Alterations in the ras oncogene and the p53 tumor suppressor gene in ultraviolet radiation-induced skin carcinogenesis

A rapid increase of the ultraviolet radiation (UVR)-related skin cancer incidence has attracted more and more public attention during the last few decades. Prevention and treatment of UVR-related skin cancer has become an important public health issue in the United States. Recent studies indicate that mutations in ras and/or p53 genes may be involved in UVR-induced skin tumor development but the precise molecular mechanism remains unclear. In this study, alterations of H-ras and p53 genes were investigated in different stages of carcinogenesis in a chronic UVR (solar simulator) exposure-induced Sencar mouse skin carcinogenesis model in order to clarify the role of the alterations of these genes during the skin carcinogenesis process and to further understand the mechanisms by which UVR causes skin cancer.^ Positive ras-p21 staining in cell membranes and cytosol were detected in 18/33 (55%) of squamous cell carcinomas (SCCs), but were not detected in UV-exposed skin, papillomas, or spindle cell tumors (SCTs). Positive staining of the malignant progression marker K13 was found in 17/33 (52%) of SCCs only. A significant positive correlation was observed between the K13 and the ras-p21 expression. Polymerase chain reaction (PCR)-based single strand conformation polymorphism (SSCP) analysis and gene sequencing analysis revealed three point mutations, one (codon 56) in UV-exposed non-tumor bearing skin and the other two (codons 21 and 13) in SCCs. No UV-specific mutation patterns were found.^ Positive p53 nuclear staining was found in 10/37 (27%) of SCCs and 12/24 (50%) of SCTs, but was not detected in normal skin or papillomas. PCR-based SSCP and sequencing analysis revealed eight point mutations in exons 5 and 6 (four in SCTs, two in SCCs, and two in UV-exposed skin) including six C-T or C-A transitions. Four of the mutations occurred at a dipyrimidine (CC) sequence. The pattern of the mutations indicated that the mutagenic lesions were induced by UVR.^ These results indicate that overexpression of ras-p21 in conjunction with aberrant expression of K13 occurred frequently in UVR-induced SCCs in Sencar mouse skin. The point mutation in the H-ras gene appeared to be a rare event in UVR skin carcinogenesis and may not be responsible for overexpression of ras-p21. UVR-induced P53 gene alteration is a frequent event in UVR-induced SCCs and later stage SCT tumors in Sencar mice skin, suggesting the p53 gene mutation plays an important role in skin tumor malignant progression. ^

Investigation of mechanisms involved in ultraviolet B radiation-induced, T cell -mediated immune suppression

Cutaneous exposure to ultraviolet-B radiation (UVR) results in the suppression of cell-mediated immune responses such as contact hypersensitivity (CHS) and delayed-type hypersensitivity (DTH). This modulation of immune responses is mediated by local or systemic mechanisms, both of which are associated with the generation of antigen-specific suppressor T lymphocytes (Ts). UV-induced Ts have been shown to be CD3+CD4+CD8 − T cells that control multiple immunological pathways. However, the precise mechanisms involved in the generation and function of these immunoregulatory cells remain unclear. We investigated the cellular basis for the generation of UV-induced Ts lymphocytes in both local and systemic models of immune suppression, and further examined the pleiotrophic function of these immunoregulatory cells. ^ We used Thy1.1 and Thy1.2 congenic mice in a draining lymph node (DLN) cell transfer model to analyze the role played by epidermal Langerhans cells in the generation of Ts cells. We demonstrate that T cells tightly adhered to antigen-presenting cells (APC) from UV-irradiated skin are the direct progenitors of UV-induced Ts lymphocytes. Our studies also reveal that UV-induced DNA-damage in the form of cyclobutyl pyrimidine dimers (CPD) in the epidermal APC is crucial for the altered maturation of these adherent T cells into Ts. ^ We used TCR transgenic mice in an adoptive transfer model and physically tracked the antigen-specific clones during immune responses in unirradiated versus UV-irradiated mice. We demonstrate that UV-induced Ts and effector TDTH cells share the same epitope specificity, indicating that both cell populations arise from the same clonal progenitors. UVR also causes profound changes in the localization and proliferation of antigen-specific T cells during an immune response. Antigen-specific T cells are not detectable in the DLNs of UV-irradiated mice after 3 days post-immunization, but are found in abundance in the spleen. In contrast, these clones continue to be found in the DLNs and spleens of normal animals several days post-immunization. Our studies also reveal that a Th2 cytokine environment is essential for the generation of Ts in UV-irradiated mice. ^ The third part of our study examined the pleiotrophic nature of UV-induced Ts. We used a model for the induction of both cellular and humoral responses to human gamma-globulin (HGG) to demonstrate that UV-induced Ts lymphocytes can suppress DTH as well as antibody responses. (Abstract shortened by UMI.) ^

