Activity 01
Inquiry Circle: Kepler's Third Law from Planetary Data
Student groups are given orbital period and radius data for the eight planets and calculate the ratio T squared divided by r cubed for each. They verify that the ratio is constant across planets, identify the physical meaning of the constant (which involves G and the Sun's mass), and discuss why this relationship is a direct consequence of Newton's gravitational law.
Analyze the conditions required for an object to maintain a stable orbit.
Facilitation TipDuring Collaborative Investigation: Kepler's Third Law from Planetary Data, circulate to ensure groups plot T² vs. r³ correctly, as errors here derail the entire activity.
What to look forPresent students with two scenarios: Satellite A orbits Earth at 500 km altitude, and Satellite B orbits at 1000 km altitude. Ask students to write: 1. Which satellite has a faster orbital velocity and why? 2. Which satellite has a shorter orbital period and why?