L'évolution du système consonantique des langues cangin

The Cangin languages are classified as an own subgroup of the Atlantic languages. Evidence for their common origin can be given by the comparative method. By means of the systematic grammatical comparison of different languages this method aims at the reconstruction of a hypothetic proto-language and allows to draw hypothesises on their diachronic linguistic development. This paper concentrates on the evolution of the consonant system of the Cangin languages.

La dénervation rénale unilatérale et le système kallikréine-bradykinine rénal chez le rat

But de l’étude L’effet antihypertenseur de la dénervation rénale chez les patients hypertendus s’explique partiellement par une augmentation de la natriurèse tubulaire. Pour étudier une contribution possible du système kallikréine-kinines (SKK) à cette natriurèse dans le rat, nous avons dosé dans le plasma et dans les tissus l’activité de la kallikréine (AK) et la concentration de la bradykinine (BK). Méthodes Pour AK, nous avons adapté et validé un essai enzymatique qui libère la para-nitroaniline à partir du tripeptide H-D-Pro-Phe-Arg-pNA ; les coefficients de variation (CV) intra-essai et inter-essai étaient inférieurs à 8 % pour AK plasmatique et tissulaire (plasma n = 6 et 13, tissu n = 4). La linéarité d’une série de dilutions confirmait la spécificité de l’essai. Le dosage de BK tissulaire se basait sur une méthode établie pour le plasma : tissus étaient homogénéisés et BK extraite et isolée par éthanol et HPLC, et finalement quantifiée par radio-immunoessai. Les CV intra- et inter-essai pour BK étaient 18 % dans le plasma (n = 8 et n = 35) et inférieurs à 16 % dans différents tissus (n = 5–8). Résultats Chez le rat mâle Wistar (n = 3), la BK plasmatique était de 8,2 ± 6,6 fmol/mL (M ± SD) et la BK tissulaire (fmol/g) variait, pour les 14 organes testés, de 14 ± 3 pour le cerveau à 521 ± 315 pour la glande sous-maxillaire. Six jours après dénervation rénale gauche, la BK rénale gauche (89 ± 9) n’était pas différente comparée à la BK rénale droite (75 ± 23). De même, l’AK était identique dans les deux reins (gauche 18,0 ± 1,5, droit 15,8 ± 1,4 μkat/g). Conclusion Un effet éventuel de la dénervation rénale unilatéral sur le SKK rénal devrait donc être bilatéral.

Analysis of polygonal cracking patterns in chloride-bearing terrains on Mars: Indicators of ancient playa settings

The ancient southern highlands on Mars (~3.5 Gyr old) contain > 600 regions that display spectral evidence in the infrared for the presence of chloride-bearing materials. Many of these locations were previously reported to display polygonal cracking patterns. We studied more than 80 of the chloride-bearing terrains using high-resolution (0.25-0.5 m/pixel) images, as well as near-infrared spectral data, to characterize the surface textures and the associated cracking patterns and mineralogies. Our study indicates that ~75% of the studied locations display polygonal cracks that resemble desiccation cracks, while some resemble salt expansion/thrust polygons. Furthermore, we detect, spectrally, the presence of smectites in association with ~30% of the studied fractured terrains. We note that smectites are a special class of swelling clay minerals that can induce formation of large desiccation cracks. As such, we suggest that the cracking patterns are indicative of the presence of smectite phyllosilicates even in the absence of spectral confirmation. Our results suggest that many chloride-bearing terrains have a lacustrine origin and a geologic setting similar to playas on Earth. Such locations would have contained ephemeral lakes that may have undergone repeated cycles of desiccation and recharging by a near-surface fluctuating water table in order to account for the salt-phyllosilicates associations. These results have notable implications for the ancient hydrology of Mars. We propose that the morphologies and sizes of the polygonal cracks can be used as paleoenvironmental, as well as lithological, indicators that could be helpful in planning future missions.

Photometric properties of Mars soils analogs

We have measured the bidirectional reflectance of analogs of dry, wet, and frozen Martian soils over a wide range of phase angles in the visible spectral range. All samples were produced from two geologic samples: the standard JSC Mars-1 soil simulant and Hawaiian basaltic sand. In a first step, experiments were conducted with the dry samples to investigate the effects of surface texture. Comparisons with results independently obtained by different teams with similar samples showed a satisfying reproducibility of the photometric measurements as well as a noticeable influence of surface textures resulting from different sample preparation procedures. In a second step, water was introduced to produce wet and frozen samples and their photometry investigated. Optical microscope images of the samples provided information about their microtexture. Liquid water, even in relatively low amount, resulted in the disappearance of the backscattering peak and the appearance of a forward-scattering peak whose intensity increases with the amount of water. Specular reflections only appeared when water was present in an amount large enough to allow water to form a film at the surface of the sample. Icy samples showed a wide variability of photometric properties depending on the physical properties of the water ice. We discuss the implications of these measurements in terms of the expected photometric behavior of the Martian surface, from equatorial to circum-polar regions. In particular, we propose some simple photometric criteria to improve the identification of wet and/or icy soils from multiple observations under different geometries.

Morphology and evolution of the ejecta of Hale crater in Argyre basin, Mars: Results from high resolution mapping

We use various data sets, including images from the High Resolution Imaging Science Experiment camera (HiRISE), to examine the ejecta of the generally fresh-looking Hale crater that occurs in the rugged mountain terrain of Nereidum Montes in the northern rim materials of the Argyre impact structure on Mars. Our investigation reveals that the distal parts of the Hale crater ejecta and other basin deposits behave like viscous flows, which we attribute to the secondary flow of ejecta mixed with water–ice-rich basin materials. Consistent with water-enrichment of the basin materials, our mapping further reveals occasionally deformed surfaces, including highly conspicuous features such as mounds and fractured plateaus that we interpret to be a result of periglacial modification, subsequent (including possibly present-day) to the transient localized melting and fluvial erosion caused by Hale-impact-generated heating. In particular, our morphometric analysis of a well-defined valley system west of Hale crater suggests that it may have been formed through hydrologic/glacial activity prior to the Hale impact, with additional modification resulting from the impact and subsequent geologic and hydrologic phenomena including glacial and periglacial activity.