Using the Chapter learning objectives for Chapter 3, discuss three learning objectives for Chapter 3
1. Describe how Tycho Brahe and Johannes Kepler contributed to our understanding of how planets move around the Sun.
2. Explain Kepler’s three laws of planetary motion.
3. Describe Newton’s three laws of motion.
4. Explain how Newton’s three laws of motion relate to momentum.
5. Define mass, volume, and density and how they differ.
6. Define angular momentum.
7. Explain what determines the strength of gravity.
8. Describe how Newton’s universal law of gravitation extends our understanding of Kepler’s laws.
9. Compare the orbital characteristics of the planets in the solar system.
10.Compare the orbital characteristics of asteroids and comets in the solar system.
11. Explain the following:
how an object (such as a satellite) can be put into orbit around Earth.
how an object (such as a planetary probe) can escape from orbit.
how the gravitational interactions of many bodies can cause perturbations in their motions.
how the planet Neptune was discovered.
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