O melanoma cutâneo maligno é uma lesão neoplásica originada nos melanócitos epidérmicos, sendo altamente invasiva e agressiva, com elevada taxa de mortalidade, cuja incidência vem aumentando nos últimos anos. O tratamento do melanoma é cirúrgico e os pacientes com metástase podem receber quimioterapia com cisplatina que ao formarem adutos com o DNA alteram o processo de replicação da célula cancerosa. Sugere-se que os sistemas de reparo do DNA tenham um papel importante na etiologia do melanoma (reparo deficiente) e no tratamento do mesmo (eficiente eliminação dos adutos). A identificação prévia da resposta dos pacientes com melanoma ao tratamento com cisplatina pode ser um indicador biológico importante na clínica oncológica. O presente trabalho teve como objetivo, a partir de linfócitos de sangue periférico de pacientes com melanoma e de controles, avaliar o dano no DNA antes e após a adição, in vitro, de cisplatina (10?M, 100?M e 250?M), além de estimar a capacidade de reparo do DNA, após a retirada da droga (1h, 2,5h e 5h). Foram utilizados os testes do micronúcleo (MN - dano basal) e do Cometa (dano basal, ação da cisplatina e reparo do DNA). A análise citogenética foi possível em 20 pacientes com melanoma (10 homens e 10 mulheres, média de 50,6 ± 5,9 anos) e 19 controles (9 homens e 10 mulheres, média de 49,9 ± 5,5 anos) que também responderam a um questionário sobre hábitos e tipos de exposição a fatores de risco ao melanoma. A frequência do dano basal pelo teste do MN e do Cometa em linfócitos de pacientes (MN = 1,2 ± 1,2 e Cometa = 59,3 ± 62,5) foi praticamente o dobro da observada nos controles (MN = 0,6 ± 1,0 e Cometa = 35,3 ± 18,6) embora a diferença entre os grupos, em ambos os testes, não tenha sido considerada estatisticamente significante (p=0,23 e p=0,85, respectivamente). O tratamento in vitro com cisplatina, em comparação com o dano basal, aumentou a frequência de Cometas nas três concentrações estudadas (10?M, 100?M e 250?M) tanto para os pacientes (65,50 ± 50,06, 72,74 ± 50,89 e 77,26 ± 44,16) quanto para os controles (66,53 ± 49,85, 66,53 ± 26,33 e 81,74 ± 43,12) diferença esta considerada significante somente para o grupo controle, nas três concentrações avaliadas (p=0,0175, p=0,0002, e p=0,0002, respectivamente). Quanto aos diferentes tempos de reparo (1h, 2,5h e 5h), após a retirada de cisplatina nas diferentes concentrações estudadas, verificou-se aumento na frequência média de Cometas tanto para os pacientes com melanoma (93,88 ± 33,7, 101,75 ± 35,7 e 99,31 ± 32,30) quanto para os controles (92,45 ± 38,4, 100,82± 38,8 e 100,81± 31,7), diferença que foi estatisticamente significante quando comparada ao dano basal observado nos pacientes (p<0,001) e nos controles (p<0,001). Resultados semelhantes foram observados quando comparados em conjunto os escores dos tempos de reparo com o escore obtido após tratamento com cisplatina nos pacientes (71,09 ± 48,2; p<=0,005) e nos controles (71,59 ± 40,5; p<=0,005). Os resultados obtidos parecem indicar um padrão de resposta semelhante em relação à cisplatina e ao reparo do DNA nos dois grupos de indivíduos avaliados. O período de incubação das células, após a retirada da cisplatina, bem como o número de indivíduos avaliados podem ter influenciado nos resultados obtidos. Por outro lado, a resposta observada nos linfócitos in vitro, pode não ser representativa do efeito in vivo da célula tumoral. Entretanto, a identificação de marcadores de resposta a tratamentos com quimioterápicos, a partir de linfócitos de sangue periférico pode ser uma estratégia de pesquisa importante