Space radiation biology]

Astronauts were constantly exposed to space radiation containing various kinds of energy with a low-dose rate during long-term stays in space. Therefore, it is important to judge correctly the biological effect of space radiation for human health. In addition, research for space radiation might give us useful information concerning birth and evolution of lives on the earth. Here, we described a view of the future about space experiments at an International Space Station. Therefore, we desire to educate the space researcher of the next generation for importance of research for space radiation.     

Delay in oral mucosal ulcer healing by aspirin is linked to the disturbances in p38 mitogen-activated protein kinase activation.

BACKGROUND: Among the early manifestations of oral mucosal impairment by nonsteroidal anti-inflammatory drugs is the delay in soft oral tissue repair brought about by the amplification of apoptotic events. In this study, we investigated the effect of a specific inhibitor of p38 mitogen-activated protein kinase (p38 MAPK), SB 203580, on the rate of buccal mucosal ulcer healing and the apoptotic processes in rats subjected to intragastric administration of aspirin. METHODS: Groups of rats with experimentally induced buccal mucosal ulcers were administered twice daily for 10 days with SB 203580 (5, 10, and 20 mg/kg) or vehicle followed 30 min later by concomitant administration (twice daily for 10 days) of aspirin at 20 mg/kg. The animals were killed at different periods of treatment and their mucosal tissue subjected to macroscopic assessment of ulcer healing rate, measurement of soluble tumor necrosis factor-alpha (TNF-alpha), and the assay of epithelial cell apoptosis. RESULTS: In the control group the ulcer healed by the tenth day and the rate of healing was not affected by SB 203580 administration, whereas a 54.8% reduction in the ulcer area was attained in the presence of aspirin administration. Moreover, by the tenth day, the delay in ulcer healing caused by aspirin was manifested in a 5.6-fold higher rate of apoptosis and a 5.2-fold higher level of soluble TNF-alpha. Treatment with SB 203580 produced dose-dependent reduction (59.5-74.8%) in aspirin-induced increase in the mucosal level of soluble TNF-alpha, evoked 53.2-69.7% decrease in the rate of epithelial cell apoptosis, and led to a marked reversal (51.8-73.9%) in aspirin-induced delay in ulcer healing. CONCLUSIONS: The results of our findings link the delay in buccal mucosal ulcer healing caused by aspirin ingestion to the disturbances in the p38 MAPK activation.     

Space radiation effects and microgravity

Humans in space are exposed both to space radiation and microgravity. The question whether radiation effects are modified by microgravity is an important aspect in risk estimation. No interaction is expected at the molecular level since the influence of gravity is much smaller than that of thermal motion. Influences might be expected, however, at the cellular and organ level. For example, changes in immune competence could modify the development of radiogenic cancers. There are no data so far in this area. The problem of whether intracellular repair of radiation-induced DNA lesions is changed under microgravity conditions was recently addressed in a number of space experiments. The results are reviewed; they show that repair processes are not modified by microgravity.     

Space radiation absorbed dose distribution in a human phantom.

The radiation risk to astronauts has always been based on measurements using passive thermoluminescent dosimeters (TLDs). The skin dose is converted to dose equivalent using an average radiation quality factor based on model calculations. The radiological risk estimates, however, are based on organ and tissue doses. This paper describes results from the first space flight (STS-91, 51.65 degrees inclination and approximately 380 km altitude) of a fully instrumented Alderson Rando phantom torso (with head) to relate the skin dose to organ doses. Spatial distributions of absorbed dose in 34 1-inch-thick sections measured using TLDs are described. There is about a 30% change in dose as one moves from the front to the back of the phantom body. Small active dosimeters were developed specifically to provide time-resolved measurements of absorbed dose rates and quality factors at five organ locations (brain, thyroid, heart/lung, stomach and colon) inside the phantom. Using these dosimeters, it was possible to separate the trapped-proton and the galactic cosmic radiation components of the doses. A tissue-equivalent proportional counter (TEPC) and a charged-particle directional spectrometer (CPDS) were flown next to the phantom torso to provide data on the incident internal radiation environment. Accurate models of the shielding distributions at the site of the TEPC, the CPDS and a scalable Computerized Anatomical Male (CAM) model of the phantom torso were developed. These measurements provided a comprehensive data set to map the dose distribution inside a human phantom, and to assess the accuracy and validity of radiation transport models throughout the human body. The results show that for the conditions in the International Space Station (ISS) orbit during periods near the solar minimum, the ratio of the blood-forming organ dose rate to the skin absorbed dose rate is about 80%, and the ratio of the dose equivalents is almost one. The results show that the GCR model dose-rate predictions are 20% lower than the observations. Assuming that the trapped-belt models lead to a correct orbit-averaged energy spectrum, the measurements of dose rates inside the phantom cannot be fully understood. Passive measurements using 6Li- and 7Li-based detectors on the astronauts and inside the brain and thyroid of the phantom show the presence of a significant contribution due to thermal neutrons, an area requiring additional study.     

