Differential α4(+)/(-)ß2 Agonist-binding Site Contributions to α4ß2 Nicotinic Acetylcholine Receptor Function within and between Isoforms.

Two α4ß2 nicotinic acetylcholine receptor (α4ß2-nAChR) isoforms exist with (α4)2(ß2)3 and (α4)3(ß2)2 subunit stoichiometries and high versus low agonist sensitivities (HS and LS), respectively. Both isoforms contain a pair of α4(+)/(-)ß2 agonist-binding sites. The LS isoform also contains a unique α4(+)/(-)α4 site with lower agonist affinity than the α4(+)/(-)ß2 sites. However, the relative roles of the conserved α4(+)/(-)ß2 agonist-binding sites in and between the isoforms have not been studied. We used a fully linked subunit concatemeric nAChR approach to express pure populations of HS or LS isoform α4ß2*-nAChR. This approach also allowed us to mutate individual subunit interfaces, or combinations thereof, on each isoform background. We used this approach to systematically mutate a triplet of ß2 subunit (-)-face E-loop residues to their non-conserved α4 subunit counterparts or vice versa (ß2HQT and α4VFL, respectively). Mutant-nAChR constructs (and unmodified controls) were expressed in Xenopus oocytes. Acetylcholine concentration-response curves and maximum function were measured using two-electrode voltage clamp electrophysiology. Surface expression was measured with (125)I-mAb 295 binding and was used to define function/nAChR. If the α4(+)/(-)ß2 sites contribute equally to function, making identical ß2HQT substitutions at either site should produce similar functional outcomes. Instead, highly differential outcomes within the HS isoform, and between the two isoforms, were observed. In contrast, α4VFL mutation effects were very similar in all positions of both isoforms. Our results indicate that the identity of subunits neighboring the otherwise equivalent α4(+)/(-)ß2 agonist sites modifies their contributions to nAChR activation and that E-loop residues are an important contributor to this neighbor effect.

The unique α4+/-α4 agonist binding site in (α4)3(ß2)2 subtype nicotinic acetylcholine receptors permits differential agonist desensitization pharmacology versus the (α4)2(ß2)3 subtype.

Selected nicotinic agonists were used to activate and desensitize high-sensitivity (HS) (α4)2(ß2)3) or low-sensitivity (LS) (α4)3(ß2)2) isoforms of human α4ß2-nicotinic acetylcholine receptors (nAChRs). Function was assessed using (86)Rb(+) efflux in a stably transfected SH-EP1-hα4ß2 human epithelial cell line, and two-electrode voltage-clamp electrophysiology in Xenopus laevis oocytes expressing concatenated pentameric HS or LS α4ß2-nAChR constructs (HSP and LSP). Unlike previously studied agonists, desensitization by the highly selective agonists A-85380 [3-(2(S)-azetidinylmethoxy)pyridine] and sazetidine-A (Saz-A) preferentially reduced α4ß2-nAChR HS-phase versus LS-phase responses. The concatenated-nAChR experiments confirmed that approximately 20% of LS-isoform acetylcholine-induced function occurs in an HS-like phase, which is abolished by Saz-A preincubation. Six mutant LSPs were generated, each targeting a conserved agonist binding residue within the LS-isoform-only α4(+)/(-)α4 interface agonist binding site. Every mutation reduced the percentage of LS-phase function, demonstrating that this site underpins LS-phase function. Oocyte-surface expression of the HSP and each of the LSP constructs was statistically indistinguishable, as measured using ß2-subunit-specific [(125)I]mAb295 labeling. However, maximum function is approximately five times greater on a "per-receptor" basis for unmodified LSP versus HSP α4ß2-nAChRs. Thus, recruitment of the α4(+)/(-)α4 site at higher agonist concentrations appears to augment otherwise-similar function mediated by the pair of α4(+)/(-)ß2 sites shared by both isoforms. These studies elucidate the receptor-level differences underlying the differential pharmacology of the two α4ß2-nAChR isoforms, and demonstrate that HS versus LS α4ß2-nAChR activity can be selectively manipulated using pharmacological approaches. Since α4ß2 nAChRs are the predominant neuronal subtype, these discoveries likely have significant functional implications, and may provide important insights for drug discovery and development.

EBNA1 Inhibitors Block Proliferation of Spontaneous Lymphoblastoid Cell Lines From Patients With Multiple Sclerosis and Healthy Controls.

BACKGROUND AND OBJECTIVES: Epstein-Barr virus (EBV) is a ubiquitous herpesvirus that establishes lifelong latency in memory B cells and has been identified as a major risk factor of multiple sclerosis (MS). B cell depletion therapies have disease-modifying benefit in MS. However, it is unclear whether this benefit is partly attributable to the elimination of EBV+ B cells. Currently, there are no EBV-specific antiviral therapies available for targeting EBV latent infection in MS and limited experimental models to study EBV in MS. METHODS: In this study, we describe the establishment of spontaneous lymphoblastoid cell lines (SLCLs) generated ex vivo with the endogenous EBV of patients with MS and controls and treated with either an Epstein-Barr virus nuclear antigen 1 (EBNA1) inhibitor (VK-1727) or cladribine, a nucleoside analog that eliminates B cells. RESULTS: We showed that a small molecule inhibitor of EBNA1, a critical regulator of the EBV life cycle, blocks the proliferation and metabolic activity of these SLCLs. In contrast to cladribine, a highly cytotoxic B cell depleting therapy currently used in MS, the EBNA1 inhibitor VK-1727 was cytostatic rather than cytotoxic and selective for EBV+ cells, while having no discernible effects on EBV- cells. We validate that VK-1727 reduces EBNA1 DNA binding at known viral and cellular sites by ChIP-qPCR. DISCUSSION: This study shows that patient-derived SLCLs provide a useful tool for interrogating the role of EBV+ B cells in MS and suggests that a clinical trial testing the effect of EBNA1 inhibitors in MS may be warranted.

