COVID, Vulnerability, and the Death of Solidarity: "Who Do We Not Save?"

Solidarity between more and less vulnerable groups is fundamental to an effective public health response to a global pandemic. Yet in the case of COVID-19, a focus on deciding who can and who cannot be protected from harm has shaped the pandemic experience and continues to determine the post-pandemic trajectory of life with SARS-CoV-2. In this paper I discuss how this has affected our understanding and acceptance of solidarity.

The Radiation Environment of Ceres and Implications for Surface Sampling.

Ceres is a large water-rich dwarf planet located within the asteroid belt. Its surface displays evidence of material sourced from a deep subsurface liquid brine layer within recent geologic time, making it a candidate ocean world with possible present-day activity. However, Ceres lacks a substantial atmosphere and likely does not possess a global magnetic field. Therefore, any material emplaced or exposed on the surface will be subject to weathering by charged particles of solar and galactic origin. We have evaluated the effect of charged particle radiation on material within the near-surface of Ceres and find that the timescale for radiation-induced modification and destruction of organics and endogenic material is ∼100 Myr to 1 Gyr within the top 10-20 cm of the surface. Furthermore, we find that the timescale for sterilization of any putative living organisms contained within material at these depths is <500 kyr. Future missions to the surface may therefore consider targeting regions with geologic ages that fall between these two timescales to avoid the risk of backward contamination while ensuring that sampled material is not heavily radiation processed.

The varied sources of faculae-forming brines in Ceres' Occator crater emplaced via hydrothermal brine effusion.

Before acquiring highest-resolution data of Ceres, questions remained about the emplacement mechanism and source of Occator crater's bright faculae. Here we report that brine effusion emplaced the faculae in a brine-limited, impact-induced hydrothermal system. Impact-derived fracturing enabled brines to reach the surface. The central faculae, Cerealia and Pasola Facula, postdate the central pit, and were primarily sourced from an impact-induced melt chamber, with some contribution from a deeper, pre-existing brine reservoir. Vinalia Faculae, in the crater floor, were sourced from the laterally extensive deep reservoir only. Vinalia Faculae are comparatively thinner and display greater ballistic emplacement than the central faculae because the deep reservoir brines took a longer path to the surface and contained more gas than the shallower impact-induced melt chamber brines. Impact-derived fractures providing conduits, and mixing of impact-induced melt with deeper endogenic brines, could also allow oceanic material to reach the surfaces of other large icy bodies.

Impact heat driven volatile redistribution at Occator crater on Ceres as a comparative planetary process.

Hydrothermal processes in impact environments on water-rich bodies such as Mars and Earth are relevant to the origins of life. Dawn mapping of dwarf planet (1) Ceres has identified similar deposits within Occator crater. Here we show using Dawn high-resolution stereo imaging and topography that Ceres' unique composition has resulted in widespread mantling by solidified water- and salt-rich mud-like impact melts with scattered endogenic pits, troughs, and bright mounds indicative of outgassing of volatiles and periglacial-style activity during solidification. These features are distinct from and less extensive than on Mars, indicating that Occator melts may be less gas-rich or volatiles partially inhibited from reaching the surface. Bright salts at Vinalia Faculae form thin surficial precipitates sourced from hydrothermal brine effusion at many individual sites, coalescing in several larger centers, but their ages are statistically indistinguishable from floor materials, allowing for but not requiring migration of brines from deep crustal source(s).

Advanced chemical stability diagrams to predict the formation of complex zinc compounds in a chloride environment.

