Sedimentary processes of the Bagnold Dunes: Implications for the eolian rock record of Mars.

The Mars Science Laboratory rover Curiosity visited two active wind-blown sand dunes within Gale crater, Mars, which provided the first ground-based opportunity to compare Martian and terrestrial eolian dune sedimentary processes and study a modern analog for the Martian eolian rock record. Orbital and rover images of these dunes reveal terrestrial-like and uniquely Martian processes. The presence of grainfall, grainflow, and impact ripples resembled terrestrial dunes. Impact ripples were present on all dune slopes and had a size and shape similar to their terrestrial counterpart. Grainfall and grainflow occurred on dune and large-ripple lee slopes. Lee slopes were ~29° where grainflows were present and ~33° where grainfall was present. These slopes are interpreted as the dynamic and static angles of repose, respectively. Grain size measured on an undisturbed impact ripple ranges between 50 µm and 350 µm with an intermediate axis mean size of 113 µm (median: 103 µm). Dissimilar to dune eolian processes on Earth, large, meter-scale ripples were present on all dune slopes. Large ripples had nearly symmetric to strongly asymmetric topographic profiles and heights ranging between 12 cm and 28 cm. The composite observations of the modern sedimentary processes highlight that the Martian eolian rock record is likely different from its terrestrial counterpart because of the large ripples, which are expected to engender a unique scale of cross stratification. More broadly, however, in the Bagnold Dune Field as on Earth, dune-field pattern dynamics and basin-scale boundary conditions will dictate the style and distribution of sedimentary processes.

Large wind ripples on Mars: A record of atmospheric evolution.

Wind blowing over sand on Earth produces decimeter-wavelength ripples and hundred-meter- to kilometer-wavelength dunes: bedforms of two distinct size modes. Observations from the Mars Science Laboratory Curiosity rover and the Mars Reconnaissance Orbiter reveal that Mars hosts a third stable wind-driven bedform, with meter-scale wavelengths. These bedforms are spatially uniform in size and typically have asymmetric profiles with angle-of-repose lee slopes and sinuous crest lines, making them unlike terrestrial wind ripples. Rather, these structures resemble fluid-drag ripples, which on Earth include water-worked current ripples, but on Mars instead form by wind because of the higher kinematic viscosity of the low-density atmosphere. A reevaluation of the wind-deposited strata in the Burns formation (about 3.7 billion years old or younger) identifies potential wind-drag ripple stratification formed under a thin atmosphere.

Deposition, exhumation, and paleoclimate of an ancient lake deposit, Gale crater, Mars.

The landforms of northern Gale crater on Mars expose thick sequences of sedimentary rocks. Based on images obtained by the Curiosity rover, we interpret these outcrops as evidence for past fluvial, deltaic, and lacustrine environments. Degradation of the crater wall and rim probably supplied these sediments, which advanced inward from the wall, infilling both the crater and an internal lake basin to a thickness of at least 75 meters. This intracrater lake system probably existed intermittently for thousands to millions of years, implying a relatively wet climate that supplied moisture to the crater rim and transported sediment via streams into the lake basin. The deposits in Gale crater were then exhumed, probably by wind-driven erosion, creating Aeolis Mons (Mount Sharp).

In situ radiometric and exposure age dating of the martian surface.

We determined radiogenic and cosmogenic noble gases in a mudstone on the floor of Gale Crater. A K-Ar age of 4.21 ± 0.35 billion years represents a mixture of detrital and authigenic components and confirms the expected antiquity of rocks comprising the crater rim. Cosmic-ray-produced (3)He, (21)Ne, and (36)Ar yield concordant surface exposure ages of 78 ± 30 million years. Surface exposure occurred mainly in the present geomorphic setting rather than during primary erosion and transport. Our observations are consistent with mudstone deposition shortly after the Gale impact or possibly in a later event of rapid erosion and deposition. The mudstone remained buried until recent exposure by wind-driven scarp retreat. Sedimentary rocks exposed by this mechanism may thus offer the best potential for organic biomarker preservation against destruction by cosmic radiation.

Elemental geochemistry of sedimentary rocks at Yellowknife Bay, Gale crater, Mars.

Sedimentary rocks examined by the Curiosity rover at Yellowknife Bay, Mars, were derived from sources that evolved from an approximately average martian crustal composition to one influenced by alkaline basalts. No evidence of chemical weathering is preserved, indicating arid, possibly cold, paleoclimates and rapid erosion and deposition. The absence of predicted geochemical variations indicates that magnetite and phyllosilicates formed by diagenesis under low-temperature, circumneutral pH, rock-dominated aqueous conditions. Analyses of diagenetic features (including concretions, raised ridges, and fractures) at high spatial resolution indicate that they are composed of iron- and halogen-rich components, magnesium-iron-chlorine-rich components, and hydrated calcium sulfates, respectively. Composition of a cross-cutting dike-like feature is consistent with sedimentary intrusion. The geochemistry of these sedimentary rocks provides further evidence for diverse depositional and diagenetic sedimentary environments during the early history of Mars.

