Large-scale cryovolcanic resurfacing on Pluto

The New Horizons spacecraft returned images and compositional data showing that terrains on Pluto span a variety of ages, ranging from relatively ancient, heavily cratered areas to very young surfaces with few-to-no impact craters. One of the regions with very few impact craters is dominated by enormous rises with hummocky flanks. Similar features do not exist anywhere else in the imaged solar system. Here we analyze the geomorphology and composition of the features and conclude this region was resurfaced by cryovolcanic processes, of a type and scale so far unique to Pluto. Creation of this terrain requires multiple eruption sites and a large volume of material (>10⁴ km³) to form what we propose are multiple, several-km-high domes, some of which merge to form more complex planforms. The existence of these massive features suggests Pluto’s interior structure and evolution allows for either enhanced retention of heat or more heat overall than was anticipated before New Horizons, which permitted mobilization of water-ice-rich materials late in Pluto’s history.

Giant icy volcanos (cryovolcanos) on Pluto are unique in the imaged solar system and provide evidence for unexpected, active geology late in Pluto’s history.

The geology and geophysics of Kuiper Belt object (486958) Arrokoth

The Cold Classical Kuiper Belt, a class of small bodies in undisturbed orbits beyond Neptune, is composed of primitive objects preserving information about Solar System formation. In January 2019, the New Horizons spacecraft flew past one of these objects, the 36-kilometer-long contact binary (486958) Arrokoth (provisional designation 2014 MU₆₉). Images from the flyby show that Arrokoth has no detectable rings, and no satellites (larger than 180 meters in diameter) within a radius of 8000 kilometers. Arrokoth has a lightly cratered, smooth surface with complex geological features, unlike those on previously visited Solar System bodies. The density of impact craters indicates the surface dates from the formation of the Solar System. The two lobes of the contact binary have closely aligned poles and equators, constraining their accretion mechanism.

Color, composition, and thermal environment of Kuiper Belt object (486958) Arrokoth

The outer Solar System object (486958) Arrokoth (provisional designation 2014 MU₆₉) has been largely undisturbed since its formation. We studied its surface composition using data collected by the New Horizons spacecraft. Methanol ice is present along with organic material, which may have formed through irradiation of simple molecules. Water ice was not detected. This composition indicates hydrogenation of carbon monoxide-rich ice and/or energetic processing of methane condensed on water ice grains in the cold, outer edge of the early Solar System. There are only small regional variations in color and spectra across the surface, which suggests that Arrokoth formed from a homogeneous or well-mixed reservoir of solids. Microwave thermal emission from the winter night side is consistent with a mean brightness temperature of 29 ± 5 kelvin.

The solar nebula origin of (486958) Arrokoth, a primordial contact binary in the Kuiper Belt

The New Horizons spacecraft's encounter with the cold classical Kuiper Belt object (486958) Arrokoth (provisional designation 2014 MU₆₉) revealed a contact-binary planetesimal. We investigated how Arrokoth formed and found that it is the product of a gentle, low-speed merger in the early Solar System. Its two lenticular lobes suggest low-velocity accumulation of numerous smaller planetesimals within a gravitationally collapsing cloud of solid particles. The geometric alignment of the lobes indicates that they were a co-orbiting binary that experienced angular momentum loss and subsequent merger, possibly because of dynamical friction and collisions within the cloud or later gas drag. Arrokoth's contact-binary shape was preserved by the benign dynamical and collisional environment of the cold classical Kuiper Belt and therefore informs the accretion processes that operated in the early Solar System.

Initial results from the New Horizons exploration of 2014 MU69, a small Kuiper Belt object

The Kuiper Belt is a distant region of the outer Solar System. On 1 January 2019, the New Horizons spacecraft flew close to (486958) 2014 MU₆₉, a cold classical Kuiper Belt object approximately 30 kilometers in diameter. Such objects have never been substantially heated by the Sun and are therefore well preserved since their formation. We describe initial results from these encounter observations. MU₆₉ is a bilobed contact binary with a flattened shape, discrete geological units, and noticeable albedo heterogeneity. However, there is little surface color or compositional heterogeneity. No evidence for satellites, rings or other dust structures, a gas coma, or solar wind interactions was detected. MU₆₉'s origin appears consistent with pebble cloud collapse followed by a low-velocity merger of its two lobes.

Impact craters on Pluto and Charon indicate a deficit of small Kuiper belt objects

The flyby of Pluto and Charon by the New Horizons spacecraft provided high-resolution images of cratered surfaces embedded in the Kuiper belt, an extensive region of bodies orbiting beyond Neptune. Impact craters on Pluto and Charon were formed by collisions with other Kuiper belt objects (KBOs) with diameters from ~40 kilometers to ~300 meters, smaller than most KBOs observed directly by telescopes. We find a relative paucity of small craters ≲13 kilometers in diameter, which cannot be explained solely by geological resurfacing. This implies a deficit of small KBOs (≲1 to 2 kilometers in diameter). Some surfaces on Pluto and Charon are likely ≳4 billion years old, thus their crater records provide information on the size-frequency distribution of KBOs in the early Solar System.