A chemical stability map is advanced by incorporating ion complexation, solubility, and chemical trajectories to predict ZnO, Zn(OH)2, ZnCO3, ZnCl2, Zn5(CO3)2(OH)6, and Zn5(OH)8Cl2·H2O precipitation as a function of the total Zn content and pH of an NaCl solution. These calculations demonstrate equilibrium stability of solid Zn products often not considered while tracking the consumed and produced aqueous Zn ion species concentrations through chemical trajectories. The effect of Cl-based ligand formation is incorporated into these stability predictions, enabling enhanced appreciation for the local corrosion conditions experienced at the Zn surface in chloride-containing environments. Additionally, the complexation of Cl- with Zn2+ is demonstrated to compete with the formation of solid phases, making precipitation more difficult. The present work also extends the chemical stability diagram derivations by incorporating a Gibbs-Thompson curvature relation to predict the effect of nanoscale precipitate phase formation on species solubility. These thermodynamic predictions correlate well with experimental results for Zn corrosion in full and alternate NaCl immersion, and have far-reaching utility in a variety of fields requiring nanoscale, semiconductor, and/or structural materials.

Landslides on Ceres: Diversity and Geologic Context.

Landslides are among the most widespread geologic features on Ceres. Using data from Dawn's Framing Camera, landslides were previously classified based upon geomorphologic characteristics into one of three archetypal categories, Type 1(T1), Type 2 (T2), and Type 3 (T3). Due to their geologic context, variation in age, and physical characteristics, most landslides on Ceres are, however, intermediate in their morphology and physical properties between the archetypes of each landslide class. Here we describe the varied morphology of individual intermediate landslides, identify geologic controls that contribute to this variation, and provide first-order quantification of the physical properties of the continuum of Ceres's surface flows. These intermediate flows appear in varied settings and show a range of characteristics, including those found at contacts between craters, those having multiple trunks or lobes; showing characteristics of both T2 and T3 landslides; material slumping on crater rims; very small, ejecta-like flows; and those appearing inside of catenae. We suggest that while their morphologies can vary, the distribution and mechanical properties of intermediate landslides do not differ significantly from that of archetypal landslides, confirming a link between landslides and subsurface ice. We also find that most intermediate landslides are similar to Type 2 landslides and formed by shallow failure. Clusters of these features suggest ice enhancement near Juling, Kupalo and Urvara craters. Since the majority of Ceres's landslides fall in the intermediate landslide category, placing their attributes in context contributes to a better understanding of Ceres's shallow subsurface and the nature of ground ice.

Primary Ciliary Dyskinesia Due to Microtubular Defects is Associated with Worse Lung Clearance Index.

PURPOSE: Primary ciliary dyskinesia (PCD) is characterised by repeated upper and lower respiratory tract infections, neutrophilic airway inflammation and obstructive airway disease. Different ultrastructural ciliary defects may affect lung function decline to different degrees. Lung clearance index (LCI) is a marker of ventilation inhomogeneity that is raised in some but not all patients with PCD. We hypothesised that PCD patients with microtubular defects would have worse (higher) LCI than other PCD patients. METHODS: Spirometry and LCI were measured in 69 stable patients with PCD. Age at testing, age at diagnosis, ethnicity, ciliary ultrastructure, genetic screening result and any growth of Pseudomonas aeruginosa was recorded. RESULTS: Lung clearance index was more abnormal in PCD patients with microtubular defects (median 10.24) than those with dynein arm defects (median 8.3, p = 0.004) or normal ultrastructure (median 7.63, p = 0.0004). Age is correlated with LCI, with older patients having worse LCI values (p = 0.03, r = 0.3). CONCLUSION: This study shows that cilia microtubular defects are associated with worse LCI in PCD than dynein arm defects or normal ultrastructure. The patient's age at testing is also associated with a higher LCI. Patients at greater risk of obstructive lung disease should be considered for more aggressive management. Differences between patient groups may potentially open avenues for novel treatments.

The geomorphology of Ceres.

Analysis of Dawn spacecraft Framing Camera image data allows evaluation of the topography and geomorphology of features on the surface of Ceres. The dwarf planet is dominated by numerous craters, but other features are also common. Linear structures include both those associated with impact craters and those that do not appear to have any correlation to an impact event. Abundant lobate flows are identified, and numerous domical features are found at a range of scales. Features suggestive of near-surface ice, cryomagmatism, and cryovolcanism have been identified. Although spectroscopic analysis has currently detected surface water ice at only one location on Ceres, the identification of these potentially ice-related features suggests that there may be at least some ice in localized regions in the crust.

