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At least 1,189 records · Page 66Linked to original sources
PubMed1999

An analysis of the SEU rate of microcircuits exposed by the various components of space radiation.

In the present paper the experimental and calculated data of SEU rate in microcircuits operating onboard spacecraft are compared. The main features of models and the calculation methods, which are incorporated in the SEREIS software package, are considered. The main features of models, and the calculation methods are considered. The contribution of the different space radiation components (ERB Protons; GCR particles and SEPs) to the SEU rate is discussed with an allowance for the shielding thickness.

Cosmic Radiation↗
PubMed1999

HZE dosimetry in space using plastic track detectors.

Plastic nuclear track detectors were used to measure the contribution of High charge Z and energy E (HZE) particles to the radiation exposure of manned space missions. Results from numerous space missions in the orbit planned for the International Space Station are compared. The measurements cover the declining phase of the last solar cycle during the past 7 years and various shielding conditions inside the US Space Shuttle and the Russian MIR-station.

Collodion↗
PubMed1999

Energy spectrum of iron nuclei measured inside the MIR space craft using CR-39 track detectors.

We have exposed stacks of CR-39 plastic nuclear track detectors inside the MIR space craft during the EUROMIR95 space mission for almost 6 months. Over this long period a large number of tracks of high LET events was accumulated in the detector foils. The etching and measuring conditions for this experiment were optimized to detect tracks of stopping iron nuclei. We found 185 stopping iron nuclei inside the stack and identified their trajectories through the material of the experiment. Based on the energy-range relation the energy at the surface of the stack was determined. These particles allow the determination of the low energy part of the spectrum of iron nuclei behind shielding material inside the MIR station.

Cosmic Radiation↗
PubMed1999

Study of fossil tracks due to 50 < or = Z < or = 92 galactic cosmic ray nuclei in meteoritic crystals: results and perspectives.

A new approach to the problem of investigation of charge and energy spectra of ultra heavy Galactic cosmic ray nuclei, based on fossil track study of extraterrestrial olivine crystals has been developed. The results of an investigation of ultra heavy Galactic cosmic ray nuclei (Z=50-92) in meteoritic olivine crystals are presented. The technique was based on calibration of olivine crystals with accelerated Xe, Au, Pb and U ions and well-controlled partial annealing of "fresh" and "fossil" tracks. It allows us to determine the charge spectra and abundances of cosmic ray nuclei based on fossil track length study in meteoritic and Moon crystals. The comparative studies of the spectra of "fossil' tracks and tracks due to 208Pb and 238U nuclei have shown that the group of 210 micrometers "fossil" tracks, first observed in 1980 at JINR is due to Th-U nuclei-products of recent r-process nucleosynthesis in our Galaxy. The method in principle allows one to resolve Pt-Pb peaks in fossil tracks, to establish the upper limit of the abundance of Z>110 nuclei in the Galactic cosmic rays at the level < or = 10(-3) to the abundance of actinide nuclei and to get information on the history of Z>50 cosmic ray nuclei in time interval up to 220 M.Y.

Calibration↗
PubMed1999

The problems of cosmic ray particle simulation for the near-Earth orbital and interplanetary flight conditions.

A wide range of the galactic cosmic ray and SEP event flux simulation problems for the near-Earth satellite and manned spacecraft orbits and for the interplanetary mission trajectories are discussed. The models of the galactic cosmic ray and SEP events in the Earth orbit beyond the Earth's magnetosphere are used as a basis. The particle fluxes in the near-Earth orbits should be calculated using the transmission functions. To calculate the functions, the dependences of the cutoff rigidities on the magnetic disturbance level and on magnetic local time have to be known. In the case of space flights towards the Sun and to the boundary of the solar system, particular attention is paid to the changes in the SEP event occurrence frequency and size. The particle flux gradients are applied in this case to galactic cosmic ray fluxes.

Cosmic Radiation↗
PubMed2000

Magnetite biomineralization and ancient life on Mars.

Certain chemical and mineral features of the Martian meteorite ALH84001 were reported in 1996 to be probable evidence of ancient life on Mars. In spite of new observations and interpretations, the question of ancient life on Mars remains unresolved. Putative biogenic, nanometer magnetite has now become a leading focus in the debate.

Exobiology↗
PubMed2002

Microbial metal-ion reduction and Mars: extraterrestrial expectations?

