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Transcript
Chapter 22The Precambrian Earth
Early Earth

The Age of Earth

Earth is estimated to be 4.56 billion years old.

Precambrian time accounts for 90% of Earth’s history, and is divided into THREE
eons:


Hadean – No signs of life

Archean – Prokaryotic organisms

Proterozoic – Eukaryotic organisms
Evidence of Earth’s Age

Crustal Rock – pg. 620

Solar System – pg. 621
Early Earth


Early Earth’s Heat Sources – pgs. 621 & 622

Gravitational Contraction

Radioactivity

Bombardment
Earth’s Cooling

Took about 200 million years, for liquid water to form.

Cooling continues to this day.
Formation of the Crust & Continents

Formation of the Crust

Differentiation


Earliest Crust


High density elements sank toward the center. – Graph pg. 624
Resembled oceanic crust, and was recycled. None exists today.
Continental Crust

Reactions with the early crust and water, created less dense material, which led to
microcontinents.

Cratons were formed, the deepest parts of the crust… up to 200km thick.

Precambrian Shields – Areas where cratons are exposed, In North America, we have the
Canadian Shield.
Formation of the Crust & Continents

Growth of the Continents

Mountain building


Laurentia


as microcontinents collided, mountains and mountain ranges were created.
Ancient North America, was created by collisions 1.8-1.6 bya.
Rodenia

1st supercontinent. Positioned at the equator, with Laurentia at the center, was composed
of 75% of all the continental crust.

Pangaea – 300 mya

Laurasia & Gondwanaland – 200 mya
Formation of the Atmosphere & Oceans

Formation of the Atmosphere – read pg. 628

Outgassing


Oxygen in the Atmosphere

Volcanoes do not typically produce Oxygen, so how’d it get into our atmosphere?

1st Oxygen producers


Volcanic eruptions released large amounts of water vapor, carbon dioxide and Nitrogen into the atmosphere.

Cyanobacteria – use photosynthesis and produce Oxygen.

These cyanobacteria clustered together by the billions and formed Stromatolites.
Evidence in Rocks – Iron Oxide presence.

Banded Iron

Red Beds
Importance of Oxygen

Animal Respiration

Ozone Layer
Formation of the Crust & Continents

Formation of the Oceans


Where did the water come from?

Outgassing

Bombardment
Earth cooled, liquid water formed, water cycle began… Rain!


Oceans and rivers formed, minerals dissolved and made the new oceans salty.
Water & Life

Liquid water made it possible for life to exist on our planet.
Early Life on Earth

Origin of Life

Primordial Soup

Miller’s Hypothesis – 1953

Read pg.633,634

How Life Might have Begun on Earth… 3 Ideas.

Copy table 22.1


Earth’s Surface

Deep Earth

Space
RNA World – read pg.635
Early Life on Earth

Proterozoic Life

Precambrian was dominated by unicellular organisms

TWO types:


Prokaryotes – NO membrane bound nucleus, smaller.

Eukaryotes – membrane bound nucleus, larger.
Multicellular Organisms

Present around 630 mya.

Ediacaran biota