Enceladus Plume Structure and Time Variability: Comparison of Cassini Observations

During three low-altitude (99, 66, 66 km) flybys through the Enceladus plume in 2010 and 2011, Cassini's ion neutral mass spectrometer (INMS) made its first high spatial resolution measurements of the plume's gas density and distribution, detecting in situ the individual gas jets within the broad plume. Since those flybys, more detailed Imaging Science Subsystem (ISS) imaging observations of the plume's icy component have been reported, which constrain the locations and orientations of the numerous gas/grain jets. In the present study, we used these ISS imaging results, together with ultraviolet imaging spectrograph stellar and solar occultation measurements and modeling of the three-dimensional structure of the vapor cloud, to constrain the magnitudes, velocities, and time variability of the plume gas sources from the INMS data. Our results confirm a mixture of both low and high Mach gas emission from Enceladus' surface tiger stripes, with gas accelerated as fast as Mach 10 before escaping the surface. The vapor source fluxes and jet intensities/densities vary dramatically and stochastically, up to a factor 10, both spatially along the tiger stripes and over time between flyby observations. This complex spatial variability and dynamics may result from time-variable tidal stress fields interacting with subsurface fissure geometry and tortuosity beyond detectability, including changing gas pathways to the surface, and fluid flow and boiling in response evolving lithostatic stress conditions. The total plume gas source has 30% uncertainty depending on the contributions assumed for adiabatic and nonadiabatic gas expansion/acceleration to the high Mach emission. The overall vapor plume source rate exhibits stochastic time variability up to a factor ∼5 between observations, reflecting that found in the individual gas sources/jets. Key Words: Cassini at Saturn-Geysers-Enceladus-Gas dynamics-Icy satellites. Astrobiology 17, 926-940.

Charon tectonics

New Horizons images of Pluto's companion Charon show a variety of terrains that display extensional tectonic features, with relief surprising for this relatively small world. These features suggest a global extensional areal strain of order 1% early in Charon's history. Such extension is consistent with the presence of an ancient global ocean, now frozen.

The geology of Pluto and Charon through the eyes of New Horizons

NASA's New Horizons spacecraft has revealed the complex geology of Pluto and Charon. Pluto's encounter hemisphere shows ongoing surface geological activity centered on a vast basin containing a thick layer of volatile ices that appears to be involved in convection and advection, with a crater retention age no greater than ~10 million years. Surrounding terrains show active glacial flow, apparent transport and rotation of large buoyant water-ice crustal blocks, and pitting, the latter likely caused by sublimation erosion and/or collapse. More enigmatic features include tall mounds with central depressions that are conceivably cryovolcanic and ridges with complex bladed textures. Pluto also has ancient cratered terrains up to ~4 billion years old that are extensionally faulted and extensively mantled and perhaps eroded by glacial or other processes. Charon does not appear to be currently active, but experienced major extensional tectonism and resurfacing (probably cryovolcanic) nearly 4 billion years ago. Impact crater populations on Pluto and Charon are not consistent with the steepest impactor size-frequency distributions proposed for the Kuiper belt.

The small satellites of Pluto as observed by New Horizons

The New Horizons mission has provided resolved measurements of Pluto's moons Styx, Nix, Kerberos, and Hydra. All four are small, with equivalent spherical diameters of ~40 kilometers for Nix and Hydra and ~10 kilometers for Styx and Kerberos. They are also highly elongated, with maximum to minimum axis ratios of ~2. All four moons have high albedos (~50 to 90%) suggestive of a water-ice surface composition. Crater densities on Nix and Hydra imply surface ages of at least 4 billion years. The small moons rotate much faster than synchronous, with rotational poles clustered nearly orthogonal to the common pole directions of Pluto and Charon. These results reinforce the hypothesis that the small moons formed in the aftermath of a collision that produced the Pluto-Charon binary.

Female neuregulin 1 heterozygous mice require repeated exposure to Δ⁹-tetrahydrocannabinol to alter sensorimotor gating function

INTRODUCTION

The schizophrenia susceptibility gene neuregulin 1 (NRG1) confers vulnerability to the neurobehavioural eff ects of cannabinoids differently across sexes. Male but not female Nrg1 heterozygous (HET) mice display facilitation of prepulse inhibition (PPI) to acute Δ⁹-tetrahydrocannabinol (THC) exposure compared to WT controls. We aim to observe whether repeated administration of THC may overcome the acute insensitivity of female Nrg1 HET mice to THC exposure.

METHODS

Female Nrg1 HET mice and WT controls were administered THC daily for 21 days, with PPI and anxiety-related behaviour in the light-dark test (LD) examined on the fi rst and last day of treatment and 21 days after cessation of dosing.

RESULTS

Following repeated, but not acute THC exposure, female Nrg1 HET mice displayed THC-induced facilitation of PPI which was not observed in WT mice treated with THC. There were no residual eff ects of THC on PPI in either genotype when assessed 21 days following the final THC dose. An anxiogenic response to THC was evident following repeated, but not acute, administration in the LD test in both genotypes.

