Back to Course

Earth & Space Science

0% Complete
0/0 Steps
  1. How This Class Works
    3 Steps
  2. Unit 1: Science and the Bible

    Lesson 1: Introduction to Earth Science
    8 Steps
    |
    3 Quizzes
  3. Unit 2: Rocks and Minerals
    Lesson 2: Minerals
    7 Steps
    |
    4 Quizzes
  4. Lesson 3: The Rock Cycle and Igneous Rocks
    7 Steps
    |
    2 Quizzes
  5. Lesson 4: Sedimentary and Metamorphic Rocks
    7 Steps
    |
    2 Quizzes
  6. Lesson 5: Rock Identification Lab
    1 Step
    |
    2 Quizzes
  7. Unit 3: Tectonics and Volcanoes
    Lesson 6: Tectonics
    7 Steps
    |
    2 Quizzes
  8. Lesson 7: Geologic Forces
    7 Steps
    |
    2 Quizzes
  9. Lesson 8: Earthquakes
    9 Steps
    |
    1 Quiz
  10. Lesson 9: Volcanoes
    9 Steps
    |
    1 Quiz
  11. Unit 4: Dating, Earth History, and Noah's Flood
    Lesson 10: Relative Dating
    5 Steps
  12. Lesson 11: Absolute Dating
    8 Steps
  13. Lesson 12: Fossils
    7 Steps
    |
    1 Quiz
  14. Lesson 13: Conventional Geologic History
    3 Steps
  15. Lesson 14: Noah's Flood
    5 Steps
    |
    1 Quiz
  16. Lesson 15: Geologic History - Lab
    5 Steps
    |
    1 Quiz
  17. Lesson 16: Units 1-4 Review
    1 Step
  18. Unit 5: Earth's Surface: Water and Processes
    Lesson 17: Weathering
    6 Steps
  19. Lesson 18: Mass Wasting
    5 Steps
  20. Lesson 19: Streams
    9 Steps
    |
    1 Quiz
  21. Lesson 20: Groundwater
    4 Steps
  22. Unit 6: Earth's Features
    Lesson 21: Glaciers and Deserts
    8 Steps
  23. Lesson 22: Earth's Resources
    4 Steps
    |
    1 Quiz
  24. Lesson 23: Oceans
    4 Steps
  25. Lesson 24: Coasts
    4 Steps
  26. Unit 7: Earth's Atmosphere
    Lesson 25: Earth's Atmosphere
    4 Steps
  27. Lesson 26: Climate Change
    6 Steps
    |
    1 Quiz
  28. Lesson 27: Atmospheric Processes
    5 Steps
  29. Lesson 28: Weather
    5 Steps
    |
    1 Quiz
  30. Unit 8: Space
    Lesson 29: Our Solar System
  31. Lesson 30: Beyond Our Solar System
  32. Lesson 31: The Origin of the Universe
  33. Lesson 32: Units 5-8 Review
    1 Step
Lesson Progress
0% Complete

1. Why is the study of rocks important?  

Rocks are important for both economical and scientific reasons. They contain things like fossils and radioactive elements that help with geological dating, and they have economic minerals such as iron ore, copper, gold, and coal. Rocks also hold fluids like drinking water, crude oil, and natural gas that we use every day. (Section 3.1)  

2. Be able to sketch the rock cycle (figure 3.4) without referring to the diagram!  

The rock cycle shows how rocks change from one type to another through processes like weathering, metamorphism, melting, and recrystallization. Any rock can be weathered into sediment, which can become sedimentary rock through lithification. Heat and pressure turn rocks into metamorphic ones, and if they melt, they become magma that cools into igneous rock. The cycle was very active during creation week, Noah’s Flood, and right after the Flood. (Section 3.2)  

3. Be able to sketch and identify the different types of plutons from photographs.  

Plutons are intrusive igneous bodies that form underground. Concordant ones like sills and laccoliths are parallel to surrounding rock layers. Discordant ones like dikes cut across layers, while stocks and batholiths are larger masses. A sketch would show magma injecting into rocks, with sills horizontal, dikes vertical, and batholiths as big blobs. (Section 3.3)  

4. What are the main criteria in the identification of igneous rocks? Can you sketch out a diagram for the identification of igneous rocks?  

The two main criteria are texture and mineral composition or color. Texture includes sizes like pegmatitic (big crystals), phaneritic (visible crystals), aphanitic (tiny crystals), porphyritic (mixed sizes), glassy (no crystals), vesicular (holes), or pyroclastic (fragments). For large crystals, use minerals like quartz or olivine; for small ones, use color like light or dark. A diagram would be a table with textures on one side and compositions across the top, naming rocks like granite or basalt. (Section 3.3.1)  

5. Can you explain Bowens Reaction Series to someone who is unfamiliar with it?  

Bowen’s Reaction Series shows how minerals form as magma cools, not all at once but over a range of temperatures. It has a discontinuous branch where minerals like olivine form first at high heat, then get replaced by pyroxene, amphibole, and biotite as it cools and silica structures get more complex. A continuous branch has plagioclase changing from calcium-rich to sodium-rich. At the bottom, quartz, potassium feldspar, and muscovite form last at lower temperatures. The original magma’s chemistry decides which minerals end up in the rock. (Section 3.3.2)  

6. Why are radiohalos important in a biblical understanding of earth history?  

Radiohalos are damage scars in biotite crystals from radioactive decay of uranium and polonium, forming only below 150°C. They show up close together because hot water from cooling plutons carries polonium away from uranium quickly. This suggests large granite bodies cooled in days, fitting a young Earth and rapid processes during Noah’s Flood, not millions of years. (Box 3.1)  

7. If you heated up a granite rock and melted it, what would melt first? Second? Third?  

In reverse of Bowen’s series, the last minerals to form would melt first. Quartz would melt first, then potassium feldspar, then muscovite mica. (Section 3.3.2)