HS-ESS1-3: Stellar Nucleosynthesis
Communicate scientific ideas about the way stars, over their life cycle, produce elements. (Energy and Matter)
Clarification Statement: Emphasis is on the way nucleosynthesis, and therefore the different elements created, varies as a function of the mass of a star and the stage of its lifetime.
Assessment Boundary: Details of the many different nucleosynthesis pathways for stars of differing masses are not assessed.
The following assessments were created by science teachers hoping to better understand the NGSS. In most cases teachers went from standard to assessment in around an hour. These are drafts and should be used accordingly. Feel free to improve these assessments or contribute to the collection. Learn more about assessment design here.
- He-Li (early Universe)
- Be-Fe (stellar fusion)
- > Fe (Supernova)
Energy and Matter
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