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The Archean Era of Precambrian Time
Chapter 11 The Archean Era of Precambrian Time
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Guiding Questions When and how did Earth and its moon come into being?
How did the core, mantle, crust form? Where did Archean rocks form, and what is their nature? When and why did large continents begin to form? Where did life arise and what kinds of life existed at the end of Archean time? Why did relatively little free oxygen accumulate in Earth’s atmosphere through Archean time?
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Precambrian Archean Precambrian Time prior to Phanerozoic Era
Archean Eon 4.6–2.5 billion years ago Proterozoic Eon
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Precambrian Geology Cratons Precambrian shield
Large under-formed portions of continents Primarily Precambrian Precambrian shield Craton exposed at surface Canadian Shield exposed by glaciation
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Precambrian Geology Continental crust formed during Archean
High heat flow required small continents
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Origin of the Universe Provide important information concerning age of Earth Fragments of larger bodies that have undergone collision and broken into pieces
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Origin of the Universe Stony meteorites Iron meteorites
Rocky composition Iron meteorites Metallic composition Stony-iron meteorites Mixture of rocky and metallic Proxy for core composition Most date around 4.6 billion years ago
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Origin of the Universe Stars cluster in galaxies Milky Way
Organized in disks Milky Way Our galaxy of stars
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Origin of the Universe Expanding universe Big Bang Galaxies move apart
Redshift Originally concentrated into a single point Big Bang 15 billion years ago Age of universe
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Origin of the Universe Galactic matter is concentrated Stars form
Our Sun Supernova Exploding star Solar nebula Dense rotational cloud
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Origin of the Solar System
Planets formed near time of sun’s formation 4.6 billion years ago Planets far from sun are formed from volatile elements Planets close to sun are rocky
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Origin of the Solar System
Rocky debris Collided to form aggregates Aggregates collided to form asteroids 40 km diameter Some coalesced to form planets
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Origin of Earth and Moon
Earth materials differentiated Dense at center Less dense silicates rose to surface Magma ocean Cooled to form crust Meteorite impacts increased concentrations of some elements in upper Earth
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Origin of Earth and Moon
Moon formed from impact Mantle of impacting body Proportions of Fe and Mg differ from Earth’s mantle
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Origin of Earth and Moon
Early atmosphere Degassing from volcanic emissions CH4 and NH3 abundant Little O2 No photosynthesis Earth’s oceans Volcanic emissions cooled, condensed Salts Carried to sea by rivers and introduced at ridges Approximately constant through time
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Origin of Earth and Moon
Moon’s maria Originally thought to be seas Craters formed by asteroids Floored by basalts Craters 3.8–4.6 billion years old Earth also impacted Tilted Earth 23.5°
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Origin of Earth and Moon
Heat Flow Decreased through time Indicates abundant hot spots, small lithospheric fragments
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Origin of Continents First crust Felsics differentiated
Basalt (oceanic) Felsics differentiated Formed nuclei of continental crusts Iceland Modern analogue
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Origin of Continents Small Archean fragments Zircon crystals
High heat flow limited continental thickness Zircon crystals 4.1–4.2 B years old Weathered from felsic rocks Canadian Shield 3.8–4.0 B years old
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Origin of Continents Greenstone belts Weakly metamorphosed
Abundant chlorite Green color Nested in high-grade felsic metamorphic rocks
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Origin of Continents Greenstone belts contain igneous rocks
Volcanics contain pillow basalts Underwater extrusion Formation of sediments in deep water Graywackes, mudstones, iron formations, volcanic sediments
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Origin of Continents Banded iron formations 3 Billion years old
Isua, southern Greenland
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Origin of Continents Continental accretion
Deep water sediments accreted to continent Marine sediments form wedge between continental masses
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Archean Life Earth is best suited known planet
Conditions right by 4.2 Billion years Western Australia organic compounds 3.5 Billion years Mars Water flowed once Life may have evolved separately
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Archean Life South African cherts contain possible mold of prokaryotic cell 3.4 Billion years Oldest unquestionable life form 3.2 Billion years old Australia Intertwined filaments
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Archean Life Stromatolites Biomarkers for cyanobacteria
3.5 Billion years Suggest photosynthesis Biomarkers for cyanobacteria 2.7 Billion years
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Archean Life Miller and Urey Modeled primitive atmosphere
Produced amino acids found in proteins Modeled primitive atmosphere Added lightning Included oxygen Amino acids found in meteorites
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Archean Life RNA world Foundation for DNA world Nucleic acid
Can replicate itself May have been catalyst for production of key proteins Foundation for DNA world
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Archean Life Sulfur reduction Mid-ocean ridges Methane production
S + H2 − > H2S + energy Methane production CO2 + 4H2 − > CH4 + 2H2O + energy Mid-ocean ridges High heat Chemosynthetic organisms Hydrogen oxidation 2H2 + O2 − > 2H2O + energy
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Archean Life Ridges offer wide range of temperatures
Organic compounds readily dissolve in warm water Protection from ultraviolet radiation Abundant phosphorous Contain metals Contain clays
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Archean Life Atmospheric Oxygen Sink Low concentrations early on
Later, O2 released through photosynthesis Sink Reservoir that grows so as to take up a chemical as it is produced Early crust was sink for O2 Pyrite (FeS2) transported but not oxidized
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