Origin of the Universe
and Our Solar System
Introduction to Earth Science
Origin of the Universe
and Our Solar System
Introduction to Earth Science
Literacy / Driving Question Board Connections
Nonfiction Science Literacy Resources
Graphic Organizers / Thinking Maps
Driving Question Boards
Multilingual Learner Language Expectations
Origin of the Universe and Our Solar System Chapters
Unit Standards
What is the NGSS & 3 Dimensional Science Learning and Why is it Important?
Science Practices - Disciplinary Core Ideas - Crosscutting Concepts
Clarification Statement: Emphasis is on the energy transfer mechanisms that allow energy from nuclear fusion in the sun’s core to reach Earth. Examples of evidence for the model include observations of the masses and lifetimes of other stars, as well as the ways that the sun’s radiation varies due to sudden solar flares (“space weather”), the 11-year sunspot cycle, and non-cyclic variations over centuries.
Boundary Statement: Assessment does not include details of the atomic and sub-atomic processes involved with the sun’s nuclear fusion.
Clarification Statement: Emphasis is on the astronomical evidence of the red shift of light from galaxies as an indication that the universe is currently expanding, the cosmic microwave background as the remnant radiation from the Big Bang, and the observed composition of ordinary matter of the universe, primarily found in stars and interstellar gases (from the spectra of electromagnetic radiation from stars), which matches that predicted by the Big Bang theory (3/4 hydrogen and 1/4 helium).
Boundary Statement: none
Clarification Statement: Emphasis is on the way nucleosynthesis, and therefore the different elements created, varies as a function of the mass of a star and the stage of its lifetime.
Boundary Statement: Details of the many different nucleosynthesis pathways for stars of differing masses are not assessed.
Clarification Statement: Emphasis is on Newtonian gravitational laws governing orbital motions, which apply to human-made satellites as well as planets and moons.
Boundary Statement: 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.
Learning Objectives / Career Connections
By the end of this chapter, students should be able to:
Explain the formation of the universe and how we observe it.
Understand the origin of our solar system.
Describe how the objects in our solar system are identified, explored, and characterized.
Describe the types of small bodies in our solar system, their locations, and how they formed.
Describe the characteristics of the giant planets, terrestrial planets, and small bodies in the solar system.
Explain what influences the temperature of a planet’s surface.
Explain why there is geological activity on some planets and not on others.
Describe different methods for dating planets and the age of the solar system.
Describe how the characteristics of extrasolar systems help us to model our own solar system.
Using ChatGPT to find local Colorado Phenomena
Use the following prompt, adjust accordingly. "I am a high school science teacher looking for a local Colorado phenomena to address NGSS standard (enter standard you are looking for... example HS-LS1-6)"
Career Connections
Connecting what students are learning to careers not only deepens their engagement in school but also helps them make more informed choices about their future. Browse the following related career profiles to discover what scientists really do on the job and what it takes to prepare for these careers. For additional profiles visit your Year at a Glance Page.
Hands On, Minds On Connections
Hands-On Labs / Lab Safety
Complete List of SAVVAS Labs and Activities
Lab Materials List
PASCO
St Vrain Science Center
Simulations
GIZMOS
Nearpod Lessons / Activities / Videos
LabXchange Lessons / Activities / Videos