Earth’s Processes and Biosphere Development

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Vocabulary flashcards covering key terms from Module 5: Earth’s Processes—origin of organic molecules, hydrothermal vents, panspermia, photosynthetic life evidence, multicellularity, land colonisation, and biosphere-driven changes to Earth’s spheres.

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33 Terms

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Urey–Miller Experiment

1953 laboratory simulation of early-Earth conditions that produced organic molecules from inorganic gases.

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WHAM Gases

Water vapour, Hydrogen, Ammonia and Methane—the gas mixture used in the Urey–Miller experiment.

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Early-Earth Lightning Simulation

Electric sparks (electrodes) used by Urey and Miller to mimic lightning as an energy source for prebiotic chemistry.

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Black Smokers

Mineral-rich hydrothermal vent chimneys on mid-ocean ridges that provide heat and chemicals for early life.

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Chemosynthesis

Process by which organisms make food using inorganic chemicals (e.g., H₂S) instead of sunlight.

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Archaebacteria

Anaerobic, extremophilic prokaryotes that obtain energy via chemosynthesis; inhabit black smokers today.

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Catalytic Clay & Metal Deposits

Particles at hydrothermal vents that speed up chemical reactions forming complex molecules.

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Panspermia

Hypothesis that amino acids or life’s precursors arrived on Earth aboard meteorites; lacks mechanism for initial synthesis.

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Cyanobacteria

First photosynthetic, oxygen-producing prokaryotes; evolved >3.5 billion years ago.

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Stromatolites

Layered limestone structures formed by colonies of cyanobacteria trapping sediment.

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Strelley Pool Fossils

3.4 billion-year-old fossilised stromatolites in Western Australia evidencing early photosynthesis.

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Photosynthesis Equation

CO₂ + H₂O → C₆H₁₂O₆ + O₂ (carbon dioxide and water produce glucose and oxygen).

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End-Cryogenian Period

Time (~635 Ma) after global glaciations when multicellular life began diversifying.

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Collagen Formation

Evolution of structural protein collagen that enabled larger, complex multicellular animals.

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Ediacaran Fauna

Soft-bodied multicellular organisms (~635–541 Ma) evidencing early animal ecosystems.

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Cambrian Explosion

Rapid diversification of animal phyla (~541 Ma) leaving abundant mineralised fossils.

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Terrestrial Advantages

Fewer predators, more resources, and stable conditions that encouraged life’s move onto land.

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Terrestrial Challenges

UV radiation, desiccation, and gravity obstacles faced by early land colonisers.

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Ozone Layer

Stratospheric O₃ shield blocking harmful UV, enabling terrestrial life.

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Arthropods (First Land Animals)

Centipedes, trilobites and relatives whose exoskeletons prevented water loss; footprints give fossil evidence.

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Plant Adaptation—True Roots

Organs evolved to absorb water/nutrients from soil, improving anchorage and resource uptake.

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Plant Adaptation—Seeds

Water-independent reproductive units allowing dispersal and embryo protection on land.

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Plant Adaptation—Woody Stems

Lignified support tissues that counter gravity and allow vertical growth.

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Animal Adaptation—Internal Fertilisation

Reproductive strategy reducing water dependence by fertilising eggs inside the body.

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Animal Adaptation—Leathery (Amniotic) Eggs

Watertight shells protecting embryos from desiccation; key to reptile success on land.

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Amphibian Dual Respiration

Use of gills in larval stage and lungs/skin as adults to exploit both aquatic and terrestrial habitats.

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Hydrosphere Change from Cyanobacteria

Decrease in CO₂, rise in O₂, and removal of Fe²⁺ ions through precipitation of iron oxides.

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Atmospheric Change from Cyanobacteria

Drop in CO₂ and CH₄, accumulation of O₂ after ocean saturation, altering greenhouse balance.

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Geosphere Change—BIFs

Formation of banded iron formations as iron oxides settled onto the seafloor.

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Proterozoic Acid Rain Weathering

Rain containing carbonic acids leached soluble iron ions from continental rocks into oceans.

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Iron Oxide Precipitation

Reaction of O₂ with Fe²⁺ to form insoluble hematite/magnetite that sank as sediment layers.

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Chert Layers

Silica-rich, iron-poor sediment bands deposited when oxygen levels temporarily fell.

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Cyclic BIF Formation

Alternating iron-rich and silica-rich layers produced by fluctuating cyanobacterial oxygen production.