Unit 4: Solar System
Duration of Days: 30
Students will know how to:
-Explain the formation of the solar system using the nebular hypothesis supported by observational evidence
-Analyze how gravity governs the motion of planets, moons, asteroids, and comets within the solar system
-Use mathematical and conceptual models to describe orbital motion, including Kepler’s laws and Newtonian gravity
-Interpret data on planetary motion to compare orbital characteristics such as period, distance, and velocity
-Compare and contrast terrestrial and gas giant planets using composition, density, and atmospheric properties
-Explain how solar system bodies formed and differentiated over time
-Analyze how space exploration and observational data have improved understanding of the solar system
Core Topics
-Solar system formation and protoplanetary disk development
-Gravitational forces and orbital motion
-Kepler’s Laws of Planetary Motion (conceptual and data-based application)
-Newton’s Law of Universal Gravitation (qualitative and quantitative reasoning)
-Planet classification and comparative planetology
-Asteroids, comets, and dwarf planets
-Space exploration and observational astronomy
NGSS Performance Expectations
HS-ESS1-1 – Develop and use models of the solar system based on gravitational interactions and formation evidence
HS-ESS1-4 – Use data from observations of solar system objects to explain formation and evolution
HS-PS2-4 – Use Newton’s laws to explain and predict orbital motion
Essential Questions students will be able to answer:
-How did the solar system form from a rotating disk of gas and dust?
-How does gravity control the motion of objects in the solar system?
-How do Kepler’s Laws describe planetary motion, and what data supports them?
-Why do planets have different compositions and structures?
-How do orbital characteristics change with distance from the Sun?
-How do comets, asteroids, and dwarf planets differ from major planets?
-How has space exploration changed our understanding of the solar system?
Science and Engineering Practices (SEPs):
-Developing and Using Models
-Analyzing and Interpreting Data
-Using Mathematics and Computational Thinking
-Constructing Explanations
Crosscutting Concepts (CCCs):
-Scale, Proportion, and Quantity
-Patterns
-Cause and Effect
-Systems and System Models
Demonstration of Learning
-Unit test with orbital motion and planetary data analysis
-Planet comparison using density, composition, and atmospheric data sets
-Orbital simulation labs modeling gravity and motion relationships
-Analysis of Kepler’s Laws using real or simulated planetary data
-Solar system formation modeling activity
-CER explaining how gravity shaped the structure of the solar system
| Lesson # | Lesson Title | Duration of Days |
|---|---|---|
| 1 | Origins of the Solar System | 5 |
| 2 | Planetary Formation and Differentiation | 10 |
| 3 | Moons, Asteroids, and Comets | 5 |
| 4 | Orbital Mechanics and Planetary Motion | 5 |
| 5 | Comparing Planetary Systems | 5 |