Tuesday, October 3, 2023, 7:12 PM
Site: Dearborn Educational Curriculum
Course: Dearborn Educational Curriculum (DEC)
Glossary: MI Science Standards
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HS-ESS1-1

by Troy Patterson - Tuesday, July 25, 2017, 1:35 PM
 
Develop a model based on evidence to illustrate the life span of the sun and the role of nuclear fusion in the sun’s core to release energy that eventually reaches Earth in the form of radiation.
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HS-ESS1-2

by Troy Patterson - Tuesday, July 25, 2017, 1:35 PM
 
Construct an explanation of the Big Bang theory based on astronomical evidence of light spectra, motion of distant galaxies, and composition of matter in the universe.
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HS-ESS1-3

by Troy Patterson - Tuesday, July 25, 2017, 1:35 PM
 
Communicate scientific ideas about the way stars, over their life cycle, produce elements.
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HS-ESS1-4

by Troy Patterson - Tuesday, July 25, 2017, 1:35 PM
 
Use mathematical or computational representations to predict the motion of orbiting objects in the solar system.
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HS-ESS1-5

by Troy Patterson - Tuesday, July 25, 2017, 1:35 PM
 
Evaluate evidence of the past and current movements of continental and oceanic crust and the theory of plate tectonics to explain the ages of crustal rocks.
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HS-ESS1-6

by Troy Patterson - Tuesday, July 25, 2017, 1:35 PM
 
Apply scientific reasoning and evidence from ancient Earth materials, meteorites, and other planetary surfaces to construct an account of Earth’s formation and early history.
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HS-ESS2-1

by Troy Patterson - Tuesday, July 25, 2017, 1:35 PM
 
Develop a model to illustrate how Earth’s internal and surface processes operate at different spatial and temporal scales to form continental and ocean-floor features.
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HS-ESS2-2

by Troy Patterson - Tuesday, July 25, 2017, 1:35 PM
 
Analyze geoscience data to make the claim that one change to Earth’s surface can create feedbacks that cause changes to other Earth systems.
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HS-ESS2-3

by Troy Patterson - Tuesday, July 25, 2017, 1:35 PM
 
Develop a model based on evidence of Earth’s interior to describe the cycling of matter by thermal convection.
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HS-ESS2-4

by Troy Patterson - Tuesday, July 25, 2017, 1:35 PM
 
Use a model to describe how variations in the flow of energy into and out of Earth’s systems result in changes in climate.