Week 2 - Precambrian (Hadean --> Mesoproterozoic) Flashcards

1
Q

When did the Earth form?

A

4.6 Ga

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2
Q

What is the principle of uniformitarianism?

A

The present is the key to the past.

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3
Q

Name the techniques used to establish stratigraphic information.

A

1) Biostratigraphy (fossils).
2) Lithostratigraphy (sequence of rocks).
3) Chronostratigraphy (radiometric dating).
4) Chemostratigraphy (chemical composition).
5) Magnetostratigraphy (magnetic properties).
6) Cyclostratigraphy (Milankovitch cycles).
7) Tephra stratigraphy (ash layers).

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4
Q

Which techniques are used for dating Precambrian rocks?

A

Chemostratigraphy and Chronostratigraphy.

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5
Q

Why are there no golden spikes in the Precambrian?

A

Rocks are linked by numerical ages using radiometric dating and chemostratigraphy.

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6
Q

What was the nature of the early Earth’s crust?

A

1) Poor in silicon dioxide, thin, dense, and basaltic.
2) Re-melting produced buoyant, silicon-rich upper crust.

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7
Q

What are cratons?

A

Silicon-rich crusts formed from early continental production.

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8
Q

When might the first subduction zones have started?

A

Around 3 Ga.

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9
Q

When and where did early life likely form?

A

Around 4 - 3.7 Ga in a warm/hot environment.

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10
Q

What are stromatolites?

A

Structures formed by communities of micro-organisms.

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11
Q

Where were the earliest stromatolites found?

A

Greenland, 3.7 Ga.

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12
Q

When was photosynthesis first invented?

A

Around 3 Ga.

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13
Q

What marked the Earth’s surface oxygenation?

A

The appearance of banded iron formations.

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14
Q

How did the rise of oxygen affect the atmosphere?

A

Reduced greenhouse gases like methane, leading to global cooling.

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15
Q

What was the Lomagundi Event?

A

A rise in organic productivity causing increased burial of light carbon.

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16
Q

How did the Huronian and Transvaal supergroups show changing conditions?

A

Huronian: reducing conditions.
Transvaal: oxidizing conditions.

17
Q

What is the “Boring Billion”?

A

A stable period from 1.8 to 0.8 Ga with little surface perturbation.

18
Q

What evolutionary progress occurred during this period?

A

The subdivision of eukaryotes into five major groups.

19
Q

Where in the UK are Precambrian rocks found?

A

England, Wales, Northern Ireland, and Scotland.

20
Q

Name the main Precambrian rock groups in Scotland.

A

1) Lewisian gneiss (3.0 – 1.7 Ga).
2) Torridonian sedimentary rocks (1.2 – 1.0 Ga).
3) Moine supergroup (1.0 – 0.87 Ga).

21
Q

What are the Hadean, Archean, and Proterozoic?

A

Hadean: Time before 4.0 Ga with no preserved rocks.
Archean: Rocks older than 2.5 Ga.
Proterozoic: After the Archean.

22
Q

What is the Giant Impact Hypothesis?

A

The Moon formed from debris after a collision with a Mars-sized body.

23
Q

Describe the early Earth’s crust.

A

Mafic, thin, and constantly growing.

24
Q

What created magma oceans?

A

The Moon-forming event melted large parts of the mantle.

25
Q

Name two early supercontinents.

A

Rodinia (1.1 – 1.0 Ga) and Nuna (1.9 – 1.8 Ga).

26
Q

When did the Great Oxygenation Event (GOE) occur?

A

Around 2.2 Ga.

27
Q

What caused the GOE?

A

Cyanobacteria producing oxygen through photosynthesis.

28
Q

What event followed the GOE?

A

The Lomagundi Event, marked by organic carbon burial.

29
Q

How did oxygen increase during the Late Proterozoic?

A

Photosynthetic organisms evolved, contributing to oxygen buildup.

30
Q

What was the Earth’s mantle like during its early formation?

A

The mantle was hotter than today due to radioactive decay, core differentiation, and the Moon-forming event.

31
Q

What tectonic process dominated early Earth?

A

Vertical tectonic processes, due to limited subduction or flatter subduction compared to modern processes.

32
Q

What was the state of the Earth after the Moon-forming event?

A

Earth retained enough heat to melt large parts of the mantle, forming a “magma ocean” for 10 million years.

33
Q

How did the rapid rotation of early Earth affect its tectonics?

A

The fast rotation helped retain heat, resulting in a “magma ocean” and possibly influencing early mantle convection patterns.

34
Q

How did the magma ocean crystallization affect the mantle?

A

It led to the formation of low shear wave velocity provinces (LLSVPs) in the mantle.

35
Q

What evidence suggests the start of plate tectonics on early Earth?

A

The presence of eclogitic diamond compositions around 3 Ga, which can only form through subduction and continental collision.

36
Q

What was the significance of Rb/Sr ratios in early Earth’s crust?

A

An increase in Rb/Sr ratios in juvenile continental crust indicated it became more silica-rich and thicker, with a maximum thickness of 40 km at the time of Rodinia assembly.