Present status of underwater medicine. Review of some challenging problems

Zusammenfassung Es wird eine Übersicht über den gegenwärtigen Stand der Unterwassermedizin gegeben. Besondere Berücksichtigung finden die in jüngster Zeit durchgeführten Forschungen, die die Grundlage für eine Erweiterung der Grenzen des Tieftauchens bereiteten, wie z.B. der 1972 durchgeführte Rekordtauchgang der Comex Gruppe, bei dem eine Tiefe von 2001 Fuss (610 m) in der Kammer erreicht wurde. Nach den in diesem Experiment erhobenen Befunden können ausgewählte und trainierte Taucher in einer Tiefe von 1400 Fuss (427 m) noch gut arbeiten und leben, wenn sie eine Helium-Sauerstoffmischung atmen. Die Ursachen des «Nervösen Hochdruck-Syndromes», sowie die kritische Volumentherorie vonMiller ⁶ als ein Erklärungsversuch für das Fehlen der narkotischen Wirkung von Helium unter hohem Druck im Vergleich zu Stickstoff werden diskutiert.

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This paper was presented in part at the XXI International Congress of Aviation and Space Medicine, September 19, 1973 in Munich (Germany, Fed. Rep.).     

Recognition of transmembrane helices by the endoplasmic reticulum translocon

Membrane proteins depend on complex translocation machineries for insertion into target membranes. Although it has long been known that an abundance of nonpolar residues in transmembrane helices is the principal criterion for membrane insertion, the specific sequence-coding for transmembrane helices has not been identified. By challenging the endoplasmic reticulum Sec61 translocon with an extensive set of designed polypeptide segments, we have determined the basic features of this code, including a 'biological' hydrophobicity scale. We find that membrane insertion depends strongly on the position of polar residues within transmembrane segments, adding a new dimension to the problem of predicting transmembrane helices from amino acid sequences. Our results indicate that direct protein-lipid interactions are critical during translocon-mediated membrane insertion.     

A high abundance of massive galaxies 3-6 billion years after the Big Bang

Hierarchical galaxy formation is the model whereby massive galaxies form from an assembly of smaller units. The most massive objects therefore form last. The model succeeds in describing the clustering of galaxies, but the evolutionary history of massive galaxies, as revealed by their visible stars and gas, is not accurately predicted. Near-infrared observations (which allow us to measure the stellar masses of high-redshift galaxies) and deep multi-colour images indicate that a large fraction of the stars in massive galaxies form in the first 5 Gyr (refs 4-7), but uncertainties remain owing to the lack of spectra to confirm the redshifts (which are estimated from the colours) and the role of obscuration by dust. Here we report the results of a spectroscopic redshift survey that probes the most massive and quiescent galaxies back to an era only 3 Gyr after the Big Bang. We find that at least two-thirds of massive galaxies have appeared since this era, but also that a significant fraction of them are already in place in the early Universe.     

The Collaborative Cross, a community resource for the genetic analysis of complex traits

The goal of the Complex Trait Consortium is to promote the development of resources that can be used to understand, treat and ultimately prevent pervasive human diseases. Existing and proposed mouse resources that are optimized to study the actions of isolated genetic loci on a fixed background are less effective for studying intact polygenic networks and interactions among genes, environments, pathogens and other factors. The Collaborative Cross will provide a common reference panel specifically designed for the integrative analysis of complex systems and will change the way we approach human health and disease.     

Climate (communication arising): impact of land-use change on climate

Urbanization and other changes in land use have an impact on surface-air temperatures. Kalnay and Cai report that the observed surface-temperature trend in part of the United States exceeds the trend in the NCEP/NCAR 50-year reanalysis (NNR) and conclude that changes in land use account for the difference (0.035 degrees C per decade according to their corrected values). Although land-use change may explain some of this discrepancy, the authors do not quantify the impact of the many changes in observational practice that occurred during the analysis period. Our findings indicate that these 'non-climatic' changes have a systematic effect that overwhelms the reported difference in trends and therefore calls Kalnay and Cai's central conclusion into question.