ESS.1.1 Life Span of the Sun and the Role of Nuclear Fission
Standard ESS.1.1 Develop a model based on evidence to illustrate the life span of the Sun and the role of nuclear fusion releasing energy in the Sun’s core. Emphasize energy transfer mechanisms that allow energy from nuclear fusion to reach Earth. Examples of evidence for the model could include observations of the masses and lifetimes of other stars, or non-cyclic variations over centuries. (PS1.C, PS3.D, ESS1.A, ESS1.B)
Science and Engineering Practice
Crosscutting Concept
Disciplinary Core Idea
ESS.1.1 Storyline