Volatile and organic compositions of sedimentary rocks in Yellowknife Bay, Gale crater, Mars.

H2O, CO2, SO2, O2, H2, H2S, HCl, chlorinated hydrocarbons, NO, and other trace gases were evolved during pyrolysis of two mudstone samples acquired by the Curiosity rover at Yellowknife Bay within Gale crater, Mars. H2O/OH-bearing phases included 2:1 phyllosilicate(s), bassanite, akaganeite, and amorphous materials. Thermal decomposition of carbonates and combustion of organic materials are candidate sources for the CO2. Concurrent evolution of O2 and chlorinated hydrocarbons suggests the presence of oxychlorine phase(s). Sulfides are likely sources for sulfur-bearing species. Higher abundances of chlorinated hydrocarbons in the mudstone compared with Rocknest windblown materials previously analyzed by Curiosity suggest that indigenous martian or meteoritic organic carbon sources may be preserved in the mudstone; however, the carbon source for the chlorinated hydrocarbons is not definitively of martian origin.

Curiosity at Gale crater, Mars: characterization and analysis of the Rocknest sand shadow.

The Rocknest aeolian deposit is similar to aeolian features analyzed by the Mars Exploration Rovers (MERs) Spirit and Opportunity. The fraction of sand <150 micrometers in size contains ~55% crystalline material consistent with a basaltic heritage and ~45% x-ray amorphous material. The amorphous component of Rocknest is iron-rich and silicon-poor and is the host of the volatiles (water, oxygen, sulfur dioxide, carbon dioxide, and chlorine) detected by the Sample Analysis at Mars instrument and of the fine-grained nanophase oxide component first described from basaltic soils analyzed by MERs. The similarity between soils and aeolian materials analyzed at Gusev Crater, Meridiani Planum, and Gale Crater implies locally sourced, globally similar basaltic materials or globally and regionally sourced basaltic components deposited locally at all three locations.

Martian fluvial conglomerates at Gale crater.

Observations by the Mars Science Laboratory Mast Camera (Mastcam) in Gale crater reveal isolated outcrops of cemented pebbles (2 to 40 millimeters in diameter) and sand grains with textures typical of fluvial sedimentary conglomerates. Rounded pebbles in the conglomerates indicate substantial fluvial abrasion. ChemCam emission spectra at one outcrop show a predominantly feldspathic composition, consistent with minimal aqueous alteration of sediments. Sediment was mobilized in ancient water flows that likely exceeded the threshold conditions (depth 0.03 to 0.9 meter, average velocity 0.20 to 0.75 meter per second) required to transport the pebbles. Climate conditions at the time sediment was transported must have differed substantially from the cold, hyper-arid modern environment to permit aqueous flows across several kilometers.

Pyroclastic activity at Home Plate in Gusev Crater, Mars.

Home Plate is a layered plateau in Gusev crater on Mars. It is composed of clastic rocks of moderately altered alkali basalt composition, enriched in some highly volatile elements. A coarsegrained lower unit lies under a finer-grained upper unit. Textural observations indicate that the lower strata were emplaced in an explosive event, and geochemical considerations favor an explosive volcanic origin over an impact origin. The lower unit likely represents accumulation of pyroclastic materials, whereas the upper unit may represent eolian reworking of the same pyroclastic materials.

Deficient hypoxia awakening response in infants of smoking mothers: possible relationship to sudden infant death syndrome.

OBJECTIVE: To determine whether fetal exposure to cigarette smoke impairs postnatal chemoreceptor control of ventilation and hypercapnic and hypoxic awakening responses. STUDY DESIGN: Smoking (n = 13) and nonsmoking (n = 34) women were recruited during pregnancy. Serum cotinine levels were measured to assess level of nicotine exposure. The infants were studied at 2 to 3 months of age for ventilatory and awakening responses to hypoxia (17%, 15% and 13% inspired O2) and hypercapnia 4%, 6%, and 8% inspired CO2). Continuous measures were analyzed with unpaired t tests and analysis of variance for repeated measures. Proportions of awakening and periodic breathing were analyzed by means of a comparison of proportions. RESULTS: The infants of smokers had lower birth weights (3022 +/- 566 vs 3518 +/- 491 gm; p < or = 0.005) and were older at the time of study (10.4 +/- 2.8 vs 8.7 +/- 1.3 weeks; p < 0.01) than the control infants. Maternal cotinine levels were higher in smokers (97.8 +/- 107 ng/ml vs no cotinine; p < 0.0001). More infants of smokers failed to awaken with hypoxia than did control infants (54% vs 15%; p = 0.006). The ventilatory responses to hypoxia and hypercapnia were similar in the two groups. All infants awakened with hypercapnia, and there was no difference in the awakening threshold for carbon dioxide (50.3 +/- 4.5 vs 48.3 +/- 5.4 mm Hg; p = 0.28). CONCLUSION: Infants of mothers who smoked during pregnancy have deficient hypoxic awakening responses, which may contribute to the increased risk of sudden infant death syndrome in infants of smoking mothers.

