Out of the frying pan into the fire: Predicted warming in alpine streams suggests hidden consequences for aquatic ectotherms.

Thermal regimes of aquatic ecosystems are predicted to change as climate warming progresses over the next century, with high-latitude and high-elevation regions predicted to be particularly impacted. Here, we have modelled alpine stream water temperatures from air temperature data and used future predicted air temperature trajectories (representative concentration pathway [rcp] 4.5 and 8.5) to predict future water temperatures. Modelled stream water temperatures have been used to calculate cumulative degree days (CDDs) under current and future climate conditions. These calculations show that degree days will accumulate more rapidly under the future climate scenarios, and with a stronger effect for higher CDD values (e.g., rcp 4.5: 18-28 days earlier [CDD = 500]; 42-55 days earlier [CDD = 2000]). Changes to the time to achieve specific CDDs may have profound and unexpected consequences for alpine ecosystems. Our calculations show that while the effect of increased CDDs may be relatively small for organisms that emerge in spring-summer, the effects for organisms emerging in late summer-autumn may be substantial. For these organisms, the air temperatures experienced upon emergence could reach 9°C (rcp 4.5) or 12°C (rcp 8.5) higher than under current climate conditions, likely impacting on the metabolism of adults, the availability of resources, including food and suitable oviposition habitat, and reproductive success. Given that the movement of aquatic fauna to the terrestrial environment represents an important flux of energy and nutrients, differential changes in the time periods to achieve CDDs for aquatic and terrestrial fauna may de-couple existing predator-prey interactions.

Morphological analysis of chiral rod clusters from a coarse-grained single-site chiral potential.

We present a coarse-grained single-site potential for simulating chiral interactions, with adjustable strength, handedness, and preferred twist angle. As an application, we perform basin-hopping global optimisation to predict the favoured geometries for clusters of chiral rods. The morphology phase diagram based upon these predictions has four distinct families, including previously reported structures for potentials that introduce chirality based on shape, such as membranes and helices. The transition between these two configurations reproduces some key features of experimental results for fd bacteriophage. The potential is computationally inexpensive, intuitive, and versatile; we expect it will be useful for large scale simulations of chiral molecules. For chiral particles confined in a cylindrical container we reproduce the behaviour observed for fusilli pasta in a jar. Hence this chiropole potential has the capability to provide insight into structures on both macroscopic and molecular length scales.

Dynamical properties of two- and three-dimensional colloidal clusters of six particles.

Colloidal clusters are important systems for studying self-assembly. Clusters of six colloidal particles attracting each other via short-ranged interactions have been recently studied both theoretically and experimentally. Here we present a computer modelling study of the thermodynamics and dynamics of these clusters using a short-ranged Morse potential in two and three dimensions. We combine energy landscape methods with comprehensive sampling, both of configurations using Markov chain Monte Carlo and also of trajectories using Langevin molecular dynamics propagation. We show that the interaction energies between the particles are probably greater than previously assumed. The rates predicted by transition state theory using harmonic vibrational densities of states are off by four orders of magnitude, since the effects of viscosity are not accounted for. In contrast, sampling short trajectories using an appropriate friction constant and discrete relaxation path sampling produces reasonable agreement with the experimental rates.

Oxygen, Silicon, and Aluminum in Lunar Samples by 14 MeV Neutron Activation.

Abundances of oxygen, silicon, and altiminutm in 27 lunar rocks and C aliquants of lunar soil have been determined by 14 MeV neutron activation. Mean abundances and standard deviations of individual abundances (in weight percent) within each type are: type A (2 rocks), 38.5 +/- 1.2 oxygen, 18.9 +/- 0.8 silicon, and 4.0 +/- 0.4 aluminum; type B (7 rocks), 39.4 +/- 1.0 oxygen, 18.7 +/- 0.8 silicon, and 5.0 +/- 0.6 aluminum; type C (18 rocks), 41.1 +/- 1.0 oxygen, 19.7 +/- 0.7 silicon, and 6.6 +/- 0.5 aluminum; soil (3 aliquants), 40.8 +/- 1.2 oxygen, 20.2 +/- 0.2 silicon, and 7.2 +/- 0.1 aluminum. Oxygen abundances are lower than those in most common terrestrial rocks and are comparable to those found in certain types of stony meteorites. From these results the lunar soil is most similar to the type C lunar rocks.

