible and near-infrared (0.4 to 2.4 µm) Bennu’s spectrum appears featureless and with a blue (negative) slope, confirming previous ground-based observations. Bennu may represent a class of objects that could have brought volatiles and organic chemistry to Earth

Academics online: reflections on gendered precarity and digital (self) surveillance

This chapter traces the shift in conceptualisations of academic time to understand what affect time and temporality has on academic women’s identities and performativities. The traditional linear career trajectory of an academic is being displaced by far more fractured academic life course. This chapter focuses on how new technologies of time operate discursively to both assist and impair academic labour, interrogating the gendered relationship between precarity and academics’ engagement with social media and academic professional networking sites. Entanglement with these websites is not simply symptomatic of an increasingly globalised and intensified academy, but is, in fact, driving the intensification of academic work, gendered job precarity, and (self) surveillance

Mutations in CTNNA1 cause butterfly-shaped pigment dystrophy and perturbed retinal pigment epithelium integrity

Butterfly-shaped pigment dystrophy is an eye disease characterized by lesions in the macula that can resemble the wings of a butterfly. Here we report the identification of heterozygous missense mutations in the CTNNA1 gene (encoding alpha-catenin 1) in three families with butterfly-shaped pigment dystrophy. In addition, we identified a Ctnna1 missense mutation in a chemically induced mouse mutant, tvrm5. Parallel clinical phenotypes were observed in the retinal pigment epithelium (RPE) of individuals with butterfly-shaped pigment dystrophy and in tvrm5 mice, including pigmentary abnormalities, focal thickening and elevated lesions, and decreased light-activated responses. Morphological studies in tvrm5 mice demonstrated increased cell shedding and the presence of large multinucleated RPE cells, suggesting defects in intercellular adhesion and cytokinesis. This study identifies CTNNA1 gene variants as a cause of macular dystrophy, indicates that CTNNA1 is involved in maintaining RPE integrity and suggests that other components that participate in intercellular adhesion may be implicated in macular disease

Exostoses of the Bony Pyramid of the Nose : A Review About an Adaptive Response to Mechanical Stimuli Exerted by In-Flight Oxygen Masks

This review addresses thickening of the bony pyramid of the nose, a condition that is caused by in-flight oxygen masks in otherwise healthy Royal Netherlands Air Force (RNLAF) F-16 pilots. The overlying skin may show temporary or permanent reddening, irritation, thickening and may become painful. Both in vitro and in vivo animal research has shown that mechanical stimuli are converted into a biochemical response through a process called mechanotransduction. Examination of the RNLAF F-16 pilots showed that the oxygen mask exerts pressure and friction on the nose. The biochemical response to chronic exposure to these stimuli results in the development of skin conditions and eventually exostoses of the bony pyramid of the nose. Painful skin conditions are most frequently observed, while the development of exostoses is rare. It lies at the extreme end of the spectrum of the pilots’ nasal conditions. The suboptimal fit of their work gear probably contributes to the pilots’ soft and bony tissue nasal conditions. Explaining the pathogenesis of the development of exostoses may aid in the development of preventive measures. Also, the obtained knowledge may be of use in similar occupational health issues that involve mechanical loading. Our conclusions are that areas containing osteocyte precursors and covered by a relatively thin cushioning layer are prone to develop a soft tissue and bony tissue response when they are chronically exposed to intermittently exerted, mechanical stimuli of sufficiently high magnitude. Modification of the suboptimally fitting oxygen mask–helmet assembly is needed to prevent symptoms associated with its use