na prática clínica, inclusive para o melanoma. / Cutaneous melanoma is a malignant tumor originated from epidermal melanocytes, highly invasive and aggressive, with high mortality, and incidence that has been increasing over the years. The treatment for melanoma is surgery and patients with metastasis may receive chemotherapy with cisplatin, that results in DNA adducts that alters the replication process in cancer cells. It is suggested that the DNA repair systems have an important role in the etiology of melanoma (risk due to deficient repair) and treatment efficiency (removal of DNA adducts can decrease the treatment results). The prior identification of the response of melanoma patients to treatment with cisplatin may be an important biological marker in clinical oncology. The aim of this study was to assess, in peripheral blood lymphocytes from melanoma patients and controls, the DNA damage before and after the addition of cisplatin (10?M, 100?M and 250?M), in vitro, and estimate the capacity of DNA repair after drug removal (1h, 2.5h and 5h). The micronucleus test (MN - basal DNA damage) and the Comet assay (basal DNA damage, action of cisplatin and DNA repair) were used for the evaluation. Cytogenetic analysis was performed in 20 melanoma patients (10 men and 10 women, average age 50.6 ± 5.9 years old) and 19 controls (9 men and 10 women, average age 49.9 ± 5.5 years old) who also answered a questionnaire on habits and types of exposure to risk factors for melanoma. The frequency of basal DNA damage by the MN test and the Comet assay in lymphocytes from patients (MN = 1.2 ± 1.2 and Comet = 59.3 ± 62.5) was nearly twice the observed in controls (MN = 0, 6 ± 1.0 and Comet = 35.3 ± 18.6), although the difference between the groups in both tests was not considered statistically significant (p = 0.23 and p = 0.85, respectively). The in vitro treatment with cisplatin, compared with the basal DNA damage, increased the frequency of Comets in the three studied concentrations (10?M, 100?M and 250?M) for patients (65.50 ± 50.06, 72.74 ± 50.89 and 77.26 ± 44.16) and for the controls (66.53 ± 49.85, 66.53 ± 26.33 and 81.74 ± 43.12) and the difference was statistically significant only for the control group, for all cisplatin concentrations (p = 0.0175, p = 0.0002 and p = 0.0002, respectively). Considering the different repair times (1h, 2.5h and 5h), after removal of cisplatin at different concentrations, there was an increase in the mean frequency of Comets for both melanoma patients (93.88 ± 33.7, 101.75 ± 35.7 and 99.31 ± 32.30) and for the controls (92.45 ± 38.4, 100.82 ± 38.8 and 100.81 ± 31.7), and the difference was statistically significant when the repair Comet score was compared to the basal DNA damage observed in patients (p <0.001) and controls (p <0.001). Similar results were observed when the Comet scores of repair times were compared to the Comet scores obtained after treatment with cisplatin in patients (71.09 ± 48.2, p <= 0.005) and controls (71.59 ± 40.5, p <= 0.005). The results seem to indicate a similar pattern of response to cisplatin and DNA repair in both groups of subjects evaluated. The period of incubation of the cells after cisplatin removal and the number of individuals studied may have influenced the results. The lymphocytes\' response, in vitro, to cisplatin may not be representative of the in vivo effect of tumor cell. However, the identification of markers of response to treatment with chemotherapy from peripheral blood lymphocytes may be an important research strategy in clinical practice, including melanoma.