Dual role of interleukin-12 on ultraviolet -induced immune suppression

Skin cancer is the most prevalent form of neoplasia, with over one million newcases diagnosed this year. UV radiation is a ubiquitous environmental agent that induces skin cancer. In addition to its carcinogenic effect, UV radiation also suppresses cell-mediated immune responses. This immune suppression is not only observed at the site of irradiation, but UV radiation also induces systemic immune suppression. Since UV radiation has a limited ability to penetrate the skin, the question of the mechanism of this systemic immune suppression arises. A number of studies have suggested that UV radiation induce systemic effects through the production of immunoregulatory cytokines, such as IL-4 and IL-10. These cytokines affect the immune response by altering systemic antigen presentation, specifically by suppressing the activation of Th1 cells while allowing the activation of Th2 cells. Because IL-12 is an important regulator of Th1 cell activation, we tested the hypothesis that administration of IL-12 could overcome UV-induced immune suppression. ^ The studies presented here are divided into dime specific aims. In the first specific aim, the ability of IL-12 to overcome UV-induced immune suppression was examined. IL-12 could overcome UV-induced immune suppression as well as prevent the generation of and neutralize the activity of preformed suppressor cells induced by UV radiation. In the second specific aim, the mechanism by which IL-12 overcomes UV-induced immune suppression was examined. IL-12 overcame UV-induced immune suppression by blocking the production of immunoregulatory cytokines such as IL-4, IL-10 and TNF-α. In the third specific aim, the effect of UV radiation on antigen presentation was investigated. UV radiation was found to decrease the production of biologically active IL-12. In addition, UV also increased the production of IL-12p40 homodimer, an antagonist of IL-12p70 heterodimer. This result suggests that IL-12 may have a dual role in the immune suppression induced by, UV radiation. On one hand the biologically active IL-12p70 heterodimer blocks UV-induced immune suppression. In contrast, IL-12p40 homodimer may mediate the suppressive effect of UV radiation. This paradox indicates that IL-12 may have a greater regulatory role in the immune response than was previously suspected. ^

Ultraviolet radiation modulates the immune system through the platelet -activating factor receptor

Ultraviolet radiation plays a critical role in the induction of non-melanoma skin cancer. UV radiation is also immune suppressive. Moreover, UV-induced systemic immune suppression is a major risk factor for skin cancer induction. Previous work had shown that UV exposure in vivo activates a cytokine cascade involving PGE2, IL-4, and IL-10 that induces immune suppression. However, the earliest molecular events that occur immediately after UV-exposure, especially those upstream of PGE2, were not well defined. To determine the initial events and mediators that lead to immune suppression after a pathological dose of UV, mouse keratinocytes were analyzed after sunlamp irradiation. It is known that UV-irradiated keratinocytes secrete the phospholipid mediator of inflammation, platelet-activating factor (PAF). Since PAF stimulates the production of immunomodulatory compounds, including PGE2, the hypothesis that UV-induced PAF activates cytokine production and initiates UV-induced immune suppression was tested. Both UV and PAF activated the transcription of cyclooxygenase (COX)-2 and IL-10 reporter gene constructs. A PAF receptor antagonist blocked UV-induced IL, 10 and COX-2 transcription. PAF mimicked the effects of UV in vivo and suppressed delayed-type hypersensitivity (DTH), and immune suppression was blocked when UV-irradiated mice were injected with a PAF receptor antagonist. This work shows that UV generates PAF-like oxidized lipids, that signal through the PAF receptor, activate cytokine transcription, and induce systemic immune suppression. ^

