No abstract

No abstract

Cerebral malaria (CM) is associated with high mortality and morbidity as a certain percentage of survivors suffers from persistent neurological sequelae. The mechanisms leading to death and functional impairments are yet not fully understood. This study investigated biochemical and morphological markers of apoptosis in the brains of mice infected with Plasmodium berghei ANKA. Cleaved caspase-3 was detected in the brains of animals with clinical signs of CM and immunoreactivity directly correlated with the clinical severity of the disease. Caudal parts of the brain showed more intense immunoreactivity for cleaved caspase-3. Double-labelling experiments revealed processing of caspase-3 primarily in neurons and oligodendrocytes. These cells also exhibited apoptotic-like morphological profiles in ultrastructural analysis. Further, cleavage of caspase-3 was found in endothelial cells. In contrast to neurons and oligodendrocytes, apoptosis of endothelial cells already occurred in early stages of the disease. Our results are the first to demonstrate processing of caspase-3 in different central nervous system cells of animals with CM. Apoptosis of endothelial cells may represent a critical issue for the development of the disease in the mouse model. Neurological signs and symptoms might be attributable, at least in part, to apoptotic degeneration of neurons and glia in advanced stages of murine CM.

No abstract

Collisions between large, similar-sized bodies are believed to shape the final characteristics and composition of terrestrial planets. Their inventories of volatiles such as water are either delivered or at least significantly modified by such events. Besides the transition from accretion to erosion with increasing impact velocity, similar-sized collisions can also result in hit-and-run outcomes for sufficiently oblique impact angles and large enough projectile-to-target mass ratios. We study volatile transfer and loss focusing on hit-and-run encounters by means of smooth particle hydrodynamics simulations, including all main parameters: impact velocity, impact angle, mass ratio and also the total colliding mass. We find a broad range of overall water losses, up to 75% in the most energetic hit-and-run events, and confirm the much more severe consequences for the smaller body also for stripping of volatile layers. Transfer of water between projectile and target inventories is found to be mostly rather inefficient, and final water contents are dominated by pre-collision inventories reduced by impact losses, for similar pre-collision water mass fractions. Comparison with our numerical results shows that current collision outcome models are not accurate enough to reliably predict these composition changes in hit-and-run events. To also account for nonmechanical losses, we estimate the amount of collisionally vaporized water over a broad range of masses and find that these contributions are particularly important in collisions of ∼ Mars-sized bodies, with sufficiently high impact energies, but still relatively low gravity. Our results clearly indicate that the cumulative effect of several (hit-and-run) collisions can efficiently strip protoplanets of their volatile layers, especially the smaller body, as it might be common, e.g., for Earth-mass planets in systems with Super-Earths. An accurate model for stripping of volatiles that can be included in future planet formation simulations has to account for the peculiarities of hit-and-run events and track compositional changes in both large post-collision fragments.