Methods II- Week 7
1.) The big question addressed in lab, and a description of what you did.
We talked a lot about the different size comparisons of each planet, plus the sun and the moon. We watched a video that showed just how large each one was which was really spooky to be honest. Then with our table groups we made a scale of about how big and how far the planets were from each other. We used Play-Doh and a measuring device to know the distance and scale.
2.) A description of what you learned in Thursday's lecture.
Some of the things we talked about Thursday
- Gibbous is never going to be an answer on the test.
- The moon has a rotation and a revolution that are identical which makes us only see the one side of the moon.
- Something called Thea hi the earth directly and some got absorbed and some bounced back, that’s why we have a tilt on an axis. - You weigh 1/6th your weight on the moon.
- The moon is about 2/4 the size of the earth so the size of the U.S is the closest comparisons.
- Capture Theory: Physics says you can’t.
- Fission Theory: This is where the Pacific Ocean came from.
- The earth was spinning so fast that a chink of it flew out into space.
- Co-formation: They formed the same time they have the same material.
- Colliding Planetesimals: The moon condescended from debris produced when other planets slammed into each other and formed solar systems.
- The dark side is the thicker than the other.
- The back side collided faster than the side that’s facing us.
- That allows the magma to stay closer to the surface.
3.) Answer questions about the weekly textbook reading:
1.) What did you learn?
I liked learning about the origin of the earth a little bit and how it ended up the way it is. Reading about how it tilted and what not was something that I was unaware of.
2.) What was most helpful?
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