Earth and Space Systems Science

Family & Community Resources Earth and Space Systems Science

Bryce Canyon

Course Overview

Course Overview

Earth and Space Systems (ESS) sciences investigate processes that operate on Earth and also address Earth's place in the solar system and the galaxy. Thus ESS involve phenomena that range in scale from the unimaginably large to the invisibly small. Earth consists of a set of systems – atmosphere, hydrosphere, geosphere, and biosphere – that are intricately interconnected. The systems have differing sources of energy, and matter cycles within and among them in multiple ways and on various time scales. Small changes in one part of one system can have large and sudden consequences in parts of other systems, or they can have no effect at all. Understanding the different processes that cause Earth to change over time (in a sense, how it “works”) therefore requires knowledge of the multiple systems’ interconnections and feedbacks. In addition, Earth is part of a broader system – the solar system- which is itself a small part of one of the many galaxies in the universe.

Students in high school continue to develop their understanding of the three disciplinary core ideas in the Earth and Space Sciences. The high school performance expectations in Earth and Space Science build on the middle school ideas and skills and allow high school students to explain more in-depth phenomena central not only to the earth and space sciences, but to life and physical sciences as well. These performance expectations blend the core ideas with scientific and engineering practices and crosscutting concepts to support students in developing useable knowledge to explain ideas across the science disciplines.

There are strong connections to mathematical practices of analyzing and interpreting data. The performance expectations strongly reflect the many societally relevant aspects of ESS (resources, hazards, environmental impacts) with an emphasis on using engineering and technology concepts to design solutions to challenges facing human society. For complete storyline and performance expectations, click here (Links to an external site.)Links to an external site.

Unit 1: Discovering New Worlds

Unit OVERVIEW


Students will independently use their learning to answer the questions, “What makes Earth ideal for life? Are there other Earth-like planets out in space?” For almost 12,000 years, Earth has been an ideal place for humans and other living things to evolve. But a once very livable Earth is becoming less livable due to human-caused stresses to Earth’s systems. After brainstorming possible solutions, students investigate the possibility of finding another Earth-like home in our galaxy. Students develop a model to explain what makes Earth an ideal place for us to live based on patterns observed at different scales in data from simulations related to the stability of stars, planet formation, and planetary motion. They then use their models and explanations to consider other solar systems and to argue from evidence about which exoplanet is most Earth-like. This unit is from New Visions and has received the NGSS Design Badge Links to an external site. for high-quality instructional materials. 

Standards

HS-ESS1-1 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.

HS-ESS1-2 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. 

HS-ESS1-3 Communicate scientific ideas about the way stars, over their life cycle, produce elements.

HS-ESS1-4 Use mathematical or computational representations to predict the motion of orbiting objects in the solar system.

Resources

Coming soon!

Link to Unit 1 Resources

 

Unit 2: Earth's History

Unit OVERVIEW


Students will formulate answers to the questions: “Why do the continents move?” and “How do people reconstruct and date events in Earth’s planetary history?” An important aspect of Earth and Space science involves making inferences about events in Earth’s history based on plate tectonics and data record that is increasingly incomplete the farther you go back in time. A key to Earth’s history is the coevolution of the biosphere with Earth’s other systems, not only in the ways that climate and environmental changes have shaped the course of evolution but also in how emerging life forms have been responsible for changing Earth. A mathematical analysis of radiometric dating is used to comprehend how absolute ages are obtained for the geologic record. Students will construct explanations for the scales of time over which Earth processes operate. The crosscutting concepts of patterns and stability and change are called out as organizing concepts for these disciplinary core ideas.  In the HS History of Earth performance expectations, students are expected to demonstrate proficiency in developing and using models, constructing explanations, and engaging in argument from evidence; and to use these practices to demonstrate understanding of the core ideas.

 

Standards

HS-ESS1-5: 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.

HS-ESS1-6: 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.

HS-ESS2-1: 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.

HS-ESS2-2: Analyze geoscience data to make the claim that one change to Earth’s surface can create feedbacks that cause changes to other Earth systems.

HS-ESS2-3: Develop a model based on evidence of Earth’s interior to describe the cycling of matter by thermal convection.