From linked marker to gene.

An area of increasing importance in human genetics research is the strategy of 'reverse genetics' or 'positional cloning', whereby a gene associated with a genetic disease is isolated on the basis of its approximate chromosomal position. This article and the accompanying centrepage diagram describe the main features of this strategy and outline the techniques involved; they are designed to be used for teaching purposes and as a general reference for those from other fields of genetics research.     

Fine-scale recombination and adaptive radiation could be linked

The difficult reconstruction of the evolutionary history of the major surface protein gene oprF highlighted an adaptive radiation in the Pseudomonas fluorescens group. The recent work of Hao (2013) showed that partial recombination events in oprF gene occurred specifically in a P. fluorescens lineage under ecological niche segregation. So, I suggest that identification of lineage-specific fine-scale recombination may be a way to detect putative adaptive radiation in bacteria.     

Terahertz radiation induces spindle disturbances in human-hamster hybrid cells

The aim of this study was to investigate and quantify the production of spindle disturbances in A(L) cells, a human-hamster hybrid cell line, by 0.106 THz radiation (continuous wave). Monolayer cultures in petri dishes were exposed for 0.5 h to 0.106 THz radiation with power densities ranging from 0.043 mW/cm(2) to 4.3 mW/cm(2) or were kept under sham conditions (negative control) for the same period. As a positive control, 100 μg/ml of the insecticide trichlorfon, which is an aneuploidy-inducing agent, was used for an exposure period of 6 h. During exposure, the sample containers were kept at defined environmental conditions in a modified incubator as required by the cells. Based on a total of 6,365 analyzed mitotic cells, the results of two replicate experiments suggest that 0.106 THz radiation is a spindle-acting agent as predominately indicated by the appearance of spindle disturbances at the anaphase and telophase (especially lagging and non-disjunction of single chromosomes) of cell divisions. The findings in the present study do not necessarily imply disease or injury but may be important for evaluating possible underlying mechanisms.     

Caffeine enhancement of radiation killing in different strains of Saccharomyces cerevisiae.

Summary Haploid and diploid wild type strains, and three classes of radiation-sensitive mutants of Saccharomyces cerevisiae were tested for enhancement of UV-inactivation by caffeine in growth medium. In addition, the sensitizing effect of caffeine was studied in a haploid and a diploid wild type strain after gamma-irradiation. The drug sensitized the UV-irradiated cells of all strains except those reported to be only slightly UV-sensitive but highly sensitive to ionizing radiation. After gamma-irradiation, no caffeine-enhancement of killing was observed in stationary phase cells of either the haploid or the diploid strain. However, log-phase cells of both strains were partially sensitized.The results of both sets of experiments suggested that caffeine interferes with a recombinational repair occurring in cells in S or G2 phase.     

Shuttle radiation dose measurements in the International Space Station orbits.

The International Space Station (ISS) is now a reality with the start of a permanent human presence on board. Radiation presents a serious risk to the health and safety of the astronauts, and there is a clear requirement for estimating their exposures prior to and after flights. Predictions of the dose rate at times other than solar minimum or solar maximum have not been possible, because there has been no method to calculate the trapped-particle spectrum at intermediate times. Over the last few years, a tissue-equivalent proportional counter (TEPC) has been flown at a fixed mid-deck location on board the Space Shuttle in 51.65 degrees inclination flights. These flights have provided data that cover the expected changes in the dose rates due to changes in altitude and changes in solar activity from the solar minimum to the solar maximum of the current 23rd solar cycle. Based on these data, a simple function of the solar deceleration potential has been derived that can be used to predict the galactic cosmic radiation (GCR) dose rates to within +/-10%. For altitudes to be covered by the ISS, the dose rate due to the trapped particles is found to be a power-law function, rho(-2/3), of the atmospheric density, rho. This relationship can be used to predict trapped dose rates inside these spacecraft to +/-10% throughout the solar cycle. Thus, given the shielding distribution for a location inside the Space Shuttle or inside an ISS module, this approach can be used to predict the combined GCR + trapped dose rate to better than +/-15% for quiet solar conditions.     

Pyrophosphate-condensing activity linked to nucleic acid synthesis.

In some preparations of DNA dependent RNA polymerase a new enzymatic activity has been found which catalyzes the condensation of two pyrophosphate molecules, liberated in the process of RNA synthesis, to one molecule of orthophosphate and one molecule of Mg (or Mn) - chelate complex with trimetaphosphate. This activity can also cooperate with DNA-polymerase, on condition that both enzymes originate from the same cells. These results point to two general conclusions. First, energy is conserved in the overall process of nucleic acid synthesis and turnover, so that the process does not require an energy influx from the cell's general resources. Second, the synthesis of nucleic acids is catalyzed by a complex enzyme system which contains at least two separate enzymes, one responsible for nucleic acid polymerization and the other for energy conservation via pyrophosphate condensation.