Explain and compare nuclear reactions (radioactive decay, fission and fusion), the energy changes associated with them and their associated safety issues.
Course Number1111 |
Course Title222 |
2001350: | Astronomy Solar/Galactic (Specifically in versions: 2014 - 2015, 2015 - 2022, 2022 - 2024, 2024 and beyond (current)) |
2020910: | Astronomy Solar/Galactic Honors (Specifically in versions: 2014 - 2015, 2015 - 2022, 2022 - 2024, 2024 and beyond (current)) |
2003350: | Chemistry 1 Honors (Specifically in versions: 2014 - 2015, 2015 - 2022, 2022 - 2024, 2024 and beyond (current)) |
2001310: | Earth/Space Science (Specifically in versions: 2014 - 2015, 2015 - 2022, 2022 - 2024, 2024 and beyond (current)) |
2001320: | Earth/Space Science Honors (Specifically in versions: 2014 - 2015, 2015 - 2022, 2022 - 2024, 2024 and beyond (current)) |
2002440: | Integrated Science 3 (Specifically in versions: 2014 - 2015, 2015 - 2022, 2022 - 2024, 2024 and beyond (current)) |
2002450: | Integrated Science 3 Honors (Specifically in versions: 2014 - 2015, 2015 - 2022, 2022 - 2024, 2024 and beyond (current)) |
2003400: | Nuclear Radiation (Specifically in versions: 2014 - 2015, 2015 - 2018 (course terminated)) |
2020710: | Nuclear Radiation Honors (Specifically in versions: 2014 - 2015, 2015 - 2022, 2022 - 2024, 2024 and beyond (current)) |
2003320: | Physical Science Honors (Specifically in versions: 2014 - 2015, 2015 - 2022, 2022 - 2024, 2024 and beyond (current)) |
2003410: | Physics 2 Honors (Specifically in versions: 2014 - 2015, 2015 - 2022, 2022 - 2024, 2024 and beyond (current)) |
2002330: | Space Technology and Engineering (Specifically in versions: 2014 - 2015, 2015 - 2018 (course terminated)) |
7920020: | Access Earth/Space Science (Specifically in versions: 2014 - 2015, 2015 - 2018, 2018 - 2023, 2023 and beyond (current)) |
2002445: | Integrated Science 3 for Credit Recovery (Specifically in versions: 2014 - 2015, 2015 - 2020 (course terminated)) |
2003500: | Renewable Energy 1 Honors (Specifically in versions: 2014 - 2015, 2015 - 2022, 2022 - 2023, 2023 - 2024, 2024 and beyond (current)) |
2003838: | Florida's Preinternational Baccalaureate Physics 2 (Specifically in versions: 2015 and beyond (current)) |
Name |
Description |
The Regulation of Nuclear Waste | In this lesson, students are presented with the problems facing the disposal of high-level nuclear waste produced at nuclear power plants along with the government agencies that regulate the nuclear waste. After learning about several disposal options, students research the pros and cons of one of these options and present their findings to the class. The class "votes" on which option they would choose if they were part of a government agency that regulated nuclear waste disposal and discuss current disposal options being debated among various government regulatory agencies. |
The Future of Fission and Fusion | Students will work collaboratively to investigate the current use of fission as an energy source in various nations across the world, as well as the safety risks associated. They will also explore the potential of fusion as a future energy source and how their assigned nation/organization interacts globally with the scientific community to further its progress. |
Life of the Party | This activity teaches students how to determine the age of an atom using an onion, cabbage, and Brussels sprouts. Aliens from another planet left these items on our planet and need our assistance determining their age. Based on the number of layers or half lives of the "elements," the students will be able to determine their age. The students will also be able to differentiate between the three types of radioactive decay and understand why radioactive elements are harmful. |
Radioactive Decay: Is It Safe for Us to Stay? | Students will collect data using inexpensive split peas and black beans in order to model how to calculate the amount of a radioactive element remaining after a specific number of half-lives have passed. Students will then use this data to outline and create a response to a scenario-based writing prompt. |
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Description |
Where Do Chemical Elements Come From? | This informational text resource is intended to support reading in the content area. What is that extremely bright light in the sky? It's a supernova: the result of a massive star collapsing in on itself. This explosion is more than just a pretty sight; it is the main source of the elements that make up our planets and all the other objects in the night sky. |
How Nuclear Power Works | This informational text is intended to support reading in the content area. Nuclear power has become a suggested solution to the issue of energy dependence, but what exactly is nuclear power? This article focuses on the many aspects of nuclear power including how it's created through fission and harnessed for electricity. Discussion of the pros and cons of nuclear energy and storage methods is also covered. |
How Tumbleweeds Spread Radiation from Old Nuclear Sites | This informational text resource is intended to support reading in the content area. The article describes how radioactive materials can be spread by biological vectors, such as tumbleweeds and rabbits, from decommissioned nuclear sites and nuclear waste storage facilities. |
Explainer: The Difference Between Radioactivity and Radiation | This informational text resource is intended to support reading in the content area. This text explains the difference between radioactivity (including radioactive decay, half-life, etc.) and radiation, and the connection between the two. |
Oslo-Experiment May Explain Massive Star Explosions | This informational text resource is intended to support reading in the content area. Some new findings about atomic nuclei may help astrophysicists create more realistic simulations of supernovae thus allowing us to see how heavier elements are formed in stars. |
The New Alchemy | This informational text is intended to support reading in the content area. This article from the American Chemical Society reviews the basics of radioactivity and transmutation as well as the history of discovering elements. |