DISCUSSION

These findings show that the acute insensitivity of female Nrg1 HET mice to THC-induced PPI facilitation may be overcome following repeated THC exposure.

Volcanic Activity on lo at the Time of the Ulysses Encounter

The population of heavy ions in lo's torus is ultimately derived from lo volcanism. Groundbased infrared observations of lo between October 1991 and March 1992, contemporaneous with the 8 February 1992 Ulysses observations of the lo torus, show that volcanic thermal emission was at the low end of the normal range at all lo longitudes during this period. In particular, the dominant hot spot Loki was quiescent. Resolved images show that there were at least four hot spots on lo's Jupiter-facing hemisphere, including Loki and a long-lived spot on the leading hemisphere (Kanehekili), of comparable 3.5-micrometer brightness but higher temperature.

Io volcanism seen by new horizons: a major eruption of the Tvashtar volcano

Jupiter's moon Io is known to host active volcanoes. In February and March 2007, the New Horizons spacecraft obtained a global snapshot of Io's volcanism. A 350-kilometer-high volcanic plume was seen to emanate from the Tvashtar volcano (62 degrees N, 122 degrees W), and its motion was observed. The plume's morphology and dynamics support nonballistic models of large Io plumes and also suggest that most visible plume particles condensed within the plume rather than being ejected from the source. In images taken in Jupiter eclipse, nonthermal visible-wavelength emission was seen from individual volcanoes near Io's sub-Jupiter and anti-Jupiter points. Near-infrared emission from the brightest volcanoes indicates minimum magma temperatures in the 1150- to 1335-kelvin range, consistent with basaltic composition.

New horizons mapping of Europa and Ganymede

The New Horizons spacecraft observed Jupiter's icy satellites Europa and Ganymede during its flyby in February and March 2007 at visible and infrared wavelengths. Infrared spectral images map H2O ice absorption and hydrated contaminants, bolstering the case for an exogenous source of Europa's "non-ice" surface material and filling large gaps in compositional maps of Ganymede's Jupiter-facing hemisphere. Visual wavelength images of Europa extend knowledge of its global pattern of arcuate troughs and show that its surface scatters light more isotropically than other icy satellites.

Jupiter cloud composition, stratification, convection, and wave motion: a view from new horizons

Several observations of Jupiter's atmosphere made by instruments on the New Horizons spacecraft have implications for the stability and dynamics of Jupiter's weather layer. Mesoscale waves, first seen by Voyager, have been observed at a spatial resolution of 11 to 45 kilometers. These waves have a 300-kilometer wavelength and phase velocities greater than the local zonal flow by 100 meters per second, much higher than predicted by models. Additionally, infrared spectral measurements over five successive Jupiter rotations at spatial resolutions of 200 to 140 kilometers have shown the development of transient ammonia ice clouds (lifetimes of 40 hours or less) in regions of strong atmospheric upwelling. Both of these phenomena serve as probes of atmospheric dynamics below the visible cloud tops.

Shear heating as the origin of the plumes and heat flux on Enceladus

Enceladus, a small icy satellite of Saturn, has active plumes jetting from localized fractures ('tiger stripes') within an area of high heat flux near the south pole. The plume characteristics and local high heat flux have been ascribed either to the presence of liquid water within a few tens of metres of the surface, or the decomposition of clathrates. Neither model addresses how delivery of internal heat to the near-surface is sustained. Here we show that the most likely explanation for the heat and vapour production is shear heating by tidally driven lateral (strike-slip) fault motion with displacement of approximately 0.5 m over a tidal period. Vapour produced by this heating may escape as plumes through cracks reopened by the tidal stresses. The ice shell thickness needed to produce the observed heat flux is at least 5 km. The tidal displacements required imply a Love number of h2 > 0.01, suggesting that the ice shell is decoupled from the silicate interior by a subsurface ocean. We predict that the tiger-stripe regions with highest relative temperatures will be the lower-latitude branch of Damascus, Cairo around 60 degrees W longitude and Alexandria around 150 degrees W longitude.

A Clathrate Reservoir Hypothesis for Enceladus' South Polar Plume

We hypothesize that active tectonic processes in the south polar terrain of Enceladus, the 500-kilometer-diameter moon of Saturn, are creating fractures that cause degassing of a clathrate reservoir to produce the plume documented by the instruments on the Cassini spacecraft. Advection of gas and ice transports energy, supplied at depth as latent heat of clathrate decomposition, to shallower levels, where it reappears as latent heat of condensation of ice. The plume itself, which has a discharge rate comparable to Old Faithful Geyser in Yellowstone National Park, probably represents small leaks from this massive advective system.

Cassini encounters Enceladus: background and the discovery of a south polar hot spot

The Cassini spacecraft completed three close flybys of Saturn's enigmatic moon Enceladus between February and July 2005. On the third and closest flyby, on 14 July 2005, multiple Cassini instruments detected evidence for ongoing endogenic activity in a region centered on Enceladus' south pole. The polar region is the source of a plume of gas and dust, which probably emanates from prominent warm troughs seen on the surface. Cassini's Composite Infrared Spectrometer (CIRS) detected 3 to 7 gigawatts of thermal emission from the south polar troughs at temperatures up to 145 kelvin or higher, making Enceladus only the third known solid planetary body-after Earth and Io-that is sufficiently geologically active for its internal heat to be detected by remote sensing. If the plume is generated by the sublimation of water ice and if the sublimation source is visible to CIRS, then sublimation temperatures of at least 180 kelvin are required.

