We explore how and why fusion occurs between atoms, what products result from this type of reaction, and how stars use this process to create energy and the atoms of which we are made.
Segment 7C: Fusion We explore how and why fusion occurs between atoms, what products result from this type of reaction, and how stars use this process to create energy and the atoms that we are made of.Premiere Date: August 1, 2018 | Runtime: 00:08:13
-Define nuclear fusion and explain when nuclear fusion occurs.
-Explain why energy is released when light nuclei come together to form heavier nuclei, and how the mass of the individual particles are more than the total mass of the nucleus after nuclear fusion occurs.
-Discuss how the sun is powered by the fusion of hydrogen into helium and explore how the atoms that make us up were created inside of stars.
binding energy (E) - the amount of energy used to keep a nucleus together; equal to the mass defect times the speed of light, squared.
fusion - when two light atomic nuclei come together, or fuse, to form a heavier nucleus, releasing energy.
mass defect (Dm) - the difference in mass between the particles within a nucleus and the particles by themselves, not bound within a nucleus.
proton-proton fusion - the multistep nuclear fusion process by which hydrogen fuses with hydrogen to form helium.
radioactive decay - the spontaneous emission of charged particles and/or energy from an atom.
The Physics in Motion teacher toolkit provides instructions and answer keys for study questions, practice problems, labs for all seven units of study. GPB offers the teacher toolkit at no cost to Georgia educators. It will be available in September 2018. To preorder your teacher toolkit, complete and submit this form to request the teacher toolkit. You only need to submit this form one time to get materials for all seven units of study.