Germline BAP1 mutations predispose to malignant mesothelioma

Because only a small fraction of asbestos-exposed individuals develop malignant mesothelioma, and because mesothelioma clustering is observed in some families, we searched for genetic predisposing factors. We discovered germline mutations in the gene encoding BRCA1 associated protein-1 (BAP1) in two families with a high incidence of mesothelioma, and we observed somatic alterations affecting BAP1 in familial mesotheliomas, indicating biallelic inactivation. In addition to mesothelioma, some BAP1 mutation carriers developed uveal melanoma. We also found germline BAP1 mutations in 2 of 26 sporadic mesotheliomas; both individuals with mutant BAP1 were previously diagnosed with uveal melanoma. We also observed somatic truncating BAP1 mutations and aberrant BAP1 expression in sporadic mesotheliomas without germline mutations. These results identify a BAP1-related cancer syndrome that is characterized by mesothelioma and uveal melanoma. We hypothesize that other cancers may also be involved and that mesothelioma predominates upon asbestos exposure. These findings will help to identify individuals at high risk of mesothelioma who could be targeted for early intervention.     

Magneto-thermal convection in solar prominences

Coronal cavities are large low-density regions formed by hemispheric-scale magnetic flux ropes suspended in the Sun's outer atmosphere. They evolve over time, eventually erupting as the dark cores of coronal mass ejections. Although coronal mass ejections are common and can significantly affect planetary magnetospheres, the mechanisms by which cavities evolve to an eruptive state remain poorly understood. Recent optical observations of high-latitude 'polar crown' prominences within coronal cavities reveal dark, low-density 'bubbles' that undergo Rayleigh-Taylor instabilities to form dark plumes rising into overlying coronal cavities. These observations offered a possible mechanism for coronal cavity evolution, although the nature of the bubbles, particularly their buoyancy, was hitherto unclear. Here we report simultaneous optical and extreme-ultraviolet observations of polar crown prominences that show that these bubbles contain plasma at temperatures in the range (2.5-12)?×?10(5) kelvin, which is 25-120 times hotter than the overlying prominence. This identifies a source of the buoyancy, and suggests that the coronal cavity-prominence system supports a novel form of magneto-thermal convection in the solar atmosphere, challenging current hydromagnetic concepts of prominences and their relation to coronal cavities.     

The sodium channel and intracellular H+ blockage in squid axons

Sodium channels in plasma membranes can be blocked by a large variety of toxins and local anaesthetics. This property, however, is not confined to relatively large molecules. For instance, extracellularly applied small ions like hydrogen may also prevent the passive transport of permeant cations across open Na+ channels. A typical feature of this phenomenon is that the blocking action of hydrogen is gradually relieved by increasing the voltage applied across the membrane. Although in the frog skeletal muscle there is no clear evidence for a similar intracellular action, we report here for the squid giant axon remarkable effects on the ionic permeability of Na+ channels when the internal perfusate contains an excess of protons. Analysing the action of low pH inside and outside the fibre in terms of a kinetic model, we could conclude that Na+ channels in squid axons are controlled by two independent groups: one with an apparent pKa of 4.6 and the other with pKa 5.8, the former feeling one-fifth of the applied membrane potential, the latter three-quarters. As with pharmacological agents, we also show that the voltage-dependence of the H+ blockage is not affected by the presence of the inactivation gate.     

Physicochemical profiling in drug research: a brief survey of the state-of-the-art of experimental techniques

This review begins with a general presentation of the new paradigm of drug discovery, with its emphasis on the rapid identification and elimination of compounds with unsuitable physicochemical and pharmacokinetic properties. The focus of the paper is on the various experimental methods used to determine such key physicochemical properties as ionization, lipophilicity and distribution in isotropic and anisotropic systems, solubility, and permeability across artificial membranes. Both traditional and high-throughput methods are presented and their limits highlighted. The text concludes with the trade-off between quantity/speed in high-throughput screening techniques versus greater data quality in the more labor-intensive methods. Received 23 April 2002; received after revision 25 June 2002; accepted 11 July 2002 RID="*" ID="*"Corresponding author.     

A new series of potential anabolic steroids: [2,3-d]-triazolosteroids

Zusammenfassung Es werden einige neue am A-Ring mit einem Triazolring kondensierte Steroide beschrieben. Diese werden durch Umsetzung der Enamine der 3-Ketosteroide mit Arylaziden oder Azidoformiaten und nachfolgende Abspaltung des basischen Restes hergestellt.     

The 'solar model problem' solved by the abundance of neon in nearby stars

The interior structure of the Sun can be studied with great accuracy using observations of its oscillations, similar to seismology of the Earth. Precise agreement between helioseismological measurements and predictions of theoretical solar models has been a triumph of modern astrophysics. A recent downward revision by 25-35 per cent of the solar abundances of light elements such as C, N, O and Ne (ref. 2) has, however, broken this accordance: models adopting the new abundances incorrectly predict the depth of the convection zone, the depth profiles of sound speed and density, and the helium abundance. The discrepancies are far beyond the uncertainties in either the data or the model predictions. Here we report neon-to-oxygen ratios measured in a sample of nearby solar-like stars, using their X-ray spectra. The abundance ratios are all very similar and substantially larger than the recently revised solar value. The neon abundance in the Sun is quite poorly determined. If the Ne/O abundance in these stars is adopted for the Sun, the models are brought back into agreement with helioseismology measurements.     

Effect of topically applied phenobarbital on O-dealkylase activity in mouse skin

Summary Topical application of phenobarbital to mice produces an increase in cutaneous microsomal proteins and apparently also of cytochrome P450, but results in a kinetically noncompetitive inhibition of p-nitrophenethole O-dealkylase activity in preparations of 10,000×g supernatant from skin.