Introduction to Fusion Energy Jerry Hughes IAP @ PSFC January 8, 2013 Acknowledgments: Catherine Fiore, Jeff Freidberg, Martin Greenwald, Zach Hartwig, Alberto Loarte, Bob Mumgaard, Geoff Olynyk Presenter’s e-mail:
[email protected] Questions to answer • What is fusion? • Why do we need it? • How do we get it on earth? • Where do we stand? • Where are we headed? What is fusion, anyway? What is fusion, anyway? What is fusion, anyway? What is fusion, anyway? Fusion is a form of nuclear energy E mc2 • A huge amount of energy is released when isotopes lighter than iron combine to form heavier nuclei, with less final mass • It is an ubiquitous energy source in the universe • It is not (yet) a practical energy source on earth Fusion is a form of nuclear energy E mc2 • A huge amount of energy is released when isotopes lighter than iron combine to form heavier nuclei, with less final mass • It is an ubiquitous energy source in the universe • It is not (yet) a practical energy source on earth Terrestrial energy sources have their origin in the nuclear fusion reactions of stars Supernova produces radioactive elements Solar heating of the Earth drives atmospheric circulation, water cycle Sun illuminates Earth Terrestrial energy sources have their origin in the nuclear fusion reactions of stars Geothermal Decay of radioactive particles generates heat in Earth’s interior Nuclear fission Supernova produces radioactive elements Splitting radioactive particles generates heat Solar heating of the Earth drives atmospheric circulation, water cycle