Devido às características especiais as nanopartículas (10-9m) estão sendo utilizadas em uma ampla gama de produtos, porém é conhecido que a utilização dessas partículas podem causar efeitos biológicos adversos, aumentando a preocupação em relação à saúde e ao meio ambiente. Recentemente, as nanopartículas de prata (AgNPs) têm sido alvo de estudos genotóxicos e citotóxicos, sendo que ainda não existe um consenso acerca da relação entre tamanho e toxicidade dessas partículas. Assim, este trabalho avaliou a citotoxicidade e a genotoxicidade das AgNPs de 10 e 100 nm nas linhagens celulares CHO-K1 e CHO-XRS5, por meio do Ensaios de Viabilidade Celular, Sobrevivência Clonogênica, Teste do Micronúcleo, o Ensaio Cometa e Cinética do Ciclo Celular por Citometria de Fluxo. Em todos os ensaios, as células foram expostas por 24 h à diferentes concentrações de AgNPs (0,025 a 5,0 g/ml) e, as células não tratadas foram utilizadas como controle negativo. A concentração de 5,0 g/ml foi citotóxica nos ensaios de Viabilidade Celular e Sobrevivência Clonogênica, sendo excluída dos ensaios de genotoxicidade. De maneira geral, as células CHO-XRS5 apresentaram menor viabilidade e maior quantidade de danos no DNA do que as células CHO-K1. As AgNPs de 10 nm causaram maiores níveis de danos no DNA em ambas as linhagens e um aumento de células em subG1 logo após o tratamento na linhagem CHO-K1. Entretanto, no tempos 24 e 72 h após o tratamento foi verificada a maior toxicidade (células em subG1) das AgNPs de 100 nm quando comparadas com suas homólogas menores (10 nm). Assim, foi observado que as AgNPs de 10 nm apresentam efeito tóxico a curto prazo similar ou maior do que a mesma concentração de partículas de 100 nm. No entanto, os efeitos genotóxicos e citotóxicos de longo prazo das AgNPs de 100 nm foram maiores do que os da partículas de 10 nm para ambas as linhagens celulares, comprovando que a exposição às AgNPs maiores (100 nm) pode causar mais efeitos biológicos adversos do que suas homólogas menores (10 nm). / Due to their particular characteristics, nanoparticles (10-9m) are being used in a range of products. However, these particles can cause adverse biological effects and because of that, there is a great concern about the health and environmental risks related to the use of these particles. Recently, silver nanoparticles (AgNPs) have been used in a variety of cytotoxicity and genotoxicity studies, but there are still controversies regarding the association between the size and the toxicity of these particles. Thus, in this study, we aimed to evaluate the cytotoxicity and genotoxicity of AgNPS (10 and 100 nm) in two different cell lines, CHO-K1 and CHO-XRS5, by performing Cell Viability assay (XTT), Clonogenic assay, Micronucleus test, Comet assay, as well as by investigating the Cell Cycle kinetics using the flow cytometry. For all the different assays, the cell cultures were exposed for 24 hours to different concentrations of AgNPs (0.025 to 5.0 g/ml) and the untreated cells were used as the negative controls. Since results from the Viability and Clonogenic assays indicated that the concentration of 5.0 g/ml was cytotoxic for both cell lines, this concentration was not included in the genotoxic assays. Our results indicated that the CHO-XRS5 cells presented a lower viability and higher levels of DNA damage compared to the CHO-K1 cells. The 10 nm-AgNPs induced greater levels of DNA damage than the 100 nm-particles in both cell lines and the former also led to a subG1 arrest soon after the treatment only in the CHO-K1 cell line. In contrast, results from all the other assays indicated that greater levels of toxicity were induced by the 100 nm-AgNPs when compared to the 10 nm-particles, both 24 and 72 h after the treatment. Thus, at the same concentration, the short-term effects of the 10 nm-AgNPs were equal to or more toxic than those of the 100 nm-particles. Nevertheless, both long-term genotoxicity and cytotoxicity induced by the 100 nm-AgNPs were greater than those induced by the 10 nm-particles for both cell lines, which suggests that the exposure to greater size particles (100 nm) can cause more adverse biological effects than the exposure to the smaller particles(10 nm).

