Three Lessons on Kepler's three laws and how they manifest in STK (useful for competition)
Kepler's "0th" Law - A background lesson on the Aristotelean/Ptolemaic Universe for contrast on Kepler's work
Kepler's three Laws - A series of lessons for intro University level physics classes on Kepler's Laws
Orbiting objects move in ellipses.
Perigee Fast, Apogee Slow
Farther out, longer orbit time.
These videos show a broader understanding of Kepler's Laws of Planetary Motion not limited in scope to STK. While less functional for our Space Mission Design, these videos give a deeper understanding of the Laws themselves and are introductory lessons for University Level Physics. The video to the left is a background on Western understanding of Space before Kepler's time to give deeper context. The videos below go into greater detail of Kepler's Laws and their applications.
Ellipses - the strange shape of motion
Equal Areas in Equal Time
Period Squared over SMA Cubed