Concepts:
Q: The orbital period of the Earth is about 365 days, what is this?
A: one year
Q: How long is a year on Venus?
Q: How old are you in Mars years?
Q: How many Earth years go by before one Jupiter year has passed?
Q: What trends do you notice in looking at your graph of orbital period vs. distance from the sun?
A: orbital period increases as distance from the sun increases
Q: Why do you think this is?
A: (hint - draw a picture) Planets farther from the sun have more distance to travel to go around the sun once -- their orbits have larger circumferences (2*pi*r).
Q: How long does it take the Earth to rotate once?
A: 24 hours
Q: What is this period of time called?
A: 1 day
Q: How long is a day on Jupiter? on Venus?
Q: What planet rotates the fastest? The slowest?
A: Jupiter, Venus
Q: Do you see any relationship between distance from sun and rotational period?
A: there isn't really any
Q: Which planets have retrograde rotations? (backwards spins)
A: Venus, Uranus, Pluto
Try this out with a beach ball and your hand: spin a beach ball (or a globe with a fixed base), and see if you can push it with your hand in the opposite direction from its spin. The spin slows down, and if you push hard enough it'll start spinning in the other direction.
Uranus is another anomaly: it not only spins backwards, but it also spins on its side, like it was hit from the side by a giant impact. The study of giant impacts and their importance in the early days of the formation of the solar system is a current field, and many scientists use clues like rotation rates and direction of spin axes to make guesses about what happened long ago.
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Galileo Solid State Imaging Team Leader: Dr. Michael J. S. Belton
The SSI Education and Public Outreach webpages were originally created and managed by Matthew Fishburn and Elizabeth Alvarez with significant assistance from Kelly Bender, Ross Beyer, Detrick Branston, Stephanie Lyons, Eileen Ryan, and Nalin Samarasinha.
Last updated: September 17, 1999, by Matthew Fishburn
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