Soil diversity and hydration as observed by ChemCam at Gale crater, Mars

The ChemCam instrument, which provides insight into martian soil chemistry at the submillimeter scale, identified two principal soil types along the Curiosity rover traverse: a fine-grained mafic type and a locally derived, coarse-grained felsic type. The mafic soil component is representative of widespread martian soils and is similar in composition to the martian dust. It possesses a ubiquitous hydrogen signature in ChemCam spectra, corresponding to the hydration of the amorphous phases found in the soil by the CheMin instrument. This hydration likely accounts for an important fraction of the global hydration of the surface seen by previous orbital measurements. ChemCam analyses did not reveal any significant exchange of water vapor between the regolith and the atmosphere. These observations provide constraints on the nature of the amorphous phases and their hydration.

Introduction to special section: early Mars

Ongoing studies of the evolution of the Martian cratered highlands, the nature of the planet's early climate, and the recent announcement of possible evidence of ancient life in the ALH 84001 meteorite have reinvigorated interest in the conditions that prevailed on Mars during its first billion years of geologic history. To address this interest and assess our current understanding of these issues, the Lunar and Planetary Institute hosted a 4-day Conference on Early Mars in Houston in April of 1997. The papers contained in this special section are a product of that meeting. The purpose of the conference was twofold: (1) to consider how impacts, volcanism, and the presence of abundant water affected the physical and chemical environment that existed on Mars 4 Gyr ago, particularly as it related to the nature of the global climate, the origin of the valley networks, the geologic and mineralogic evolution of the surface, the aqueous geochemistry of groundwater, and the existence of local environments that may have been conducive to the development of indigenous life and the preservation of its signature in the geologic record; and (2) to discuss what observations or experiments might he included in future spacecraft missions to test the ideas and expectations arising from purpose 1. While pertinent issues of early atmospheric and solar evolution were also addressed, the primary discussion at the conference focused on the evidence and constraints provided by the geologic records of Earth, the Moon, and Mars and analysis of the SNC meteorites. The papers contained in this special section span the full range of these topics, including the stability of the early atmosphere to erosion by the solar wind, the geologic environment from which the SNC meteorites originated, geomorphic evidence regarding the nature of the early Martian climate and hydrologic cycle, the potential impact of the past and present environment on the preserved signature of ancient life, and a discussion of the capabilities of a lander-based X ray diffraction and fluorescence instrument to assess the potential for past fossilization from the mineralogy of the current local surface environment. The issues raised at the conference, and by the papers included in this special section, will be the focus of ongoing attention as the intensity and scope of Mars exploration increases over the next decade.

Chronic ethanol exposure potentiates NMDA excitotoxicity in cerebral cortical neurons

The effect of acute and chronic ethanol exposure on excitotoxicity in cultured rat cerebral cortical neurons was examined. Neuronal death was quantitated by measuring the accumulation of lactate dehydrogenase (LDH) in the culture media 20 h after exposure to NMDA. Addition of NMDA (25-100 microM) to the culture dishes for 25 min in Mg(2+)-free buffer resulted in a dose-dependent increase in LDH accumulation. Phase-contrast microscopy revealed obvious signs of cellular injury as evidenced by granulation and disintegration of cell bodies and neuritic processes. Chronic exposure of neuronal cultures to ethanol (100 mM) for 96 h followed by its removal before NMDA exposure, significantly increased NMDA-stimulated LDH release by 36 and 22% in response to 25 microM and 50 microM NMDA, respectively. Neither basal LDH release nor that in response to maximal NMDA (100 microM) stimulation was altered by chronic alcohol exposure. In contrast to the effects of chronic ethanol on NMDA neurotoxicity, inclusion of ethanol (100 mM) only during the NMDA exposure period significantly reduced LDH release by approximately 50% in both control and chronically treated dishes. This reduction by acute ethanol was also observed under phase-contrast microscopy as a lack of development of granulation and a sparing of disintegration of neuritic processes. These results indicate that chronic exposure of ethanol to cerebral cortical neurons in culture can sensitize neurons to excitotoxic NMDA receptor activation.