22 20 Early Earth Atmosphere and Ocean (2)
Introduction to Earth and Marine Geology (MSCI *112)
Instructor: Prof Stewart
Contact:
Phone: [Not provided]
Email: jstewar6@coastal.edu
Early Earth during the Precambrian
The Earth is approximately 4.56 billion years old.
The oldest known rocks date back to about 4.04 billion years.
The largest unit of geochronology on Earth is the Precambrian, lasting more than 4 billion years.
Precambrian is further divided into three eons:
Hadean
Archean
Proterozoic
Hadean Eon
Prelude to the Earth’s formation from approximately 4.6 to 3.8 billion years ago.
Characterized by:
Initial growth of the Earth through accretion (the process of gradual accumulation).
Formation of the Earth's core and the Earth's magnetic field.
Presence of a magma ocean approximately 400 km thick.
Formation of the crust and protocontinents, possibly indicative of early plate tectonics.
Atmospheric Conditions during the Hadean
Extremely reducing primary atmosphere containing:
Methane (CH₄)
Ammonia (NH₃)
Hydrogen (H₂)
Transition to moderately reducing secondary atmosphere composed of:
Water vapor (H₂O)
Carbon dioxide (CO₂)
Nitrogen (N₂)
Sulfur dioxide (SO₂)
Major contributors to atmospheric conditions:
Volcanic outgassing.
Condensation of water vapor leading to the formation of primitive oceans.
Formation of Oceanic Crust
First oceanic crust (mafic in composition) was formed from the cooling of the magma ocean as early as 4.3 billion years ago.
Development of small felsic protocontinents, which were thinner compared to modern continents, eventually forming the core of late continents.
Potentially Biogenic Carbon
Evidence of potentially biogenic carbon has been found in a 4.1 billion-year-old zircon.
Studies involving zircon indicate the presence of both inorganic and organic carbon.
Archean Eon
The Archean Eon spans from 3.8 to 2.5 billion years ago, marked by significant geological and biological developments:
Continued development of oceanic crust and protocontinents initiated subduction processes leading to the formation of continents.
Formation of gneiss within subduction zones.
Greenstone Belt
Characteristics of the Archean crust include the presence of greenstone belts, which are:
Comprised of large chunks of weakly metamorphosed mafic crust and deep-sea sediments.
Metamorphosed felsic (continental) crust surrounds these belts.
The term derives its name from the green hue of the metamorphic mineral chlorite.
Often originated from oceanic environments or forearc/back-arc basins.
Cratons
Definition: Cratons are the ancient, stable portions of a continent that have remained relatively unchanged for vast geological timescales.
Cratons can be categorized into:
Shields: Areas where Precambrian rocks are exposed.
Platforms: Areas with buried Precambrian rocks.
Banded Iron Formation (BIF)
Definition: Banded Iron Formations are stratified sedimentary deposits, typically consisting of alternating thin layers of chert, hematite, and magnetite, formed primarily between 3.7 and 1.8 billion years ago.
Context: Indicates the presence of dissolved iron in early oceans and serves as evidence of the oxygen produced by early photosynthetic life.
The presence of cyanobacteria likely contributed to the release of oxygen during photosynthesis, influencing the iron precipitation patterns observed in BIF deposits.
Archean Eon - Beginning of Life
Archean life forms are predominantly characterized as:
Single-celled prokaryotes, lacking membrane-bound nuclei and cellular organelles, representative of early bacterial forms.
A significant evolutionary event during this period was the development of autotrophic processes, particularly photosynthesis, evidenced by 3.5 billion-year-old prokaryotic fossils from Australia.
Oxygenation Events
Increase in atmospheric and oceanic oxygen levels can be associated with various geological formations and dynamics, such as:
Banded Iron Formations, pointing to a significant role of cyanobacteria in atmospheric changes.
Stromatolites: sedimentary structures formed by cyanobacterial activity which trap sediments within mat-like formations.
Proterozoic Eon
The Proterozoic Eon spans from 2.5 to 0.542 billion years ago, characterized by major geological and biological developments:
Development of a continental crust that accounts for 80-90% of Earth's surface area.
Continents become larger and stabilize considerably.
Emergence of extensive sedimentary rock formations and sedimentary basins across the planet.
A rise in atmospheric oxygen concentration roughly 10%.
Tectonic Activity
Active plate tectonics during the Proterozoic Eon led to:
Development of the highest grade metamorphic rocks.
Occurrences of supercontinent cycles, notably the formation of Rodinia around 1 billion years ago, followed by its fragmentation around 750 million years ago.
Periodic significant climate oscillations alternating between greenhouse and icehouse conditions known as Snowball Earth episodes.
Geological Features of the Grand Canyon
Investigation of geological layers in the Grand Canyon reveals crucial information about Earth's history, illustrating formations from various periods.
Key formations observed include:
Kaibab Plateau
Kaibab Formation
Torowap Formation
Coconino Sandstone
Hermit Shale
Redwall Limestone
and several unconformities, both within and across geological time frames.
Late Proterozoic Eon Developments
Oxygen accumulation through the Archean and Proterozoic Eons played an essential role in the evolution and complexity of living organisms.
Although numerous Banded Iron Formations formed during this time, fossil evidence remains scarce, primarily due to the preeminence of microscopic, soft-bodied organisms that became subject to metamorphosis over time.
Early Eukaryotes
Emergence of single-celled eukaryotes and multicellular organisms, largely depended on free oxygen in the atmosphere to sustain their metabolic processes.
Notable features distinguishing eukaryotes include:
Membrane-bound nucleus
Presence of organelles
Larger quantity of DNA when compared to prokaryotes
Inflexible cell walls versus flexible cell walls in eukaryotes, allowing for more complex cellular interactions and possible endocytosis.
Asexual and sexual reproductive capabilities in eukaryotes versus asexual reproduction in prokaryotes.
Contrast Between Prokaryotes and Eukaryotes
Prokaryotes:
Lack of membrane-bound nuclei
Less complex DNA structure
Absence of internal cellular subdivisions
Inflexible cell walls leading to limited cellular engulfment abilities.
Eukaryotes:
Contain membrane-bound nuclei and organelles
More extensive DNA content (approximately 1000x) than prokaryotes
Flexible cell walls permitting more complex interactions.
Summary of Eons
The earth underwent significant developmental changes throughout its history marked by the following eons:
Hadean:
Known as “Hell” (4.6 to 3.8 Ga), characterized by internal differentiation and the formation of oceans and protocontinents.
Archean:
Termed “Ancient” (3.8 to 2.5 Ga), marked by the birth of continents and the emergence of the earliest life forms.
Proterozoic:
Labeled “Before life” (2.5 to 0.542 Ga), noted for the development of tectonic plates, significant oxygen buildup in the atmosphere, and the appearance of multicellular life.