The missing large impact craters on Ceres.

Asteroids provide fundamental clues to the formation and evolution of planetesimals. Collisional models based on the depletion of the primordial main belt of asteroids predict 10-15 craters >400 km should have formed on Ceres, the largest object between Mars and Jupiter, over the last 4.55 Gyr. Likewise, an extrapolation from the asteroid Vesta would require at least 6-7 such basins. However, Ceres' surface appears devoid of impact craters >∼280 km. Here, we show a significant depletion of cerean craters down to 100-150 km in diameter. The overall scarcity of recognizable large craters is incompatible with collisional models, even in the case of a late implantation of Ceres in the main belt, a possibility raised by the presence of ammoniated phyllosilicates. Our results indicate that a significant population of large craters has been obliterated, implying that long-wavelength topography viscously relaxed or that Ceres experienced protracted widespread resurfacing.

Controlling the corrosion and cathodic activation of magnesium via microalloying additions of Ge.

The evolution of corrosion morphology and kinetics for magnesium (Mg) have been demonstrated to be influenced by cathodic activation, which implies that the rate of the cathodic partial reaction is enhanced as a result of anodic dissolution. This phenomenon was recently demonstrated to be moderated by the use of arsenic (As) alloying as a poison for the cathodic reaction, leading to significantly improved corrosion resistance. The pursuit of alternatives to toxic As is important as a means to imparting a technologically safe and effective corrosion control method for Mg (and its alloys). In this work, Mg was microalloyed with germanium (Ge), with the aim of improving corrosion resistance by retarding cathodic activation. Based on a combined analysis herein, we report that Ge is potent in supressing the cathodic hydrogen evolution reaction (reduction of water) upon Mg, improving corrosion resistance. With the addition of Ge, cathodic activation of Mg subject to cyclic polarisation was also hindered, with beneficial implications for future Mg electrodes.

Pitted terrain on Vesta and implications for the presence of volatiles.

We investigated the origin of unusual pitted terrain on asteroid Vesta, revealed in images from the Dawn spacecraft. Pitted terrain is characterized by irregular rimless depressions found in and around several impact craters, with a distinct morphology not observed on other airless bodies. Similar terrain is associated with numerous martian craters, where pits are thought to form through degassing of volatile-bearing material heated by the impact. Pitted terrain on Vesta may have formed in a similar manner, which indicates that portions of the surface contain a relatively large volatile component. Exogenic materials, such as water-rich carbonaceous chondrites, may be the source of volatiles, suggesting that impactor materials are preserved locally in relatively high abundance on Vesta and that impactor composition has played an important role in shaping the asteroid's geology.

Dawn at Vesta: testing the protoplanetary paradigm.

The Dawn spacecraft targeted 4 Vesta, believed to be a remnant intact protoplanet from the earliest epoch of solar system formation, based on analyses of howardite-eucrite-diogenite (HED) meteorites that indicate a differentiated parent body. Dawn observations reveal a giant basin at Vesta's south pole, whose excavation was sufficient to produce Vesta-family asteroids (Vestoids) and HED meteorites. The spatially resolved mineralogy of the surface reflects the composition of the HED meteorites, confirming the formation of Vesta's crust by melting of a chondritic parent body. Vesta's mass, volume, and gravitational field are consistent with a core having an average radius of 107 to 113 kilometers, indicating sufficient internal melting to segregate iron. Dawn's results confirm predictions that Vesta differentiated and support its identification as the parent body of the HEDs.

On-demand release of corrosion-inhibiting ions from amorphous Al-Co-Ce alloys.

