Action of light on Micrococcus roseus

1974 ◽  
Vol 20 (7) ◽  
pp. 1015-1021 ◽  
Author(s):  
E. H. Schwartzel ◽  
J. J. Cooney

Micrococcus roseus is killed by exposure to a continuous spectrum of white light (3000 ft-c (32 292 lm/m2)) in the presence of air and the dye, toluidine blue. Comparison of rates of photodynamic killing for log and stationary phase cells and for two pigmentation mutants indicated that photosensitivity could not be correlated with amount of carotenoid or with carotenoid-chromophore length. Moreover, cells grown in medium containing diphenylamine (DPA) did not contain significant quantities of colored carotenoids; they were not as sensitive to photodynamic killing as fully pigmented cells. Photodynamic killing was accompanied by selective release of magnesium and calcium and by release of UV-absorbing material. In the absence of added photosensitizer, M. roseus, the two mutants, or DPA-inhibited cells were not killed when exposed to white light at intensities as high as 22 000 ft-c (236 806 lm/m2) for as long as 9 h, and cells did not release UV-absorbing material. Under these conditions M. roseus and the yellow mutant did not release as much magnesium or calcium as when subjected to photodynamic killing, but DPA-grown cells leaked sodium, magnesium, and calcium. These observations are consistent with several suggestions: (i) carotenoids do not serve as photochemical buffers in M. roseus; (ii) growth in medium containing DPA or mutations leading to altered pigmentation change membrane organization leading to altered photosensitivity; (iii) M. roseus has an efficient repair mechanism which renders it resistant to photodynamic killing unless an exogenous photosensitizer is present.


Solar Physics ◽  
1982 ◽  
Vol 80 (1) ◽  
pp. 113-127 ◽  
Author(s):  
Eijiro Hiei




1966 ◽  
Vol 12 (4) ◽  
pp. 691-698 ◽  
Author(s):  
O. C. Thierry ◽  
J. J. Cooney

Growth of and carotenoid synthesis by Micrococcus roseus are optimum at pH 6.8 and pH 7.5 in a defined medium. Maximum growth and pigment content were obtained in aerobic cultures at 25 C. Supplementing the medium with more than 0.2% NaCl resulted in less growth and decreased pigment content per unit mass of cells. At pH 7.5 the absence of visible light had no effect on growth or pigment content, but at pH 6.8 both were decreased in dark-grown cultures. Biotin did not reverse inhibition of growth in the dark. Dark inhibition was reversed by exposure of lag or early log phase cultures to visible light for 30 min, but late log or stationary phase cultures grown in the dark did not respond. Stationary phase dark-grown cultures resumed growth and pigment synthesis during a 24-h period in light. Serial culture in the dark did not result in a further decrease in growth or pigment synthesis; and when cells from serial cultures grown in darkness were used as inoculum for cultures grown in the light, maximum growth and pigment synthesis occurred. These data suggest that light is required for induction of maximum growth and pigment synthesis. A crude action spectrum was determined and suggests that light in the range from 625 to 700 mμ may be responsible for photoinduction.None of the environmental variations altered the absorption spectrum of pigment extracts. Conditions which were optimum for growth were also optimum for pigment synthesis.



2006 ◽  
Vol 72 (6) ◽  
pp. 4436-4439 ◽  
Author(s):  
Val�rie Decraene ◽  
Jonathan Pratten ◽  
Michael Wilson

ABSTRACT Simple methods of reducing the microbial load on surfaces in hospitals are needed to reduce the risk of hospital-associated infections. Here we report on the ability of a cellulose acetate coating containing the photosensitizers toluidine blue and rose bengal to kill microbes (Staphylococcus aureus, Escherichia coli, Clostridium difficile, a bacteriophage, and Candida albicans) on its surface when illuminated with white light.



2016 ◽  
Vol 4 (12) ◽  
pp. 2199-2207 ◽  
Author(s):  
Gi Byoung Hwang ◽  
Sacha Noimark ◽  
Kristopher Page ◽  
Sandeep Sehmi ◽  
Alexander J. Macrobert ◽  
...  

Toluidine blue O (TBO) dye together with either silver (Ag) nanoparticles (NPs), gold (Au) NPs, or a mixture of Ag and Au NPs (Mix Ag–Au NPs) were incorporated into polyurethane to make antimicrobial surfaces using a swell-encapsulation-shrink process.



Genetics ◽  
1979 ◽  
Vol 93 (1) ◽  
pp. 81-103
Author(s):  
M Heude ◽  
E Moustacchi

ABSTRACT Three main features regarding the loss of mitochondrial genetic markers among rhomutants induced by ultraviolet irradiation are reported: (a) the frequency of loss of six loci examined increases with UV dose; (b) preferential loss of one region of the mitochondrial genome observed in spontaneous rho-mutants is enhanced by UV; and (c) the loss of each marker results from large deletions. Marker loss in rho-mutants was also investigated under conditions that modulate rho-induction. Liquid holding of irradiated exponential or stationary phase cells, as well as a split-dose regime applied to stationary phase cells, results in rho-mutants in which the loss of markers is correlated with rho-induction: the more sensitive the cells are to rho-induction, the more frequent are the marker losses among rho-clones derived from these cells. This correlation is not found in exponential-phase cells submitted to a split-dose treatment, suggesting that a different mechanism is involved in the latter case. It is known that UV-induced pyrimidine dimers are not excised in a controlled manner in mitochondrial DNA. How-ever, our studies indicate that an accurate repair mechanism (of the recombinational type ?) can lead to the restoration of mitochondrial genetic information in growing cells.





1967 ◽  
Vol 28 ◽  
pp. 177-206
Author(s):  
J. B. Oke ◽  
C. A. Whitney

Pecker:The topic to be considered today is the continuous spectrum of certain stars, whose variability we attribute to a pulsation of some part of their structure. Obviously, this continuous spectrum provides a test of the pulsation theory to the extent that the continuum is completely and accurately observed and that we can analyse it to infer the structure of the star producing it. The continuum is one of the two possible spectral observations; the other is the line spectrum. It is obvious that from studies of the continuum alone, we obtain no direct information on the velocity fields in the star. We obtain information only on the thermodynamic structure of the photospheric layers of these stars–the photospheric layers being defined as those from which the observed continuum directly arises. So the problems arising in a study of the continuum are of two general kinds: completeness of observation, and adequacy of diagnostic interpretation. I will make a few comments on these, then turn the meeting over to Oke and Whitney.



1994 ◽  
Vol 144 ◽  
pp. 541-547
Author(s):  
J. Sýkora ◽  
J. Rybák ◽  
P. Ambrož

AbstractHigh resolution images, obtained during July 11, 1991 total solar eclipse, allowed us to estimate the degree of solar corona polarization in the light of FeXIV 530.3 nm emission line and in the white light, as well. Very preliminary analysis reveals remarkable differences in the degree of polarization for both sets of data, particularly as for level of polarization and its distribution around the Sun’s limb.



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