Section 1-4 Teaching Outline

Book J

Earth Science

Exploring the Planets Software:

    NASA News: Come up with three questions per team that you will ask the class.

      Slide 1: Two main features of the Moon

                1. Highlands (Terra)

                2. Lowlands (Maria)

                    Button: Compare to Earth

                    Highlighted: Highlands: older and heavily cratered

                    Highlighted: Cratered: Cratered
                                    Caldera: Caldera:no raised rims

                    Highlighted Maria: Basaltic Lava Flows, (seas)
                            EX: Basalt samples from earth

                        Highlighted Basalt:

                        Highlighted: Mare: singular of Maria

                               Highlighted:  Basaltic Lava
       Slide 2: Features found on the moon. Craters, Volcanic Flows, Tectonic Features, No Atmosphere, No water.

                    Highlighted: Tectonic: The folding and faulting of a planets crust.

                    Highlighted: Atmosphere: the sphere of gas surrounding a planet including water vapor

       Slide 3: The Far side of the moon

                    Only photographed from space craft. Why?

                    Older and more cratered than the Earth side of the Moon.

       Slide 4: The orbit, Rotation and Revolution of the Moon.

            Why are they the same?

       Slide 5: There were six mission to the Moon. 3 Astronauts per mission. 2 astronauts per mission went to

the surface. Discuss Lunar Command Module and Lunar Lander     Highlighted: Regolith: the broken pieces of rocks and minerals that make up a planets surface.        Slide 6: Since there is no air or atmosphere on the moon there is no sounds. You couldn't hear someone scream or an avalanche or a meteor impact. You might feel the vibration through your feet.        Slide 7: There is also no weather on the Moon so footprints or craters will remain for thousands or millions of years. Nothing to wash or blow them away.        Slide 8: Button: Replay:
                    Gravity on the moon is 1/6th the gravity of Earth.

        Assignment: calculate your weight on the Moon. Divide your weight by 6.

How much would you weigh with a 160 lbs space suite on?        Slide 9: Cratering before 3.8 billion years ago was very intense.The solar system was full of rock and ice that the planets smashed into as they traveled
                    around the sun. At first these impacts were very intense but over time the impacts lessened as the asteroids and comets were swept up. View video: Heaven and Hell        Slide 10: This is an image of an average moon crater 85 km across, 3 km deep with 2 km mountains in the center        Slide 11:Some extremely huge craters are also found on the moon one example is Orientale a Multiringed basin. This basin is 2500 km in diameter
    Button: Compare to Earth (it's as large as Texas)
    Highlighted: Multi-Ringed Basin
       Slide 12:The surface of the moon is covered by shattered rocks sometimes fused together by the heat of
the impacts. This type of rock is called Breccia.

    Highlighted: Breccia: rock made from the jagged broken pieces of other rocks andMinerals

    EX: Show samples of Breccia

        Slide 13: Typical highland rock is a type of plagioclase feldspar.
    EX: Feldspar
        Slide 14: For the Moon to be made up of layers of different types of rock it must have once been molten that allowed the rocks to seperate by density.

                Highlighted: Magma Ocean: 4.5 Billion years ago it was molten 4.4 Billion years ago solid crust started forming creating the early highlands

Magma
Lava
        Slide 15:Layers seperate by density

        Slide 16:After the crust cools magma flooded the low lying areas forming maria.

                Button: Compare to Earth

        Slide 17: Formation of Maria starts with a meteor impact.

        Slide 18: cracks in the crust allow Maria to flow to the surface filling low areas.

        Slide 19: Rilles: rilles are stream like valleys on the moon.
                Does the moon have water to form valleys?

                What could flow on the surface and cause valleys?

            Highlighted: Rilles: note the lunar dune buggy

            Highlighted: Lava Flows

            Button: Compare to Earth

        Slide 20:Rilles ended up being about 3 billion years old. 1.4 billion years younger than the highlands.

Rilles formed at about the same time as the maria.
 
Button: Compare to Earth: rilles are formed from channels or rivers of lava or possible collapsed lava channels
        Slide 21: Basalt vesicles. Forms like bubbles in root beer.

        Slide 22: Pyroclastic : pyro=fire, clastic=broken

             Highlighted: pyroclastic

            Button: compare to Earth

        Slide 23: The soil is made of frozen droplets of lava

        Slide 24: the orange droplets contain high amounts of titanium

        Slide 25: Highlighted: Cinder cones form from pyroclastic eruptions

                Highlighted: Compare to Earth

        Slide 26: Wrinkle Ridges: Tectonic features caused by the cooling of the Moon's crust.

                Highlighted: Wrinkle Ridges

        Slide 27: Highlighted: Landslides: gravity pulls material downward.

                Highlighted: Falls: occur at the base of cliffs

                Highlighted: Flows: flow across large flat areas on water or air.

                Highlighted:Slides: large sections of slope move down hill and pile up at the base of the slope
         Slide 28: Large flows occur on the moon and travel over many kilometers

                Highlighted: Compare to Earth. Giant flows kilometers long

        Slide 29: The Structure of the Moon

                Crust: made of Feldspar
                Mare: Basalt
                Mantle: Olivine and Pyroxene (Minerals in Basalt)
                Core: Possibly Metallic

        Slide 30: Moon Formation

        Slide 31: Formation demonstration of a major impact forming the moon.

        Slide 32: The combining of metallic cores on Earth.

        Slide 33: Summary

      1. Giant Impact
      2. Ocean of Magma
      3. Light feldspar crust forms
      4. Period of impacts
      5. Large multi-ringed basins
      6. Maria forms
      7. No wind or water erosion
      8. Light tectonic features from cooling
      9. Landslides form gravity
Slide 34: Quiz
Section 1-4 Teaching Outline
Book J
Earth Science

Earth’s Moon pp. 39-44

Activating Prior Knowledge

Hold up a rock.

Have them imagine that this rock was the size of a large building moving through space

Have them imagine it coming through earths atmosphere and hitting the earth.

What do you think would happen?

Anticipatory Set
Discover: Why do craters look diferent from each other?

Items Used: Sand and 3 different size objects.

Procedure:

                        See steps on page 39J

Assign Reading

            Guide for Reading

Presentation The Structure and Origin of the Moon
    1. 4.5 billion years ago a large object the size of Mars struck the Earth with a Glancing Blow.
    2. This ripped off a large portion of the Earth’s molten crust.
    3. The Earth Being molten quickly reformed
    4. The blasted part of the earth still molted collected into a large droplet caught in earth’s gracity.
    5. This later became the moon
    6. This may explain why the earth does not have a full crust but a series of small continetal plates that do not completely cover the earth’s surface, which are made of basically the same material as the moon.
Looking at the Moon from Earth VIDEO. Show Cosmos Heaven and hell which shows first the tunguska comet impact and then the meteor impact on the moon. Missions to the Moon p. 42