A giant impact origin for Pluto's small moons and satellite multiplicity in the Kuiper belt

The two newly discovered satellites of Pluto (P1 and P2) have masses that are small compared to both Pluto and Charon-that is, between 5 x 10(-4) and 1 x 10(-5) of Pluto's mass, and between 5 x 10(-3) and 1 x 10(-4) of Charon's mass. This discovery, combined with the constraints on the absence of more distant satellites of Pluto, reveal that Pluto and its moons comprise an unusual, highly compact, quadruple system. These facts naturally raise the question of how this puzzling satellite system came to be. Here we show that P1 and P2's proximity to Pluto and Charon, the fact that P1 and P2 are on near-circular orbits in the same plane as Pluto's large satellite Charon, along with their apparent locations in or near high-order mean-motion resonances, all probably result from their being constructed from collisional ejecta that originated from the Pluto-Charon formation event. We also argue that dust-ice rings of variable optical depths form sporadically in the Pluto system, and that rich satellite systems may be found--perhaps frequently--around other large Kuiper belt objects.

Discovery of two new satellites of Pluto

Pluto's first known satellite, Charon, was discovered in 1978. It has a diameter (approximately 1,200 km) about half that of Pluto, which makes it larger, relative to its primary, than any other moon in the Solar System. Previous searches for other satellites around Pluto have been unsuccessful, but they were not sensitive to objects less, similar150 km in diameter and there are no fundamental reasons why Pluto should not have more satellites. Here we report the discovery of two additional moons around Pluto, provisionally designated S/2005 P 1 (hereafter P1) and S/2005 P 2 (hereafter P2), which makes Pluto the first Kuiper belt object known to have multiple satellites. These new satellites are much smaller than Charon, with estimates of P1's diameter ranging from 60 km to 165 km, depending on the surface reflectivity; P2 is about 20 per cent smaller than P1. Although definitive orbits cannot be derived, both new satellites appear to be moving in circular orbits in the same orbital plane as Charon, with orbital periods of approximately 38 days (P1) and approximately 25 days (P2).

Titan's Atmospheric Temperatures, Winds, and Composition

Temperatures obtained from early Cassini infrared observations of Titan show a stratopause at an altitude of 310 kilometers (and 186 kelvin at 15 degrees S). Stratospheric temperatures are coldest in the winter northern hemisphere, with zonal winds reaching 160 meters per second. The concentrations of several stratospheric organic compounds are enhanced at mid- and high northern latitudes, and the strong zonal winds may inhibit mixing between these latitudes and the rest of Titan. Above the south pole, temperatures in the stratosphere are 4 to 5 kelvin cooler than at the equator. The stratospheric mole fractions of methane and carbon monoxide are (1.6 +/- 0.5) x 10(-2) and (4.5 +/- 1.5) x 10(-5), respectively.

Engineering inhibitors highly selective for the S1 sites of Ser190 trypsin-like serine protease drug targets

BACKGROUND

Involved or implicated in a wide spectrum of diseases, trypsin-like serine proteases comprise well studied drug targets and anti-targets that can be subdivided into two major classes. In one class there is a serine at position 190 at the S1 site, as in urokinase type plasminogen activator (urokinase or uPA) and factor VIIa, and in the other there is an alanine at 190, as in tissue type plasminogen activator (tPA) and factor Xa. A hydrogen bond unique to Ser190 protease-arylamidine complexes between O gamma(Ser190) and the inhibitor amidine confers an intrinsic preference for such inhibitors toward Ser190 proteases over Ala190 counterparts.

RESULTS

Based on the structural differences between the S1 sites of Ser190 and Ala190 protease-arylamidine complexes, we amplified the selectivity of amidine inhibitors toward uPA and against tPA, by factors as high as 220-fold, by incorporating a halo group ortho to the amidine of a lead inhibitor scaffold. Comparison of K(i) values of such halo-substituted and parent inhibitors toward a panel of Ser190 and Ala190 proteases demonstrates pronounced selectivity of the halo analogs for Ser190 proteases over Ala190 counterparts. Crystal structures of Ser190 proteases, uPA and trypsin, and of an Ala190 counterpart, thrombin, bound by a set of ortho (halo, amidino) aryl inhibitors and of non-halo parents reveal the structural basis of the exquisite selectivity and validate the design principle.

CONCLUSIONS

Remarkable selectivity enhancements of exceptionally small inhibitors are achieved toward the uPA target over the highly similar tPA anti-target through a single atom substitution on an otherwise relatively non-selective scaffold. Overall selectivities for uPA over tPA as high as 980-fold at physiological pH were realized. The increase in selectivity results from the displacement of a single bound water molecule common to the S1 site of both the uPA target and the tPA anti-target because of the ensuing deficit in hydrogen bonding of the arylamidine inhibitor when bound in the Ala190 protease anti-target.

