Differences
This shows you the differences between two versions of the page.
Both sides previous revision Previous revision Next revision | Previous revision Next revisionBoth sides next revision | ||
course_planning:183_projects:s23_week_3_geostationary_orbit [2023/01/25 19:51] – hallstein | course_planning:183_projects:s23_week_3_geostationary_orbit [2023/01/25 20:14] – hallstein | ||
---|---|---|---|
Line 102: | Line 102: | ||
* **Tutor Question: | * **Tutor Question: | ||
* **Expected Answer: | * **Expected Answer: | ||
- | |||
- | {{course_planning: | ||
</ | </ | ||
Line 185: | Line 183: | ||
<WRAP alert> | <WRAP alert> | ||
- | The addition of the non-constant Newtonian force is challenging for students. | + | The addition of the non-constant Newtonian force is challenging for students. |
</ | </ | ||
<WRAP tip> | <WRAP tip> | ||
==Tutor Questions: | ==Tutor Questions: | ||
- | * **Question: | + | * **Question: |
- | * **Expected Answer: | + | |
- | Aside from just eyeballing it, we can add in a graph of the distance from the center of Earth! (Moved to separate part C of the problem) | + | |
- | <code python> | + | |
- | # | + | |
- | separationGraph = PhysGraph(numPlots=1) | + | |
- | + | ||
- | # | + | |
- | separationGraph.plot(t, | + | |
- | </ | + | |
- | + | ||
- | | + | |
* **Expected Answer: | * **Expected Answer: | ||
Line 210: | Line 197: | ||
* **Expected Answer: | * **Expected Answer: | ||
- | {{course_planning:georobitconceptualq2.png}} | + | * **Question:** How can you prove that the orbit is actually circular? |
+ | * **Expected Answer: | ||
+ | Part C includes adding this graph: | ||
+ | |||
+ | <code python> | ||
+ | # | ||
+ | separationGraph = PhysGraph(numPlots=1) | ||
+ | |||
+ | # | ||
+ | separationGraph.plot(t, | ||
+ | </ | ||
</ | </ | ||
Line 218: | Line 215: | ||
* Groups should have developed a working code that models any gravitational orbit around the Earth and be able to explain what and how they did it. | * Groups should have developed a working code that models any gravitational orbit around the Earth and be able to explain what and how they did it. | ||
- | * For groups that get through this part (it's tough for many groups), they should check that the orbit is circular and explain that and they should add arrows to represent different physical quantities (i.e., momentum of the satellite, etc.). | + | * For groups that get through this part (it's tough for many groups), they should check that the orbit is circular and explain that and they should add arrows to represent different physical quantities (i.e., |
</ | </ | ||
Line 284: | Line 281: | ||
Changes made to the given code: | Changes made to the given code: | ||
+ | {{course_planning: | ||
====== Project 3: Part C: Geostationary orbit ====== | ====== Project 3: Part C: Geostationary orbit ====== | ||
Line 366: | Line 364: | ||
Modification of solution to part B to get |r| vs t, |Fnet| vs t and Fnet,x and P,x vs t: | Modification of solution to part B to get |r| vs t, |Fnet| vs t and Fnet,x and P,x vs t: | ||
+ | {{course_planning: | ||