Dissimilatory metal-ion-reducing bacteria (DMRB) can couple the reduction of a variety of different metal ions to cellular respiration and growth. The excitement of this metabolic group lies not only in the elucidation of a new type of metabolism, but also in the potential use of these abilities for the removal of toxic organics, and in their ability to reduce (and thus, detoxify) other toxic metals, such as U(VI) and Cr(VI). This review focuses on recent advances in the study of DMRB, including the use of external electron shuttles to enhance rates of metal reduction; genome sequencing and consequent genomic and proteomic analyses; new imaging approaches for high resolution analysis of both cells and chemical components; the demonstration of fractionation of stable isotopes of iron during iron reduction; and the elucidation of the types and patterns of secondary mineral formation during metal reduction. One of the secondary minerals is magnetite, the subject of intense controversy regarding the possibility of evidence for life from the Martian meteorite ALH84001. This review thus ends with a short consideration of the evidence for magnetic 'proof' of the existence of past life on Mars.

Bacteria↗
PubMed2001

PM3, AM1, MNDO and MINDO3 semi-empirical IR spectra simulations for compounds of interest for Titan's chemistry: diazomethane, methyl azide, methyl isocyanide, diacetylene and triacetylene.

Four semi-empirical methods (PM3, AM1, MNDO and MINDO3) have been tested to find the best auxiliary tool for the gas chromatography/Fourier transform IR spectroscopy/mass spectrometry (GC/FTIR/MS) identification of five compounds of interest for Titan's atmospheric chemistry as test compounds: diacetylene, triacetylene, diazomethane, methyl azide, methyl isocyanide. Of the four methods, MINDO3 can be considered as the most appropriate method to facilitate the identification of such and similar compounds, since (1) the simulated IR spectra best match the experimental spectra for four compounds of five studied; and (2) MINDO3 provides the best linearity between the calculated and experimental frequencies (correlation coefficient of 0.995; a scaling factor of 0.84 can be applied to afford better correspondence between the calculated and experimental wavenumbers). None of the semi-empirical methods tested is able to predict (even approximately) infrared band intensities, and therefore a spectral intensity pattern.

Acetylene↗
PubMed2002

Near-infrared spectroscopic study of nontronites and ferruginous smectite.

The existence of life on planets such as Mars depend upon the presence of water. This water may not necessarily be as liquid or crystalline water but may be as interlayer water such as is found in smectitic clays. One group of smectites, relevant to the search for interplanetary life are those which have a high iron content, known as nontronites. Near-IR reflectance spectroscopy has been used to show the presence of water and hydroxyl units in these minerals. Three near-IR spectral regions are identified, (a) the high frequency region between 6400 and 7400 cm(-1) attributed to the first overtone of the hydroxyl stretching mode; (b) the 4800-5400 cm(-1) region attributed to water combination modes; and (c) the 4000-4800 cm(-1) region attributed to the combination of the stretching and deformation modes of the FeFeOH units of nontronite. Two types of hydroxyl groups were identified using near-IR spectroscopy, hydroxyl units coordinated to the iron, and hydroxyl groups from water in the nontronite structure. The first hydroxyls are characterised by several bands, firstly in the 7055-7098 cm(-1) region assigned to the first overtone of the AlFeOH stretching unit, secondly in the 6958-6878 cm(-1) region attributed to the FeFeOH unit. The overtone of the hydroxyl stretching frequency of water was observed at around 6800 cm(-1). These observations show that nontronites can be a source of water that may support life.

Aluminum Silicates↗
PubMed1999

Variations in the strength of the infrared forbidden 2328.2 cm-1 fundamental of solid N2 in binary mixtures.

We present the 2335-2325 cm-1 infrared spectra and band positions, profiles and strengths (A values) of solid nitrogen and binary mixtures of N2 with other molecules at 12 K. The data demonstrate that the strength of the infrared forbidden N2 fundamental near 2328 cm-1 is moderately enhanced in the presence of NH3, strongly enhanced in the presence of H2O and very strongly enhanced (by over a factor of 1000) in the presence of CO2, but is not significantly affected by CO, CH4, or O2. The mechanisms for the enhancements in N2-NH3 and N2-H2O mixtures are fundamentally different from those proposed for N2-CO2 mixtures. In the first case, interactions involving hydrogen-bonding are likely the cause. In the latter, a resonant exchange between the N2 stretching fundamental and the 18O = 12C asymmetric stretch of 18O12C16O is indicated. The implications of these results for several astrophysical issues are briefly discussed.

Ammonia↗
PubMed2000

PM3, AM1, MINDO3 semi-empirical IR spectra simulations for some nitriles of interest for Titan's chemistry.