(Table 2) Weight percent organic carbon from ODP Site 138-847

As the length of marine cores increases and sampling intervals decrease, the need for rapid and inexpensive means of determining sediment composition has become apparent. In this study we examine one potentially useful technique for assessing compositional changes in marine cores, diffuse reflectance spectrophotometry. We examined near-ultraviolet, visible, and near-infrared reflectance spectra from five data sets. Each data set consists of calibration samples and test samples. The calibration samples' spectra were related to a sediment component using multiple linear regression. The resulting regression or calibration equations were then evaluated using the test samples. Calibration equations were written relating spectra to several sediment components incduding carbonate (Atlantic and east Pacific Rise ODP Site 847), organic carbon content (Atlantic and east Pacific Rise), and opal content (east Pacific Rise). The correlation coefficients for the regression equations ranged from a high of 0.99 for carbonate and opal at ODP Site 847 to a low of 0.97 for Atlantic carbonate indicating that spectral variations are highly correlated to sediment composition. All of the equations include a substantial number of variables from shorter visible and longer near ultraviolet wavelengths suggesting that these wavelengths are especially important for devices designed specifically to scan marine cores. Although equations for estimating organic and carbonate content appear independent of other sediment components, the opal equation is strongly dependent on carbonate content indicating that opal concentration is correlated to carbonate content. Tests of the calibration equations indicated that all our equations reasonably estimate the pattern of changes, either down core or in surface sediments. Where our spectral estimates have difficulty is with absolute values, frequently over or underestimating observed values by a substantial amount. Within these limitations diffuse reflectance spectrophotometry can be a useful tool for characterizing marine cores and as our understanding of the relationship between spectra and mineralogy improves so will estimates of absolute values.

(Table 1) Chlorophyll concentration and pigment composition of carotenoids in three heathland bryophytes, northern Sweden

Background and Aims: Anthropogenic depletion of stratospheric ozone in Arctic latitudes has resulted in an increase of ultraviolet-B radiation (UV-B) reaching the biosphere. UV-B exposure is known to reduce aboveground biomass and plant height, to increase DNA damage and cause accumulation of UV-absorbing compounds in polar plants. However, many studies on Arctic mosses tended to be inconclusive. The importance of different water availability in influencing UV-B impacts on lower plants in the Arctic has been poorly explored and might partially explain the observed wide variation of responses, given the importance of water in controlling bryophyte physiology. This study aimed to assess the long-term responses of three common sub-Arctic bryophytes to enhanced UV-B radiation (+UV-B) and to elucidate the influence of water supply on those responses. Results: Responses were species specific: H. splendens responded most to +UV-B, with reduction in both annual growth (-22%) and sporophyte production (-44%), together with increased b-carotene, violaxanthin, total chlorophyll and NPQ, and decreased zeaxanthin and de-epoxidation of the xanthophyll cycle pool (DES). Barbilophozia lycopodioides responded less to +UV-B, showing increased b-carotene and sclerophylly and decreased UV-absorbing compounds. Polytrichum commune only showed small morphogenetic changes. No effect of UV-B on bryophyte cover was observed. Water availability had profound effects on bryophyte ecophysiology, and plants showed, in general, lower growth and ETR, together with a higher photoprotection in the drier site. Water availability also influenced bryophyte responses to +UV-B and, in particular, responses were less detectable in the drier site. Conclusions: Impacts of UV-B exposure on Arctic bryophytes were significant, in contrast to modest or absent UV-B effects measured in previous studies. The impacts were more easily detectable in species with high plasticity such as H. splendens and less obvious, or more subtle, under drier conditions. Species biology and water supply greatly influences the impact of UV-B on at least some Arctic bryophytes and could contribute to the wide variation of responses observed previously.