Hepatotoxic effects of tacrine administration in patients with Alzheimer's disease.

OBJECTIVE: To characterize the hepatic effects of tacrine treatment in patients with Alzheimer's disease. DESIGN: Controlled trials of tacrine therapy consisting of two blinded, parallel-group trials; three blinded, enrichment-design trials; and their respective open-label extensions. SETTING: Multicenter clinical trials in the United States, France, and Canada. PATIENTS: A total of 2446 men and women at least 50 years of age with a diagnosis of probable Alzheimer's disease of mild to moderate severity and in good health without significant hepatic, cardiovascular, or renal disease. INTERVENTION: Administration of tacrine vs placebo, with weekly measurement of serum hepatic enzymes. MAIN OUTCOME MEASURES: Incidence, maximum severity, and timing of event for serum alanine aminotransferase (ALT) elevation. RESULTS: Among the 2446 patients who received tacrine in clinical trials, ALT levels greater than the upper limit of normal (ULN) occurred on at least one occasion in 1203 patients (49%), ALT levels greater than three times the ULN occurred in 621 patients (25%), and ALT levels greater than 20 times the ULN occurred in 40 patients (2%). The elevated ALT levels were generally asymptomatic and occurred more frequently in women than men. The mean time from initiation of tacrine treatment to first ALT level greater than three times the ULN was 50 days, and 90% of all initial ALT levels greater than three times the ULN occurred during the first 12 weeks of treatment. Of 145 patients who discontinued tacrine treatment because of an ALT level greater than three times the ULN and were rechallenged, 127 (88%) were able to resume long-term therapy with the drug. In all instances, discontinuing tacrine completely reversed elevations in ALT levels, and no deaths related to hepatotoxicity occurred. CONCLUSIONS: These data suggest that the potential for serious hepatic toxicity can be reduced through careful monitoring of ALT levels in patients who may benefit from tacrine therapy.

A controlled trial of tacrine in Alzheimer's disease. The Tacrine Study Group.

OBJECTIVE: To compare efficacy and safety of tacrine hydrochloride with placebo in patients with probable Alzheimer's disease. DESIGN: A 12-week, double-blind, placebo-controlled, parallel-group study. SETTING: Outpatients at 23 centers. PATIENTS: Men and women with probable Alzheimer's disease, at least 50 years old, mildly to moderately impaired, without other significant medical conditions. INTERVENTIONS: In the initial 6 weeks, patients received placebo, 20 mg/d of tacrine, or 40 mg/d of tacrine. In the second 6 weeks, half received the same treatment and half increased tacrine dose: those receiving placebo increased to 20 mg/d, those receiving 20 mg/d increased to 40 mg/d, and those receiving 40 mg/d increased to 80 mg/d. PRIMARY OUTCOME MEASURES: Alzheimer's Disease Assessment Scale (ADAS) cognitive component and clinician-rated Clinical Global Impression of Change (CGIC). RESULTS: Four hundred sixty-eight patients entered. After 12 weeks, dose-related improvement was significant on the ADAS cognitive (P = .014), clinician-rated CGIC (P = .014), and caregiver-rated CGIC (P = .006). Comparison of 80 mg/d with placebo showed significant improvement on the ADAS cognitive (P = .015), clinician-rated CGIC (P = .016), and caregiver-rated CGIC (P = .028). Significant effects appeared as early as 6 weeks on the ADAS cognitive and caregiver-rated CGIC. Among patients receiving 80 mg/d of tacrine, 51% achieved a four-point or greater improvement of the ADAS cognitive component after 12 weeks of treatment. Reversible asymptomatic transaminase elevations greater than three times normal occurred in 25% of patients. Other treatment-related events included nausea and/or vomiting (8%), diarrhea (5%), abdominal pain (4%), dyspepsia (3%), and rash (3%). CONCLUSIONS: These results confirm the efficacy and safety of tacrine in some patients with Alzheimer's disease. After 12 weeks, the magnitude of the treatment effect is clinically important and recognized by the physician and caregiver. Liver toxicity is reversible and easily detected by weekly alanine aminotransferase determinations.

GLC of morphine and co-extractants in the rapid analysis of post mortem blood.

A qualitative study of over 70 drugs and related compounds was carried out. The study incorporated a recognised procedure for the analysis of morphine in post mortem blood. Stock solutions of the compounds were reacted with heptafluorobutyric acid anhydride and the derivatives were examined by gas-liquid chromatography on an OV-17 column using electron capture detection. The results were tabulated with respect to retention time, minimum detectable amount, and reactivity.