Difference between revisions of "HS-ESS1-3"
(Section order: Vocabulary now comes before Performance Level Descriptions) |
(PLDs: add example released question per level (editor judgment)) |
||
| Line 109: | Line 109: | ||
| Level4 = Communicate scientific ideas about the way stars, over their life cycles, produce elements. | | Level4 = Communicate scientific ideas about the way stars, over their life cycles, produce elements. | ||
| Level3 = Describe or identify one scientific idea from a source about how stars, over their life cycles, produce different elements depending on their masses or their life cycle. | | Level3 = Describe or identify one scientific idea from a source about how stars, over their life cycles, produce different elements depending on their masses or their life cycle. | ||
| + | | Example3 = [[Questions:Evidence for the Big Bang Theory#q5|January 2026 Question 5]] | ||
| Level2 = Identify the given scientific idea that describes how different elements are produced by different types of stars over their life cycle. | | Level2 = Identify the given scientific idea that describes how different elements are produced by different types of stars over their life cycle. | ||
| + | | Example2 = [[Questions:Evidence for the Big Bang Theory#q4|January 2026 Question 4]] | ||
| Level1 = Given a scientific idea, identify the claim, from those provided, that describes how stars form elements over their life cycle. | | Level1 = Given a scientific idea, identify the claim, from those provided, that describes how stars form elements over their life cycle. | ||
| + | | Example1 = [[Questions:Energy in the Sun#q5|August 2025 Question 5]] | ||
}} | }} | ||
Revision as of 02:40, 16 October 2026
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.
Reference Tables
Relevant reference tables:
Regents Exam Questions
Released New York State Regents exam questions that assess HS-ESS1-3 are listed here by exam and question cluster. Each link opens the question with its answer key.
Vocabulary
Terms from the Earth & Space Science Glossary that come from this standard or from the released exam questions that assess it.
- atomic nuclei
- brightness
- compositional elements
- Earth
- electromagnetic energy
- element formation
- elements
- heavier elements
- helium
- hydrogen
- iron
- life cycle
- light spectra
- mass
- mass of a star
- massive stars
- neutron
- nuclear fusion
- nucleosynthesis
- proton
- stars
- supernova
- universe
- carbon – Aug 2026, June 2026, Jan 2026, Aug 2025, June 2025
- constellation – June 2026
- galaxy – June 2026, Jan 2026
- gamma-ray burst – June 2026
- gravitational collapse – Aug 2025
- latitude – June 2026
- main sequence – Aug 2026, June 2026
- model – June 2026
- multiple-star system – June 2026
- Northern Hemisphere – June 2026
- oxygen – Aug 2026, Jan 2026, Aug 2025, June 2025
- radiation – Aug 2026
- red giant – Aug 2026, June 2026
- solar mass – Aug 2026, June 2025
- stellar evolution – June 2026, Aug 2025
- supergiant – Aug 2026
- surface temperature – Aug 2026
- velocity – Aug 2026
Performance Level Descriptions
Every Regents exam question on HS-ESS1-3 is written to match one of the performance level descriptions (PLDs) below.
NGSS Dimensions
Performance expectation HS-ESS1-3 was developed using the following elements from the NRC document A Framework for K-12 Science Education:
- Obtaining, Evaluating, and Communicating Information
- Communicate scientific ideas (e.g., about phenomena and/or the process of development and the design and performance of a proposed process or system) in multiple formats (including orally, graphically, textually, and mathematically).
- ESS1.A: The Universe and Its Stars
- The study of stars' light spectra and brightness is used to identify compositional elements of stars, their movements, and their distances from Earth.
- Other than the hydrogen and helium formed at the time of the Big Bang, nuclear fusion within stars produces all atomic nuclei lighter than and including iron, and the process releases electromagnetic energy. Heavier elements are produced when certain massive stars achieve a supernova stage and explode.
- Energy and Matter
- In nuclear processes, atoms are not conserved, but the total number of protons plus neutrons is conserved.