Biostratigraphy, magnetostratigraphy, granulometry, isotopes and clay mineral composition of ODP Site 188-1165

During Ocean Drilling Program Leg 188 to Prydz Bay, East Antarctica, several of the shipboard scientists formed the High-Resolution Integrated Stratigraphy Committee (HiRISC). The committee was established in order to furnish an integrated data set from the Pliocene portion of Site 1165 as a contribution to the ongoing debate about Pliocene climate and climate evolution in Antarctica. The proxies determined in our various laboratories were the following: magnetostratigraphy and magnetic properties, grain-size distributions (granulometry), near-ultraviolet, visible, and near-infrared spectrophotometry, calcium carbonate content, characteristics of foraminifer, diatom, and radiolarian content, clay mineral composition, and stable isotopes. In addition to the HiRISC samples, other data sets contained in this report are subsets of much larger data sets. We included these subsets in order to provide the reader with a convenient integrated data set of Pliocene-Pleistocene strata from the East Antarctic continental margin. The data are presented in the form of 14 graphs (in addition to the site map). Text and figure captions guide the reader to the original data sets. Some preliminary interpretations are given at the end of the manuscript.

Chemical and mineral compositions of basalts and volcanic glasses from DSDP Sites 65-483 and 65-485

Major and rare earth element (REE) data for basalts from Holes 483, 483B, and 485A of DSDP Leg 65, East Pacific Rise, mouth of the Gulf of California, support a simple fractional crystallization model for the genesis of rocks from this suite. The petrography and mineral chemistry (presented in detail elsewhere) provide no evidence for magma mixing, but rather a simple multistage cooling process. Based on its lowest TiO2 content (0.88%), FeO*/MgO ratio (0.95 with total Fe as FeO), and Mg# (100 Mg/Mg + Fe" = 70), sample 483-17-2-(78-83) has been selected as the most primitive primary magma of the samples analyzed. This is supported by the REE data which show this sample has the lowest total REE content, a La/Sm_cn (chondrite-normalized) = 0.36, and Eu/Sm_cn = 1.05. Because other samples analyzed have higher SiO2, lower Mg#, and a negative Eu anomaly (Eu/Sm_cn as low as 0.89), they are most likely derivative magmas. Wright-Doherty and trace element modelling support fractional crystallization of 14.1% plagioclase (An88), 6.7% olivine (Fo86), and 4.7% clinopyroxene (Wo41En49Fs10) from 483-17-2-(78-83) to form the least differentiated sample with Mg# = 63. The La/Sm_cn of this derivative magma is almost identical to the parent magma (0.35 to 0.36), but the other samples have higher La/Sm_cn (0.45 to 0.51), more total REE, and lower Mg# (60 to 56). Both Wright-Doherty and trace element modelling indicate that the primary magma chosen cannot produce these more evolved samples. For the major elements, the TiO2 and P2O5 are too low in the calculated versus the observed (1.38 to 1.90; 0.11 to 0.17, respectively, for example). Rayleigh fractionation calculates a lower La/Sm_cn and requires about 60% crystal removal versus 40% for the Wright-Doherty. These more evolved samples must be derived from a parent magma different from the one selected here and, unfortunately, not sampled in this study. A magma formed by a smaller degree of partial melting with slightly more residual clinopyroxene left in the mantle than for sample 483-17-2-(78-83) is required.