Rhenium-osmium isotope systematics of carbonaceous chondrites.

Rhenium and osmium concentrations and Os isotopic compositions of eight carbonaceous chondrites, one LL3 ordinary chondrite, and two iron meteorites were determined by resonance ionization mass spectrometry. Iron meteorite (187)Re/(186)Os and (l87)Os/(l86)Os ratios plot on the previously determined iron meteorite isochron, but most chondrite data plot 1 to 2 percent above this meteorite isochron. This suggests either that irons have significantly younger Re-Os closure ages than chondrites or that chondrites were formed from precursor materials with different chemical histories from the precursors of irons. Some samples of Semarkona (LL3) and Murray (C2M) meteorites plot 4 to 6 percent above the iron meteorite isochron, well above the field delineated by other chondrites. Murray may have lost Re by aqueous leaching during its preterrestrial history. Semarkona could have experienced a similar loss of Re, but only slight aqueous alteration is evident in the meteorite. Therefore, the isotopic composition of Semarkona could reflect assembly of isotopically heterogeneous components subsequent to 4.55 billion years ago or Os isotopic heterogeneities in the primordial solar nebula.

Moon: possible nature of the body that produced the imbrian basin, from the composition of apollo 14 samples.

Soils from the Apollo 14 site contain nearly three times as much meteoritic material as soils from the Apollo 11, Apollo 12, and Luna 16 sites. Part of this material consists of the ubiquitous micrometeorite component, of primitive (carbonaceous-chondrite-like) composition. The remainder, seen most conspicuously in coarse glass and norite fragments, has a decidedly fractionated composition, with volatile elements less than one-tenth as abundant as siderophiles. This material seems to be debris of the Cyprus-sized planetesimal that produced the Imbrian basin. Compositionally this planetesimal has no exact counterpart among known meteorite classes, though group IVA irons come close. It also resembles the initial composition of the earth as postulated by the two-component model. Apparently the Imbrian planetesimal was an Earth satellite swept up by the moon during tidal recession or capture, or an asteroid deflected by Mars into terrestrial space.

Volatile elements in apollo 16 samples: possible evidence for outgassing of the moon.

Several Apollo 16 breccias, including one containing goethite, are strikingly enriched in volatile elements such as bromine, cadmium, germanium, antimony, thallium, and zinc. Similar but smaller enrichments are found in all highland soils. It appears that volcanic processes took place in the lunar highlands, involving the release of volatiles including water. The lunar thallium/uranium ratio is 2 x 10-(4) of the cosmic ratio, which suggests that the moon's original water content could not have exceeded the equivalent of a layer 22 meters deep. The cataclastic anorthosites at the Apollo 16 site may represent deep ejecta from the Nectaris basin.

Osmium-187 enrichment in some plumes: evidence for core-mantle interaction?

Calculations with data for asteroidal cores indicate that Earth's outer core may have a rhenium/osmium ratio at least 20 percent greater than that of the chondritic upper mantle, potentially leading to an outer core with an osmium-187/osmium-188 ratio at least 8 percent greater than that of chondrites. Because of the much greater abundance of osmium in the outer core relative to the mantle, even a small addition of metal to a plume ascending from the D" layer would transfer the enriched isotopic signature to the mixture. Sources of certain plume-derived systems seem to have osmium-187/osmium-l88 ratios 5 to 20 percent greater than that for chondrites, consistent with the ascent of a plume from the core-mantle boundary.

Glazed lunar rocks: origin by impact.

The glassy coating of lunar rock 12017 is enriched in 15 trace elements relative to the crystalline interior. It apparently consists chiefly of shock-melted rock, somewhat richer in rare earth elements and alkali metals than rock 12017 itself. The glass has been contaminated by about 0.5 percent carbonaceous-chondrite-like material or, alternatively, by a mixture of 0.06 to 0.3 percent fractionated meteoritic material and approximately 10 to 15 percent local soil. The glazing seems to represent molten material splashed from a nearby meteorite impact and not in situ melting by a sudden increase in solar luminosity.

