Purpose
Hepatocellular cancer (HCC) is a deadly and most rapidly increasing cancer in the USA and worldwide. The etiology and factors involved in development of HCC remain largely unknown. A marked decrease in zinc occurs in HCC. Its role and involvement in HCC has not been identified. We investigated the relationship of cellular zinc changes to the development of malignancy, and the identification of potential zinc transporters associated with the inability of hepatoma cells to accumulate zinc.
Methods
The detection of relative zinc levels in situ in normal hepatic cells vs. hepatoma was performed on normal and HCC tissue sections. ZIP1, 2, 3, and 14 transporters were identified by immunohistochemistry.
Results
Intracellular zinc levels are markedly decreased in HCC hepatoma cells vs. normal hepatic cells in early stage and advanced stage malignancy. ZIP14 transporter is localized at the plasma membrane in normal hepatocytes, demonstrating its functioning for uptake and accumulation of zinc. The transporter is absent in the hepatoma cells and its gene expression is downregulated. The change in ZIP14 is concurrent with the decrease in zinc. ZIP1, 2, 3 are not associated with normal hepatocyte uptake of zinc, and HCC zinc depletion. HepG2 cells exhibit ZIP14 transporter. Zinc treatment inhibits their growth.
Conclusions
ZIP14 downregulation is likely involved in the depletion of zinc in the hepatoma cells in HCC. These events occur early in the development of malignancy possibly to protect the malignant cells from tumor suppressor effects of zinc. This provides new insight into important factors associated with HCC carcinogenesis.
The James Webb Space Telescope (JWST) is a large, infrared space telescope that has recently started its science program which will enable breakthroughs in astrophysics and planetary science. Notably, JWST will provide the very first observations of the earliest luminous objects in the universe and start a new era of exoplanet atmospheric characterization. This transformative science is enabled by a 6.6 m telescope that is passively cooled with a 5 layer sunshield. The primary mirror is comprised of 18 controllable, low areal density hexagonal segments, that were aligned and phased relative to each other in orbit using innovative image-based wave front sensing and control algorithms. This revolutionary telescope took more than two decades to develop with a widely distributed team across engineering disciplines. We present an overview of the telescope requirements, architecture, development, superb on-orbit performance, and lessons learned. JWST successfully demonstrates a segmented aperture space telescope and establishes a path to building even larger space telescopes.
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