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Published by
 Australian Academy of Science
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Activities | Thinking ahead fusion energy for the 21st century?
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- General Atomics Fusion Education (USA)
- Starpower By manipulating magnetic
field strength, power, fuel, density, pressure, shape and boundary, students
attempt to produce at least 1000 MW of electricity from a fusion reactor.
- Internet Plasma Physics Education Experience (USA)
Provides information about fusion and a number of applets, including:
Also includes interactive modules on matter, electricity, magnetism, energy and fusion.
- An Educator's Reference Desk Lesson Plan (USA)
- Magnetic forces an introduction to magnetic attraction, strength of force and the magnetic forces of the Earth.
- ScienceNetLinks (American Association for the Advancement of Science, USA)
- Risks and benefits students assess and weigh the risks and benefits associated with innovations in science and technology.
- Radioactive decay: A sweet simulation of a half-life demonstrates that the rates of decay of unstable nuclei can be measured, that the exact time that a certain nucleus will decay cannot be predicted, and that
it takes a very large number of nuclei to find the rate of decay.
- Isotopes of pennies provides lessons about radioactivity
and isotopes using coins to represent subatomic particles.
- What do scientists do? students develop an understanding of the diversity and nature of various science disciplines.
- ThinkQuest (Oracle Education Foundation, USA)
- Basic fusion – provides background information on fusion reactions and then checks submitted answers to questions.
- Binding energy – provides background information on binding energy and then checks submitted answers to questions.
- Energy Information Administration (Department of Energy, USA)
- Energy source web quest students learn about energy sources using web-based resources and create PowerPoint presentations to teach other students.
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External sites are not endorsed by the Australian Academy of Science.
Posted February 2007.

The Australian Foundation for Science is a supporter of Nova.
This topic is sponsored by the Research School of
Physical Sciences and Engineering at the Australian National University, the Australian Nuclear Science and Technology Organisation, the School of
Mathematical and Physical Sciences at the University of Newcastle and the School of Physics at the University of Sydney.
© Australian Academy of Science
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