High Academic Standards for Students
HS.E1U1.11: Analyze and interpret data to determine how energy from the Sun affects weather patterns and climate.
Coastal Winds and Clouds
Coastal Winds and Clouds - Metric
Seasons Around the World
Seasons in 3D
HS+E.E1U1.1: Construct an explanation based on evidence for how the Sun’s energy transfers between Earth’s systems.
Coastal Winds and Clouds
Coastal Winds and Clouds - Metric
Greenhouse Effect - Metric
HS+E.E1U1.2: Develop and use models to describe how variations in the flow of energy into and out of Earth’s systems result in changes in climate.
HS.E1U1.12: Develop and use models of the Earth that explains the role of energy and matter in Earth’s constantly changing internal and external systems (geosphere, hydrosphere, atmosphere, biosphere).
Plate Tectonics
Rock Cycle
Water Cycle
HS+E.E1U1.4: Analyze and interpret geoscience data to make the claim that dynamic interactions with Earth’s surface can create feedbacks that cause changes to other Earth systems.
HS+E.E1U1.5: Obtain, evaluate, and communicate information on the effect of water on Earth’s materials, surface processes, and groundwater systems.
Erosion Rates
River Erosion
Weathering
HS+E.E1U1.6: Obtain, evaluate, and communicate information of the theory of plate tectonics to explain the differences in age, structure, and composition of Earth’s crust.
HS+E.E1U1.8: Develop and use models to illustrate how Earth's internal and surface processes operate over time to form, modify, and recycle continental and ocean floor features.
HS+E.E1U3.10: Ask questions, define problems, and evaluate a solution to a complex problem, based on prioritized criteria and tradeoffs, that account for a range of constraints, including cost, safety, reliability, and aesthetics, as well as possible social, cultural, and environmental impacts.
Genetic Engineering
Nitrogen Cycle
HS.E2U1.15: Construct an explanation based on evidence to illustrate the role of nuclear fusion in the life cycle of a star.
HS+E.E2U1.12: Obtain, evaluate, and communicate scientific information about the way stars, throughout their stellar stages, produce elements and energy.
HS.E2U1.16: Construct an explanation of how gravitational forces impact the evolution of planetary motion, structure, surfaces, atmospheres, moons, and rings.
Orbital Motion - Kepler's Laws
Tides - Metric
HS+E.E2U1.13: Analyze and interpret data showing how gravitational forces are influenced by mass and the distance between objects.
HS+E.E2U1.14: Use mathematics and computational thinking to explain the movement of planets and objects in the solar system.
Gravitational Force
Orbital Motion - Kepler's Laws
HS.E2U1.17: Construct an explanation of the origin, expansion, and scale of the universe based on astronomical evidence.
Big Bang Theory - Hubble's Law
HS+E.E2U1.16: Obtain, evaluate, and communicate information about patterns of size and scale of our solar system, our galaxy, and the universe.
H-R Diagram
Solar System Explorer
Star Spectra
HS+E.E2U2.17: Obtain, evaluate, and communicate the impact of technology on human understanding of the formation, scale, and composition of the universe.
Correlation last revised: 9/15/2020