Development of serine protease inhibitors displaying a multicentered short (<2.3 A) hydrogen bond binding mode: inhibitors of urokinase-type plasminogen activator and factor Xa

Novel scaffolds that bind to serine proteases through a unique network of short hydrogen bonds to the catalytic Ser195 have been developed. The resulting potent serine protease inhibitors were designed from lead molecule 2-(2-hydroxyphenyl)1H-benzoimidazole-5-carboxamidine, 6b, which is known to display several modes of binding. For instance, 6b can recruit zinc and bind in a manner similar to that reported by bis(5-amidino-2-benzimidazolyl)methane (BABIM) (Nature 1998, 391, 608-612).(1) Alternatively, 6b can bind in the absence of zinc through a multicentered network of short (<2.3 A) hydrogen bonds. The lead structure was optimized in the zinc-independent binding mode toward a panel of six human serine proteases to yield optimized inhibitors such as 2-(3-bromo-2-hydroxy-5-methylphenyl)-1H-indole-5-carboxamidine, 22a, and 2-(2-hydroxybiphenyl-3-yl)-1H-indole-5-carboxamidine, 22f. Structure-activity relationships determined that, apart from the amidine function, an indole or benzimidazole and an ortho substituted phenol group were also essential components for optimal potency. The affinities (K(i)) of 22a and 22f, for example, bearing these groups ranged from 8 to 600 nM toward a panel of six human serine proteases. High-resolution crystal structures revealed that the binding mode of these molecules in several of the enzymes was identical to that of 6b and involved short (<2.3 A) hydrogen bonds among the inhibitor hydroxyl oxygen, Ser195, and a water molecule trapped in the oxyanion hole. In summation, novel and potent trypsin-like serine protease inhibitors possessing a unique mode of binding have been discovered.

Case study using descriptive analysis to estimate hidden costs in processing third party prescriptions

OBJECTIVE

To identify and quantify additional hidden costs associated with processing third party prescriptions.

DESIGN/SETTING

Using time and motion techniques, the frequency of rejected third party prescriptions and the time involved to resolve those rejections were measured in one supermarket chain pharmacy and one independent pharmacy. From this information, additional costs attributed to processing third party prescriptions were calculated.

RESULTS

In a market where almost 95% of all prescriptions are third party reimbursed, payers rejected 18.7% and 22.3% of the prescriptions submitted by the supermarket chain and independent pharmacies, respectively. Additional or hidden costs for rejected prescriptions averaged $1.10 at the supermarket chain pharmacy and $1.54 at the independent pharmacy, with the difference attributable to the higher level of pharmacy staff involvement in resolving rejections at the independent pharmacy. When additional costs for all third party prescriptions were calculated, the average additional cost per third party prescription dropped to $0.44 for the supermarket chain pharmacy and $0.61 for the independent pharmacy.

CONCLUSION

Increasing pharmacist availability for pharmaceutical care requires decreasing time spent in the dispensing process, especially resolving third party problems. Systems analysis and time and motion techniques were effectively used to more accurately measure the time and costs associated with processing third party prescriptions. Actual costs found in this study were considerable, but significantly less than those reported previously in studies using estimates and surveys.

Discovery of gaseous S2 in Io's Pele plume

Spectroscopy of Io's Pele plume against Jupiter by the Hubble Space Telescope in October 1999 revealed absorption due to S2 gas, with a column density of 1.0 +/- 0.2 x 10(16) per square centimeter, and probably also SO(2) gas with a column density of 7 +/- 3 x 10(16) per square centimeter. This SO2/S2 ratio (3 to 12) is expected from equilibration with silicate magmas near the quartz-fayalite-magnetite or wüstite-magnetite buffers. Condensed S3 and S4, probable coloring agents in Pele's red plume deposits, may form by polymerization of the S2, which is unstable to ultraviolet photolysis. Diffuse red deposits near other Io volcanoes suggest that venting and polymerization of S2 gas is a widespread feature of Io volcanism.

Io's thermal emission from the Galileo photopolarimeter-radiometer

Galileo's photopolarimeter-radiometer instrument mapped Io's thermal emission during the I24, I25, and I27 flybys with a spatial resolution of 2.2 to 300 kilometers. Mapping of Loki in I24 shows uniform temperatures for most of Loki Patera and high temperatures in the southwest corner, probably resulting from an eruption that began 1 month before the observation. Most of Loki Patera was resurfaced before I27. Pele's caldera floor has a low temperature of 160 kelvin, whereas flows at Pillan and Zamama have temperatures of up to 200 kelvin. Global maps of nighttime temperatures provide a means for estimating global heat flow.

Community pharmacy residency programs, 1997-1998

OBJECTIVE

To obtain a descriptive "snapshot" of community pharmacy residency programs active in 1997-1998.

DESIGN

Survey (telephone interview) of community pharmacy residency program directors.

METHODS

An advance letter to residency directors stated the purpose of the study and requested written information on their residency program. Using a scripted questionnaire, telephone interviews were conducted with each residency director.