Biosignature hide and seek.

A new model predicts locations on the surface of radiation-blasted Europa, the ocean moon of Jupiter, where biochemical signatures of life emergent from the subsurface ocean might survive long enough for detection on the moon's changing surface.

Energetic Radiation From Galactic Cosmic Ray Interactions With Saturn's Main Rings.

Saturn's main rings have an energetic particle and gamma ray photon radiation environment produced by ring interactions of galactic cosmic ray (GCR) protons and heavier ions penetrating the planetary dipolar magnetic field. Accurate models of this radiation environment are important for interpretation of Pioneer 11 and Cassini in situ measurements near the rings and for constraints on radiolytic contributions to neutral gas production and ice chemistry. A GEANT (GEometry ANd Tracking) based simulation is used to model flux spectra of protons, electrons, positrons, charged pions, neutrons, and gamma ray photons emitted from GCR interactions with H2O ice spheres approximating the ring material. Dependent on location in the A to D rings within the planetary magnetic field of Saturn, only GCR protons above respective energies of 20 to 72 GeV can reach the rings without being deflected away by the magnetic field. Calculated differential and integral fluxes from our simulations have good agreement with in situ Pioneer-11 measurements in selected energy channels. The charged particle and neutral radiation measurements are sensitive, respectively, to the sizes and areal mass densities of ring bodies. Computed gamma ray emission fluxes are 8% of our calculated limit for detection from the Earth by the Fermi Large Area Telescope. Addition of charged particle sensors and neutron-photon imaging spectrometers to a future Saturn Ring Observer mission would provide valuable information on the ring mass structure. The present paper provides a foundation for modeling of Pioneer 11 and Cassini radiation measurements across the main rings and future measurements of radiation from the rings.

Immunolabeling demonstrates the interdependence of mouse brain alpha4 and beta2 nicotinic acetylcholine receptor subunit expression.

Immunolabeling of beta2 and alpha4 subunits was quantitated in brain sections (14 mum) using [(125)I]mAb 270 and [(125)I]mAb 299, respectively. Specificity was demonstrated by signal loss in beta2(-/-) and alpha4(-/-) brain sections, respectively. Even mild paraformaldehyde fixation severely affected immunolabeling, so this study used unfixed sections. Immunolabeling autoradiography was used to map and quantitate the effects of beta2 and alpha4 subunit-null mutations on their putative partner subunits' protein expression. [(125)I]mAb 299 labeling was nearly eliminated in beta2(-/-) sections, although dorsal interpeduncular nucleus (IPN) retained a faint signal. Therefore, alpha4 subunit expression is almost universally beta2-dependent. In contrast, alpha4-null mutation effects on [(125)I]mAb 270 immunolabeling varied widely among brain regions. In corticothalamic regions, [(125)I]mAb 270 labeling was eliminated. However, in habenulopeduncular regions, alpha4 genotype had no effect. Other (predominantly dopaminergic and optic tract) nuclei also retained reduced [(125)I]mAb 270 labeling in alpha4(-/-) sections. Thus, although most beta2 subunit protein expression is alpha4-dependent, this dependence is not universal. Presumably, residual beta2 subunits are found in non-alpha4* subtypes. Together, these results show that immunolabeling is applicable to reliable, quantitative investigations of neuronal nAChRs, and that subunit-null mutants can be appropriate controls for such experiments. In situ mRNA hybridization was also performed to determine if altered mRNA transcription mediated the interdependence of alpha4 and beta2 subunit expression. alpha4-Null mutation did not affect beta2 mRNA expression, nor did beta2 genotype affect alpha4 mRNA expression. Consequently, it seems that the two subunits' effects on each other's expression are mediated at the protein, rather than gene expression level.

Clathrate hydrates of oxidants in the ice shell of Europa.

Europa's icy surface is radiolytically modified by high-energy electrons and ions, and photolytically modified by solar ultraviolet photons. Observations from the Galileo Near Infrared Mapping Spectrometer, ground-based telescopes, the International Ultraviolet Explorer, and the Hubble Space Telescope, along with laboratory experiment results, indicate that the production of oxidants, such as H2O2, O2, CO2, and SO2, is a consequence of the surface radiolytic chemistry. Once created, some of the products may be entrained deeper into the ice shell through impact gardening or other resurfacing processes. The temperature and pressure environments of regions within the europan hydrosphere are expected to permit the formation of mixed clathrate compounds. The formation of carbon dioxide and sulfur dioxide clathrates has been examined in some detail. Here we add to this analysis by considering oxidants produced radiolytically on the surface of Europa. Our results indicate that the bulk ice shell could have a approximately 1.7-7.6% by number contamination of oxidants resulting from radiolysis at the surface. Oxidant-hosting clathrates would consequently make up approximately 12-53% of the ice shell by number relative to ice, if oxidants were entrained throughout. We examine, in brief, the consequences of such contamination on bulk ice shell thickness and find that clathrate formation could lead to substantially thinner ice shells on Europa than otherwise expected. Finally, we propose that double occupancy of clathrate cages by O2 molecules could serve as an explanation for the observation of condensed-phase O2 on Europa. Clathrate-sealed, gas-filled bubbles in the near surface ice could also provide an effective trapping mechanism, though they cannot explain the 5771 A (O2)2 absorption.