A set of the semi-empirical methods (PM3, AM1, MNDO and MINDO3) has been tested to find the best auxiliary tool for the identification of nitriles by gas chromatography/Fourier transform IR spectroscopy/mass spectrometry, considering five nitriles of interest for Titan's chemistry as test compounds: acetonitrile, acrylonitrile, cyanoacetylene, 2-butynenitrile and dicyanoacetylene. Of the four semi-empirical methods, MNDO can be considered as the most advantageous auxiliary tool for the gas chromatography/Fourier transform IR spectroscopy/mass spectrometry (GC/FTIR/MS) identification of nitriles of interest for Titan's atmospheric chemistry, since (1) the simulated IR spectra best match the experimental (in some cases AM1 gives comparable results); (2) it provides the best linearity between the calculated and experimental frequencies (correlation coefficient of 0.990); a scaling factor of 0.90 can be applied to afford better correspondence between the calculated and experimental wavenumbers. At the same time, none of the methods is able to predict infrared intensities and a spectral intensity pattern.

Computer Simulation↗
PubMed2003

Bdelloid rotifers as model system to study developmental biology in space.

Bdelloid rotifers are suitable model systems for space experiments. Due to their developmental pattern they appear adequate to investigate the role of the cytoskeleton during oogenesis and during early developmental stages, and to reflect the effects of disturbances in the spatial arrangement of cytoskeletal components. The effect of weightlessness on the developmental pattern of a bdelloid rotifer will be studied in the International Space Station: in preparation for it we are performing ground-based experiments on the development of rotifer embryos under either increased or decreased gravity. The model studied is Macrotrachela quadricornifera, a species of rotifers belonging to the Bdelloidea class. Samples exposed to gravity disturbance were analyzed for morphology and fitness-related parameters. Rotifers were exposed over several days to altered gravity conditions and the morphology of eggs laid during this period were investigated using a confocal laser microscope. A subset of eggs was allowed to hatch to determine newborn developmental time and age at maturity. High (up to 20 g) gravity was obtained in a slow centrifuge suitable for animal cultivation over several days. To produce low (simulated 0.0001 g) gravity a Random Positioning Machine equipped with a 'rotifer bioreactor' was used. Under all conditions the rotifer retained normal life-history traits, and did not show permanent changes in embryo morphology, regardless to the stresses to which it was exposed. Only some modification of the shape of early embryos, experiencing 20 g, has been noted, but later developmental stages appeared unaffected, and normal juveniles hatched. Whether this result indicates any capacity to repair damage during embryogenesis of these Spiralia experiencing 20 g is an open question. The significance of the result as well as the use of instruments to simulate gravity perturbations are discussed.

Animals↗
PubMed2003

New facilities and instruments for developmental biology research in space.

Three new ESA facilities will be available for biological experiments in Space, Biopack on the Space Shuttle and two instruments on the International Space Station (ISS): BIOLAB in the European "Columbus" Laboratory and the European Modular Cultivation System (EMCS) in the US Lab "Destiny". The experiments are housed in standard Experiment Containers, allowing either research in microgravity or acceleration studies with variable g-levels, if mounted on the centrifuges. While Biopack provides only thermal control, BIOLAB and EMCS supply each container with a dedicated atmosphere (controlled CO2, O2 concentration and relative humidity, trace gas removal): EMCS contains also fresh and wastewater reservoirs on its rotors. Power and data lines are available in all the described facilities. Highly automated systems, like BIOLAB's Handling Mechanism and Analysis Instruments, support the telescience concept and help reducing crew time in orbit. A BioGlovebox with its support instruments allows unique research possibilities in Space. The feasibility of experiment hardware inside the containers has been studied by ESA for several kinds of Experiment Support Equipment with potential use for research in Developmental Biology: design concepts for experiments with small eggs, cells and tissues, with small aquatic animals, with insects and with plants are described in this article.

Animals↗
PubMed1999

Teaching of space life sciences.

Space life sciences is not really a new life sciences discipline such as immunology was some decades ago and it may never be so. Rather it is a field that will provide each existing life sciences discipline with new and more information gathered from space research. In fact, the danger is that space research will be confined in a separate discipline, and thus it will be cut off from classical ground research. Conversely, scientists should increasingly consider spaceflight as a tool and should integrate the findings of space research into their traditional disciplines. A brief survey of topics and main findings in the various subdisciplines of space life sciences is provided. This is followed by a discussion of typical problems encountered such as access to space, controls, ground-based simulations, medical care in space, extravehicular activity, and environmental control and life support. As many space life sciences courses are initiated around the world either by space agencies or universities or jointly, there is a need to consider the international, intercultural, and interdisciplinary aspects of such programs. It is argued that the growing knowledge derived from space research should be integrated into the regular teaching of life sciences rather than leaving it confined to a separate field. Teaching of space life sciences is a prime candidate for the application of the new techniques of "cyberspace education", where interactive learning and globalization of the learning process will take a leading place. The experts and student body are dispersed over many nations, research is of necessity conducted on a basis of international cooperation. The conduct of tele-education is discussed and existing information sources and courses are listed.

Biological Science Disciplines↗