RESULTS

Descriptive statistics were used to portray the data. There were 13 active community pharmacy residency programs with 20 filled residency sites nationwide at the time of the study. Results revealed that 9 (69%) programs were funded by multiple sources, 3 programs were funded solely by the affiliated college, and 1 program was funded solely by the affiliated pharmacy. Of the 10 residency programs that had been in existence for longer than 1 year, 7 (70%) had the same funding source as they did the first year. Respondents provided descriptions of the residency programs, along with insight into the challenges of creating such programs. At the time of publication (November 1999), there were 50 active community residency sites within the 21 active community pharmacy residency programs. Several other programs are planned for implementation in July 2000.

CONCLUSION

In general, community pharmacy residency programs continue to grow in number, and funding has been sustained due to the programs' successful outcomes. The results of this study provide a framework for the improvement of existing community pharmacy residency programs and the development of additional ones.

Temperatures on europa from galileo photopolarimeter-radiometer: nighttime thermal anomalies

Galileo observations of Europa's thermal emission show low-latitude diurnal brightness temperatures in the range of 86 to 132 kelvin. Nighttime temperatures form an unexpected pattern, with high temperatures on the bright ejecta blanket of the crater Pwyll and an equatorial minimum in temperatures after sunset, uncorrelated with surface albedo or geology. The nighttime anomalies may be due to regional thermal inertia variations of an unknown origin, which are equivalent to a two- to threefold variation in thermal conductivity, or to endogenic heat fluxes locally reaching 1 watt per square meter. Endogenic heat flow at this high level, although consistent with some geological evidence, is theoretically unlikely.

High-temperature silicate volcanism on Jupiter's moon Io

Infrared wavelength observations of Io by the Galileo spacecraft show that at least 12 different vents are erupting lavas that are probably hotter than the highest temperature basaltic eruptions on Earth today. In at least one case, the eruption near Pillan Patera, two independent instruments on Galileo show that the lava temperature must have exceeded 1700 kelvin and may have reached 2000 kelvin. The most likely explanation is that these lavas are ultramafic (magnesium-rich) silicates, and this idea is supported by the tentative identification of magnesium-rich orthopyroxene in lava flows associated with these high-temperature hot spots.

Long vs. short monitoring intervals for peach harvesters exposed to foliar azinphos-methyl residues

A dermal monitoring study of peach harvesters exposed to azinphos-methyl (AM) residues was conducted in Sutter County, California. Harvesters were paid by piecework, which allowed characterization of the relationship between dermal exposure (DE) and time or production. Workers wore 2 long-sleeved knit T-shirts for each monitoring interval and also provided a hand residue sample. Dislodgeable foliar residue (DFR) samples were also collected. The highest correlations were found for inner shirts vs. production and DE vs. time worked (r2 = 0.67, P < 0.01). DE was greatest after 2-h exposures and reached equilibrium after 3 h, indicating that exposure estimates from shorter intervals would overestimate exposure.

Cyclic hexapeptide analogs of somatostatin containing bridge modifications. Syntheses and conformational analyses

The cyclic hexapeptide c[Pro6-Phe7-D-Trp8-Lys9-Thr10-Phe11] displays higher bioactivity than native somatostatin in inhibiting the release of growth hormone. The superscript numbers refer to the location of the residues in native somatostatin. To investigate the structural role played by the Phe11-Pro6 bridging region, we have synthesized a series of cyclic hexapeptide analogs of somatostatin incorporating peptidomimetics and retro-inverso modifications at the bridging region. Among them, two analogs contain the retro-inverso modification mAla6-gPhe11 at the bridging region, and five analogs contain 2-aminocyclopentane carboxylic acid (2-Ac5c) and 1-aminocyclopentane carboxylic acid (1-Ac5c) as proline mimetics. The conformational preferences of these analogs have been studied using 1H-NMR and computer simulations. All of these analogs maintain conformations similar to those of the parent cyclic hexapeptide around the Phe7-D-Trp8-Lys9-Thr10 tetrapeptide region consisting of a beta II' turn. However, they display different conformational features around the bridging region. The R-mAla analog and the five Ac5c analogs show only a trans amide bond for Phe11-Pro6 in the bridging region, while the S-mAla analog displays a cis/trans isomerization for the same amide linkage in the bridging region. The R-mAla and the five Ac5c analogs do not bind to the somatostatin receptor, while the S-mAla analog displays a high binding activity. Applying our recently proposed model for bioactivity of somatostatin analogs, we examined the structure-bioactivity relationships for these somatostatin analogs. This investigation provides valuable insight into the structural role played by the bridging region.