Rhenium-osmium isotope constraints on the age of iron meteorites.

Rhenium and osmium concentrations and the osmium isotopic compositions of iron meteorites were determined by negative thermal ionization mass spectrometry. Data for the IIA iron meteorites define an isochron with an uncertainty of approximately +/-31 million years for meteorites approximately 4500 million years old. Although an absolute rheniumosmium closure age for this iron group cannot be as precisely constrained because of uncertainty in the decay constant of (187)Re, an age of 4460 million years ago is the minimum permitted by combined uncertainties. These age constraints imply that the parent body of the IIAB magmatic irons melted and subsequently cooled within 100 million years after the formation of the oldest portions of chondrites. Other iron meteorites plot above the IIA isocbron, indicating that the planetary bodies represented by these iron groups may have cooled significantly later than the parent body of the IIA irons.

Rhenium-osmium and samarium-neodymium isotopic systematics of the stillwater complex.

Isotopic data for the Stillwater Complex, Montana, which formed about 2700 Ma (million years ago), were obtained to evaluate the role of magma mixing in the formation of strategic platinum-group element (PGE) ore deposits. Neodymium and osmium isotopic data indicate that the intrusion formed from at least two geochemically distinct magmas. Ultramafic affinity (U-type) magmas had initial epsilon(Nd) of -0.8 to -3.2 and a chondritic initial (187)Os/(186)Os ratio of approximately 0.88, whereas anorthositic affinity (A-type) magmas had epsilon(Nd) of -0.7 to +1.7 and an initial (187)Os/(186)Os ratio of approximately -1.13. These data suggest that U-type magmas were derived from a lithospheric mantle source containing recycled crustal materials whereas A-type magmas originated either by crustal contamination of basaltic magmas or by partial melting of basalt in the lower crust. The Nd and Os isotopic data also suggest that Os, and probably the other PGEs in ore horizons such as the J-M Reef, was derived from A-type magmas. The Nd and Os isotopic heterogeneity observed in rocks below the J-M Reef also suggests that A-type magmas were injected into the Stillwater U-type magma chamber at several stages during the development of the Ultramafic series.

Vitamin D-mediated gene regulation in phenotypically defined human B cell subpopulations.

Isolation of distinct subpopulations of density-fractionated normal human B lymphocytes reveals that the requirements for up-regulation of the vitamin D receptor (VDR) and initiation of 1alpha,25-dihydroxyvitamin D3 [1alpha,25-(OH)2D3]-mediated genomic trans-activation are dependent upon the state of cellular activation. The kinetics of the response differ widely among these B cell subpopulations. However, these density-fractionated B cell subpopulations are phenotypically diverse and therefore are not representative of distinct stages of B cell maturation and differentiation. To examine the role of B cell differentiation on the induction and maintenance of biological receptivity to 1,25-(OH)2D3, we purified naive, germinal center, and memory B cells based on their expression of CD38 and CD44 surface antigens and surface Ig isotype. These phenotypically defined B cell subpopulations were all found to constitutively express VDR, and all exhibited similar activation requirements and kinetics for initiation of 1,25(OH)2D3-mediated genomic trans-activation. Taken together, these results suggest that defined stages of differentiation in normal B cells are not significant predicators of VDR expression or receptivity to 1,25-(OH)2D3. Rather, the degree of cellular activation, regardless of maturation stage, determines whether the effects of this immunoregulatory hormone will influence a mature B lymphocyte.

Differential regulation of gene transcription in subpopulations of human B lymphocytes by vitamin D3.

