Star Light, Star Bright, How Did You Get There?
This is the last part of the evidence of the Big Bang Theory. Students will learn of nucleosynthesis and the products of the big bang. They will watch videos and engage in activities that model the big bang and nucleosynthesis. This is part of a series of lessons.
Lesson Grade Level
10th GradeLesson Plan Link/URL
https://docs.google.com/presentation/d/1OuX9VjYsGHyD3uC9ppUkN2fEDDWab_yHH8yzwUA…Subject Area
Science Earth and Space Science E2: Earth & the Universe Engineering S4: Apply Science to EngineeringRelated Content
In this lesson, students use the Kepler’s Laws PhET Simulation to collect data on the period and average radius of the planetary orbits. They graph and analyze that data to derive Kepler’s 3rd Law.
This is a high-school level hands-on project that allows students to build their own working sundial, make predictions and assess their accuracy. This lesson ties in with the study of Kepler's Laws.
Problem - Solution is a type of text structure. The objective of this lesson is for students to further understand defining problems and identifying solutions. Students will make a 3D model using