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Universe and global climate — Foundational

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Level 1: Foundational

Identify, describe, state, calculate — recall facts and use standard relationships (typical early Year 10).

  1. Redshift of light from distant galaxies is most often interpreted as evidence that:

  2. The cosmic microwave background is important because it:

  3. The Big Bang model in science primarily describes:

  4. Light-element abundances (especially hydrogen and helium) support early-universe ideas because:

  5. Which set names the four spheres used in energy-flow models related to climate?

  6. Greenhouse gases in the atmosphere matter for climate mainly because they:

  7. Albedo refers to:

  8. The hydrosphere includes:

  9. Stars are important in models of the universe partly because they:

  10. Fossil fuels connect to the carbon cycle because they:

  11. In Earth-systems models of climate, the geosphere refers broadly to:

  12. Hubble’s law links galaxy recession speed to distance in a linear picture. It supports:

  13. Astronomers use galaxies and their spectra across the sky when studying cosmic history because:

  14. The lower atmosphere is mostly nitrogen and oxygen by volume; trace gases such as CO₂ still matter for climate because:

  15. Thermal expansion of seawater as it warms contributes to:

  16. Photosynthesis moves CO₂ into organic matter; respiration and decay return carbon. In the fast surface carbon cycle this mainly affects:

  17. Latitude affects climate partly because:

  18. Permafrost thaw can feed back to climate because it may release:

  19. Ocean acidification is tied to rising atmospheric CO₂ because more CO₂ dissolves and shifts seawater carbonate chemistry, lowering pH. This mainly concerns the:

  20. The Coriolis effect influences large-scale winds and currents because:

  21. El Niño–Southern Oscillation is an example of:

  22. Deforestation can alter climate forcing partly by changing:

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