Histological and bacteriological findings in long-term ileocystoplasty and colocystoplasty in the rat

The long-term effects of bladder reconstruction using bowel were studied in rats. Bladder surgery consisted of cystotomy and closure, ileo- or colocystoplasty, or placement of a reverse serosal (Thal) patch of ileum. At least one-third of all groups received prophylactic cefaclor, postoperatively. Monthly urine cultures were obtained, and survivors were sacrificed at 1 year. Antimicrobial therapy markedly reduced the incidence of chronic colonization after cystoplasty. However, the majority of rats in the Thal patch group remained colonized because of acquired vesicoileal fistulae. Vesical stones were often present in this group and were also seen in 6 of 43 (14%) and 3 of 33 (9%) in the ileocystoplasty and colocystoplasty groups, respectively. Transitional cell papillomas and/or hyperplasia was seen at 20 of 42 (48%) uroileal and 20 of 31 (64%) urocolonic anastomoses (p = .15). Hyperplastic lesions could not be correlated with bacteriuria. Focal nonpapillary transitional cell carcinoma was seen once in the colocystoplasty group, and low grade papillary transitional cell tumors were noted once in each of the cystostomy and ileocystoplasty groups and twice in Thal patch rats with ileovesical fistulae. These findings suggest that the rat uroenteric anastomosis is susceptible to proliferative change which is rarely malignant in nature and occurs in the presence or absence of bacteriuria.

Patch graft urethroplasty using dye enhanced laser tissue welding with a human protein solder: a preclinical canine model

We investigated the use of the KTP-532 laser to perform a patch graft urethroplasty in 24 adult male dogs using the inner preputial skin as the donor site. In group 1 (12 dogs) repairs were completed with conventional microsuturing techniques, while in group 2 (12 dogs) they were completed using the KTP-532 laser. In the laser welding group the addition of a protein solder (40% human albumin) doped with fluorescein was used. Assessment parameters included a preoperative and postoperative retrograde urethrogram, measurement of intraluminal bursting pressure in the first 6 animals in each group, operative time and histology. Operative time was 42% faster and acute intraluminal bursting pressures were significantly higher in the laser-solder group. No fistulas occurred in the laser-solder group compared to a 50% fistula rate in the suture group. Significant radiographic abnormalities were seen in the urethras of the suture repair group.

Metastatic renal tumor presenting as ovarian clear cell carcinoma

Patients with clear cell adenocarcinoma of the kidney often present with metastatic disease, in some cases involving organs in which primary clear cell tumors occur. Under these circumstances, diagnosis of the renal primary tumor may be delayed. Herein we present a case of renal cell carcinoma metastatic to the ovaries initially treated as primary ovarian disease, until the appearance of other metastases prompted the discovery of its true origin. A high index of suspicion and the histologic characteristics of these tumors may allow earlier diagnosis and treatment of a renal primary tumor.

Studies of the hormonal control of postnatal testicular descent in the rat

Dihydrotestosterone is believed to control the transinguinal phase of testicular descent based on hormonal manipulation studies performed in postnatal rats. In the present study, these hormonal manipulation experiments were repeated, and the results were compared with those obtained using the antiandrogens flutamide and cyproterone acetate. 17 beta-estradiol completely blocked testicular descent, but testosterone and dihydrotestosterone were equally effective in reversing this inhibition. Neither flutamide nor cyproterone acetate prevented testicular descent in postnatal rats despite marked peripheral antiandrogenic action. Further analysis of the data revealed a correlation between testicular size and descent. Androgen receptor blockade did not produce a marked reduction in testicular size and consequently did not prevent testicular descent, whereas estradiol alone caused marked testicular atrophy and testicular maldescent. Reduction of the estradiol dosage or concomitant administration of androgens or human chorionic gonadotropin resulted in both increased testicular size and degree of descent. These data suggest that growth of the neonatal rat testis may contribute to its passage into the scrotum.

Topochemical design of bioactive peptides and peptidomimetics

For the studies of bioactive peptides, our laboratories have been employed an integrated approach including synthesis, bioassays, and conformational analysis. To obtain highly potent, selective and metabolically stable analogs, peptidomimetics such as peptide backbone modifications (retro-inverso structures), constrained amino acids, and cyclic structures have been incorporated into many bioactive peptide sequences. The conformational studies of the resulting analogs have led to topochemical models for the bioactivities of those peptides. This lecture will be focused on the results of such studies on opioids and somatostatin. We have synthesized numerous opioid analogs with various peptidomimetics based on three classes: enkephalins, dermorphin-deltorphins, and morphiceptins. Many of these analogs exhibit high potency, selectivity, and metabolic stability. Conformational studies of these analogs have enabled us to define the structural characteristics necessary for bioactivities of morphiceptins, dermorphins, enkephalins, and deltorphins. From these results, we can propose conformational models responsible for bioactivities at the mu- and delta-receptors. Our studies of cyclic somatostatin analogs are based on the highly active Merck analog c(-Pro6-Phe7-D-Trp8-Lys9-Thr10-Phe11-) (where the superscripts denote position in native somatostatin). To investigate the topochemical preference of backbone and side chains, unusual amino acids, including beta-methylphenylalanine7 or 11, beta-methyltryptophan8, as well as backbone modifications such as retro-inverso structures have been incorporated. The bioactivity profiles of these peptidomimetic molecules provide much information on the effects of backbone and side chain constraints on bioactivity.

