Chapter 3: Orbits and Gravity
Newton's laws showed that objects at rest stay at rest, and those in motion keep moving in a straight line unless acted on by a force. It is gravity that dictates the motion of the planets around the Sun.
Newton's laws showed that objects at rest stay at rest, and those in motion keep moving in a straight line unless acted on by a force. It is gravity that dictates the motion of the planets around the Sun.
By the end of this section, you will be able to:
Kepler's laws describe the shape and speed of a planet's orbit around the Sun — the geometry behind today's eclipse lecture.
A wonderful question to start with. As you watch, listen for how the phases of the Moon line up with what we actually see in the sky1.
Anytime. When the video wraps, say the word and I'll quiz you on the eclipse geometry.