Difference between revisions of "HS-ESS1-3"
From NY Science Standards Wiki
Line 23: | Line 23: | ||
| CC1 = | | CC1 = | ||
}} | }} | ||
− | + | <!-- | |
== {{Connectionsheading}} == | == {{Connectionsheading}} == | ||
{{connectionsmessage}} | {{connectionsmessage}} | ||
Line 32: | Line 32: | ||
| MATH1 = | | MATH1 = | ||
}} | }} | ||
− | + | --> | |
{{Pagecontributors}} | {{Pagecontributors}} | ||
Revision as of 11:28, 1 April 2025
Communicate scientific ideas about the way stars, over their life cycle, produce elements.
Clarification statement: Emphasis is on how nucleosynthesis 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.
Resources
Examples and discussion of resources for the learning, teaching, and assessment of HS-ESS1-3.

Assessment
What assessment of HS-ESS1-3 might look like on a NY state exam.

NGSS Dimensions
Performance expectation HS-ESS1-3 was developed using the following elements from the NRC document A Framework for K-12 Science Education:
Science and Engineering Practices
Disciplinary Core Ideas
Crosscutting Concepts
Page contributors: Conrad Richman, Caroline Leonard