Controlled release technologies are often used to supply chemicals or drugs at given rates. Release often occurs on contact with solution. However, some applications, such as corrosion protection, require containment of the active species in a reservoir and their slow release when needed. Conductive polymers have been used as reservoirs for corrosion inhibitors whose triggered release occurs by galvanic reduction or ion exchange. This work shows one of the first examples of pH-controlled release of corrosion-inhibiting ions from an amorphous metallic coating where the pH change that triggers release is a consequence of the onset of corrosion. This corrosion-inhibition strategy provides further corrosion protection beyond the traditional roles of barrier and sacrificial cathodic protection using a metal coating. For instance, zinc galvanizing provides sacrificial cathodic protection and acts as a barrier, but does not supply inhibitor ions. In the coating described here, protection of an underlying structural alloy exposed at coating defects is demonstrated by inhibitor ion release in addition to barrier function and sacrificial cathodic protection.

The professional role of breast cancer nurses in multi-disciplinary breast cancer care teams.

Since the 1970s breast cancer services have witnessed considerable changes in the management of patients. One significant change was the introduction of specialist core personnel, including the breast care nurse (BCN). The role of the BCN has been gaining credence rapidly in the British NHS and this service is perhaps the paradigm of care for other services. With the lack of specific evidence of the role of specialist nurses in the breast care team, the current study aims to explore this area by in-depth interviews with core team members, and observations of 16 multi-disciplinary teams in England. The study explores the following themes: Nurses' unique informal management leadership role in ensuring the co-ordination, communication and planning of the team work; nurses' innovatory role in making the bureaucracy respond to patients and their relatives needs; nurses supportive role in the provision of expert advice and guidance to other members of the team; nurses confidence and humour in well-performing teams; and the limitations of the professional role of the breast cancer nurse. This study indicates that there is evidence that the BCN is practicing at an advanced level of practice. However, there is a severe lack of evidence-based description of that advanced practice. Cancer nurses including the BCNs should develop and participate in programmes of research in line with cancer legislation in order to build an evidence base that ultimately supports their unique role.

Sudden onset of pitting corrosion on stainless steel as a critical phenomenon.

Stainless steels undergo a sharp rise in pitting corrosion rate as the potential, solution concentration, or temperature is changed only slightly. We report experiments using real-time microscopic in situ visualizations that resolve the nucleation and evolution of individual pits during the transition. They suggest that the sudden onset of corrosion is explained by an explosive autocatalytic growth in the number of metastable pits and that stabilization of individual pits takes place only later. This finding agrees with a theoretical approach treating the onset of pitting corrosion as a cooperative critical phenomenon resulting from interactions among metastable pits, and it extends perspectives on the control and prevention of corrosion onset.

Breast cancer teams: the impact of constitution, new cancer workload, and methods of operation on their effectiveness.

National guidance and clinical guidelines recommended multidisciplinary teams (MDTs) for cancer services in order to bring specialists in relevant disciplines together, ensure clinical decisions are fully informed, and to coordinate care effectively. However, the effectiveness of cancer teams was not previously evaluated systematically. A random sample of 72 breast cancer teams in England was studied (548 members in six core disciplines), stratified by region and caseload. Information about team constitution, processes, effectiveness, clinical performance, and members' mental well-being was gathered using appropriate instruments. Two input variables, team workload (P=0.009) and the proportion of breast care nurses (P=0.003), positively predicted overall clinical performance in multivariate analysis using a two-stage regression model. There were significant correlations between individual team inputs, team composition variables, and clinical performance. Some disciplines consistently perceived their team's effectiveness differently from the mean. Teams with shared leadership of their clinical decision-making were most effective. The mental well-being of team members appeared significantly better than in previous studies of cancer clinicians, the NHS, and the general population. This study established that team composition, working methods, and workloads are related to measures of effectiveness, including the quality of clinical care.

Chronic traumatic and congenital diaphragmatic hernias: presentation and surgical management.

