Distribution of aliphatic amines in CO,CV, and CK carbonaceous chondrites and relation to mineralogy and processing history

The analysis of water‐soluble organic compounds in meteorites provides valuable insights into the prebiotic synthesis of organic matter and the processes that occurred during the formation of the solar system. We investigated the concentration of aliphatic monoamines present in hot acid water extracts of the unaltered Antarctic carbonaceous chondrites, Dominion Range (DOM) 08006 (CO3) and Miller Range (MIL) 05013 (CO3), and the thermally altered meteorites, Allende (CV3), LAP 02206 (CV3), GRA 06101 (CV3), Allan Hills (ALH) 85002 (CK4), and EET 92002 (CK5). We have also reviewed and assessed the petrologic characteristics of the meteorites studied here to evaluate the effects of asteroidal processing on the abundance and molecular distributions of monoamines. The CO3, CV3, CK4, and CK5 meteorites studied here contain total concentrations of amines ranging from 1.2 to 4.0 nmol g^?1 of meteorite; these amounts are 1–3 orders of magnitude below those observed in carbonaceous chondrites from the CI, CM, and CR groups. The low‐amine abundances for CV and CK chondrites may be related to their extensive degree of thermal metamorphism and/or to their low original amine content. Although the CO3 meteorites, DOM 08006 and MIL 05013, do not show signs of thermal and aqueous alteration, their monoamine contents are comparable to those observed in moderately/extensively thermally altered CV3, CK4, and CK5 carbonaceous chondrites. The low content of monoamines in pristine CO carbonaceous chondrites suggests that the initial amounts, and not asteroidal processes, play a dominant role in the content of monoamines in carbonaceous chondrites. The primary monoamines, methylamine, ethylamine, and n‐propylamine constitute the most abundant amines in the CO3, CV3, CK4, and CK5 meteorites studied here. Contrary to the predominance of n‐ω‐amino acid isomers in CO3 and thermally altered meteorites, there appears to be no preference for the larger n‐amines.     

Assessment of boundary-element method for modelling a free-floating sloped wave energy device. Part 1: Numerical modelling

The boundary-element method has been widely used as a design tool in the offshore and ship building industry for more than 30 years. Its application to wave energy conversion is, however, more recent. This paper deals with the numerical modelling of a free-floating sloped wave energy device. The power take-off mechanism of the device consists of an immersed tube with a piston sliding inside. The modelling is done using the boundary-element method package WAMIT. The model is first worked out for the case where the axis of the tube is vertical. It is then derived for the tube inclined and successfully verified against numerical benchmark data. A companion paper presents results of a detailed comparison with a physical model study.     

Molecular distribution, 13C‐isotope,and enantiomeric compositions of carbonaceous chondrite monocarboxylic acids

The water‐soluble organic compounds in carbonaceous chondrite meteorites constitute a record of the synthetic reactions occurring at the birth of the solar system and those taking place during parent body alteration and may have been important for the later origins and development of life on Earth. In this present work, we have developed a novel methodology for the simultaneous analysis of the molecular distribution, compound‐specific δ¹³C, and enantiomeric compositions of aliphatic monocarboxylic acids (MCA) extracted from the hot‐water extracts of 16 carbonaceous chondrites from CM, CR, CO, CV, and CK groups. We observed high concentrations of meteoritic MCAs, with total carbon weight percentages which in some cases approached those of carbonates and insoluble organic matter. Moreover, we found that the concentration of MCAs in CR chondrites is higher than in the other meteorite groups, with acetic acid exhibiting the highest concentration in all samples. The abundance of MCAs decreased with increasing molecular weight and with increasing aqueous and/or thermal alteration experienced by the meteorite sample. The δ¹³C isotopic values of MCAs ranged from ?52 to +27‰, and aside from an inverse relationship between δ¹³C value and carbon straight‐chain length for C₃–C₆ MCAs in Murchison, the ¹³C‐isotopic values did not correlate with the number of carbon atoms per molecule. We also observed racemic compositions of 2‐methylbutanoic acid in CM and CR chondrites. We used this novel analytical protocol and collective data to shed new light on the prebiotic origins of chondritic MCAs.     

