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Revision as of 11:29, 1 April 2025
Use mathematical or computational representations to predict the motion of orbiting objects in the solar system.
Clarification statement: Emphasis is on Newtonian gravitational laws governing orbital motions, which apply to human-made satellites as well as planets and moons.
Assessment boundary: Mathematical representations for the gravitational attraction of bodies and Kepler’s Laws of orbital motions should not deal with more than two bodies, nor involve calculus.
Resources
Examples and discussion of resources for the learning, teaching, and assessment of HS-ESS1-4.
This section could be expanded upon. You can help out by adding to this section.
Assessment
What assessment of HS-ESS1-4 might look like on a NY state exam.
This section could be expanded upon. You can help out by adding to this section.
NGSS Dimensions
Performance expectation HS-ESS1-4 was developed using the following elements from the NRC document A Framework for K-12 Science Education: