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  • 1
    Publication Date: 2015-09-01
    Description: Human mutations that truncate the massive sarcomere protein titin [TTN-truncating variants (TTNtvs)] are the most common genetic cause for dilated cardiomyopathy (DCM), a major cause of heart failure and premature death. Here we show that cardiac microtissues engineered from human induced pluripotent stem (iPS) cells are a powerful system for evaluating the pathogenicity of titin gene variants. We found that certain missense mutations, like TTNtvs, diminish contractile performance and are pathogenic. By combining functional analyses with RNA sequencing, we explain why truncations in the A-band domain of TTN cause DCM, whereas truncations in the I band are better tolerated. Finally, we demonstrate that mutant titin protein in iPS cell-derived cardiomyocytes results in sarcomere insufficiency, impaired responses to mechanical and beta-adrenergic stress, and attenuated growth factor and cell signaling activation. Our findings indicate that titin mutations cause DCM by disrupting critical linkages between sarcomerogenesis and adaptive remodeling.〈br /〉〈br /〉〈a href="https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4618316/" target="_blank"〉〈img src="https://static.pubmed.gov/portal/portal3rc.fcgi/4089621/img/3977009" border="0"〉〈/a〉   〈a href="https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4618316/" target="_blank"〉This paper as free author manuscript - peer-reviewed and accepted for publication〈/a〉〈br /〉〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Hinson, John T -- Chopra, Anant -- Nafissi, Navid -- Polacheck, William J -- Benson, Craig C -- Swist, Sandra -- Gorham, Joshua -- Yang, Luhan -- Schafer, Sebastian -- Sheng, Calvin C -- Haghighi, Alireza -- Homsy, Jason -- Hubner, Norbert -- Church, George -- Cook, Stuart A -- Linke, Wolfgang A -- Chen, Christopher S -- Seidman, J G -- Seidman, Christine E -- EB017103/EB/NIBIB NIH HHS/ -- HG005550/HG/NHGRI NIH HHS/ -- HL007374/HL/NHLBI NIH HHS/ -- HL115553/HL/NHLBI NIH HHS/ -- HL125807/HL/NHLBI NIH HHS/ -- K08 HL125807/HL/NHLBI NIH HHS/ -- T32 HL007208/HL/NHLBI NIH HHS/ -- Department of Health/United Kingdom -- Howard Hughes Medical Institute/ -- New York, N.Y. -- Science. 2015 Aug 28;349(6251):982-6. doi: 10.1126/science.aaa5458.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Division of Cardiovascular Medicine, Brigham and Women's Hospital, Boston, MA 02115, USA. jthinson@partners.org cseidman@genetics.med.harvard.edu. ; Department of Biomedical Engineering, Boston University, Boston, MA 02215, USA. The Wyss Institute for Biologically Inspired Engineering at Harvard University, Boston, MA 02115, USA. ; Department of Genetics, Harvard Medical School, Boston, MA 02115, USA. ; Division of Cardiovascular Medicine, Beth Israel Deaconess Medical Center, Boston, MA 02215, USA. ; Department of Cardiovascular Physiology, Ruhr University Bochum, MA 3/56 D-44780, Bochum, Germany. ; The Wyss Institute for Biologically Inspired Engineering at Harvard University, Boston, MA 02115, USA. Department of Genetics, Harvard Medical School, Boston, MA 02115, USA. ; Cardiovascular and Metabolic Sciences, Max Delbruck Center for Molecular Medicine, Berlin, Germany. ; Division of Cardiovascular Medicine, Brigham and Women's Hospital, Boston, MA 02115, USA. Department of Genetics, Harvard Medical School, Boston, MA 02115, USA. Howard Hughes Medical Institute, Chevy Chase, MD 20815, USA. ; Cardiovascular and Metabolic Sciences, Max Delbruck Center for Molecular Medicine, Berlin, Germany. DZHK (German Center for Cardiovascular Research), Partner Site Berlin, Berlin, Germany. ; National Institute for Health Research (NIHR) Biomedical Research Unit in Cardiovascular Disease at Royal Brompton and Harefield National Health Service (NHS) Foundation Trust, Imperial College London, London, UK. National Heart Centre and Duke-National University, Singapore, Singapore. ; Division of Cardiovascular Medicine, Brigham and Women's Hospital, Boston, MA 02115, USA. Department of Genetics, Harvard Medical School, Boston, MA 02115, USA. Howard Hughes Medical Institute, Chevy Chase, MD 20815, USA. jthinson@partners.org cseidman@genetics.med.harvard.edu.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/26315439" target="_blank"〉PubMed〈/a〉
    Keywords: Adrenergic beta-Agonists/pharmacology ; Cardiomyopathy, Dilated/*genetics/pathology/*physiopathology ; Cells, Cultured ; Connectin/chemistry/*genetics/*physiology ; Heart Rate ; Humans ; Induced Pluripotent Stem Cells/*physiology ; Isoproterenol/pharmacology ; Mutant Proteins/chemistry/physiology ; *Mutation, Missense ; Myocardial Contraction ; Myocytes, Cardiac/*physiology ; RNA/genetics/metabolism ; Sarcomeres/*physiology/ultrastructure ; Sequence Analysis, RNA ; Signal Transduction ; Stress, Physiological
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 2
    Publication Date: 2013-08-31
    Description: Thermal-infrared (10 and 20 micron) images of Comet Austin were obtained on UT 30.6 Apr., 1.8, 2.8, and 3.6 May 1990. The NASA-Marshall Space Flight Center 20 pixel bolometer array at the NASA 3 meter Infrared Telescope Facility in Hawaii was used. The 10.8 micron (FWHM = 5.3 microns) maps were obtained with maximum dimensions of 113 arcsec (57,500 km) in RA and 45 arcsec (23,000 km) in declination, with a pixel size of 4.2 x 4.2 arcsec. A smaller, 45 x 18 arcsec, map was obtained in the 19.2 micron (FWHM = 5.2 microns) bandpass. At the time of these observations Comet Austin's heliocentric and geocentric distances were 0.7 and 0.5 AU respectively. The peak flux density (within the brightest pixel) was 23 + or - 2 Janskys for the first three dates and only marginally lower the last day; i.e., within the observational uncertainties no evidence was found for day-to-day variability like that observed in Comet Halley. A dynamical analysis of the morphology of the extended dust emission is used to constrain the size distribution and production rate of the dust particles. The results of this analysis are compared with similar studies carried out on comets P/Giacobini-Zinner, P/Brorsen-Metcalf, P/Halley, P/Tempel 2, and Wilson (1987).
    Keywords: ASTROPHYSICS
    Type: Lunar and Planetary Inst., Abstracts for the International Conference on Asteroids, Comets, Meteors 1991; p 35
    Format: application/pdf
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