HS-ESS2-7: Construct an argument based on evidence about the simultaneous coevolution of Earth’s systems and life on Earth.

Resources

Coming soon!

Link to Unit 3 Resources

 

Unit 3: Earth's Systems

Unit OVERVIEW


Students will be able to use their learning to independently formulate answers to the questions: “How do the major Earth systems interact?” and “How do the properties and movements of water shape Earth’s surface and affect its systems?” Students can develop models and explanations for the ways that feedbacks between different Earth systems control the appearance of Earth’s surface. Central to this is the tension between internal systems, which are largely responsible for creating land at Earth’s surface (e.g., volcanism and mountain building), and the sun-driven surface systems that tear down the land through weathering and erosion.Through the Howard County Watershed Report Card program, students will be able to collect and analyze data on the Howard County Watershed in their schoolyard and at a local stream. Students understand the role that water plays in affecting weather. Students understand chemical cycles such as the water and carbon cycle. Students can examine the ways that human activities cause feedbacks that create changes to other systems. The crosscutting concepts of energy and matter; structure and function; stability and change; interdependence of science, engineering, and technology; and influence of engineering, technology, and science on society and the natural world are called out as organizing concepts for these disciplinary core ideas. In the HS. Earth’s Systems performance expectations, students are expected to demonstrate proficiency in developing and using models, planning and carrying out investigations, analyzing and interpreting data, and engaging in argument from evidence; and use these practices to demonstrate understanding of the core ideas.

 

Standards

HS-ESS2-1: 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.

HS-ESS2-2: Analyze geoscience data to make the claim that one change to Earth’s surface can create feedbacks that cause changes to other Earth systems.

HS-ESS2-5: Plan and conduct an investigation of the properties of water and its effects on Earth materials and surface processes.

HS-ESS3-1: Construct an explanation based on evidence for how the availability of natural resources, occurrence of natural hazards, and changes in climate have influenced human activity. 

Resources

Coming Soon!

Link to Unit 3 Resources

 

 

Unit 4: Weather & Climate Change

Unit OVERVIEW


Students will formulate an answer to the questions: “What regulates weather and climate?”, “How do humans depend on Earth’s resources?” and “How do people model and predict the effects of human activities on Earth’s climate?” Students understand the system interactions that control weather and climate, with a major emphasis on the mechanisms and implications of climate change. Students understand the analysis and interpretation of different kinds of geoscience data allow students to construct explanations for the many factors that drive climate change over a wide range of time scales. Students also understand the complex and significant interdependencies between humans and the rest of Earth’s systems through the impacts of natural hazards, our dependencies on natural resources, and the environmental impacts of human activities.The crosscutting concepts of cause and effect and stability and change are called out as organizing concepts for these disciplinary core ideas. In the HS. Weather and Climate performance expectations, students are expected to demonstrate proficiency in developing and using models and analyzing and interpreting data; and to use these practices to demonstrate understanding of the core ideas. Students will demonstrate proficiency in constructing explanations and designing solutions, and engaging in argument from evidence; and use these practices to demonstrate understanding of the core ideas.

 

Standards

HS-ESS2-2: Analyze geoscience data to make the claim that one change to Earths surface can create feedbacks that cause changes to other Earth systems.

HS-ESS2-4: Use a model to describe how variations in the flow of energy into and out of the Earths systems result in changes in climate.

HS-ESS2-6: Develop a quantitative model to describe the cycling of carbon among the hydrosphere, atmosphere, geosphere, and biosphere.

HS-ESS3-1: Construct an explanation based on evidence for how the availability of natural resources, occurrence of natural hazards, and changes in climate have influenced human activity.

HS-ESS3-4: Evaluate or refine a technological solution that reduces impacts of human activities on natural systems.

HS-ESS3-5: Analyze geoscience data and the results from global climate models to make an evidence-based forecast of the current rate of global or regional climate change and associated future impacts to Earth systems.

HS-ESS3-6: Use a computational representation to illustrate the relationships among Earth systems and how those relationships are being modified due to human activity.

Resources

Coming soon!

Link to Unit 4 Resources

 

This course content is offered under a  CC Attribution Non-Commercial Share Alike Links to an external site. license. Content in this course can be considered under this license unless otherwise noted.