BACKGROUND: The diagnosis of chronic diaphragmatic hernias, whether due to congenital defects or trauma, may be difficult to make and may rely on clinical suspicion in the setting of persistent nondiagnostic radiographic findings. Repair is indicated to avoid catastrophic cardiopulmonary compromise and/or incarceration of abdominal organs. STUDY OBJECTIVES: To review the varied presentations and treatment of chronic diaphragmatic hernia. DESIGN: Retrospective review. SETTING: University of Washington and Harborview Medical Center, Seattle, Washington. PATIENTS: Between 1997 and 2001, nine patients presented with chronic diaphragmatic hernia (two congenital cases, seven post-traumatic cases). Four cases involved the right diaphragm. The following clinical features were noted: asymptomatic, chest radiograph showing bowel herniation (n=1); chest wall mass (n=1); asymptomatic with the chest radiograph showing marked elevation of hemidiaphragm (n=1); dyspnea with the chest radiograph showing marked elevation of hemidiaphragm (n=1); diarrhea and heartburn (n=1); generalized gastrointestinal upset (n=1); recurrent pneumonia (n=2); recurring effusions (n=4); and dyspnea on exertion (n=5). INTERVENTIONS: Diagnosis was confirmed by chest radiograph in two patients, chest computed tomography scan in one patient, barium studies in three patients and thoracoscopy in three patients. All hernias were repaired via thoracotomy, and two hernias were repaired with artificial patch. CONCLUSIONS: Patients with chronic diaphragmatic hernias present with a variety of symptoms and radiographic findings. When radiology or symptoms suggest bowel involvement, barium studies are appropriate. In other cases, chest computed tomography scans and/or thoracoscopy are useful. Repair is accomplished through the ipsilateral chest, with primary repair of the diaphragm preferred over patch repair.

Drawing a line: situating moral boundaries in genetic medicine.

Bioethics traditionally focuses on establishing moral limits between different types of acts. However, boundaries are established by communities and individuals who differ in the constraints shaping their moral world. Phase boundaries, the sites of transition between two physical phases such as a liquid and a gas, provide a metaphor for 'drawing a line' in bioethics discourse. Phase boundaries occur where the physical constraints allow both phases to coexist in stable equilibrium. This relationship can also be considered in reverse, using the known position of the phase boundary to disclose the physical constraints. By analogy, instead of trying to locate the 'correct' moral boundary, the alternative perspective of 'reverse ethics' works from a commonly accepted boundary to examine the constraints of the moral world that are being used to establish it. Genetic interventions into the human body provide interesting examples of boundary establishment. In gene therapy, focusing on boundaries has resulted in a model of moral permissibility that ignores some alternative standpoints and increases the potential for conflict between them. Reverse ethics examines such conflicts in terms of the nature of moral worlds that have come into contact with each other, taking seriously the diversity of factors governing the location of a boundary, in ways that might help shift some entrenched lines of conflict.

When norms normalize: the case of genetic "enhancement".

As the possibility of genetic intervention becomes more concrete, defining and regulating ethically permissible interventions must include a consideration of the implicit as well as explicit consequences. These include the moral implications of defining "enhancement" by reference to a standard of normality. Some authors have called into question the standard ethical concerns about genetic enhancement, but the distinction between enhancing and therapeutic interventions is still structured as relatively unproblematic. However, determining the boundary between therapy and enhancement will have feedback effects on the socially implemented definitions of what counts as normal in human embodiment. Positioning the interface between permissible and nonpermissible interventions at the same place as the boundaries between therapy and enhancement, and between normal and abnormal embodiment, (1) uses biology to justify a moral evaluation, (2) privileges the single standpoint of the genetically canonical person, and (3) enhances the dichotomy between "normal" and "not normal". Assuming that the limit of permissibility along the interventional continuum is coterminous with the definitions of enhancement and of normality, distracts from the work of uncovering the real grounds to setting limits to genetic manipulation.