Measuring impact crater depth throughout the solar system

One important, almost ubiquitous, tool for understanding the surfaces of solid bodies throughout the solar system is the study of impact craters. While measuring a distribution of crater diameters and locations is an important tool for a wide variety of studies, so too is measuring a crater's “depth.” Depth can inform numerous studies including the strength of a surface and modification rates in the local environment. There is, however, no standard data set, definition, or technique to perform this data-gathering task, and the abundance of different definitions of “depth” and methods for estimating that quantity can lead to misunderstandings in and of the literature. In this review, we describe a wide variety of data sets and methods to analyze those data sets that have been, are currently, or could be used to derive different types of crater depth measurements. We also recommend certain nomenclature in doing so to help standardize practice in the field. We present a review section of all crater depths that have been published on different solar system bodies which shows how the field has evolved through time and how some common assumptions might not be wholly accurate. We conclude with several recommendations for researchers which could help different data sets to be more easily understood and compared.     

Revised recommended methods for analyzing crater size-frequency distributions

Impact crater populations help us to understand solar system dynamics, planetary surface histories, and surface modification processes. A single previous effort to standardize how crater data are displayed in graphs, tables, and archives was in a 1978 NASA report by the Crater Analysis Techniques Working Group, published in 1979 in Icarus. The report had a significant lasting effect, but later decades brought major advances in statistical and computer sciences while the crater field has remained fairly stagnant. In this new work, we revisit the fundamental techniques for displaying and analyzing crater population data and demonstrate better statistical methods that can be used. Specifically, we address (1) how crater size-frequency distributions (SFDs) are constructed, (2) how error bars are assigned to SFDs, and (3) how SFDs are fit to power-laws and other models. We show how the new methods yield results similar to those of previous techniques in that the SFDs have familiar shapes but better account for multiple sources of uncertainty. We also recommend graphic, display, and archiving methods that reflect computers’ capabilities and fulfill NASA's current requirements for Data Management Plans.     

Geology of the Blue Lagoon

The geology of the Blue Lagoon, Abereiddy Bay, South Wales, has been studied for over a hundred years, and is the type locality for the Abereiddian sub‐stage of the Darriwilian (Ordovician), due to its outstanding fossil assemblages. Despite the work done on the Blue Lagoon, its geological significance has not yet been examined. Strata preserved at the Blue Lagoon comprises Avalonian volcanics and marine sediments. This feature examines Avalonia's palaeogeography, the structure and stratigraphy of Abereiddy Bay and the global significance of the geology at these classic localities.     

Postrevolutionary land encroachments in Cairo: Rhizomatic urban space making and the line of flight from illegality

After the January 2011 revolution, new and unpermitted constructions on previously empty land went up across Cairo at striking speed. This paper explores a case of such land encroachments carried out by waste collectors in the neighbourhood of Manshiet Nasser in Cairo, Egypt. It begins with theoretical debates about the production of urban space, arguing that the de Certeauian paradigm, in which urban marginals poach or hijack others' spaces evanescently, fails to account for the way such encroachments produce permanent new spaces rhizomatically alongside the pre‐existing order. The paper then turns to a close examination of the events in Manshiet Nasser. Although in a broad view the actors are marginals living in the ‘informal’ city, the conditions enabling the encroachments were such that only the wealthiest and most powerful members of the ‘community’ benefitted. In a context of generalized ‘illegality’, the squatters rely on practical norms and de facto recognitions to obtain some degree of tenure security. Since these efforts rely on and play off legal norms even as the squatters violate them, the paper argues that property rights in this context should be understood not in classificatory terms based on the legal/illegal binary, but rather through a trajectory of ‘becoming‐legal’: a ‘line of flight’ that approaches legality asymptotically.     

A fungal epizootic in mussels at a deep-sea hydrothermal vent

Mass mortalities due to disease are important determinants of population and community structure in marine ecosystems, but the speed at which an epizootic may sweep through a population, combined with rapid selection for disease‐resistant stocks, can mask the ecological impact of disease in all but the most closely monitored populations. We document an emergent epizootic event in the deep sea that is occurring in mussels (Bathymodiolus brevior) at the Mussel Hill hydrothermal vent in Fiji Basin and we identify the causal agent as a black yeast (order Chaetothyriales) that elicits a pronounced host immune response and is associated with tissue deterioration. The yeast was not observed in other invertebrate taxa (the gastropods Ifremeria nautilei, Alviniconcha aff. hessleri; the limpets Lepetodrilus schrolli, Symmetromphalus aff. hageni; the polychaetes Branchipolynoe pettiboneae, Amphisamytha cf. galapagensis) associated with the mussel bed, nor in mussels (Bathymodiolus brevior) collected from adjacent Lau Basin mussel beds. Massive mussel mortality resulting from the fungal infection is anticipated at the Mussel Hill site in Fiji Basin; we expect that epizootic outbreaks in dense invertebrate communities have the potential to be major determinants of community structure in deep‐sea chemosynthetic ecosystems. The possibility that submersible assets may serve as vectors for transport of the fungus warrants further attention.     