Comparative study of methods to couple hindered peptides

A comparative study of modern coupling reactions involving Boc-protected amino acid derivatives and dipeptides with N-terminal alpha,alpha-dialkylation and N-methylation was carried out. The coupling reactions were run using either equimolar amounts of the amino and activated carboxyl components or an excess of the activated carboxyl component. Yields of the target tripeptide Boc-Phe-Xaa-Phe-OBzl (Xaa = (NMe)Ala, (NMe)Aib, or (NMe) alpha Ac5c) were compared. Less than 10% of the product was obtained from methods utilizing pivaloyl mixed anhydride, pentafluorophenyl ester or acyl fluoride activation when Xaa = (NMe)Aib and (NMe) alpha Ac5c. At room temperature, significant yields of these two products were obtained from reactions which utilized an excess of the HBTU reagent (O-benzotriazol-1-yl-N,N,N',N'-tetramethyluronium hexafluorophosphate), the PyBroP reagent (bromo-tris-pyrrolidino-phosphonium hexafluorophosphate) or Boc-Phe-NCA (Boc-protected phenylalanine N-carboxyanhydride). Moreover, the Boc-Phe-NCA method was superior when used over a prolonged reaction time or at elevated temperature.

Comparison of the effects of the 5 alpha-reductase inhibitor finasteride and the antiandrogen flutamide on prostate and genital differentiation: dose-response studies

Studies were performed to compare the effects of 5 alpha-reductase inhibition and antiandrogen receptor blockade on differentiation of male internal and external genital structures and prostate in the rat. Dose-response studies were performed on male rats treated in utero during the period of sexual differentiation with either the potent 5 alpha-reductase inhibitor finasteride or the antiandrogen flutamide. The treated animals were raised to adulthood and killed, and genital structures were evaluated. Treatment with the 5 alpha-reductase inhibitor finasteride at a dose of 25 mg/kg.day resulted in significant feminization of the external genitalia. There was no further feminization of the genitalia at doses up to 300 mg/kg.day. Wolffian ductal differentiation occurred at all doses evaluated. Seminal vesicle weight, however, significantly decreased at 25 mg/kg.day, but without a further decrease at higher doses of the 5 alpha-reductase inhibitor. Vas deferens and epididymal weights were unchanged at all doses evaluated. There was a significant decrease in prostate size at 25 and 50 mg/kg.day, with no further decrease at higher doses. In flutamide-treated animals, complete feminization of the genitalia occurred at 24 mg/kg.day in all animals. At 18 mg/kg.day, Wolffian ductal differentiation occurred, but seminal vesicle weight was decreased. At dosages of 100, 200, and 300 mg/kg.day flutamide, the vas deferens was absent unilaterally or bilaterally, with small remnants of epididymal head and tail present. At dosages of 24 mg/kg.day and above, the prostate was absent. Studies with the 5 alpha-reductase inhibitor finasteride demonstrate the dependency of prostate and male external genital differentiation on dihydrotestosterone (DHT). However, unlike androgen receptor blockade with flutamide, finasteride did not totally abolish prostate differentiation or completely feminize the external genitalia, despite increasingly higher doses. Since there is no evidence of multiple 5 alpha-reductase isoenzymes to date in the rat, these results suggest that testosterone (T) can compensate for DHT to some degree at the level of the androgen receptor. Wolffian differentiation, however, was not affected by inhibition of DHT, demonstrating its T dependency, but seminal vesicle growth was impaired. Thus, inhibition of 5 alpha-reductase activity limits seminal growth potential in adulthood. Studies with the antiandrogen flutamide show that at doses significantly above that required to completely block prostate differentiation and cause genital feminization, Wolffian ductal differentiation is significantly impaired. Thus, higher doses of flutamide are needed to block the paracrine effect of T on the Wolffian ducts.

Quantitation of urinary Tamm-Horsfall protein in children with urinary tract infection

It has been suggested that urinary Tamm-Horsfall protein (THP) prevents colonization of the urinary tract by binding uropathogens. We tested the hypothesis that low urinary THP levels may predispose to urinary tract infection (UTI) by measuring THP levels in children. We studied a cohort of 35 girls with uncomplicated recurrent UTI (group 1) that was compared with 27 patients with myelomeningoceles undergoing clean intermittent catheterization (group 2) and 16 female controls (group 3). We measured urinary THP in both aggregated (aTHP) and disaggregated form (dTHP), leukocyte esterase activity, urine chemistries and culture. No significant differences in dTHP or aTHP levels were seen between groups 1 and 3, but group-1 patients had higher dTHP levels than group-2 patients (p < 0.008). History of reflux or the presence of bacteriuria or pyuria at the time of urine collection did not affect dTHP levels; in contrast, pyuria or bacteriuria at the time of sampling was associated with markedly lower aTHP levels when compared with sterile samples (p < 0.0001). For all groups, measured quantities of dTHP did not correlate with aTHP levels. We conclude that excretion of dTHP in children with history of recurrent UTI is not reduced. In contrast, concentrations of aTHP are profoundly depressed in children during times of UTI, suggesting a role for THP in the pathogenesis of UTI. Assaying THP in its aggregated form may prove valuable when studying its physiologic function and merits further investigation.