Mutations in 15-hydroxyprostaglandin dehydrogenase cause primary hypertrophic osteoarthropathy

Digital clubbing, recognized by Hippocrates in the fifth century BC, is the outward hallmark of pulmonary hypertrophic osteoarthropathy, a clinical constellation that develops secondary to various acquired diseases, especially intrathoracic neoplasm. The pathogenesis of clubbing and hypertrophic osteoarthropathy has hitherto been poorly understood, but a clinically indistinguishable primary (idiopathic) form of hypertrophic osteoarthropathy (PHO) is recognized. This familial disorder can cause diagnostic confusion, as well as significant disability. By autozygosity methods, we mapped PHO to chromosome 4q33-q34 and identified mutations in HPGD, encoding 15-hydroxyprostaglandin dehydrogenase, the main enzyme of prostaglandin degradation. Homozygous individuals develop PHO secondary to chronically elevated prostaglandin E(2) levels. Heterozygous relatives also show milder biochemical and clinical manifestations. These findings not only suggest therapies for PHO, but also imply that clubbing secondary to other pathologies may be prostaglandin mediated. Testing for HPGD mutations and biochemical testing for HPGD deficiency in patients with unexplained clubbing might help to obviate extensive searches for occult pathology.     

Towards a Radical Constructivist Understanding of Science

Constructivism is the idea thatwe construct our own world rather than it beingdetermined by an outside reality. Its mostconsistent form, Radical Constructivism (RC),claims that we cannot transcend ourexperiences. Thus it doesn't make sense to saythat our constructions gradually approach thestructure of an external reality. The mind isnecessarily an epistemological solipsist, incontrast to being an ontological solipsist whomaintains that this is all there is, namely asingle mind within which the only world exists.RC recognizes the impossibility of the claimthat the world does not exist. Yet, RC has thepotential to go much further. I claim that RCprovides the foundation of a new world-view inwhich we can overcome hard scientific problems.Thus, the paper is urging us to carry RCfurther, not just on philosophical grounds, butalso into the domain of science.     

Presentation of viral antigen controlled by a gene in the major histocompatibility complex

We describe a mutant human cell line (LBL 721.174) that has lost a function required for presentation of intracellular viral antigens with class I molecules of the major histocompatibility complex (MHC), but retains the capacity to present defined epitopes as extracellular peptides. The cell also has a defect in the assembly and expression of class I MHC molecules, which we show can be restored by exposure of the cells to a peptide epitope. This phenotype suggests a defect in the association of intracellular antigen with class I molecules similar to that described for the murine mutant RMA-S (ref. 5), but in the present case the genetic defect can be mapped within the MHC locus on human chromosome 6.     

A star in a 15.2-year orbit around the supermassive black hole at the centre of the Milky Way

Many galaxies are thought to have supermassive black holes at their centres-more than a million times the mass of the Sun. Measurements of stellar velocities and the discovery of variable X-ray emission have provided strong evidence in favour of such a black hole at the centre of the Milky Way, but have hitherto been unable to rule out conclusively the presence of alternative concentrations of mass. Here we report ten years of high-resolution astrometric imaging that allows us to trace two-thirds of the orbit of the star currently closest to the compact radio source (and massive black-hole candidate) Sagittarius A*. The observations, which include both pericentre and apocentre passages, show that the star is on a bound, highly elliptical keplerian orbit around Sgr A*, with an orbital period of 15.2 years and a pericentre distance of only 17 light hours. The orbit with the best fit to the observations requires a central point mass of (3.7 +/- 1.5) x 10(6) solar masses (M(*)). The data no longer allow for a central mass composed of a dense cluster of dark stellar objects or a ball of massive, degenerate fermions.     

Alternative nucleotide incision repair pathway for oxidative DNA damage.

The DNA glycosylase pathway, which requires the sequential action of two enzymes for the incision of DNA, presents a serious problem for the efficient repair of oxidative DNA damage, because it generates genotoxic intermediates such as abasic sites and/or blocking 3'-end groups that must be eliminated by additional steps before DNA repair synthesis can be initiated. Besides the logistical problems, biological evidence hints at the existence of an alternative repair pathway. Mutants of Escherichia coli and mice (ref. 4 and M. Takao et al., personal communication) that are deficient in DNA glycosylases that remove oxidized bases are not sensitive to reactive oxygen species, and the E. coli triple mutant nei, nth, fpg is more radioresistant than the wild-type strain. Here we show that Nfo-like endonucleases nick DNA on the 5' side of various oxidatively damaged bases, generating 3'-hydroxyl and 5'-phosphate termini. Nfo-like endonucleases function next to each of the modified bases that we tested, including 5,6-dihydrothymine, 5,6-dihydrouracil, 5-hydroxyuracil and 2,6-diamino-4-hydroxy-5-N-methylformamidopyrimidine residues. The 3'-hydroxyl terminus provides the proper end for DNA repair synthesis; the dangling damaged nucleotide on the 5' side is then a good substrate for human flap-structure endonuclease and for DNA polymerase I of E. coli.     

The dusk flank of Jupiter's magnetosphere

Limited single-spacecraft observations of Jupiter's magnetopause have been used to infer that the boundary moves inward or outward in response to variations in the dynamic pressure of the solar wind. At Earth, multiple-spacecraft observations have been implemented to understand the physics of how this motion occurs, because they can provide a snapshot of a transient event in progress. Here we present a set of nearly simultaneous two-point measurements of the jovian magnetopause at a time when the jovian magnetopause was in a state of transition from a relatively larger to a relatively smaller size in response to an increase in solar-wind pressure. The response of Jupiter's magnetopause is very similar to that of the Earth, confirming that the understanding built on studies of the Earth's magnetosphere is valid. The data also reveal evidence for a well-developed boundary layer just inside the magnetopause.