Comets are the most active around their perigees. The increased outgassing can lead to a coma thick enough to effectively absorb the solar EUV radiation, which engenders a self-shielding comet nucleus and inner layers of the ionosphere. This effect of self-shielding can be calculated by the attenuation of the sunlight according to the Beer-Lambert law. Here we focus on the perihelion of comet 67P/Churyumov-Gerasimenko, the target comet of the ESA Rosetta mission. We calculate attenuated photoionization frequencies and implement these into an ionospheric model constructed in a recent project work (by the same author). The ionization frequencies and ion number densities are calculated as a function of cometocentric distance and compared with the latest published peer-reviewed article by Heritier et al. (2017). Overall, the agreement is fairly good. The most significant difference is the discrepancy of number densities of O2 ions, which is higher in our model by nearly an order of magnitude. This discrepancy is attributed to the fact that Heritier et al (2017) only considered charge transfer processes for the formation of O2+, while we identify photoionization of O2 as the main production mechanism.

The ESA Rosetta spacecraft investigated comet 67P/Churyumov-Gerasimenko duringtwo years from August 2014 to the end of September 2016. The dual Langmuir probewas used to measure plasma parameters including the thermal energy of theelectrons. The observed thermal energy (or temperature) of the electrons was ratherhigh, in the range 5-10 eV almost throughout the mission. However, near perihelionthe Langmuir probe measurements indicated the prevalence of two electronpopulations with distinct temperatures, one hot (5-10 eV) and one cold (less than 1eV). It has been hypothesized that the electrons of the colder population wereformed relatively close to the nucleus and that they subsequently cooled by inelasticcollisions with the neutral gas. In this project work we develop a model for studyingelectron cooling in a cometary coma. The model takes into account collisions withwater molecules as well as the influence of a radial ambipolar electric field. / Rymdsonden Rosetta från ESA undersökte kometen 67P/Churyumov Gerasimenkounder mer än två år, från augusti 2014 till slutet av september 2016.En Langumirprob användes för att undersökta plasmamiljön runt kometen, tillexempel elektronernas termiska energi. Den observerade termiska energin förelektronerna (eller elektrontemperaturen) var ganska hög, ca 5-10 eV undernästan hela uppdraget, men när kometen var nära perihelium detekterade instrumentenäven kalla elektroner, med en energi under 1 eV, distinkta från devarma. En hypotes är att dessa kalla elektroner bildas nära kärnan av att varmaelektroner genomgår inelastiska kollisioner med den neutrala gasen och tapparsin energi. I detta projekt utvecklar vi en modell för att studera elektronernasbeteende i koman. Modellen tar hänsyn till kollisioner med neutrala vattenmolekylersåväl som påverkan av ett radiellt ambipolärt elektriskt fält.

Background: Oxidative damage is one of the most frequent types of cell components damage leading to oxidation of lipids, proteins and the molecule of DNA. As a consequence, there is a higher occurrence of several pathologies such as atherosclerosis, neurodegenerative diseases, cancer; or diabetes. In our study, influence of whole body anesthesia during minor surgery on the level of DNA damage was examined using comet assay technique. Methods: The basic principle of this method is fixing the cells (lymphocytes) in agarose, their lysis for the removal of membranes, incubation with the specific enzymes and electrophoresis of the released cell nuclei. During the electrophoresis, free low-molecular weight and negatively charged fragments of DNA move towards anode which causes the formation of the typical comet cell shape. Finally, the gels are stained by ethidium bromide (DNA intercalating dye) and visualized. Results: We have observed single strand breakages (SSBs) and, with the use of modified assay using specific enzymes for detection of specific lesions, also oxidized purines and pyrimidines. The extent of DNA damage as determined by the intensity of the tail of the comet was quantified using LUCIA Comet Assay (Laboratory Imaging, Czech Republic) software for image analysis. The results were used...