Experiment: Ultraviolet radiation modulates the physiological responses of the calcified rhodophyte Corallina officinalis to elevated CO2

Ocean acidification reduces the concentration of carbonate ions and increases those of bicarbonate ions in seawater compared with the present oceanic conditions. This altered composition of inorganic carbon species may, by interacting with ultraviolet radiation (UVR), affect the physiology of macroalgal species. However, very little is known about how calcareous algae respond to UVR and ocean acidification. Therefore, we conducted an experiment to determine the effects of UVR and ocean acidification on the calcified rhodophyte Corallina officinalis using CO2-enriched cultures with and without UVR exposure. Low pH increased the relative electron transport rates (rETR) but decreased the CaCO3 content and had a miniscule effect on growth. However, UVA (4.25 W m-2) and a moderate level of UVB (0.5 W m-2) increased the rETR and growth rates in C. officinalis, and there was a significant interactive effect of pH and UVR on UVR-absorbing compound concentrations. Thus, at low irradiance, pH and UVR interact in a way that affects the multiple physiological responses of C. officinalis differently. In particular, changes in the skeletal content induced by low pH may affect how C. officinalis absorbs and uses light. Therefore, the light quality used in ocean acidification experiments will affect the predictions of how calcified macroalgae will respond to elevated CO2.

Effects of ultraviolet radiation and CO2 increase on winter phytoplankton assemblages in a temperate coastal lagoon

Increases in ultraviolet radiation (UVR) and CO2 affect phytoplankton growth and mortality in a variety of different ways. However, in situ responses of natural phytoplankton communities to climate change, as well as its effects on phytoplankton annual cycles, are still largely unknown. Although temperature and UVR have been increasing in temperate latitudes during winter, this season is still particularly neglected in climate change studies, being considered a non-active season regarding phytoplankton growth and production. Additionally, coastal lagoons are highly productive ecosystems and very vulnerable to climate change. This study aims, therefore, to evaluate the short-term effects of increased UVR and CO2 on the composition and growth of winter phytoplankton assemblages in a temperate coastal lagoon. During winter 2012, microcosm experiments were used to evaluate the isolated and combined effects of UVR and CO2, under ambient and high CO2 treatments, exposed to ambient UV levels and photosynthetically active radiation (PAR), or to PAR only. Phytoplankton composition, abundance, biomass and photosynthetic parameters were evaluated during the experiments. Significant changes were observed in the growth of specific phytoplankton groups, leading to changes in community composition. The cyanobacterium Synechococcus was dominant at the beginning of the experiment, but it was negatively affected by UVR and CO2. Diatoms clearly benefited from high CO2 and UVR, particularly Thalassiosira. Despite the changes observed in specific phytoplankton groups, growth and production of the whole phytoplankton community did not show significant responses to UVR and/or CO2.

Alleviation of solar ultraviolet radiation (UVR)-induced photoinhibition in diatom Chaetoceros curvisetus by ocean acidification

The study aimed to unravel the interaction between ocean acidification and solar ultraviolet radiation (UVR) in Chaetoceros curvisetus. Chaetoceros curvisetus cells were acclimated to high CO2 (HC, 1000 ppmv) and low CO2 concentration (control, LC, 380 ppmv) for 14 days. Cell density, specific growth rate and chlorophyll were measured. The acclimated cells were then exposed to PAB (photosynthetically active radiation (PAR) + UV-A + UV-B), PA (PAR + UV-A) or P (PAR) for 60 min. Photochemical efficiency (phi PSII), relative electron transport rate (rETR) and the recovery of ?PSII were determined. HC induced higher cell density and specific growth rate compared with LC. However, no difference was found in chlorophyll between HC and LC. Moreover, phi PSII and rETRs were higher under HC than LC in response to solar UVR. P exposure led to faster recovery of phi PSII, both under HC and LC, than PA and PAB exposure. It appeared that harmful effects of UVR on C. curvisetus could be counteracted by ocean acidification simulated by high CO2 when the effect of climate change is not beyond the tolerance of cells.