Investigating cross-contamination of aquifers

Shallow aquifers can cross-contaminate deeper aquifers through penetration of an intervening aquitard, via sandy intervals in the aquitard, along well casings, across long well screens, or around aquitard pinchouts. Distinguishing among these potential pathways requires the use of evaluation tools that may support or eliminate certain pathways. These tools include groundwater gradient and aquitard penetration calculations, aquifer pumping test interpretation techniques, chemical concentration plots and statistical methods, hydraulic conductivity-based travel time calculations, pumping-concentration tests, methods for evaluating leaky wells, and methods for evaluating aquitard continuity. Based on analysis of several of these techniques at three sites experiencing aquifer cross-contamination, the authors conclude that calculation of flow rates for various pathways is the single most useful method to confirm or refute specific pathways. Evaluation of leaky wells and aquitard continuity generally must be coupled with other tools to adequately test specific pathways. While fingerprinting, statistical analysis or ratio analysis of contaminants from various sources and receptors was not completed for any of the evaluated sites, the authors believe that these techniques have strong potential for confirming or eliminating pathways. Future research in this area is suggested. Furthermore, the interpretation of pumping-concentration tests is not well developed and needs further assessment.

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Resumen Acuíferos someros pueden ocasionar contaminación transversal de acuíferos profundos mediante la penetración de un acuitardo intermedio, a través de intervalos arenosos en el acuitardo, a lo largo del revestimiento de pozos, o en las inmediaciones de lentes de acuitardos. Para distinguir entre estas trayectorias potenciales se requiere el uso de herramientas de evaluación que pueden apoyar o eliminar ciertas trayectorias. Estas herramientas incluyen cálculos de gradientes de agua subterránea y penetración de acuitardos, técnicas de interpretación de pruebas de bombeo de acuíferos, diagramas de concentración química y métodos estadísticos, estimaciones de conductividad hidráulica en base al tiempo de viaje, pruebas de concentración de bombeo, métodos para evaluar pozos con fugas, y métodos para evaluar la continuidad de acuitardos. Basándose en el análisis de varias de estas técnicas en tres sitios que experimentan contaminación transversal de acuíferos, los autores concluyen que la estimación de ritmos de flujo para varias trayectorias es el único método más útil para confirmar o rechazar trayectorias de flujo específicas. La evaluación de pozos con fugas y continuidad de acuitardos generalmente debe estar acompañada con otras herramientas para probar adecuadamente trayectorias específicas. Aunque no se completó para ninguno de los sitios evaluados técnicas de huellas, análisis estadístico o análisis de relaciones de contaminantes de varias fuentes y receptores, los autores creen que estas técnicas tienen fuerte potencial en la confirmación o eliminación de trayectorias. Se sugiere investigación futura en esta área. Además, la interpretación de pruebas de concentración de bombeo no se ha desarrollado bien y necesita evaluación posterior.

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Résumé Les aquifères de surface peuvent contaminer les aquifères plus profonds à travers un aquitard, un intersection sableuse dans laquitard, le long des forages et de leur crépines, ou de la terminaison biseautée des aquitards. Distinguer et sélectionner ces différents modes de contamination nécessite lutilisation doutils dévaluation. Ces outils incluent le gradient découlement des eaux souterraines et le calcul de pénétration des aquitards, les techniques dinterprétation des essais de pompage, les méthodes dinterprétation chimiques et de traitement statistique, les calculs des temps de transferts sur base de la conductivité, les tests de pompage couplé aux analyses de concentration, les méthodes pour évaluer linfiltration directe alimentant les forages, et les méthodes permettant dévaluer la continuité des aquitards. Basé sur lanalyse de plusieurs de ces techniques sur trois sites expérimentales présentant des contaminations transversale, les auteurs concluent que le calcul des rapports découlement est la méthode la plus simple pour confirmer ou refuser les voies spécifiques. Alors que le traçage, les analyses statistiques et les analyses de la contamination provenant de différentes sources et récepteurs nétait pas complètes pour la plus part des différents sites évalués nétaient pas compléments certains, les auteurs croient que ces techniques ont un potentiel fort pour confirmer ou éliminer ces techniques. Des recherches futures dans cette zone est suggérée. Par ailleurs, linterprétation des tests de pompage couplés à lanalyse des concentrations nest pas développée et nécessite de meilleurs estimations.