Background: The human organism is exposed daily to many endogenous and exogenous substances that are the source of oxidative damage. Cell structures, including DNA (deoxyribonucleic acid) in the nucleus are damaged due to high concentrations of these substances and accumulation of oxidative stress in cells. The predominance of these damaging processes may later be responsible for human diseases such as cancer, neurodegenerative diseases or heart failure. In our study, we observed oxidative damage at the DNA level due to spinal anesthesia. Methods: Sample processing was performed by comet analysis. The principle consists in fixation of cells (lymphocytes) in the agarose gel, lysis of cell structures for nucleotide release, incubation with specific enzymes and exposure to electrophoresis. Damaged, negatively charged parts of the DNA in the electric field are directed to the positive charged anode, creating a typical comet shape. For visualization, the gels were stained with ethidium bromide (DNA intercalating dye). Results: We have quantified single-strand breaks, oxidized purines and pyrimidines (use of enzymes to detect specific damages). The results are reported in percentage of DNA in the comet's tail. The principle is to compare the intensity of the comet's tail with the total comet intensity....

The joint European Space Agency and Japan Aerospace Exploration Agency mission Comet Interceptor seeks to perform a flyby of a Small Solar System Body (SSSB), through use of a multi-element spacecraft. It comprises a primary spacecraft and two subspacecraft, the latter of which will encounter the intercepted object at a small enough distance that its end-of-life might occur at an impact of either the object itself or its potential coma. The Optical Periscopic Imager for Comets (OPIC) is an instrument implemented on one of these small probes which will generate monochromatic images during the encounter. Given a limited data budget before the possible impact, there is a need for data prioritization to ensure that only the most scientifically relevant data is collected. To enable this, algorithms for autonomously cropping an object nucleus from an image were developed during this thesis work. As the computational capabilities of OPIC are limited, the algorithms were required to be of low computational complexity. Additionally, given that the close environment of SSSB in general and comets in particular often exhibit considerable quantities of gas and dust which can generate cluttering in images, the algorithms developed were required to be resistant to noise. Three image cropping algorithms were developed with varying computational complexities. These were tested for cropping accuracy and relative execution times on data from both previous space missions as well as simulated photorealistic images. All three algorithms were able to properly find a bounding box of an object nucleus and any of its significant plumes. The accuracy in cropping correctness of the region borders generated increased with the computational complexity of the algorithms.

Cette thèse porte sur l’étude expérimentale et théorique de quatre instabilités associées à l’émergence de motifs réguliers sur des substrats érodables ou fortement déformables,instabilités liées à l’hydrodynamique sur un relief modulé.La première partie porte sur l’étude de l’instabilité d’une plaque élastique fixée aux deux bouts et soumise à un écoulement fluide permanent. La solution plane est instable vis-à-vis d’ondes propagatives, lorsque l’écoulement est suffisamment fort. La sélection de fréquence et de longueur d’onde est caractérisée expérimentalement en fonction de la vitesse de l’écoulement. Ces quantités suivent remarquablement les lois d’échelle obtenues par l’analyse de stabilité linéaire du problème. Le principe de l’expérience pourrait être appliqué à la récupération d’énergie.La deuxième partie porte sur une analyse théorique de la formation de rides géantes sur la comète 67P, récemment observées par la sonde Rosetta. Nous montrons comment le dégazage de vapeur se produit au travers d’une couche poreuse granulaire superficielle et comment l’alternance jour/nuit conduit à des gradients de pression gigantesques qui engendrent des vents thermiques de surface. Ces motifs apparaissent comme étant les analogues de rides qui se forment à la surface de lit sableux dans un écoulement visqueux.L’analyse de stabilité linéaire du problème permet de prédire quantitativement l’émergence de ces rides à la longueur d’onde et à la vitesse de propagation observées. Cette description fournit un outil robuste et fiable pour décrire les processus d’érosion et d’accrétion dans l’évolution des petits corps.Dans la troisième partie, nous proposons un modèle pour l’apparition de motifs de sublimation sur Pluton, tels que ceux observés sur Sputnik Planum. La formation et l’évolution de ces motifs proviennent de la sublimation/condensation différentielle de la glace d’azote.Nous montrons que l’atmosphère de Pluton possède des propriétés (température et pression)peu variables en espace et en temps. Nous analysons les différents mécanismes d’instabilité en compétition et concluons à un mécanisme original, basé sur le mélange et e transport de chaleur dans l’atmosphère, plutôt qu’au mécanisme des pénitents, basé sur l’auto-éclairement de la surface de glace.Enfin, nous avons étudié théoriquement l’instabilité de formation des rides éoliennes en considérant les trajectoires des grains résonantes avec le relief. Cette modélisation prend en compte de manière simple et effective les effets collectifs du transport de sédiments. Le modèle est validé à partir de simulations numériques existantes, elles mêmes calées sur des expériences contrôlées. / This thesis is devoted to the experimental and theoretical investigations of four instabilitiesassociated with the emergence of regular patterns over erodible/flexible substrates, andrelated to hydrodynamics over a modulated relief.First, the instability of a flexible sheet clamped at both ends and submitted to a permanentwind is investigated. The flat sheet solution is unstable towards propagative waves, forstrong enough wind. We experimentally study the selection of frequency and wavenumberas a function of the wind velocity. These quantities obey simple scaling laws derived froma linear stability analysis of the problem. This phenomenon may be applied for energyharvesting.Second, an explanation is proposed for the giant ripples observed by spacecraft Rosettaat the surface of the comet 67P. We show that the outgassing flow across a porous surfacegranular layer and the strong pressure gradient associated with the day-night alternanceare responsible for thermal superficial winds. We show that these unexpected patterns areanalogous to ripples emerging on granular beds submitted to viscous shear flows. Linearstability analysis of the problem quantitatively predicts the emergence of bedforms at theobserved wavelength and their propagation. This description provides a reliable tool topredict the erosion and accretion processes controlling the evolution of small solar systembodies.Third, we propose a model for rhythmic, dune-like patterns observed on SputnikPlanum of Pluto. Their emergence and evolution are related to the differential condensation/sublimation of nitrogen ice. We show that the temperature and pressure in Pluto’satmosphere are almost homogeneous and steady, and that heat flux from the atmospheredue to convection and turbulent mixing is responsible for the emergence of these sublimationpatterns, in contrast to the penitentes instability due to solar radiation.Last, we report an analytical model for the aeolian ripple instability by considering theresonant grain trajectories over a modulated sand bed, taking the collective effect in thetransport layer into account. The model is tested against existing numerical simulationsthat match experimental observations.

The plasma environment of an active comet provides a unique setting for plasma physics research. The complex interaction of newly created cometary ions with the flowing plasma of the solar wind gives rise to a plethora of plasma physics phenomena, that can be studied over a large range of activity levels as the distance to the sun, and hence the influx of solar energy, varies. In this thesis, we have used measurements of the spacecraft potential by the Rosetta Langmuir probe instrument (LAP) to study the evolution of activity of comet 67P/Churyumov-Gerasimenko as it approached the sun from 3.6 AU in August 2014 to 2.1 AU in March 2015. The measurements are validated by cross-calibration to a fully independent measurement by an electrostatic analyzer, the Ion Composition Analyzer (ICA), also on board Rosetta. The spacecraft was found to be predominantly negatively charged during the time covered by our investigation, driven so by a rather high electron temperature of ~5 eV resulting from the low collision rate between electrons and the tenuous neutral gas. The spacecraft potential exhibited a clear covariation with the neutral density as measured by the ROSINA Comet Pressure Sensor (COPS) on board Rosetta. As the spacecraft potential depends