Lecture 20 – Jovian Planets, Part 2/2
Summary / Checklist of the Main Concepts to Understand and Remember
Uranus | ||
How far is Uranus from the Sun on average, in AU? | ||
Can Uranus be seen without a telescope? | ||
• | How wide is it, compared to Earth? What is Uranus' surface like, and why? | |
What is special about Uranus' rotation, and how do we think it came to be that way? | ||
Which spacecraft from Earth has flow by Uranus and taken pictures? | ||
• | Moons: Approximately how many? What is special about the moon Miranda? | |
• | Rings: Does Uranus have any? What are they like (compared to Saturn's)? | |
Neptune | ||
How far is Neptune from the Sun on average, in AU? | ||
Can Neptune be seen without a telescope? How was Neptune discovered? | ||
• | How wide is it, compared to Earth? What is Neptune's surface like, and why? | |
Which spacecraft from Earth has flow by Neptune and taken pictures? | ||
• | Moons: Approximately how many? What is special about the moon Triton? | |
• | Rings: Does Neptune have any? What are they like (compared to Saturn's)? | |
Topics from the lecture page and textbook not listed above [or between square brackets]
were not covered in class;
Underlined words indicate that I will expect students to remember a number or a name related to that topic.
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