Effects of nitrogen dioxide and tobacco smoke on retention of inhaled bacteria.
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Biomedical subjects
Publications and source records attributed to R Ehrlich.
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The effects of moisture and oxygen concentration on germination of Bacillus cereus and B. subtilis var. niger spores were investigated in a simulated Martian environment. Less moisture was required for germination than for vegetative growth of both organisms. A daily freeze-thaw cycle lowered moisture requirements for spore germination and vegetative growth of both organisms, as compared with a constant 35 C environment. Oxygen had a synergistic effect by lowing the moisture requirements for vegetative growth, and possibly germination, of both organisms. Oxygen was not required for spore germination of either organism, but was required for vegetative growth of B. subtilis and for sporulation of both organisms.
Data obtained from Mariner IV indicate that the barometric pressure on Mars is considerably lower than previously estimated. Current estimates from Mariner IV indicate a range from 4 to 7 mb and by near infrared spectroscopy 33-56 mb. Inasmuch as the pressure has a marked influence on availability of water, this should affect the existence of Martian life. At the maximum temperatures recorded on Mars, namely 25 degrees C, a barometric pressure of 30 mb is required for the retention of free water. The lower pressure, 4 mb, would suggest that the moisture is present as a vapor above the freezing point and consequently it is not available for utilizing by living cells. The lower estimates of barometric pressure also inversely affect the carbon dioxide concentration in the Martian atmosphere. Our previous studies have demonstrated that spores of Bacillus cereus survive, germinate and grow in a simulated Martian environment (2.4% CO2, 98 mb) supplemented with moisture. The studies described in this paper were designed to determine the effect of low barometric pressures (10 to 98 mb Hg) and high concentrations of carbon dioxide (37 to 100%) in the simulated Martian environment on survival and growth of B cereus. The organism was inoculated into a felsite-limonite soil at 8% moisture level. The temperature cycles used were 8 hr at -65 degrees C and 16 hr at 25 degrees C, or 20 hr at -65 degrees C and 4 hr at 25 degrees C. The data suggest that the organism after achieving maximum growth in the simulated Martian environment (2.4% CO2, 98 mb) immediately enters into the growth phase upon reinoculation into fresh soil. These data reflect upon the possibility of contamination through air movements. Based upon currently available Martian environmental data, the probability of contamination of Mars by terrestrial micro-organisms will be discussed.
Quantitative studies were conducted to evaluate the efficiency of the slit sampler in collecting airborne Serratia marcescens and Bacillus subtilis var. niger, and to compare it with the collecting efficiency of the all-glass impinger AGI-30. The slit sampler was approximately 50% less efficient than the AGI-30. This ratio remained the same whether liquid or dry cultures were disseminated when the sample was taken at 2 min of aerosol cloud life. At 30 min of aerosol cloud life, this ratio was approximately 30% for B. subtilis var. niger. S. marcescens recoveries by the slit sampler were, however, only 17% lower than the AGI-30 at 30 min of cloud age, indicating a possible interaction involving the more labile vegetative cells, aerosol age, and method of collection.
Experimental data are presented which demonstrate that the complement-fixing antibody response in individual mice can be used for quantitative assay of Coxiella burnetii. The method allows the replacement of a single guinea pig with a single mouse, thus resulting in considerable savings in caging requirements and animal costs.
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Studies conducted in our laboratory have established that a number of potential soil microbes could survive a simulated Martian environment. In view of the uncertainty of the Martian environment and the importance of noncontamination of extraterrestrial bodies, studies were performed with common soil microbes to determine the minimal environment necessary to produce a complete growth cycle. The effects of diurnal temperature cycling (+25 degrees C to -65 degrees C) and of limiting concentrations of moisture and oxygen on spore germination, vegetative growth and sporulation of Bacillus cereus and B. subtilis have been determined. The results indicated that diurnally temperature-cycled heat-shocked spores of B. cereus in the simulated Martian atmosphere: 1) survived when the moisture concentration was < or = 4%; 2) germinated but became nonviable when the moisture concentration was > 4 < 8%; 3) germinated with subsequent vegetative growth when a) the moisture concentration was > or = 8%, and b) the concentration was > or = 6% and the partial pressure of oxygen was 15 mm; 4) sporulated when the moisture concentration was > or = 6% and the partial pressure of oxygen was 15 mm. Similar data for heat-shocked spores of B. subtilis in the simulated Martian atmosphere, diurnally temperature-cycled, indicated that the spores: 1) survived when the moisture concentration was > or = 6%; 2) germinated but became nonviable when the moisture concentration was > 1 < 4%; 3) germinated with subsequent vegetative growth when the moisture concentration was > or = 8%; 4) sporulated when the moisture concentration was > or = 6% and the partial pressure of oxygen was > or = 10 mm. Preliminary studies with B. cereus and B. subtilis spores produced in the simulated Martian environment and reintroduced into this environment indicated that vegetative cell growth and sporulation were normal. These data are discussed with regard to the probability of contamination of extraterrestrial bodies.