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Universe and global climate — Foundational
Level 1: Foundational
Identify, describe, state, calculate — recall facts and use standard relationships (typical early Year 10).
Redshift of light from distant galaxies is most often interpreted as evidence that:
The cosmic microwave background is important because it:
The Big Bang model in science primarily describes:
Light-element abundances (especially hydrogen and helium) support early-universe ideas because:
Which set names the four spheres used in energy-flow models related to climate?
Greenhouse gases in the atmosphere matter for climate mainly because they:
Albedo refers to:
The hydrosphere includes:
Stars are important in models of the universe partly because they:
Fossil fuels connect to the carbon cycle because they:
In Earth-systems models of climate, the geosphere refers broadly to:
Hubble’s law links galaxy recession speed to distance in a linear picture. It supports:
Astronomers use galaxies and their spectra across the sky when studying cosmic history because:
The lower atmosphere is mostly nitrogen and oxygen by volume; trace gases such as CO₂ still matter for climate because:
Thermal expansion of seawater as it warms contributes to:
Photosynthesis moves CO₂ into organic matter; respiration and decay return carbon. In the fast surface carbon cycle this mainly affects:
Latitude affects climate partly because:
Permafrost thaw can feed back to climate because it may release:
Ocean acidification is tied to rising atmospheric CO₂ because more CO₂ dissolves and shifts seawater carbonate chemistry, lowering pH. This mainly concerns the:
The Coriolis effect influences large-scale winds and currents because:
El Niño–Southern Oscillation is an example of:
Deforestation can alter climate forcing partly by changing: