This is part 7 of an 8 part session series on Star Evolution. Find Part 1 here.
By using computer animations students will explore two main energy production cycles of stars to understand how hydrogen is converted into helium and energy is released.
Age Range: 14 – 17 years
Prep. Time: Zero, if Activity 2 is done before
Lesson Time: 20 mins
Cost per activity: Printing of student’s worksheets
Includes the use of: Computer for each group of students