We have previously shown that freshly extirpated normal human tonsil B cells, which are phenotypically diverse, representing different stages of cellular activation and differentiation, are refractory to the effects of 1,25-dihydroxyvitamin D3 [1,25-(OH)2D3] and require specific activation signals for induction of responsiveness. To determine whether these diversely activated B cell populations respond to 1,25-(OH)2D3, human tonsil B cells were density fractionated and evaluated biochemically and functionally. Low density tonsil B cells, representing the centroblastic fraction, were observed to constitutively express vitamin D receptor message and protein. In contrast, high density quiescent tonsillar B cells had no detectable vitamin D receptor message or protein and required stimulation in vitro for their up-regulation. Biological responsiveness to 1,25-(OH)2D3 was assessed by messenger RNA (mRNA) expression of the vitamin D-dependent enzyme, 25-hydroxyvitamin D3 24-hydroxylase. Low density centroblastic B cells did not require exogenous surface activation for expression of 24-hydroxylase mRNA, which was detectable after 6 h of culture in the presence of 1,25-(OH)2D3. In contrast, high density tonsil B cells required in vitro activation for induction of 24-hydroxylase mRNA, and expression was not detectable for up to 48 h of culture. These observations suggest that reactivity of normal B cell populations to vitamin D is dependent upon their specific stage of activation.

Severity of illness classification for infection control departments: a study in nosocomial pneumonia.

BACKGROUND: A subjective severity of illness classification was evaluated in a study of nosocomial pneumonia. This is a 5-category system based on the determination of the control of underlying illness and the risk of death during current hospital admission. METHODS: A case-control study was performed with 128 cases of nosocomial pneumonia and 252 control patients. An additional 60 case and 90 control patients were used to compare this classification with APACHE II scoring in intensive care unit patients. RESULTS: In univariate analysis, the severity illness classification was significantly associated with nosocomial pneumonia risk (p < 0.01). APACHE II adequately predicted mortality rate but was not statistically significantly associated with nosocomial pneumonia risk among intensive care unit patients. In logistic regression analysis, the severity of illness classification, surgery, age, nasogastric tube placement, and histamine blockers each showed significant independent association with nosocomial pneumonia. CONCLUSIONS: The role of the severity of illness classification for risk stratification in nosocomial pneumonia is valid. Its roles in the evaluation of surgical wound infection, nosocomial bacteremia, and quality of care remain to be determined in subsequent studies.

Distribution of skeletal metastases in prostatic and lung cancer. Mechanisms of skeletal metastases.

The distribution of skeletal metastases in prostatic and lung cancer was examined to test the hypothesis that prostatic carcinoma spreads by a unique hematogenous route. Abnormal technetium-99m methylene diphosphonate bone scans were retrospectively reviewed in 71 patients with prostatic carcinoma and 41 patients with lung cancer comparing patterns of osseous involvement. Differences in the distribution of lesions were not significant. It is concluded that prostatic carcinoma does not metastasize to specific skeletal sites by a singular hematogenous pathway.

Uranium and thorium abundances in chondritic meteorites.

Neutron-activation analyses for uranium and thorium are reported for 42 chondrite meteorite "falls" and 1 "find" covering 15 of the 20 Van Schmus-Wood chondrite types. The mean uranium and thorium abundances of the 5 chemical groups show a trend with C group (U = 0.012(0) atoms/10(6) Si atoms, Th = 0.045(4) atoms/10(6) Si atoms, Th U = 3.7(8)) > H, L and LL groups (U = 0.008(3), Th = 0.028(0), Th U = 3.4(5)) > E group (U = 0.005(9), Th = 0.021(8), Th U = 3.6(9)). With the possible exception of the C3 chondrites, the mean abundances for each petrologic type within a given chemical group are identical.

Methods for the separation of rhenium, osmium and molybdenum applicable to isotope geochemistry.

Effective methods are described for the chemical separation of rhenium, osmium and molybdenum. The methods are based on distillation and anion-exchange chromatography, and have been the basis for rhenium-osmium isotope studies of ore deposits and meteorites. Successful anion-exchange separation of osmium requires both recognition and careful control of the osmium species in solution; thus, distillation of osmium tetroxide from a mixture of sulfuric acid and hydrogen peroxide is preferred to anion-exchange. Distribution coefficients measured for perrhenate in sulfuric acid media are sufficiently high (K(d) > 500) for rhenium to be directly loaded onto an ion-exchange column from a distillation residue and subsequently eluted with nitric acid. Polymerization of molybdenum species during elution is prevented by use of a solution that is 1M in hydrochloric acid and 1M in sodium chloride.