107 research outputs found

    Can Tetrahymena thermophila help us better understand the activity of proto-oncogenes and their associated gene regulation?

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    Nearly all of us have been affected by cancer, a deadly disease that has its roots in mitotic dysregulation. Proto-oncogenes, or regulated growth genes, are present in all eukaryotic cells. In many tumors, the regulatory elements that allow for homeostatic growth have been silenced or lost to mutations, resulting in pathological overgrowth of cells. Tetrahymena thermophila are free-living eukaryotic unicellular organisms that generally reproduce asexually via mitosis. Our previous studies have shown that these organisms appear to express homologues of the proto-oncogene, Ras, and its signaling partner, Raf. The Ras/Raf uncoupler BAY-293 reduces mitotic signaling in this organism, apparently by decreasing gene expression as indicated by the increased level of histone acetylation seen with drug treatment. Another proto-oncogene involved in vertebrate mitotic signaling is the tyrosine phosphatase SHP2, encoded by the gene PTPN11. This protein is instrumental in recruiting a number of pathways involved in mitosis and differentiation, including the Ras/Raf pathway. BLAST searches of the Tetrahymena Genome Database using the SHP2 sequence indicate a high likelihood that Tetrahymena have a SHP2 homolog, making this an intriguing target for drug study. We hypothesized that inhibiting SHP2 would reduce mitosis in Tetrahymena; however, the SHP2 inhibitor PHPS significantly increased cell division in this organism while decreasing histone acetylation. PHPS increased levels of tyrosine phosphorylation and nucleolar activity in Tetrahymena; the distribution of phosphorylation throughout the cell was also affected. In summary, we see that while the Ras homolog in Tetrahymena affects mitosis in a manner that is similar to vertebrates, the SHP2 homolog does not. Therefore, Tetrahymena would be a useful model system in which to study drugs that affect the Ras/Raf portion of growth factor signaling

    Using ice core measurements from Taylor Glacier, Antarctica, to calibrate in situ cosmogenic 14 C production rates by muons

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    Cosmic rays entering the Earth’s atmosphere produce showers of secondary particles such as protons, neutrons, and muons. The interaction of these particles with oxygen-16 (16O) in minerals such as ice and quartz can produce carbon-14 (14C). In glacial ice, 14C is also incorporated through trapping of 14C-containing atmospheric gases (14CO2, 14CO, and 14CH4). Understanding the production rates of in situ cosmogenic 14C is important to deconvolve the in situ cosmogenic and atmospheric 14C signals in ice, both of which contain valuable paleoenvironmental information. Unfortunately, the in situ 14C production rates by muons (which are the dominant production mechanism at depths of > 6m solid ice equivalent) are uncertain. In this study, we use measurements of in situ 14C in ancient ice (> 50 ka) from the Taylor Glacier, an ablation site in Antarctica, in combination with a 2D ice flow model to better constrain the compound-specific rates of 14C production by muons and the partitioning of in situ 14C between CO2, CO, and CH4. Our measurements show that 33.7% (11.4%; 95% confidence interval) of the produced cosmogenic 14C forms 14CO and 66.1% (11.5%; 95% confidence interval) of the produced cosmogenic 14C forms 14CO2. 14CH4 represents a very small fraction (< 0.3%) of the total. Assuming that the majority of in situ muogenic 14C in ice forms 14CO2, 14CO, and 14CH4, we also calculated muogenic 14C production rates that are lower by factors of 5.7 (3.6–13.9; 95% confidence interval) and 3.7 (2.0–11.9; 95% confidence interval) for negative muon capture and fast muon interactions, respectively, when compared to values determined in quartz from laboratory studies (Heisinger et al., 2002a, b) and in a natural setting (Lupker et al., 2015). This apparent discrepancy in muogenic 14C production rates in ice and quartz currently lacks a good explanation and requires further investigation

    The twilight of the Liberal Social Contract? On the Reception of Rawlsian Political Liberalism

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    This chapter discusses the Rawlsian project of public reason, or public justification-based 'political' liberalism, and its reception. After a brief philosophical rather than philological reconstruction of the project, the chapter revolves around a distinction between idealist and realist responses to it. Focusing on political liberalism’s critical reception illuminates an overarching question: was Rawls’s revival of a contractualist approach to liberal legitimacy a fruitful move for liberalism and/or the social contract tradition? The last section contains a largely negative answer to that question. Nonetheless the chapter's conclusion shows that the research programme of political liberalism provided and continues to provide illuminating insights into the limitations of liberal contractualism, especially under conditions of persistent and radical diversity. The programme is, however, less receptive to challenges to do with the relative decline of the power of modern states
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