on plasma density and electron temperature, this shows that the neutral gas and the plasma are closely coupled. The neutral density and negative spacecraft potential were higher in the northern hemisphere, which experienced summer conditions during the investigated period due to the nucleus spin axis being tilted toward the sun. In this hemisphere, we found a clear variation of spacecraft potential with comet longitude, exactly as seen for the neutral gas, with coincident peaks in neutral density and spacecraft potential magnitude roughly every 6 h, when sunlit parts of the neck region of the bi- lobed nucleus were in view of the spacecraft. The plasma density was estimated to have increased during the investigated time period by a factor of 8-12 in the northern hemisphere and possibly as much as a factor of 20-44 in the southern hemisphere, due to the combined effects of seasonal changes and decreasing heliocentric distance. The spacecraft potential measurements obtained by LAP generally exhibited good correlation with the estimates from ICA, confirming the accuracy of both of these instruments for measurements of the spacecraft potential. / <p>QC 20200602</p>

Shisha-Tabak benötigt im Vergleich zur Zigarette höhere Konzentrationen des Feuchthaltemittels Glycerin. Seit Mai 2016 ist die bis dahin gültige Limitierung von Feuchthaltemitteln in Tabak auf 5 % aufgehoben. Derzeit ist das toxikologische Profil des Glycerins jedoch noch nicht hinreichend erforscht. Ziel dieser Arbeit war es, Glycerin auf mögliche zyto- und genotoxische Effekte zu untersuchen, um so das Gefährdungspotenzial durch Glycerin im Shisha-Tabak zu beurteilen und die tabakkontrollpolitische Situation in Deutschland zu diskutieren. Dafür wurden Lymphozyten sowie Nasenschleimhautzellen von 10 Patienten für eine Stunde Glycerin (0,001 mol/l bis 6,0 mol/l) exponiert. Durch den Trypanblau-Ausschlusstest wurden die Zellen auf Zytotoxizität, mittels Einzelzellgelelektrophorese (Comet Assay) und Mikrokern-Test auf Genotoxizität untersucht. Im Trypanblau-Ausschlusstest traten bei Lymphozyten sowie nasalen Mukosazellen signifikante Vitalitätsabfälle ab Glycerin-Konzentrationen von 1,0 mol/l auf. Im Comet Assay konnten für beide Zellgruppen signifikante Unterschiede des Olive Tail Moments (OTM) ab 1,0 mol/l nachgewiesen werden. Beim Mikrokern-Test zeigten sich keine signifikanten Zunahmen der Mikrokern-Anzahl. Es konnten zyto- und genotoxische Effekte ab Konzentrationen von 1,0 mol/l nachgewiesen werden. Dies überschreitet die reale Glycerin-Belastung im Hauptstromrauch der Shisha jedoch deutlich. Dennoch handelt es sich bei Genotoxizität um ein stochastisches Risiko. Ebenso sind toxische Effekte, beispielsweise durch Erhitzung, bereits bei geringeren Konzentrationen denkbar. Für eine umfangreichere Beurteilung von Feuchthaltemitteln im Shisha-Tabak sind weitere Untersuchungen indiziert. Darüber hinaus besteht enormer Handlungsbedarf zur weiteren Einführung tabakkontrollpolitischer Maßnahmen in Deutschland. / Shisha tobacco has a higher amount of glycerol than cigarette tobacco. Moreover, new legislation in Germany cancels the old limitation of humectants in shisha tobacco. Although higher amounts of glycerol in tobacco are expected, the knowledge of the toxicological profile of glycerol regarding human cells is incomplete. Aim of the study was to test glycerol for cytotoxic and genotoxic effects and to discuss the risk of humectants in shisha tobacco and the situation of German tobacco control. Lymphocytes and nasal mucosa cells of 10 patients were exposed to different glycerol levels (0.001 mol/l to 6.0 mol/l). Cytotoxic effects were examined by trypan blue exclusion test, genotoxic effects by comet assay and micronucleus test. The trypan blue exclusion test revealed significant cytotoxic effects on lymphocytes and nasal mucosa cells for glycerol concentrations of 1.0 mol/l and higher. In the comet assay a significant DNA damage could be shown for glycerol levels of 1.0 mol/l and higher. No significant micronucleus formation was monitored. While the geno- and cytotoxicity were seen in concentrations of glycerol clearly exceeding the concentrations in main stream smoke of shishas, genotoxicity is a stochastic risk occurring even at subtoxic levels. Furthermore, toxicity in lower levels could result from tobacco combustion or interactions with other smoke components. For an extensive evaluation of the risks of humectants in shisha tobacco further studies are needed. In addition, there is an enormous need for introducing further measures of tobacco control policy in Germany.