Communicate scientific ideas about the way stars, over their life cycle, produce elements.
Standard detail
HS-ESS1-3
Performance Expectation
Depth 2Parent ID: EA28EDD0DFE60131CA7868A86D17958EStandard set: Grades 9, 10, 11, 12
Original statement
Quick facts
- Statement code
- HS-ESS1-3
- Standard ID
- EA2A0D50DFE60131CA7B68A86D17958E
- ASN identifier
- S2454589
- Subject
- Science
- Grades
- 09, 10, 11, 12
- Ancestor IDs
- EA28EDD0DFE60131CA7868A86D17958EEA288970DFE60131CA7768A86D17958E
- Source document
- Next Generation Science Standards (2013)
- License
- CC BY 3.0 US
- Dataset notes
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.