Week 3: The Moon, Phases, and Different Sides

 

  1. What did you do in lab today?

    1. We did an experiment looking into why the front and back sides of the moon look different and why different parts of the moon have thicker crusts than others. We got to experiment with different thicknesses of the moon's crust to see how craters are created. 

  2. What was the big question?

    1. Why does the moon have two very different-looking sides? 

  3. What did you learn in Thursday’s discussion?

    1. Earth facing side of the Moon is 200 degrees warmer 

    2. There is gravity on the moon, but it is just a lot less than there is on Earth 

    3. There are many different theories on how the moon was created 

    4. The moon is in its new moon phase just before and after a solar eclipse 

    5. The moon is about the size of the United States 

  4. Read chapter 3 of the online textbook.

    1. What did you learn?

      1. I learned that the moon has craters because it lacks an atmosphere to protect it from impact, and there is no weather to erode the craters away. I also learned that the Moon’s gravity causes tides in the ocean. I have been to the ocean multiple times, and I never knew what caused high tide and low tide. 

    2. What was the most helpful?

      1. I found the image that shows the position of the Moon, Earth, and Sun during all the different moon phases very helpful. I am a visual learner, so this was helpful in showing me where each of these is instead of someone just telling me. We talked about moon phases in lab today, which emphasized the different positions for each phase. 

    3. What do you need more information on?

      1. I do not need any more information on anything from the textbook. I think this chapter was very well written and provided a lot of details and information about what we talked about in this week's lab. 

  5. What questions, concerns, and/or comments do you have?

    1. I do not have any questions, concerns, and/or comments after this week’s lecture and lab.

Comments

Post a Comment

Popular posts from this blog

Week 5: Stars, Galaxies, and the Origin of our Solar System

  What did you do in lab today? Today in lab, we started out by all sharing our presentations. My group's presentation was on black holes. The other presentations were on life cycles of stars, galaxies, meteors, meteorites, and craters, and our solar system.  What was the big question? What are the life cycles of stars, galaxies, black holes, and inner and outer planets?  What did you learn in Thursday’s discussion? When our sun turned on, it likely blew all of the gases off the inner four planets  Red giants burn fuel and lose mass, therefore increasing in size due to less mass  Three primary shapes of galaxies Spiral  The Milky Way  Elliptical Irregular  There are over 2 trillion galaxies  Black holes are the center of galaxies  There are 143 known moons surrounding the outer planets Read chapter 5 of the online textbook. What did you learn? I learned that Hayley’s comet has a return date predicted for the middle of the year in 2061. ...
Read more

Week 4: Scale Model Solar System

Image
  What did you do in lab today? Today in lab, we created a scale to represent the distance between the first 4 planets, the sun, and the moon. This scale helped us understand how small the planets and the moon are compared to the sun. It also helped show us the distance between them. We made our planets out of playdough, and then used a measuring tape to measure out the distance. We place our planets all around the bottom floor of Lindquist.  What was the big question? What we think vs. what is real What did you learn in Thursday’s discussion? Origin of the Universe (Big Bang) A subatomic particle inflated to an unimaginably huge size in a fraction of a second  Expansion, not an explosion  Earth was created 4.65 billion years ago - not in the Big Bang  Dust and debris - most likely from a former star that exploded  Read chapter 4 of the online textbook. What did you learn? I learned that the four inner planets’ surfaces are rocky, and the four outer planets...
Read more

Week 14: Science of Climate Change

  What did you do in lab today? We looked into how much carbon dioxide is in the atmosphere. We learned how they figured out how much carbon dioxide was in the atmosphere. It has been increasing over time, leading to an increase in temperature.  PhET Simulation  CH4  Visible photons do not get stopped Not all infrared photons get stopped, but some of them do and then get “spit” back out  CO2 The visible photons just go right through it and do not get stopped Not all infrared photons get stopped, but some of them do and then get “spit” back out  H2O The visible photons just go right through it and do not get stopped Not all infrared photons get stopped, but some of them do and then get “spit” back out  N2 The visible photons and infrared photons do not get stopped and go right through  O2 The visible photons and infrared photons do not get stopped and go right through  Greenhouse ga s: a gas that absorbs and re-emits infrared light  CH4 C...
Read more